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        <title xml:lang="fr">Projet d' une nouvelle mechanique : avec un examen de l' opinion de M. Borelli sur les propriétez des poids suspendus par des cordes</title>
        <title xml:lang="fr">Projet d' une nouvelle mechanique : avec un examen de l' opinion de M. Borelli sur les propriétés des poids suspendus par des cordes</title>
        <author>Varignon, Pierre</author>
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        <date>1687</date>
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  <text>
    <body xml:lang="fr" type="free">
      <div type="section">
        <pb facs="0001" />
        <pb facs="0002" />
        <pb facs="0003" />
        <pb facs="0004" />
        <pb facs="0005" />
        <pb facs="0006" />
        <pb facs="0007" />
        <pb facs="0008" />
        <note />
        <note />
        <note />
        <pb facs="0009" />
      </div>
      <div type="section">
        <head xml:space="preserve">PROJET <lb />D’UNE NOUVELLE <lb />MECHANIQUE</head>
        <head rend="italics" xml:space="preserve">AVEC</head>
        <p>
          <s xml:space="preserve">Un Examen de l’opinion de M. </s>
          <s xml:space="preserve">BORELLI, <lb />ſur les propriétez des Poids ſuſpendus <lb />par des Cordes.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0009-01" />
          <label>0009-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">A PARIS,</head>
        <p>
          <s xml:space="preserve">Chez {la Vcuve d’<hi rend="small caps">Edme</hi> <hi rend="small caps">Martin</hi>, \\ <hi rend="small caps">Jean</hi> <hi rend="small caps">Boudot</hi>, \\ &amp; </s>
          <s xml:space="preserve"><hi rend="small caps">Estienne</hi> <hi rend="small caps">Martin</hi>,} ruë S. </s>
          <s xml:space="preserve">Jaques, \\ au Soleil d’or.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve">M. DC. LXXXVII. <lb />AVEC PRIVILEGE DU ROI.</head>
        <pb facs="0010" />
        <pb facs="0011" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0011-01" />
          <label>0011-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">A MESSIEURS <lb />DE <lb />L’ACADEMIE <lb />ROYALE <lb />DES SCIENCES@</head>
        <p rend="italics">
          <s xml:space="preserve">MESSIEVRS, <lb />Fe n’ay pas crû devoir expoſer au <lb />jugement du public ce Projet d’une
</s>
          <pb facs="0012" />
          <s xml:space="preserve"><fw type="head">EPITRE.</fw>
Nouvelle Mècbanique, ſans m’ap-<lb />puyer d’une auſſi grande autboritè <lb />que la vôtre, moy qui n’ay encore au-<lb />cun nom dans les Lettres, &amp; </s>
          <s xml:space="preserve">qui dois <lb />par conſèquent me dèfier de ces pre-<lb />miers mouvemens que @amour des <lb />Sciences inſpire àceux qui commencent <lb />à s’y apliquer. </s>
          <s xml:space="preserve">Sans cela on pourroit <lb />juſtement m’accuſer de quelque tèmèri-<lb />tè, d’avoir entrepris de dècouvrir dans <lb />cette matière ce que tant de ſc1;</s>
          <s xml:space="preserve">avans <lb />Autbeurs n’ont pas dècouvert; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">je <lb />craindrois de m’être laiſſè tromper <lb />par ces illuſions flateuſes de la nou-<lb />veautè qui abuſent d’ordinaire les <lb />bommes, lorſqu’ils ſe piquent d’avoir <lb />des opinions particulières. </s>
          <s xml:space="preserve">Fe puis dire <lb />neanmoins, <hi rend="small caps">Messieurs</hi>, que ce <lb />n’eſt pas l’ambition de me ſignaler par <lb />des idèes extraordinaires qui m’a
</s>
          <pb facs="0013" />
          <s xml:space="preserve"><fw type="head">EPITRE.</fw>
pouſſè à ècrire ce petit traitè; </s>
          <s xml:space="preserve">c’eſt un <lb />Eſſay que j’ay voulu faire de mes for-<lb />ces pour être connu de vous, &amp; </s>
          <s xml:space="preserve">pour <lb />vous donner occaſion de m’encourager <lb />dans l’ètude que j’ay embraſsèe. </s>
          <s xml:space="preserve">Si je <lb />n’ay pas tout ce qui eſt nècèſſaire pour <lb />inſtruire les autres, j’ay du moins <lb />toute la docilitè qu’il faut pour être <lb />inſtruit: </s>
          <s xml:space="preserve">je ne me flatte point auſſi <lb />d’avoir ètabli des principes certains <lb />dans ce Projet, n’y d’en pouvoir <lb />tirer des conſèquences infaillibles: <lb /></s>
          <s xml:space="preserve">Vous enjugerez mieux que perſonne, <lb /><hi rend="small caps">Messieurs</hi>, Vous qui pènètrez ſi <lb />avant dans les Sciences les plus rele-<lb />vèes. </s>
          <s xml:space="preserve">On ſçait que rien n’ècbape à <lb />vos ſoins &amp; </s>
          <s xml:space="preserve">à vôtre èxactitude; </s>
          <s xml:space="preserve">La <lb />Nature ſi avare aux autres de ſes <lb />treſors &amp; </s>
          <s xml:space="preserve">ſi obſtinèe à ſe cacber, n’a <lb />pû ſe dèfendre contre la pènètration <lb />de vôtre eſprit &amp; </s>
          <s xml:space="preserve">contre la ſubtilitè
</s>
          <pb facs="0014" />
          <s xml:space="preserve"><fw type="head">EPITRE.</fw>
de vos recbercbes; </s>
          <s xml:space="preserve">vous en avez plus <lb />dècouvert en vingt ans, qu’on n’a-<lb />voit fait en pluſieurs Siècles. </s>
          <s xml:space="preserve">Vos <lb />Obſervations Aſtronomiques ont dè-<lb />voilè (pour ainſi dire) des Planettes <lb />qui ſe dèroboient à nos yeux; </s>
          <s xml:space="preserve">vos <lb />meſures ſi prèciſes ſur la terre, par <lb />raport à celles que vous preniez en <lb />même tems dans le Ciel, ont rècti-<lb />fiè mille erreurs de nos anciens Geo-<lb />grapbes. </s>
          <s xml:space="preserve">La Pbyſique vous doit <lb />ce qu’elle a de plus curieux, ſoit <lb />dans la diſſection du Corps bumain <lb />&amp; </s>
          <s xml:space="preserve">des Animaux, ſoit dans la deſ-<lb />cription &amp; </s>
          <s xml:space="preserve">dans l’analyſe des Plan-<lb />tes, des Eaux &amp; </s>
          <s xml:space="preserve">des Mineraux. <lb /></s>
          <s xml:space="preserve">Lue ne vous doivent point auſſi les <lb />Matbematiques en gènèral pour <lb />tant d’ouvrages celebres que vous <lb />avez mis au jour? </s>
          <s xml:space="preserve">Enfin, il n’y a
</s>
          <pb facs="0015" />
          <s xml:space="preserve"><fw type="head">EPITRE.</fw>
point de Science que vous n’ayez <lb />perfectionnèe &amp; </s>
          <s xml:space="preserve">que vous n’enri-<lb />cbiſſiez de tems en tems par vos <lb />travaux. </s>
          <s xml:space="preserve">Lue n’attend on pas en-<lb />core de vous, animez comme vous <lb />êtes par les bienfaits d’un Grand <lb />Roy, qui veut renàre ſon Regne <lb />auſſi glorieux par les Sciences &amp; </s>
          <s xml:space="preserve">par <lb />les Arts, qu’il l’eſt dèja par ſes <lb />prodigieuſes Conqueſtes, &amp; </s>
          <s xml:space="preserve">par tou-<lb />tes ſes Hèroϊques actions? </s>
          <s xml:space="preserve">A quoy <lb />ne devez vous pas aſpirer vous-<lb />meſmes aujourd’buy ſous la protè-<lb />ction d’un Miniſtre ſi ſage &amp; </s>
          <s xml:space="preserve">ſi vi-<lb />gilant, qui excite tout le monde par <lb />ſes ordres &amp; </s>
          <s xml:space="preserve">par ſon exemple à <lb />illuſtrer &amp; </s>
          <s xml:space="preserve">à cèlèbrer un Regne ſi <lb />plein de merveilles ? </s>
          <s xml:space="preserve">Souffrez donc, <lb /><hi rend="small caps">Messieurs</hi>, s’il vous plaît, <lb />vous qui êtes comme à la ſource de
</s>
          <pb facs="0016" />
          <s xml:space="preserve"><fw type="head">EPITRE.</fw>
toutes les Sciences bumaines, &amp; </s>
          <s xml:space="preserve">à qui <lb />rien ne manque pour continuer vos <lb />recbercbes, &amp; </s>
          <s xml:space="preserve">pour augmenter vos <lb />connoiſſances, que j’oſe vous offrir <lb />&amp; </s>
          <s xml:space="preserve">mettre au jour ce que j’ay puisè <lb />dans cette ſource, &amp; </s>
          <s xml:space="preserve">qu’en eſſayant <lb />de vous ſuivre &amp; </s>
          <s xml:space="preserve">de vous imiter, je <lb />puiſſe quelquefois profiter de vos <lb />lumières, &amp; </s>
          <s xml:space="preserve">vous aſſeurer que je ſuis <lb />avec une parfaite vènèration,</s>
        </p>
        <p>
          <s xml:space="preserve">MESSIEVRS,</s>
        </p>
        <p>
          <s xml:space="preserve">Vôtre tres-humble &amp; </s>
          <s xml:space="preserve">tres-<lb />obéϊſſant ſerviteur</s>
        </p>
        <p>
          <s xml:space="preserve">V<hi rend="small caps">ARIGNON.</hi></s>
        </p>
        <pb facs="0017" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0017-01" />
          <label>0017-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">PREFACE.</head>
        <p>
          <s xml:space="preserve">A L’ouverture du ſecond Tome des <lb />Lettres de Monſieur Deſcartes, je <lb />tombai ſur un endroit de la 24. </s>
          <s xml:space="preserve">où <lb />il dit que c’eſt une cboſe ridicule, <lb />que de vouloir employer la raiſon du Le-<lb />vier dans la Poulie. </s>
          <s xml:space="preserve">Cette réfléxion m’en <lb />fit faire une autre@<unclear reason="illegible" />: </s>
          <s xml:space="preserve">Sçavoir s’il eſt plus rai-<lb />ſonnable de s’imaginer un levier dans un <lb />poids qui eſt ſur un plan incliné, que dans <lb />une poulie. </s>
          <s xml:space="preserve">Aprés y avoir penſé, il me <lb />ſembla que ces deux machines étant pour le <lb />moins auſſi ſimples que le levier, elles n’en <lb />devoient avoir aucune dépendance, &amp; </s>
          <s xml:space="preserve">que <lb />ceux qui les y rapportoient, n’y étoient forcez <lb />que parce que leurs principes n’avoient pas aſſez <lb />d’étenduë pour en pouvoir démontrer les pro-<lb />priétez indépendamment les unes des autres.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">En effet en éxaminant ces principes un peu
</s>
          <pb facs="0018" />
          <s xml:space="preserve"><fw type="head">PREFACE.</fw>
de prês, il me parut qu’ils ne pouvoient ſervir, <lb />tout au plus, qu’à démontrer que l’equilibre <lb />ſe trouve toujours dans un levier auquel ſont <lb />appliquez deux poids qui ſont entr’ eux en <lb />raiſon rèciproque des diſtances de leurs lignes <lb />de direction à ſon point d’appui; </s>
          <s xml:space="preserve">encore n’é-<lb />toit-ce qu’en ce cas: </s>
          <s xml:space="preserve">1°. </s>
          <s xml:space="preserve">Que ce levier fût <lb />droit. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Que ſon point d’appui fût entre les <lb />lignes de direction des poids qui y ſont appli-<lb />quez. </s>
          <s xml:space="preserve">3°. </s>
          <s xml:space="preserve">Lue ces mêmes lignes fuſſent pa-<lb />ralleles entr’elles, &amp; </s>
          <s xml:space="preserve">perpendiculaιres à ce <lb />levier. </s>
          <s xml:space="preserve">Auſſi Guid-Ubalde, &amp; </s>
          <s xml:space="preserve">les autres qui <lb />s’en tiennent à la démonſtration d’Archimede, <lb />ont-ils été obligez de faire@<unclear reason="illegible" />revenir de gré ou <lb />de force toutes ſortes de machines à cette <lb />eſpece de levier, &amp; </s>
          <s xml:space="preserve">de réduire de même tous <lb />les autres cas à celui-ci.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">C’eſt peut-être ce qui a porté M. </s>
          <s xml:space="preserve">Deſcartes, <lb />&amp; </s>
          <s xml:space="preserve">M. </s>
          <s xml:space="preserve">Vvallis a prendre une autre route; <lb /></s>
          <s xml:space="preserve">quoi qu’il en ſoit, ce n’a pas été ſans ſuccez: </s>
          <s xml:space="preserve"><lb />puiſque celle qu’ils ont ſuivie, conduit éga-<lb />lement à la connoiſſance des uſages de chacune <lb />de ces machines, ſans être obligé de les faire <lb />dépendre l’une de l’autre; </s>
          <s xml:space="preserve">outre qu’elle à mené <lb />M. </s>
          <s xml:space="preserve">Vvallis beaucoup plus loin qu’aucun
</s>
          <pb facs="0019" />
          <s xml:space="preserve"><fw type="head">PREFACE.</fw>
Autheur, que je ſçache, n’eût encore été de <lb />ce côté-là.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">La comparaiſon que je fis de ces deux <lb />fortes de principes, me fit ſentir que ceux d’Ar-<lb />chimede n’étoient ny ſi étendus, ny ſi con-<lb />vainquants que ceux de M. </s>
          <s xml:space="preserve">Deſcartes, &amp; </s>
          <s xml:space="preserve">de <lb />M. </s>
          <s xml:space="preserve">Vvallis; </s>
          <s xml:space="preserve">mais je ne ſentis point que les uns <lb />ny les autres m’éclairaſſent beaucoup: </s>
          <s xml:space="preserve">J’en <lb />cherchai la raiſon, &amp; </s>
          <s xml:space="preserve">ce défaut me parut venir <lb />de ce que ces Autheurs ſe ſont tous plus atta-<lb />chez à prouver la néceſſité de l’équilibre, qu’à <lb />montrer la maniére dont il ſe fait.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">Ce fut ce qui me fit réſoudre à prendre le <lb />parti d’épier moi-même la nature, &amp; </s>
          <s xml:space="preserve">d’eſſayer <lb />ſi en la ſuivant pas à pas, je ne pourrois point <lb />apercevoir comment elle s’y prend pour faire <lb />que deux puiſſances, ſoit égales, ſoit inégales, <lb />demeurent en équilibre. </s>
          <s xml:space="preserve">Enfin je m’appliquai <lb />à chercher l’équilibre lui-même dans ſa ſource, <lb />ou pour mieux dire, dans ſa génération.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">Le premier objet qui me vint à l’eſprit, ce <lb />fut un poids qu’une puiſſance ſoutient ſur <lb />un plan incliné; </s>
          <s xml:space="preserve">D’abord je me le repréſentai
</s>
          <pb facs="0020" />
          <s xml:space="preserve"><fw type="head">PREFACE.</fw>
de telle figure que le concours de ſa ligne de <lb />direction avec celle de cette puiſſance, ſe fit <lb />dans quelqu’un de ſes points: </s>
          <s xml:space="preserve">De-là je vis que <lb />leur concours d’action ſe faiſant auſſi par ce <lb />moyen dans ce ſeul point, il devenoit alors <lb />ſon centre de direction: </s>
          <s xml:space="preserve">De ſorte que ſi ce <lb />plan eut manqué tout d’un coup, ce corps au-<lb />roit néceſſairement ſuivi l’impreſſion de ce <lb />point. </s>
          <s xml:space="preserve">Je cherchai enſuite quelle devoit être <lb />cette impreſſion, &amp; </s>
          <s xml:space="preserve">j’aperçus que celles que <lb />faiſoient ſur ce point, &amp; </s>
          <s xml:space="preserve">la peſanteur de ce <lb />poids, &amp; </s>
          <s xml:space="preserve">la puiſſance qui le retenoit, étant <lb />les mêmes que s’il eut été pouſſé en même-<lb />tems par deux forces qui leur euſſent été éga-<lb />les, &amp; </s>
          <s xml:space="preserve">qui euſſent agi ſuivant leurs lignes de <lb />direction: </s>
          <s xml:space="preserve">J’aperçus, dî-je, qu’il lui en réſultoit <lb />une impreſſion compoſée ſuivant une ligne <lb />qui étoit la diagonale d’un parallelogramme <lb />fait ſous des parties de ces lignes de direction, <lb />qui étoient entr’elles, comme ce poids &amp; </s>
          <s xml:space="preserve"><lb />cette puiſſance: </s>
          <s xml:space="preserve">D’où je vis que l’impreſſion <lb />de ce corps ſe faiſoit alors ſuivant cette diago-<lb />nale, qui devenoit en ce cas ſa ligne de di-<lb />rection; </s>
          <s xml:space="preserve">mais que ce plan lui étant perpendi-<lb />culairement oppoſé, il la ſoutenoit toute en-<lb />tiére; </s>
          <s xml:space="preserve">ce qui faiſoit que ce poids ainſi pouſſé
</s>
          <pb facs="0021" />
          <s xml:space="preserve"><fw type="head">PREF ACE.</fw>
par le concours d’action de ſa peſanteur &amp; </s>
          <s xml:space="preserve">de <lb />la puiſſance qui lui étoit appliquée, demeuroit <lb />ſur ce plan incliné de même que s’il eut été <lb />horizontal, &amp; </s>
          <s xml:space="preserve">que cette impreſſion compoſée <lb />n’eut été qu’un effet de ſa ſeule peſanteur.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">De cette penſée j’en vis naître pluſieurs <lb />autres, &amp; </s>
          <s xml:space="preserve">jem’aperçus 1°. </s>
          <s xml:space="preserve">Que toute l’impreſ-<lb />ſion que ce plan recevoit alors de ce poids <lb />ainſi ſoutenu par cette puiſſance, ſe faiſoit <lb />ſuivant cette diagonale. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Que ſa charge, <lb />c’eſt-à-dire, la force de cette même impreſ-<lb />ſion, étoit à ce poids &amp; </s>
          <s xml:space="preserve">à cette puiſſance, <lb />comme cette même diagonale à chacun des <lb />côtez qui les répréſentent dans ſon parallelo-<lb />gramme. </s>
          <s xml:space="preserve">3°. </s>
          <s xml:space="preserve">Que ce poids, &amp; </s>
          <s xml:space="preserve">cette puiſſance <lb />étoient toujours entr’eux comme ces mêmes <lb />côtez, c’eſt-à-dire, en raiſon réciproque des <lb />ſinus des angles que font leurs lignes de direc-<lb />tion avec cette diagonale, ou (ce qui revient <lb />au même ) en raiſon réciproque des diſtances <lb />de quelque point que ce ſoit de cette diago-<lb />nale à leur lignes de direction. </s>
          <s xml:space="preserve">Je vis enfin <lb />preſque tout à la fois quantité de choſes tou-<lb />tes nouvelles qu’on verra dans les Corollaires <lb />de la propoſition des ſurfaces.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0022" />
        <fw type="head">PREF ACE.</fw>
        <p>
          <s xml:space="preserve">Aprés avoir ainſi trouvé la maniére dont <lb />l’équilibre ſefait ſur des plans inclinez, je cher-<lb />chai par le même chemin comment des poids <lb />ſoutenus avec des cordes ſeulement, ou appli-<lb />quez à des poulies, ou bien à des leviers, font <lb />équilibre entr’eux, ou avec les puiſſances qui <lb />les ſoutiennent; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">j’aperçus de même que tout <lb />cela ſe faiſoit encore par la voye des mouve-<lb />mens compoſez, &amp; </s>
          <s xml:space="preserve">avec tant d’uniformité <lb />que je ne pûs m’empêcher de croire que cette <lb />voye ne fût véritablement celle que ſuit la <lb />nature dans le concours d’action de deux <lb />poids, ou de deux puiſſances, en faiſant que <lb />leurs impreſſions particulieres, quelque pro-<lb />portion qu’elles ayent, ſe confondent en un@ <lb />ſeule qui ſe décharge toute entiére ſur le point <lb />ou ſe fait cét équilibre: </s>
          <s xml:space="preserve">De ſorte que la <lb />raiſon Phyſique des effets qu’on admire le <lb />plus dans les machines me parut être juſte-<lb />ment celle des mouvemens compoſez.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">Je me démontrai d’abord par cett@ mé-<lb />thode, &amp; </s>
          <s xml:space="preserve">ſans le ſecours d’aucune machine, <lb />les propriétez des poids ſuſpendus avec des <lb />cordes, en quelque nombre qu’elles ſoient, &amp;</s>
          <s xml:space="preserve">
</s>
          <pb facs="0023" />
          <s xml:space="preserve"><fw type="head">PREF ACE.</fw>
pour tous les angles poſſibles qu’elles peuvent <lb />faire entr’elles. </s>
          <s xml:space="preserve">De-là je paſſai à une démonſ-<lb />tration des poulies qui comprend toutes les <lb />directions poſſibles des puiſſances, ou des <lb />poids qui y ſont appliquez, ſoit que le centre <lb />de ces poulies demeure fixe, ſoit qu’on le ſup-<lb />poſe mobile. </s>
          <s xml:space="preserve">Enſuite au lieu de la démonſtra-<lb />tion qu’on ne fait ordinairement que pour les <lb />plans inclinez, j’en trouvai une qui s’étend <lb />généralement à toutes ſortes de ſurfaces, &amp; </s>
          <s xml:space="preserve">à <lb />toutes les directions poſſibles des puiſſances, <lb />ou des poids qui y ſont appliquez. </s>
          <s xml:space="preserve">Enfin d’une <lb />ſeule démonſtration je découvris les proprié-<lb />tez de toutes les eſpeces de leviers, de quel-<lb />que figure, &amp; </s>
          <s xml:space="preserve">dans quelque ſituation qu’ils <lb />ſoient, &amp; </s>
          <s xml:space="preserve">pour toutes les directions poſſibles <lb />des puiſſances, ou des poids qui y ſont appli-<lb />quez.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">Des vuës ſi étenduës me ſurprirent, &amp; </s>
          <s xml:space="preserve">l’é-<lb />vidence avec laquelle le détail de tout cela <lb />me paroiſſoit, indépendamment même du <lb />général, me confirma encore dans l’opinion <lb />ou j’étois, qu’il faut entrer dans la génération <lb />d e l’équilibre pour y voir en ſoi, &amp; </s>
          <s xml:space="preserve">pour y <lb />reconnoître les propriétez que tous les autres
</s>
          <pb facs="0024" />
          <s xml:space="preserve"><fw type="head">PREF ACE.</fw>
principes ne prouvent, tout au plus, que par <lb />néceſſité de conſéquence.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">Il y a encore un avantage dans la route <lb />que je tiens, c’eſt qu’elle facilite extrémement <lb />le calcul des forces, tant des poids, que des <lb />puiſſances, en ce que leurs raports y ſont tou-<lb />jours déterminez immédiatement par les ſinus <lb />des angles que font leurs lignes de direction <lb />avec celle de l’impreſſion qui réſulte de <lb />leur concours d’action, &amp; </s>
          <s xml:space="preserve">que cette méthode <lb />détermine pour le point ou elles concourent. <lb /></s>
          <s xml:space="preserve">On y voit, que lors que deux puiſſances, <lb />ou deux poids, ou bien une puiſſance &amp; </s>
          <s xml:space="preserve">un <lb />poids font équilibre, ſoit avec des cordes <lb />ſeulement, ſoit à l’aide de quelque poulie, de <lb />quelque ſurface, ou de quelque levier que ce <lb />ſoit; </s>
          <s xml:space="preserve">ils ſont toujours entr’ eux en raiſon réci-<lb />proque des ſinus de ces mêmes angles.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">J’avois deſſein d’expliquer avec cette mé-<lb />thode les effets les plus ſurprenans, &amp; </s>
          <s xml:space="preserve">les plus <lb />difficiles des machines compoſées que l’on ren-<lb />contre dans les arts, &amp; </s>
          <s xml:space="preserve">dans la nature; </s>
          <s xml:space="preserve">mais cela <lb />demandoit plus de loiſir, &amp; </s>
          <s xml:space="preserve">même un plus <lb />grand nombre d’expériences que l’état de ma
</s>
          <pb facs="0025" />
          <s xml:space="preserve"><fw type="head">PREF ACE.</fw>
fortune ne me peut permetre: </s>
          <s xml:space="preserve">c’eſt pour cela <lb />que je me ſuis déterminé à ne donner préſente-<lb />ment que les Propoſitions fondamentales de <lb />la Méchanique: </s>
          <s xml:space="preserve">peut-être que de plus habiles <lb />gens que moy, &amp; </s>
          <s xml:space="preserve">qui ſeront plus en état de <lb />faire cette entrepriſe, voudront bien ſe donner <lb />la peine d’en faire l’application à la Phyſique.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">Mais en attendant, je ne laiſſeray pas d’a-<lb />maſſer tout ce que je pouray d’expériences <lb />pour ce deſſein; </s>
          <s xml:space="preserve">c’eſt pourquoy je prie ceux <lb />qui n’auront pas en vuë d’y travailler, de vou-<lb />loir bien me communiquer celles qu’ils croi-<lb />ront s’y pouvoir rapporter: </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">ſur tout de <lb />me faire part de tout ce qui leur viendra de <lb />difficultez ou de lumieres ſur les principes <lb />qu’on propoſe icy, leur promettant d’en uſer <lb />avec toute la docilité d’un homme qui ne <lb />cherche que la vérité.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0026" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0026-01" />
          <label>0026-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">AVER TISSE MENT.</head>
        <p rend="italics">
          <s xml:space="preserve">LES corollaires qu’on verra <lb />citez dans la Solution de cba-<lb />que Problême ſuivant, ſeront de la <lb />Propoſition fondamentale qui le pré-<lb />cède. </s>
          <s xml:space="preserve">C’eſt de peur d’ennuyer par <lb />des rèpètitions trop frèquentes qu’on <lb />ne la citera point.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0027" n="1" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0027-01" />
          <label>0027-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">PROJET <lb />D’UNE <lb />NOUVELLE MECHANIQUE.</head>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0027-02" />
          <label>0027-02</label>
        </figure>
        <p rend="italics">
          <s xml:space="preserve">CE C 1<unclear reason="illegible" /> n’ètant que pour ceux qui entendent aſſez <lb />ces matières pour en pouvoir juger, on ne s’arrê-<lb />tera point à répéter des Définitions, ny des Axio-<lb />mes qui ſe trouvent par tout; </s>
          <s xml:space="preserve">en voici ſeulcment <lb />un, avec une demande, &amp; </s>
          <s xml:space="preserve">quelques Lemmes <lb />particuliérement néceſſaires pour l’intelligence de ce Projet.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Axiome</hi>.</head>
        <p>
          <s xml:space="preserve">Les eſpaces que parcourt un même corps, ou des <lb />corps égaux dans des tems égaux, ſont entre-eux <lb />comme les forces qui les meuvent; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">réciproque-<lb />ment lorſque ces Eſpaces ſont entre-eux comme ces
</s>
          <pb facs="0028" n="2" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
forces, elles les font parcourir au même corps, ou à <lb />
<ptr xml:id="note-0028-01a" corresp="note-0028-01" type="noteAnchor" />
des corps égaux en tems égaux.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0028-01" corresp="note-0028-01a" place="margin">LEMMES.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demande</hi>.</head>
        <p>
          <s xml:space="preserve">On ſuppoſe ici que dans tout corps qui ſe meut, <lb />ou qui fait effort pour ſe mouvoir, il y a toûjours <lb />un certain point qui ſurchargé de l’impreſſion de <lb />tous les autres, détermine ce corps à ſuivre celle <lb />qu’il a pour lors vers l’endroit où il tend. </s>
          <s xml:space="preserve">On ne ſe <lb />met point en peine que ce point ſoit le même dans <lb />toutes les ſituations poſſibles de ce corps: </s>
          <s xml:space="preserve">c’eſt aſſez <lb />que dans chaque ſituation il y en ait un que l’on <lb />appelle ici ſon Centre de gravité, ou, plus générale-<lb />ment ſon Centre de direction, ou, d’équilibre, du moins <lb />pour le tems qu’il détermine ainſi ce corps à ſuivre <lb />ſon impreſſion; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">la ligne qui joint ce point avec <lb />celui où il tend, s’appelle ſa Ligne de direction.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">On ne met ceci en ſuppoſition que pour abréger; </s>
          <s xml:space="preserve">autrement <lb />on le pourroit dèmontrer: </s>
          <s xml:space="preserve">car il n’y arien de plus évident que <lb />de tous les points d’un corps, il y en a toûjours, &amp; </s>
          <s xml:space="preserve">même <lb />néceſſairement, quelqu’un autour duquel l’impreſſion qu’ils <lb />ont tous vers le côtè ou ce corps tend, ſe trouve ſi ègalement <lb />partagèe qu’ils demeureroient en èquilibre deſſus, ſi ſans cban-<lb />ger la ſituation de ce corps par raport à l’endroit où il tend, <lb />on le rendoit fixe; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſèquent l’impreſſion d’un tel <lb />point ainſi ſurcbargè de celle de tous les autres, étant l<unclear reason="illegible" />a <lb />même que s’il ètoit le ſeul qui en eût, il doit déterminer ce <lb />corps à la ſuivre.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">Il n’y a rien-là, ce me ſemble, que de clair; </s>
          <s xml:space="preserve">cependant <lb />s’il ſe trouvoit quelqu’un qui faute de le voir de même, fit <lb />difficultè de l’accorder, il peut prendre dans la ſuite les corps <lb />dont on parlera, pou@ des points qui ayent la peſanteur, ou <lb />l’impreſſion qu’on y ſuppoſe; </s>
          <s xml:space="preserve">ou bien pour des puiſſances appli-<lb />quées de même, &amp; </s>
          <s xml:space="preserve">qui leur ſoient ègales: </s>
          <s xml:space="preserve">parce que les démonſ-
</s>
          <pb facs="0029" n="3" />
          <s xml:space="preserve"><fw type="head">ME’CHANIQUE.</fw>
trations ſuivantes ſe peuvent également appliquor aux uns <lb />
<ptr xml:id="note-0029-01a" corresp="note-0029-01" type="noteAnchor" />
&amp; </s>
          <s xml:space="preserve">aux autres.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0029-01" corresp="note-0029-01a" place="margin">LEMMES.</note>
            </div>
          </body>
        </floatingText>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0029-01" />
          <label>0029-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">LEMME I.</head>
        <p rend="italics">
          <s xml:space="preserve">LE poids A ètant ſuſpendu à une corde EH, ou à deux <lb />
<ptr xml:id="note-0029-02a" corresp="note-0029-02" type="noteAnchor" />
MH &amp; </s>
          <s xml:space="preserve">NH attacbèes à un même point fixe H; <lb /></s>
          <s xml:space="preserve">ou bien ſoutenu ſur un pieu EH, ou ſur deux MH &amp; </s>
          <s xml:space="preserve">NH <lb />appuyez auſſi ſur un même point H: </s>
          <s xml:space="preserve">en ſorte que la li-<lb />gne A H, qui joint ſon Centre de gravitè A avec ſon <lb />point de ſuſpenſion, ou d’apuy, faſſe quelque angle que c@ <lb />ſoit avec ſa ligne de direction AK: </s>
          <s xml:space="preserve">Ce poids tombera de A <lb />vers B le long de l’arc A B dont H eſt le centre, juſqu’à <lb />ce que la ligne AH ſoit dans la perpendiculaire, ou dans <lb />le plan borizontal H B, &amp; </s>
          <s xml:space="preserve">étant arrivé en B, ily demeu-<lb />rera, ſi l’on n’y ſuppoſe à’autre cauſe que ſa peſanteur.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0029-02" corresp="note-0029-02a" place="margin">fig. 1. <lb />2. <lb />3. <lb />4.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstr ation</hi>.</head>
        <p>
          <s xml:space="preserve">L’effet de la peſanteur du poids A, c’eſt de l’ap-<lb />procher ( byp. </s>
          <s xml:space="preserve">) du centre de la terre, c’eſt-à-dire, <lb />( dem. </s>
          <s xml:space="preserve">) d’en approcher ſon centre de gravité A, <lb />tant que rien ne l’en empêche. </s>
          <s xml:space="preserve">Or dans la ſituation <lb />preſente rien ne l’empêche de s’en approcher de la <lb />longueur de A K, en tombant le long de l’arc A B <lb />juſqu’en B; </s>
          <s xml:space="preserve">au contraire étant arrivé en B, la cor-<lb />de E H, ou les cordes M H &amp; </s>
          <s xml:space="preserve">N H; </s>
          <s xml:space="preserve">ou bien le plan <lb />horizontal H B, le retiennent &amp; </s>
          <s xml:space="preserve">l’empêchent de <lb />deſcendre davantage; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent ce poids <lb />dans la ſituation preſente tombera le long de l’arc A B <lb />juſqu’en B, &amp; </s>
          <s xml:space="preserve">y étant arrivé, il y demeurera. </s>
          <s xml:space="preserve">Ce <lb />qu’il faloit demontrer.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi>.</head>
        <p>
          <s xml:space="preserve">On prouvera de même que tout autre corps, de
</s>
          <pb facs="0030" n="4" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
quelque côté qu’il tende, appuyé ſeulement ſur un <lb />
<ptr xml:id="note-0030-01a" corresp="note-0030-01" type="noteAnchor" />
de ſes points, ou même ſur une de ſes faces, de quel-<lb />que largeur qu’elle ſoit, doit neceſſairement avancer <lb />du côté ou il eſt pouſſé par ſa peſanteur, ou par <lb />quelqu’autre force que ce ſoit, non-ſeulement tant <lb />que ſa ligne de direction ne paſſe point par ce point <lb />d’apuy, ny par aucun de la partie de cette face ſur <lb />laquelle il s’appuye; </s>
          <s xml:space="preserve">mais encore tant qu’elle n’eſt <lb />point perpendiculaire au plan, ou à la ſurface qui ſe <lb />trouve à ſon paſſage; </s>
          <s xml:space="preserve">c’eſt-à-dire, tant que ſon centre <lb />de direction n’eſt point appuyé: </s>
          <s xml:space="preserve">Car ce centre pou-<lb />vant encore avancer du côté où il tend, la force qui <lb />le pouſſe, ne manquera pas de l’y obliger; </s>
          <s xml:space="preserve">Mais auſſi <lb />par une raiſon toute contraire, ſi-tôt que l’un, &amp; </s>
          <s xml:space="preserve"><lb />l’autre arrivera, ce corps demeurera néceſſairement <lb />en cet état.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0030-01" corresp="note-0030-01a" place="margin">LEMMES.</note>
            </div>
          </body>
        </floatingText>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0030-01" />
          <label>0030-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">LEMME II.</head>
        <p rend="italics">
          <s xml:space="preserve">LE poids MN étant ſuſpendu par deux cordes P M &amp; </s>
          <s xml:space="preserve"><lb />
<ptr xml:id="note-0030-02a" corresp="note-0030-02" type="noteAnchor" />
RN, attacbées aux clous P &amp; </s>
          <s xml:space="preserve">R, &amp; </s>
          <s xml:space="preserve">qui prolon-<lb />gées concourent en H, ſa ligne de diréction A H paſſera <lb />par ce point de concours.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0030-02" corresp="note-0030-02a" place="margin">fig. 5. <lb />6.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration</hi>.</head>
        <p>
          <s xml:space="preserve">Premiérement ( fig. </s>
          <s xml:space="preserve">5. </s>
          <s xml:space="preserve">) l’effort que le poids M N <lb />fait pour attirer le point P de la corde P M vers M, <lb />étant le même qu’il feroit contre le point H, ſi cette <lb />corde prolongée y étoit attachée, &amp; </s>
          <s xml:space="preserve">non plus en P; <lb /></s>
          <s xml:space="preserve">ce corps, ou ce poids eſt ſoutenu par cette corde, <lb />comme ſi elle n’étoit attachée qu’en H. </s>
          <s xml:space="preserve">Pour la <lb />même raiſon il eſt auſſi ſoutenu par la corde R N, <lb />comme ſi étant prolongée, elle n’étoit attachée qu’en <lb />H: </s>
          <s xml:space="preserve">Il eſt donc ſoutenu par ces deux cordes enſem-
</s>
          <pb facs="0031" n="5" />
          <s xml:space="preserve"><fw type="head">ME’CHANIQUE.</fw>
ble, comme ſi l’une, &amp; </s>
          <s xml:space="preserve">l’autre étant prolongée, elles <lb />
<ptr xml:id="note-0031-01a" corresp="note-0031-01" type="noteAnchor" />
n’étoient attachées qu’en ce ſeul point: </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par con-<lb />ſéquent ( Lemm. </s>
          <s xml:space="preserve">1. </s>
          <s xml:space="preserve">) la ligne de direction A K de ce <lb />poids ainſi ſuſpendu, paſſera par le point H où les <lb />cordes P M &amp; </s>
          <s xml:space="preserve">R N concourent. </s>
          <s xml:space="preserve">Ce qu’il F.</s>
          <s xml:space="preserve">D.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0031-01" corresp="note-0031-01a" place="margin">LEMMES.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">Secondement ( fig. </s>
          <s xml:space="preserve">6. </s>
          <s xml:space="preserve">) l’effort que le poids M N fait <lb />pour attirer le point P de ſa corde P M vers M, étant <lb />le même que celui dont il preſſe ſon point C vers H, <lb />il eſt encore ſoutenu par cette corde, comme il le <lb />ſeroit par le pieu C H. </s>
          <s xml:space="preserve">Et pour la même raiſon il <lb />eſt ſoutenu par la corde R N, comme il le ſeroit par <lb />le pieu D H: </s>
          <s xml:space="preserve">Donc il eſt ſoutenu par ces deux cor-<lb />des, comme il le ſeroit par ces deux pieux enſemble: <lb /></s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent ( Lemm. </s>
          <s xml:space="preserve">1. </s>
          <s xml:space="preserve">) la ligne de direction <lb />A K de ce poids ainſi ſuſpendu, paſſera encore par le <lb />point H. </s>
          <s xml:space="preserve">Ce qu’il F. </s>
          <s xml:space="preserve">D.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> I.</head>
        <p>
          <s xml:space="preserve">De-là il eſt clair que de quelque côté que tende <lb />le corps M N, &amp; </s>
          <s xml:space="preserve">que ſa ligne de direction ſoit tour-<lb />née, ſoit que cette impreſſion lui vienne de ſa pe-<lb />ſanteur, ou de quelque autre force, cette ligne de <lb />direction paſſera toûjours par le point H, ou les cor-<lb />des qui le retiennent, doivent concourir, ou con-<lb />courent en effet.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> II.</head>
        <p>
          <s xml:space="preserve">De ſorte que ſi ces cordes ne concourent qu’à une <lb />diſtance infinie, c’eſt-à-dire qu’elles ſoient paralleles <lb />entre-elles, cette ligne de direction ſera auſſi parallele <lb />à l’une &amp; </s>
          <s xml:space="preserve">à l’autre.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0031-01" />
          <label>0031-01</label>
        </figure>
        <pb facs="0032" n="6" />
        <fw type="head">NOUVELLE</fw>
        <note xml:space="preserve" place="margin">LEMMES.</note>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0032-01" />
          <label>0032-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">LEMME III.</head>
        <p rend="italics">
          <s xml:space="preserve">SI le point A ſans peſanteur eſt pouſſé en même tems, <lb />
<ptr xml:id="note-0032-02a" corresp="note-0032-02" type="noteAnchor" />
&amp; </s>
          <s xml:space="preserve">uniformément par deux puiſſances E &amp; </s>
          <s xml:space="preserve">F ſuivant <lb />les lignes A C &amp; </s>
          <s xml:space="preserve">A B, qui faſſent entre-elles quelque an-<lb />gle C A B que ce ſoit, &amp; </s>
          <s xml:space="preserve">que la force dont agit la puiſ-<lb />ſance E, ſoit à celle dont agit la puiſſance F, comme A C <lb />à A B. </s>
          <s xml:space="preserve">Ce point A ſuivra la Diagonale A D du paral-<lb />lelogramme B C fait ſous ces deux lignes.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0032-02" corresp="note-0032-02a" place="margin">fig. 7.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration</hi>.</head>
        <p>
          <s xml:space="preserve">Le point A pouſſé par la puiſſance E vers C D, <lb />l’eſt de même que s’il y étoit porté avec la ligne A B <lb />toûjours parallele à elle-même, de la même viteſſe <lb />qu’il y eſt pouſſé; </s>
          <s xml:space="preserve">Nous pouvons donc le regarder <lb />comme pouſſé de cette maniére vers C D avec la <lb />ligne A B toûjours parallelle à elle-même, ou à C D, <lb />au même tems qu’il eſt pouſſé par la puiſſance F <lb />le long de la même ligne A B. </s>
          <s xml:space="preserve">Or cela bien conçu, <lb />il eſt clair qu’en quelque point, par exemple G, que <lb />la ligne A B rencontre A D, le point A s’y trouvera <lb />toûjours: </s>
          <s xml:space="preserve">parce que la force qui le porte avec A B <lb />vers C D, eſt à celle qui le porte le long de la mê-<lb />me A B, comme ( byp. </s>
          <s xml:space="preserve">) A C à A B; </s>
          <s xml:space="preserve">c’eſt-à-dire, en <lb />tirant H K par le point G parallele à A B, comme <lb />A K à K G: </s>
          <s xml:space="preserve">Donc ( ax. </s>
          <s xml:space="preserve">) au même tems que A B <lb />parcourt A K, &amp; </s>
          <s xml:space="preserve">qu’elle arrive avec le point A en <lb />H K, ce même point parcourt une partie de A B <lb />égale à K G; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent il ſe trouve alors <lb />en G. </s>
          <s xml:space="preserve">On démontrera de même qu’au même tems <lb />que A B arrive en C D, le point A ſe trouve en D; <lb /></s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">ainſi dans tous les autres points de la Diagona-<lb />le A D: </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent ce point ainſi pouſſé ſe
</s>
          <pb facs="0033" n="7" />
          <s xml:space="preserve"><fw type="head">ME’CHANIQUE.</fw>
meuvra exactement le long de cette ligne. </s>
          <s xml:space="preserve">Ce qu’il <lb />
<ptr xml:id="note-0033-01a" corresp="note-0033-01" type="noteAnchor" />
F. </s>
          <s xml:space="preserve">D.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0033-01" corresp="note-0033-01a" place="margin">LEMMES.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> I.</head>
        <p>
          <s xml:space="preserve">Quand bien même les forces dont agiſſent les puiſ-<lb />ſances E &amp; </s>
          <s xml:space="preserve">F augmenteroient ou diminuëroient, <lb />pourvu que ce fut ſuivant la même proportion de <lb />part &amp; </s>
          <s xml:space="preserve">d’autre; </s>
          <s xml:space="preserve">ce même point ſe meuvroit encore <lb />exactement le long de A D: </s>
          <s xml:space="preserve">parce que ces forces <lb />ſeroient encore entre-elles comme A C à A B, ou <lb />comme A K à K G.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> II.</head>
        <p>
          <s xml:space="preserve">C’eſt la même choſe que le point A ſoit pouſſé le <lb />long de A D par le concours d’action des puiſſances <lb />E &amp; </s>
          <s xml:space="preserve">F, ou qu’il y ſoit pouſſé par une ſeule puiſſance <lb />d’une viteſſe égale à celle que lui cauſent ces deux <lb />enſemble.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> III.</head>
        <p>
          <s xml:space="preserve">Puiſque le point A parcourt A D &amp; </s>
          <s xml:space="preserve">A B en même <lb />tems, la force, ou le compoſé de forces, qui le pouſ-<lb />ſe le long de A D, eſt à celle qui le pouſſe le long <lb />de A B, ( ax. </s>
          <s xml:space="preserve">) comme A D à A B. </s>
          <s xml:space="preserve">Et pour la même <lb />raiſon, elle eſt à celle dont il eſt pouſſé le long de <lb />A C, comme A D à A C.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0033-01" />
          <label>0033-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">LEMME IV.</head>
        <p rend="italics">
          <s xml:space="preserve">PRèſentement que le point A ſoit le centre de diréction <lb />
<ptr xml:id="note-0033-02a" corresp="note-0033-02" type="noteAnchor" />
du corps E F, &amp; </s>
          <s xml:space="preserve">que ce corps ſoit pouſſè en même tems <lb />&amp; </s>
          <s xml:space="preserve">uniformèment par deux puiſſances appliquées en E &amp; </s>
          <s xml:space="preserve"><lb />en F, ſuivant les lignes E C &amp; </s>
          <s xml:space="preserve">F B, qui paſſent par le <lb />point A, avec des forces qui ſoient entr’elles comme A C
</s>
          <pb facs="0034" n="8" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
&amp; </s>
          <s xml:space="preserve">A B: </s>
          <s xml:space="preserve">que l’on acbeve le parallelogramme B C, &amp; </s>
          <s xml:space="preserve">que <lb />
<ptr xml:id="note-0034-01a" corresp="note-0034-01" type="noteAnchor" />
l’on regarde pour un moment ce corps comme s’il n’avoit au-<lb />cune peſanteur. </s>
          <s xml:space="preserve">Quelque angle BAC que ces lignes faſſe<unclear reason="illegible" />nt <lb />entr’elles, ce corps ainſi pouſſè ſuivra la diagonale A D.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0033-02" corresp="note-0033-02a" place="margin">fig. 8.</note>
              <note xml:space="preserve" xml:id="note-0034-01" corresp="note-0034-01a" place="margin">LEMMES.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration</hi>.</head>
        <p>
          <s xml:space="preserve">Les lignes EC &amp; </s>
          <s xml:space="preserve">FB, ſuivant leſquelles les puiſ-<lb />ſances E &amp; </s>
          <s xml:space="preserve">F agiſſent, paſſant ( byp. </s>
          <s xml:space="preserve">) par le point A, <lb />il eſt pouſſé en même-tems, &amp; </s>
          <s xml:space="preserve">uniformement ſuivant <lb />ces mêmes lignes vers CD &amp; </s>
          <s xml:space="preserve">BD, par des forces <lb />qui ſont entr’elles, ( byp. </s>
          <s xml:space="preserve">) comme A C à A B: </s>
          <s xml:space="preserve">Donc <lb />( Lem. </s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve">) le point A, &amp; </s>
          <s xml:space="preserve">par conſéquent auſſi <lb />( Dem. </s>
          <s xml:space="preserve">) le corps EF ſuivra la diagonale AD. </s>
          <s xml:space="preserve">Ce <lb />qu’il F. </s>
          <s xml:space="preserve">D.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> I.</head>
        <p>
          <s xml:space="preserve">On voit que c’eſt la même choſe que le corps EF <lb />ſoit pouſſé ſuivant AD par le concours d’action de <lb />deux puiſſances appliquées en E, &amp; </s>
          <s xml:space="preserve">en F, ſuivant <lb />des lignes EC &amp; </s>
          <s xml:space="preserve">FB qui paſſent par ſon centre de <lb />gravité A, ou qu’il y ſoit pouſſé par une ſimple <lb />puiſſance d’une viteſſe égale à celle que lui cauſent <lb />ces deux enſemble: </s>
          <s xml:space="preserve">de ſorte que ſi AD étoit perpen-<lb />diculaire à l’horizon, &amp; </s>
          <s xml:space="preserve">que la peſanteur, que nous <lb />concevons préſentement être dans ce corps, l’em-<lb />portât le long de cette ligne avec une ſemblable vi-<lb />teſſe, il la ſuivroit de même que s’il n’avoit en effet <lb />aucune peſanteur, &amp; </s>
          <s xml:space="preserve">qu’il fût pouſſé de la maniére <lb />que nous venons de dire, par les deux puiſſances <lb />E &amp; </s>
          <s xml:space="preserve">F.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> II.</head>
        <p>
          <s xml:space="preserve">C’eſt pour cela auſſi que ce corps étant pouſſé par <lb />ſa peſanteur ſuivant A D perpendiculaire à l’hori-<lb />zon, s’il lui ſurvenoit quelqu’autre force qui le
</s>
          <pb facs="0035" n="9" />
          <s xml:space="preserve"><fw type="head">ME’CHANIQUE.</fw>
pouſſât de même ſuivant quelqu’autre ligne qui ren-<lb />
<ptr xml:id="note-0035-01a" corresp="note-0035-01" type="noteAnchor" />
contrât celle-cy; </s>
          <s xml:space="preserve">Quelque angle que ces deux lignes <lb />fiſſent entr’elles, ce corps ſuivroit la diagonale d’un <lb />parallelogramme fait ſous des parties de ces lignes, <lb />qui depuis le point de leur rencontre, fuſſent entre-<lb />elles, comme la peſanteur de ce poids &amp; </s>
          <s xml:space="preserve">cette nou-<lb />velle force: </s>
          <s xml:space="preserve">Il la ſuivroit, dis-je, de la même <lb />maniére que s’il n’étoit pouſſé que par une ſeule <lb />puiſſance ſuivant cette diréction, &amp; </s>
          <s xml:space="preserve">d’une viteſſe <lb />égale à celle que lui pouroient cauſer ces deux en-<lb />ſemble.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0035-01" corresp="note-0035-01a" place="margin">LEMMES.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> III.</head>
        <p>
          <s xml:space="preserve">Il ſuit encore de cette propoſition, &amp; </s>
          <s xml:space="preserve">du Corol-<lb />laire 3. </s>
          <s xml:space="preserve">du Lemme 3.</s>
          <s xml:space="preserve">, que la force dont le corps E F <lb />eſt pouſſé le long de A D, eſt à celle dont la puiſ-<lb />ſance F le pouſſe le long de A B, comme A D à A B; <lb /></s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">à celle dont la puiſſance E le pouſſe le long de A C, <lb />comme A D à A C.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0035-01" />
          <label>0035-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">LEMME V.</head>
        <p rend="italics">
          <s xml:space="preserve">L E S trois côtez d’un triangle réctiligne, quel qu’il ſoit, <lb />
<ptr xml:id="note-0035-02a" corresp="note-0035-02" type="noteAnchor" />
ſont entr’eux, comme les ſinus des angles auſquels ils <lb />ſont ooppoſez.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0035-02" corresp="note-0035-02a" place="margin">fig 9.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration</hi>.</head>
        <p>
          <s xml:space="preserve">Soit ABD tel triangle réctiligne qu’on voudra, <lb />inſcrit dans un cercle, dont C ſoit le centre; </s>
          <s xml:space="preserve">ſur <lb />quelqu’un de ſes côtez, comme A B, ſoit menée du <lb />centre C la perpendiculaire C E avec la ligne C A. <lb /></s>
          <s xml:space="preserve">Il eſt clair que A E eſt le ſinus de l’angle A C E, <lb />qui eſt égal à l’angle D; </s>
          <s xml:space="preserve">Donc A B eſt le double du
</s>
          <pb facs="0036" n="10" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
ſinus de l’angle D. </s>
          <s xml:space="preserve">Et pour la même raiſon, BD eſt <lb />
<ptr xml:id="note-0036-01a" corresp="note-0036-01" type="noteAnchor" />
le double du ſinus de l’angle BAD; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">AD le dou-<lb />ble auſſi de celui de l’angle B: </s>
          <s xml:space="preserve">Donc les trois côtez <lb />de cetriangle ſont entr’eux, comme le double du ſinus <lb />de chacun des angles auſquels ils ſont oppoſez: </s>
          <s xml:space="preserve">Donc <lb />ils ſont auſſi entr’eux, comme ces mêmes ſinus. </s>
          <s xml:space="preserve">Ce <lb />qu’il F. </s>
          <s xml:space="preserve">D.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0036-01" corresp="note-0036-01a" place="margin">LEMMES.</note>
            </div>
          </body>
        </floatingText>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0036-01" />
          <label>0036-01</label>
        </figure>
        <pb facs="0037" n="11" />
        <fw type="head">MECHANIQUE.</fw>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0037-01" />
          <label>0037-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">PROPOSITION <lb />FONDAMENTALE <lb />DES POIDS SUSPENDUS <lb />AVEC DES CORDES</head>
        <p>
          <s xml:space="preserve">En quelque nombre qu’elles ſoient; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">pour <lb />tousles angles poſſibles qu’elles peuvent faire <lb />entre-elles.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">LE Poids K ſoutenu avec les cordes P B &amp; </s>
          <s xml:space="preserve">C R par <lb />
<ptr xml:id="note-0037-01a" corresp="note-0037-01" type="noteAnchor" />
les puiſſances P &amp; </s>
          <s xml:space="preserve">R, &amp; </s>
          <s xml:space="preserve">en équilibre avec elles, eſt <lb />toujours à cbacune d’elles, comme le ſinus de l’angle P A R que <lb />leurs cordes font entre-elles, à chacun des ſinus des angles <lb />RAK &amp; </s>
          <s xml:space="preserve">PAK que font avec la ligne de direction AK <lb />de ce poids, chacune de ces cordes réciproquement priſes. </s>
          <s xml:space="preserve">Par <lb />exemple, il eſt à la puiſſance P, comme le ſinus de R A P <lb />au ſinus de R A K; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">à la puiſſance R, comme le mème <lb />ſinus de R A P au ſinus de P A K.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0037-01" corresp="note-0037-01a" place="margin">fig. 10. <lb />11. <lb />12. <lb />13. <lb />14. <lb />15. <lb />16. <lb />17.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration</hi>.</head>
        <p>
          <s xml:space="preserve">Les impreſſions particuliéres que font les puiſſances <lb />P &amp; </s>
          <s xml:space="preserve">R, ſur le point A de ce corps, (fig. </s>
          <s xml:space="preserve">10. </s>
          <s xml:space="preserve">11. </s>
          <s xml:space="preserve">12. <lb /></s>
          <s xml:space="preserve">13. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">14.) </s>
          <s xml:space="preserve">ou de ſa corde, (fig. </s>
          <s xml:space="preserve">15.) </s>
          <s xml:space="preserve">étant les mê-<lb />mes qu’elles feroient, ſi elles le pouſſoient chacune <lb />ſuivant ſa ligne de direction AP &amp; </s>
          <s xml:space="preserve">AR: </s>
          <s xml:space="preserve">1°. </s>
          <s xml:space="preserve">Ce
</s>
          <pb facs="0038" n="12" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
point regardé comme tiré ſeulement par ces deux <lb />
<ptr xml:id="note-0038-01a" corresp="note-0038-01" type="noteAnchor" />
puiſſances, doit tendre (Lemm. </s>
          <s xml:space="preserve">3.) </s>
          <s xml:space="preserve">le long de quelque <lb />ligne AD, quiſoit la diagonale d’un parallelogramme <lb />fait ſous des parties AB &amp; </s>
          <s xml:space="preserve">AC des lignes de direction <lb />des puiſſances P &amp; </s>
          <s xml:space="preserve">R, qui ſoient entre-elles, comme <lb />ces mêmes puiſſances. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Cette ligne AD doit être <lb />la même que la ligne de direction A K de ce poids <lb />prolongée du côté de D: </s>
          <s xml:space="preserve">autrement ces lignes A K <lb />&amp; </s>
          <s xml:space="preserve">AD faiſant en A quelque angle entre-elles, ce <lb />point ainſi pouſſé, ou tiré ſuivant la ligne AD par <lb />le concours d’action de ces puiſſances, &amp; </s>
          <s xml:space="preserve">à même <lb />tems ſuivant ſa ligne de direction A K par la peſan-<lb />teur du poids K, devroit (Lemm. </s>
          <s xml:space="preserve">3.) </s>
          <s xml:space="preserve">ſuivre une <lb />troiſiéme ligne qui fût la Diagonale d’un parallelo-<lb />gramme fait ſous des parties de ces lignes priſes de-<lb />puis A, &amp; </s>
          <s xml:space="preserve">qui fuſſent entre-elles, comme la force <lb />dont ce point eſt tiré par ces puiſſances ſuivant AD, <lb />eſt à la peſanteur du poids K; </s>
          <s xml:space="preserve">ainſi ce poids ne ſeroit <lb />plus en équilibre avec ces puiſſances, ce qui eſt contre <lb />l’hypothêſe. </s>
          <s xml:space="preserve">3°. </s>
          <s xml:space="preserve">La force dont ce point eſt tiré ſuivant <lb />AD, eſt auſſi égale à la peſanteur de ce poids; </s>
          <s xml:space="preserve">au-<lb />trement cette ligne étant la même que la ligne de di-<lb />rection de ce poids, il ſe meuvroit encore en haut, ou <lb />en bas ſelon la différence de ces forces, ce qui eſt <lb />encore contre l’hypothêſe: </s>
          <s xml:space="preserve">Donc ce point eſt tiré <lb />de A vers D par le concours d’action des puiſſances <lb />P &amp; </s>
          <s xml:space="preserve">R ſuivant la ligne de direction de ce poids, &amp; </s>
          <s xml:space="preserve"><lb />d’une force êgale à ſa peſanteur. </s>
          <s xml:space="preserve">Or la force dont il <lb />eſt ainſi tiré de A vers D, eſt à celle dont la puiſ-<lb />ſance P le tire à elle, comme (Lemm. </s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">3.) </s>
          <s xml:space="preserve">A D <lb />à A B; </s>
          <s xml:space="preserve">c’eſt-à-dire, (Lemm. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">comme le ſinus de <lb />l’angle D B A, ou de ſon complement PAR, (BC <lb />eſt un parallelogramme) au ſinus de l’angle BDA, <lb />ou de RAK égal à celui-ci, ou à ſon complement: <lb /></s>
          <s xml:space="preserve">Donc ce poids eſt à la puiſſance P, comme le ſinus
</s>
          <pb facs="0039" n="13" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
de l’angle PAR, au ſinus de l’angle RAK. </s>
          <s xml:space="preserve">On dé-<lb />
<ptr xml:id="note-0039-01a" corresp="note-0039-01" type="noteAnchor" />
montrera de même que ce même poids eſt à la puiſ-<lb />ſance R, comme le même ſinus de l’angle PAR, au <lb />ſinus de l’angle PAK.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0038-01" corresp="note-0038-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
              <note xml:space="preserve" xml:id="note-0039-01" corresp="note-0039-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">Voilà pour les ſix premiers cas. </s>
          <s xml:space="preserve">(fig. </s>
          <s xml:space="preserve">10. </s>
          <s xml:space="preserve">11. </s>
          <s xml:space="preserve">12. </s>
          <s xml:space="preserve">13. <lb /></s>
          <s xml:space="preserve">14. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">15.) </s>
          <s xml:space="preserve">Pour les deux autres, (fig. </s>
          <s xml:space="preserve">16. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">17.) </s>
          <s xml:space="preserve"><lb />il ne faut que concevoir le poids K de telle figure <lb />que le point A lui appartienne; </s>
          <s xml:space="preserve">c’eſt-à-dire qu’il lui <lb />ſoit continu, ſans àugmenter ny diminuër ſa peſan-<lb />teur, ni ſans changer ſon centre de gravité, non <lb />plus que les angles RAK &amp; </s>
          <s xml:space="preserve">PAK que font les <lb />cordes que tiennent les puiſſances P &amp; </s>
          <s xml:space="preserve">R, avec ſa <lb />ligne de direction A K. </s>
          <s xml:space="preserve">Or cela bien conçu, il eſt <lb />clair par ce qui vient d’être dit, que la peſanteur <lb />de tout le poids K eſt égale à la force dont le point A <lb />en ce cas ſeroit pouſſé, ou tiré de A vers D: </s>
          <s xml:space="preserve">ainſi <lb />une telle force étant (Lemm. </s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">3.) </s>
          <s xml:space="preserve">à celle de la <lb />puiſſance P, comme AD à AB; </s>
          <s xml:space="preserve">le poids K, qui eſt le <lb />même (byp.) </s>
          <s xml:space="preserve">que s’il avoit une telle figure, eſt encore <lb />ici à la puiſſance P, qui eſt encore auſſi (byp) la même, <lb />comme AD à AB; </s>
          <s xml:space="preserve">c’eſt-à-dire, (Lemm. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">comme <lb />le ſinus de l’angle DBA, ou de ſon complement PAR, <lb />au ſinus de l’angle BDA, ou de RAK qui lui eſt <lb />égal; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">de même à la puiſſance R, comme le ſinus <lb />du même angle PAR au ſinus de l’angle PAK.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">Et par conſéquent, quelque ſoit le poids K, &amp; </s>
          <s xml:space="preserve">de <lb />quelque maniére qu’il ſoit ſoutenu avec les cordes <lb />BP, &amp; </s>
          <s xml:space="preserve">CR par les puiſſances P &amp; </s>
          <s xml:space="preserve">R, il eſt toujours <lb />à chacune de ces puiſſances, comme le ſinus de l’an-<lb />gle que leurs cordes font entre-elles, à chacun des <lb />ſinus des angles que font chacune de ces cordes ré-<lb />ciproquement priſes avec ſa ligne de direction. </s>
          <s xml:space="preserve">Ce <lb />qu’il F. </s>
          <s xml:space="preserve">D.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">Ce ſeroit ici le lieu de répondre à la digreſſion que Monſieur
</s>
          <pb facs="0040" n="14" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
Borelli à faite contre ce ſentiment dans ſon Traité du mo u-<lb />
<ptr xml:id="note-0040-01a" corresp="note-0040-01" type="noteAnchor" />
vement des Animaux, tom. </s>
          <s xml:space="preserve">1. </s>
          <s xml:space="preserve">chap. </s>
          <s xml:space="preserve">13. </s>
          <s xml:space="preserve">Mais la bréveté <lb />qu’on s’eſt propoſée dans cet eſſay, ne permet pas de s’étendre <lb />ici autant qu’il faudroit pour cela: </s>
          <s xml:space="preserve">On en verra dans peu <lb />un examen particulier, où l’on fera voir en quoy cet Illuſtre <lb />Autbeur s’eſt mépris.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0040-01" corresp="note-0040-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> I.</head>
        <p>
          <s xml:space="preserve">Il ſuit de cette propoſition que les puiſſances P &amp; </s>
          <s xml:space="preserve"><lb />R ſont entr’elles en raiſon réciproque des ſinus des <lb />angles que font leurs lignes de direction avec celle <lb />du poid qu’elles ſoutiennent, c’eſt-à-dire, en raiſon <lb />réciproque des diſtances de leurs lignes de direction <lb />à celle de ce poids.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> II.</head>
        <p>
          <s xml:space="preserve">D’où l’on voit qu’en mettant une troiſiéme puiſ-<lb />ſance, dont le nom ſoit K, à la place de ce poids, <lb />qui faſſe équilibre, comme lui, avec les deux P &amp; </s>
          <s xml:space="preserve">R <lb />qui le ſoutiennent: </s>
          <s xml:space="preserve">ces trois puiſſances K, P, &amp; </s>
          <s xml:space="preserve">R <lb />ſeront entr’elles, comme les ſinus des angles P A R, <lb />RAK, &amp; </s>
          <s xml:space="preserve">PAK.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> III.</head>
        <p>
          <s xml:space="preserve">D’où il ſuit, non ſeulement que chacune de ces <lb />puiſſances, de quelque maniére qu’on les prenne, <lb />eſt toûjours plus petite que la ſomme des deux autres, <lb />de même que chacun de ces ſinus eſt toujours moin-<lb />dre que la ſomme des deux autres.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> IV.</head>
        <p>
          <s xml:space="preserve">Mais encore qu’elles ſont toutes trois priſes à <lb />diſcrétion deux à deux, en raiſon réciproque des ſinus <lb />des angles que font leurs cordes, ou leurs lignes de <lb />diréction avec celle de la troiſiéme; </s>
          <s xml:space="preserve">C’eſt-à-dire,
</s>
          <pb facs="0041" n="15" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
en raiſon réciproque des diſtances de leurs lignes de <lb />
<ptr xml:id="note-0041-01a" corresp="note-0041-01" type="noteAnchor" />
diréction à quelque point que ce ſoit de celle de la <lb />troiſiéme.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0041-01" corresp="note-0041-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Crollaire</hi> V.</head>
        <p>
          <s xml:space="preserve">Il ſuit encore de cette propoſition, que de quel-<lb />que côté que tende le corps K, ſoit que cette impreſ-<lb />ſion lui vienne de ſa peſanteur, ou de quelqu’autre <lb />force; </s>
          <s xml:space="preserve">celle de cette impreſſion, tant que ce corps <lb />ſera en équilibre avec les puiſſances P &amp; </s>
          <s xml:space="preserve">R, ſera <lb />toujours à celle dont chacune d’elles le retient, com-<lb />me le ſinus de l’angle P A R que font leurs cordes <lb />entr’elles, à chacun des ſinus des angles R A K &amp; </s>
          <s xml:space="preserve"><lb />PAK, que font chacune de ces cordes réciproque-<lb />ment priſes, avec la ligne de direction A K de ce <lb />corps, qui paſſe toûjours (Lem. </s>
          <s xml:space="preserve">2. </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">1.) </s>
          <s xml:space="preserve">par le <lb />point A de leur concours.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> VI.</head>
        <p>
          <s xml:space="preserve">Ce qui fait voir que ſi l’angle de ces cordes étoit infi-<lb />niment aigu, c’eſt-à-dire, qu’elles fuſſent paralleles <lb />entre-elles, la force, quelle qu’elle fût, dont ce corps <lb />agiroit contre ces puiſſances, ſeroit égale à la ſomme <lb />de celles dont elles lui reſiſtent: </s>
          <s xml:space="preserve">De ſorte que s’il <lb />agiſſoit ſeulement comme poids, il ſeroit alors égal <lb />à la ſomme de ces puiſſances; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">chacune d’elle ſeroit <lb />à l’autre en raiſon réciproque des diſtances de leurs <lb />lignes de direction à celle de ce corps, ou de ce poids, <lb />qui pour lors leur ſeroit (Lem. </s>
          <s xml:space="preserve">2. </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">2.) </s>
          <s xml:space="preserve">auſſi parallele.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> VII.</head>
        <p>
          <s xml:space="preserve">Il ſuit de plus, que ſi le poids K eſt à chacune des <lb />puiſſances P &amp; </s>
          <s xml:space="preserve">R, comme les ſinus de l’angle R A P, <lb />à chacun des ſinus des angles R A K &amp; </s>
          <s xml:space="preserve">P A K, elles <lb />le ſoutiendront en cet état, &amp; </s>
          <s xml:space="preserve">feront équilibre avec
</s>
          <pb facs="0042" n="16" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
lui: </s>
          <s xml:space="preserve">Car ces deux puiſſances étant alors entr’elles, <lb />
<ptr xml:id="note-0042-01a" corresp="note-0042-01" type="noteAnchor" />
comme les ſinus des angles BDA &amp; </s>
          <s xml:space="preserve">BAD, c’eſt-à-<lb />dire, (Lem. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">comme AB à BD, ou à CA qui lui <lb />eſt égale; </s>
          <s xml:space="preserve">l’impreſſion compoſée qui réſulte du <lb />concours d’action de ces deux puiſſances ſur le point <lb />A, doit (Lem. </s>
          <s xml:space="preserve">3.) </s>
          <s xml:space="preserve">le faire tendre de A vers D ſui-<lb />vant AD, d’une force qui ſoit à celle de chacune <lb />de ces puiſſances P &amp; </s>
          <s xml:space="preserve">R, (Lem. </s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">3.) </s>
          <s xml:space="preserve">comme <lb />AD eſt à chacun des côtez AB &amp; </s>
          <s xml:space="preserve">AC, ou BD, du <lb />parallelogramme BC; </s>
          <s xml:space="preserve">ou bien (Lemm. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">comme <lb />le ſinus de l’angle DBA, ou de ſon complement <lb />PAR, à chacun des ſinus des angles BDA &amp; </s>
          <s xml:space="preserve">BAD, <lb />ou de RAK &amp; </s>
          <s xml:space="preserve">de PAK, quileur ſontégaux, ou qui <lb />ſont leurs complemens; </s>
          <s xml:space="preserve">c’eſt-à-dire, (byp.) </s>
          <s xml:space="preserve">comme <lb />le poids K à chacune de ces puiſſances: </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſé-<lb />quent la force dont ces puiſſances tirent ou pouſſent <lb />le point A de ce corps, ou de ſa corde vers D, eſt <lb />égale à celle, dont il eſt tiré vers K ſuivant la même <lb />ligne DK par la peſanteur de ce poids: </s>
          <s xml:space="preserve">ainſi elles <lb />le doivent ſoutenir en cet état, &amp; </s>
          <s xml:space="preserve">demeurer en équi-<lb />libre avec lui.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0042-01" corresp="note-0042-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> VIII.</head>
        <p>
          <s xml:space="preserve">Ce qui fait voir que l’on peut faire ſoutenir quel-<lb />
<ptr xml:id="note-0042-02a" corresp="note-0042-02" type="noteAnchor" />
que grand poids K, que ce ſoit, à quelque puiſſance R <lb />que ce puiſſe être par le moyen d’une corde ſeulement. <lb /></s>
          <s xml:space="preserve">Il ne faut pour cela que de quelque point D comme <lb />centre, avec le rayon A D perpendiculaire à l’hori-<lb />zon, &amp; </s>
          <s xml:space="preserve">pris à diſcrétion, décrire l’arc A C B; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">y <lb />ayant inſcrit A C qui ſoit à A D, comme la puiſ-<lb />ſance R au poids K, joignez D C, &amp; </s>
          <s xml:space="preserve">apres avoir <lb />dirigé par le point A la corde A P de ce poids pa-<lb />rallelement à C D, attachez-la au crochet P, &amp; </s>
          <s xml:space="preserve">luy <lb />appliquez en A la puiſſance R ſuivant A C. </s>
          <s xml:space="preserve">Il eſt <lb />clair par le Corollaire précédent que cette puiſſance
</s>
          <pb facs="0043" n="17" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
étant (byp.) </s>
          <s xml:space="preserve">à ce poids comme A C à A D; </s>
          <s xml:space="preserve">c’eſt-à-<lb />
<ptr xml:id="note-0043-01a" corresp="note-0043-01" type="noteAnchor" />
dire, (Lemm. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">comme le ſinus de l’angle D, ou <lb />de ſon égal D A P, au ſinus de l’angle D C A, ou deſon <lb />complement PAC; </s>
          <s xml:space="preserve">elle ſe ſoutiendraen cet état.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0042-02" corresp="note-0042-02a" place="margin">fig. 18.</note>
              <note xml:space="preserve" xml:id="note-0043-01" corresp="note-0043-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> IX.</head>
        <p>
          <s xml:space="preserve">Ainſi il n’y a point de force R, quelque petite qu’on <lb />l’imagine, qui ne ſoit capable de mouvoir quelque <lb />grand poids K que ce ſoit, ſuſpendu à une corde, <lb />&amp; </s>
          <s xml:space="preserve">de le faire ſortir de la ligne PF qui tombe à plomb <lb />de ſon point de ſuſpenſion: </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">cela, juſqu’à ce que <lb />les ſinus des angles que font leurs lignes de direction <lb />AC &amp; </s>
          <s xml:space="preserve">AD avec AP, qui va du point où elles <lb />concourent, à ce point de ſuſpenſion, ſoient en raiſon <lb />réciproque de ce poids &amp; </s>
          <s xml:space="preserve">de cette puiſſance.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> X.</head>
        <p>
          <s xml:space="preserve">Et parce que ce mouvement eſt impoſſible, à moins <lb />que ce poids ne monte de même que le point A de ſa <lb />corde, du moins de la hauteur du ſinus verſe H E <lb />de l’angle APE fait par la partie AP de ſa corde, <lb />avec la ligne AF, qui tombe à plomb de ſon point A <lb />de ſuſpenſion: </s>
          <s xml:space="preserve">il ſuit évidemment qu’il n’y a point <lb />de force, quelque petite qu’on l’imagine, qui ne ſoit <lb />capable de faire monter du moins à cette hauteur <lb />quelque grand poids que ce ſoit à l’aide ſeulement <lb />d’une corde attachée à quelque point fixe.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">La raiſon pour laquelle on dit ici du moins, c’eſt pour <lb />s’ accommoder à toute bypothêſe: </s>
          <s xml:space="preserve">car ſi l’on regarde les lignes <lb />de direction des poids comme paralleles entre-elles, ce poids <lb />monte-ici juſtement de cette hauteur; </s>
          <s xml:space="preserve">mais ſi elles concourent <lb />en quelque endroit du monde, il doit néceſſairement monter <lb />plus baut, &amp; </s>
          <s xml:space="preserve">ce d’autant plus (quoi. </s>
          <s xml:space="preserve">qu’en proportion diffé-<lb />rente) que l’angle que fait ſa ligne de direction avec celle qui
</s>
          <pb facs="0044" n="18" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
tombe à plomb de ſon point de ſuſpenſion, lorſque ce poids <lb />
<ptr xml:id="note-0044-01a" corresp="note-0044-01" type="noteAnchor" />
n’eſt plus dans cette même ligne, eſt plus obtus. </s>
          <s xml:space="preserve">Tout cela eſt <lb />clair; </s>
          <s xml:space="preserve">c’eſt pourquoi on ne s’y arrête pas davantage.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0044-01" corresp="note-0044-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XI.</head>
        <p>
          <s xml:space="preserve">Il ſuit encore du Corollaire 7. </s>
          <s xml:space="preserve">que ſi au lieu du <lb />
<ptr xml:id="note-0044-02a" corresp="note-0044-02" type="noteAnchor" />
poid K, on mettoit quelque nouvelle puiſſance, (quel-<lb />le ſoit auſſi appellée K) qui fûtaux deux premiéres P <lb />&amp; </s>
          <s xml:space="preserve">R, commele ſinus de l’angle P A R, aux ſinus des <lb />angles RAK, &amp; </s>
          <s xml:space="preserve">PAK; </s>
          <s xml:space="preserve">c’eſt-à-dire, que ces trois <lb />puiſſances K, P, &amp; </s>
          <s xml:space="preserve">R fuſſent entr’elles, comme les <lb />ſinus de ces trois angles PAR, RAK, &amp; </s>
          <s xml:space="preserve">PAK; <lb /></s>
          <s xml:space="preserve">elles demeureroient en équilibre entr’elles, de ſorte <lb />qu’aucune ne l’emporteroit ſur aucune autre.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0044-02" corresp="note-0044-02a" place="margin">fig. 10. <lb />11. <lb />12. <lb />13. <lb />14. <lb />15. <lb />16. <lb />17.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XII.</head>
        <p>
          <s xml:space="preserve">Ce qui fait encore voir, que ſans rien changer à <lb />l’inclinaiſon des cordes B P &amp; </s>
          <s xml:space="preserve">C R de ces puiſſances, <lb />une infinité d’autres miſes en leurs places, pouront <lb />demeurer en équilibre trois à trois, pourvu qu’elles <lb />ſoient entr’elles, comme ces trois premiéres.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XIII.</head>
        <p>
          <s xml:space="preserve">On peut auſſi en changeant l’inclinaiſon de ces <lb />cordes conſerver l’équilibre de ces trois premiéres <lb />puiſſances K, P, &amp; </s>
          <s xml:space="preserve">R, dans ſix variations différentes <lb />de leurs angles, pourvu que ces puiſſances faſſent <lb />échange entr’elles de leurs cordes, juſqu’à ce que <lb />chacune d’elles ſe trouve appliquée ſucceſſivement <lb />à chacune de ces cordes pendant deux ſituations dif-<lb />férentes des deux autres. </s>
          <s xml:space="preserve">Pour l’appercevoir il ne faut <lb />que s’imaginer que lorſque deux de ces puiſſances, <lb />par exemple P &amp; </s>
          <s xml:space="preserve">R, font échange de leurs cordes, il <lb />ſe fait en même-tems une échange des angles que <lb />ces mêmes cordes faiſoient auparavant avec celle de
</s>
          <pb facs="0045" n="19" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
la puiſſance K, qui n’en change point alors, ſans qu’il <lb />
<ptr xml:id="note-0045-01a" corresp="note-0045-01" type="noteAnchor" />
arrive encore aucun changement à celui qu’elles font <lb />entr’elles: </s>
          <s xml:space="preserve">de cette maniére l’on aura deux des cas <lb />dont il eſt ici queſtion. </s>
          <s xml:space="preserve">On en trouvera encore deux <lb />en concevant de même l’échange des angles qui ſe <lb />fait dans l’échange des cordes de P &amp; </s>
          <s xml:space="preserve">de K; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">encore <lb />deux pour l’échange de celles de K &amp; </s>
          <s xml:space="preserve">de R: </s>
          <s xml:space="preserve">c’eſt ainſi <lb />qu’on les aura tous ſix.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0045-01" corresp="note-0045-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XIV.</head>
        <p>
          <s xml:space="preserve">Mais tant que chacune de ces puiſſances demeure <lb />appliquée à la même corde, l’on ne peut en changer <lb />la direction, c’eſt-à-dire, l’inclinaiſon de ces cordes, <lb />ſans en rompre l’équilibre; </s>
          <s xml:space="preserve">parce qu’il n’eſt pas poſ-<lb />ſible de trouver ſeulement deux ſituations de cordes, <lb />ou les ſinus de ces trois angles R A P, R A K, &amp; </s>
          <s xml:space="preserve">P A K, <lb />ayent le même raport entr’eux.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XV.</head>
        <p>
          <s xml:space="preserve">C’eſt ce qui fait que tout autant de fois que les <lb />angles RAP, que font entr’elles les cordes des puiſ-<lb />ſances P &amp; </s>
          <s xml:space="preserve">R, ſont différens, les poids qu’elles ſou-<lb />tiennent ſont différens auſſi. </s>
          <s xml:space="preserve">En effet plus cet angle <lb />eſt obtus, plus le poids qu elles ſoutiennent, doit être <lb />petit, quoi-qu’en proportion différente: </s>
          <s xml:space="preserve">puiſque plus <lb />cet angle eſt obtus, moins eſt grande la raiſon de AD <lb />à AB, &amp; </s>
          <s xml:space="preserve">à BD; </s>
          <s xml:space="preserve">c’eſt-à-dire, (Lemm. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">celle du <lb />ſinus de l’angle DBA, ou de ſon complement PAR, <lb />à chacun des ſinus de l’angle BDA, ou de RAK qui <lb />lui eſt égal, ou ſon complement; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">de l’angle BAD, <lb />ou PAK encore égal à celui-ci, ou ſon complement: <lb /></s>
          <s xml:space="preserve">qui eſt juſtement celle que ce poids doit alors avoir à <lb />chacune de ces puiſſances pour demeurer en équilibre <lb />avec elles; </s>
          <s xml:space="preserve">De ſorte que cet angle peut être ſi obtus <lb />que ces mêmes puiſſances pourront faire équilibre
</s>
          <pb facs="0046" n="20" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
avec ce poids, quelque petit qu’il ſoit: </s>
          <s xml:space="preserve">c’eſt ainſi qu’il <lb />
<ptr xml:id="note-0046-01a" corresp="note-0046-01" type="noteAnchor" />
peut diminuer à l’infini, &amp; </s>
          <s xml:space="preserve">faire cependant tou-<lb />jours équilibre avec elles, que@ques grandes qu’on les <lb />ſuppoſe.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0046-01" corresp="note-0046-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XVI.</head>
        <p>
          <s xml:space="preserve">Voilà ce qui peut arriver en changeant la direction <lb />de l’une, &amp; </s>
          <s xml:space="preserve">de l’autre de ces deux puiſſances; </s>
          <s xml:space="preserve">Mais à <lb />n’en déplacer qu’une: </s>
          <s xml:space="preserve">1°. </s>
          <s xml:space="preserve">Si elles ſont égales, ou ſi <lb />étant inégales, il s’en trouve une qui ait une direc-<lb />tion horizontale, il eſt clair qu’on changeroit le ra-<lb />port des ſinus des angles que leurs cordes font avec <lb />la ligne de direction du poids qu’elles ſoutiennent: <lb /></s>
          <s xml:space="preserve">ainſi (Cor. </s>
          <s xml:space="preserve">I.) </s>
          <s xml:space="preserve">elles ne pouroient plus ſoutenir n’y ce <lb />poids, ny aucun autre. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Au contraire ſi étant inéga-<lb />les, elles n’ont aucune de leurs cordes qui ſoit hori-<lb />zontale; </s>
          <s xml:space="preserve">au lieu du poids qu’elles ſoutiennent, on <lb />poura encore leur en faire ſoutenir un autre, pourvu <lb />qu’on change tellement celle de leurs directions qui <lb />fait le plus grand angle avec celle du poids qu’elles <lb />ſoutiennent, qu’on lui en faſſe faire un autre encore <lb />avec elle, qui ſoit le complement du premier: </s>
          <s xml:space="preserve">Car <lb />les ſinus des angles de leurs cordes avec la direction <lb />du poids appliqué à leur point de concours, étant <lb />encore les mêmes qu’auparavant, elles en pouront <lb />encore ſoutenir un (Cor. </s>
          <s xml:space="preserve">II.) </s>
          <s xml:space="preserve">à qui elles ſeront com-<lb />me ces mêmes ſinus réciproquement pris, à celui de <lb />l’angle que feront alors leurs cordes entr’elles; </s>
          <s xml:space="preserve">c’eſt-<lb />à-dire, qui ſera à celui qu’elles ſoutenoient aupara-<lb />vant, comme ce dernier ſinus à celui de l’angle qu’el-<lb />les faiſoient alors entr’elles. </s>
          <s xml:space="preserve">Mais auſſi par une raiſon <lb />toute contraire en tout autre changement de cette <lb />lignede direction ces deux puiſſances ne peuvent plus <lb />rien ſoutenir.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0047" n="21" />
        <fw type="head">MECHANIQUE.</fw>
        <p rend="italics">
          <s xml:space="preserve">La raiſon pour laquelle on vient de demander que ce <lb />
<ptr xml:id="note-0047-01a" corresp="note-0047-01" type="noteAnchor" />
changement ſe fit dans celle des directions de ces puiſſances, qui <lb />fait le plus grand angle avec celle du poids qu’elles ſoutien-<lb />nent; </s>
          <s xml:space="preserve">c’eſt que ſi l’on faiſoit un tel cbangement à l’autre, l’an-<lb />gle des cordes ſe tourneroit en deſſous, ce qui détermineroit <lb />l’action de ces deux puiſſances à ſeconder ſa peſanteur, plutôt <lb />qu’àla ſoutenir.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0047-01" corresp="note-0047-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />d s cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XVII.</head>
        <p>
          <s xml:space="preserve">Puiſque ce poids pour faire équilibre avec les <lb />puiſſances P &amp; </s>
          <s xml:space="preserve">R, doit toujours être à chacune d’elles, <lb />comme le ſinus de l’angle PAR de leurs cordes, à <lb />chacun des ſinus des angles RAK &amp; </s>
          <s xml:space="preserve">PAK: </s>
          <s xml:space="preserve">Il ſuit <lb />évidemment que ſi enfin cet angle, à force de deve-<lb />nir obtus, devenoit à rien; </s>
          <s xml:space="preserve">c’eſt-à-dire, que R A &amp; </s>
          <s xml:space="preserve"><lb />AP ne fiſſent plus qu’une même ligne droite, ce poids <lb />ſeroit auſſi réduit à rien, &amp; </s>
          <s xml:space="preserve">ces deux puiſſances agi-<lb />roient ſeulement alors l’une contre l’autre: </s>
          <s xml:space="preserve">ainſi tant <lb />qu’il reſte quelque poids attaché à ces cordes entre ces <lb />puiſſances, elles font toujours quelque angle PAR <lb />que ce ſoit.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XVIII.</head>
        <p>
          <s xml:space="preserve">De-là on voit qu’il n’y a point de force imaginable, <lb />n’y de poids, quelques grands qu’on les conçoive, qui <lb />appliquez aux extrémitez d’une corde parfaitement <lb />fléxible, la puiſſent tellement bander qu’elle devienne <lb />parfaitement droite, pour peu de peſanteur qu’on y <lb />ſuppoſe: </s>
          <s xml:space="preserve">car quelque prodigieuſe que ſoit cette force, <lb />&amp; </s>
          <s xml:space="preserve">quelques grands que ſoient ces poids, ils auront <lb />toujours quelque raport à la peſanteur de cette corde: <lb /></s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent elle ſe courbera toujours.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">Iuſqu’ici nous n’avons eu aucun égard à cette peſan-<lb />@eur de cordes, c’eſt pour cela que nous n’y avons conſidéré
</s>
          <pb facs="0048" n="22" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
que l’angle qu’elles font entr’elles à l’endroit ou le poids <lb />
<ptr xml:id="note-0048-01a" corresp="note-0048-01" type="noteAnchor" />
qu’elles ſoutiennent, leur eſt attacbé: </s>
          <s xml:space="preserve">ce ſera en les conſidé-<lb />rant de même que nous prendrons quelque jour leur peſanteur <lb />pourune infinité de poids, qui leur étant appliquez dans toute <lb />leur longueur, leur font faire une infinité d’angles quinous ſer-<lb />viront à en déterminer la courbure pour toutes ſortes d’bypo-<lb />theſes.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0048-01" corresp="note-0048-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XIX.</head>
        <p>
          <s xml:space="preserve">On pourroit encore de même démontrer le raport <lb />du poids K ſuſpendu partrois cordes, ou par davanta-<lb />ge, même juſqu’à l’infini, aux puiſſances qui le ſou-<lb />tiendroient; </s>
          <s xml:space="preserve">en prenant pour une ſeule, l’impreſſion <lb />compoſée de chacun des points, ou deux de ces cor-<lb />des concourent, laquelle réſulte du concours d’action <lb />des deux puiſſances qui y ſont appliquées; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">ainſi <lb />toujours de même, juſqu’à ce qu’enfin toutes ces <lb />puiſſances, en quelque nombre qu’elles ſoient, fuſſent <lb />réduites à deux ſeulement: </s>
          <s xml:space="preserve">ce qui réduiroit toujours <lb />tous ces cas, quclques différens qu’ils fuſſent, à celui <lb />de la propoſition préſente, qui pour cela a été appel-<lb />lée Fondamentale.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Remarque</hi>.</head>
        <p>
          <s xml:space="preserve">Lorſque de chacun des nocuds qui lient enſemble les <lb />cordes avec leſquelles un poids eſt ſoutenu par plu-<lb />ſieurs puiſſances, ſuivant chacune ſa direction, il <lb />ne s’en répand point plus de trois dans un même <lb />plan; </s>
          <s xml:space="preserve">alors cette réduction ſe peut faire ſans con-<lb />noître aucun raport entre ces puiſſances, n’y d’au-<lb />cune d’elles à ce poids. </s>
          <s xml:space="preserve">Mais lorſque le contraire <lb />arrive, c’eſt-à-dire, lorſque d’un même næud il ſe <lb />répand plus de trois cordes dans un même plan; </s>
          <s xml:space="preserve">alors <lb />pour chacun de ces plans, il faut connoître entre leſ-<lb />quelles on voudra des forces qui y ſont appliquées.</s>
          <s xml:space="preserve">
</s>
          <pb facs="0049" n="23" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
autant de raports, moins trois, qu’il y aura de telles <lb />
<ptr xml:id="note-0049-01a" corresp="note-0049-01" type="noteAnchor" />
forces, ou qu’un même noeud y répandra de cordes. <lb /></s>
          <s xml:space="preserve">Par exemple, pour 4. </s>
          <s xml:space="preserve">cordes, il ne faudra connoître <lb />qu’un tel raport. </s>
          <s xml:space="preserve">Pour 5. </s>
          <s xml:space="preserve">il en faudra 2. </s>
          <s xml:space="preserve">Pour 6. </s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve"><lb />Pour 7. </s>
          <s xml:space="preserve">4. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">ainſi toujours 3. </s>
          <s xml:space="preserve">moins que le nombre <lb />de ces cordes.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0049-01" corresp="note-0049-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſ@u-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <p rend="italics">
          <s xml:space="preserve">On n’entre point dans le détail de tout ceci, de peur de ſe <lb />trop éloigner de la breveté qu’on s’eſt propoſée; </s>
          <s xml:space="preserve">outre qu’en voi-<lb />la, ce me ſemble, aſſez pour juger de l’étenduë &amp; </s>
          <s xml:space="preserve">de la fécondité <lb />de ces principes: </s>
          <s xml:space="preserve">on le verra démontré dans un autre ouvrage.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0049-01" />
          <label>0049-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">PROBLEME.</head>
        <p rend="italics">
          <s xml:space="preserve">LEs forces de trois bommes K, P, &amp; </s>
          <s xml:space="preserve">R, étant données, <lb />ou même ſeulement le raport qu’elles ont entr’elles, les <lb />appliquer tellement à trois cordes A K, A P, &amp; </s>
          <s xml:space="preserve">A R, qui <lb />aboutiſſent à un même næud A, qu’aucun des trois ne l’emporte <lb />ſur aucun des deux autres.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Solution</hi>.</head>
        <p>
          <s xml:space="preserve">Premièremènt, s’il y a quelqu’une des forces de <lb />ces trois perſonnes, qui ſoit égale, ou plus grande que <lb />la ſomme de celles des deux autres, ce Problême par <lb />le Corollaire 3. </s>
          <s xml:space="preserve">de la propoſition préſente eſt impoſ-<lb />ſible.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">Secondement ſi chacune de ces forces, de quelque <lb />maniére qu’on les prenne, eſt en effet moindre que <lb />la ſomme des deux autres; </s>
          <s xml:space="preserve">placez à diſcretion une de <lb />ces trois perſonnes, par exemple K, &amp; </s>
          <s xml:space="preserve">lui donnez la <lb />direction AK qu’il vous plaira. </s>
          <s xml:space="preserve">Ayant prolongé à <lb />diſcretion AK du côté de E, faite ſur AE le triangle <lb />AEF, tel que ſes trois côtez AE, EF, &amp; </s>
          <s xml:space="preserve">AF, ſoient <lb />entr’eux, comme les forces de ces trois perſonnes K,
</s>
          <pb facs="0050" n="24" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
P, &amp; </s>
          <s xml:space="preserve">R. </s>
          <s xml:space="preserve">Placez enſuite la perſonne R ſuivant le côté <lb />
<ptr xml:id="note-0050-01a" corresp="note-0050-01" type="noteAnchor" />
AF de ce triangle, &amp; </s>
          <s xml:space="preserve">la perſonne P ſuivant AP paral-<lb />lele à EF. </s>
          <s xml:space="preserve">Cela fait, ces trois hommes ſeront dans la <lb />ſituation requiſe pour demeurer en équilibre.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0050-01" corresp="note-0050-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration</hi></head>
        <p>
          <s xml:space="preserve">Leurs forces K, P, &amp; </s>
          <s xml:space="preserve">R ſont (Hyp.) </s>
          <s xml:space="preserve">entr’elles, <lb />comme AE, EF, &amp; </s>
          <s xml:space="preserve">AF; </s>
          <s xml:space="preserve">C’eſt-à-dire, (Lemm. </s>
          <s xml:space="preserve">5.) <lb /></s>
          <s xml:space="preserve">comme les ſinus des angles AFE, EAF, &amp; </s>
          <s xml:space="preserve">AEF, <lb />qui ſont les mêmes que ceux desangles PAR, RAK, <lb />&amp; </s>
          <s xml:space="preserve">PAK: </s>
          <s xml:space="preserve">Donc (Corol. </s>
          <s xml:space="preserve">II.) </s>
          <s xml:space="preserve">ces trois hommes demeu-<lb />reront ainſien équilibre, ſans qu’aucun d’eux le puiſſe <lb />emporter ſur lequel que ce ſoit de deux autres. </s>
          <s xml:space="preserve">Ce <lb />qu’il faloit faire.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0050-01" />
          <label>0050-01</label>
        </figure>
        <pb facs="0051" n="25" />
        <fw type="head">MECHANIQUE.</fw>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0051-01" />
          <label>0051-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">PROPOSITION <lb />FONDAMENTALE <lb />DES POULIES,</head>
        <p>
          <s xml:space="preserve">Soit que le centre en demeure fixe, ſoit qu’on <lb />le ſuppoſe mobile; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">pour toutes les <lb />directions poſſibles des puiſſances, ou des <lb />poids qui y ſont appliquez.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">SOit la puiſſance, ou le poids D appliquè, ou ſuſpendu <lb />
<ptr xml:id="note-0051-01a" corresp="note-0051-01" type="noteAnchor" />
au centre mobile d’une poulie A, autour de laquelle paſſe <lb />la corde PMNR, dont les extremitez ſont retenuës par <lb />les puiſſances P &amp; </s>
          <s xml:space="preserve">R: </s>
          <s xml:space="preserve">quelque angle MHN que faſ-<lb />ſent entre-elles les parties MP, &amp; </s>
          <s xml:space="preserve">NR de cette corde, <lb />prolongées juſqu’àce qu’elles concourent en H; </s>
          <s xml:space="preserve">le poids, ou la <lb />puiſſance D, ſera toujours à cbacune des puiſſances P &amp; </s>
          <s xml:space="preserve">R, <lb />comme le ſinus de cet angle, au ſinus de ſa moitié.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0051-01" corresp="note-0051-01a" place="margin">fig. 20 <lb />21. <lb />22. <lb />23.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration.</hi></head>
        <p>
          <s xml:space="preserve">Il eſt clair que tant quele poids, ou la puiſſance D, <lb />demeure ainſi en équilibre avec les puiſſances P &amp; </s>
          <s xml:space="preserve">R <lb />ſur la poulie A, non-ſeulement cette poulie demeure <lb />ſans mouvement; </s>
          <s xml:space="preserve">mais encore la corde PMNR de-<lb />meure fixe deſſus ſans gliſſer, n’y ſe mouvoir non plus <lb />que ſi elley étoit colée, ou phyſiquement unie depuis</s>
        </p>
        <pb facs="0052" n="26" />
        <fw type="head">NOUVELLE</fw>
        <p>
          <s xml:space="preserve">M juſqu’à N; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">les points M, &amp; </s>
          <s xml:space="preserve">N de cette corde <lb />
<ptr xml:id="note-0052-01a" corresp="note-0052-01" type="noteAnchor" />
ſont auſſi fixes ſur cette poulie, tant que dure cet <lb />équilibre, que ſi en effet PM, &amp; </s>
          <s xml:space="preserve">RN étoient deux <lb />cordes, qui y fuſſent ſéparément attachées: </s>
          <s xml:space="preserve">Les puiſ-<lb />ſances P, &amp; </s>
          <s xml:space="preserve">R reſi ſtent donc au poids, ou à la puiſſan-<lb />ce D, de même que ſi MP, &amp; </s>
          <s xml:space="preserve">RN étoient deux cor-<lb />des différentes &amp; </s>
          <s xml:space="preserve">attachées aux points M &amp; </s>
          <s xml:space="preserve">N de la <lb />poulie A, ſuivant les tangentes en cespoints: </s>
          <s xml:space="preserve">De ſorte <lb />que l’on peut regarder cette poulie comme un corps <lb />qui tend vers D, ſuivant AD, d’une force égale à <lb />celle du poids, ou de la puiſſance D; </s>
          <s xml:space="preserve">mais qui eſt re-<lb />tenu avec les cordes PM &amp; </s>
          <s xml:space="preserve">RN par les puiſſances <lb />P &amp; </s>
          <s xml:space="preserve">R. </s>
          <s xml:space="preserve">Or en ce cas, non-ſeulement ſa ligne de di-<lb />rection AD paſſeroit (Lemm. </s>
          <s xml:space="preserve">2. </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">1.) </s>
          <s xml:space="preserve">par le point H, <lb />ou concourent ces cordes prolongées; </s>
          <s xml:space="preserve">mais encore <lb />cette poulie regardée avec une telle impreſſion, ſeroit <lb />(prop. </s>
          <s xml:space="preserve">fond. </s>
          <s xml:space="preserve">des cordes. </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">aux puiſſances P, &amp; </s>
          <s xml:space="preserve">R, <lb />qui la retiennent, comme le finus de l’angle MHN, <lb />aux ſinus des angles NHA, &amp; </s>
          <s xml:space="preserve">MHA: </s>
          <s xml:space="preserve">Donc en effet <lb />la ligne de direction AD de la poulie A ainſi tirée <lb />par le poids, ou la puiſſance D, contre les puiſſances <lb />P &amp; </s>
          <s xml:space="preserve">R, paſſe toujours par le point H, ou leurs cordes <lb />prolongées concourent; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">le poids, ou la puiſſance <lb />D, eſt auſſi à chacune de ces puiſſances, comme le <lb />ſinus de l’angle MHN à chacun des ſinus des angles <lb />NHA, &amp; </s>
          <s xml:space="preserve">MHA. </s>
          <s xml:space="preserve">Or à cauſe que HA, paſſe auſſi <lb />parle centre de cette poulie, &amp; </s>
          <s xml:space="preserve">que MH, &amp; </s>
          <s xml:space="preserve">NH ſont <lb />deux tangentes, les angles NHA, &amp; </s>
          <s xml:space="preserve">MHA, ſont <lb />chacun la moitié de l’angle MHN: </s>
          <s xml:space="preserve">Donc le poids, <lb />ou la puiſſance D, eſt toujours à chacune de puiſſan-<lb />ces P &amp; </s>
          <s xml:space="preserve">R, comme le ſinus de l’angle MHN, que <lb />ſont leurs cordes entr’elles, au ſinus de ſa moitié. </s>
          <s xml:space="preserve">Ce <lb />qu’il faloit démontrer.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0052-01" corresp="note-0052-01a" place="margin">DES <lb />POULIES.</note>
            </div>
          </body>
        </floatingText>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0052-01" />
          <label>0052-01</label>
        </figure>
        <pb facs="0053" n="27" />
        <fw type="head">MECHANIQUE.</fw>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> I.</head>
        <note xml:space="preserve" place="margin">DES <lb />POULIES.</note>
        <p>
          <s xml:space="preserve">Il ſuit de-là que le poids, ou la puiſſance D, tant <lb />que dure cet équilibre, eſt toujours à chacune des <lb />puiſſances P, &amp; </s>
          <s xml:space="preserve">R, en raiſon réciproque des ſinus des <lb />angles que font les lignes de direction de ce poids, &amp; </s>
          <s xml:space="preserve"><lb />de cette puiſſance avec celle de l’autre; </s>
          <s xml:space="preserve">c’eſt-à-dire, <lb />en raiſon réciproque des diſtances des lignes de di-<lb />rection de ce poids &amp; </s>
          <s xml:space="preserve">de cette puiſſance, à quelque <lb />point que ce ſoit de celle de l’autre. </s>
          <s xml:space="preserve">Et pour la même <lb />raiſon les puiſſances P &amp; </s>
          <s xml:space="preserve">R ſont auſſi entr’elles en <lb />raiſon rèciproque des diſtances de leurs lignes de di-<lb />rection à quelque point que ce ſoit de celle du poids, <lb />ou de la puiſſance D, qu’elles ſoutiennent.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> II.</head>
        <p>
          <s xml:space="preserve">Si la puiſſance, ou le poids D, (le tout étant <lb />appliqué à la poulie A comme cy-deſſus) eſt à chacune <lb />des puiſſances P, &amp; </s>
          <s xml:space="preserve">R, comme le ſinus de l’angle <lb />MHN, que font leurs cordes entr’elles, au ſinus de <lb />ſa moitié; </s>
          <s xml:space="preserve">elles le ſoutiendront en cet état: </s>
          <s xml:space="preserve">parce <lb />que cette raiſon étant la même qu’il doit avoir aux <lb />puiſſances qui l’y pourroient ſoutenir; </s>
          <s xml:space="preserve">les puiſſances <lb />p, &amp; </s>
          <s xml:space="preserve">R leur ſont néceſſairement égales; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſé-<lb />quent étant appliquées de même, elles l’y doivent <lb />auſſi ſoutenir.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> III.</head>
        <p>
          <s xml:space="preserve">Ce qui fait voir que lorſque lepoids D, eſt à cha-<lb />cune des puiſſances P, &amp; </s>
          <s xml:space="preserve">R, en raiſon réciproque des <lb />diſtances des lignes de direction de ce poids, &amp; </s>
          <s xml:space="preserve">de <lb />cette puiſſance, à quelque point que ce ſoit de celle <lb />de l’autre, il demeure en équilibre avec elles. </s>
          <s xml:space="preserve">Ce <lb />qu’on dit du poids D ſe doit auſſi de la puiſſance D.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0054" n="28" />
        <fw type="head">NOUVELLE</fw>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> IV.</head>
        <note xml:space="preserve" place="margin">DES <lb />POULIES.</note>
        <p>
          <s xml:space="preserve">Il ſuit de plus de cette propoſition que les puiſ-<lb />ſances P, &amp; </s>
          <s xml:space="preserve">R agiſſent contre la puiſſance, ou le poids <lb />D; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">ce poids, ou cette puiſſance réciproquement <lb />auſſi contr’elles, de la même maniére que ſi leurs cor-<lb />des PM, &amp; </s>
          <s xml:space="preserve">RN, prolongées juſqu’en H, y etoient <lb />noiiées avec la corde AD du poids, ou de la puiſſance <lb />D; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">que la poulie A étant ôtée, elles tiraſſent contre <lb />ce poids, ou contre cette puiſſance ſuivant les mêmes <lb />angles MHA, &amp; </s>
          <s xml:space="preserve">NHA: </s>
          <s xml:space="preserve">puis qu’alors le poids, ou la <lb />puiſſance D ſeroit encore (prop. </s>
          <s xml:space="preserve">fond. </s>
          <s xml:space="preserve">des cordes. </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">2. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve"><lb />5.) </s>
          <s xml:space="preserve">à chacune d’elles, comme le ſinus de l’angle MHN <lb />de leurs cordes, au ſinus de la moitié de cet angle. <lb /></s>
          <s xml:space="preserve">Ainſi que les puiſſances P &amp; </s>
          <s xml:space="preserve">R ſoutiennent le poids, <lb />ou la puiſſance D, par le moyen de la poulie A, avec <lb />la même corde PMNR; </s>
          <s xml:space="preserve">ou qu’elles ſoutiennent l’un <lb />ou l’autre ſans poulie, mais avec chacune une corde <lb />PH, &amp; </s>
          <s xml:space="preserve">RH, noiiée avec AD en H; </s>
          <s xml:space="preserve">C’eſt toujours <lb />la même choſe, pourvu que les angles de ces cordes <lb />avec la ligne de direction du poids, ou de la puiſſan-<lb />ce D, ſoient les mêmes dans l’un &amp; </s>
          <s xml:space="preserve">l’autre cas.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> V.</head>
        <p>
          <s xml:space="preserve">On voit encore que ſi au lieu du poids, ou de la <lb />puiſſance D, on attachoit la corde AD à quelque <lb />clou, comme en D, ou ailleurs; </s>
          <s xml:space="preserve">ce clou feroit la même <lb />réſiſtance contre les puiſſances P, &amp; </s>
          <s xml:space="preserve">R, que fait pré-<lb />ſentement le poids, ou la puiſſance D: </s>
          <s xml:space="preserve">ainſi n’étant <lb />arrivé aucun changement du côté de ces puiſſances, <lb />la direction de la corde AD ſeroit non ſeulement en-<lb />core la même qu’auparavant, c’eſt-à-dire, qu’elle <lb />diviſeroit encore l’angle MHN en deux parties éga-<lb />les; </s>
          <s xml:space="preserve">mais encore la réſiſtance de ce clou ſeroit égale <lb />à celle du poids, ou de la puiſſance D: </s>
          <s xml:space="preserve">D’où il ſuit</s>
        </p>
        <pb facs="0055" n="29" />
        <fw type="head">MECHANIQUE.</fw>
        <p>
          <s xml:space="preserve">I°. </s>
          <s xml:space="preserve">Que lors qu’une poulie ſur laquelle deux puiſſan-<lb />
<ptr xml:id="note-0055-01a" corresp="note-0055-01" type="noteAnchor" />
ces font équilibre, comme ici P &amp; </s>
          <s xml:space="preserve">R, eſt ſuſpenduë <lb />ou retenuë par une corde telle qu’eſt ici AD, cette <lb />corde ſe dirige toujours en ſorte qu’elle diviſe en <lb />deux également l’angle des tangentes de cette poulie <lb />aux points ou les cordes de ces puiſſances la touchent. <lb /></s>
          <s xml:space="preserve">(Il eſt clair que la même choſe arriveroit, ſi au lieu <lb />de ces puiſſances on appliquoit à leurs cordes des poids <lb />qui demeuraſſent de même en équilibre ſur cette pou-<lb />lie) 2°. </s>
          <s xml:space="preserve">La charge du clou, ou la corde qui retient cette <lb />poulie, eſt attachée, étant égale à la réſiſtance qu’il fait <lb />contre chacune de ces puiſſances, ou des poids mis en <lb />leurs places; </s>
          <s xml:space="preserve">eſt à chacun d’eux, ou d’elles, comme le <lb />ſinus de l’angle de ces tangentes, au ſinus de ſa moitié.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0055-01" corresp="note-0055-01a" place="margin">DES <lb />POULIES.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> VI.</head>
        <p>
          <s xml:space="preserve">Préſentement ſi la poulie A, au lieu d’être arrêtée <lb />en D, ou en quelqu’autre point de ſa corde AD, <lb />étoit ſeulement fixe en ſon centre A; </s>
          <s xml:space="preserve">les puiſſances <lb />P &amp; </s>
          <s xml:space="preserve">R agiſſant encore deſſus de la même maniére <lb />qu’auparavant, &amp; </s>
          <s xml:space="preserve">cette poulie leur faiſant auſſi en-<lb />core la même réſiſtance qu’elle leur faiſoit, lors qu’elle <lb />étoit retenuë parla corde AH; </s>
          <s xml:space="preserve">elle doit en recevoir <lb />encore la même impreſſion, &amp; </s>
          <s xml:space="preserve">ſuivant la même di-<lb />rection qu’auparavant: </s>
          <s xml:space="preserve">Ainſi l’effort commun des <lb />puiſſances P &amp; </s>
          <s xml:space="preserve">R ſur cette poulie, ne tend encore <lb />qu’à la mouvoir ſuivant HA avec la même force dont <lb />elles tiroient auparavant contre le poids, ou la puiſ-<lb />ſance D, ou contre le clou qu’on vient de ſuſpoſer en <lb />D: </s>
          <s xml:space="preserve">de ſorte que la charge de cette poulie, lors qu’elle eſt <lb />fixe, eſt toujours à chacune des puiſſances P &amp; </s>
          <s xml:space="preserve">R, ou <lb />à chacun des poids qui leur étant égaux, ſeroient mis <lb />en leurs places, comme le ſinus de l’angle de leurs par-<lb />ties de cordes PM &amp; </s>
          <s xml:space="preserve">RN prolongées juſqu’à ce <lb />qu’elles concourent, au ſinus de ſa moitié.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0056" n="30" />
        <fw type="head">NOUVELLE</fw>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> VII.</head>
        <note xml:space="preserve" place="margin">DES <lb />POULIES.</note>
        <p>
          <s xml:space="preserve">D’où il ſuit que plus l’angle MHN, que ces par-<lb />ties de corde prolongées du côté de H, font entr’elles, <lb />ſera obtus, moins ſera grande la charge de la poulie A, <lb />ſoit que le centre en ſoit fixe, ou qu’il ſoit mobile: <lb /></s>
          <s xml:space="preserve">parce que plus cet angle ſera obtus, moins ſera grande <lb />la raiſon de ſon ſinus au ſinus de ſa moitié, quoi qu’en <lb />proportion difféentes: </s>
          <s xml:space="preserve">De ſorte que cet angle peut <lb />être ſi obtus, que la poulie A ne ſera chargée que ſi <lb />peu qu’on voudra des puiſſances P &amp; </s>
          <s xml:space="preserve">R: </s>
          <s xml:space="preserve">juſques-là <lb />même qu’elle pourroit être ſoutenuë contre elles <lb />par une puiſſance, ou un poids D indéfiniment petit, <lb />c’eſt-à-dire, moindre que quelque poids donné, que <lb />ce ſoit: </s>
          <s xml:space="preserve">Car il ne faut pour cela qu’ouvrir l’angle <lb />MHN, que font entr’elles les parties de corde PM <lb />&amp; </s>
          <s xml:space="preserve">RN, juſqu’à ce qu’enfin ſon ſinus ſoit au ſinus de <lb />ſa moitié en moindre raiſon que le poids donné, à <lb />chacune des puiſſances P &amp; </s>
          <s xml:space="preserve">R.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> VIII.</head>
        <p>
          <s xml:space="preserve">Au contraire on peut rendre cet angle MHN <lb />ſiaigu que la puiſſance, ou le poids D, ou quel-<lb />qu’autre en ſa place, devra être plus grand que <lb />chacune des puiſſances P &amp; </s>
          <s xml:space="preserve">R pour être en équilibre <lb />avec elles; </s>
          <s xml:space="preserve">mais ce poids ne peut pas ainſi augmèn-<lb />ter à l’infini, de même que nous venons de dire qu’il <lb />peut diminuer; </s>
          <s xml:space="preserve">Car ne pouvant jamais être plus <lb />grand que lors que cet angle eſt infiniment aigu, <lb />c’eſt-à-dire, lors que les parties de corde MP &amp; </s>
          <s xml:space="preserve">NR <lb />ſont paralleles; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">le ſinus de cet angle n’étant encore <lb />alors que double du ſinus de ſa moitié, ce poids ne <lb />peut être tout au plus que double de chacune des puiſ-<lb />ſances P &amp; </s>
          <s xml:space="preserve">R.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0057" n="31" />
        <fw type="head">MECHANIQUE.</fw>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> IX.</head>
        <note xml:space="preserve" place="margin">DES <lb />POULIES.</note>
        <p>
          <s xml:space="preserve">D’ou l’on voit en général que lors qu’un poids fait <lb />ainfi équilibre avec deux puiſſances, ou avec deux au-<lb />tres poids par le moyen de quelque poulie à moufle, <lb />il ne peut être tout au plus que double de chacune de <lb />ces puiſſances, ou de ces autres poids; </s>
          <s xml:space="preserve">mais au con-<lb />traire il peut diminuer à l’infini, &amp; </s>
          <s xml:space="preserve">faire cependant <lb />toujours équilibre avec elles, ou avec ces poids, quoi <lb />qu’ils demeurent toujours les mêmes.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> X.</head>
        <p>
          <s xml:space="preserve">Ce qui fait voir que ſur une infinité de cas diffé-<lb />rens ou cet équilibre peut arriver, il n’y en a qu’un <lb />feul ou le poids, ou bien la puiſſance D, puiſſe être <lb />double de chacune des puiſſances P &amp; </s>
          <s xml:space="preserve">R; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">que dans <lb />tousles autres il eſt toujours moindre que double, &amp; </s>
          <s xml:space="preserve"><lb />même moindre à l’infini que chacune d’elles.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">Tous ceux qwi ſe mêlent de Mècbanique, ſcavent aſſez <lb />que l’on regarde ordinairement comme génèrale &amp; </s>
          <s xml:space="preserve">comme <lb />abſolument vraye cette propoſition: </s>
          <s xml:space="preserve">qu’un poids attaché, <lb />ou ſuſpendu au centre mobile d’une poulie à moufle, <lb />&amp; </s>
          <s xml:space="preserve">en équilibre avec une puiſſance appliquée à l’ex-<lb />trémitè d’une corde qui embraſſant cette poulie, à <lb />ſon autre extrémité retenuë par quelque clou, ou <lb />autrement, eſt double de cette puiſſance. </s>
          <s xml:space="preserve">Cependant <lb />on voit par ce dernier Corollaire que ſur une infinité de cas <lb />diffèrens, ou cet équilibre peut arriver, cette propoſition n’eſt <lb />vraye que dans un ſeul, qui eſt lors que les parties de corde <lb />gui touchent cette poulie ſont paralleles; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">fauſſe dans tous <lb />les autres. </s>
          <s xml:space="preserve">Il eſt vrai que dans la dèmonſtration que les Au-<lb />teurs qui l’ont avancèe, en donnent, ils ſuppoſent tous que ces <lb />parties de corde touchent cette poulie aux extrèmitez d’un <lb />même diametre, &amp; </s>
          <s xml:space="preserve">conſèquemment qu’elles ſont paralleles;</s>
          <s xml:space="preserve">
</s>
          <pb facs="0058" n="32" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
mais outre qu’il eſt rare qu’elles le ſoient, c’eſt que n’ayant <lb />
<ptr xml:id="note-0058-01a" corresp="note-0058-01" type="noteAnchor" />
point fait cette reſtriction dans leur propoſition, ils la regar-<lb />dent dans la ſuite comme générale, &amp; </s>
          <s xml:space="preserve">l’appliquent indiffé-<lb />remment à toutes les machines ou l’on ſe ſert de moufles, ſans <lb />avoir égard à la ſituation de leurs cordes; </s>
          <s xml:space="preserve">Ce qui les a jettez <lb />dans des mépriſes conſidérables, comme on le verra dans les <lb />Corollaires 15. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">17.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0058-01" corresp="note-0058-01a" place="margin">DES <lb />POULIES.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XI.</head>
        <p>
          <s xml:space="preserve">Soit que le centre de la poulie A demeure fixe, <lb />ſoit qu’on le ſuppoſe mobile, tant que ces puiſſances <lb />demeurent ainſi en équilibre aux extrémitez P &amp; </s>
          <s xml:space="preserve">R <lb />d’une même corde paſſée par deſſus, ou par deſſous <lb />cette poulie, elles ſont toujours égales: </s>
          <s xml:space="preserve">puiſque quel-<lb />que ſoit la charge de cette poulie, ſi elle eſt fixe, ou <lb />bien le poids qui y eſt attaché, ſi elle eſt mobile; </s>
          <s xml:space="preserve">cette <lb />charge, ou ce poids, tant que dure cet équilibre, eſt <lb />toujours à chacune d’elles, comme le ſinus de l’angle <lb />de leurs parties de corde, au ſinus de ſa moitié.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XII.</head>
        <p>
          <s xml:space="preserve">Si ces parties de corde des puiſſances P, &amp; </s>
          <s xml:space="preserve">R, <lb />lorſqu’elles ſoutiennent la puiſſance, ou le poids D, <lb />ne ſont point paralleles, ces deux mêmes puiſſances <lb />le pourront ſoutenir dans deux ſituations différentes <lb />de leurs cordes; </s>
          <s xml:space="preserve">parce que ces cordes peuvent faire <lb />des angles égaux en H de part &amp; </s>
          <s xml:space="preserve">d’autre de la poulie <lb />A, avec ſa ligne de direction AH, ſoit en s’écartant <lb />l’une de l’autre, (fig. </s>
          <s xml:space="preserve">20. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">22.) </s>
          <s xml:space="preserve">ſoit en s’approchant; <lb /></s>
          <s xml:space="preserve">(fig. </s>
          <s xml:space="preserve">21. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">23.) </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent les mêmes puiſſan-<lb />ces P, &amp; </s>
          <s xml:space="preserve">R, qui dans l’une de ces ſituations de cor-<lb />des, ſont capables de ſoutenir la puiſſance, ou le <lb />poids D, le pourront encore ſoutenir dans l’autre.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0059" n="33" />
        <fw type="head">MECHANIQUE.</fw>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XIII.</head>
        <note xml:space="preserve" place="margin">DES <lb />POULIES.</note>
        <p>
          <s xml:space="preserve">Mais ſi les parties de corde des puiſſances P &amp; </s>
          <s xml:space="preserve">R <lb />ſont paralleles, elles ne pourront ſoutenir la puiſſan-<lb />ce, ou le poids D qu’en cette ſeule ſituation; </s>
          <s xml:space="preserve">parce <lb />qu’il n’eſt pas poſſible d’en trouver d’autre, ou cette <lb />puiſſance, ou bien ce poids, ſoit double de chacune <lb />des puiſſances P &amp; </s>
          <s xml:space="preserve">R qui le ſoutiennent.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XIV.</head>
        <p>
          <s xml:space="preserve">On voit encore de cette propoſition que le poids <lb />
<ptr xml:id="note-0059-02a" corresp="note-0059-02" type="noteAnchor" />
D étant en équilibre avec la puiſſance R, par le <lb />moyen de pluſieurs moufles A, B, C, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">Séparez, <lb />&amp; </s>
          <s xml:space="preserve">appliquez le long du poteau EG, ou de quelqu’au-<lb />tre corps que ce ſoit, de la maniére qu’on les voit <lb />ici; </s>
          <s xml:space="preserve">eſt à cette puiſſance, comme le produit des ſinus <lb />des angles H, K, L, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">que font, lors qu’on les pro-<lb />longe, les parties des cordes EK, FL, GR, &amp;</s>
          <s xml:space="preserve">c. <lb /></s>
          <s xml:space="preserve">qui touchent ces poulies; </s>
          <s xml:space="preserve">au produit des ſinus de <lb />chacun leur moitié: </s>
          <s xml:space="preserve">Car ſelon la propoſition préſen-<lb />te, la réſiſtance de la poulie A, ou bien le poids D eſt <lb />à la réſiſtance de la poulie B, comme le ſinus de l’angle <lb />H, au ſinus de ſa moitié. </s>
          <s xml:space="preserve">La réſiſtance de la poulie <lb />B eſt auſſi à celle de la poulie C, comme le ſinus de <lb />l’angle K, au ſinus de ſa moitié. </s>
          <s xml:space="preserve">Enfin la réſiſtance <lb />de la poulie C eſt encore à celle de la puiſſance R, <lb />comme le ſinus de l’angle L, au ſinus de ſa moitié; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve"><lb />ainſi de même à l’infini: </s>
          <s xml:space="preserve">Donc en multipliant par <lb />ordre les termes de toutes ces proportions, c’eſt-à-<lb />dire, les antécédens par les antécédens, &amp; </s>
          <s xml:space="preserve">les conſé-<lb />quens par les conſéquens, on aura le poids D à la <lb />puiſſance R, comme le produit des ſinus des angles <lb />H, K, L, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">au produit des ſinus de chacun leur <lb />moitié.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0059-02" corresp="note-0059-02a" place="margin">fig. 24. <lb />205.</note>
            </div>
          </body>
        </floatingText>
        <pb facs="0060" n="34" />
        <fw type="head">NOUVELLE</fw>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XV.</head>
        <note xml:space="preserve" place="margin">DES <lb />POULIES.</note>
        <p>
          <s xml:space="preserve">Il ſuit de ce dernier Corollaire que ſur une in-<lb />finité de cas différens, ou le poids D peut être en <lb />équilibre avec la puiſſance R, à l’aide de pluſieurs <lb />moufles, de la maniére qu’ils ſont ici; </s>
          <s xml:space="preserve">il n’y en a qu’un <lb />ſeul, ou ce poids ſoit à cette puiſſance comme le der-<lb />nier terme d’une progreſſion double, qui en a autant <lb />qu’il y a de moufles, plus un, eſt au premier; </s>
          <s xml:space="preserve">c’eſt-à-<lb />dire, ici, comme 8. </s>
          <s xml:space="preserve">à 1. </s>
          <s xml:space="preserve">C’eſt lors que les parties de <lb />corde qui ſont tangentes de ces moufles, ſont paralle-<lb />les entr’elles: </s>
          <s xml:space="preserve">parce que les angles H, K, L, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">étant <lb />alors infiniment aigus, leurs ſinus ſont doubles des <lb />ſinus de leurs moitiez. </s>
          <s xml:space="preserve">Pour dans tous les autres, il <lb />eſt toujours à cette puiſſance en moindre raiſon que <lb />ce dernier terme au premier, &amp; </s>
          <s xml:space="preserve">même, en moindre à <lb />l’infini: </s>
          <s xml:space="preserve">parce que les angles H, K, L, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">ne pou-<lb />vant devenir plus aigus que lorſque ces parties de <lb />cordes ſont paralleles, les raiſons de leurs ſinus aux <lb />ſinus de leurs moitiez, ne peuvent auſſi jamais être <lb />chacune plus grande que celle de 2. </s>
          <s xml:space="preserve">à I. </s>
          <s xml:space="preserve">au contraire <lb />ces angles pouvant devenir toujours plus obtus juſqu’à <lb />l’infini, les raiſons de leurs ſinus aux ſinus de leurs <lb />moitiez, peuvent auſſi diminuer à l’infini.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">On voit aſſez la mépriſe de ceux qui dans cet uſage des <lb />poulies à moufle, ont avancé comme propoſition générale que le <lb />poids D eſt à la puiſſance R, comme le dernier terme <lb />d’une progreſſion double, qui en à autant qu’il y a <lb />de moufles, plus un, eſt au premier. </s>
          <s xml:space="preserve">Ce qui les a trom-<lb />pez c’eſt l’uſage trop étendu qu’ils ont donné à la propoſition <lb />raportée dans la réfléxion qui ſuit le Corollaire 10. </s>
          <s xml:space="preserve">de la <lb />propoſition préſente.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0060-01" />
          <label>0060-01</label>
        </figure>
        <pb facs="0061" n="35" />
        <fw type="head">MECHANIQUE.</fw>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XVI.</head>
        <note xml:space="preserve" place="margin">DES <lb />POULIES.</note>
        <p>
          <s xml:space="preserve">Préſentement ſi l’on ſe ſert de pluſieurs poulies <lb />liées enſemble, comme on les voit dans les figures 26. <lb /></s>
          <s xml:space="preserve">
<ptr xml:id="note-0061-02a" corresp="note-0061-02" type="noteAnchor" />
&amp; </s>
          <s xml:space="preserve">27. </s>
          <s xml:space="preserve">Il ſuit encore de cette propoſition que la puiſ-<lb />ſance R eſt au poids D qu’elle ſoutient à l’aide de ces <lb />poulies, comme le produit des ſinus des moitiez de <lb />chacun des angles que font, ſi on les prolonge, les <lb />cordes tangentes des poulies mobiles L, K, &amp; </s>
          <s xml:space="preserve">H, à la <lb />ſomme des produits de chacun des ſinus de ces mêmes <lb />angles par les ſinus des moitiez de chacun des autres. <lb /></s>
          <s xml:space="preserve">Par exemple, ſoit le ſinus de l’angle de ces cordes fait <lb />en A, appellé a; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">celui de ſa moitié appellé b. </s>
          <s xml:space="preserve">Celui de <lb />l’angle C, appellé c; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">celui de ſa moitié appellé d. </s>
          <s xml:space="preserve"><lb />Enfin celui de l’angle E, appellé e; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">celui de ſa moi-<lb />tié appellé f. </s>
          <s xml:space="preserve">Cela ſuppoſé il ſuit, dî-je, de cette pro-<lb />poſition que la puiſſance R en ce cas eſt au poids D, <lb />comme bàf à adf + cbf + ebd. </s>
          <s xml:space="preserve">Parceque la corde <lb />RRORNRM étant également bandée dans tou-<lb />tes ſes parties, &amp; </s>
          <s xml:space="preserve">d’une force égale à celle de la puiſ-<lb />ſance R; </s>
          <s xml:space="preserve">on la peut regarder, tant que dure cet équi-<lb />libre, comme diviſée en autant de cordes RRO, <lb />RN, &amp; </s>
          <s xml:space="preserve">RM, qu’il y a de poulies L, K, &amp; </s>
          <s xml:space="preserve">H, dans <lb />l’écharpe LH; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">chacune de ces cordes comme fixe <lb />en O, N, &amp; </s>
          <s xml:space="preserve">M, &amp; </s>
          <s xml:space="preserve">tirée du côté de R, R, &amp; </s>
          <s xml:space="preserve">R par la <lb />puiſſance R, ou par d’autres qui lui ſoient égales. </s>
          <s xml:space="preserve"><lb />Et parce que les poulies L, K, &amp; </s>
          <s xml:space="preserve">H, portent chacune <lb />quelque choſe du poids D, regardons-le auſſi comme <lb />diviſé en autant de parties x, y, &amp; </s>
          <s xml:space="preserve">z, dont la partie x <lb />ſoit portée par la poulie L; </s>
          <s xml:space="preserve">la partie y, par la poulie <lb />K; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">la partie z, par la poulie H.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0061-02" corresp="note-0061-02a" place="margin">fig. 26.</note>
            </div>
          </body>
        </floatingText>
        <pb facs="0062" n="36" />
        <fw type="head">NOUVELLE</fw>
        <p>
          <s xml:space="preserve">Cela conçcû il eſt clair par la propoſition qu’on vient <lb />
<ptr xml:id="note-0062-01a" corresp="note-0062-01" type="noteAnchor" />
de démontrer</s>
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0062-01" corresp="note-0062-01a" place="margin">DES <lb />POULIES.</note>
            </div>
          </body>
        </floatingText>
        <note xml:space="preserve" place="margin"> <lb />que{ # {x. R :: a. b. \\ R. y :: d. c.} # Donc {x. y :: ad. bc. \\ &amp; \\ x. x + y :: ad. ad + bc. # }Donc <lb /># {z. R :: e. f. \\ R. x :: b. a.} # Donc z. x :: eb. fa. <lb /></note>
        <p>
          <s xml:space="preserve">z. </s>
          <s xml:space="preserve">x + y :</s>
          <s xml:space="preserve">: adeb. </s>
          <s xml:space="preserve">aadf + abcf. </s>
          <s xml:space="preserve">Donc z. </s>
          <s xml:space="preserve">z + x + y :</s>
          <s xml:space="preserve">: <lb />adeb. </s>
          <s xml:space="preserve">adeb + aadf + abcf. </s>
          <s xml:space="preserve">Or R. </s>
          <s xml:space="preserve">z :</s>
          <s xml:space="preserve">: f. </s>
          <s xml:space="preserve">e. </s>
          <s xml:space="preserve">Donc R. <lb /></s>
          <s xml:space="preserve">z + x + y = D :</s>
          <s xml:space="preserve">: adefb. </s>
          <s xml:space="preserve">adeeb + aadef + aebcf. </s>
          <s xml:space="preserve">Et en <lb />diviſant les deux terniers termes de cette derniére <lb />proportion, par ae, l’on aura R. </s>
          <s xml:space="preserve">D :</s>
          <s xml:space="preserve">: dfb. </s>
          <s xml:space="preserve">edb + <lb />adf + bcf. </s>
          <s xml:space="preserve">Ce qu’il faloit démontrer.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XVII.</head>
        <p>
          <s xml:space="preserve">D’où il ſuit que dans cet uſage des poulies, lors <lb />que les parties de corde, qui touchent celles de l’é-<lb />charpe LH, ſont paralleles, la puiſſance R eſt au <lb />poids D, comme l’unité au double du nombre des <lb />poulies ſuſpenduës; </s>
          <s xml:space="preserve">mais que dans tout autre cas, <lb />elle lui eſt toujours en plus grande raiſon; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">même, <lb />cette raiſon augmente, quoi qu’en proportion diffé-<lb />rente, à meſure que les angles A, C &amp; </s>
          <s xml:space="preserve">E deviennent <lb />moins aigus, ou plus obtus.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">On voit aſſez que tous ces Corollaires avec une infinité <lb />d’autres qu’on pourroit encore tirer de cette propoſition, dé-<lb />pendent abſolument de ſon univerſalité, &amp; </s>
          <s xml:space="preserve">que ſans cela <lb />il ſeroit impoſſible de réſoudre une infinité de Problêmes <lb />qu’on peut faire ſur cette matiére. </s>
          <s xml:space="preserve">Par exemple celui-ci.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0062-01" />
          <label>0062-01</label>
        </figure>
        <pb facs="0063" n="37" />
        <fw type="head">MECHANIQUE.</fw>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0063-01" />
          <label>0063-01</label>
        </figure>
        <note xml:space="preserve" place="margin">DES <lb />POULIES.</note>
      </div>
      <div type="section">
        <head xml:space="preserve">PROBLEME.</head>
        <p rend="italics">
          <s xml:space="preserve">F Aire ſoutenir quelque poids D que ce ſoit, à quelque <lb />
<ptr xml:id="note-0063-02a" corresp="note-0063-02" type="noteAnchor" />
puiſſance R que ce puiſſe être, par le moyen d’une ſeule <lb />poulie à moufle.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0063-02" corresp="note-0063-02a" place="margin">fig. 28.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Solution</hi></head>
        <p>
          <s xml:space="preserve">Premiérement ſi cette puiſſance eſt plus grande <lb />que ce poids, faite ſur EH perpendiculaire à l’hori-<lb />zon, &amp; </s>
          <s xml:space="preserve">priſe à diſcretion, le triangle Iſocelle EFH, <lb />dont chacun des côtez EF, &amp; </s>
          <s xml:space="preserve">FH, ſoit en même rai-<lb />ſon à ſa baſe EH, que la puiſſance R, dont il eſt <lb />queſtion, eſt au poids D. </s>
          <s xml:space="preserve">Du point H tirez HG per-<lb />pendiculaire à HF, &amp; </s>
          <s xml:space="preserve">égale au rayon de la poulie <lb />A, dont on ſe veut ſervir; </s>
          <s xml:space="preserve">du point G faite encore <lb />GM parallele à HE, &amp; </s>
          <s xml:space="preserve">qui rencontre HF en M; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve"><lb />de ce même point M faite auſſi MA parallele à HG, <lb />&amp; </s>
          <s xml:space="preserve">qui rencontre auſſi EH en A; </s>
          <s xml:space="preserve">placez enſuite en <lb />ce point le centre de la poulie A, &amp; </s>
          <s xml:space="preserve">ſuſpendez le poids <lb />D à cette poulie ſuivant AH. </s>
          <s xml:space="preserve">Enfin aprés avoir di-<lb />rigé la partie MR dè ſa corde ſuivant HF, &amp; </s>
          <s xml:space="preserve">ſon <lb />autre partie PN parallelement à EF; </s>
          <s xml:space="preserve">arrêtez cette <lb />corde par un bout au clou P, &amp; </s>
          <s xml:space="preserve">appliquez à l’autre <lb />la puiſſance R: </s>
          <s xml:space="preserve">cela fait elle ſoutiendra ce poids en <lb />cet état.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration.</hi></head>
        <p>
          <s xml:space="preserve">Le poids D peut être ſoutenu en cet état (Cor. </s>
          <s xml:space="preserve">2.) <lb /></s>
          <s xml:space="preserve">par deux puiſſances, à chacune deſquelles il ſoit <lb />comme le ſinus de l’angle RHP, au ſinus de ſa moitié <lb />EHR, ou EHP; </s>
          <s xml:space="preserve">c’eſt-à-dire, (Lemm. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">comme <lb />EH à EF, ou bien (hyp.) </s>
          <s xml:space="preserve">comme il eſt à la puiſſance <lb />R: </s>
          <s xml:space="preserve">Donc le clou P faiſant la fonction d’une de ces
</s>
          <pb facs="0064" n="38" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
puiſſances, celle-ci ſoutiendra ce poids en cet état. </s>
          <s xml:space="preserve">Ce <lb />
<ptr xml:id="note-0064-01a" corresp="note-0064-01" type="noteAnchor" />
qu’il faloit faire.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0064-01" corresp="note-0064-01a" place="margin">DES <lb />POULIES.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">Secondement, ſi c’eſt le poids D qui ſoit plus <lb />grand que la puiſſance R, quelque grand qu’il ſoit, <lb />&amp; </s>
          <s xml:space="preserve">quelque petite elle, qu’elle puiſſe être, on le lui <lb />
<ptr xml:id="note-0064-02a" corresp="note-0064-02" type="noteAnchor" />
pourra encore faire ſoutenir: </s>
          <s xml:space="preserve">voici comment. </s>
          <s xml:space="preserve">Ayant <lb />décrit du centre F avec le rayon HF perpendicu-<lb />laire à l’horizon, &amp; </s>
          <s xml:space="preserve">pris à diſcretion, l’arc HEB; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve"><lb />y ayant inſcrit une ligne HE, qui ſoit à HF, comme <lb />la puiſſance R au poids D; </s>
          <s xml:space="preserve">joignez FE, &amp; </s>
          <s xml:space="preserve">faite en-<lb />ſuite HG perpendiculaire à HF, &amp; </s>
          <s xml:space="preserve">égale au rayon de <lb />la poulie A, dont on ſe veut ſervir; </s>
          <s xml:space="preserve">Du point G faite <lb />encore GM parallele à HE, &amp; </s>
          <s xml:space="preserve">qui rencontre HF en <lb />M, d’où il faut faire encore MA parallele à HG, &amp; </s>
          <s xml:space="preserve">qui <lb />rencontre HE en A, où vous placerez le centre de <lb />la poulie A, à laquelle vous appliquerez la puiſſance <lb />R ſuivant AH, &amp; </s>
          <s xml:space="preserve">le poids D ſuivant HF, l’autre <lb />bout de ſa corde étant attaché en P fuivant NP pa-<lb />rallele à EF. </s>
          <s xml:space="preserve">Cela fait la puiſſance R ſoutiendra en-<lb />core le poids D en cet état.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0064-02" corresp="note-0064-02a" place="margin">fig. 29.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration.</hi></head>
        <p>
          <s xml:space="preserve">Cette puiſſance peut faire équilibre en cet état avec <lb />deux autres, pourvu qu’elle ſoit à chacune d’elles, <lb />(Cor. </s>
          <s xml:space="preserve">2.) </s>
          <s xml:space="preserve">comme le ſinus de l’angle PHF, au ſinus <lb />de ſa moitié PHE, ou à EF; </s>
          <s xml:space="preserve">c’eſt-à-dire, (Lemm. </s>
          <s xml:space="preserve">5.) <lb /></s>
          <s xml:space="preserve">Comme HE à HF, ou EHF; </s>
          <s xml:space="preserve">ou bien (hyp.) </s>
          <s xml:space="preserve">comme <lb />elle eſt au poids D: </s>
          <s xml:space="preserve">Donc le clou P faiſant la fonc-<lb />tion d’une de ces puiſſances, &amp; </s>
          <s xml:space="preserve">le poids D celle de <lb />l’autre, la puiſſance R doit le ſoutenir en cet état. </s>
          <s xml:space="preserve"><lb />Ce qu’il F. </s>
          <s xml:space="preserve">D.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire.</hi></head>
        <p>
          <s xml:space="preserve">On voit que l’on peut toujours faire ſoutenir quel-
</s>
          <pb facs="0065" n="39" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
que poids que ce ſoit, à quelque puiſſance que ce <lb />
<ptr xml:id="note-0065-01a" corresp="note-0065-01" type="noteAnchor" />
puiſſe être, par le moyen d’une ſeule poulie à mouf-<lb />fle: </s>
          <s xml:space="preserve">en appliquant le moindre des deux au centre <lb />mobile de cette poulie, &amp; </s>
          <s xml:space="preserve">le plus grand au bout libre <lb />de la corde qui l’embraſſe. </s>
          <s xml:space="preserve">La raiſon en eſt évidente <lb />par les Corollaires 7. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">8.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0065-01" corresp="note-0065-01a" place="margin">DES <lb />POULIES.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Remarque.</hi></head>
        <p>
          <s xml:space="preserve">Il n’eſt pas cependant toujours néceſſaire de les <lb />diſpoſer ainſi: </s>
          <s xml:space="preserve">car s’il arrive que le plus grand des <lb />deux ne ſoit point plus que double de l’autre, on ſera <lb />libre d’appliquer celuy qu’on voudra au centre mo-<lb />bile de la poulie A: </s>
          <s xml:space="preserve">puiſque, qu’il y ſoit, (Cor. </s>
          <s xml:space="preserve">8.) <lb /></s>
          <s xml:space="preserve">ou non, (Cor. </s>
          <s xml:space="preserve">7.) </s>
          <s xml:space="preserve">il peut toujours monter juſqu’à <lb />être double de l’autre, mais jamais davantage: </s>
          <s xml:space="preserve">(Cor. </s>
          <s xml:space="preserve">8.) </s>
          <s xml:space="preserve"><lb />ainſi lorſque l’un des deux (la puiſſance ou le poids) <lb />fera plus que double de l’autre, il faudra néceſſai-<lb />rement les appliquer ſuivant le Corollaire ci-deſſus; </s>
          <s xml:space="preserve"><lb />c’eſt-à-dire, appliquer le moindre au centre du mouf-<lb />fle dont on ſe ſert, &amp; </s>
          <s xml:space="preserve">le plus grand ou bout libre <lb />de la corde qui embraſſe cette poulie à moufle.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0065-01" />
          <label>0065-01</label>
        </figure>
        <pb facs="0066" n="40" />
        <fw type="head">NOUVELLE</fw>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0066-01" />
          <label>0066-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">PROPOSITION <lb />FONDAMENTALE <lb />DES POIDS SOUTENUS</head>
        <p>
          <s xml:space="preserve">Sur quelque eſpéce de ſurfaces que ceſoit; <lb /></s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">pour toutes les directions poſſibles <lb />des puiſſances qui y ſont appliquées.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">TELLE que ſoit la ſurface GH; </s>
          <s xml:space="preserve">le poids EO, &amp; </s>
          <s xml:space="preserve"><lb />
<ptr xml:id="note-0066-01a" corresp="note-0066-01" type="noteAnchor" />
la puiſſance R qui le ſoutient deſſus, ſont toujours en-<lb />tr’ eux en raiſon réciproque des ſinus des angles que font leurs <lb />lignes de direction avec AD tirée perpendiculairement du point <lb />A de leur concours, ſur la ſurface GH.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0066-01" corresp="note-0066-01a" place="margin">fig. 30. <lb />31. <lb />32. <lb />33. <lb />34. <lb />35. <lb />36.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration.</hi></head>
        <p>
          <s xml:space="preserve">A fin que ce poids &amp; </s>
          <s xml:space="preserve">cette puiſſance demeurent ainſi <lb />en equilibre ſur la ſurface GH, telle qu’elle ſoit, <lb />il faut 1°. </s>
          <s xml:space="preserve">que leurs lignes de direction EB &amp; </s>
          <s xml:space="preserve">FC, <lb />ſe rencontrent en quelque point A: </s>
          <s xml:space="preserve">car ſi elles étoient <lb />paralleles, il eſt clair que le centre de gravité de ce <lb />poids pourroit encore deſcendre d’une longueur éga-<lb />le à la diſtance qu’elles auroient entr’elles; </s>
          <s xml:space="preserve">ce qui <lb />eſt contre l’hypothêſe. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Les impreſſions particu-<lb />liéres que font ſur le point A, &amp; </s>
          <s xml:space="preserve">la peſanteur de ce <lb />poids, &amp; </s>
          <s xml:space="preserve">la puiſſance R qui le retient; </s>
          <s xml:space="preserve">étant les mê-<lb />mes que ſi ce point étoit pouſſé en même temps par
</s>
          <pb facs="0067" n="41" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
deux forces qui leur fuſſent égales, ſuivant leurs lignes <lb />
<ptr xml:id="note-0067-01a" corresp="note-0067-01" type="noteAnchor" />
de direction AC &amp; </s>
          <s xml:space="preserve">AB:</s>
          <s xml:space="preserve">le poids EO ainſi ſoutenu ſur <lb />la ſurface GH par le concours d’action de ſa peſan-<lb />teur &amp; </s>
          <s xml:space="preserve">de la puiſſance R, doittendre (Lem. </s>
          <s xml:space="preserve">4. </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">2.) <lb /></s>
          <s xml:space="preserve">ſuivant quelque ligne AD qui ſoit la diagonale d’un <lb />parallelogramme fait ſous des parties AC &amp; </s>
          <s xml:space="preserve">AB de <lb />leurs lignes de direction, qui ſoient entr’elles, com-<lb />me ce poids eſt à cette puiſſance. </s>
          <s xml:space="preserve">3°. </s>
          <s xml:space="preserve">Cette ligne AD <lb />doit toujours être perpendiculaire à la ſurface GH, <lb />telle qu’elle ſoit; </s>
          <s xml:space="preserve">par exemple, au point O: </s>
          <s xml:space="preserve">autrement <lb />AD devenant alors la ligne dedirection de ce corps, il <lb />rouleroit ou couleroit (Cor. </s>
          <s xml:space="preserve">Lemm. </s>
          <s xml:space="preserve">1.) </s>
          <s xml:space="preserve">vers H, ou vers <lb />G, ſelon que cette ligne ſe trouveroit au-deſſus ou <lb />au-deſſous du point O. </s>
          <s xml:space="preserve">4°. </s>
          <s xml:space="preserve">Cette même ligne doit <lb />encore paſſer par quelqu’un des points où ce poids <lb />touche cette ſurface, c’eſt-à-dire, par quelqu’un des <lb />points de ſa baze: </s>
          <s xml:space="preserve">autrement, &amp; </s>
          <s xml:space="preserve">pour la même rai-<lb />ſon, il rouleroit, ou couleroit encore du côté qu’elle <lb />s’en écarteroit. </s>
          <s xml:space="preserve">5°. </s>
          <s xml:space="preserve">La force dont ce poids eſt ainſi <lb />pouſſé ou tiré ſuivant AD par le concours d’action <lb />de ſa peſanteur &amp; </s>
          <s xml:space="preserve">de la puiſſance R, eſt à celle de <lb />cette puiſſance, (Lemm. </s>
          <s xml:space="preserve">4. </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">3.) </s>
          <s xml:space="preserve">comme AD à AB; </s>
          <s xml:space="preserve"><lb />c’eſt-à-dire, (Lem. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">commele ſinus de l’angle DBA, <lb />ou de ſon complement BAC, au ſinus de l’an-<lb />gle BDA, ou de DAC qui luy eſt égal. </s>
          <s xml:space="preserve">Elle <lb />eſt auſſi pour la même raiſon à la peſanteur de ce <lb />poids, comme le ſinus du même angle BAC, au ſinus <lb />de BAD: </s>
          <s xml:space="preserve">Ainſi la peſanteur de ce poids eſt à la <lb />force de cette puiſſance, comme le ſinus de l’angle <lb />BAD au ſinus de l’angle DAC; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent <lb />ce poids, &amp; </s>
          <s xml:space="preserve">cette puiſſance ſont entr’eux en raiſon <lb />réciproque des ſinus des angles que font leurs li-<lb />gnes de diréction avec la ligne tirée de leur point de <lb />concours perpendiculairement à la ſurfacc GH, <lb />telle quelle ſoit. </s>
          <s xml:space="preserve">Ce qu’il F.</s>
          <s xml:space="preserve">D.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0067-01" corresp="note-0067-01a" place="margin">DES POIDS <lb />ſoutenus ſur <lb />des ſurfaces.</note>
            </div>
          </body>
        </floatingText>
        <pb facs="0068" n="42" />
        <fw type="head">NOUVELLE</fw>
        <note xml:space="preserve" place="margin">DES POIDS <lb />ſoutenus ſur <lb />des ſurfaces.</note>
        <p rend="italics">
          <s xml:space="preserve">Les cas ou le point de concours de ces lignes de direction <lb />ſe trouve encore dans ce poids, mais au-deſſous de ſon centre <lb />de gravité, ſe réſoudront comme ceux des figures 33. </s>
          <s xml:space="preserve">34. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve"><lb />36. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">ceux où il ſe trouvera debors, ſe réſoudront auſſi de <lb />même, en regardant ſeulement ce point comme apparte-<lb />nant à ce poids, de la maniére que nous avons fait en traitant <lb />des poids ſoutenus avec des cordes ſeulement, figure 16. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">17. <lb /></s>
          <s xml:space="preserve">Tout cela eſt aiſé; </s>
          <s xml:space="preserve">c’eſt pourquoy on n’exprime point ici les <lb />figures de tous ces cas.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">On n’exprime point non plus la figure d’aucune ſurface <lb />borizontale: </s>
          <s xml:space="preserve">parce que la ligne de direction de quelque poids <lb />que ce ſoit, lui étant toujours perpendiculaire, il s’y ſoutient <lb />de lui-même, &amp; </s>
          <s xml:space="preserve">ſans le ſecours d’aucune puiſſance, par la <lb />même raiſon qu’il en a beſoin, comme l’on vient de voir, pour <lb />demeurer ſur quelque autre ſurface que ce ſoit. </s>
          <s xml:space="preserve">Cette propo-<lb />ſition ne laiſſe pas cependant de s’étendre encore juſques-là, <lb />comme on le verra dans les Corollaires 9. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">10. </s>
          <s xml:space="preserve">ainſi on <lb />n’en peut pas concevoir une plus générale.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> I.</head>
        <p>
          <s xml:space="preserve">On voit des articles 3. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">4. </s>
          <s xml:space="preserve">de cette démonſtra-<lb />tion que le poids EO ne peut-être ſoutenu par quel-<lb />que puiſſance R que ce ſoit, ſur quelque ſurface <lb />quece puiſſe être, à moins que la ligne AD ne tombe <lb />perpendiculairement ſur cette ſurface, &amp; </s>
          <s xml:space="preserve">qu’elle ne <lb />paſſe en même temps par quelqu’un des points ou <lb />ce poids touche cette même ſurface; </s>
          <s xml:space="preserve">c’eſt-à-dire, <lb />par quelqu’un des points de la baze de ce même <lb />poids.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> II.</head>
        <p>
          <s xml:space="preserve">Mais auſſi pour la même raiſon dés que l’un &amp;</s>
          <s xml:space="preserve">
</s>
          <pb facs="0069" n="43" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
l’autre arrivera, la puiſſance qui y ſera alors appli-<lb />
<ptr xml:id="note-0069-01a" corresp="note-0069-01" type="noteAnchor" />
quée ne manquera pas de l’y ſoutenir.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0069-01" corresp="note-0069-01a" place="margin">DES POIDS <lb />ſoutenus ſur <lb />des ſutfaces.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> III.</head>
        <p>
          <s xml:space="preserve">De-là on voit qu’il n’y a point non plus de puiſſan-<lb />ce capable de ſoutenir un poids rond, ou quelque <lb />ſphére que ce ſoit, ſur quelque ſurface que ce puiſſe <lb />être, à moins que le concours de leurs lignes de di-<lb />rection ne ſe faſſe dans ſon centre de grandeur; </s>
          <s xml:space="preserve">parce <lb />que c’eſt le ſeul point de ce corps, d’où l’on puiſſe <lb />tirer une ligne qui paſſe par ſa baze, &amp; </s>
          <s xml:space="preserve">qui ſoit en <lb />même temps perpendiculaire à la ſurface ſur laquelle <lb />il eſt ſoutenu. </s>
          <s xml:space="preserve">Dans tout autre configuration de poids, <lb />il en va tout autrement: </s>
          <s xml:space="preserve">parce que l’on y peut trou-<lb />ver pluſieurs points, d’où il eſt poſſible de tirer de <lb />telles perpendiculaires.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> IV.</head>
        <p>
          <s xml:space="preserve">Il n’y a point encore de puiſſance R, telle quelle <lb />ſoit, qui puiſſe ſoutenir aucun poids ſur quelque ſur-<lb />face que ce puiſſe être, à moins que ſa ligne de di-<lb />rection AR ne ſe trouve dans le complement NAO <lb />de l’angle CAO, que fait la ligne de direction AC <lb />de ce poids avec AO tirée du point A perpendiculai-<lb />rement à cette ſurface GH. </s>
          <s xml:space="preserve">Car 1°. </s>
          <s xml:space="preserve">ſi elle concou-<lb />roit avec AN elle ne feroit plus aueun angle avec <lb />AC: </s>
          <s xml:space="preserve">ainſi cette puiſſance porteroit ſeule tout ce poids, <lb />&amp; </s>
          <s xml:space="preserve">non avec ce plan; </s>
          <s xml:space="preserve">ce qui eſt contre l’hypothêſe. <lb /></s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Si cette ligne de direction concouroit avec AO, <lb />ou ſi elle ſortoit de l’angle NAO, la diagonale AD <lb />du parallelogramme BC ſe tourneroit vers G; </s>
          <s xml:space="preserve">ce <lb />qui feroit néceſſairement (Corol. </s>
          <s xml:space="preserve">Lemm. </s>
          <s xml:space="preserve">I.) </s>
          <s xml:space="preserve">tomber ce <lb />poids de ce côté-là, ce qui eſt encore contre l’hypo-<lb />thêſe. </s>
          <s xml:space="preserve">Donc la ligne de direction AB de la puiſſance <lb />R, doit toujours ſe trouver dans le complement NAO
</s>
          <pb facs="0070" n="44" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
<ptr xml:id="note-0070-01a" corresp="note-0070-01" type="noteAnchor" />
de l’angle CAO: </s>
          <s xml:space="preserve">de ſorte que c’eſt-là tout l’eſpace <lb />du mouvement qu’elle peut avoir.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0070-01" corresp="note-0070-01a" place="margin">DES POIDS <lb />ſoutenus ſur <lb />des ſurfaces.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> V.</head>
        <p>
          <s xml:space="preserve">Le plan BAC, ou le parallelogramme BC de <lb />cette ligne avec AC ligne de direction du poids <lb />EO, eſt auſſi toujours perpendiculaire à la ſur-<lb />face que la ligne GH repreſente, &amp; </s>
          <s xml:space="preserve">ſur laquelle ce <lb />poids eſt ſoutenu; </s>
          <s xml:space="preserve">puiſque la diagonale AD de ce pa-<lb />rallelogramme BC, l’eſt toujours à cette même ſur-<lb />face.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> VI.</head>
        <p>
          <s xml:space="preserve">On voit auſſi de l’article cinquiéme de la demonſ-<lb />tration ci-deſſus, que le poids EO eſt à la charge de <lb />cette ſurface, c’eſt-à-dire, à l’impreſſion que lui &amp; </s>
          <s xml:space="preserve">la <lb />puiſſance R font enſemble deſſus, ou à la réſiſtance <lb />qu’elle leur fait, comme le ſinus de l’angle BAD, au <lb />ſinus de l’angle BAC.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> VII.</head>
        <p>
          <s xml:space="preserve">D’où il ſuit que le poids EO, la charge de la ſur-<lb />face GH, &amp; </s>
          <s xml:space="preserve">la puiſſance R, ſont entr’eux comme <lb />les ſinus des angles BAD, BAC, ou ABD ſon com-<lb />plement, &amp; </s>
          <s xml:space="preserve">DAC, ou ADB qui lui eſt égal; </s>
          <s xml:space="preserve">c’eſt-à-<lb />dire, (Lemm. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">comme les lignes BD, AD, &amp; </s>
          <s xml:space="preserve"><lb />AB.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> VIII.</head>
        <p>
          <s xml:space="preserve">D’où il ſuit encore que plus l’angle BAC eſt obtus, <lb />moins la charge de cette ſurface eſt grande: </s>
          <s xml:space="preserve">de ſorte <lb />qu’il le peut devenir juſqu’à un tel point, quelle ſera <lb />ſi petite qu’on voudra; </s>
          <s xml:space="preserve">c’eſt ainſi qu’elle peut dimi-<lb />nuer à l’infini.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0071" n="45" />
        <fw type="head">MECHANIQUE.</fw>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> IX.</head>
        <note xml:space="preserve" place="margin">DES POIDS <lb />ſoutenus ſur <lb />des ſurfaces.</note>
        <p>
          <s xml:space="preserve">Mais elle ne peut pas augmenter de même; </s>
          <s xml:space="preserve">parce <lb />que ne pouvant jamais être plus grande, que lorſque <lb />cet angle eſt infiniment aigu; </s>
          <s xml:space="preserve">c’eſt-à-dire, lorſque <lb />les lignes AC &amp; </s>
          <s xml:space="preserve">AB concourent avec AO: </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">AD <lb />n’étant encore alors qu’égale à la ſomme de AB &amp; </s>
          <s xml:space="preserve">de <lb />BD; </s>
          <s xml:space="preserve">la charge de cette ſurface, qui eſt alors hori-<lb />zontale ne peut jamais être plus grande que la ſomme <lb />de ce poids, &amp; </s>
          <s xml:space="preserve">de cette puiſſance.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">On entend ici par ſurface horizontale unplan qui le ſoit, <lb />ou bien un point d’une ſurface courbe dont toutes les tangentes <lb />ſoient auſſi borizontales.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> X.</head>
        <p>
          <s xml:space="preserve">On voit encore qu’il faut d’autant moins de force <lb />
<ptr xml:id="note-0071-02a" corresp="note-0071-02" type="noteAnchor" />
pour ſoutenir ainſi un poids ſuivant la même direc-<lb />tion AB ſur un même point de quelque ſurface <lb />que ce ſoit, que cette ſurface, ſi elle eſt droite <lb />(fig. </s>
          <s xml:space="preserve">30. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">33.) </s>
          <s xml:space="preserve">ou bien ſi elle eſt courbe; </s>
          <s xml:space="preserve">(fig. </s>
          <s xml:space="preserve">32. <lb /></s>
          <s xml:space="preserve">36.)</s>
          <s xml:space="preserve">, que ſa tangente au point ou la perpendiculai-<lb />re AO la rencontre, eſt plus inclinée, quoi qu’en <lb />proportion différente: </s>
          <s xml:space="preserve">parce que la raiſon du ſinus <lb />de l’angle CAD, au ſinus de l’angle BAD, en eſt <lb />toujours moindre; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">comme cette inclinaiſon avec <lb />l’horizon peut diminuer à l’infini, la force qu’il faut <lb />pour ſoutenir quelque poids ſuivant la même direc-<lb />tion ſur quelqu’une de ces ſurfaces, ſoit droite, ſoit <lb />courbe, peut auſſi diminuer à l’infini: </s>
          <s xml:space="preserve">De ſorte que <lb />lorſqu’elle ſera infiniment inclinée; </s>
          <s xml:space="preserve">c’eſt-à-dire, ho-<lb />rizontale, du moins dans le point où la perpendicu-<lb />laire AO la rencontre, cette force ſera nulle, &amp; </s>
          <s xml:space="preserve">ré-<lb />duite à zéro; </s>
          <s xml:space="preserve">c’eſt-à-dire, qu’il n’en faudra plus du <lb />tout pour l’y ſoutenir.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0071-02" corresp="note-0071-02a" place="margin">fig 30. <lb />32. <lb />33. <lb />36.</note>
            </div>
          </body>
        </floatingText>
        <pb facs="0072" n="46" />
        <fw type="head">NOUVELLE</fw>
        <note xml:space="preserve" place="margin">DES POIDS <lb />ſoutenus ſur <lb />des ſurfaces.</note>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XI.</head>
        <p>
          <s xml:space="preserve">Au contraire pour ſoutenir ce poids ſur le même <lb />point d’une ſurface toujours également inclinée, telle <lb />quelle ſoit, mais ſuivant différentes directions de <lb />puiſſance; </s>
          <s xml:space="preserve">il faut d’autant plus de forces que l’angle <lb />DAB fait dans l’eſpace NAD par la perpendiculaire <lb />AO avec la ligne de direction AB de la puiſſance qui <lb />ſoutient ce poids, differe davantage de l’angle droit: <lb /></s>
          <s xml:space="preserve">parce qu’alors la raiſon du ſinus de l’angle CAD, au ſi-<lb />nus de l’angle BAD, en ſera d’autant plus grande, quoi <lb />qu’en proportion différente: </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">conime cet angle peut-<lb />être plus ou moins grand qu’un angle droit, &amp; </s>
          <s xml:space="preserve">en diffé-<lb />rer de plus en plus juſqu’au concours de AB avec AN, <lb />ou avec AO, ſans que AB ſorte de l’eſpace NAO; </s>
          <s xml:space="preserve">la <lb />puiſſance qui ſoutient ce poids peut auſſi augmenter <lb />juſques-là: </s>
          <s xml:space="preserve">mais différemment ſelon que AB s’appro-<lb />che de l’une, ou de l’autre de ces deux lignes. </s>
          <s xml:space="preserve">Car <lb />1°. </s>
          <s xml:space="preserve">ne pouvant jamais être plus grande par l’appro-<lb />che de AB vers AN, que lorſque l’angle NAB, que <lb />ces lignes font entr’elles, eſt le plus petit qu’elles <lb />puiſſent faire; </s>
          <s xml:space="preserve">c’eſt-à-dire, celui qu’elles font immé-<lb />diatement avant que de concourir; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">le ſinus de CAD <lb />étant encore alors un peu moindre que celui de <lb />BAO, quoique d’une difference infiniment petite: </s>
          <s xml:space="preserve"><lb />Cette puiſſance ne peut être tout au plus de ce côté-là, <lb />qu’un peu moindre que ce poids d’une différence qui <lb />ſoit auſſi infiniment petite. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Au contraire du côté de <lb />AO elle pent augmenter à l’infini: </s>
          <s xml:space="preserve">parce que la raiſon <lb />du ſinus de CAD, à celuy de BAD, augmentant à <lb />meſure quela ligne AB s’approche de AO, en s’éloi-<lb />gnant de la ſituation qu’elle auroit ſi elle faiſoit un an-<lb />gle droit avec AO; </s>
          <s xml:space="preserve">cette force peut auſſi augmenter <lb />de ce côté-là juſqu’à ce que AB, &amp; </s>
          <s xml:space="preserve">AO concourent. </s>
          <s xml:space="preserve"><lb />Or en ce cas l’angle BAD étant infiniment petit, la
</s>
          <pb facs="0073" n="47" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
raiſon du ſinus de CAD à celui de cet angle, ſera auſſi <lb />
<ptr xml:id="note-0073-01a" corresp="note-0073-01" type="noteAnchor" />
infinie; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent auſſi celle de cette puiſ-<lb />ſance à ce poids. </s>
          <s xml:space="preserve">Ce qui fait voir que cette puiſ-<lb />ſance peut augmenter à l’infini dans le mouvement <lb />qu’elle peut avoir depuis la ſituation où ſa ligne de <lb />direction feroit un angle droit avec la perpendiculaire <lb />AO, juſqu’au concours de ces deux mêmes lignes, &amp; </s>
          <s xml:space="preserve"><lb />demeurer cependant toûjours en équilibre avec le <lb />même poids, &amp; </s>
          <s xml:space="preserve">ſur le même point d’une ſurface in-<lb />clinée, telle quelle ſoit.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0073-01" corresp="note-0073-01a" place="margin">DES POIDS <lb />ſoutenus ſur <lb />des ſurfaces.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XII.</head>
        <p>
          <s xml:space="preserve">Pour les plans perpendiculaires à l’horizon, ou plu-<lb />
<ptr xml:id="note-0073-02a" corresp="note-0073-02" type="noteAnchor" />
tôt paralleles à la ligne de direction de ce poids; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve"><lb />pour les points des ſurfaces courbes, d’où l’on peut <lb />tirer des tangentes qui ſoient auſſi perpendiculai-<lb />res à l’horizon: </s>
          <s xml:space="preserve">la ligne de direction AB de la puiſ-<lb />ſance qui ſoutient ce poids ſur, ou contre ces plans, <lb />ou ces points de ſurfaces courbes, ne pouvant (Co-<lb />rol. </s>
          <s xml:space="preserve">4.) </s>
          <s xml:space="preserve">s’éloigner de la ſituation où elle ſeroit, ſi <lb />elle faiſoit un angle droit avec AO, qu’en s’appro-<lb />chant de AO, puiſque l’angle NAO en ce cas eſt <lb />droit; </s>
          <s xml:space="preserve">cette puiſſance ne peut auſſi augmenter que <lb />de ce côté-là: </s>
          <s xml:space="preserve">De ſorte qu’elle peut à la vérité aug-<lb />menter à l’infini de même que ſur les ſurfaces incli-<lb />nées: </s>
          <s xml:space="preserve">mais elle ne peut jamais être moins grande <lb />que lorſque ſa ligne de direction AB fait le plus petit <lb />angle qu’elle puiſſe faire avec AN; </s>
          <s xml:space="preserve">c’eſt-à-dire, <lb />qu’en ne ſurpaſſant ce poids que d’une différence in-<lb />finiment petite.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0073-02" corresp="note-0073-02a" place="margin">fig. 31. <lb />34. <lb />35.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XIII.</head>
        <note xml:space="preserve" place="margin">fig. 30. <lb />31. <lb />32. <lb />33. <lb />34. <lb />35. <lb />36.</note>
        <p>
          <s xml:space="preserve">De ſorte que dés le moment que AB &amp; </s>
          <s xml:space="preserve">AN vien-<lb />nent à concourir enſemble, le ſinus de CAD deve-<lb />nant alors égal à celui de BAD, cette puiſſance de-
</s>
          <pb facs="0074" n="48" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
<ptr xml:id="note-0074-01a" corresp="note-0074-01" type="noteAnchor" />
vient auſſi égale à ce poids, qui ceſſe auſſi-tôt de s’ap-<lb />puyer ſur, ou contre la ſurface GH, telle qu’elle <lb />ſoit.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0074-01" corresp="note-0074-01a" place="margin">DES POIDS <lb />ſoutenus ſur <lb />des ſurfaces.</note>
            </div>
          </body>
        </floatingText>
        <p rend="italics">
          <s xml:space="preserve">Ce n’eſt que pour ne pas embaraſſer l’imagination de ceux <lb />qui ſont accoutumez à regarder une ſurface perpendiculaire à <lb />l’horizon, comme parallele à la ligne de direction d’un poids, &amp; </s>
          <s xml:space="preserve"><lb />une horizontale, comme lui étant perpendiculaire; </s>
          <s xml:space="preserve">que l’on s’eſt <lb />accommodé à cette bypotbêſe dans ces trois derniers Corollaires: <lb /></s>
          <s xml:space="preserve">car pour les rendre auſſi généraux qu’on les puiſſe imaginer, &amp; </s>
          <s xml:space="preserve"><lb />pour toutes ſortes d’bypotbêſes, il ne faut que regarder les plans, <lb />ou les tangentes des ſurfaces courbes, que l’on dit ici perpen-<lb />diculaires à l’borizon, comme paralleles ſeulement à la ligne <lb />de direction de ce poids, ſans avoir égard à l’angle qu’elles <lb />font, ou qu’elles peuvent faire avec l’borizon. </s>
          <s xml:space="preserve">De même celles <lb />que l’on appelle ici borizontales, ſe doivent ſeulement regar-<lb />der comme perpendiculaires à cette ligne. </s>
          <s xml:space="preserve">De cette maniére ces <lb />Corollaires ſeront ſi généraux, qu’ils ſe pourront appliquer à <lb />toutes les directions poſſibles d’un corps ſoutenu ſur ou contre <lb />quelque ſurface que ce puiſſe être.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">Il eſt encore bon de remarquer que lorſqu’on dit ici qu’un <lb />poids eſt ſoutenu ſur le même point d’une ſurface, l’on ne pré-<lb />tend pas dire qu’il ne la rencontre jamais qu’en un ſeul point; <lb /></s>
          <s xml:space="preserve">mais on entend ſeulement que la ligne AD, qui tombe du <lb />point A perpendiculairement deſſus, la rencontre toujours dans <lb />le même point O, tant que ce poids eſt ſoutenu deſſus, quoi que <lb />ce ſoit ſuivant différentes directions de puiſſances. </s>
          <s xml:space="preserve">La raiſon <lb />de cette précaution eſt évidente du côté des ſurfaces courbes, <lb />dont tous les points ont cbacun une tangente d’une direction <lb />particuliére. </s>
          <s xml:space="preserve">Pour du côté des plans, on la reconnoîtra dans <lb />le Corollaire 23. </s>
          <s xml:space="preserve">où l’on verra que dans l’bypotbêſe du con-<lb />cours des lignes de direction des poids en quelque points de la <lb />terre que ce ſoit, ils ne péſent pas toujours également deſſus, <lb />quoique la ligne de direction de la puiſſance qui leur eſt appli-
</s>
          <pb facs="0075" n="49" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE</fw>
quée demeure toujours la même. </s>
          <s xml:space="preserve">Au contraire, ils péſent tou-<lb />
<ptr xml:id="note-0075-01a" corresp="note-0075-01" type="noteAnchor" />
jours également ſur le même point de quelque ſurface que ce <lb />ſoit, à moins qu’on ne change la ligne de direction de cotte <lb />puiſſance, ou la ſi@uation de cette ſurface. </s>
          <s xml:space="preserve">C’eſt pour cela <lb />que dans les trois Corollaires précédens, où l’on examine ſépa-<lb />rément le changement que peut cauſer dans l’action d’un poids <lb />les différentes inclinaiſons de la même, ou des différentes ſurfaces <lb />ſur leſquelles il eſt ſoutenu, &amp; </s>
          <s xml:space="preserve">les différentes lignes de direction des <lb />puiſſances qui l’yſoutiennent;</s>
          <s xml:space="preserve">on l’aregardé comme appliqué non-<lb />ſeulement à la même ſurface, mais auſſi toujours au même point.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0075-01" corresp="note-0075-01a" place="margin">DES POIDS <lb />ſoutenus ſur <lb />des ſurfaces.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XIV.</head>
        <p>
          <s xml:space="preserve">Puiſque la puiſſance qui ſoutient quelque poids <lb />que ce ſoit ſur le même point de quelque ſurface <lb />que ce puiſſe être, eſt d’autant plus grande que <lb />ſa ligne de direction AB s’éloigne davantage de la <lb />ſituaton où elle feroit un angle droit avec AO, ſans <lb />cependant ſortir de l’eſpace NAO: </s>
          <s xml:space="preserve">Il s’enſuit qu’elle <lb />n’eſt jamais moindre que lorſqu’elle eſt parallele au <lb />plan, ou à quelqu’une des tangentes au point de la ſur-<lb />face courbe, ſur lequel ce poids eſt ſoutenu.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XV.</head>
        <p>
          <s xml:space="preserve">D’où l’on voit dans l’hypothêſe ordinaire, ou l’on <lb />
<ptr xml:id="note-0075-02a" corresp="note-0075-02" type="noteAnchor" />
regarde HK comme parallele à AC, que les triangles <lb />BAD, HKG étant alors ſemblables, cette puiſſance qui <lb />eſt à ce poids (Cor. </s>
          <s xml:space="preserve">7.) </s>
          <s xml:space="preserve">comme AB à BD, lui ſera auſſi <lb />comme HK à HG: </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">comme elle eſt alors la moin-<lb />dre qu’elle puiſſe jamais être ſelon le Corollaire précé-<lb />dent; </s>
          <s xml:space="preserve">il s’enſuit qu’elle ne peut jamais être en moindre <lb />raiſon au poids qu’elle ſoutient ſur un plan incliné, <lb />qu’eſt celle de la hauteur de ce plan à ſa longueur.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0075-02" corresp="note-0075-02a" place="margin">fig. 30.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XVI.</head>
        <p>
          <s xml:space="preserve">On voit encore que toute puiſſance qui peut ſoute-
</s>
          <pb facs="0076" n="50" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
<ptr xml:id="note-0076-01a" corresp="note-0076-01" type="noteAnchor" />
nir un poids ſur un plan incliné ſuivant une ligne <lb />de direction, qui faſſe avec une perpendiculaire faite <lb />ſur AD au point A, un angle moindre que celui de <lb />cette perpendiculaire avec AN; </s>
          <s xml:space="preserve">l’y peut ſoutenir <lb />
<ptr xml:id="note-0076-02a" corresp="note-0076-02" type="noteAnchor" />
encore, &amp; </s>
          <s xml:space="preserve">ſur le même point, ſuivant une autre ligne <lb />de direction, qui paſſant de l’autre coté de cette per-<lb />pendiculaire, faſſe avec elle un angle égal au pre-<lb />mier: </s>
          <s xml:space="preserve">car les deux angles que font alors ces deux li-<lb />gnes de direction avec AD, étant complemens à deux <lb />droits, l’un de l’autre, leurs ſinus ſeront égaux; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve"><lb />par conſéquent ils ſeront en même raiſon au ſinus de <lb />l’angle CAD; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent auſſi ce même poids <lb />ſeroit alors en même raiſon aux puiſſances, qui pla-<lb />cées ſuivant ces différentes directions, le ſoutien-<lb />droient l’une aprés l’autre; </s>
          <s xml:space="preserve">ainſi elles ſeroient égales <lb />entr’elles: </s>
          <s xml:space="preserve">Donc la même puiſſance qui ſoutient ce <lb />poids ſuivant une de ces directions, le peut encore <lb />ſoutenir ſuivant l’autre ſur le même plan incliné <lb />GH.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0076-01" corresp="note-0076-01a" place="margin">DES POIDS <lb />ſoutenus ſur <lb />des ſurfaces.</note>
              <note xml:space="preserve" xml:id="note-0076-02" corresp="note-0076-02a" place="margin">fig 30. <lb />33.</note>
            </div>
          </body>
        </floatingText>
        <p rend="italics">
          <s xml:space="preserve">On verra par le Corollaire 23. </s>
          <s xml:space="preserve">que pour rendre ce dernier <lb />Corollaire général pour toutes ſortes d’hypotbéſes, il faut que <lb />ce poids ſe trouve alors ſur le même point d’un plan toujours <lb />également incliné.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XVII.</head>
        <p>
          <s xml:space="preserve">1°. </s>
          <s xml:space="preserve">Si AB ne concourt point avec la perpendiculaire <lb />faite ſur AD au point A, la puiſſance R qui ſoutiet le <lb />poid EO ſuivant cette même ligne AB, eſt à ce même <lb />poids en plus grande raiſon que le ſinus de CAD au ſi-<lb />nus total; </s>
          <s xml:space="preserve">c’eſt-à-dire, dans l’hypoth êſe ordinaire, en <lb />plus grande raiſon que la hauteur dé ce plan (Cor. <lb /></s>
          <s xml:space="preserve">14. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">15.) </s>
          <s xml:space="preserve">à ſa longueur. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Si l’angle de cette per-<lb />pendiculaire avec la ligne de direction AB de cette <lb />puiſſance, eſt moindre que l’angle de cette même per-
</s>
          <pb facs="0077" n="51" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
pendiculaire avec AN, cette puiſſance eſt auſſi moin-<lb />
<ptr xml:id="note-0077-01a" corresp="note-0077-01" type="noteAnchor" />
dre que ce poids: </s>
          <s xml:space="preserve">puiſque de quelque côté que AB <lb />faſſe cet angle avec cette pendiculaire, la puiſſance qui <lb />ſoutiendra ce poids, (Cor. </s>
          <s xml:space="preserve">16.) </s>
          <s xml:space="preserve">ſera la même; </s>
          <s xml:space="preserve">il s’enſuit <lb />(Cor. </s>
          <s xml:space="preserve">II. </s>
          <s xml:space="preserve">n. </s>
          <s xml:space="preserve">I.) </s>
          <s xml:space="preserve">qu’elle ſera moindre que ce poids dans <lb />l’un &amp; </s>
          <s xml:space="preserve">l’autrecas: </s>
          <s xml:space="preserve">ainſi l’on peut conclure en général <lb />qu’une même puiſſance peut ſoutenir un même poids <lb />ſur un même plan incliné ſuivant deux différentes di-<lb />rections: </s>
          <s xml:space="preserve">pourvu qu’elle ſoit moindre que ce poids, &amp; </s>
          <s xml:space="preserve"><lb />qu’elle lui ſoit cependant en plus grande raiſon que le <lb />ſinus de l’angle CAD au ſinus total; </s>
          <s xml:space="preserve">c’eſt-à-dire, dans <lb />l’hypothêſe ordinaire, où l’on regarde la ligne de di-<lb />rection de ce poids comme parallele à la hauteur de ce <lb />plan: </s>
          <s xml:space="preserve">pourvu que cette puiſſance moindre que ce <lb />poids, lui ſoit cependant en plus grande raiſon que la <lb />hauteur de ce plan à ſa longueur.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0077-01" corresp="note-0077-01a" place="margin">DES POIDS <lb />ſoutenus ſur <lb />des ſurfaces.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XVIII.</head>
        <p>
          <s xml:space="preserve">En tout autre cas; </s>
          <s xml:space="preserve">c’eſt-à-dire, lorſque cette puiſ-<lb />ſance eſt plus grande que ce poids, ou du moins qu’el-<lb />le lui eſt égale, ou bien lorſqu’elle lui eſt en même <lb />raiſon que le ſinus de l’angle CAD au ſinus total, <lb />elle ne le peut ſoutenir ſur le même point de ce plan <lb />que ſuivant une ſeule direction. </s>
          <s xml:space="preserve">Tout cela eſt mani-<lb />feſte par une raiſon toute contraire à celle du Corol-<lb />laire précédent.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">On voit aſſez comment ces quatre derniers Corollaires ſe <lb />peuvent appliquer à toutes ſortes de ſurfaces courbes, pour les <lb />points ou elles peuvent être touchées par des plans inclinez. <lb /></s>
          <s xml:space="preserve">Il n’eſt pas difficile non plus de reconnoitre ce qui leur peut <lb />convenir de ce que nous allons encore dire des ſurfaces planes; </s>
          <s xml:space="preserve"><lb />c’eſt pourquoi nous ne parlerons plus d’orénavant que de <lb />celles-ci.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0078" n="52" />
        <fw type="head">NOUVELLE</fw>
        <note xml:space="preserve" place="margin">DES POIDS <lb />ſoutenus ſur <lb />des ſurfaces.</note>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XIX.</head>
        <p>
          <s xml:space="preserve">Puiſque (Cor. </s>
          <s xml:space="preserve">7.) </s>
          <s xml:space="preserve">le poids EO, la puiſſance R, &amp; </s>
          <s xml:space="preserve"><lb />la charge du plan GH, ſont entr’eux comme les li-<lb />
<ptr xml:id="note-0078-02a" corresp="note-0078-02" type="noteAnchor" />
gnes BD, BA, &amp; </s>
          <s xml:space="preserve">AD; </s>
          <s xml:space="preserve">ſi la ligne de direction de la <lb />puiſſance R eſt parallele au plan GH, &amp; </s>
          <s xml:space="preserve">AC celle de <lb />ce poids parallele auſſi à HK hauteur de ce plan: </s>
          <s xml:space="preserve">ce <lb />poids, cette puiſſance, &amp; </s>
          <s xml:space="preserve">la charge de ce même plan, <lb />ſeront entr’eux comme la longueur de ce plan, ſa hau-<lb />teur, &amp; </s>
          <s xml:space="preserve">ſa baſe; </s>
          <s xml:space="preserve">c’eſt-à-dire, comme GH, HK, &amp; </s>
          <s xml:space="preserve"><lb />KG; </s>
          <s xml:space="preserve">parce qu’alors les triangles GHK, &amp; </s>
          <s xml:space="preserve">DBA ſont <lb />ſemblables.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0078-02" corresp="note-0078-02a" place="margin">fig. 30.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XX.</head>
        <p>
          <s xml:space="preserve">Et pour la même raiſon, ſi cette ligne de direction <lb />
<ptr xml:id="note-0078-03a" corresp="note-0078-03" type="noteAnchor" />
AB eſt parallele à l’horizon; </s>
          <s xml:space="preserve">c’eſt-à-dire, à la baze <lb />GK de ce plan; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">que AC ſoit encore parallele à ſa <lb />hauteur HK: </s>
          <s xml:space="preserve">Ce poids, cette puiſſance, &amp; </s>
          <s xml:space="preserve">la charge <lb />de ce plan, ſeront alors entr’eux comme la baze de <lb />de ce plan, ſa hauteur, &amp; </s>
          <s xml:space="preserve">ſa longueur; </s>
          <s xml:space="preserve">c’eſt-à-dire, <lb />comme GK, KH, HG; </s>
          <s xml:space="preserve">parce qu’alors les triangles <lb />GKH, &amp; </s>
          <s xml:space="preserve">DBA ſont encore ſemblables.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0078-03" corresp="note-0078-03a" place="margin">fig. 33.</note>
            </div>
          </body>
        </floatingText>
        <p rend="italics">
          <s xml:space="preserve">Fuſqu’ici nous n’avons regardé le même poids que comme <lb />appliqué au même endroit d’un plan toujours également incli-<lb />né: </s>
          <s xml:space="preserve">Mais s’il ſe trouvoit ſucceſſivement en différens points, <lb />qu’arriveroit-il? </s>
          <s xml:space="preserve">Le voici.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XXI.</head>
        <p>
          <s xml:space="preserve">Il ſuit encore de cette propoſition que les puiſſances <lb />
<ptr xml:id="note-0078-04a" corresp="note-0078-04" type="noteAnchor" />
P &amp; </s>
          <s xml:space="preserve">R qui ſoutiennent ſucceſſivement le même poids <lb />A, ou des poids égaux ſur les points O, &amp; </s>
          <s xml:space="preserve">Q d’un <lb />même plan HG, ſont entr’elles en raiſon compoſée <lb />de celles des ſinus des angles QAD, &amp; </s>
          <s xml:space="preserve">QAP; </s>
          <s xml:space="preserve">OAR <lb />&amp; </s>
          <s xml:space="preserve">OAD: </s>
          <s xml:space="preserve">car puiſque la puiſſance P eſt au poids A
</s>
          <pb facs="0079" n="53" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE</fw>
appliqué en Q, comme le ſinus de l’angle QAD, au <lb />
<ptr xml:id="note-0079-01a" corresp="note-0079-01" type="noteAnchor" />
ſinus de l’angle QAP; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">quele même poids appliqué <lb />en O, eſt à la puiſſance R, comme le ſinus de l’angle <lb />OAR, à celui de l’angle OAD: </s>
          <s xml:space="preserve">Il ſuit en multipliant <lb />par ordre ces deux rangées de proportionnelles; </s>
          <s xml:space="preserve">que <lb />la puiſſance P eſt à la puiſſance R, comme le produit <lb />des finus des angles QAD, &amp; </s>
          <s xml:space="preserve">OAR, au produit de <lb />ceux des angles QAP, &amp; </s>
          <s xml:space="preserve">OAD; </s>
          <s xml:space="preserve">c’eſt-à-dire, en <lb />raiſon compoſée de celles des ſinus des angles QAD, <lb />&amp; </s>
          <s xml:space="preserve">QAP; </s>
          <s xml:space="preserve">OAR, &amp; </s>
          <s xml:space="preserve">OAD.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0078-04" corresp="note-0078-04a" place="margin">fig. 37. <lb />38.</note>
              <note xml:space="preserve" xml:id="note-0079-01" corresp="note-0079-01a" place="margin">DES POIDS <lb />ſoutenus ſur <lb />des ſurfaces.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XXII.</head>
        <p>
          <s xml:space="preserve">D’où l’on voit que tant que les lignes de direction <lb />AP, &amp; </s>
          <s xml:space="preserve">AR ſont la même, ou paralleles entr’elles, <lb />&amp; </s>
          <s xml:space="preserve">que celles du poids A appliqué en Q, &amp; </s>
          <s xml:space="preserve">en O, ſont <lb />auſſi paralleles; </s>
          <s xml:space="preserve">les angles QAP, &amp; </s>
          <s xml:space="preserve">OAR étant <lb />alors égaux entr’eux, de même que les angles QAD, <lb />&amp; </s>
          <s xml:space="preserve">OAD, les puiſſances P &amp; </s>
          <s xml:space="preserve">R ſont auſſi pour lors <lb />égales; </s>
          <s xml:space="preserve">ce qui fait voir que ce même poids A péſe <lb />alors également ſur quelque point O, ou Q de ce <lb />plan, qu’il ſoit appliqué.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XXIII.</head>
        <p>
          <s xml:space="preserve">Au contraire, s’il n’y a que les lignes de de direc-<lb />tion AP, &amp; </s>
          <s xml:space="preserve">AR, de ces puiſſances qui ſoient paral-<lb />leles entr’elles, &amp; </s>
          <s xml:space="preserve">que celles de ce même poids A ap-<lb />pliqué ſucceſſivement en O, &amp; </s>
          <s xml:space="preserve">en Q, concourent en <lb />quelque point D, que ce ſoit; </s>
          <s xml:space="preserve">par exemple, au cen-<lb />tre de la terre: </s>
          <s xml:space="preserve">les angles QAP, &amp; </s>
          <s xml:space="preserve">OAR étant en-<lb />core égaux, les puiſſances P &amp; </s>
          <s xml:space="preserve">R ſeront entr’elles <lb />comme les ſinus des angles QAD, &amp; </s>
          <s xml:space="preserve">OAD; </s>
          <s xml:space="preserve">ou bien, <lb />à cauſe des paralleles QA, AO, ces puiſſances ſeront <lb />entr’elles comme les ſinus des angles SAD, &amp; </s>
          <s xml:space="preserve">ASA, <lb />ou ASD ſon complement; </s>
          <s xml:space="preserve">c’eſt-à-dire, (Lem. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">com-<lb />me DS à AD. </s>
          <s xml:space="preserve">Ce qui fait voir qu’en ce cas plus le poids</s>
        </p>
        <pb facs="0080" n="54" />
        <fw type="head">NOUVELLE</fw>
        <note xml:space="preserve" place="margin">DES POIDS <lb />ſoutenus ſur <lb />des ſurfaces.</note>
        <p>
          <s xml:space="preserve">A eſt haut ſur le plan HG, plus auſſi la puiſſance qui l’y <lb />doit ſoutenir ſuivant une certaine direction, doit être <lb />grande.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">On voit préſentement qu’il peut y avoir bien de la diffé-<lb />rence entre un poids ſoutenu ſur un même plan, &amp; </s>
          <s xml:space="preserve">un poids <lb />ſoutenu ſur le même point du plan; </s>
          <s xml:space="preserve">c’eſt auſſi pour cela qu’on <lb />à pris ſoin ci-deſſus de ne les pas confondre, &amp; </s>
          <s xml:space="preserve">de faire re-<lb />marquer cette différence dans la ſeconde réfléxion qui ſuit le <lb />Corollaire 13.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XXIV.</head>
        <p>
          <s xml:space="preserve">Mais s’il n’y a que les lignes de direction du poids <lb />A placé tantôt en O, &amp; </s>
          <s xml:space="preserve">tantôt en Q, qui ſoient pa-<lb />ralleles entr’elles; </s>
          <s xml:space="preserve">les puiſſances P &amp; </s>
          <s xml:space="preserve">R ſeront alors <lb />entr’elles comme les ſinus des angles OAR, &amp; </s>
          <s xml:space="preserve">QAP; <lb /></s>
          <s xml:space="preserve">c’eſt-à-dire, en raiſon réciproque des ſinus des angles <lb />que font leurs lignes de direction avec AO, &amp; </s>
          <s xml:space="preserve">AQ, <lb />tirées des points A ou ces lignes de direction con-<lb />courent avec celles de ce poids, perpendiculairement <lb />au plan GH.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XXV.</head>
        <p>
          <s xml:space="preserve">Si préſentement on conçoit que les puiſſances P &amp; </s>
          <s xml:space="preserve">R <lb />ſoient égales, &amp; </s>
          <s xml:space="preserve">que les poids A &amp; </s>
          <s xml:space="preserve">A ſoient différens; <lb /></s>
          <s xml:space="preserve">on trouvera de méme que ces poids, qu’elles ſoutien-<lb />nent ſur les points Q &amp; </s>
          <s xml:space="preserve">O du plan GH, ſeront entr’-<lb />eux en raiſon compoſée de celles des ſinus des angles <lb />QAP, &amp; </s>
          <s xml:space="preserve">QAD; </s>
          <s xml:space="preserve">OAD, &amp; </s>
          <s xml:space="preserve">OAR; </s>
          <s xml:space="preserve">c’eſt-à-dire, com-<lb />me le produit des ſinus des angles QAP &amp; </s>
          <s xml:space="preserve">OAD, au <lb />produit de ceux des angles QAD &amp; </s>
          <s xml:space="preserve">OAR: </s>
          <s xml:space="preserve">De ſorte <lb />que 1°. </s>
          <s xml:space="preserve">Lorſque les lignes de direction de ces puiſ-<lb />ſances ſont paralleles entr’elles, &amp; </s>
          <s xml:space="preserve">celles de ces poids <lb />paralleles auſſi; </s>
          <s xml:space="preserve">ces poids ſont égaux. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Mais s’il <lb />n’y a que celles de ces puiſſances qui le ſoient; </s>
          <s xml:space="preserve">ces
</s>
          <pb facs="0081" n="55" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
poids ſont entr’eux en raiſon réciproque des <lb />
<ptr xml:id="note-0081-01a" corresp="note-0081-01" type="noteAnchor" />
ſinus des angles que font leurs lignes de direction <lb />avec les perpendiculaires au plan GH en Q, &amp; </s>
          <s xml:space="preserve">en O. <lb /></s>
          <s xml:space="preserve">3°. </s>
          <s xml:space="preserve">Au contraire s’il n’y a que les lignes de direction <lb />de ces poids qui ſoient paralleles entr’elles; </s>
          <s xml:space="preserve">ils ſeront <lb />entr’eux en même raiſon que les ſinus des angles que <lb />font ces mêmes perpendiculaires avec les lignes de di-<lb />rection des puiſſances qui les ſoutiennent.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0081-01" corresp="note-0081-01a" place="margin">DES POIDS <lb />ſoutenus ſur <lb />des ſurfaces.</note>
            </div>
          </body>
        </floatingText>
        <p rend="italics">
          <s xml:space="preserve">Il y auroit encore bien des Corollaires à tirer de cette pro-<lb />poſition non-ſeulement par raport aux plans, mais auſſi par <lb />raport aux poli-plans: </s>
          <s xml:space="preserve">en voilà aſſés pour en pouvoir juger.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0081-01" />
          <label>0081-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">PROBLEME.</head>
        <p rend="italics">
          <s xml:space="preserve">L Apaiſſance R étant donnée, la diſpoſer tellement qu’elle <lb />
<ptr xml:id="note-0081-02a" corresp="note-0081-02" type="noteAnchor" />
puiſſe ſoutenir le poids EO auſſi donné, ſur le <lb />plan GHMN incliné, &amp; </s>
          <s xml:space="preserve">ſuivant ſa longueur GH, de la <lb />hauteur HK; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">ſuivant ſa largeur GN, de la hauteur <lb />NL.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0081-02" corresp="note-0081-02a" place="margin">fig. 39. <lb />40.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Solution.</hi></head>
        <p>
          <s xml:space="preserve">Aiant placé ce poids en quelque point, ou partie <lb />de ce plan qu’il vous plaira, de quelqu’un des points <lb />ou ſa baze le touche; </s>
          <s xml:space="preserve">par exemple, du point O, tirez <lb />OD perpendiculaire à ce plan, marquez auſſi la ligne <lb />de direction FC de ce poids, qui rencontre auſſi ce <lb />plan en L, &amp; </s>
          <s xml:space="preserve">OD prolongée en A. </s>
          <s xml:space="preserve">Enſuite de quel-<lb />que point C qu’il vous plaira de la ligne AC, faite <lb />AC à CD, comme le poids EO à la puiſſance R. <lb /></s>
          <s xml:space="preserve">1°. </s>
          <s xml:space="preserve">Si CD n’eſt pas aſſez longue pour atteindre de C <lb />juſqu’en quelque point D de la ligne AD, ce Pro-<lb />blême eſt impoſſible: </s>
          <s xml:space="preserve">parce que la diagonale tirée du
</s>
          <pb facs="0082" n="56" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
<ptr xml:id="note-0082-01a" corresp="note-0082-01" type="noteAnchor" />
point A dans le parallelogramme fait ſous ces deux <lb />lignes; </s>
          <s xml:space="preserve">c’eft-à-dire, ſous AC &amp; </s>
          <s xml:space="preserve">CD, étant alors dif-<lb />férente de AD, elle ne ſeroit pas perpendiculaire à <lb />ce plan: </s>
          <s xml:space="preserve">ainſi ce poids rouleroit alors (n. </s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve">Demonſt.) <lb /></s>
          <s xml:space="preserve">du côté de L. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Mais ſi CD peut atteindre juſqu’en <lb />quelque point D de la ligne AD, achevez le paral-<lb />lelogramme BC, &amp; </s>
          <s xml:space="preserve">placez la puiſſance R ſuivant <lb />AB: </s>
          <s xml:space="preserve">alors elle ſoutiendra ce poids ſur ce plan.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0082-01" corresp="note-0082-01a" place="margin">DES POIDS <lb />ſoutenus ſur <lb />des ſurfaces.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration.</hi></head>
        <p>
          <s xml:space="preserve">Puiſque (Hyp.) </s>
          <s xml:space="preserve">cette puiſſance eſt à ce poids com-<lb />me CD, ou AB qui lui eſt égale, eſt à AC; </s>
          <s xml:space="preserve">leur con-<lb />cours d’action doit le pouſſer (Lemm. </s>
          <s xml:space="preserve">4. </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">2.) <lb /></s>
          <s xml:space="preserve">ſuivant AD perpendiculaire (Hyp.) </s>
          <s xml:space="preserve">au plan GM, <lb />&amp; </s>
          <s xml:space="preserve">qui paſſe auſſi (Hyp.) </s>
          <s xml:space="preserve">par la baſe de ce poids: </s>
          <s xml:space="preserve"><lb />Donc (Cor. </s>
          <s xml:space="preserve">2.) </s>
          <s xml:space="preserve">il doit demeurer deſſus en équilibre <lb />avec cette puiſſance. </s>
          <s xml:space="preserve">Ce qu’il F. </s>
          <s xml:space="preserve">D.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> I.</head>
        <p>
          <s xml:space="preserve">Il eſt clair que ſi la puiſſance R ceſſoit de retenir le <lb />poids EO, il couleroit le long de OL.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> II.</head>
        <p>
          <s xml:space="preserve">Si CD eſt la plus petite ligne qui puiſſe atteindre <lb />de C juſqu’en AD; </s>
          <s xml:space="preserve">c’eſt-à-dire, ſi l’angle ADC eſt <lb />droit, l’angle BAD le ſera auſſi; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent <lb />cette puiſſance eſt la plus petite (Cor. </s>
          <s xml:space="preserve">14.) </s>
          <s xml:space="preserve">qui puiſ-<lb />ſe ſoutenir ce poids ſur ce plan, &amp; </s>
          <s xml:space="preserve">elle ne l’y poura <lb />ſoutenir non plus que (Cor. </s>
          <s xml:space="preserve">16.) </s>
          <s xml:space="preserve">ſuivant cette ſeule <lb />direction.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> III.</head>
        <p>
          <s xml:space="preserve">Si CD n’eſt pas la plus petite qui puiſſe atteindre <lb />depuis C juſqu’en AD, mais qu’elle ſoit cependant <lb />cncore moindre que AC; </s>
          <s xml:space="preserve">cette même puiſſance poura
</s>
          <pb facs="0083" n="57" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
ſoutenir ce poids ſuivant deux directions différentes; <lb /></s>
          <s xml:space="preserve">
<ptr xml:id="note-0083-01a" corresp="note-0083-01" type="noteAnchor" />
parce qu’en ce cas CD poura rencontrer AD en deux <lb />points également éloignez de la perpendiculaire tirée <lb />du point C ſur AD. </s>
          <s xml:space="preserve">Ce qui revient au Corollaire 16. <lb /></s>
          <s xml:space="preserve">de la propoſition précédente.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0083-01" corresp="note-0083-01a" place="margin">DESPOIDS <lb />ſoutenus ſur <lb />des ſurfaces.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> IV.</head>
        <p>
          <s xml:space="preserve">Enfin ſi CD eſt plus grande que AC, elle ne poura <lb />encore ſoutenir ce poids que ſuivant cette ſeule di-<lb />rection. </s>
          <s xml:space="preserve">Ce qui revient auſſi au Corollaire 18.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> V.</head>
        <p>
          <s xml:space="preserve">Mais auſſi CD pouvant être infiniment plus gran-<lb />de que AC, cette puiſſance peut auſſi être infiniment <lb />plus grande que ce poids, &amp; </s>
          <s xml:space="preserve">demeurer cependant tou-<lb />jours en équilibre avec lui. </s>
          <s xml:space="preserve">Ce qui revient encore au <lb />nombre 2. </s>
          <s xml:space="preserve">du Corollaire 11.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">Tout cela ſe peut aiſément appliquer à toutes ſortes de <lb />ſurfaces courbes: </s>
          <s xml:space="preserve">ceux pour qui ce Projet eſt écrit le voyent <lb />aſſez.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0083-01" />
          <label>0083-01</label>
        </figure>
        <pb facs="0084" n="58" />
        <fw type="head">NOUVELLE</fw>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0084-01" />
          <label>0084-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">PROPOSITION <lb />FONDAMENTALE <lb />POUR <lb />TOUTES SOR TES DE LEVIERS,</head>
        <p>
          <s xml:space="preserve">De quelque eſpéce, &amp; </s>
          <s xml:space="preserve">dans quelque ſituation <lb />qu’ils ſoient; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">pour toutes les directions <lb />poſſibles des puiſſances, ou des poids qui y <lb />ſont appliquez.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">SOIENT les puißances E &amp; </s>
          <s xml:space="preserve">F appliquées aux points <lb />
<ptr xml:id="note-0084-01a" corresp="note-0084-01" type="noteAnchor" />
O &amp; </s>
          <s xml:space="preserve">X du Levier MN, de quelque eſpéce, &amp; </s>
          <s xml:space="preserve">en <lb />quelque ſituation qu’il ſoit; </s>
          <s xml:space="preserve">quelque angle OAX que faſ-<lb />ſent auſſi entr’elles, les lignes de direction de ces puiſſances, <lb />indéfiniment prolongées vers A: </s>
          <s xml:space="preserve">Ces deux puißances feroni <lb />équilibre ſur le point fixe B de ce levier, par ou paſſe la dia-<lb />gonale AG du parallelogramme RS, dont les côtez AS &amp; </s>
          <s xml:space="preserve">AR <lb />ſont entr’eux, comme les puiſſances E, &amp; </s>
          <s xml:space="preserve">F.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0084-01" corresp="note-0084-01a" place="margin">fig 41. <lb />42. <lb />43. <lb />44. <lb />45. <lb />46.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration.</hi></head>
        <p>
          <s xml:space="preserve">Concevons pour un moment que MAN eſt la <lb />figure de ce Levier, &amp; </s>
          <s xml:space="preserve">qu’au lieu d’être tiré, ou <lb />pouſſé par les puiſſances E &amp; </s>
          <s xml:space="preserve">F, ſon point A ſoit ſeu-
</s>
          <pb facs="0085" n="59" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
lement pouſſé, mais en même-tems, vers R ſuivant <lb />
<ptr xml:id="note-0085-01a" corresp="note-0085-01" type="noteAnchor" />
AR par une puiſſance égale à F, &amp; </s>
          <s xml:space="preserve">vers S ſuivant AS <lb />par une autre puiſſance égale à E. </s>
          <s xml:space="preserve">Il eſt conſtant <lb />(Lemm. </s>
          <s xml:space="preserve">3.) </s>
          <s xml:space="preserve">que l’impreſſion compoſée que ce point <lb />recevroit alors du concours d’action de ces deux <lb />puiſſances, s’il étoit ainſi pouſſé, ne tendroit qu’à le <lb />mouvoir ſuivant la diagonale AG du parallelogram-<lb />me RS; </s>
          <s xml:space="preserve">ainſi ne faiſant d’impreſſion ſur tout le corps <lb />MAN, qu’autant que le point A, à raiſon de l’ob-<lb />ſtacle qu’il leur fait, lui en communique, toute l’ac-<lb />tion de ces deux puiſſances ſur ce corps, ſe trouveroit <lb />réünie dans la ſeule ligne AG, ou AB; </s>
          <s xml:space="preserve">ſi donc il <lb />ſe trouvoit quelque point fixe dans cette ligne, par <lb />exemple B, ce point ſoutiendroit, lui ſeul, toute <lb />l’impreſſion de ces deux puiſſances ſur ce corps, ou <lb />ce Levier; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent ce corps n’en ayant <lb />alors que ce qu’elles lui en communiquent, demeu-<lb />reroit ainſi en équilibre ſur ce point, ſans qu’aucune <lb />d’elles l’emportât ſur l’autre. </s>
          <s xml:space="preserve">Oſtons préſentement <lb />ces deux puiſſances, &amp; </s>
          <s xml:space="preserve">remettons les deux premiéres <lb />E, &amp; </s>
          <s xml:space="preserve">F en action comme auparavant, prenant encore <lb />MAN pour la figure du Levier, ou elles ſont appli-<lb />quées. </s>
          <s xml:space="preserve">Il eſt clair que ces deux puiſſances faiſant <lb />toute la même impreſſion ſur le point A de ce Levier, <lb />&amp; </s>
          <s xml:space="preserve">ſuivant la même direction AG, que faiſoient <lb />auparavant celles que nous leur avions ſuppoſées <lb />égales; </s>
          <s xml:space="preserve">leur action doit ſe trouver de même que <lb />celle de ces deux ſuppoſées, toute réünie dans la <lb />ſeule ligne AB: </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent le point fixe B la <lb />ſoutenant, lui ſeul, toute entiére, elles doivent encore <lb />demeurer en équilibre ſur ce point. </s>
          <s xml:space="preserve">Et ſi enfin on <lb />retranche la partie MAN du corps AMN, en ſorte <lb />qu’il n’en reſte plus que le Levier MN: </s>
          <s xml:space="preserve">Il eſt encore <lb />clair que les puiſſances E &amp; </s>
          <s xml:space="preserve">F agiſſant encore ſur ce <lb />levier de même que lors qu’il étoit joint à la partie
</s>
          <pb facs="0086" n="60" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
<ptr xml:id="note-0086-01a" corresp="note-0086-01" type="noteAnchor" />
retranchée, toute leur action doit encore ſe trouver <lb />réünie dans le ſeul point B de ce levier, par ou paſſe <lb />la diagonale AG du parallelogramme RS; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par <lb />conſéquent, elles doivent encore demeurer en équi-<lb />libre ſur ce point. </s>
          <s xml:space="preserve">Ce qu’il faloit démontrer.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0085-01" corresp="note-0085-01a" place="margin">DES <lb />LEVIERS.</note>
              <note xml:space="preserve" xml:id="note-0086-01" corresp="note-0086-01a" place="margin">DES <lb />LEVIERS.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> I.</head>
        <p>
          <s xml:space="preserve">On voit aſſez qu’en quelque ſituation, de quel-<lb />que eſpéce, &amp; </s>
          <s xml:space="preserve">de quelque figure, que ſoit le levier <lb />auquel deux puiſſances, telles qu’elles ſoient, ſont <lb />appliquées, elles ſeront toujours en équilibre, quelque <lb />angle que faſſent entr’elles leurs lignes de direction, <lb />tant qu’il y aura un point fixe de ce levier dans la <lb />diagonale AG; </s>
          <s xml:space="preserve">c’eſt pourquoi on ne s’arrête point <lb />ici à exprimer les figures detous les cas de cette pro-<lb />poſition, chacun le pourra faire à ſon loiſir.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> II.</head>
        <p>
          <s xml:space="preserve">On voit encore que les deux mêmes puiſſances E <lb />&amp; </s>
          <s xml:space="preserve">F peuvent faire ſucceſſivement équilibre ſur une <lb />infinité de points B de ce même levier en changeant <lb />ſeulement leurs directions: </s>
          <s xml:space="preserve">puis qu’on les peut varier <lb />en tant de maniéres que AG paſſera ſucceſſivement <lb />par tous les points imaginables de ce levier, excepté <lb />par les points O &amp; </s>
          <s xml:space="preserve">X, où ces deux puiſſances ſont <lb />appliquées.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> III.</head>
        <p>
          <s xml:space="preserve">Ce qui fait voir que dans la ſuppoſition du concours <lb />des lignes de direction des poids au centre de la terre, <lb />leurs centres de gravité, ou de direction peuvent chan-<lb />ger inceſſamment à meſure qu’ils s’en approchent, ou <lb />qu’ils s’en éloignent, ſelon la différente ſituation qu’ils <lb />peuvent avoir par raport à lui, excepté dans les ſphéri-<lb />ques. </s>
          <s xml:space="preserve">On nes’arrête point à démontrer cela ſur des fi-
</s>
          <pb facs="0087" n="61" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
gures particuliéres, parce qu’il ſuit ſi naturellement <lb />
<ptr xml:id="note-0087-01a" corresp="note-0087-01" type="noteAnchor" />
du Corollaire 2. </s>
          <s xml:space="preserve">qu’il n’y a perſonne qui ne le puiſſe <lb />faire de ſoi-même.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0087-01" corresp="note-0087-01a" place="margin">DES <lb />LEVIERS.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> IV.</head>
        <p>
          <s xml:space="preserve">On voit de plus de cette propoſition que le point fixe <lb />de ce levier, où bien ſon appui B eſt pouſſé de A vers <lb />G ſuivant AG par l’impreſſion compoſée qu’il reçoit <lb />du concours d’action de ces deux puiſſances, &amp; </s>
          <s xml:space="preserve">que <lb />la réſiſtance qu’il leur fait, étant égale à cette même <lb />impreſſion, eſt à la force de chacune d’elles (Lemm. <lb /></s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">3.) </s>
          <s xml:space="preserve">Comme la diagonale AG à chacun des <lb />côtez du parallelogramme RS, qui les répréſen-<lb />tent; </s>
          <s xml:space="preserve">c’eſt-à-dire, que cette réſiſtance du point fixe, <lb />où bien de l’appui B de ce levier, eſt à la force de la <lb />puiſſance E, comme AG à AS; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">à celle de la puiſ-<lb />ſance F, comme la même AG à AR.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> V.</head>
        <p>
          <s xml:space="preserve">D’où il ſuit que lors que l’angle OAX eſt infini-<lb />ment aigu, c’eſt-à-dire, lors que les lignes de direc-<lb />tion EX &amp; </s>
          <s xml:space="preserve">OF des puiſſances E &amp; </s>
          <s xml:space="preserve">F ſont paralleles, <lb />le point A étant alors infiniment éloigné de B, la <lb />ligne AG, c’eſt-à-dire, (Cor. </s>
          <s xml:space="preserve">4.) </s>
          <s xml:space="preserve">la direction de <lb />l’appui B leur eſt auſſi parallele, &amp; </s>
          <s xml:space="preserve">toujours vers <lb />l’endroit, où tendent ces deux puiſſances, lors qu’elles <lb />tirent du même côté; </s>
          <s xml:space="preserve">ou bien vers celui, ou tend la <lb />plus proche de cet appui, lors qu’elles tirent de diffé-<lb />rens cótez.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> VI.</head>
        <p>
          <s xml:space="preserve">Il ſuit encore du Corollaire 4. </s>
          <s xml:space="preserve">pour tous les leviers <lb />
<ptr xml:id="note-0087-02a" corresp="note-0087-02" type="noteAnchor" />
de l’eſpéce exprimée dans les figures 41. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">42. </s>
          <s xml:space="preserve">que <lb />plus l’angle OAX, que les lignes de direction des <lb />puiſſances E &amp; </s>
          <s xml:space="preserve">F, font entr’elles, ſera obtus, moins
</s>
          <pb facs="0088" n="62" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
<ptr xml:id="note-0088-01a" corresp="note-0088-01" type="noteAnchor" />
ſera grande la charge de l’appui B de chacun de ces le-<lb />viers; </s>
          <s xml:space="preserve">parce que plus cet angle ſera obtus, moins ſera <lb />grande la raiſon de AG aux côtez du parallelogramme <lb />RS, dont elle eſt diagonale, quoi qu’en proportion <lb />différente: </s>
          <s xml:space="preserve">De ſorte que l’on peut faire cet angle <lb />ſi obtus que la charge de l’appui B de ce levier ſera <lb />ſi petite qu’on voudra, quoi que les deux mêmes <lb />puiſſances demeurent toujours en équilibre deſſus; <lb /></s>
          <s xml:space="preserve">juſque-là même qu’elle peut devenir indéfiniment <lb />petite, c’eſt-à-dire, moindre que quelque poids don-<lb />né que ce ſoit. </s>
          <s xml:space="preserve">Il ne faut pour cela qu’ouvrir l’angle <lb />OAX juſqu’à ce que la diagonale AG du paralle-<lb />logramme RS, ſoit à chacun de ſes côtez AR &amp; </s>
          <s xml:space="preserve"><lb />AS en moindre raiſon que celle qui eſt entre ce poids <lb />donné, &amp; </s>
          <s xml:space="preserve">chacune des puiſſances F &amp; </s>
          <s xml:space="preserve">E que l’on ſup-<lb />poſe appliquées à ce levier.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0087-02" corresp="note-0087-02a" place="margin">fig. 41. <lb />42.</note>
              <note xml:space="preserve" xml:id="note-0088-01" corresp="note-0088-01a" place="margin">DES <lb />LEVIERS.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> VII.</head>
        <p>
          <s xml:space="preserve">La charge de ce point ne peut pas de même <lb />augmenter à l’infini: </s>
          <s xml:space="preserve">Car ne pouvant jamais être <lb />plus grande que lors que l’angle OAX eſt infini-<lb />ment aigu, c’eſt-à-dire, lors que les lignes de direc-<lb />tion de ces deux puiſſances ſont paralleles; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">la <lb />diagonale AG n’étant encore alors qu’égale à la <lb />ſomme des côtez AR &amp; </s>
          <s xml:space="preserve">RG du parallelogramme <lb />RS alors infiniment long; </s>
          <s xml:space="preserve">la charge de cet appui ne <lb />peut être, tout au plus, qu’égale à la ſomme des puiſ-<lb />ſances E &amp; </s>
          <s xml:space="preserve">F.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> VIII.</head>
        <note xml:space="preserve" place="margin">fig. 43. <lb />44. <lb />45. <lb />46.</note>
        <p>
          <s xml:space="preserve">Pour les leviers des eſpeces exprimées dans les <lb />figures 43. </s>
          <s xml:space="preserve">44. </s>
          <s xml:space="preserve">45. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">46. </s>
          <s xml:space="preserve">Il en va tout autrement: <lb /></s>
          <s xml:space="preserve">car plus l’angle OAX eſt obtus, plus la charge, <lb />ou la réſiſtance de l’appui B eſt grande; </s>
          <s xml:space="preserve">parce que <lb />la raiſon de la diagonale AG à chacun des côtez du
</s>
          <pb facs="0089" n="63" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
parallelogramme RS, en eſt plus grande, quoi qu’en <lb />
<ptr xml:id="note-0089-01a" corresp="note-0089-01" type="noteAnchor" />
proportion différente; </s>
          <s xml:space="preserve">mais elle ne peut pas pour <lb />cela augmenter à l’infini: </s>
          <s xml:space="preserve">car ne pouvant jamais être <lb />plus grande que lors que cet angle eſt infiniment <lb />obtus, c’eſt-à-dire, lors que les lignes de direction <lb />de ces puiſſances concourent en une ſeule ligne <lb />droite; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">la diagonale AG n’étant alors qu’égale à <lb />la ſomme des côtez AR &amp; </s>
          <s xml:space="preserve">GR du parallelogramme <lb />RS alors encore infiniment long; </s>
          <s xml:space="preserve">la réſiſtance de cet <lb />appui ne peut par conféquent être encore, toutau plus, <lb />qu’égale à la ſomme des forces de ces deux puiſſances.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0089-01" corresp="note-0089-01a" place="margin">DES <lb />LEVIERS.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> IX.</head>
        <p>
          <s xml:space="preserve">Au contraire, plus cet angle OAX eſt aigu, <lb />moins eſt grande la charge, ou la réſiſtance de l’ap-<lb />pui B dece levier: </s>
          <s xml:space="preserve">car plus cet angle eſt aigu, moins <lb />eſt grande la raiſon de la diagonale AG aux côtez <lb />du parallelogramme RS, quoi qu’en proportion dif-<lb />férente; </s>
          <s xml:space="preserve">mais elle ne peut pas non plus ainſi diminuer <lb />à l’infini de même que nous venons de dire (Cor. </s>
          <s xml:space="preserve">6.) <lb /></s>
          <s xml:space="preserve">qu’elle le peut dans les leviers de l’eſpece exprimée <lb />dans les figures 41. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">42. </s>
          <s xml:space="preserve">Car ne pouvant jamais être <lb />moindre que lors que cet angle eſt infiniment aigu, <lb />c’eſt-à-dire, lors que les lignes de direction de ces <lb />puiſſances deviennent parallel’es; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">le point G, qui <lb />à meſure que cet angle devient plus aigu, s’approche <lb />de plus en plus de la ligne AR, (fig. </s>
          <s xml:space="preserve">43. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">44.) </s>
          <s xml:space="preserve"><lb />ou AS (fig. </s>
          <s xml:space="preserve">45. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">46.) </s>
          <s xml:space="preserve">entrant alors dans cette <lb />ligne, AG demeure encore égale à la différence de <lb />AR à AS; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent la charge, ou la réſiſ-<lb />tance d’e l’appui B ne peut jamais être moindre que <lb />la différence des forces des puiſſances E &amp; </s>
          <s xml:space="preserve">F.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> X.</head>
        <p>
          <s xml:space="preserve">D’où l’on voit en général 1°. </s>
          <s xml:space="preserve">que dans toutes ſor-
</s>
          <pb facs="0090" n="64" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
<ptr xml:id="note-0090-01a" corresp="note-0090-01" type="noteAnchor" />
tes de Leviers, de quelque figure, en quelque ſitua-<lb />tion, &amp; </s>
          <s xml:space="preserve">de quelque eſpéce qu’ils ſoient, quelles que <lb />ſoient auſſi les lignes de direction de puiſſances, ou <lb />des poids qui y ſont appliquez, la charge de leur apui <lb />
<ptr xml:id="note-0090-02a" corresp="note-0090-02" type="noteAnchor" />
ne peut être jamais plus grande (Corol. </s>
          <s xml:space="preserve">7. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">8.) <lb /></s>
          <s xml:space="preserve">que la ſomme de ces poids, ou de ces puiſſances. </s>
          <s xml:space="preserve"><lb />2°. </s>
          <s xml:space="preserve">que dans les leviers de l’eſpéce exprimée par les <lb />figures 41. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">42. </s>
          <s xml:space="preserve">elle peut (Cor. </s>
          <s xml:space="preserve">6.) </s>
          <s xml:space="preserve">diminuer à l’infi-<lb />ni. </s>
          <s xml:space="preserve">3°. </s>
          <s xml:space="preserve">Mais que dans toute autre eſpéce (fig. </s>
          <s xml:space="preserve">43. </s>
          <s xml:space="preserve">44. </s>
          <s xml:space="preserve"><lb />45. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">46.) </s>
          <s xml:space="preserve">elle ne peut jamais être moindre (Cor. </s>
          <s xml:space="preserve">9.) </s>
          <s xml:space="preserve"><lb />que la différence des deux puiſſances, ou des deux <lb />poids qui y ſont appliquez.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0090-01" corresp="note-0090-01a" place="margin">DES <lb />LEVIERS.</note>
              <note xml:space="preserve" xml:id="note-0090-02" corresp="note-0090-02a" place="margin">fig. 41. <lb />42. <lb />43. <lb />44. <lb />45. <lb />46.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">Perſonne que je fçache n’avoit encore démontré la charge, <lb />n’y la direction des points d’apuy des leviers: </s>
          <s xml:space="preserve">il ne paroit p@ls <lb />même qu’il ſoit aiſé de le faire par les principes ordinaires; <lb /></s>
          <s xml:space="preserve">ſans cela cependant il y à bien des Problêmes qu’on ne ſçau-<lb />roit réſoudre. </s>
          <s xml:space="preserve">Par exemple, ſans la connoiſſance de la direc-<lb />tion des apuis, il n’eſt pas poſſible de démontrer qu’elles doi-<lb />vent être les directions de deux puiſſances, ſoit égales, <lb />ſoit inégales, pour qu’elles puiſſent faire équilibre ſur <lb />quelque levier que ce ſoit, dont l’apui eſt une ſphére; </s>
          <s xml:space="preserve">n’y <lb />ſur combien de points de ce levier ainſi apuié, il eſt poſſi-<lb />ble qu’elles faſſent équilibre en changeant ſeulement <lb />leurs directions. </s>
          <s xml:space="preserve">Il n’eſt pas poſſible non plus ſans la connoiſ-<lb />ſance &amp; </s>
          <s xml:space="preserve">de la direction, &amp; </s>
          <s xml:space="preserve">de la charge des apuis des leviers de <lb />trouver le point d’apui de celui auquel tant de puiſ-<lb />ſances qu’on voudra, ſoient appliquées, pour toutes <lb />les directions poſſibles dans leſquelles on les peut ſup-<lb />poſer; </s>
          <s xml:space="preserve">ny deux puiſſances étant données avec leurs <lb />directions &amp; </s>
          <s xml:space="preserve">leurs points d’application à un levier, <lb />de trouver quelle doit être la direction, &amp; </s>
          <s xml:space="preserve">le point <lb />d’application d’une troiſiéme puiſſance auſſi donnée, <lb />pour que toutes trois enſemble faſſent équilibre ſur <lb />quelque point donné, que ce ſoit, de ce levier. </s>
          <s xml:space="preserve">Ilfaut
</s>
          <pb facs="0091" n="65" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
penſer la même choſe de tout autre Problême ſur les leviers <lb />
<ptr xml:id="note-0091-01a" corresp="note-0091-01" type="noteAnchor" />
dont la ſolution dépend de la détermination de la charge, <lb />&amp; </s>
          <s xml:space="preserve">de la direction de leurs apuis.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0091-01" corresp="note-0091-01a" place="margin">DES <lb />LEVIERS.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XI.</head>
        <p>
          <s xml:space="preserve">Il ſuit encore de cette propoſition que les puiſſan-<lb />ces E &amp; </s>
          <s xml:space="preserve">F, qui demeurent ainſi en équilibre ſur le <lb />levier MN, ſont en raiſon réciproque des lignes BD <lb />&amp; </s>
          <s xml:space="preserve">BP tirées de ſon point d’apui B perpendiculaire-<lb />ment ſur leurs lignes de direction, qu’elles quelles <lb />ſoient: </s>
          <s xml:space="preserve">Car puiſque la puiſſance E eſt à la puiſſance <lb />F, comme AS, ou GR à AR; </s>
          <s xml:space="preserve">c’eſt-à-dire, (Lemm. <lb /></s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">comme le ſinus de l’angle GAR, ou de OAB ſon <lb />(fig. </s>
          <s xml:space="preserve">41. </s>
          <s xml:space="preserve">42. </s>
          <s xml:space="preserve">43. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">44.) </s>
          <s xml:space="preserve">égal, ou (fig. </s>
          <s xml:space="preserve">45. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">46.) </s>
          <s xml:space="preserve"><lb />ſon complement, eſt au ſinus de l’angle RGA, ou de <lb />XAB ſon (fig. </s>
          <s xml:space="preserve">41. </s>
          <s xml:space="preserve">42. </s>
          <s xml:space="preserve">43. </s>
          <s xml:space="preserve">45. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">46.) </s>
          <s xml:space="preserve">égal, ou (fig. </s>
          <s xml:space="preserve"><lb />44.) </s>
          <s xml:space="preserve">ſon complement; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">que d’ailleurs BP eſt le <lb />ſinus de l’angle OAB, &amp; </s>
          <s xml:space="preserve">BD celui de l’angle XAB: </s>
          <s xml:space="preserve">Il <lb />ſuit quela puiſſance E eſt à la puiſſance F, comme BP <lb />à BD; </s>
          <s xml:space="preserve">c’eſt-à-dire, en raiſon réciproque des diſtances <lb />de leurs lignes de direction, au point d’appui de leur <lb />levier. </s>
          <s xml:space="preserve">Ce qui fait que lors que l’angle OAX eſt <lb />infiniment aigu, c’eſt-à-dire, lors que les lignes de <lb />direction de ces deux puiſſances ſont paralleles, &amp; </s>
          <s xml:space="preserve"><lb />que ce levier eſt droit, quelque ſituation qu’il ait, <lb />ces deux puiſſances ſont toujours entr’elles, tant <lb />que dure leur équilibre, en raiſon réciproque des <lb />bras de ce levier pris depuis ſon point d’appui, juſ-<lb />qu’aux points où elles lui ſont appliquées.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XII.</head>
        <p>
          <s xml:space="preserve">L’inverſe de ce dernier Corollaire ſuit encore ma-<lb />nifeſtement de cette propoſition: </s>
          <s xml:space="preserve">ſçavoir que lors
</s>
          <pb facs="0092" n="66" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
que ces deux puiſſances ſont en raiſon réciproque <lb />
<ptr xml:id="note-0092-01a" corresp="note-0092-01" type="noteAnchor" />
des diſtances de leurs lignes de direction au point <lb />d’appui de leur levier, de quelque eſpece qu’il ſoit, <lb />elles demeurent toûjours en équilibre; </s>
          <s xml:space="preserve">puis - qu’un tel <lb />point ne ſe peut trouver ailleurs que dans la diagonale <lb />AG du parallelogramme RS: </s>
          <s xml:space="preserve">ainſi lorſque, leurs lignes <lb />de direction étant paralleles, &amp; </s>
          <s xml:space="preserve">leur levier droit, <lb />elles ſont en raiſon réciproque des bras de ce levier, <lb />elles demeurent toujours enéquilibre deſſus.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0092-01" corresp="note-0092-01a" place="margin">DES <lb />LEVIERS.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> XIII.</head>
        <p rend="italics">
          <s xml:space="preserve">D’où l’on voit en général que lors que deux puiſſances <lb />font équilibre ſur un levier, de quelque eſpece, &amp; </s>
          <s xml:space="preserve">en quelque <lb />ſituation qu’il ſoit, elles ſont toujours entr’elles en raiſon <lb />réciproque des diſtances de leurs lignes de direction au point <lb />d’appui de ce levier. </s>
          <s xml:space="preserve">Et réciproquement auſſi, lors qu’elles <lb />ſont en raiſon réciproque des diſtances de ces mémes lignes au <lb />point d’appui de ce levier, de quelque eſpece, de quelque figure, <lb />&amp; </s>
          <s xml:space="preserve">en quelque ſituation qu’il ſoit, elles font toujours équilibre <lb />deſſus.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">Voila ce qu’on appelle ordinairement le premier principe <lb />de Méchanique, &amp; </s>
          <s xml:space="preserve">ce que perſonne, du moins que je con-<lb />noiſſe, n’avoit encore démontré de cette maniére, n’y ſi gé-<lb />néralement. </s>
          <s xml:space="preserve">Le voici encore d’une autre façon.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0092-01" />
          <label>0092-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">LEMME VI.</head>
        <p rend="italics">
          <s xml:space="preserve">S I deux puiſſances D &amp; </s>
          <s xml:space="preserve">E appliquées au même point A <lb />
<ptr xml:id="note-0092-02a" corresp="note-0092-02" type="noteAnchor" />
d’un levier AB, dont le point fixe ſoit B, ſont entr’elles <lb />en raiſon réciproque des ſinus des angles que font leurs lignes <lb />de direction, qu’elles quelles ſoient, avec ce levier; </s>
          <s xml:space="preserve">elles <lb />demeureront en équilibre.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0092-02" corresp="note-0092-02a" place="margin">fig. 47. <lb />48. <lb />49.</note>
            </div>
          </body>
        </floatingText>
        <pb facs="0093" n="67" />
        <fw type="head">MECHANIQUE.</fw>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration.</hi></head>
        <note xml:space="preserve" place="margin">DES <lb />LEVIERS.</note>
        <p>
          <s xml:space="preserve">Le point A ainſi tiré par les puiſſances D &amp; </s>
          <s xml:space="preserve">E, <lb />doit en recevoir une impreſſion ſuivant quelque <lb />ligne AG qui ſoit la diagonale d’un parallelogramme <lb />RS fait ſous des parties de leurs lignes de direction <lb />AS &amp; </s>
          <s xml:space="preserve">AR qui ſoient entr’elles, (Lemm. </s>
          <s xml:space="preserve">3.) </s>
          <s xml:space="preserve">comme <lb />ces mêmes puiſſances; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">la force de cette impreſſion <lb />doit être à chacune des puiſſances D &amp; </s>
          <s xml:space="preserve">E, comme <lb />(Lem. </s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">3.) </s>
          <s xml:space="preserve">AG à chacune des lignes AS &amp; </s>
          <s xml:space="preserve">AR, <lb />ou SG qui lui eſt égale; </s>
          <s xml:space="preserve">c’eſt-à-dire, (Lem. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">comme <lb />le ſinus de l’angle ASG, à chacun des ſinus des angles <lb />AGS, ou GAR qui lui eſt égal, &amp; </s>
          <s xml:space="preserve">GAS; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſé-<lb />quent les puiſſances D &amp; </s>
          <s xml:space="preserve">E ſont entr’elles, commeles ſi-<lb />nus GAR &amp; </s>
          <s xml:space="preserve">GAS. </s>
          <s xml:space="preserve">Elles ſont auſſi (hyp.) </s>
          <s xml:space="preserve">entr’elles, com-<lb />me les ſinus des angles RAB &amp; </s>
          <s xml:space="preserve">SAB; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſé-<lb />quent les ſinus de GAR &amp; </s>
          <s xml:space="preserve">de RAB, de même que <lb />ceux de GAS &amp; </s>
          <s xml:space="preserve">SAB ſont égaux entr’eux: </s>
          <s xml:space="preserve">donc les an-<lb />gles GAR &amp; </s>
          <s xml:space="preserve">RAB, auſſi-bien que GAS &amp; </s>
          <s xml:space="preserve">SAB, ſont <lb />auſſi égaux, ou, du moins, complemens l’un de l’autre à <lb />deux droits. </s>
          <s xml:space="preserve">D’où il ſuit que AG eſt en ligne droite avec <lb />AB; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent le point fixe B dulevier AB ſou-<lb />tient, lui ſeul, l’impreſſion toute entiére que le point A <lb />reçoit du concours d’action des puiſſances D &amp; </s>
          <s xml:space="preserve">E; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">ce <lb />point demeurant ainſi en repos, ces puiſſances doivent <lb />auſſi par conſéquent demeurer en équilibre. </s>
          <s xml:space="preserve">Ce qu’il <lb />faloit démontrer.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> I.</head>
        <p>
          <s xml:space="preserve">On voit de-là qu’une même puiſſance peut ainſi <lb />faire ſucceſſivement équilibre avec pluſieurs autres, <lb />quelques grandes, ou quelques petites qu’on les ſuppo-<lb />ſe, pourvu qu’elle ſoit à chacune d’elles en raiſon ré-
</s>
          <pb facs="0094" n="68" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
<ptr xml:id="note-0094-01a" corresp="note-0094-01" type="noteAnchor" />
ciproque des ſinus des angles que font avec ce levier <lb />ſa ligne de direction, &amp; </s>
          <s xml:space="preserve">celle de la puiſſance avec <lb />laquelle on la compare; </s>
          <s xml:space="preserve">c’eſt-à-dire, pourvû que les <lb />produits de ces deux puiſſances par les perpendicu-<lb />laires tirées du point d’appui de ce levier ſur leurs <lb />lignes de direction, ſoient égaux.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0094-01" corresp="note-0094-01a" place="margin">DES <lb />LEVIERS.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> II.</head>
        <p>
          <s xml:space="preserve">D’où l’on voit que l’action d’une puiſſance ne ſe <lb />prend pas ſeulement de la grandeur de ſa force; </s>
          <s xml:space="preserve">mais <lb />auſſi de la diſtance de ſa ligne de direction au point <lb />d’appui du levier ſur lequel elle agit: </s>
          <s xml:space="preserve">De ſorte que <lb />le produit de cette diſtance par la force de cette puiſ-<lb />ſance, eſt la meſure juſte de ſon action, ou de l’im-<lb />preſſion qu’elle fait ſur ce levier.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> III.</head>
        <p>
          <s xml:space="preserve">Ainſi en quelque point que ce ſoit d’un levier <lb />quelle ſoit appliquée, pourvû que la diſtance du <lb />point d’appui de ce levier à ſa ligne de direction ſoit <lb />toujours la même, ſon action ſur ce levier ſera auſſi <lb />toujours la même.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> IV.</head>
        <p>
          <s xml:space="preserve">Et par la même raiſon ſi différentes puiſſances éga-<lb />les agiſſoient ſucceſſivement ſuivant la même direc-<lb />tion, ou ſuivant des directions également diſtantes <lb />du point d’appui du levier auquel elles ſeroient appli-<lb />quées; </s>
          <s xml:space="preserve">leurs actions ſur ce levier ſeroient auſſi-<lb />égales.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> V.</head>
        <p>
          <s xml:space="preserve">Et réciproquement ſi ces puiſſances ainſi appliquées <lb />à ce levier agiſſent également ſur lui, elles ſeront
</s>
          <pb facs="0095" n="69" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
auſſi égales entr’elles: </s>
          <s xml:space="preserve">puis que les diſtances de leurs <lb />
<ptr xml:id="note-0095-01a" corresp="note-0095-01" type="noteAnchor" />
lignes de direction au point d’appui du levier auquel <lb />elles ſont appliquées, ſont (hyp.) </s>
          <s xml:space="preserve">égales, &amp; </s>
          <s xml:space="preserve">que les <lb />produits de chacune d’elles par la force de chacune <lb />de ces puiſſances, ſont (Cor. </s>
          <s xml:space="preserve">2.) </s>
          <s xml:space="preserve">auſſi égaux.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0095-01" corresp="note-0095-01a" place="margin">DES <lb />LEVIERS.</note>
            </div>
          </body>
        </floatingText>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0095-01" />
          <label>0095-01</label>
        </figure>
        <pb facs="0096" n="70" />
        <fw type="head">NOUVELLE</fw>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0096-01" />
          <label>0096-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">AUTRE <lb />PROPOSITION <lb />DES LEVIERS, <lb />Pour tous les cas poſſibles de la fondamentale <lb />précédente.</head>
        <p rend="italics">
          <s xml:space="preserve">SI les puiſſances E &amp; </s>
          <s xml:space="preserve">F appliquées à diſſérens points X <lb />
<ptr xml:id="note-0096-01a" corresp="note-0096-01" type="noteAnchor" />
&amp; </s>
          <s xml:space="preserve">O du levier BO, de quelque ſigure, de quelque eſpéce, <lb />&amp; </s>
          <s xml:space="preserve">en quelque ſituation qu’il ſoit; </s>
          <s xml:space="preserve">ſont entr’elles en raiſon <lb />rèciproque des diſtances BD &amp; </s>
          <s xml:space="preserve">BP de leurs lignes de direction <lb />XE &amp; </s>
          <s xml:space="preserve">OF, qu’elles quelles ſoient, au point ſixe B de ce <lb />levier; </s>
          <s xml:space="preserve">c’eſt-à-dire, ſi E. </s>
          <s xml:space="preserve">F. </s>
          <s xml:space="preserve">:</s>
          <s xml:space="preserve">: BP. </s>
          <s xml:space="preserve">BD. </s>
          <s xml:space="preserve">Ces deux <lb />puiſſances ainſi appliquées demeureront en équilibre ſur ce <lb />levier.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0096-01" corresp="note-0096-01a" place="margin">ſig 50. <lb />51. <lb />52.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration</hi>.</head>
        <p>
          <s xml:space="preserve">Si la puiſſance E étoit appliquée en O ſuivant une <lb />ligne de direction OQ, dont la diſtance BQ au point <lb />d’appui B de ce levier, fût égale à BD qui eſt celle <lb />de ce même point à la ligne de direction XE qu’elle <lb />a préſentement, cette puiſſance (Lemm. </s>
          <s xml:space="preserve">6.) </s>
          <s xml:space="preserve">demeu-<lb />reroit en équilibre avec la puiſſance F. </s>
          <s xml:space="preserve">Or l’action <lb />de cette puiſſance appliquée en X ſuivant XE, eſt <lb />la même (Lemm. </s>
          <s xml:space="preserve">6. </s>
          <s xml:space="preserve">Corol. </s>
          <s xml:space="preserve">3.) </s>
          <s xml:space="preserve">qu’elle ſeroit alors ſur <lb />ce levier: </s>
          <s xml:space="preserve">Donc ces deux puiſſances ainſi appliquées
</s>
          <pb facs="0097" n="71" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
en X &amp; </s>
          <s xml:space="preserve">en O, doivent demeurer en équilibre. </s>
          <s xml:space="preserve">Ce qu’il <lb />
<ptr xml:id="note-0097-01a" corresp="note-0097-01" type="noteAnchor" />
faloit démontrer.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0097-01" corresp="note-0097-01a" place="margin">DES <lb />LEVIERS.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi>.</head>
        <p>
          <s xml:space="preserve">Il ſuit réciproquement de cette propoſition que ſi <lb />les puiſſances E &amp; </s>
          <s xml:space="preserve">F font équilibre ſur quelque levier <lb />que ce ſoit, elles ſeront entr’elles en raiſon récipro-<lb />que des diſtances de ſon point d’appui à leurs lignes de <lb />direction: </s>
          <s xml:space="preserve">puis que ſi quelque nouvelle puiſſance miſe <lb />en la place, par exemple, de la puiſſance E, &amp; </s>
          <s xml:space="preserve">appli-<lb />quée comme elle au levier BO, étoit en telle raiſon à la <lb />puiſſance F, elle feroit équilibre avec elle. </s>
          <s xml:space="preserve">Orune telle <lb />puiſſance (Lemm. </s>
          <s xml:space="preserve">6. </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">ſeroit égale à la puiſſance <lb />E: </s>
          <s xml:space="preserve">Donc la puiſſance E ſeroit auſſi alors à la puiſſance <lb />F en raiſon réciproque des diſtances de leurs lignes <lb />de direction au point d’appui du levier ſur lequel <lb />elles feroient équilibre.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">On ne met point ici tous les Corollaires qu’on pourroit tirer <lb />tant de cette propoſition, que de la précédente, par raport à la <lb />Balance, à la Romaine, au Tour, aux Rouës à dent, aux Ci-<lb />ſeaux, aux Tenailles, aux Etocs, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">ce ſera lors qu’on en <lb />fera l’application à la phyſique; </s>
          <s xml:space="preserve">D’ailleurs tres-peu d’atten-<lb />tion ſuſſit préſentement pour en déduire beaucoup plus que la <lb />breveté, qu’on s’eſt propoſée dans ce projet, ne permet de ſaire.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0097-01" />
          <label>0097-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">PROBLEME.</head>
        <p rend="italics">
          <s xml:space="preserve">TANT de puiſſances qu’on voudra appliquées à un <lb />
<ptr xml:id="note-0097-02a" corresp="note-0097-02" type="noteAnchor" />
même levier; </s>
          <s xml:space="preserve">par exemple, les cinq que voici M, N, <lb />O, P, Q, étant données avec leurs lignes de direction AM, <lb />CN, EO, HP, &amp; </s>
          <s xml:space="preserve">GQ, quelles quelles ſoient; </s>
          <s xml:space="preserve">trouver le <lb />point de ce levier ſur lequel elles peuvent ainſi appliquées de-<lb />meurer toutes enſemble en équilibre.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0097-02" corresp="note-0097-02a" place="margin">ſig. 53. <lb />54. <lb />55. <lb />56. <lb />57. <lb />58. <lb />59.</note>
            </div>
          </body>
        </floatingText>
        <pb facs="0098" n="72" />
        <fw type="head">NOUVELLE</fw>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Solution</hi>.</head>
        <note xml:space="preserve" place="margin">DES <lb />LEVIERS.</note>
        <p>
          <s xml:space="preserve">Premiérement ſi ces lignes de direction ſont toutes <lb />
<ptr xml:id="note-0098-02a" corresp="note-0098-02" type="noteAnchor" />
paralleles entr’elles, de quelque côté que ces puiſ-<lb />ſances tirent, il faut prendre ſur le levier AH pro-<lb />longé s’il en eſt beſoin, H λ à G λ, commela puiſſance <lb />Q eſt à la puiſſance P, &amp; </s>
          <s xml:space="preserve">I’on aura le point λ ſur le-<lb />quel ces deux puiſſances ainſi appliquées feroient <lb />é<unclear reason="illegible" />quilibre, (Corol. </s>
          <s xml:space="preserve">12.) </s>
          <s xml:space="preserve">ſi elles étoient ſeules. </s>
          <s xml:space="preserve">La <lb />direction de ce point (Cor. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">étant vers Q paralle-<lb />lement à HP, c’eſt-à-dire, (hyp.) </s>
          <s xml:space="preserve">à EO; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">ſa charge <lb />étant (Cor. </s>
          <s xml:space="preserve">7. </s>
          <s xml:space="preserve">ſig. </s>
          <s xml:space="preserve">53.) </s>
          <s xml:space="preserve">égale à la ſomme des forces de <lb />ces deux puiſſances, ou (Cor. </s>
          <s xml:space="preserve">9. </s>
          <s xml:space="preserve">ſig. </s>
          <s xml:space="preserve">54. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">55.) </s>
          <s xml:space="preserve">à leur <lb />diffèrence: </s>
          <s xml:space="preserve">au lieu d’elles on en peut ſuppoſer une <lb />nouvelle de cette valeur appliquée en ce point λ, &amp; </s>
          <s xml:space="preserve"><lb />dirigée du côté de la puiſſance Q parallelement à EO. <lb /></s>
          <s xml:space="preserve">Il eſt clair que cette nouvelle puiſſance faiſant la <lb />même impreſſion ſur ce levier que les puiſſances P &amp; </s>
          <s xml:space="preserve"><lb />Q y en faiſoient auparavant, ſon centre d’équilibre <lb />avec la puiſſance O, ſera le point lequel les trois <lb />puiſſances O, P, &amp; </s>
          <s xml:space="preserve">Q feroient équilibre, ſi elles <lb />étoient ſeules, &amp; </s>
          <s xml:space="preserve">appliquées comme elles ſont: </s>
          <s xml:space="preserve"><lb />l’ayant donc trouvé comme l’on vient de faire le point <lb />λ; </s>
          <s xml:space="preserve">c’eſt-à-dire, ayant fait λF à FE, comme la puiſ-<lb />ſance O, à la charge qui réſulte au point λ du concours <lb />d’action des puiſſances P &amp; </s>
          <s xml:space="preserve">Q; </s>
          <s xml:space="preserve">on aura le point F <lb />dont la direction ſera encore (Cor. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">parallele à celle <lb />de ces puiſſances, &amp; </s>
          <s xml:space="preserve">du côté de Q; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">la charge en <lb />ſera égale (Cor. </s>
          <s xml:space="preserve">7. </s>
          <s xml:space="preserve">ſig. </s>
          <s xml:space="preserve">53.) </s>
          <s xml:space="preserve">à la ſomme de ces trois-ci <lb />O, P, &amp; </s>
          <s xml:space="preserve">Q; </s>
          <s xml:space="preserve">ou (ſig. </s>
          <s xml:space="preserve">54.) </s>
          <s xml:space="preserve">à la ſomme de la puiſſance <lb />O, &amp; </s>
          <s xml:space="preserve">de la diſſérence qui eſt entre les puiſſances P &amp; </s>
          <s xml:space="preserve"><lb />Q; </s>
          <s xml:space="preserve">ou enſin (Cor. </s>
          <s xml:space="preserve">9. </s>
          <s xml:space="preserve">ſig. </s>
          <s xml:space="preserve">55.) </s>
          <s xml:space="preserve">à la diſſérence qui eſt <lb />entre la puiſſance O, &amp; </s>
          <s xml:space="preserve">la diſſèrence des puiſſances <lb />P &amp; </s>
          <s xml:space="preserve">Q: </s>
          <s xml:space="preserve">ainſi au lieu de la puiſſance O, &amp; </s>
          <s xml:space="preserve">de celle que <lb />nous avons ſuppoſée en λ, ſi nous en concevons en-
</s>
          <pb facs="0099" n="73" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
core un autre de la valeur de la charge du point F, <lb />
<ptr xml:id="note-0099-01a" corresp="note-0099-01" type="noteAnchor" />
appliquée en ce point, &amp; </s>
          <s xml:space="preserve">dirigée du côté de la puiſ-<lb />ſance Q parallelement à NC; </s>
          <s xml:space="preserve">nous trouverons ſon <lb />centre d’equilibre D avec la puiſſance N, de même <lb />que nous avons déja trouvé les points F, &amp; </s>
          <s xml:space="preserve">λ. </s>
          <s xml:space="preserve">Enſin <lb />ôtant encore la puiſſance N avec celle qui étoit appli-<lb />quée en F, &amp; </s>
          <s xml:space="preserve">mettant à leur défaut au point D une <lb />autre puiſſance égale à ſa charge, &amp; </s>
          <s xml:space="preserve">dirigée du côté <lb />de la puiſſance O parallelement à AM; </s>
          <s xml:space="preserve">on trouvera <lb />encore le centre de direction B qui lui eſt commun <lb />avec la puiſſance M, de même que l’on vient de faire <lb />les points λ, F, &amp; </s>
          <s xml:space="preserve">D; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">ce point B ſera (Cor. </s>
          <s xml:space="preserve">12.) <lb /></s>
          <s xml:space="preserve">celui ſur lequel les cinq puiſſances M, N, O, P, &amp; </s>
          <s xml:space="preserve">Q, <lb />ainſi dirigées demeureront en équilibre. </s>
          <s xml:space="preserve">Ce qu’il <lb />faloit premiérement trouver.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0098-02" corresp="note-0098-02a" place="margin">ſig. 53. <lb />54. <lb />55.</note>
              <note xml:space="preserve" xml:id="note-0099-01" corresp="note-0099-01a" place="margin">DES <lb />LEVIERS</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> I.</head>
        <p>
          <s xml:space="preserve">On voit aſſez que ſi ce levier AH, (ſig. </s>
          <s xml:space="preserve">55.)</s>
          <s xml:space="preserve">ſe fû@t <lb />terminé en H, ce Problême en ce cas auroit été im-<lb />poſſible.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> II.</head>
        <p>
          <s xml:space="preserve">Ce que nous venons de démontrer des leviers <lb />
<ptr xml:id="note-0099-02a" corresp="note-0099-02" type="noteAnchor" />
droits, ſe peut fort aiſément appliquer à toutes ſor-<lb />tes de leviers courbes; </s>
          <s xml:space="preserve">par exemple, à celui de la fig. <lb /></s>
          <s xml:space="preserve">56. </s>
          <s xml:space="preserve">en faiſant ſeulement à diſcretion quelque ligne <lb />droite ah, qui rencontre (il n’importe comment) <lb />toutes les lignes de direction des puiſſances M, N, <lb />O, P, &amp; </s>
          <s xml:space="preserve">Q, en a, c, e, h, &amp; </s>
          <s xml:space="preserve">g: </s>
          <s xml:space="preserve">car la regardant com-<lb />me un levier auquel ces puiſſances ſont appliquées <lb />en ces mêmes points, on en trouvera, comme l’on <lb />vient de faire, le point d’appui b, avec ſa ligne de <lb />direction bB, qui rencontrant le levier AH, donnera <lb />le point B qui ſera ſon point d’appui: </s>
          <s xml:space="preserve">Puis que les <lb />rapports de diſtances de ce point aux lignes de di-
</s>
          <pb facs="0100" n="74" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
rection de ces puiſſ nces, qui ſont (hyp &amp; </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">5. <lb /></s>
          <s xml:space="preserve">
<ptr xml:id="note-0100-01a" corresp="note-0100-01" type="noteAnchor" />
paralleles à b B, ſont les mêmes que ceux des diſtances <lb />du point b à ces mêmes lignes.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0099-02" corresp="note-0099-02a" place="margin">ſig. 56.</note>
              <note xml:space="preserve" xml:id="note-0100-01" corresp="note-0100-01a" place="margin">DES <lb />LEVIERS.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">Secondement, s’il ſe trouve quelques -unes des <lb />
<ptr xml:id="note-0100-02a" corresp="note-0100-02" type="noteAnchor" />
lignes de direction des puiſſances données, qui ne ſoient <lb />point paralleles entr’elles, quelles que ſoient les autres, <lb />&amp; </s>
          <s xml:space="preserve">de quelque côté que ces puiſſances tirent encore; <lb /></s>
          <s xml:space="preserve">Voici comment on pourra trouver le point d’appui <lb />du levier AH auquel elles ſont appliquées. </s>
          <s xml:space="preserve">Soient, ſi <lb />l’on veut, les directions HP &amp; </s>
          <s xml:space="preserve">GQ des puiſſan-<lb />ces P &amp; </s>
          <s xml:space="preserve">Q, non paralleles, &amp; </s>
          <s xml:space="preserve">qu’elles ſe rencon-<lb />trent en V: </s>
          <s xml:space="preserve">faite VR à VS, comme la puiſſance P à <lb />la puiſſance Q; </s>
          <s xml:space="preserve">achevez le parallelogramme RS, <lb />&amp; </s>
          <s xml:space="preserve">faite la diagonale VK qui rencontre en λ le <lb />levier AH prolongé juſqu’où il en ſera beſoin: </s>
          <s xml:space="preserve">ce <lb />point ſera (prop. </s>
          <s xml:space="preserve">ſond.) </s>
          <s xml:space="preserve">celui ſur lequel ces deux puiſ-<lb />ſances ainſi appliquées feroient équilibre, ſi elles <lb />étoient ſeules; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">ſa charge, dont la direction eſt <lb />de V vers K ſuivant VK, (Cor. </s>
          <s xml:space="preserve">4.) </s>
          <s xml:space="preserve">ſera à chacune <lb />des puiſſances P, &amp; </s>
          <s xml:space="preserve">Q, comme VK à chacune des <lb />lignes VR &amp; </s>
          <s xml:space="preserve">VS qui les répréſentent: </s>
          <s xml:space="preserve">De ſorte que <lb />ſi au lieu de ces deux puiſſances, on en appliquoit <lb />quelqu’autre au point λ de ce levier, ſuivant cette <lb />même direction VK, &amp; </s>
          <s xml:space="preserve">qui eût ce même raport à <lb />chacune d’elles, c’eſt-à-dire, qui ſût égale à la <lb />charge de ce point; </s>
          <s xml:space="preserve">elle feroit ſeule ainſi appliquée <lb />la même impreſſion ſur ce levier que font préſente-<lb />ment ces deux enſemble; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent ſon <lb />centre d’équilibre avec la puiſſance O, ſeroit celui <lb />des trois puiſſances, O, P, &amp; </s>
          <s xml:space="preserve">Q; </s>
          <s xml:space="preserve">c’eſt-à-dire, le <lb />point ſur lequel elles feroient equilibre, ſi elles <lb />étoient ſeules, &amp; </s>
          <s xml:space="preserve">ainſi appliquées. </s>
          <s xml:space="preserve">S’il arrive que <lb />VK &amp; </s>
          <s xml:space="preserve">OE ſoient paralleles, on trouvera ce point <lb />comme l’on a fait dans l’hypothêſe des directions
</s>
          <pb facs="0101" n="75" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
paralleles; </s>
          <s xml:space="preserve">mais ſi elles ſe rencontrent en quelque <lb />
<ptr xml:id="note-0101-01a" corresp="note-0101-01" type="noteAnchor" />
point T, il faut, comme l’on vient de faire, prendre <lb />TY à TZ, comme la puiſſance ſuppoſée en λ, eſt à <lb />la puiſſance O; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">ayant achevé le parallelogramme <lb />YZ, faite ſa diagonale TX qui rencontre en F le <lb />levier AH: </s>
          <s xml:space="preserve">ce point ſera encore (Prop. </s>
          <s xml:space="preserve">fond.) </s>
          <s xml:space="preserve">celui <lb />ſur lequel ces deux puiſſances, ou bien ces trois-ici O, <lb />P, &amp; </s>
          <s xml:space="preserve">Q, feroient équilibre, ſi elles étoient ſeules, &amp; </s>
          <s xml:space="preserve"><lb />appliquees ſuivant les conditions de ce Problême; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve"><lb />ſa charge, dont la direction eſt de T vers X, (Cor. </s>
          <s xml:space="preserve">4.) <lb /></s>
          <s xml:space="preserve">eſt en ce cas à la puiſſance O, comme TX à TZ: </s>
          <s xml:space="preserve">ôtant <lb />donc encore cette puiſſance avec celle que nous <lb />avions ſuppoſée en λ au lieu des puiſſances P &amp; </s>
          <s xml:space="preserve">Q; </s>
          <s xml:space="preserve"><lb />&amp; </s>
          <s xml:space="preserve">en mettant une autre en F, dirigée de T vers X <lb />ſuivant TX, &amp; </s>
          <s xml:space="preserve">qui ſoit à la puiſſance O, comme <lb />TX à TZ; </s>
          <s xml:space="preserve">elle fera encore ſeule ainſi appliquée la <lb />même impreſſion ſur le leuier AH, que lui faiſoient <lb />auparavant les trois puiſſances O, P, &amp; </s>
          <s xml:space="preserve">Q; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par <lb />conſéquent ſon centre d’équilibre avec la puiſſance <lb />N, ſera celui des quatres puiſſances N, O, P, &amp; </s>
          <s xml:space="preserve">Q. </s>
          <s xml:space="preserve"><lb />S’il arrive que TX &amp; </s>
          <s xml:space="preserve">NC ſoient paralleles, on trou-<lb />vera encore ce point comme dans la première partie <lb />de cette ſolution; </s>
          <s xml:space="preserve">mais ſi elles ſe rencontrent en quel-<lb />que point β, il faut encore prendre βγ à βε, comme <lb />la puiſſance ſuppoſée en F, eſt à la puiſſance N; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve"><lb />ayant achevé le parallelogramme εγ, il faut prolon-<lb />ger ſa diagonale βδ juſqu’à ce qu’elle rencontre le <lb />levier AH en D, &amp; </s>
          <s xml:space="preserve">ce point ſera (prop. </s>
          <s xml:space="preserve">fond.) </s>
          <s xml:space="preserve">celui <lb />ſur lequel ces deux puiſſances, ou bien ces quatre-ci <lb />N, O, P, &amp; </s>
          <s xml:space="preserve">Q, feroient équilibre, ſi elles étoient <lb />ſeules, &amp; </s>
          <s xml:space="preserve">appliquées ſuivant les directions données <lb />de ce problême. </s>
          <s xml:space="preserve">La direction de ce point ſera encore <lb />de β vers δ ſuivant βδ, (Cor. </s>
          <s xml:space="preserve">4.) </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">ſa charge ſera <lb />auſſi à la puiſſance N, comme βδ à βε: </s>
          <s xml:space="preserve">ainſi au lieu <lb />de la puiſſance N, &amp; </s>
          <s xml:space="preserve">de celle que nous venons de
</s>
          <pb facs="0102" n="76" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
ſuppoſer en F, ſi l’on en ſuppoſe encore quelqu’autre <lb />
<ptr xml:id="note-0102-01a" corresp="note-0102-01" type="noteAnchor" />
en D, dirigée de β vers δ ſuivant βδ, &amp; </s>
          <s xml:space="preserve">qui ſoit à la <lb />puiſſance N, comme βδ à βε; </s>
          <s xml:space="preserve">cette nouvelle puiſ-<lb />ſance ainſi appliquée au levier AH, fera encore <lb />feule ſur lui la même impreſſion que faiſoient aupa-<lb />ravant les quatre puiſſances N, O, P, &amp; </s>
          <s xml:space="preserve">Q; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par <lb />conſéquent ſon centre d’équilibre avec la puiſſance <lb />M, ſera celui des cinq puiſſances données dans ce <lb />problême. </s>
          <s xml:space="preserve">S’il arrive que βδ ſoit parallele à AM, on <lb />trouvera encore ce point comme l’'on a fait dans le cas <lb />des directions paralleles; </s>
          <s xml:space="preserve">mais ſi elles ſe rencontrent <lb />en quelque point L, il faut encore prendre L θ à Lω, <lb />comme la puiſſance qu’on ſuppoſe en D, eſt à la puiſ-<lb />ſance M; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">ayant achevé le parallelogramme ωθ, il <lb />faut tirer la diagonale LI, qui rencontrant le levier <lb />AH, donnera le point B pour centre d’equilibre <lb />(Prop. </s>
          <s xml:space="preserve">fond.) </s>
          <s xml:space="preserve">de ces deux puiſſances; </s>
          <s xml:space="preserve">c’eſt-à-dire en <lb />remettant à la place de celle qu’on ſuppoſe en D, les <lb />quatre N, O, P, &amp; </s>
          <s xml:space="preserve">Q, qu’elle ſuppléoit; </s>
          <s xml:space="preserve">ſur lequel <lb />les cinq puiſſances données, &amp; </s>
          <s xml:space="preserve">appliquées ſuivant <lb />les conditions de ce Problême, feront équilibre. </s>
          <s xml:space="preserve">Ce <lb />qu’il faloit encore trouver.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0100-02" corresp="note-0100-02a" place="margin">ſig 57. <lb />58. <lb />59.</note>
              <note xml:space="preserve" xml:id="note-0101-01" corresp="note-0101-01a" place="margin">DES <lb />LEVIERS.</note>
              <note xml:space="preserve" xml:id="note-0102-01" corresp="note-0102-01a" place="margin">DES <lb />LEVIERS.</note>
            </div>
          </body>
        </floatingText>
        <p rend="italics">
          <s xml:space="preserve">Ce Problème, tout facile qu’il paroit à réſoudre par les <lb />principes q@’on ſuit ici, eſt peut - é<unclear reason="illegible" />tre un des plus diſſiciles <lb />qu’on puiſſe propoſer à ceux qui ſont dans les principes ordi-<lb />naires; </s>
          <s xml:space="preserve">non ſeulement quant à la maniére de déterminer les <lb />points d’appui des levi<unclear reason="illegible" />ers pour toutes les directions poſſibles <lb />des puiſſances, ou des poids qui y ſont appliquez; </s>
          <s xml:space="preserve">mais auſſi <lb />quant à celle de reconnoitre leur direction, &amp; </s>
          <s xml:space="preserve">leur charge, <lb />de quelque eſpece, &amp; </s>
          <s xml:space="preserve">dans quelque ſituation qu’ils ſoient: <lb /></s>
          <s xml:space="preserve">C’eſt peut ètre auſſi ce qui a fait que les Mécbaniciens, qui <lb />ont entrepris de démontrer le cas de la figu<unclear reason="illegible" />re 53. </s>
          <s xml:space="preserve">n’ont oſé tou-<lb />ch@r aux autres.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0103" n="77" />
        <fw type="head">MECHANIQUE.</fw>
        <p rend="italics">
          <s xml:space="preserve">Outre les Poulies, les Surfaces, &amp; </s>
          <s xml:space="preserve">les Leviers, on met <lb />
<ptr xml:id="note-0103-01a" corresp="note-0103-01" type="noteAnchor" />
encore la Vis au rang des machines qu’on regarde comme <lb />capitales entre celles qui ſont propres à faciliter les mouve-<lb />mens; </s>
          <s xml:space="preserve">mais parce que cette dernière ſe rapporte toute au plan <lb />incliné &amp; </s>
          <s xml:space="preserve">au levier, dont on va voir qu’elle eſt compoſée, <lb />nous n’en dirons ici que tres@ peu de choſes.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0103-01" corresp="note-0103-01a" place="margin">DES <lb />LEVIERS.</note>
            </div>
          </body>
        </floatingText>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0103-01" />
          <label>0103-01</label>
        </figure>
        <pb facs="0104" n="78" />
        <fw type="head">NOUVELLE</fw>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0104-01" />
          <label>0104-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">DE LA VIS <lb />REMARQUES. <lb />I.</head>
        <p>
          <s xml:space="preserve">ON voit aſſez que tout l’uſage de la Vis eſt de <lb />tirer, ou de repouſſer ſuivantla direction de ſon <lb />axe tout ce qui lui fait quelque réſiſtance; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">ſi elle <lb />eſtſixe, la force, ou le corps contre lequel on s’en ſert, <lb />doit tirer, ou preſſer ſon écrouë du côté diametra-<lb />lement oppoſé à celui vers lequel il eſt forcé d’avan-<lb />cer. </s>
          <s xml:space="preserve">Au contraire ſi c’eſt l’écrouë qui ſoit ſixe, cette <lb />force, où ce corps doit tirer, ou preſſer la vis elle-<lb />même de ce même côté.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve">II.</head>
        <p>
          <s xml:space="preserve">De ſorte, que dans l’uſage de la vis, lors qu’elle <lb />eſt ſixe, l’on doit regarder tous les points de ſon <lb />écrouë, comme tirez ou preſſez parallelement à ſon <lb />axe du côté que cette écrouë eſt preſſée, ou tirée par <lb />la force, ou par le poids dont elle eſt chargée.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve">III.</head>
        <p>
          <s xml:space="preserve">D’où l’on voit que les lignes de direction de tous <lb />ces points, ſont toutes obliques à celui des pas de <lb />cette vis ſur lequel ceux de ces points qui le tou-<lb />chent, s’appuyent; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent (démonſt. </s>
          <s xml:space="preserve">des
</s>
          <pb facs="0105" n="79" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
ſurf. </s>
          <s xml:space="preserve">n. </s>
          <s xml:space="preserve">3.) </s>
          <s xml:space="preserve">ſi cette vis, &amp; </s>
          <s xml:space="preserve">ſon écrouë étoient Mathé-<lb />
<ptr xml:id="note-0105-01a" corresp="note-0105-01" type="noteAnchor" />
matiquement juſtes, chacun d’eux tendroit à couler <lb />du côté que ſa ligne de direction s’écarteroit de la <lb />perpendiculaire tirée de lui à ce pas; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">parce que <lb />cet écartement ſe feroit pour tous du même côté, à <lb />cauſe du paralleliſme de toutes ces lignes, &amp; </s>
          <s xml:space="preserve">de la <lb />pente uniforme du cordon de cette vis dans toute <lb />ſa longueur: </s>
          <s xml:space="preserve">Il ſuit évidemment que tous ces points <lb />devroient s’accorder dans un même mouvement qui <lb />emportât cette écrouë ſuivant le fil de ce cordon, <lb />c’eſt-à-dire, en tournoyant du côté de cet écartement; <lb /></s>
          <s xml:space="preserve">ſi dans ſon frotement avec la vis, l’inégalité de leurs <lb />parties ne les acrochoient point enſemble.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0105-01" corresp="note-0105-01a" place="margin">DELA VIS.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve">IV.</head>
        <p>
          <s xml:space="preserve">La même choſe ſe doit entendre de tous les points <lb />de la vis, ſi c’eſt l’écrouë qui ſoit fixe.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve">V.</head>
        <p>
          <s xml:space="preserve">Ainſi à regarder l’une &amp; </s>
          <s xml:space="preserve">l’autre dans une juſteſſe <lb />Mathématique, il faut néceſſairement quelque force <lb />pour retenir celle des deux qui eſt mobile, contre <lb />l’impreſſion de la force, ou du poids qui la charge. <lb /></s>
          <s xml:space="preserve">La voici.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0105-01" />
          <label>0105-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">PROPOSITION <lb />DE LA VIS.</head>
        <p rend="italics">
          <s xml:space="preserve">LOrſqu’une puiſſance ſoutient quelque poids, ou l’action <lb />de quelque autre force à l’aide d’une vis, ſoit que<unclear reason="illegible" /> <lb />cette vis ſoit fixe, ou que ce ſoit ſon écrouë cette puiſſance
</s>
          <pb facs="0106" n="80" />
          <s xml:space="preserve"><fw type="head">NOUVELLE</fw>
eſt toujours à ce poids, ou a cette force, quelle qu’elle ſoit, <lb />
<ptr xml:id="note-0106-01a" corresp="note-0106-01" type="noteAnchor" />
comme la diſtance qui eſt entre deux des pas de cette vis, à <lb />la circonfèrence a’un cercle, dont le rayon eſt égal à la diſtance <lb />qui eſt entre cette puiſſance &amp; </s>
          <s xml:space="preserve">l’axe de cette mème vis.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0106-01" corresp="note-0106-01a" place="margin">DELAVIS</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration</hi>.</head>
        <p>
          <s xml:space="preserve">Premiérement ſi la vis VXYZ eſt fixe, concevons que <lb />
<ptr xml:id="note-0106-02a" corresp="note-0106-02" type="noteAnchor" />
le point A de ſon écrouë PQ ſoit retenu ſur un de ſes <lb />pas GH par quelque puiſſance R dont la direction AB <lb />ſoit dans le plan de cette écrouë, &amp; </s>
          <s xml:space="preserve">perpendiculaire à <lb />EP qui y eſt auſſi, &amp; </s>
          <s xml:space="preserve">qui paſſe par le point A. </s>
          <s xml:space="preserve">Il eſt clair <lb />que cette puiſſance retenant par ce moyen toute l’é-<lb />crouë PQ, ce point A fait ſur elle la même impreſſion <lb />que s’il ſoutenoit lui ſeul toute l’action du poids, ou de <lb />la force, quelle qu’elle ſoit, qui pouſſe cette écrouë, <lb />ou qui la tire (Remarq. </s>
          <s xml:space="preserve">1.) </s>
          <s xml:space="preserve">vers ZY parallelement à <lb />l’axe MS de cette vis: </s>
          <s xml:space="preserve">Ainſi l’on peut regarder le <lb />point A de cette écrouë, comme ayant lui ſeul ſuivant <lb />AC perpendiculaire au plan de cette écrouë, &amp; </s>
          <s xml:space="preserve">pa-<lb />rallele à MS, toute l’impreſſion qu’elle reçoit de ſa <lb />charge; </s>
          <s xml:space="preserve">de ſorte que ſi l’on fait AD perpendiculaire <lb />au pas GH de cette vis, &amp; </s>
          <s xml:space="preserve">que de quelque point D <lb />de cette ligne, l’on acheve le parallelogramme BC, <lb />on verra (prop. </s>
          <s xml:space="preserve">fond. </s>
          <s xml:space="preserve">des ſurf.) </s>
          <s xml:space="preserve">que la puiſſance R ſera à <lb />la charge de l’écrouë PQ, comme AB, à AC, ou à BD <lb />qui lui eſt égale; </s>
          <s xml:space="preserve">c’eſt-à-dire, à cauſe que le triangle <lb />HFG roulé ſur la vis VXYZ, eſt ſemblable au <lb />triangle ABD; </s>
          <s xml:space="preserve">comme HF au demi tour FG de cette <lb />vis, ou comme 2HF, c’eſt-à-dire, HK à un tour <lb />entier. </s>
          <s xml:space="preserve">Or regardant EAP comme un levier dont <lb />l’appui eſt le point E de l’axe MS de cette vis, &amp; </s>
          <s xml:space="preserve">qui <lb />ſe trouve dans le plan de ſon écrouë; </s>
          <s xml:space="preserve">la puiſſance P, <lb />dont la direction eſt auſſi dans ce même plan, &amp; </s>
          <s xml:space="preserve">per-<lb />pendiculaire à EP, &amp; </s>
          <s xml:space="preserve">conſéquemment parallele à AB,
</s>
          <pb facs="0107" n="81" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
ſoutenant ainſi (Hyp.) </s>
          <s xml:space="preserve">le point A, ou la charge de <lb />
<ptr xml:id="note-0107-01a" corresp="note-0107-01" type="noteAnchor" />
l’écrouë PQ au lieu de la puiſſance R, eſt à cette der-<lb />niére puiſſance, (Lemm 6. </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">2.) </s>
          <s xml:space="preserve">comme EA à EP, <lb />ou comme le tour entier de cette vis à la circonfé-<lb />rence d’un cercle dont le rayon ſoit EP: </s>
          <s xml:space="preserve">Ainſi en <lb />multipliant par ordre ces deux rangées de proportio-<lb />nelles, l’on aura la puiſſance P à la charge de l’écrouë <lb />PQ, comme la diſtance HK qui eſt entre deux des <lb />pas de cette vis, à la circonference d’un cercle dont <lb />le rayon eſt égal à la diſtance EP qui eſt entre cette <lb />fance &amp; </s>
          <s xml:space="preserve">l’axe de cette même vis.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0106-02" corresp="note-0106-02a" place="margin">ſig. 60.</note>
              <note xml:space="preserve" xml:id="note-0107-01" corresp="note-0107-01a" place="margin">DELA VIS.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">Secondement, ſi c’eſt l’écrouë PQ qui ſoit fixe, <lb />concevons que le point A appartient à la vis VXYZ, &amp; </s>
          <s xml:space="preserve"><lb />qu’il eſt retenu ſur le pas de cette écrouë par quelque <lb />puiſſance R dont la direction ſoit encore ſuivant AB <lb />qu’on ſuppoſe dans le plan de cetteécrouë, &amp; </s>
          <s xml:space="preserve">perpen-<lb />diculaire à EP qui y eſt auſſi. </s>
          <s xml:space="preserve">Il eſt encore clair que <lb />cette puiſſance retenant par ce moyen toute la vis <lb />VXYZ, ce point A fait encore ſur elle la même <lb />impreſſion ſuivant AC parallele à MS, que s’il ſou-<lb />tenoit, lui ſeul, toute l’action de ce qui pouſſe, (re-<lb />marq. </s>
          <s xml:space="preserve">1.) </s>
          <s xml:space="preserve">ou de ce qui tire cette vis vers ZY: </s>
          <s xml:space="preserve">ainſi pour <lb />la même raiſon que ci-deſſus, la puiſſance R ſera <lb />encore à la charge de cette vis, comme AB à BD; <lb /></s>
          <s xml:space="preserve">c’eſt-à-dire, comme HF à FG, ou bien comme HK <lb />au circuit de cette vis; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">la puiſſance T, qui au lieu de <lb />la puiſſance R retient cette vis, eſt auſſi à cette dernié-<lb />re puiſſance, (Lemm. </s>
          <s xml:space="preserve">6. </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">2.) </s>
          <s xml:space="preserve">comme EA à ST, ou <lb />comme un tour entier de cette vis à la circonférence <lb />d’un cercle dont ST ſoit le rayon: </s>
          <s xml:space="preserve">ainſi en multi-<lb />pliant encore par ordre ces deux rangées de propor-<lb />tionnelles, on aura encore la puiſſance T à la charge <lb />de cette vis, comme la diſtance qui eſt entre deux de <lb />ſes pas, à la circonférence d’un cercle dont le rayon eſt <lb />égal à la diſtance qui eſt entre cette puiſſance &amp; </s>
          <s xml:space="preserve">l’axe de <lb />cette même vis.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0108" n="82" />
        <fw type="head">NOUVELLE</fw>
        <p>
          <s xml:space="preserve">Donc lors qu’une puiſſance ſoutient un poids, ou <lb />
<ptr xml:id="note-0108-01a" corresp="note-0108-01" type="noteAnchor" />
l’action de quelqu’autre force que ce ſoit, à l’aide <lb />d’une vis, ſoit que cette vis ſoit fixe, ou que ce ſoit <lb />ſon écrouë, cette puiſſance eſt toujours à ce poids, ou <lb />à cette force, commela diſtance qui eſt entre deux des <lb />pas de cette vis, à la circonférence d’un cercle, dont <lb />le rayon eſt égal à la diſtance qui eſt entre cette puiſ-<lb />ſance &amp; </s>
          <s xml:space="preserve">l’axe de cette même vis. </s>
          <s xml:space="preserve">Ce qu’il faloit dé-<lb />montrer.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0108-01" corresp="note-0108-01a" place="margin">DE LA VIS.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> I.</head>
        <p>
          <s xml:space="preserve">D’où l’on voit que pour peu que la raiſon d’une <lb />puiſſance à un poids, ou à quelqu’autre force, ſur-<lb />paſſe celle de la diſtance, qui eſt entre deux des pas <lb />d’une vis, à la circonférence d’un cercle, dont le <lb />rayon ſoit la diſtance de l’axe de cette vis à cette <lb />puiſſance, elle pourra ainſi appliquée ſurmonter ce <lb />poids, ou cette force à l’aide de cette vis, &amp; </s>
          <s xml:space="preserve">elle le <lb />fera dautant plus aiſément que cette raiſon ſera plus <lb />grande.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">L’obſtacle que le frotement de la vis avec ſon écrouë <lb />fait à ce mouvement, doit être compté comme faiſant partie <lb />de ſa charge: </s>
          <s xml:space="preserve">c’eſt ainſi qu’on la peut réduire à une juſteſſe <lb />Mathématique, de meme que toute autre machine.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> II.</head>
        <p>
          <s xml:space="preserve">D’où il ſuit que plus les pas d’une vis ſont ſerrez, <lb />&amp; </s>
          <s xml:space="preserve">que la diſtance de ſon axe à la puiſſance qui y eſt <lb />appliquée, eſt grande, plus il eſt facile à cette puiſ-<lb />ſance de ſurmonter le poids, ou la force qui agit <lb />contr’elle.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> III.</head>
        <p>
          <s xml:space="preserve">Il ſuit encore de cette propoſition qu’une même
</s>
          <pb facs="0109" n="83" />
          <s xml:space="preserve"><fw type="head">MECHANIQUE.</fw>
puiſſance peut également mouvoir un même poids, <lb />
<ptr xml:id="note-0109-01a" corresp="note-0109-01" type="noteAnchor" />
ou ſurmonter une même force, à l’aide d’une même <lb />vis, ſoit qu’on la ſuppoſe appliquée à cette vis, où <lb />qu’elle le ſoit à ſon écrouë pourvû qu’elle ſoit éga-<lb />lement diſtante de ſon axe dans l’un &amp; </s>
          <s xml:space="preserve">l’autre cas.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0109-01" corresp="note-0109-01a" place="margin">DELA VIS.</note>
            </div>
          </body>
        </floatingText>
        <p rend="italics">
          <s xml:space="preserve">On ne dit rien ici du Coin, de la Scie, du Mortier, &amp;</s>
          <s xml:space="preserve">c. <lb /></s>
          <s xml:space="preserve">ce ſont plûtôt des inſtrumens, ou des outils propres à faciliter <lb />la diviſion d’un corps, que des machines qui puiſſent en fa-<lb />ciliter le mouvement; </s>
          <s xml:space="preserve">on aura peut-ê<unclear reason="illegible" />tre un jour occaſion d’en <lb />parler.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0110" />
        <pb facs="0111" />
      </div>
      <div type="section">
        <head xml:space="preserve">EXAMEN <lb />DE L’OPINION <lb />DE M BORELLI <lb />SUR LES PROPRIETEZ DES POIDS <lb />ſuſpendus par des cordes.</head>
        <pb facs="0112" />
        <pb facs="0113" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0113-01" />
          <label>0113-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">AVERTISSEMENT.</head>
        <p rend="italics">
          <s xml:space="preserve">C’EST ici l’éxamen promis dans la réfléxion qui <lb />ſuit la preuve de la premiére propoſition du Trojet <lb />précédent. </s>
          <s xml:space="preserve">On ne croyoit pas d’abord le pouvoir donner <lb />ici; </s>
          <s xml:space="preserve">mais s’étant trouvé fait plûtôt qu’on ne s’y étoit <lb />attendu, on le joint à ce projet. </s>
          <s xml:space="preserve">On a été naturelle-<lb />ment conduit par les principes qu’on y ſuit, à une <lb />propoſition ſur les proprietez des poids ſuſpendus par <lb />des cordes, qui s’eſt trouvée la meſme que celle que <lb />Monſieur Borelli avoit critiquée dans Stévin, <lb />&amp; </s>
          <s xml:space="preserve">dans Hérigone; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">ç’a été par la neceſſité de <lb />la juſtiſier qu’on s’eſt trouvé engagé à l’examen de ſa <lb />critique.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">On diviſe cet examen en deux Cbapitres: </s>
          <s xml:space="preserve">dans le <lb />premier on fait voir que le ſentiment que M. <lb /></s>
          <s xml:space="preserve">Borelli reprend dans H’erigone, dans Stévin, &amp; </s>
          <s xml:space="preserve">dans <lb />les autres; </s>
          <s xml:space="preserve">bien loin d’ètre contraire, comme il l’a <lb />crû, à la 68. </s>
          <s xml:space="preserve">propoſition du Tome premier de ſon traité <lb />du mouvement des Animaux, en eſt une ſuite ſi né-<lb />ceſſaire, que s’il eut fait encore quelques pas, il y ſeroit <lb />infailliblement entré. </s>
          <s xml:space="preserve">On indique enſuite dans ce <lb />meſme Chapitre quelques paralogiſmes que cet Au-<lb />theur a commis, lors meſme qu’il croyoit en voir dans <lb />les raiſonnemens qu’il a critiquez.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0114" />
        <fw type="head">AVERTISSEMENT.</fw>
        <p rend="italics">
          <s xml:space="preserve">Dans le ſecond Cbapitre, apres avoir encore donné <lb />quelques démonſtrations du ſentiment d’Hèrigone &amp; </s>
          <s xml:space="preserve"><lb />des autres, toutes différentes de celles que M. </s>
          <s xml:space="preserve">Borelli <lb />a critiqu@es; </s>
          <s xml:space="preserve">on rend par la metbode du Projet <lb />précedent les Lemmes ſur leſquels cet Au beur a fondé <lb />tout ce qu’il a dit de la force des Muſcles, beaucoup <lb />plus généraux qu’ils ne le peuvent eſtre par la ſienne.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">Au reſte ſi l’on attaque une erreur ou M. <lb /></s>
          <s xml:space="preserve">Borelli eſt tombé, on n’en eſt pas moins perſuadé <lb />du mérite ex@raordinaire de ce grand bomme, dont <lb />les principaux Ouvrages doivent eſtre mis au nombre <lb />des Livres les plus originaux qui ayent paru dans ce <lb />ſiecle-ci; </s>
          <s xml:space="preserve">mais il n’y a perſonne qui ne puiſſe faire un <lb />fauxpas, ſur tout dans des matieres auſſi delicates que <lb />celles-ci, &amp; </s>
          <s xml:space="preserve">où le paralogiſme ſe gliſſe auſſi facile-<lb />ment.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">Tout ce qu’on citera de cet Auteur dans cet exa-<lb />men, ſera pris du Tome premier de ſon Traité du mou-<lb />vement des Animaux, de l’édition de Rome, faite en <lb />1680. </s>
          <s xml:space="preserve">On ſpécifie l’édition à cauſe des pages qu’on en <lb />citera quelques fois.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0115" n="89" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0115-01" />
          <label>0115-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">EXAMEN <lb />DE L’OPINION <lb />DE M. BORELLI <lb />Sur les propriétez des Poids ſuſpendus <lb />par des cordes.</head>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0115-02" />
          <label>0115-02</label>
        </figure>
      </div>
      <div type="section">
        <head rend="italics" xml:space="preserve">ET AT DE LA QUESTION.</head>
        <p>
          <s xml:space="preserve"><hi rend="small caps">MOnsieur</hi> <hi rend="small caps">Borelli</hi> dans ſon Traité du <lb />mouvement des Animaux Tome 1. </s>
          <s xml:space="preserve">Chapi-<lb />tre 13. </s>
          <s xml:space="preserve">a fait une fort longue digreſſion pour prou-<lb />ver que Hérigone, Stévin, &amp; </s>
          <s xml:space="preserve">pluſieurs autres ſe <lb />ſont trompez d’avoir avancé comme propoſition gé-<lb />nérale que le poids T ſoutenu avec les cordes obliques AC <lb />
<ptr xml:id="note-0115-01a" corresp="note-0115-01" type="noteAnchor" />
&amp; </s>
          <s xml:space="preserve">BC par deux poids, ou deux puiſſances R &amp; </s>
          <s xml:space="preserve">S; </s>
          <s xml:space="preserve">eſt à chacun
</s>
          <pb facs="0116" n="90" />
          <s xml:space="preserve"><fw type="head">EXAMEN DE L’OPINION</fw>
d’eux, ou d’elles, comme la partie HC de ſa ligne de di-<lb />
<ptr xml:id="note-0116-01a" corresp="note-0116-01" type="noteAnchor" />
rection à chacun des côtez CN &amp; </s>
          <s xml:space="preserve">MC du parallelogramme <lb />MN, dont elle eſt diagonale. </s>
          <s xml:space="preserve">Cet Autheur dit (pag. <lb /></s>
          <s xml:space="preserve">” 137.) </s>
          <s xml:space="preserve">que cette propoſition priſe dans toute ſon <lb />étenduë &amp; </s>
          <s xml:space="preserve">ſans reſtriction, lui paroît ſuſpecte <lb />pour bien des raiſons; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">même qu’il la croit capa-<lb />ble de jetter dans l’erreur.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0115-01" corresp="note-0115-01a" place="margin">ſig. @@</note>
              <note xml:space="preserve" xml:id="note-0116-01" corresp="note-0116-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">Il réduit toutes ces prétenduës raiſons à trois: <lb /></s>
          <s xml:space="preserve">1°. </s>
          <s xml:space="preserve">il dit (pag. </s>
          <s xml:space="preserve">138.) </s>
          <s xml:space="preserve">avoir démontré dans le ſcholie <lb />” de la 68. </s>
          <s xml:space="preserve">propoſition du Tome 1. </s>
          <s xml:space="preserve">de ce traité, que <lb />les deux puiſſances R &amp; </s>
          <s xml:space="preserve">S appliquées au poids T <lb />ſuivant des direction obliques, peuvent demeurer <lb />en équilibre avec lui, non ſeulement quelque <lb />raport qu’elles ayent entr’elles, fût-il plus grand, <lb />ou moindre que celui de NC à CM, mais encore de <lb />quelque maniére que le raport de la ſomme de ces <lb />deux puiſſances à ce poids, fût différent de celui <lb />de la ſomme de NC &amp; </s>
          <s xml:space="preserve">MC à CH. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">il a fait, dit-<lb />il, auſſi pluſieurs expériences qui lui paroiſſent <lb />confirmer ce ſentiment. </s>
          <s xml:space="preserve">3°. </s>
          <s xml:space="preserve">Enfin il a crû voir du <lb />paralogiſme dans deux démonſtrations qu’il a criti-<lb />quées, dont la premiére paroît être du P.</s>
          <s xml:space="preserve">Pardie, &amp; </s>
          <s xml:space="preserve">l’au-<lb />tre commune au reſte des Autheurs qu’il attaque.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">Il eſt conſtant que de toutes ces raiſons la premiére <lb />eſt non ſeulement la principale, mais encore l’unique <lb />qui puiſſe ſervir à la deciſion de ce différent: </s>
          <s xml:space="preserve">Car 1°. </s>
          <s xml:space="preserve">en <lb />fait d’exactitude &amp; </s>
          <s xml:space="preserve">de préciſion, l’expérience ne <lb />prouve rien; </s>
          <s xml:space="preserve">ſur tout ici, ou la réſiſtance qui vient <lb />du frotement des poulies avec leurs pivots, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">rend <lb />ces ſortes d’expériences poſſibles en tant de manieres <lb />différentes, qu’il n’y a preſque point de ſentiment <lb />pour, ou contre lequel on n’en puiſſe faire à ſon gré. <lb /></s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Qu’il y ait, ou qu’il n’y ait point de paralogiſme
</s>
          <pb facs="0117" n="91" />
          <s xml:space="preserve"><fw type="head">DE M. BORELLI.</fw>
dans les raiſonnemens qué cet Autheur critique, on <lb />
<ptr xml:id="note-0117-01a" corresp="note-0117-01" type="noteAnchor" />
n’en peut rien conclure non plus contre le ſentiment <lb />qu’il attaque; </s>
          <s xml:space="preserve">puiſque la vérité ne dépend point du <lb />tout de la maniere dont on la démontre.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0117-01" corresp="note-0117-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſe@-<lb />lemen@.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">Toute la queſtion préſente ſe réduit donc à ſça-<lb />voir ſi en effet M. </s>
          <s xml:space="preserve">Borelli a démontré dans le <lb />ſcholie de ſa 6 8. </s>
          <s xml:space="preserve">Propoſition Tome 1. </s>
          <s xml:space="preserve">que les “ <lb />deux puiſſances R &amp; </s>
          <s xml:space="preserve">S appliquées au poids T <lb />ſuivant des directions obliques, peuvent demeu-<lb />rer en équilibre avec lui, non ſeulement quelque <lb />raport qu’elles ayent entr’elles, fût-il plus grand, <lb />ou moindre que celui de NC à CM; </s>
          <s xml:space="preserve">mais encore <lb />de quelque maniére que le raport de la ſomme de <lb />ces deux puiſſances à ce poids, fût différent de <lb />celui de la ſomme de NC &amp; </s>
          <s xml:space="preserve">MC à CH. </s>
          <s xml:space="preserve">Que dî-je? <lb /></s>
          <s xml:space="preserve">Ce ſeroit aſſez pour détruire la propoſition qu’il <lb />rejette, s’il avoit ſeulement démontré un cas ou ce <lb />poids pût ainſi demeurer en équilibré avec ces puiſ-<lb />ſances, ſans être à chacune d’elles, comme la partie <lb />CH de ſa ligne de direction, qui fait la diagonale du <lb />parallelogramme MN, à chacune des parties de leurs <lb />cordes, qui lui ſervent de côtez. </s>
          <s xml:space="preserve">Mais bien loin de <lb />l’avoir fait, la propoſition d’où il tire le ſcholie en <lb />queſtion, prouve tout le contraire, je veux dire, le <lb />ſentiment d’où il a crû qu’elle le devoit cloigner.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">C’eſt ce qu’on va faire voir dans le premier <lb />Chapitre de cet Examen; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">dans le ſecond, aprés <lb />avoir encore donné quelques démonſtrations de ce <lb />même ſentiment, toutes différentes de celles que <lb />M. </s>
          <s xml:space="preserve">Borelli a critiquées, on rendra par la méthode <lb />du Projet précédent les Lemmes qu’il a déduits de ſa <lb />68. </s>
          <s xml:space="preserve">propoſition, beaucoup plus généraux qu’ils ne le <lb />peuvent être par la ſienne.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0118" n="92" />
        <fw type="head">EXAMEN DE L’OPINION</fw>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0118-01" />
          <label>0118-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">CHAPITRE I. <lb />SENTIMENT D’HERIGONE, <lb />DE STEVIN, &amp;c. <lb />SUR LES PROPRIETEZ DES POIDS <lb />ſuſpendus par des cordes, <lb />Démontré par la propoſition même que M. BORELLI <lb />avoit cru leur être contraire.</head>
        <p>
          <s xml:space="preserve">LE ſcholie de la 68. </s>
          <s xml:space="preserve">propoſition de M. </s>
          <s xml:space="preserve">Borel-<lb />li, dont il eſt ici queſtion, porte ” 1°. </s>
          <s xml:space="preserve">Qu’a-<lb />” vec les mêmes inclinaiſons de cordes, le poids qui <lb />y eſt ſuſpendu, &amp; </s>
          <s xml:space="preserve">les forces qui le ſoutiennent, <lb />peuvent varier en mille manieres différentes ſans <lb />
<ptr xml:id="note-0118-01a" corresp="note-0118-01" type="noteAnchor" />
que pour cela il ceſſe de faire équilibre avec elles; <lb /></s>
          <s xml:space="preserve">pourvû que la puiſſance R ſoit à la partie X de ce poids, <lb />comme GC à GF, ou comme AC à CH; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">que <lb />la puiſſance S ſoit à ſon autre partie Z, comme IC à <lb />IK, ou comme BC à CH.</s>
          <s xml:space="preserve">..</s>
          <s xml:space="preserve">..</s>
          <s xml:space="preserve">..</s>
          <s xml:space="preserve">. 2° Ce même ſcholie <lb />porte réciproquement qu’en retenant les mêmes <lb />poids; </s>
          <s xml:space="preserve">c’eſt - à - dire ici, les mêmes forces, (pourvû que <lb />celui du milieu ſoit moindre que les deux extrê-<lb />mes) on peut changer l’inclinaiſon de leurs cordes <lb />ſans en rompre l’équilibre.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0118-01" corresp="note-0118-01a" place="margin">ſig. 1.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">Il eſt clair que la premiére partie de ce ſcholie <lb />peut avoir deux ſens bien différens. </s>
          <s xml:space="preserve">1°. </s>
          <s xml:space="preserve">Elle peut <lb />ſignifier que dans cette variation de poids &amp; </s>
          <s xml:space="preserve">de
</s>
          <pb facs="0119" n="93" />
          <s xml:space="preserve"><fw type="head">DE M. BORELLI.</fw>
forces, ou cet Autheur veut que l’équilibre ſe con-<lb />
<ptr xml:id="note-0119-01a" corresp="note-0119-01" type="noteAnchor" />
ſerve ſans changer l’inclinaiſon de leurs cordes, ce <lb />poids demeure toujours à chacune de ces puiſſances <lb />en même raiſon que la diagonale CH du parallelo-<lb />gramme MN, à chaque partie de leurs cordes, qui <lb />lui ſert de côté; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">en cela on va voir que cette conſé-<lb />quence eſt parfaitement juſte, mais auſſi (Cor. </s>
          <s xml:space="preserve">12. <lb /></s>
          <s xml:space="preserve">de la Prop. </s>
          <s xml:space="preserve">fond. </s>
          <s xml:space="preserve">des poids ſuſpendus par des cordes, du <lb />Proiet précéd.) </s>
          <s xml:space="preserve">parfaitement conforme au ſentiment <lb />que cet Autheur attaque. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Au contraire, ſi on lui <lb />fait ſigniſier que cet équilibre puiſſe ſubſiſter ſans un <lb />tel raport; </s>
          <s xml:space="preserve">alors on conclud tres-mal, &amp; </s>
          <s xml:space="preserve">même au-<lb />tant contre cet Autheur que contre Hérigone, <lb />&amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">J’en dis tout autant de la ſeconde partie de <lb />ce même ſcholie; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">pour le démontrer, je vais <lb />faire voir que la propoſition d’où M. </s>
          <s xml:space="preserve">Borelli le <lb />tire, prouve tout le contraire, &amp; </s>
          <s xml:space="preserve">que s’il y eût <lb />fait un peu plus d’attention, elle l’auroit infaillible-<lb />ment conduit au ſentiment d’où il a crû qu’elle le <lb />devoit éloigner; </s>
          <s xml:space="preserve">je veux dire, à croire (du moins <lb />pour tous les cas qu’elle comprend) que le poids T <lb />ſoutenu avec les cordes obliques AC &amp; </s>
          <s xml:space="preserve">BC par deux poids, <lb />ou deux puiſſances R &amp; </s>
          <s xml:space="preserve">S, eſt toujours à chacun d’eux, ou <lb />d’elles, comme la partie HC de ſa ligne de direction, à cbacun <lb />descôtez CN &amp; </s>
          <s xml:space="preserve">MC du parallelogramme MN, dont elle <lb />eſt diagonale. </s>
          <s xml:space="preserve">Voici comment.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0119-01" corresp="note-0119-01a" place="margin">DES POIDS <lb />ſoutenus avcc <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">Selon cet Autheur (Prop. </s>
          <s xml:space="preserve">68) lorſque les puiſ-<lb />ſances R &amp; </s>
          <s xml:space="preserve">S ſoutiennent enſemble le poids T, la <lb />puiſſance R ſoutient pour ſa part une partie X de ce <lb />poids, de même qu’elle feroit, ſi elle étoit appliquée <lb />ſuivant ſa même direction AC avec cette partie X au <lb />levier horizontal CG; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">la puiſſance S ſoutient auſſi <lb />pour la ſienne l’autre partie Z de ce même poids, <lb />de même qu’elle feroit, ſi elle étoit auſſi appliquée
</s>
          <pb facs="0120" n="94" />
          <s xml:space="preserve"><fw type="head">EXAMEN DE L’OPINION</fw>
ſuivant ſa même direction CB avec cette partie Z au <lb />
<ptr xml:id="note-0120-01a" corresp="note-0120-01" type="noteAnchor" />
levier CI qu’on ſuppoſe encore horizontal &amp; </s>
          <s xml:space="preserve">égal <lb />au premier: </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent ſi l’on regarde (Cor 2. <lb /></s>
          <s xml:space="preserve">Lem. </s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve">du Projet précéd.) </s>
          <s xml:space="preserve">l’impreſſion que la puiſſance <lb />S fait ſuivant CB ſur le noeud C qui retient enſemble <lb />les cordes de ces puiſſances &amp; </s>
          <s xml:space="preserve">de ce poids, comme <lb />compoſée de deux impreſſions particuliéres, dont <lb />l’une eſt ſuivant l’horizontale CO, &amp; </s>
          <s xml:space="preserve">l’autre ſuivant <lb />la perpendiculaire CH; </s>
          <s xml:space="preserve">on trouvera que ce que cette <lb />puiſſance lui en fait ſuivant CO, eſt égal à la réſiſ-<lb />tance que feroit alors contre ce même point, &amp; </s>
          <s xml:space="preserve">ſui-<lb />vant cette même ligne, le levier CG pour empêcher <lb />la corde ACX de ſe redreſſer; </s>
          <s xml:space="preserve">c’eſt-à-dire, égal à la <lb />charge de l’apui G de ce même levier. </s>
          <s xml:space="preserve">Or (Cor. </s>
          <s xml:space="preserve">4. </s>
          <s xml:space="preserve"><lb />Prop. </s>
          <s xml:space="preserve">fond. </s>
          <s xml:space="preserve">des leviers du Proj. </s>
          <s xml:space="preserve">précéd.) </s>
          <s xml:space="preserve">la puiſſance R <lb />eſt à la charge de cet apui, comme le côté AC du <lb />parallelogramme AE, à ſa diagonale CG; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">la force <lb />de l’impreſſion que fait la puiſſance S ſur ce même <lb />point C ſuivant CO, eſt (Cor. </s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve">Lemm. </s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve">du Projet <lb />précéd.) </s>
          <s xml:space="preserve">à celle de cette même puiſſance ſuivant CB, <lb />c’eſt-à-dire, à cette puiſſance, elle-même, comme <lb />le côté OC du parallelogramme OH, à ſa diagonale <lb />BC; </s>
          <s xml:space="preserve">c’eſt-à-dire, en faiſant IK perpendiculaire ſur <lb />BC, comme CK à CI égale (Hyp.) </s>
          <s xml:space="preserve">à CG: </s>
          <s xml:space="preserve">Donc la <lb />puiſſance R eſt à la puiſſance S, comme le produit <lb />de AC par CK, au quarré de CG. </s>
          <s xml:space="preserve">Or en faiſant GF <lb />perpendiculaire ſur AC, les triangles AGC &amp; </s>
          <s xml:space="preserve">GFC <lb />étant ſemblables, le produit de AC par CF eſt égal <lb />au quarré de CG: </s>
          <s xml:space="preserve">Donc la puiſſance R eſt à la puiſ-<lb />ſance S, comme le produit de AC par CK au produit <lb />de la même AC par CF, c’eſt-à-dire, comme CK à <lb />CF; </s>
          <s xml:space="preserve">ou bien, à cauſe des rayons IC &amp; </s>
          <s xml:space="preserve">CG (byp.) </s>
          <s xml:space="preserve"><lb />égaux, comme le ſinus de KIC égal à BCH, au ſinus <lb />de FGC égal à ACH: </s>
          <s xml:space="preserve">Donc la puiſſance R eſt à la <lb />puiſſance S, comme le ſinus de l’angle BCH à celui
</s>
          <pb facs="0121" n="95" />
          <s xml:space="preserve"><fw type="head">DE M. BORELLI.</fw>
de l’angle ACH qui, à cauſe du parallelogramme <lb />
<ptr xml:id="note-0121-01a" corresp="note-0121-01" type="noteAnchor" />
MN, eſt égal à CHM: </s>
          <s xml:space="preserve">Donc (Lemm. </s>
          <s xml:space="preserve">5. </s>
          <s xml:space="preserve">du Projet <lb />précéd) la puiſſance R eſt à la puiſſance S, comme <lb />HM, ou comme ſon égale NC à CM.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0120-01" corresp="note-0120-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />l@ment.</note>
              <note xml:space="preserve" xml:id="note-0121-01" corresp="note-0121-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">Voilà ce que M. </s>
          <s xml:space="preserve">Borelli devoit premiérement <lb />conclure de ſa 68. </s>
          <s xml:space="preserve">propoſition, ſinon en géné-<lb />ral, du moins pour tous les cas qu’elle com-<lb />prend: </s>
          <s xml:space="preserve">Sçavoir que lorſque deux puiſſances R &amp; </s>
          <s xml:space="preserve">S ſou-<lb />tiennent enſemble quelque poids T avec des cordes ſeulement, <lb />elles ſont toujours @ntr’elles en même raiſon que les parties <lb />CN &amp; </s>
          <s xml:space="preserve">MC de leurs cordes, qui ſervent de côtez au pa-<lb />rallelogramme MN, qui a pour diagonale une partie CH <lb />de la li@ne de direction du poids qu’elles ſoutiennent. </s>
          <s xml:space="preserve">De là <lb />en faiſant MP &amp; </s>
          <s xml:space="preserve">NQ perpendiculaires ſur HC, ces <lb />lignes marquant toujours CP égale à HQ, cet Au-<lb />theur auroit trouvé, comme il a fait (pag. </s>
          <s xml:space="preserve">137.) <lb /></s>
          <s xml:space="preserve">que chacune des puiſſances R &amp; </s>
          <s xml:space="preserve">S, étant toujours (par <lb />le Cor. </s>
          <s xml:space="preserve">de ſa 69. </s>
          <s xml:space="preserve">Prop.) </s>
          <s xml:space="preserve">à tout ce poids, comme chacun <lb />des côtez CN &amp; </s>
          <s xml:space="preserve">MC du parallelogramme MN, à la <lb />ſomme de leurs ſublimitez CP &amp; </s>
          <s xml:space="preserve">CQ; </s>
          <s xml:space="preserve">lui eſt auſſi <lb />toujours comme cbacun de ces mêmes côtez à la diagonale <lb />CH de ce même para@lelogramme. </s>
          <s xml:space="preserve">Ce qu’il faloit démon-<lb />trer.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">Quoi que cette conſéquence ſuive néceſſairement de la <lb />68. </s>
          <s xml:space="preserve">Propoſition de M. </s>
          <s xml:space="preserve">Borelli, cependant parce-que cette <lb />Propoſition ne peut pas s’appliquer aux cas ou une de <lb />ces pu@ſſances ſe trouve avoir ſa direction au deſſous de <lb />l’borizontale qui paſſe par le point où leurs cordes ſe com-<lb />muniquent, elle n’en eſt pas une ſuitte ſi générale que de la <lb />Propoſition fondamentale des poids ſuſpendus par des cordes <lb />du Projet précédent: </s>
          <s xml:space="preserve">C’eſt pour cela qu’on ſe contente ici de <lb />dire, que ſi cet Autbeur eût fait un peu plus d’attention à <lb />ſa 68. </s>
          <s xml:space="preserve">Prop. </s>
          <s xml:space="preserve">il auroit aperçû que tout ce que nous venons <lb />d’en conclure, eſt abſolument vrai, du moins pour tous <lb />les cas qu’elle comprend.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0122" n="96" />
        <fw type="head">EXAMEN DE L’OPINION</fw>
        <p>
          <s xml:space="preserve">Telle eſt la conſéquence que Monſieur Borelli <lb />
<ptr xml:id="note-0122-01a" corresp="note-0122-01" type="noteAnchor" />
devoit tirer de ſa 68. </s>
          <s xml:space="preserve">Propoſition; </s>
          <s xml:space="preserve">s’il l’eût fait, il <lb />auroit aperçû 1°. </s>
          <s xml:space="preserve">que la premiére partie du ſcholie <lb />qu’il en tire, n’eſt vraye qu’en cas que la variation <lb />du poids T &amp; </s>
          <s xml:space="preserve">des forces ſ &amp; </s>
          <s xml:space="preserve">S, entre leſquels il dit <lb />que l’équilibre ſe peut conſerver ſans changer l’in-<lb />clinaiſon de leurs cordes, ſoit telle que ce poids de-<lb />meure toujours à chacune de ces puiſſances en même <lb />raiſon que la diagonale CH du parallelogramme <lb />MN, à chaque partie de leurs cordes qui lui ſert de <lb />côté. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Il auroit encore vû que la ſeconde partie <lb />de ce même ſcholie eſt abſolument fauſſe; </s>
          <s xml:space="preserve">puis qu’il <lb />n’eſt pas poſſible de faire le moindre changement <lb />auquel que ce ſoit des angles ACB, ACH, &amp; </s>
          <s xml:space="preserve">BCH, <lb />ſans changer en même - tems le raport qui eſt, ou <lb />entre les côtez du parallelogramme MN, ou entre <lb />quelqu’un d’eux &amp; </s>
          <s xml:space="preserve">ſa diagonale; </s>
          <s xml:space="preserve">c’eſt - à - dire, puis <lb />que (byp.) </s>
          <s xml:space="preserve">on ne change rien au raport qui eſt entre <lb />ce poids &amp; </s>
          <s xml:space="preserve">chacune de ces puiſſances, ſans faire ceſſer <lb />la reſſemblance de ces deux raports: </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſe-<lb />quent auſſi, ſuivant ce qui vient d’être conclu de la <lb />68. </s>
          <s xml:space="preserve">Propoſition de M. </s>
          <s xml:space="preserve">Borelli, ſans rompre l’équili-<lb />bre de ce poids avec ces puiſſances.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0122-01" corresp="note-0122-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des c<unclear reason="illegible" />otdes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Remarque.</hi></head>
        <p>
          <s xml:space="preserve">Ayant demontré, comme l’on vient de faire, <lb />que le ſentiment, dont il eſt ici queſtion, bien loin <lb />d’être contraire à la 68. </s>
          <s xml:space="preserve">Propoſit. </s>
          <s xml:space="preserve">de M. </s>
          <s xml:space="preserve">Borelli, <lb />comme cet Autheur l’a crû, en eſt une ſuitte ſi né-<lb />ceſſaire que, s’il eût fait encore quelques pas, il <lb />l’auroit linfailliblement trouvé: </s>
          <s xml:space="preserve">c’eſt encore une nou-<lb />velle raiſon de ne nous point arrêter aux expériences <lb />qu’il objecte à Stévin, à Hérigone, &amp; </s>
          <s xml:space="preserve">aux autres, &amp; </s>
          <s xml:space="preserve"><lb />de ne toucher à la critique qu’il a faite de leurs rai-
</s>
          <pb facs="0123" n="97" />
          <s xml:space="preserve"><fw type="head">DE M. BORELLI.</fw>
ſonnemens, que pour indiquer les fauſſes ſuppo-<lb />
<ptr xml:id="note-0123-01a" corresp="note-0123-01" type="noteAnchor" />
ſitions ſur leſquelles il s’eſt appuyé pour y trouver <lb />du paralogiſme: </s>
          <s xml:space="preserve">Il y en a trois que voici.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0123-01" corresp="note-0123-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">1°. </s>
          <s xml:space="preserve">Dans la Critique qu’il a faite du premier de <lb />ces raiſonnemens, qui paroît être du P. </s>
          <s xml:space="preserve">Pardie, <lb />aprés avoir dit que, ſi l’on regarde la corde AC com-<lb />me une verge de fer mobile autour du point fixe A, <lb />
<ptr xml:id="note-0123-02a" corresp="note-0123-02" type="noteAnchor" />
à laquelle le poids T ſoit attaché, ce poids ſera ſou-<lb />tenu avec cette verge par ce point fixe, de même que <lb />ſur un plan CI perpendiculaire à AC; </s>
          <s xml:space="preserve">il fait IL per-<lb />pendiculaire à l’horizontale LC, &amp; </s>
          <s xml:space="preserve">(pag. </s>
          <s xml:space="preserve">139.) </s>
          <s xml:space="preserve">il <lb />dit: </s>
          <s xml:space="preserve">patet quod pondus T.</s>
          <s xml:space="preserve">..</s>
          <s xml:space="preserve">..</s>
          <s xml:space="preserve">..</s>
          <s xml:space="preserve">. ad vim quâ idem T inni-<lb />titur, &amp; </s>
          <s xml:space="preserve">comprimit idem planum IC, eſt ut IC ad LC.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0123-02" corresp="note-0123-02a" place="margin">ſig. 2.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Dans la Critique qu’il fait enſuite du rai-<lb />ſonnement de Hérigone, de Stévin, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">aprés <lb />
<ptr xml:id="note-0123-03a" corresp="note-0123-03" type="noteAnchor" />
avoir regardé le poids T ſoutenu par les cordes AC <lb />&amp; </s>
          <s xml:space="preserve">BC, comme s’il l’étoit ſur les plans CK perpendi-<lb />culaire à AC, &amp; </s>
          <s xml:space="preserve">CG perpendiculaire à CB, inéga-<lb />lement inclinez, il dit (pag. </s>
          <s xml:space="preserve">141.) </s>
          <s xml:space="preserve">Tunc pondus T <lb />dum moveri niteretur per duas rectas inclinatas CK &amp; </s>
          <s xml:space="preserve">CG, <lb />cogeretur moveri, aut niſum exercere per diagonalem CO <lb />ſecantem angulum GCK bifariam.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0123-03" corresp="note-0123-03a" place="margin">ſig. 3.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">Outre cette ſuppoſition, M. </s>
          <s xml:space="preserve">Borelli ſe ſert en-<lb />core ici de la premiére qu’il a déja faite contre le <lb />P. </s>
          <s xml:space="preserve">Pardie. </s>
          <s xml:space="preserve">Il dit (pag. </s>
          <s xml:space="preserve">141.) </s>
          <s xml:space="preserve">aprés avoir fait CP <lb />perpendiculaire à l’horizontale KG: </s>
          <s xml:space="preserve">Idem pondus ab-<lb />ſolutum T ad vim, quâ comprimit planum CO, eandem <lb />rationem babebit quàm CO ad OP.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">3°. </s>
          <s xml:space="preserve">Enfin ces deux ſuppoſitions ne lui ſuffiſant pas <lb />encore pour trouver à redire au raiſonnement d’Hé-
</s>
          <pb facs="0124" n="98" />
          <s xml:space="preserve"><fw type="head">EXAMEN DE L’OPINION</fw>
rigone, de Stévin, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">il y en ajoûte une troi-<lb />
<ptr xml:id="note-0124-01a" corresp="note-0124-01" type="noteAnchor" />
ſiéme qui ne vaut pas mieux. </s>
          <s xml:space="preserve">Vis, dit-il au même en-<lb />droit, quam patitur planum CO à compreſſione ponderis T <lb />aqualis eſt viribus ambarum potentiarum R &amp; </s>
          <s xml:space="preserve">S, quæ <lb />ſuſtinendo idem pondus in tali ſitu plani CO inclinati vicem <lb />ſupplent.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0124-01" corresp="note-0124-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <p rend="italics">
          <s xml:space="preserve">On ne démontre point ici la fauſſeté de toutes ces ſup-<lb />poſitions: </s>
          <s xml:space="preserve">elle eſt trop évidente par la propoſition des Sur-<lb />faces du Projet précédent, pour s’y arrêter davantage. <lb /></s>
          <s xml:space="preserve">D’ailleurs c’eſt, ce me ſemble, avoir ſuffiſamment répondu <lb />à M. </s>
          <s xml:space="preserve">Borelli que d’avoir démontré, comme l’on vient de <lb />faire, le ſentiment d’Hérigone, de Stévin, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">par la <lb />Propoſition même que cet Autbeur croyoit leur être contraire: </s>
          <s xml:space="preserve"><lb />c’eſt auſſi tout ce qu’on s’étoit propoſé dans ce premier Cba-<lb />pitre; </s>
          <s xml:space="preserve">paſſons au ſecond.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0124-01" />
          <label>0124-01</label>
        </figure>
        <pb facs="0125" n="99" />
        <fw type="head">DE M. BORELLI</fw>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0125-01" />
          <label>0125-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">CHAPITRE II. <lb />NOUVELLES DEMONSTRATIONS <lb />du ſentiment d’Hérigone, de Stévin, &amp;c.</head>
        <head xml:space="preserve">Sur les propriétez des poids ſuspendus par <lb />des cordes.</head>
        <head xml:space="preserve">AVEC QUELQUES PROPOSITIONS <lb />de M. Borelli renduës par la méthode du Projet <lb />précédent beaucoup plus générales qu’elles <lb />ne le peuvent être par la ſienne.</head>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0125-02" />
          <label>0125-02</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">AVER TISSEMENT.</head>
        <p rend="italics">
          <s xml:space="preserve">LE Poids T étant ſoutenu par deux, ou pluſieurs puiſ-<lb />ſances R, S, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">Si des extrémitez G, H, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">des <lb />
<ptr xml:id="note-0125-01a" corresp="note-0125-01" type="noteAnchor" />
parties CG, CH, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">de leurs cordes qui leur ſoient pro-<lb />portionnelles, on fait GP, HQ, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">perpendiculaires ſur <lb />ſa ligne de direction CD; </s>
          <s xml:space="preserve">elles y déſigncront depuis leurs <lb />points de rencontre P, Q, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">juſqu’au point C ou cette <lb />ligne concourt avec ces cordes, certaines parties CP, CQ <lb />&amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">d@nt nous parlerons ſouvent dans la ſuite; </s>
          <s xml:space="preserve">C’eſt pour-<lb />quoy nous leur allons donner des noms.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0125-01" corresp="note-0125-01a" place="margin">ſig. 4. <lb />5.</note>
            </div>
          </body>
        </floatingText>
        <pb facs="0126" n="100" />
        <fw type="head">EXAMEN DE L’OPINION</fw>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Definition</hi> I.</head>
        <note xml:space="preserve" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
        <p>
          <s xml:space="preserve">Lorſque ces parties CP, CQ, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">ſe trouveront <lb />au-deſſus du point C, nous les appellerons les ſublimitez <lb />des puiſſances qui les auront déterminées par leurs <lb />proportionnelles.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Definition</hi> II.</head>
        <p>
          <s xml:space="preserve">Et celles de ces lignes qui ſe trouveront au-deſſous <lb />de ce même point C, nous les appellerons les Pro-<lb />fondeurs de ces mêmes puiſſances.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">Selon ces définitions C P eſt la Sublimité de la puiſſance R <lb />dans les fig. </s>
          <s xml:space="preserve">4. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">5. </s>
          <s xml:space="preserve">CL eſt encore la Sublimité de la <lb />puiſſance S dans la fig. </s>
          <s xml:space="preserve">4. </s>
          <s xml:space="preserve">Mais dans la fig. </s>
          <s xml:space="preserve">5. </s>
          <s xml:space="preserve">CL eſt la <lb />Profondeur de cette mème puiſſance.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">On avertit encore que lorſqu’on comparera à la ſublimi-<lb />té, ou à la profondeur de ces puiſſances, des parties de leurs <lb />cordes qui leur ſoient proportionnelles, on ne l’entendra pas <lb />indiffèremment de toutes les proportionnelles qu’on pouroit <lb />leur aſſigner; </s>
          <s xml:space="preserve">mais ſeulement de celles qui déterminent les ſu-<lb />blimitez, ou les profondeurs en queſtion.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0126-01" />
          <label>0126-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">PROPOSITION I.</head>
        <p rend="italics">
          <s xml:space="preserve">LE poids T ſoutenu avec les cordes AC &amp; </s>
          <s xml:space="preserve">BC par les <lb />
<ptr xml:id="note-0126-02a" corresp="note-0126-02" type="noteAnchor" />
puiſſances R &amp; </s>
          <s xml:space="preserve">S, &amp; </s>
          <s xml:space="preserve">en équilibre avec elles, eſt tou-<lb />jours à chacune d’elles, comme la partie DC de ſa ligne de ái-<lb />rection, à chacun des còtez GC &amp; </s>
          <s xml:space="preserve">HC du parallelogramme <lb />GH, dont elle eſt diagonale.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0126-02" corresp="note-0126-02a" place="margin">ſig. 4. <lb />5. <lb />6. <lb />7.</note>
            </div>
          </body>
        </floatingText>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0126-02" />
          <label>0126-02</label>
        </figure>
        <pb facs="0127" n="101" />
        <fw type="head">DE M. BORELLI.</fw>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstrations.</hi></head>
        <note xml:space="preserve" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
        <p>
          <s xml:space="preserve">1°. </s>
          <s xml:space="preserve">Voyez celle qu’on a donnée de cette même <lb />propoſition dans le Projet précédent.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Voyez ci-aprés la Remarque qui ſuitle Corol-<lb />laire de la Prop. </s>
          <s xml:space="preserve">3.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">3°. </s>
          <s xml:space="preserve">Soient conçûs les leviers MC &amp; </s>
          <s xml:space="preserve">NC placez <lb />
<ptr xml:id="note-0127-02a" corresp="note-0127-02" type="noteAnchor" />
chacun en ligne droite avec chacune des directions <lb />AC &amp; </s>
          <s xml:space="preserve">BC des puiſſances R &amp; </s>
          <s xml:space="preserve">S. </s>
          <s xml:space="preserve">De leurs points <lb />d’appui M &amp; </s>
          <s xml:space="preserve">N pris à diſcretion, ſoient tirées MF <lb />&amp; </s>
          <s xml:space="preserve">NK perpendiculairement à ces mêmes lignes ré-<lb />ciproquement priſes, &amp; </s>
          <s xml:space="preserve">ML avec NO perpendicu-<lb />laires auſſi à la ligne de direction DCE de ce même <lb />poids. </s>
          <s xml:space="preserve">Enfin de quelqu’un des points D de cette <lb />même ligne faite DH &amp; </s>
          <s xml:space="preserve">DG paralleles à AC &amp; </s>
          <s xml:space="preserve">à <lb />CB. </s>
          <s xml:space="preserve">Cela fait, il eſt clair que le levier CN, étant <lb />(hyp.) </s>
          <s xml:space="preserve">en ligne droite avec la ligne de dìrection CB <lb />de la puiſſance S, ſupplée néceſſairement tout l’effet <lb />de cette puiſſance; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">que par conſéquent la puiſ-<lb />ſance R pourroit ſuivant ſa même direction AC ſou-<lb />tenir ſeule le poids T avec ce levier ainſi placé, de <lb />même qu’elle le ſoutient préſentement avec la puiſ-<lb />ſance S. </s>
          <s xml:space="preserve">Pour la même raiſon la puiſſance S pourroit <lb />auſſi le ſoutenir ſeule avec le levier CM, de même <lb />qu’elle le ſoutient préſentement avec la puiſſance <lb />R: </s>
          <s xml:space="preserve">lepoids T eſt donc ſoutenu par le concours d’ac-<lb />tion des puiſſances R &amp; </s>
          <s xml:space="preserve">S, de même qu’il le ſeroit <lb />par la ſeule puiſſance R appliquée avec lui au levier <lb />NC, ou bien par la ſeule puiſſance S appliquée auſſi <lb />avec lui au levier CM. </s>
          <s xml:space="preserve">Or dans le premier cas la <lb />puiſſance R ſeroit (Prop. </s>
          <s xml:space="preserve">fond. </s>
          <s xml:space="preserve">des leviers Cor. </s>
          <s xml:space="preserve">13. </s>
          <s xml:space="preserve">du <lb />Projet précéd.) </s>
          <s xml:space="preserve">au poids T, comme NO à NK; </s>
          <s xml:space="preserve">c’eſt-<lb />à-dire, comme le ſinus de l’angle NCO, ou de
</s>
          <pb facs="0128" n="102" />
          <s xml:space="preserve"><fw type="head">EXAMEN DE L’OPINION</fw>
DCH, à celui de l’angle NCK, ou de CHD. </s>
          <s xml:space="preserve">Et <lb />
<ptr xml:id="note-0128-01a" corresp="note-0128-01" type="noteAnchor" />
dans le ſecond cas le poids T, pour la même raiſon, <lb />ſeroit à la puiſſance S, comme MF à ML; </s>
          <s xml:space="preserve">c’eſt-à-dire <lb />encore, comme le ſinus de l’angle MCF, ou de CHD, <lb />à celui de l’angle MCL, ou de HDC: </s>
          <s xml:space="preserve">Donc la puiſ-<lb />ſance R, le poids T, &amp; </s>
          <s xml:space="preserve">la puiſſance S, ſont entr’eux, <lb />comme les ſinus des angles DCH, CHD, &amp; </s>
          <s xml:space="preserve">HDC; <lb /></s>
          <s xml:space="preserve">c’eſt-à-dire, ( Demm. </s>
          <s xml:space="preserve">5. </s>
          <s xml:space="preserve">du Projet précéd.) </s>
          <s xml:space="preserve">comme les <lb />lignes DH, CD, &amp; </s>
          <s xml:space="preserve">CH: </s>
          <s xml:space="preserve">Le poids T eſt done à la <lb />puiſſance R, comme CD à DH, ou à CG; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">à la <lb />puiſſance S, comme la même CD à CH. </s>
          <s xml:space="preserve">Ce qu’il faloit <lb />démontrer.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0127-02" corresp="note-0127-02a" place="margin">fig. 4. <lb />5.</note>
              <note xml:space="preserve" xml:id="note-0128-01" corresp="note-0128-01a" place="margin">DES POIDS <lb />foutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">4°. </s>
          <s xml:space="preserve">Si au lieu des puiſſances R &amp; </s>
          <s xml:space="preserve">S, les cordes AC <lb />&amp; </s>
          <s xml:space="preserve">BC étoient attachees aux extrémitez de quelque le-<lb />vier AB, dont l’appui D fut dans la ligne direction de <lb />
<ptr xml:id="note-0128-02a" corresp="note-0128-02" type="noteAnchor" />
DCE du poids T. </s>
          <s xml:space="preserve">Il eſt clair qu’en quelque fitua-<lb />tion que ce levier ſe trouvât alors, (Lemm. </s>
          <s xml:space="preserve">@. </s>
          <s xml:space="preserve">du <lb />Projet précéd.) </s>
          <s xml:space="preserve">il y demeureroit, &amp; </s>
          <s xml:space="preserve">que la charge de <lb />ſon point d’appui ſeroit alors égale au poids T. </s>
          <s xml:space="preserve">Il <lb />eſt encore clair que les extrémitez A &amp; </s>
          <s xml:space="preserve">B de ce mê-<lb />me levier ſeroient auſſi tirées ſuivant AC &amp; </s>
          <s xml:space="preserve">BC, <lb />chacune avec une force égale à celle de la puiſſance <lb />R, ou S qu’elle ſupplée. </s>
          <s xml:space="preserve">Or les forces avec leſquelles <lb />les points A &amp; </s>
          <s xml:space="preserve">B de ce levier ſeroient ainſi tirez ſui-<lb />vant AC &amp; </s>
          <s xml:space="preserve">BC, ſeroient entr’elles, ( Cor. </s>
          <s xml:space="preserve">13. </s>
          <s xml:space="preserve">prop. <lb /></s>
          <s xml:space="preserve">fond. </s>
          <s xml:space="preserve">des leviers du Projet précéd.) </s>
          <s xml:space="preserve">comme DF &amp; </s>
          <s xml:space="preserve">DK <lb />tirées du point D perpendiculairement ſur BC &amp; </s>
          <s xml:space="preserve"><lb />AC; </s>
          <s xml:space="preserve">c’eſt-à-dire, en faiſant le parallelogramme GH, <lb />comme les ſinus des angles DCH &amp; </s>
          <s xml:space="preserve">CDH, ou <lb />(Lemm. </s>
          <s xml:space="preserve">5. </s>
          <s xml:space="preserve">du Proiet précéd.) </s>
          <s xml:space="preserve">comme les côtez DH &amp; </s>
          <s xml:space="preserve"><lb />HC de ce parallelogramme. </s>
          <s xml:space="preserve">Ces mêmes forces ſe-<lb />roient auſſi ( Cor. </s>
          <s xml:space="preserve">4. </s>
          <s xml:space="preserve">Prop. </s>
          <s xml:space="preserve">fond. </s>
          <s xml:space="preserve">des leviers au Projet <lb />précèd.) </s>
          <s xml:space="preserve">chacune à la charge du point d’appui D de <lb />ce levier, c’eſt-à-dire, au poids T, comme chacun
</s>
          <pb facs="0129" n="103" />
          <s xml:space="preserve"><fw type="head">DE M. BORELLI.</fw>
ces de mêmes côtez à la diagonale DC: </s>
          <s xml:space="preserve">les forces <lb />
<ptr xml:id="note-0129-01a" corresp="note-0129-01" type="noteAnchor" />
des puiſſances R &amp; </s>
          <s xml:space="preserve">S, c’eſt-à-dire, ces mêmes puiſ-<lb />ſances, elles-mêmes, ſont donc entr’elles, comme <lb />DH, ou GC &amp; </s>
          <s xml:space="preserve">HC; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">au poids T, comme chacun <lb />de ces mêmes côtez du parallelogramme GH, à ſa <lb />diagonale DC. </s>
          <s xml:space="preserve">Cequ’il faloit démontrer.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0128-02" corresp="note-0128-02a" place="margin">fig. 6. <lb />7.</note>
              <note xml:space="preserve" xml:id="note-0129-01" corresp="note-0129-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement</note>
            </div>
          </body>
        </floatingText>
        <p rend="italics">
          <s xml:space="preserve">On pourroit encore démontrer cette mème Propoſition en <lb />ſe ſervant des plans inclinez, pourvû qu’on en prit un qui <lb />fut perpendiculaire à la direction de quelqu’une des deux <lb />puiſſances qui ſoutiennent ce poids: </s>
          <s xml:space="preserve">Car cette puiſſance &amp; </s>
          <s xml:space="preserve"><lb />la cbarge de ce plan alors égales, n’ayant qu’un mème <lb />rapport avec ce poids, non plus qu’avec l’autre puiſſance <lb />qu’on conſidére en ce cas comme le ſoutenant ſeule ſur ce plan; <lb /></s>
          <s xml:space="preserve">on trouveroit par le Cor. </s>
          <s xml:space="preserve">7. </s>
          <s xml:space="preserve">de la Prop. </s>
          <s xml:space="preserve">des Surfaces du <lb />Projet précédent, que ce poids eſt toujours à chacune de ces <lb />puiſſances, comme le ſinus de l’angle que leurs cordes font <lb />entr’elles, à chacun des ſinus des angles que font avec la <lb />ligne de direction de ce poids chacune de ces cordes récipro-<lb />quement priſes. </s>
          <s xml:space="preserve">Tout cela eſt préſentement trop clair pour <lb />s’y arréter davantage.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> I.</head>
        <p>
          <s xml:space="preserve">On peut conclure généralement de ces démon-<lb />
<ptr xml:id="note-0129-02a" corresp="note-0129-02" type="noteAnchor" />
ſtrations, ce que nous n’avons conclu ( chap. </s>
          <s xml:space="preserve">1.) </s>
          <s xml:space="preserve">dela <lb />68. </s>
          <s xml:space="preserve">Propoſition de M. </s>
          <s xml:space="preserve">Borelli, quepour les cas qu’elle <lb />comprend: </s>
          <s xml:space="preserve">Sçavoir qu’il n’y en à aucun de poſſible, <lb />ou l’on puiſſe conſerver l’équilibre du poids T avec <lb />les puiſſances R &amp; </s>
          <s xml:space="preserve">S, en changeant le rapport qu’elles <lb />ont entr’elles, ou avec lui; </s>
          <s xml:space="preserve">à moins qu’on ne change <lb />en même-tems l’inclinaiſon de leurs cordes: </s>
          <s xml:space="preserve">non plus <lb />qu’en changeant l’inclinaiſon de ces cordes, ſans <lb />changer auſſi le rapport de ces mêmes puiſſances, <lb />ou entr’elles, ou avec ce poids: </s>
          <s xml:space="preserve">parce que ſans cela <lb />il n’eſt pas poſſible de faire que chacun des côtez CH
</s>
          <pb facs="0130" n="104" />
          <s xml:space="preserve"><fw type="head">EXAMEN DE L’OPINION</fw>
&amp; </s>
          <s xml:space="preserve">CG du parallelogramme GH, continuë d’être à ſa <lb />
<ptr xml:id="note-0130-01a" corresp="note-0130-01" type="noteAnchor" />
diagonale DC, comme chacune des puiſſances R &amp; </s>
          <s xml:space="preserve">S <lb />au poids T; </s>
          <s xml:space="preserve">ce qui doit cependant être, comme onle <lb />vient de voir, pour qu’elles faſſent équilibre avec lui.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0129-02" corresp="note-0129-02a" place="margin">fig. 4. <lb />5. <lb />6. <lb />7.</note>
              <note xml:space="preserve" xml:id="note-0130-01" corresp="note-0130-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <p rend="italics">
          <s xml:space="preserve">On peut comparer ce Corollaire aux Scholies des Pro-<lb />poſitions 68. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">69. </s>
          <s xml:space="preserve">M. </s>
          <s xml:space="preserve">Borelli.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> II.</head>
        <p>
          <s xml:space="preserve">Il ſuit encore de ces démonſtrations que chacune <lb />des puiſſances R &amp; </s>
          <s xml:space="preserve">S eſt au poids T, comme chacune <lb />
<ptr xml:id="note-0130-02a" corresp="note-0130-02" type="noteAnchor" />
des parties GC &amp; </s>
          <s xml:space="preserve">HC de leurs cordes, qui leurs ſont <lb />proportionelles, à la ſomme ( fig. </s>
          <s xml:space="preserve">4.) </s>
          <s xml:space="preserve">de leurs ſublimi-<lb />tez, ou à la difference (fig. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">quieſt entre la ſublimité <lb />de l’une &amp; </s>
          <s xml:space="preserve">la profondeur de l’autre: </s>
          <s xml:space="preserve">parce que dans <lb />le parallelogramme GH les angles GCD &amp; </s>
          <s xml:space="preserve">CDH <lb />étant égaux, auſſi-bien que les lignes GC &amp; </s>
          <s xml:space="preserve">DH; <lb /></s>
          <s xml:space="preserve">de plus les angles qui ſe font en P &amp; </s>
          <s xml:space="preserve">en Q, étant auſſi <lb />(avert.) </s>
          <s xml:space="preserve">égaux, les triangles GPC &amp; </s>
          <s xml:space="preserve">HQD ſont <lb />non ſeulement ſemblables, mais encore leurs côtez <lb />CP &amp; </s>
          <s xml:space="preserve">DQ ſont égaux: </s>
          <s xml:space="preserve">Donc (fig. </s>
          <s xml:space="preserve">4.) </s>
          <s xml:space="preserve">CP plus CQ <lb />eſt égal à DQ plus CQ, &amp; </s>
          <s xml:space="preserve">( fig. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">CP moins CQ <lb />ſera auſſi égal à DQ moins CQ. </s>
          <s xml:space="preserve">Or ( fig. </s>
          <s xml:space="preserve">4.) </s>
          <s xml:space="preserve">DQ <lb />plus CQ eſt égal à CD, de même (fig. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">que <lb />DQ moins CQ: </s>
          <s xml:space="preserve">Donc ( fig. </s>
          <s xml:space="preserve">4.) </s>
          <s xml:space="preserve">CP plus CQ eſt égal <lb />à CD, auſſi-bien (fig. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">que CP moins CQ. </s>
          <s xml:space="preserve">Or <lb />ſelon les démonſtrations précédentes chacune des <lb />puiſſances R &amp; </s>
          <s xml:space="preserve">S eſt au poids T, comme chacune de <lb />leurs proportionelles CG &amp; </s>
          <s xml:space="preserve">HC à CD: </s>
          <s xml:space="preserve">Donc cha-<lb />cune de ces mêmes puiſſances eſt à ce poids, comme <lb />chacune de ces mêmes proportionelles à CP ( fig. </s>
          <s xml:space="preserve">4.) </s>
          <s xml:space="preserve"><lb />plus CQ, ou (fig. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">à CP moins CQ; </s>
          <s xml:space="preserve">c’eſt-à-dire, <lb />(Def. </s>
          <s xml:space="preserve">1. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">2.) </s>
          <s xml:space="preserve">à la ſomme ( fig. </s>
          <s xml:space="preserve">4.) </s>
          <s xml:space="preserve">de leurs ſublimitez, <lb />ou bien ( fig. </s>
          <s xml:space="preserve">5.) </s>
          <s xml:space="preserve">à la différence qui eſt entre la ſublimi-<lb />té de l’une &amp; </s>
          <s xml:space="preserve">la profondeur de l’autre.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0130-02" corresp="note-0130-02a" place="margin">fig. 4. <lb />5.</note>
            </div>
          </body>
        </floatingText>
        <pb facs="0131" n="105" />
        <fw type="head">DE M. BORELLI.</fw>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> III.</head>
        <note xml:space="preserve" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
        <p>
          <s xml:space="preserve">D’où l’on voit que la ſomme des deux puiſſances <lb />qui ſoutiennent un poids avec des cordes, eſt tou-<lb />jours à ce poids, comme la ſomme des longueurs de <lb />leurs cordes, qui leur ſont proportionelles, à la ſomme <lb />de leurs ſublimitez, ou à la différence qui eſt entre de <lb />la ſublimité de l’une &amp; </s>
          <s xml:space="preserve">la profondeur de l’autre.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">On peut comparer encore ces deux derniers Corollaires à la <lb />69. </s>
          <s xml:space="preserve">Prop. </s>
          <s xml:space="preserve">de M. </s>
          <s xml:space="preserve">Borelli, &amp; </s>
          <s xml:space="preserve">au Corollaire qu’il entire.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0131-01" />
          <label>0131-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">PROPOSITION II.</head>
        <p rend="italics">
          <s xml:space="preserve">DE quelque maniére qu’un poids T ſoit ſoutenu avee <lb />
<ptr xml:id="note-0131-02a" corresp="note-0131-02" type="noteAnchor" />
des cordes par quelque nombre de puiſſances A, B, D, <lb />E, F, &amp; </s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">que ce ſoit, appliquèes à un même nœud C; </s>
          <s xml:space="preserve">ſi l’ on <lb />prend ſur leurs cordes autant de parties CG, CR, CM, CN, <lb />CP, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">qui leurs ſoient proportionelles, &amp; </s>
          <s xml:space="preserve">que ſous deux <lb />de ces parties, par exemple, ſous GC &amp; </s>
          <s xml:space="preserve">RC, l’on faſſe un <lb />parallelogramme RG, dont la diagonale CH faſſe encore <lb />avecune autre de ces parties CM le parallelogramme HM, <lb />dont la diagonale CL faſſe encore avec une autre de ces <lb />parties CN le parallelogramme LN, dont la diagonale <lb />CQ faſſe encore avec une autre de ces parties CP le paral-<lb />lelogramme PQ, &amp; </s>
          <s xml:space="preserve">ainſi juſqu’à la derniére de ces propor-<lb />tionelles. </s>
          <s xml:space="preserve">On verra 1°. </s>
          <s xml:space="preserve">Que la diagonale du dernier de ces <lb />parallelogrammes, qui eſt ici CK, ſera dans la ligne de di-<lb />rection du poids T. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Et que chacune de ces puiſſances ſera <lb />à ce poids, comme chacune de ces proportionelles, ſelon qu’el-<lb />les leurs répoudent, eſt à cette même diagonale.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0131-02" corresp="note-0131-02a" place="margin">fig. 2.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration.</hi></head>
        <p>
          <s xml:space="preserve">1°. </s>
          <s xml:space="preserve">Puiſque ( hyp.) </s>
          <s xml:space="preserve">la puiſſance A eſt à la puiſ-
</s>
          <pb facs="0132" n="106" />
          <s xml:space="preserve"><fw type="head">EXAMEN DE L’OPINION</fw>
ſance B, comme CG à CR, il réſultera (Lemm. </s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve">du <lb />
<ptr xml:id="note-0132-01a" corresp="note-0132-01" type="noteAnchor" />
Projet précèd.) </s>
          <s xml:space="preserve">de leur concours d’action ſur le point <lb />C, un@ impreſſion compoſée ſuivant CH, d’une force <lb />qui ſera (Cor. </s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve">du même Lemm.) </s>
          <s xml:space="preserve">à chacune de ces <lb />puiſſances, comme CH à chacune des lignes CG &amp; </s>
          <s xml:space="preserve"><lb />CR qui les répreſentent: </s>
          <s xml:space="preserve">l’impreſſion, que font en-<lb />ſemble ces deux puiſſances ſur le point C, eſt donc <lb />la même que celle que feroit ſeule ſur ce même point <lb />quelque nouvelle puiſſance qui, lui étant appliquée <lb />ſuivant CH, au lieu d’elles, leur ſeroit à chacune, <lb />comme CH à chacune des lignes CG &amp; </s>
          <s xml:space="preserve">CR: </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par <lb />conſèquent les 3. </s>
          <s xml:space="preserve">puiſſances A, B, D, doivent faire <lb />enſemble la même impreſſion ſur le point C que cette <lb />nouvelle puiſſance ( je l’appelle H ) feroit alors avec <lb />la puiſſance D. </s>
          <s xml:space="preserve">Or (Lemm 3. </s>
          <s xml:space="preserve">du Projet précéd.) </s>
          <s xml:space="preserve">l’im-<lb />preſſion qui réſulteroit alors du concours d’action <lb />des puiſſances D &amp; </s>
          <s xml:space="preserve">H ſur le point C, ſe feroit ſui-<lb />vant CL, d’une force qui ſeroit (Cor. </s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve">du même <lb />Lemm.) </s>
          <s xml:space="preserve">à celle de la puiſſance D, comme CL à CM: <lb /></s>
          <s xml:space="preserve">Donc l’impreſſion compoſée qui réſulte du concours <lb />d’action des 3. </s>
          <s xml:space="preserve">puiſſances A, B, D, ſur le point C, <lb />ſe fait en effet ſuivant CL, d’une force qui eſt à <lb />celle de la puiſſance D, comme CL à CM: </s>
          <s xml:space="preserve">elles ne <lb />font donc toutes trois enſemble ſur ce point que la <lb />même impreſſion que feroit ſeule quelqu’autre puiſ-<lb />ſance (je l’appelle L) qui appliquée ſuivant CL, au <lb />lieu de ces trois, ſeroit à la puiſſance D, comme CL <lb />à CM: </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent les 4. </s>
          <s xml:space="preserve">puiſſances A, B, D, E, <lb />ne doivent faire ſur le point C que la même impreſ-<lb />ſion que feroit alors la puiſſance L avec la puiſſance <lb />E. </s>
          <s xml:space="preserve">Or (Lemm. </s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve">du Projet Projet précéd.) </s>
          <s xml:space="preserve">l’impreſſion qui <lb />réſulteroit alors du concours d’action de ces deux <lb />dernieres puiſſances ſur le point C, ſe feroit ſuivant <lb />CQ, d’une force qui ſeroit ( Cor. </s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve">du même Lemm.) </s>
          <s xml:space="preserve"><lb />à celle de la puiſſance E, comme CQ à CN: </s>
          <s xml:space="preserve">Donc
</s>
          <pb facs="0133" n="107" />
          <s xml:space="preserve"><fw type="head">DE M. BORELLI.</fw>
l’impreſſion compoſée qui réſulte du concours d’ac-<lb />
<ptr xml:id="note-0133-01a" corresp="note-0133-01" type="noteAnchor" />
tion des 4. </s>
          <s xml:space="preserve">puiſſances A, B, D, E, ſur le point C, <lb />ſe fait en effet ſuivant la ligne CQ, d’une force qui <lb />eſt à celle de la puiſſance E, comme CQ à CN. </s>
          <s xml:space="preserve">On <lb />prouvera de même que l’impreſſion compoſée qui <lb />réſulte du concours d’action des 5. </s>
          <s xml:space="preserve">puiſſances A, B, <lb />D, E, F, ſe fait auſſi ſuivant CK, d’une force qui <lb />eſt à la puiſſance F, comme CK à CP. </s>
          <s xml:space="preserve">Et ainſi tou-<lb />jours de même juſqu’à la derniére des puiſſances <lb />appliquées à ce poids: </s>
          <s xml:space="preserve">D’où il ſuit que l’impreſſion <lb />compoſée qui réſulte du concours d’action de toutes <lb />ces puiſſances ſur le point C, en quelque nombre <lb />qu’elles ſoient, ſe fait toujours ſuivant la diagonale <lb />du dernier des parallelogrammes faits comme l’on <lb />vient de dire, c’eſt-à-dire ici, ſuivant CK: </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par <lb />conſéquent (n. </s>
          <s xml:space="preserve">2. </s>
          <s xml:space="preserve">Demonſt. </s>
          <s xml:space="preserve">Prop. </s>
          <s xml:space="preserve">fond. </s>
          <s xml:space="preserve">des poids ſoutenus <lb />par des cordes du Projet précéd.) </s>
          <s xml:space="preserve">cette diagonale eſt <lb />toujours en ligne droite avec CT, c’eſt-à-dire, dans <lb />la ligne de direction du poids T. </s>
          <s xml:space="preserve">Ce qu’il faloit dé-<lb />montrer.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0132-01" corresp="note-0132-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſcu-<lb />lement.</note>
              <note xml:space="preserve" xml:id="note-0133-01" corresp="note-0133-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">On vient de voir que le poids T eſt ſoutenu <lb />par les puiſſances A, B, D, E, F, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">De même qu’il <lb />le ſeroit, par exemple ici, par la puiſſance F aidée <lb />d’une autre appliquée ſuivant CQ, à qui elle ſeroit <lb />comme CP à CQ ( les directions de toutes demeu-<lb />rant toujours les mêmes): </s>
          <s xml:space="preserve">Donc (prop. </s>
          <s xml:space="preserve">1.) </s>
          <s xml:space="preserve">la puiſ-<lb />ſance F eſt au poids T, comme CP à CK. </s>
          <s xml:space="preserve">Or ( hyp.) <lb /></s>
          <s xml:space="preserve">la puiſſance F eſt à chacune des puiſſances E, D, B, A, <lb />&amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">comme CP à chacune des parties de leurs cordes, <lb />CN, CM, CR, CG, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">Donc chacune de ces <lb />puiſſances eſt au poids T, comme chacune de ces <lb />proportionelles, ſelon qu’elles leurs répondent, eſt à la <lb />diagonale CK. </s>
          <s xml:space="preserve">Ce qu’on vient de dire de la puiſſance <lb />F, ſe prouvera de même de toute autre dont la pro-
</s>
          <pb facs="0134" n="108" />
          <s xml:space="preserve"><fw type="head">EXAMEN DE L’OPINION</fw>
portionelle feroit un des côtez du parallelogramme <lb />
<ptr xml:id="note-0134-01a" corresp="note-0134-01" type="noteAnchor" />
qu’on vient de démontrer avoir toujours ſa diago-<lb />nale, comme ici CK, dans la ligne de direction du <lb />poids T: </s>
          <s xml:space="preserve">Ainſi en général de quelque maniére qu’un <lb />poids ſoit ſoutenu avec des cordes par quelque nom-<lb />bre de puiſſances que ce ſoit, appliquées à un même <lb />nœud, chacune de ces puiſſances eſt toujours à ce <lb />poids, comme chacune de leurs proportionelles qui <lb />ſervent de côtez aux parallelogrammes dont il eſt ici <lb />queſtion, eſt à la diagonale du dernier, qu’on vient <lb />de voir ſe trouver toujours dans ſa ligne de direction. <lb /></s>
          <s xml:space="preserve">Ce qu’il faloit démontrer.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0134-01" corresp="note-0134-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cord@s ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire.</hi></head>
        <p>
          <s xml:space="preserve">D’où l’on voit que toutes ces puiſſances priſes <lb />enſemble ſont toujours au poids T qu’elles ſoutien-<lb />nent, comme la ſomme de leurs proportionelles CG, <lb />CR, CM, CN, CP, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">à la diagonale du paralle-<lb />logramme qu’on vient de démontrer (n. </s>
          <s xml:space="preserve">1.) </s>
          <s xml:space="preserve">ſe trou-<lb />ver toujours dans la ligne de direction de ce poids: <lb /></s>
          <s xml:space="preserve">De ſorte que, lorſque toutes ces puiſſances ſont éga-<lb />les entr’elles, ces mêmes proportionelles l’étant auſſi, <lb />la ſomme de toutes ces puiſſances eſt à ce poids, com-<lb />me une de ces proportionelles à une partie de cette <lb />diagonale diviſée en autant d’égales qu’il y a de telles <lb />puiſſances; </s>
          <s xml:space="preserve">c’eſt-à-dire ici, comme laquelle que ce <lb />ſoit, des lignes CG, CR, CM, CN, CP, à {1/5} de <lb />CK.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">Pour exprimer le raport que nous venons de trouver <lb />entre ce poids &amp; </s>
          <s xml:space="preserve">les puiſſances qui le ſoutiennent, d’une <lb />maniére qui en rende le calcul plus facile, ſoit le Lemme <lb />ſuivant.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0134-01" />
          <label>0134-01</label>
        </figure>
        <pb facs="0135" n="109" />
        <fw type="head">DE M. BORELLI.</fw>
        <note xml:space="preserve" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſcu-<lb />lement.</note>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0135-01" />
          <label>0135-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">LEMME.</head>
        <p rend="italics">
          <s xml:space="preserve">DE quelque maniére que la ligne droite CP paſſe par <lb />
<ptr xml:id="note-0135-02a" corresp="note-0135-02" type="noteAnchor" />
une des pointes C du parallelogramme IE, ſi des trois <lb />autres pointes G, I, E, on tire ſur la même CP les trois <lb />perpendiculaires GL, IP, VE: </s>
          <s xml:space="preserve">ſa partie CL compriſe <lb />entre le point C, &amp; </s>
          <s xml:space="preserve">la perpendiculaire GL qui part de la <lb />pointe G qui lui eſt oppoſée, eſt toujours égale à la ſomme de <lb />ſes deux autres parties CP &amp; </s>
          <s xml:space="preserve">CV compriſes entre ce même <lb />point C &amp; </s>
          <s xml:space="preserve">les perpendiculaires IP &amp; </s>
          <s xml:space="preserve">EV, lors que ces <lb />deux perpendiculaires tombent du même côté de C; </s>
          <s xml:space="preserve">ou à la <lb />diffèrence de ces deux parties, lors que ces deux perpendiculaires <lb />tombent de différens côtez.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0135-02" corresp="note-0135-02a" place="margin">fig. 9. <lb />10. <lb />11. <lb />12. <lb />13. <lb />14. <lb />15. <lb />16.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration.</hi></head>
        <p>
          <s xml:space="preserve">Joignez IE &amp; </s>
          <s xml:space="preserve">GC qui ſe coupent par la moitié <lb />l’une &amp; </s>
          <s xml:space="preserve">l’autre en K, &amp; </s>
          <s xml:space="preserve">apres avoir fait QK perpen-<lb />diculaire à CP, concevez un plan qui paſſe par QK, <lb />à qui CP ſoit perpendiculaire, &amp; </s>
          <s xml:space="preserve">ſur lequel des <lb />points I &amp; </s>
          <s xml:space="preserve">E, tombent auſſi perpendiculairement <lb />IM, &amp; </s>
          <s xml:space="preserve">EN; </s>
          <s xml:space="preserve">Enfin joignez QM &amp; </s>
          <s xml:space="preserve">QN. </s>
          <s xml:space="preserve">Cela fait, <lb />ſoit que QK, QM, &amp; </s>
          <s xml:space="preserve">QN, ſe confondent en une <lb />ſeule ligne, ſoit qu’elles en faſſent trois différentes, <lb />il eſt clair que puis que les lignes IM, PQ, NE, &amp; </s>
          <s xml:space="preserve"><lb />VQ, ſont toutes (Hyp.) </s>
          <s xml:space="preserve">perpendiculaires à ce plan, <lb />elles ſont auſſi toutes paralleles entr’elles; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par <lb />conſéquent 1°. </s>
          <s xml:space="preserve">IM &amp; </s>
          <s xml:space="preserve">PQ ſont dans un même plan <lb />avec PI &amp; </s>
          <s xml:space="preserve">QM: </s>
          <s xml:space="preserve">Ainſi les angles en M, Q, &amp; </s>
          <s xml:space="preserve">P, <lb />étant (hyp) droits, MP ſera un parallelogramme. <lb /></s>
          <s xml:space="preserve">On prouvera de même que VN eſt auſſi un paralle-<lb />logramme: </s>
          <s xml:space="preserve">Donc IM eſt égale à PQ, &amp; </s>
          <s xml:space="preserve">EN égale <lb />à VQ. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">De ce que IM &amp; </s>
          <s xml:space="preserve">EN ſont paralleles en-
</s>
          <pb facs="0136" n="110" />
          <s xml:space="preserve"><fw type="head">EXAMEN DE L’OPINION</fw>
tr’elles, il ſuit auſſi que les angles MIK &amp; </s>
          <s xml:space="preserve">NEK <lb />
<ptr xml:id="note-0136-01a" corresp="note-0136-01" type="noteAnchor" />
ſont égaux; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent, ſi l’on joint KM &amp; </s>
          <s xml:space="preserve"><lb />KN, les angles en M &amp; </s>
          <s xml:space="preserve">en N étant (hyp.) </s>
          <s xml:space="preserve">égaux, <lb />auſſi-bien que les lignes IK &amp; </s>
          <s xml:space="preserve">KE, les triangles IMK <lb />&amp; </s>
          <s xml:space="preserve">ENK ſeront non ſeulement ſemblables, mais en-<lb />core IM ſera égale à EN. </s>
          <s xml:space="preserve">Or on vient de voir (n. </s>
          <s xml:space="preserve">1.) <lb /></s>
          <s xml:space="preserve">que IM eſt égale à PQ, &amp; </s>
          <s xml:space="preserve">EN égale à VQ: </s>
          <s xml:space="preserve"><lb />Donc PQ eſt égale à VQ: </s>
          <s xml:space="preserve">Donc (fig. </s>
          <s xml:space="preserve">9. </s>
          <s xml:space="preserve">11. </s>
          <s xml:space="preserve">12. </s>
          <s xml:space="preserve">13. </s>
          <s xml:space="preserve"><lb />&amp; </s>
          <s xml:space="preserve">14.) </s>
          <s xml:space="preserve">CP plus CV, ou ( fig. </s>
          <s xml:space="preserve">10. </s>
          <s xml:space="preserve">14. </s>
          <s xml:space="preserve">15. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">16.) </s>
          <s xml:space="preserve"><lb />CP moins CV, eſt égal à deux fois CQ. </s>
          <s xml:space="preserve">Or à cauſe <lb />que les triangles CGL, &amp; </s>
          <s xml:space="preserve">CKQ ſont ſemblables, &amp; </s>
          <s xml:space="preserve"><lb />que CG eſt double de CK; </s>
          <s xml:space="preserve">CL ſera auſſi double de <lb />CQ: </s>
          <s xml:space="preserve">Donc (fig. </s>
          <s xml:space="preserve">9. </s>
          <s xml:space="preserve">11. </s>
          <s xml:space="preserve">12. </s>
          <s xml:space="preserve">13. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">14.) </s>
          <s xml:space="preserve">CP plus CV, <lb />ou (fig. </s>
          <s xml:space="preserve">10. </s>
          <s xml:space="preserve">14. </s>
          <s xml:space="preserve">16. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">16.) </s>
          <s xml:space="preserve">CP moins CV, eſt égale <lb />à CL. </s>
          <s xml:space="preserve">Ce qu’il faloit dèmontrer.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0136-01" corresp="note-0136-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0136-01" />
          <label>0136-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">PROPOSITION III.</head>
        <p rend="italics">
          <s xml:space="preserve">T Outes choſes étant les mèmes que dans la propoſition <lb />
<ptr xml:id="note-0136-02a" corresp="note-0136-02" type="noteAnchor" />
précédente, on trouvera préſentement que chacune des <lb />puiſſances A, B, D, E, F, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">eſt au poids T qu’elles <lb />ſoutiennent, comme chacune de leurs proportionelles CG, CR, <lb />CM, CN, CP, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">à la ſomme de leurs ſublimitez moins <lb />celle de leurs profondeurs.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0136-02" corresp="note-0136-02a" place="margin">fig. 8. <lb />17.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration.</hi></head>
        <p>
          <s xml:space="preserve">De toutes les pointes des parallelogrammes GR, <lb />
<ptr xml:id="note-0136-03a" corresp="note-0136-03" type="noteAnchor" />
HM, LN, QP, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">tirez Gg, Hh, Rr, Ll, Mm, Qq, <lb />Nn, Pp, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">perpendiculairement ſur la ligne de di-<lb />rection du poids T, prolongée indéfiniment de part <lb />&amp; </s>
          <s xml:space="preserve">d’autre. </s>
          <s xml:space="preserve">Cela fait, vous trouverez par le Lemme <lb />précédent. </s>
          <s xml:space="preserve">1°. </s>
          <s xml:space="preserve">Ch = Cg Cr. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Cl = Cm -<lb />Ch: </s>
          <s xml:space="preserve">Donc Cl = Cm - Cg + Cr. </s>
          <s xml:space="preserve">3°. </s>
          <s xml:space="preserve">Cq =
</s>
          <pb facs="0137" n="111" />
          <s xml:space="preserve"><fw type="head">DE M. BORELLI.</fw>
Cl + Cn: </s>
          <s xml:space="preserve">Donc Cq = Cm - Cg + Cr + Cn. <lb /></s>
          <s xml:space="preserve">
<ptr xml:id="note-0137-01a" corresp="note-0137-01" type="noteAnchor" />
4°. </s>
          <s xml:space="preserve">Ck = Cq - Cp: </s>
          <s xml:space="preserve">Donc Ck = Cm - Cg + <lb />Cr + Cn - Cp. </s>
          <s xml:space="preserve">Enfin continuant toujours ainſi <lb />juſqu’à la diagonale qui ſetrouve toujours ( Prop. </s>
          <s xml:space="preserve">2.) <lb /></s>
          <s xml:space="preserve">dans la ligne de ditection du poids T, on trouvera <lb />de même que cette diagonale eſt toujours égale à <lb />Cm - Cg + Cr + Cn - Cp ± &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">Or on vient <lb />de voir ( Prop. </s>
          <s xml:space="preserve">2.) </s>
          <s xml:space="preserve">que chacune des puiſſances A, B, <lb />D, E, F, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">eſt auſſi toujours au poids T qu’elles <lb />ſoutiennent, comme chacune de leurs proportio-<lb />nelles CG, CR, CM, CN, CP, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">à cette même <lb />diagonale: </s>
          <s xml:space="preserve">Donc chacune de ces puiſſances eſt à ce <lb />poids, comme chacune de ces proportionelles à Cm + <lb />Cr + Cn - Cg - Cp ± &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">C’eſt-à-dire, ( Def. </s>
          <s xml:space="preserve"><lb />1. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">2.) </s>
          <s xml:space="preserve">à la ſomme de leurs ſublimitez Cm, Cr, <lb />Cn, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">moins la ſomme de leurs profondeurs Cg, <lb />Cp, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">D’où l’on voit en général, que de qu@lque <lb />maniére qu’un poids ſoit ſoutenu avec des cordes <lb />par quelque nombre de puiſſances que ce ſoit, appli-<lb />quées à un même nœud, chacune de ces puiſſances <lb />eſt toujours à ce poids, comme chacune de leurs pro-<lb />portionelles, à la ſomme de leurs ſublimitez moins <lb />celle de leurs profondeurs. </s>
          <s xml:space="preserve">Ce qu’il faloit démon-<lb />trer.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0136-03" corresp="note-0136-03a" place="margin">fig. 8.</note>
              <note xml:space="preserve" xml:id="note-0137-01" corresp="note-0137-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Autre</hi> <hi rend="small caps">Demonstration.</hi></head>
        <p>
          <s xml:space="preserve">Soient encore les lignes CG, CR, CM, CN, CP, <lb />&amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">proportionelles aux puiſſances A, B, D, E, F, <lb />
<ptr xml:id="note-0137-02a" corresp="note-0137-02" type="noteAnchor" />
&amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">proportionelles aux puiſſances A, B, D, E, F, <lb />&amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">concevez par le point C, où elles ſe communi-<lb />quent, un plan horizontal OH, c’eſt-à-dire, per-<lb />pendiculaire à la ligne de direction du poids T; </s>
          <s xml:space="preserve">tirez <lb />enſuite des extrémitez de ces proportionelles G, R, <lb />M, N, P, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">autant de perpendiculaires ſur le <lb />plan OH, &amp; </s>
          <s xml:space="preserve">ſur la ligne de direction du poids T <lb />indéfiniment prolongée de part &amp; </s>
          <s xml:space="preserve">d’autre: </s>
          <s xml:space="preserve">en faiſant
</s>
          <pb facs="0138" n="112" />
          <s xml:space="preserve"><fw type="head">EXAMEN DE L’OPINION</fw>
depuis C ſur le plan OH autant de lignes CH, CQ, <lb />
<ptr xml:id="note-0138-01a" corresp="note-0138-01" type="noteAnchor" />
CL, CO, CK, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">qui joignent ce point avec les <lb />perpendiculaires qui tombent ſur ce plan, on aura <lb />autant de parallelogrammes rectangles Hg, Qr, Lm, <lb />On, Kp, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">qui exprimeront ( Lemm 3. </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">2. </s>
          <s xml:space="preserve">du <lb />Projet précédent) que chacune de ces puiſſances, par <lb />exemple la puiſſance A, fait la même impreſſion ſur le <lb />point C, que feroient deux autres puiſſances appliquées <lb />à ce point, l’une ſuivant CH, &amp; </s>
          <s xml:space="preserve">l’autre ſuivant Cg, à <lb />chacune deſquelles celle-ci ſeroit comme @G à cha-<lb />cune de ces mêmes lignes: </s>
          <s xml:space="preserve">Le point C eſt donc tiré <lb />vers bas ſuivant la ligne de direction du poids T par <lb />la puiſſance A, d’une force (Cor. </s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve">du même Lemm) <lb />à qui cette puiſſance eſt comme CG à C@. </s>
          <s xml:space="preserve">Pour la <lb />même raiſon, il eſt encore tiré ſuivant la ligne de di-<lb />rection de même poids, 1°. </s>
          <s xml:space="preserve">Vers bas, par la puiſſance <lb />F, d’une force à qui elle eſt comme CP à Cp; </s>
          <s xml:space="preserve">&amp;</s>
          <s xml:space="preserve">c. <lb /></s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Vers haut, par la puiſſance B, d’une force à qui <lb />elle eſt comme CR à Cr; </s>
          <s xml:space="preserve">par la puiſſance D, d’une <lb />force à qui elle eſt comme CM à Cm; </s>
          <s xml:space="preserve">par la puiſſance <lb />E, d’une force à qui elle eſt, comme CN à Cn; </s>
          <s xml:space="preserve">&amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve"><lb />Or (hyp.) </s>
          <s xml:space="preserve">la puiſſance A eſt à chacune des puiſſances <lb />B, D, E, F, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">comme ſa proportionelle CG à cha-<lb />cune des leurs CR, CM, CN, CP, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">Donc la <lb />puiſſance A eſt à chacune des forces avec leſquelles <lb />le point C eſt tiré ſuivant la ligne de direction du <lb />poids T, 1°. </s>
          <s xml:space="preserve">Vers bas par les puiſſances A, F, <lb />&amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">comme CG à chacune de leurs profondeurs <lb />Cg, Cp, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Vers haut par les puiſſances <lb />B, D, E, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">comme la même CG à chacune de <lb />leurs ſublimitez Cr, Cm, Cn, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">Donc cette <lb />même puiſſance A eſt à la ſomme de toutes les forces <lb />avec leſquelles le point C eſt tiré ſuivant la ligne de <lb />direction du poids T, 1°. </s>
          <s xml:space="preserve">Vers bas par les puiſſances <lb />A, F, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">comme ſa proportionelle CG à la ſomme
</s>
          <pb facs="0139" n="113" />
          <s xml:space="preserve"><fw type="head">DE M. BORELLI.</fw>
de leurs profondeurs Cg, Cp, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Vers haut <lb />
<ptr xml:id="note-0139-01a" corresp="note-0139-01" type="noteAnchor" />
par les puiſſances B, D, E, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">comme la même CG <lb />à la ſomme de leurs ſublimitez Cr, Cm, Cn, &amp;</s>
          <s xml:space="preserve">c. <lb /></s>
          <s xml:space="preserve">Or la ſomme faite de la peſanteur de ce poids, &amp; </s>
          <s xml:space="preserve"><lb />des forces avec leſquelles le point C eſt tiré vers <lb />bas ſuivant la ligne de direction de ce même poids <lb />par les puiſſances A, F, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">étant diamétralement <lb />oppoſée à la ſomme de celles avec leſquelles ce même <lb />point eſt tiré en même-tems vers haut ſuivant cette <lb />même ligne par les puiſſances B, D, E, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">au-<lb />cune de ces deux ſommes de forces ne l’emportant <lb />ſur l’autre; </s>
          <s xml:space="preserve">puiſque (hyp.) </s>
          <s xml:space="preserve">le poids T ne monte n’y <lb />deſcend: </s>
          <s xml:space="preserve">c’eſt une conſéquence néceſſaire qu’elles <lb />ſoient égales: </s>
          <s xml:space="preserve">Donc la puiſſance A eſt non ſeulement <lb />à la ſomme des forces avec leſquelles le point C eſt <lb />tiré vers bas, ſuivant la ligne de direction du poids <lb />T par les puiſſances A, F, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">comme ſa propor-<lb />tionelle CG à la ſomme de leurs profondeurs Cg, <lb />Cp, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">Mais auſſi à la ſomme faite de cette pre-<lb />miére &amp; </s>
          <s xml:space="preserve">de la peſanteur de ce même poids, comme <lb />la même CG à la ſomme des ſublimitez Cr, Cm, <lb />Cn, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">des puiſſances B, D, E, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">Donc la puiſ-<lb />ſance A eſt à cette derniére ſomme moins la pre-<lb />miére; </s>
          <s xml:space="preserve">c’eſt-à-dire, à la peſanteur ſeule du poids <lb />T, où à ce poids lui - même, comme ſa proportio-<lb />nelle CG à la ſomme des ſublimitez Cr, Cm, Cn, <lb />&amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">moins la ſomme des profondeurs Cg, Cp, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve"><lb />Or ( Hyp.) </s>
          <s xml:space="preserve">chacune des puiſſances B, D, E, F, <lb />&amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">eſt à la puiſſance A, comme chacune de leurs <lb />proportionelles CR, CM, CN, CP, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">à ſa pro-<lb />portionelle CG: </s>
          <s xml:space="preserve">Donc chacune des puiſſances A, <lb />B, D, E, F, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">eſt au poids T qu’elles ſoutien-<lb />nent, comme chacune de leurs proportionelles à la <lb />ſomme de leurs ſublimitez moins celle de leurs pro-<lb />fondeurs. </s>
          <s xml:space="preserve">Ce qu’il faloit démontrer.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0137-02" corresp="note-0137-02a" place="margin">fig. 17.</note>
              <note xml:space="preserve" xml:id="note-0138-01" corresp="note-0138-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
              <note xml:space="preserve" xml:id="note-0139-01" corresp="note-0139-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <pb facs="0140" n="114" />
        <fw type="head">EXAMEN DE L’OPINION</fw>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire.</hi></head>
        <note xml:space="preserve" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
        <p>
          <s xml:space="preserve">On voit préſentement en général que la ſomme <lb />de toutes les puiſſances qui ſoutiennent un poids <lb />avec des cordes qui ſe tiennent par un même nœud, <lb />en quelque nombre qu’elles ſoient, quelque pro-<lb />portion qu’elles ayent entr’elles, &amp; </s>
          <s xml:space="preserve">de quelque ma-<lb />niére qu’elles lui ſoient appliquées; </s>
          <s xml:space="preserve">eſt toujours à <lb />ce poids, comme la ſomme des parties de leurs cor-<lb />des qui leurs ſont (Chap. </s>
          <s xml:space="preserve">2. </s>
          <s xml:space="preserve">Avert ) proportionelles, <lb />à la ſomme de leurs ſublimitez moins celle de leurs <lb />profondeurs.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">On peut comparer tout ceci avec les Propoſitions 70. </s>
          <s xml:space="preserve">73. <lb /></s>
          <s xml:space="preserve">74. </s>
          <s xml:space="preserve">de M. </s>
          <s xml:space="preserve">Borelli, &amp; </s>
          <s xml:space="preserve">on verra non ſeulement qu’elles ſont <lb />tres-limitées; </s>
          <s xml:space="preserve">mais encore qu’avec ſa méthode on ne peut pas <lb />aller ſi loin.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Remarque.</hi></head>
        <p>
          <s xml:space="preserve">En faiſant la ſeconde des deux démonſtrations <lb />précédentes, il m’en eſt encore venu une de la pre-<lb />miére Propoſition: </s>
          <s xml:space="preserve">la voici.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">Le poids T étant donc ſoutenu avec des cordes par deux <lb />puiſſances R &amp; </s>
          <s xml:space="preserve">S; </s>
          <s xml:space="preserve">des angles G &amp; </s>
          <s xml:space="preserve">H du parallelogramme <lb />
<ptr xml:id="note-0140-02a" corresp="note-0140-02" type="noteAnchor" />
GH, dont la diagonale CD fait partie de la ligne de di-<lb />rection de ce poids, ſoient faites GM &amp; </s>
          <s xml:space="preserve">HN paralleles à <lb />cette diagonale, &amp; </s>
          <s xml:space="preserve">perpendiculaires à MCN; </s>
          <s xml:space="preserve">achevez <lb />les parallelogrammes MP &amp; </s>
          <s xml:space="preserve">NQ. </s>
          <s xml:space="preserve">Cela fait, vous trou-<lb />verez encore de la maniére que nous avons fait la ſeconde <lb />des deux démonſtrations précédentes, que le poids T eſt aux <lb />puiſſances R &amp; </s>
          <s xml:space="preserve">S, comme la partie CD de ſa ligne de di-<lb />rection aux parties CG &amp; </s>
          <s xml:space="preserve">CH de leurs cordes, qui font <lb />les côtez du parallelogramme GH, dont elle eſt diagonale.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0140-02" corresp="note-0140-02a" place="margin">fig. 18. <lb />19.</note>
            </div>
          </body>
        </floatingText>
        <pb facs="0141" n="115" />
        <fw type="head">DE M. BORELLI.</fw>
        <p>
          <s xml:space="preserve">Car (Cor. </s>
          <s xml:space="preserve">2. </s>
          <s xml:space="preserve">Lem. </s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve">du Projet précéd.) </s>
          <s xml:space="preserve">la puiſſance <lb />
<ptr xml:id="note-0141-01a" corresp="note-0141-01" type="noteAnchor" />
R fait ſur le point C la même impreſſion que fe-<lb />roient deux autres puiſſances appliquées à ce point, <lb />l’une ſuivant CP, &amp; </s>
          <s xml:space="preserve">l’autre ſuivant CM, à chacune <lb />deſquelles celle-ci ſeroit, comme CG à chacune de <lb />ces lignes: </s>
          <s xml:space="preserve">Le point C reçoit donc en même - tems <lb />deux impreſſions différentes de la puiſſance R, l’une <lb />ſuivant CP, d’une force qui eſt à celle de cette puiſ-<lb />ſance, (Cor. </s>
          <s xml:space="preserve">3. </s>
          <s xml:space="preserve">du même Lemm.) </s>
          <s xml:space="preserve">comme CP à CG, &amp; </s>
          <s xml:space="preserve"><lb />l’autre ſuivant CM, d’une force qui eſt auſſi (par le <lb />mème Cor.) </s>
          <s xml:space="preserve">à celle de cette même puiſſance, comme CM <lb />à CG. </s>
          <s xml:space="preserve">Pour la même raiſon ce même point C reçoit <lb />encore en même - tems deux impreſſions différentes <lb />de la puiſſance S, l’une ſuivant CQ, d’une force <lb />qui eſt à celle de cette puiſſance, comme CQ à CH; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve"><lb />l’autre ſuivant CN, d’une force qui eſt auſſi à celle de <lb />cette même puiſſance, comme CN à CH. </s>
          <s xml:space="preserve">Or 1°. </s>
          <s xml:space="preserve">La <lb />force de l’impreſſion que reçoit le point C de la puiſ-<lb />ſance R ſuivant CM, eſt égale à celle qu’il reçoit <lb />en même - tems de la puiſſance S ſuivant CN; </s>
          <s xml:space="preserve">puis <lb />qu’elles ſont diamétralement oppoſées, &amp; </s>
          <s xml:space="preserve">qu’aucu-<lb />ne des deux (byp.) </s>
          <s xml:space="preserve">ne ſurmonte l’autre: </s>
          <s xml:space="preserve">La force <lb />de la puiſſance R eſt donc à celle de l’impreſſion que <lb />reçoit le point C de la puiſſance S ſuivant CN, com-<lb />me CG à CM. </s>
          <s xml:space="preserve">Or CM eſt égale à CN; </s>
          <s xml:space="preserve">puis que <lb />les triangles GPD &amp; </s>
          <s xml:space="preserve">HQC ſemblables, &amp; </s>
          <s xml:space="preserve">GD <lb />égale à CH rendent GP égale à HQ; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">que les <lb />parallelogrammes MP &amp; </s>
          <s xml:space="preserve">NQ rendent auſſi GP <lb />égale à CM, &amp; </s>
          <s xml:space="preserve">HQ égale à CN: </s>
          <s xml:space="preserve">Donc la puiſſance <lb />R eſt à la force de l’impreſſion que le point C reçoit <lb />de la puiſſance S ſuivant CN, comme CG à CN. <lb /></s>
          <s xml:space="preserve">Or on vient de voir que la force de cette même im-<lb />preſſion eſt à la puiſſance S, comme CN à CH: </s>
          <s xml:space="preserve"><lb />Donc la puiſſance R eſt à la puiſſance S, comme <lb />CG à CH: </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">On vient de voir auſſi que la puiſſan-
</s>
          <pb facs="0142" n="116" />
          <s xml:space="preserve"><fw type="head">EXAMEN DE L’OPINION</fw>
ce S eſt à la force de l’impreſſion qu’elle fait ſur le <lb />
<ptr xml:id="note-0142-01a" corresp="note-0142-01" type="noteAnchor" />
point C ſuivant CQ, comme CH à CQ: </s>
          <s xml:space="preserve">Donc la <lb />puiſſance R eſt auſſi à la force de cette même im-<lb />preſſion, comme CG à CQ; </s>
          <s xml:space="preserve">c’eſt - à - dire, comme <lb />CG à DP; </s>
          <s xml:space="preserve">puis que les triangles GPD &amp; </s>
          <s xml:space="preserve">HQC <lb />ſemblables, &amp; </s>
          <s xml:space="preserve">GD égale à CH, rendent DP égale <lb />à CQ. </s>
          <s xml:space="preserve">On vient de voir encore que cette même <lb />puiſſance R eſt à la force de l’impreſſion qu’elle fait <lb />ſur ce même point C ſuivant CP, comme CG à CP: <lb /></s>
          <s xml:space="preserve">Donc la puiſſance R eſt à la ſomme, où à la diffé-<lb />rence des forces de ces deux impreſſions faites ſur <lb />le point C ſuivant CP &amp; </s>
          <s xml:space="preserve">CQ, par elle &amp; </s>
          <s xml:space="preserve">par la puiſ-<lb />ſance S, comme CG à la ſomme, où à la différence <lb />de ces deux lignes. </s>
          <s xml:space="preserve">Or (fig. </s>
          <s xml:space="preserve">18.) </s>
          <s xml:space="preserve">la ſomme de ces <lb />deux lignes, où (fig. </s>
          <s xml:space="preserve">19.) </s>
          <s xml:space="preserve">leur différence, eſt égale <lb />à la diagonale CD du parallelogramme GH; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve"><lb />(fig. </s>
          <s xml:space="preserve">18.) </s>
          <s xml:space="preserve">la ſomme, où (fig. </s>
          <s xml:space="preserve">19.) </s>
          <s xml:space="preserve">la différence des <lb />forces de ces deux impreſſions, eſt auſſi égale au <lb />poids T: </s>
          <s xml:space="preserve">Donc la puiſſance R eſt au poids T, com-<lb />me CG à CD: </s>
          <s xml:space="preserve">On vient de démontrer (n. </s>
          <s xml:space="preserve">1.) </s>
          <s xml:space="preserve">que <lb />cettemême puiſſance R eſt auſſi à la puiſſance S, com-<lb />me CG à CH: </s>
          <s xml:space="preserve">Donc les puiſſances R &amp; </s>
          <s xml:space="preserve">S, &amp; </s>
          <s xml:space="preserve">le <lb />poids T ſont entr’eux , comme les lignes CG, CH, <lb />&amp; </s>
          <s xml:space="preserve">CD: </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par conſéquent ce poids eſt à chacune <lb />d’elles, comme la partie CD de ſa ligne de direction <lb />à chacune des parties de leurs cordes, qui font les <lb />côtez du parallelogramme GH, dont elle eſt diago-<lb />nale. </s>
          <s xml:space="preserve">Ce qu’il faloit démontrer.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0141-01" corresp="note-0141-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement</note>
              <note xml:space="preserve" xml:id="note-0142-01" corresp="note-0142-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">On voit de-là, que ſi par le point C où ſe com-<lb />muniquent les deux cordes qui ſoutiennent quel-<lb />que poids que ce ſoit, on fait MN perpendiculaire à <lb />la ligne de direction de ce poids, &amp; </s>
          <s xml:space="preserve">qu’aprés avoir pris <lb />de part &amp; </s>
          <s xml:space="preserve">d’autre ſur cette ligne CM &amp; </s>
          <s xml:space="preserve">CN ègales en-<lb />tr’elles, on faſſe aux points M &amp; </s>
          <s xml:space="preserve">N les perpendiculaires
</s>
          <pb facs="0143" n="117" />
          <s xml:space="preserve"><fw type="head">DE M. BORELLI.</fw>
MG &amp; </s>
          <s xml:space="preserve">NH qui rencontrent auxpoints G &amp; </s>
          <s xml:space="preserve">H les <lb />
<ptr xml:id="note-0143-01a" corresp="note-0143-01" type="noteAnchor" />
cordes des puiſſances qui ſoutiennent ce poids: </s>
          <s xml:space="preserve">elles <lb />en détermineront des parties CG, CH, qui ſeront <lb />toujours proportionelles à ces mêmes puiſſances.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0143-01" corresp="note-0143-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <p rend="italics">
          <s xml:space="preserve">Si M. </s>
          <s xml:space="preserve">Borelli eut fait rèflèxion que les puiſſances R &amp; </s>
          <s xml:space="preserve"><lb />S n’agiſſent pas ſeulement contre le poids T, mais auſſi <lb />l’une contre l’autre ; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">que de même qu’elles concourent en-<lb />ſemble pour empêcber que ce poids n’attire à lui (fig. </s>
          <s xml:space="preserve">18.) <lb /></s>
          <s xml:space="preserve">le nœud C, de même auſſi cbacune d’elles concourt avec <lb />lui pour empêcber que l’autre ne l’emporte. </s>
          <s xml:space="preserve">Si, dî - je, il avoit <lb />fait cette rèfléxion, il auroit vû ſans doute que chacune. </s>
          <s xml:space="preserve">de <lb />ces puiſſances fait impreſſion ſur ce nœud, non ſeulement <lb />ſuivant la direction du poids qu’elles ſoutiennent, pour le <lb />tenir toujours à même hauteur; </s>
          <s xml:space="preserve">mais auſſi ſuivant l’hori-<lb />zontale MCN, pour empêcher qu’aucune d’elles ne l’attire <lb />n’y à droit, n’y à gaucbe: </s>
          <s xml:space="preserve">D'où il auroit infailliblement conclu <lb />que ces impreſſions horizontales, ètant diamétralement <lb />oppoſées, doivent toujours être égales. </s>
          <s xml:space="preserve">De-là voyant qu’el-<lb />les augmentent, où diminuent néceſſairement à meſure que <lb />les angles que font les cordes de ces puiſſances avec la ligne <lb />de direction du poids qu’elles ſoutiennent, s’aprochent, où <lb />s’éloignent de l’angle droit, il auroit enfin aperçû l’impoſſibi-<lb />litè de faire, finon aucun, du moins un tel changement à leurs <lb />d. </s>
          <s xml:space="preserve">rections ſans en rompre l’équilibre.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">@e dis ſinon aucun changement, parce qu’il a été <lb />démontré (Cor. </s>
          <s xml:space="preserve">1. </s>
          <s xml:space="preserve">Prop. </s>
          <s xml:space="preserve">1.) </s>
          <s xml:space="preserve">qu’il n’eſt pas poſſible d’y <lb />en faire aucun ſans rompre l’équilibre qui eſt (hyp.) </s>
          <s xml:space="preserve">entre <lb />ces puiſſances, &amp; </s>
          <s xml:space="preserve">le poids qu’elles ſoutiennent. </s>
          <s xml:space="preserve">Nous <lb />l’avons même conclu (Chap. </s>
          <s xml:space="preserve">1.) </s>
          <s xml:space="preserve">de la 68. </s>
          <s xml:space="preserve">Prop. </s>
          <s xml:space="preserve">d’où cet <lb />Autheur tire un ſcbolie tout contraire par un raiſonnement dont <lb />le défaut eſt préſentement aiſé à découvrir; </s>
          <s xml:space="preserve">Voyez-le.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">Sur ce qu’on vient de dire de l’uſage des impreſſions hori-
</s>
          <pb facs="0144" n="118" />
          <s xml:space="preserve"><fw type="head">EXAMEN DE L’OPINION</fw>
zontales que font ſur le nœud C (fig. </s>
          <s xml:space="preserve">18. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">19.) </s>
          <s xml:space="preserve">les puiſſan-<lb />
<ptr xml:id="note-0144-01a" corresp="note-0144-01" type="noteAnchor" />
ces R &amp; </s>
          <s xml:space="preserve">S, il eſt aiſé de juger de celui des impreſſions ſem-<lb />blables que font auſſi ſur le nœud C de leurs cordes ſuivant <lb />le plan OH (fig. </s>
          <s xml:space="preserve">17.) </s>
          <s xml:space="preserve">les puiſſances A, B, D, E, F, <lb />&amp; </s>
          <s xml:space="preserve">C. </s>
          <s xml:space="preserve">auſſi ne s’y arrêtera-t-on pas davantage.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0144-01" corresp="note-0144-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0144-01" />
          <label>0144-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">PROPOSITION IV.</head>
        <p rend="italics">
          <s xml:space="preserve">DE quelque maniére qu’un poids ſoit ſoutenu avec des <lb />cordes par quelque nombre de puiſſances que ce ſoit, <lb />appliquées à tant de nœuds qu’on voudra; </s>
          <s xml:space="preserve">chacune d’elles eſt <lb />toujours à ce poids en raiſon compoſée d’autant d’autres raiſons <lb />qu’il y a de nœuds entre cette puiſſance &amp; </s>
          <s xml:space="preserve">ce poids: </s>
          <s xml:space="preserve">Sçavoir <lb />par chaque nœud, de la raiſon qui eſt entre la proportionelle <lb />à la force dont ce nœud eſt tiré ſuivant la corde qui lui donne <lb />communication avec cette puiſſance, &amp; </s>
          <s xml:space="preserve">la ſomme des ſu-<lb />blimitez moins celle des profondeurs de toutes les forces dont <lb />les branches dans leſquelles ce même nœud ſe diviſe, ſont <lb />tirèes chacune ſuivant ſa direction contre la réſiſtance qui leur <lb />vient par la corde de communication de lui à ce poids.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Demonstration</hi>.</head>
        <p>
          <s xml:space="preserve">Soit le poids T dont la corde C p ſe diviſe en tant <lb />
<ptr xml:id="note-0144-02a" corresp="note-0144-02" type="noteAnchor" />
de branches CZ, CX, CY, Cφ, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">qu’on vou-<lb />dra, dont celles qu’on voudra, ſe diviſent encore <lb />en pluſieurs branches, &amp; </s>
          <s xml:space="preserve">celles qu’on voudra encore <lb />de celles-ci en pluſieurs autres de la maniére qu’on <lb />voit ici; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">toujours de même juſqu’auſſi loin qu’on <lb />voudra. </s>
          <s xml:space="preserve">Commencez au premier nœud C à marquer <lb />ſur les branches CZ, XC, YC, Cφ, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">des parties <lb />CM, CN, CP, Cθ, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">qui ſoient entr’elles com-<lb />me les forces avec leſquelles ces cordes ſont tirées <lb />chacune ſuivant ſa direction. </s>
          <s xml:space="preserve">Faites - en autant ſur
</s>
          <pb facs="0145" n="119" />
          <s xml:space="preserve"><fw type="head">DE M. BORELLI</fw>
les branches dans leſquelles celles-ci ſe ſubdiviſent; <lb /></s>
          <s xml:space="preserve">
<ptr xml:id="note-0145-01a" corresp="note-0145-01" type="noteAnchor" />
&amp; </s>
          <s xml:space="preserve">toujours de même juſqu’aux derniéres auſquelles <lb />les puiſſances A, E, D, B, F, G, H, I, K, φ, &amp;</s>
          <s xml:space="preserve">c. <lb /></s>
          <s xml:space="preserve">ſont appliquées. </s>
          <s xml:space="preserve">Cela fait, aprés avoir marqué des <lb />extrémitez de toutes ces proportionelles (Avertiſſ. </s>
          <s xml:space="preserve"><lb />Chap. </s>
          <s xml:space="preserve">2.) </s>
          <s xml:space="preserve">les ſublimitez &amp; </s>
          <s xml:space="preserve">les profondeurs de toutes <lb />ces forces, on trouvera que chacune de ces puiſ-<lb />ſances, par exemple, la puiſſance D eſt toujours à <lb />ce poids en raiſon compoſée d’autant d’autres rai-<lb />ſons telles que cette propoſition porte, qu’il y a de <lb />nœuds entre cette puiſſance &amp; </s>
          <s xml:space="preserve">lui: </s>
          <s xml:space="preserve">Car 1°. </s>
          <s xml:space="preserve">La puiſ-<lb />ſance D étant (hyp) à la puiſſance E, comme O S <lb />à OV.</s>
          <s xml:space="preserve">, elle eſt auſſi (Prop. </s>
          <s xml:space="preserve">3.) </s>
          <s xml:space="preserve">à la force dont<unclear reason="illegible" /> le <lb />nœud O leur réſiſte ſuivant OZ, comme OS à la <lb />ſomme de leurs ſublimitez O ſ &amp; </s>
          <s xml:space="preserve">O u. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Cette <lb />même force étant auſſi (hyp.) </s>
          <s xml:space="preserve">aux puiſſances A &amp; </s>
          <s xml:space="preserve">B, <lb />comme ZR à ZL &amp; </s>
          <s xml:space="preserve">ZQ, elle eſt de méme (Prop. </s>
          <s xml:space="preserve"><lb />3.) </s>
          <s xml:space="preserve">à la réſiſtance que leur fait le nœud Z ſuivant <lb />Z C, comme Z R à la ſomme des ſublimitez Z r &amp; </s>
          <s xml:space="preserve"><lb />Z q moins la profondeur Z l. </s>
          <s xml:space="preserve">3°. </s>
          <s xml:space="preserve">Enfin la valeur <lb />de cette réſiſtance étant encore (hyp.) </s>
          <s xml:space="preserve">aux forces <lb />dont le nœud C eſt tiré ſuivant C X, C Y, C φ. </s>
          <s xml:space="preserve">&amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve"><lb />comme CM à CN, CP, C θ, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">elle eſt auſſi <lb />(Prop. </s>
          <s xml:space="preserve">3.) </s>
          <s xml:space="preserve">au poids T, comme CM à la ſomme des <lb />ſublimitez C m, C n, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">moins celle des profondeurs <lb />Cλ, C p, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">Donc en multipliant par ordre ces <lb />trois rangées de proportionelles, la puiſſance D ſe <lb />trouvera au poids T, comme le produit fait des <lb />trois antécédens OS, ZR, &amp; </s>
          <s xml:space="preserve">CM, au produit fait <lb />de leur trois conſéquens Oſ + Ou, Zr + Zq -<lb />Zl, &amp; </s>
          <s xml:space="preserve">Cm + Cn - Cp - Cλ. </s>
          <s xml:space="preserve">C’eſt - à - dire, en <lb />raiſon compoſée des trois raiſons de OS à Oſ + <lb />Ou, de Z R à Zr + Zq - Zl, &amp; </s>
          <s xml:space="preserve">de CM à Cm + <lb />Cn - Cp - Cλ, qu’on voit telles que cette pro-<lb />poſition porte. </s>
          <s xml:space="preserve">Or il n’y a en eſfet que trois nœuds
</s>
          <pb facs="0146" n="120" />
          <s xml:space="preserve"><fw type="head">EXAMEN DE L’OPINION</fw>
O, Z, &amp; </s>
          <s xml:space="preserve">C, entre cette puiſſance &amp; </s>
          <s xml:space="preserve">ce poids: </s>
          <s xml:space="preserve">Donc <lb />
<ptr xml:id="note-0146-01a" corresp="note-0146-01" type="noteAnchor" />
la puiſſance D eſt au poids T en raiſon compoſée <lb />d’autant d’autres raiſons telles que cette propoſition <lb />porte, qu’il y a de nœuds entre cette puiſſance &amp; </s>
          <s xml:space="preserve"><lb />ce poids. </s>
          <s xml:space="preserve">On prouvera de même que la puiſſance A <lb />eſt à ce poids en raiſon compoſée de ZL à Z r + <lb />Z q - Zl, &amp; </s>
          <s xml:space="preserve">de CM à C m + C n - C p - C λ. <lb /></s>
          <s xml:space="preserve">On trouvera encore de même que la puiſſance F <lb />eſt à ce même poids en raiſon compoſée de X β à <lb />X b + X f, &amp; </s>
          <s xml:space="preserve">de CN à C m + C n - C p - C λ; </s>
          <s xml:space="preserve"><lb />&amp; </s>
          <s xml:space="preserve">ainſi de toutes les autres puiſſances, en quelque <lb />nombre qu’elles ſoient, de quelque maniére, &amp; </s>
          <s xml:space="preserve">à <lb />quelque nombre de nœuds qu’elles ſoient appli-<lb />quées. </s>
          <s xml:space="preserve">D’où l’on voit en général, que de quelque <lb />maniére qu’un poids ſoit ſoutenu avec des cordes <lb />par quelque nombre de puiſſances que ce ſoit, ap-<lb />pliquées à tant de nœuds qu’on voudra, chacune <lb />d’elles eſt toujours à ce poids en raiſon compoſée <lb />d’autant d’autres telles que cette propoſition porte, <lb />qu’il y a de nœuds entre cette puiſſance &amp; </s>
          <s xml:space="preserve">ce poids. </s>
          <s xml:space="preserve"><lb />Ce qu’il faloit démontrer.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0144-02" corresp="note-0144-02a" place="margin">fig. 20.</note>
              <note xml:space="preserve" xml:id="note-0145-01" corresp="note-0145-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
              <note xml:space="preserve" xml:id="note-0146-01" corresp="note-0146-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> I.</head>
        <p>
          <s xml:space="preserve">On voit qu’en prenant ZR égale à O ſ + O u, <lb />avec ZL &amp; </s>
          <s xml:space="preserve">ZQ à ZR en même proportion qu’elles <lb />ſont ici; </s>
          <s xml:space="preserve">de plus CM égale à Zq + Zr - Zl, <lb />avec CN, CP, Cθ, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">auſſi à CM en même <lb />proportion qu’elles ſont ici; </s>
          <s xml:space="preserve">la puiſſance D ſera au <lb />poids T, comme OS à Cm + Cn - Cλ - Cp ±<unclear reason="illegible" /> <lb />&amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">c’eſt-à-dire, comme ſa proportionelle à la ſomme <lb />des ſublimitez moins celle des profondeurs des for-<lb />ces avec leſquelles les branches du premier nœud <lb />C ſont tirées chacune ſuivant ſa direction. </s>
          <s xml:space="preserve">Il en faut <lb />penſer autant de toutes les autres puiſſances appli-<lb />quées au poids T, ſoit de prés, ſoit de loin.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0147" n="121" />
        <fw type="head">DE M. BORELLI.</fw>
        <p rend="italics">
          <s xml:space="preserve">On peut comparer cette propoſition avec ce Corollaire à la <lb />
<ptr xml:id="note-0147-01a" corresp="note-0147-01" type="noteAnchor" />
propoſition 78. </s>
          <s xml:space="preserve">de M. </s>
          <s xml:space="preserve">Borelli.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0147-01" corresp="note-0147-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> II.</head>
        <p>
          <s xml:space="preserve">Lors qu’un poids attaché à une corde qui a plu-<lb />
<ptr xml:id="note-0147-02a" corresp="note-0147-02" type="noteAnchor" />
ſieurs nœuds par chacun deſquels, entre toutes <lb />les branches qui en naiſſent, il n’y en a qu’une qui <lb />ſe ſubdiviſe en d’autres branches: </s>
          <s xml:space="preserve">lors dî-je que le <lb />poids T attaché à une telle corde, eſt ſoutenu par <lb />pluſieurs puiſſances Y, X, S, R, V, Z, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">telle-<lb />ment appliquées aux derniéres de ces branches que <lb />tous les nœuds F, E, C, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">d’où elles naiſſent, ſe <lb />trouvent dans la ligne de direction de ce poids; <lb /></s>
          <s xml:space="preserve">chacune de ces puiſſances, en quelque nombre qu’el-<lb />les ſoient, eſt toujours à ce poids, comme la pro-<lb />portionelle de cette même puiſſance à la ſomme des <lb />ſublimitez moins celle des profondeurs de tout ce <lb />qu’il y en a d’appliquées à ce même poids: </s>
          <s xml:space="preserve">car ſi l’on <lb />prend ſur les branches de chaque nœud des parties <lb />OF, EI, CB, CA, EH, FK, FN, EM, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve"><lb />proportionelles aux forces avec leſquelles chacune <lb />d’elles eſt tirée ſuivant ſa direction, &amp; </s>
          <s xml:space="preserve">que des ex-<lb />trémitez de ces mêmes parties on marque (avert. </s>
          <s xml:space="preserve"><lb />Chap. </s>
          <s xml:space="preserve">2.) </s>
          <s xml:space="preserve">leurs ſublimitez avec leurs profondeurs; </s>
          <s xml:space="preserve"><lb />on trouvera 1°. </s>
          <s xml:space="preserve">que les proportionelles FN, EM, <lb />&amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">qui ſe trouvent dans la ligne de direction de ce <lb />poids, ſont égales aux ſublimitez FN, FM, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">des <lb />forces avec leſquelles elles ſont tirées ſuivant leur <lb />direction, c’eſt-à-dire, ſuivant cette même ligne. </s>
          <s xml:space="preserve"><lb />2°. </s>
          <s xml:space="preserve">On trouvera encore que chacune de ces mêmes <lb />proportionelles, par exemple FN eſt auſſi toujours <lb />égale à la ſomme des ſublimitez moins celle des pro-<lb />fondeurs des forces, ou des puiſſances appliquées au
</s>
          <pb facs="0148" n="122" />
          <s xml:space="preserve"><fw type="head">EXAMEN DE L’OPINION</fw>
nœud E qui eſt immédiatement au-deſſus du nœud <lb />
<ptr xml:id="note-0148-01a" corresp="note-0148-01" type="noteAnchor" />
F depuis lequel cette proportionelle a été priſe: <lb /></s>
          <s xml:space="preserve">puis que (hyp) cette même proportionelle, &amp; </s>
          <s xml:space="preserve">(Prop. </s>
          <s xml:space="preserve"><lb />3.) </s>
          <s xml:space="preserve">cette même ſomme ſont à la proportionelle EI <lb />de la puiſſance X, comme la force dont le nœud E <lb />eſt tire ſuivant la corde EF, eſt à cette même puiſſan-<lb />ce. </s>
          <s xml:space="preserve">Pour la même raiſon EM eſt égale à la ſomme <lb />des ſublimitez moins celle des profondeurs des forces <lb />où des puiſſances appliquées au nœud C qui eſt im-<lb />médiatement au-deſſus de E; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">ainſi des autres <lb />proportionelles qui ſe trouvent dans la ligne de di-<lb />rection du poids T. </s>
          <s xml:space="preserve">De-là on verra que chacune des <lb />ſublimitez FN, EM, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">des forces qui ſuivent la direc-<lb />tion de ce poids, eſt toujours égale à la ſomme des ſu-<lb />blimitez moins celle des profondeurs des forces, ou <lb />des puiſſances appliquées au nœud qui eſt immédia-<lb />tement au-deſſus de celui depuis lequel elle ſe prend: </s>
          <s xml:space="preserve"><lb />D’où il ſuit que la ſublimité FN qui ſe prend depuis <lb />le plus bas de tous ces nœuds, eſt égale à la ſomme <lb />des ſublimitez moins celle des profondeurs de toutes <lb />les puiſſances X, V, S, R, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">appliquées à tous <lb />les autres nœuds E, C, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">Or on vient de voir <lb />dans le Corollaire précédent que chacune de toutes <lb />les puiſſances qui ſoutiennent le poids T, par exem-<lb />ple S, ou Y, eſt à ce poids, comme ſa proportio-<lb />nelle CB, ou OF à la ſomme des ſublimitez moins <lb />celle des profondeurs des forces avec leſquelles <lb />toutes les branches du plus bas nœud F ſont tirées <lb />chacune ſuivant ſa direction contre le poids T; </s>
          <s xml:space="preserve"><lb />c’eſt-à-dire, à la ſomme faite de la ſublimité FN, <lb />&amp; </s>
          <s xml:space="preserve">de la ſomme des ſublimitez moins les profondeurs <lb />des puiſſances Y, Z, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">immédiatement appliquées <lb />au nœud F: </s>
          <s xml:space="preserve">Donc chacune des puiſſances Y, X, S, <lb />R, V, Z, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">eſt en ce cas au poids T, comme ſa
</s>
          <pb facs="0149" n="123" />
          <s xml:space="preserve"><fw type="head">DE M. BORELLI.</fw>
proportionelle à la ſomme des ſublimitez, moins celle <lb />
<ptr xml:id="note-0149-01a" corresp="note-0149-01" type="noteAnchor" />
des profondeurs de tout ce qu’il y en a d’appliquées <lb />à ce même poids.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0147-02" corresp="note-0147-02a" place="margin">fig. 21. <lb />22.</note>
              <note xml:space="preserve" xml:id="note-0148-01" corresp="note-0148-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
              <note xml:space="preserve" xml:id="note-0149-01" corresp="note-0149-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> III.</head>
        <p>
          <s xml:space="preserve">D’où l’on voit que la ſomme de toutes ces puiſ-<lb />ſances eſt à ce poids, comme la ſomme de leurs pro-<lb />portionelles à la ſomme de leurs ſublimitez moins <lb />celle de leurs profondeurs: </s>
          <s xml:space="preserve">De ſorte que s’il n’y <lb />en avoit que deux d’appliquées à chaque nœud <lb />dont l’une tirât à droit &amp; </s>
          <s xml:space="preserve">l’autre à gauche, &amp; </s>
          <s xml:space="preserve">que <lb />toutes celles de chaque côté fuſſent égales entr’elles, <lb />&amp; </s>
          <s xml:space="preserve">avec des directions paralleles entr’elles; </s>
          <s xml:space="preserve">la ſomme <lb />(fig. </s>
          <s xml:space="preserve">21.) </s>
          <s xml:space="preserve">des ſublimitez, par exemple F o, + F k, où <lb />Ei + Eh, où Cb + Ca, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">des deux puiſſances ap-<lb />pliquées au quel que ce ſoit des nœuds F, E, C, &amp;</s>
          <s xml:space="preserve">c. <lb /></s>
          <s xml:space="preserve">ou bien la différence (fig. </s>
          <s xml:space="preserve">22.) </s>
          <s xml:space="preserve">de la ſublimité de l’une <lb />à la profondeur de l’autre, par exemple Fk,- Fo, <lb />ou Eh - Ei, au Ca - Cb, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">étant alors la même <lb />pour tous ces nœuds, auſſi-bien que les proportio-<lb />nelles de ces puiſſances; </s>
          <s xml:space="preserve">la ſomme de ces mêmes <lb />puiſſances ſeroit alors au poids T, comme la ſomme <lb />des proportionelles de deux d’entr’elles appliquées à un <lb />même nœud, quel qu’il ſoit, eſt à la ſomme (fig. </s>
          <s xml:space="preserve">21.) </s>
          <s xml:space="preserve"><lb />des ſublimitez de ces deux puiſſances, où (fig. </s>
          <s xml:space="preserve">22.) </s>
          <s xml:space="preserve">à la <lb />différence qui eſt entre la ſublimité de l’une, &amp; </s>
          <s xml:space="preserve">la <lb />profondeur del ’autre.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> IV.</head>
        <p>
          <s xml:space="preserve">Ce qui fait enfin voir que ſi toutes les puiſſances <lb />Y, X, S, R, V, Z, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">étoient égales entr’elles, &amp; </s>
          <s xml:space="preserve"><lb />que toutes leurs directions fiſſent avec celle de ce <lb />poids des angles égaux auſſi entr’eux, leur ſomme <lb />ſeroit alors à ce même poids, (fig. </s>
          <s xml:space="preserve">21.) </s>
          <s xml:space="preserve">comme une <lb />de leurs proportionelles à une de leurs ſublimitez,
</s>
          <pb facs="0150" n="124" />
          <s xml:space="preserve"><fw type="head">EXAMEN DE L’OPINION</fw>
l’une &amp; </s>
          <s xml:space="preserve">l’autre choiſie à diſcretion; </s>
          <s xml:space="preserve">c’eſt - à - dire, <lb />
<ptr xml:id="note-0150-01a" corresp="note-0150-01" type="noteAnchor" />
comme le ſinus total au ſinus du complement de <lb />celui qu’on voudra de ces mêmes angles.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0150-01" corresp="note-0150-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <p rend="italics">
          <s xml:space="preserve">On peut encore comparer ces trois Corollaires à la Propo-<lb />ſition 71. </s>
          <s xml:space="preserve">de M. </s>
          <s xml:space="preserve">Borelli &amp; </s>
          <s xml:space="preserve">au Corollaire qu’il en tire.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> V.</head>
        <p>
          <s xml:space="preserve">On voit encore de cette propoſition que dans l’hy-<lb />
<ptr xml:id="note-0150-02a" corresp="note-0150-02" type="noteAnchor" />
pothéſe ou les lignes de direction de tous les points <lb />du corps A D concourent au centre E de la terre, <lb />de quelque maniére que ce poids ſoit ſoutenu par <lb />tant de puiſſances F, G, H, I, K, L, M, N, &amp;</s>
          <s xml:space="preserve">c. <lb /></s>
          <s xml:space="preserve">qu’on voudra avec des cordes qui lui ſoient appli-<lb />quées en tant de points A, B, C, D, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">qu’on vou-<lb />dra; </s>
          <s xml:space="preserve">chacune de ces puiſſances ſera toujours à ce <lb />poids, comme chacune de leurs proportionelles à la <lb />ſomme des ſublimitez des forces avec leſquelles ces <lb />points A, B, C, D, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">ſont tirez ſuivant les lignes <lb />AE, BE, CE, DE, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">par le concours d’action <lb />des puiſſances qui y ſont appliquées: </s>
          <s xml:space="preserve">des ſublimitez, <lb />dî-je, déterminées comme dans le Corollaire 1. </s>
          <s xml:space="preserve">Car <lb />il eſt clair que ce poids agit contre toutes ces puiſſan-<lb />ces de même que feroit une force qui lui ſeroit égale, <lb />ſi AE, BE, CE, DE, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">étoient autant de cor-<lb />des attachées enſemble au point E par un nœud <lb />commun auquel cette force fut appliquée ſuivant la <lb />direction ZE du centre de gravité de ce poids. </s>
          <s xml:space="preserve">Or <lb />en ce cas les points A, B, C, D, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">étant comme <lb />autant de nœuds auſquels ſont appliquées, chacune <lb />ſuivant ſa direction, les puiſſances F, G, H, I, K, <lb />L, M, N, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">ſi l’on prend depuis E ſur chacune <lb />des lignes AE, BE, CE, DE, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">une partie Eg, <lb />Ef, Ec, Eb, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">égale à la ſomme des ſublimitez
</s>
          <pb facs="0151" n="125" />
          <s xml:space="preserve"><fw type="head">DE M. BORELLI.</fw>
moins celle des profondeurs des puiſſances appli-<lb />
<ptr xml:id="note-0151-01a" corresp="note-0151-01" type="noteAnchor" />
quées à chacun des points A, B, C, D, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">On <lb />trouvera (Cor 1.) </s>
          <s xml:space="preserve">que chacune de toutes ces puiſ-<lb />ſances F, G, H, I, K, L, M, N, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">ſeroit alors à <lb />la force qu’on ſuppoſe en E, comme chacune de leurs <lb />proportionelles DO, CP, BQ, DX, AR, CV, BT, <lb />AS, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">à la ſomme des ſublimitez, El, Ee, Ed, <lb />Ea, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">des forces dont les nœuds A, B, C, D, &amp;</s>
          <s xml:space="preserve">c. <lb /></s>
          <s xml:space="preserve">ſeroient alors tirez, chacun ſuivant la ligne qui le <lb />joint avec le point E: </s>
          <s xml:space="preserve">Donc chacune de ces mêmes <lb />puiſſances eſt en effet au poids AD, comme chacune <lb />de leurs proportionelles à la ſomme de telles ſubli-<lb />mitez des forces avec leſquelles les points A, B, C, D, <lb />&amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">ſont tirez ſuivant les lignes AE, BE, CE, DE, <lb />&amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">par le concours d’action de celles qui y ſont ap-<lb />pliquées.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0150-02" corresp="note-0150-02a" place="margin">fig. 23. <lb />24.</note>
              <note xml:space="preserve" xml:id="note-0151-01" corresp="note-0151-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <p rend="italics">
          <s xml:space="preserve">Si les forces, avec leſquelles les différens points A, B, C, <lb />D, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">du corps AD, ſont tirez ſuivant des lignes qui con-<lb />courent au centre E de la terre, par le concours d’action des <lb />puiſſances qui y ſont appliquées, avoient quelque profondeur, <lb />on trouveroit de même que chacune de toutes les puiſſances qui <lb />ſoutiennent ce poids, lui ſeroit en même raiſon que chacune de <lb />leurs proportionnelles à la ſomme de telles ſublimitez moins <lb />celle des profondeurs de ces mêmes forces: </s>
          <s xml:space="preserve">mais ce cas étant <lb />naturellement impoſſible; </s>
          <s xml:space="preserve">puiſqu’il faudroit pour cela que ce <lb />poids comprît pour le moins plus du quart de la circonférence <lb />de la terre, on n’a pas crû qu’il fût néceſſaire de l’exprimer.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> VI.</head>
        <p>
          <s xml:space="preserve">On voit préſentement que dans l’hypotheſe ordi-<lb />naire, ou l’on regarde les directions AE, BE, CE, <lb />DE, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">comme paralleles entr’elles, chacune des <lb />ſublimitez El, Ee, Ed, Ea, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">déterminées ſur
</s>
          <pb facs="0152" n="126" />
          <s xml:space="preserve"><fw type="head">EXAMEN DE L’OPINION</fw>
ZE par chacune des proportionelles Eg, Ef, Ec, <lb />
<ptr xml:id="note-0152-01a" corresp="note-0152-01" type="noteAnchor" />
Eb, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">qu’on vient de prendre egales à la ſomme <lb />des ſublimitez moins celle des profondeurs des puiſ-<lb />ſances appliquées à chacun des points A, B, C, D, <lb />&amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">étant alors égales à ces mêmes proportionelles; <lb /></s>
          <s xml:space="preserve">chacune de ce qu’il y a de puiſſances ainſi appliquées <lb />à ce poids, ſçavoir F, G, H, I, K, L, M, N, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">eſt <lb />toujours en ce cas à ce même poids, comme chacune <lb />de leurs proportionelles à la ſomme de toutes leurs <lb />ſublimitez moins celle de toutes leurs profondeurs.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0152-01" corresp="note-0152-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> VII.</head>
        <p>
          <s xml:space="preserve">D’où il ſuit que dans la même hypothêſe la ſom-<lb />me de toutes ces puiſſances eſt à ce poids, comme <lb />la ſomme de leurs proportionelles à la ſomme de leurs <lb />ſublimitez moins celle de leurs profondeurs: </s>
          <s xml:space="preserve">De <lb />ſorte que s’il n’y en avoit que deux d’appliquées à <lb />chaque point, dont l’une tirât à droit, &amp; </s>
          <s xml:space="preserve">l’autre à <lb />gauche; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">que toutes celles de chaque côté fuſſent <lb />égales entr’elles, &amp; </s>
          <s xml:space="preserve">avec des directions qui fiſſent <lb />avec celle du point où elles ſont appliquées, des angles <lb />de@chaque côté égaux entr’eux: </s>
          <s xml:space="preserve">la ſomme (fig. </s>
          <s xml:space="preserve">23.) </s>
          <s xml:space="preserve">des <lb />ſublimitez, par exemple Ar + Aſ, ou Bq + Bt, <lb />ou Cp + Cu, ou Do + Dx, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">des deux puiſſances <lb />appliquées au quel que ce ſoit des nœuds A, B, <lb />C, D, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">ou bien (fig. </s>
          <s xml:space="preserve">24.) </s>
          <s xml:space="preserve">la différence de la ſu-<lb />blimité de l’une à la profondeur de l’autre, par <lb />exemple Ar - Aſ, ou Bq - Bt, ou Cp - Cu, ou <lb />Do - Dx, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">étant alors la même pour tous ces <lb />points, auſſi-bien que les proportionelles de ces puiſ-<lb />ſances; </s>
          <s xml:space="preserve">la ſomme de toutes ces puiſſances ſeroit <lb />alors au poids AD, comme la ſomme des proportio-<lb />nelles de deux d’entr’elles appliquées à un même <lb />point, quel qu’il ſoit, eſt à la ſomme (fig. </s>
          <s xml:space="preserve">23.) </s>
          <s xml:space="preserve">de leurs
</s>
          <pb facs="0153" n="127" />
          <s xml:space="preserve"><fw type="head">DE M. BORELLI.</fw>
ſublimitez, ou (fig. </s>
          <s xml:space="preserve">24.) </s>
          <s xml:space="preserve">à la différence qui eſt entre <lb />
<ptr xml:id="note-0153-01a" corresp="note-0153-01" type="noteAnchor" />
la ſublimité de l’une &amp; </s>
          <s xml:space="preserve">la profondeur de l’autre.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0153-01" corresp="note-0153-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Corollaire</hi> VIII.</head>
        <p>
          <s xml:space="preserve">Ce qui fait enfin voir que ſi toutes les puiſſances <lb />F, G, H, I, K, L, M, N, &amp;</s>
          <s xml:space="preserve">c. </s>
          <s xml:space="preserve">étoient égales en-<lb />tr’elles, &amp; </s>
          <s xml:space="preserve">que toutes leurs directions fiſſent avec <lb />celles des points où elles ſont appliquées, des angles <lb />égaux entr’eux; </s>
          <s xml:space="preserve">leur ſomme ſeroit alors au poids <lb />CD (fig. </s>
          <s xml:space="preserve">23.) </s>
          <s xml:space="preserve">comme une de leurs proportionelles <lb />à une de leurs ſublimitez, de quelque maniére qu’on <lb />les prenne; </s>
          <s xml:space="preserve">c’eſt-à-dire, comme le ſinus total au ſinus <lb />du complement de celui qu’on voudra de ces mêmes <lb />angles.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">On peut enfin comparer ces quatre derniers corollaires à <lb />la Propoſition 72. </s>
          <s xml:space="preserve">de M. </s>
          <s xml:space="preserve">Borelli, &amp; </s>
          <s xml:space="preserve">au corollaire qu’il <lb />en tire.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">Tels ſont les principes généraux de tout ce que cet Au-<lb />theur a dit des poids ſuſpendus par des cordes, &amp; </s>
          <s xml:space="preserve">de l’uſage <lb />qu’il en a fait pour exprimer la force des muſcles; </s>
          <s xml:space="preserve">c’eſt ce <lb />qu’on s’étoit propoſé d’établir dans ce Chapitre par la mé-<lb />@hode du Projet précédent: </s>
          <s xml:space="preserve">qu’on voye préſentement ſi la <lb />ſienne peut aller juſques-là, &amp; </s>
          <s xml:space="preserve">ſi elle peut conduire à la So-<lb />lution du Problême ſuivant.</s>
          <s xml:space="preserve" />
        </p>
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0153-01" />
          <label>0153-01</label>
        </figure>
      </div>
      <div type="section">
        <head xml:space="preserve">PROBLEME.</head>
        <p rend="italics">
          <s xml:space="preserve">DIx puiſſances φ, A, E, D, B, F, G, H, I, K, <lb />
<ptr xml:id="note-0153-02a" corresp="note-0153-02" type="noteAnchor" />
appliquées à pluſieurs nœuds de cordes, étant données <lb />avec les angles que toutes ces cordes font entr’elles; </s>
          <s xml:space="preserve">trouver
</s>
          <pb facs="0154" n="128" />
          <s xml:space="preserve"><fw type="head">EXAMEN DE L’OPINION</fw>
la valeur du poids T que toutes ces puiſſances ainſi appli-<lb />
<ptr xml:id="note-0154-01a" corresp="note-0154-01" type="noteAnchor" />
quées ſoutiennent enſemble.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0153-02" corresp="note-0153-02a" place="margin">fig. 20.<unclear reason="illegible" /></note>
              <note xml:space="preserve" xml:id="note-0154-01" corresp="note-0154-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve"><hi rend="small caps">Solution</hi>.</head>
        <p>
          <s xml:space="preserve">Soit la valeur de chaque puiſſance, &amp; </s>
          <s xml:space="preserve">de chaque <lb />angle donné dans la Table ſuivante.</s>
          <s xml:space="preserve" />
        </p>
        <note xml:space="preserve" place="margin"> <lb />Puiſſance. # Livres. # # Angle. # Deg. # M. <lb />φ # 5. # # θCT # 45. # 30. <lb />A # 4. # {1/4} # MCT # 150. # 20. <lb />E # 7. # {1/4} # LZC # 58. # 30. <lb />D # 12. # {1/2} # RZC # 112. # 15. <lb />B # 14. # # VOZ # 151. <lb />F # 11. # {1/2} # SOZ # 110. <lb />G # 17. # # QZC # 143. <lb />H # 7. # {1/2} # NCT # 145. <lb />I # 16. # # βXC # 131. # 30. <lb />K # 13. # {1/2} # hXC # 123. # 30. <lb /># PCT # 64. # 40. <lb /># δYC # 62. <lb /># zYC # 107. # 20. <lb /># eYC # 151. # 40. <lb /></note>
        <pb facs="0155" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0155-01" />
          <label>0155-01</label>
        </figure>
        <pb facs="0155a" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0155a-01" />
          <label>0155a-01</label>
        </figure>
        <pb facs="0156" />
        <pb facs="0157" />
        <pb facs="0157a" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0157a-01" />
          <label>0157a-01</label>
        </figure>
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        <pb facs="0159" />
        <pb facs="0159a" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0159a-01" />
          <label>0159a-01</label>
        </figure>
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        <pb facs="0161" />
        <pb facs="0161a" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0161a-01" />
          <label>0161a-01</label>
        </figure>
        <pb facs="0162" />
        <pb facs="0163" />
        <pb facs="0163a" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0163a-01" />
          <label>0163a-01</label>
        </figure>
        <pb facs="0164" />
        <pb facs="0165" />
        <pb facs="0165a" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0165a-01" />
          <label>0165a-01</label>
        </figure>
        <pb facs="0166" />
        <pb facs="0167" />
        <pb facs="0167a" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0167a-01" />
          <label>0167a-01</label>
        </figure>
        <pb facs="0168" />
        <pb facs="0169" />
        <pb facs="0169a" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0169a-01" />
          <label>0169a-01</label>
        </figure>
        <pb facs="0170" />
        <pb facs="0171" />
        <pb facs="0171a" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0171a-01" />
          <label>0171a-01</label>
        </figure>
        <pb facs="0172" />
        <pb facs="0173" />
        <pb facs="0173a" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0173a-01" />
          <label>0173a-01</label>
        </figure>
        <pb facs="0174" />
        <pb facs="0175" />
        <pb facs="0175a" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0175a-01" />
          <label>0175a-01</label>
        </figure>
        <pb facs="0176" />
        <pb facs="0177" />
        <pb facs="0177a" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0177a-01" />
          <label>0177a-01</label>
        </figure>
        <pb facs="0178" />
        <pb facs="0179" />
        <pb facs="0179a" />
        <figure>
          <graphic url="http://echo.mpiwg-berlin.mpg.de/zogilib?fn=/permanent/library/xxxxxxxx/figures/0179a-01" />
          <label>0179a-01</label>
        </figure>
        <pb facs="0180" />
        <pb facs="0181" n="129" />
        <fw type="head">DE M. BORELLI.</fw>
        <p>
          <s xml:space="preserve">Cela ſuppoſé, ſur les branches des cordes auſquel-<lb />
<ptr xml:id="note-0181-01a" corresp="note-0181-01" type="noteAnchor" />
les les puiſſances φ, A, E, D, B, F, G, H, I, K, <lb />ſont immédiatement appliquées, ſoient priſes depuis <lb />leurs nœuds des parties θC, LZ, VO, SO, QZ, βX, <lb />hX, δY, zY, eY, qui ſoient entr’elles, comme les <lb />forces de ces mêmes puiſſances, c’eſt-à-dire, comme <lb />les chifres qui leur répondent dans la Table pré-<lb />cédente.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0181-01" corresp="note-0181-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">Préſentement ſi l’on regarde chacune de ces pro-<lb />portionelles comme un ſinus total, le ſinus de la diffé-<lb />rence d’un angle droit à l’angle d’application de la <lb />puiſſance qui rèpond à cette proportionelle, ſera la <lb />ſublimité, ou la profondeur de cette même puiſſance: <lb /></s>
          <s xml:space="preserve">par exemple, ſi l’on prend la proportionelle C θ <lb />de la puiſſance φ, pour un ſinus total, ſa profondeur <lb />Cλ ſera le ſinus de l’angle Cθλ, qui eſt la différen-<lb />ce de θCλ angle d’application de cette puiſſance, à <lb />un angle droit. </s>
          <s xml:space="preserve">De même en prenant la proportio-<lb />nelle V O de la puiſſance E, pour un ſinus total, ſa <lb />ſublimité Ou ſera le ſinus de l'angle OVu, qui eſt la <lb />diffèrence d’un angle droit à ſon angle d’application <lb />V O Z; </s>
          <s xml:space="preserve">de cette facon nous aurons les ſublimi-<lb />tez &amp; </s>
          <s xml:space="preserve">les profondeurs de toutes ces puiſſances par les <lb />analogies ſuivantes.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0182" n="130" />
        <fw type="head">EXAMEN DE L’OPINION</fw>
        <note xml:space="preserve" place="margin"> <lb />Comme # au # # # # Ainſi # # à <lb />Le ſinus total # Sinus # de \\ l’angle # de \\ Deg. M. \\ différence \\ de 90. deg. \\ à l’angle \\ d’applica- \\ tion # de la \\ puiſ- \\ ſan- \\ ce. # La propor- \\ tionelle \\ de cette \\ méme puiſ- \\ ſance # de # Saſubli- \\ mité, ou \\ à ſa pro- \\ fondeur # de <lb /># 7009093. # Cθλ # 44. 30. # φ # Cθ # 5. # Cλ # 3. {1013093./2000000.} <lb /># 5224986. # ZLl # 31. 30. # A # ZL # 4. {1/4} # Z l # 2. {4412381./20000000.} <lb /># 8746197. # OVu # 61. # E # OV # 7. {1/4} # Ou # 6. {13639713./40000000.} <lb />10000000.{ # 3420202. # OSſ # 20. # D # OS # 12. {1/2} # Oſ # 4. {110101./400000.} <lb /># 7986355. # ZQq # 53. # B # ZQ # 14. # Zq # 11. {180897./1000000.} <lb /># 6626201. # Xβf # 41. 30. # F # X β # 11. {1/2} # Xf # 7. {6439043./20000000.} <lb /># 5519370. # Xhb # 33. 30. # G # Xh # 17. # Xh # 9. {382929./1000000.} <lb /># 4694716. # Yδd # 28. # H # Yδ # 7. {1/2} # Yd # 3. {521037./1000000.} <lb /># 2979303. # Yzx # 17. 20. # I # Yz # 16. # Yx # 4. {479303./625000.} <lb /># 8802014. # Yeg # 61. 40. # K # Ye # 13. {1/2} # Yg # 11. {8827189./10000000.} <lb /></note>
        <p>
          <s xml:space="preserve">Aprés avoir ainſi trouvé la valeur de chacune des ſu-<lb />blimitez &amp; </s>
          <s xml:space="preserve">des profondeurs de toutes les puiſſances qui <lb />ſoutiennent le poids T; </s>
          <s xml:space="preserve">ſoit priſe Z R égale à Ou <lb />plus O ſ; </s>
          <s xml:space="preserve">c’eſt-à-dire, ſuivant les analogies précéden-<lb />tes, égale à 6. </s>
          <s xml:space="preserve">{13639713.</s>
          <s xml:space="preserve">/40000000.</s>
          <s xml:space="preserve">} plus 4. </s>
          <s xml:space="preserve">{110101.</s>
          <s xml:space="preserve">/400000.</s>
          <s xml:space="preserve">}; </s>
          <s xml:space="preserve">ou bien en ré-<lb />duiſant ces deux fractions à une même dénomina-
</s>
          <pb facs="0183" n="131" />
          <s xml:space="preserve"><fw type="head">DEM. BORELLI.</fw>
tion, égale à 10. </s>
          <s xml:space="preserve">{24649813.</s>
          <s xml:space="preserve">/40000000.</s>
          <s xml:space="preserve">}. </s>
          <s xml:space="preserve">Aprés cela O V étant à Z R, <lb />
<ptr xml:id="note-0183-01a" corresp="note-0183-01" type="noteAnchor" />
comme la puiſſance E à la force dont le point Z eſt <lb />tiré ſuivant ZO par le concours d’action des puiſ-<lb />ſances D &amp; </s>
          <s xml:space="preserve">E; </s>
          <s xml:space="preserve">Z R ſera la proportionelle de cette <lb />force, &amp; </s>
          <s xml:space="preserve">l’angle R Z C étant (hyp.) </s>
          <s xml:space="preserve">de 112. </s>
          <s xml:space="preserve">deg. </s>
          <s xml:space="preserve">15. <lb /></s>
          <s xml:space="preserve">min. </s>
          <s xml:space="preserve">ſa diffèrence à un angle droit; </s>
          <s xml:space="preserve">c’eſt-à-dire, <lb />l’angle ZRr ſera de 22. </s>
          <s xml:space="preserve">deg. </s>
          <s xml:space="preserve">15. </s>
          <s xml:space="preserve">min. </s>
          <s xml:space="preserve">Ce qui don-<lb />nera par une analogie ſemblable aux précédentes, <lb />3. </s>
          <s xml:space="preserve">{74265285916559.</s>
          <s xml:space="preserve">/200000000000000.</s>
          <s xml:space="preserve">} pour la valeur de Zr ſublimité de cette <lb />force: </s>
          <s xml:space="preserve">puiſque ZR de 10. </s>
          <s xml:space="preserve">{24642813.</s>
          <s xml:space="preserve">/40000000.</s>
          <s xml:space="preserve">} eſt à 3. </s>
          <s xml:space="preserve">{17426@285916559.</s>
          <s xml:space="preserve">/200000000000000.</s>
          <s xml:space="preserve">} <lb />comme le ſinus total 10000000. </s>
          <s xml:space="preserve">à 3786486. </s>
          <s xml:space="preserve">ſinus <lb />de l’angle ZRr de 22. </s>
          <s xml:space="preserve">deg. </s>
          <s xml:space="preserve">15. </s>
          <s xml:space="preserve">min.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0183-01" corresp="note-0183-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">Soit enſuitte 1°. </s>
          <s xml:space="preserve">C M égale à Zq plus Zr moins <lb />Zl; </s>
          <s xml:space="preserve">c’eſt-à-dire, ſuivant les analogies que nous ve-<lb />nons de trouver, égale à 11. </s>
          <s xml:space="preserve">{180897.</s>
          <s xml:space="preserve">/1000000} plus 3. </s>
          <s xml:space="preserve">{174265285916559.</s>
          <s xml:space="preserve">/200000000@00000.</s>
          <s xml:space="preserve">} <lb />moins 2. </s>
          <s xml:space="preserve">{4412381.</s>
          <s xml:space="preserve">/20000000.</s>
          <s xml:space="preserve">}; </s>
          <s xml:space="preserve">ou bien en réduiſant ces trois frac-<lb />tions à une même dénomination, égale à 12. </s>
          <s xml:space="preserve">{1663208759165@9.</s>
          <s xml:space="preserve">/200000000000000}. <lb /></s>
          <s xml:space="preserve">Ce qui donnera par une analogie ſemblable aux pré-<lb />cédentes, 11. </s>
          <s xml:space="preserve">{74566272432665199141.</s>
          <s xml:space="preserve">/500000000000000000000.</s>
          <s xml:space="preserve">} pour la valeur de la <lb />ſublimité Cm: </s>
          <s xml:space="preserve">puis que 12. </s>
          <s xml:space="preserve">{166320875916559.</s>
          <s xml:space="preserve">/200000000000000.</s>
          <s xml:space="preserve">} eſt à 11. </s>
          <s xml:space="preserve"><lb />{745662724;</s>
          <s xml:space="preserve">2665199141.</s>
          <s xml:space="preserve">/500000000000000000000.</s>
          <s xml:space="preserve">}, comme le ſinus total 10000000. </s>
          <s xml:space="preserve">à <lb />8689196. </s>
          <s xml:space="preserve">ſinus de l’angle CMm de 60. </s>
          <s xml:space="preserve">deg. </s>
          <s xml:space="preserve">20. </s>
          <s xml:space="preserve"><lb />min. </s>
          <s xml:space="preserve">qui eſt la différence d’un angle droit à l’angle <lb />M C T de (hyp.) </s>
          <s xml:space="preserve">150. </s>
          <s xml:space="preserve">deg. </s>
          <s xml:space="preserve">20. </s>
          <s xml:space="preserve">min.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">Faite de même C N égale à Xb plus Xf; </s>
          <s xml:space="preserve">c’eſt-<lb />à-dire, ſuivant les analogies de la table précédente, <lb />égale à 9. </s>
          <s xml:space="preserve">{382929.</s>
          <s xml:space="preserve">/1000000.</s>
          <s xml:space="preserve">} plus 7. </s>
          <s xml:space="preserve">{64,9043.</s>
          <s xml:space="preserve">/20000000.</s>
          <s xml:space="preserve">}; </s>
          <s xml:space="preserve">ou bien en réduiſant <lb />ces deux fractions à une même dénomination, égale <lb />à 16. </s>
          <s xml:space="preserve">{14097623.</s>
          <s xml:space="preserve">/20000000}. </s>
          <s xml:space="preserve">Ce qui donnera par une analogie ſem-<lb />blable aux précédentes, 13. </s>
          <s xml:space="preserve">{136767694854583/200000000000000.</s>
          <s xml:space="preserve">} pour la va-<lb />leur de la ſublimité Cn: </s>
          <s xml:space="preserve">puis que 16. </s>
          <s xml:space="preserve">{14097623.</s>
          <s xml:space="preserve">/20000000.</s>
          <s xml:space="preserve">} eſt à <lb />13. </s>
          <s xml:space="preserve">{136767694854583.</s>
          <s xml:space="preserve">/200000000000000.</s>
          <s xml:space="preserve">}, comme le ſinus total 10000000. </s>
          <s xml:space="preserve">à
</s>
          <pb facs="0184" n="132" />
          <s xml:space="preserve"><fw type="head">EXAMEN DE L’OPINION</fw>
8191521. </s>
          <s xml:space="preserve">ſinus de l’angle CNn de 55. </s>
          <s xml:space="preserve">deg. </s>
          <s xml:space="preserve">qui eſt <lb />
<ptr xml:id="note-0184-01a" corresp="note-0184-01" type="noteAnchor" />
la différence d’un angle droit à l’angle NCT de <lb />(hyp.) </s>
          <s xml:space="preserve">145. </s>
          <s xml:space="preserve">deg.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0184-01" corresp="note-0184-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />de@cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
        <p>
          <s xml:space="preserve">3°. </s>
          <s xml:space="preserve">Enſin ſoit encore C P égale à Yg plus Yx <lb />moins Yd; </s>
          <s xml:space="preserve">c’eſt-à-dire, ſuivant les analogies de la <lb />table précédente, égale à 11. </s>
          <s xml:space="preserve">{8827189.</s>
          <s xml:space="preserve">/10000000.</s>
          <s xml:space="preserve">} plus 4. </s>
          <s xml:space="preserve">{479303.</s>
          <s xml:space="preserve">/625000.</s>
          <s xml:space="preserve">} moins <lb />3. </s>
          <s xml:space="preserve">{521037.</s>
          <s xml:space="preserve">/1000000.</s>
          <s xml:space="preserve">}; </s>
          <s xml:space="preserve">ou bien en réduiſant ces trois fractions à <lb />une même dénomination, égale à 12. </s>
          <s xml:space="preserve">{232141683.</s>
          <s xml:space="preserve">/282000000.</s>
          <s xml:space="preserve">}. </s>
          <s xml:space="preserve">Ce qui <lb />donnera par une analogie encore ſemblable aux <lb />précédentes, 5. </s>
          <s xml:space="preserve">{686442223302177.</s>
          <s xml:space="preserve">/1410000000000000.</s>
          <s xml:space="preserve">} pour la valeur de la pro-<lb />fondeur C p: </s>
          <s xml:space="preserve">puis que 12. </s>
          <s xml:space="preserve">{232141683.</s>
          <s xml:space="preserve">/282000000.</s>
          <s xml:space="preserve">} eſt à 5. </s>
          <s xml:space="preserve">{686442223302177.</s>
          <s xml:space="preserve">/1410000000000000.</s>
          <s xml:space="preserve">}, <lb />comme le ſinus total 10000000. </s>
          <s xml:space="preserve">à 4278838. </s>
          <s xml:space="preserve">ſinus <lb />de l’angle CPp de 25. </s>
          <s xml:space="preserve">deg. </s>
          <s xml:space="preserve">20. </s>
          <s xml:space="preserve">min. </s>
          <s xml:space="preserve">qui eſt la diffè-<lb />rence d’un angle droit à l’angle P C T de (hyp.) </s>
          <s xml:space="preserve">64. <lb /></s>
          <s xml:space="preserve">deg. </s>
          <s xml:space="preserve">40. </s>
          <s xml:space="preserve">min.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">De tout cela on voit preſentement que <lb />la {Subl. </s>
          <s xml:space="preserve">Cm \\ Subl. </s>
          <s xml:space="preserve">Cn \\ Prof. </s>
          <s xml:space="preserve">Cλ \\ Prof. </s>
          <s xml:space="preserve">Cp} eſt ègale à {11. </s>
          <s xml:space="preserve">{74566272432665199141.</s>
          <s xml:space="preserve">/500000000000000000000.</s>
          <s xml:space="preserve">}. </s>
          <s xml:space="preserve">\\ 13. </s>
          <s xml:space="preserve">{136767694854583.</s>
          <s xml:space="preserve">/200000000000000.</s>
          <s xml:space="preserve">} \\ 3. </s>
          <s xml:space="preserve">{1013093.</s>
          <s xml:space="preserve">/2000000.</s>
          <s xml:space="preserve">} \\ 5. </s>
          <s xml:space="preserve">{686442223302377.</s>
          <s xml:space="preserve">/1410000000000000.</s>
          <s xml:space="preserve">}</s>
        </p>
        <p>
          <s xml:space="preserve">De ſorte qu’en réduiſant toutes ces fractions à une <lb />même dénomination, on aura Cm + Cn - Cλ -<lb />Cp = 15. </s>
          <s xml:space="preserve">{5919081693@137450578881.</s>
          <s xml:space="preserve">/70500000000000000000000}. </s>
          <s xml:space="preserve">Or ayant pris, comme <lb />nous venons de faire, 1° CR = Oſ + Ou. </s>
          <s xml:space="preserve">2°. </s>
          <s xml:space="preserve">CM <lb />= Zq + Zr - Zl. </s>
          <s xml:space="preserve">3° CN = Xf + Xb. </s>
          <s xml:space="preserve">4°. </s>
          <s xml:space="preserve">CP <lb />= Yg + Yx - Yd; </s>
          <s xml:space="preserve">chacune des puiſſances qui <lb />ſoutiennent ainſi le poids T; </s>
          <s xml:space="preserve">par exemple, la puiſ-<lb />ſance E eſt (Prop. </s>
          <s xml:space="preserve">4. </s>
          <s xml:space="preserve">Cor. </s>
          <s xml:space="preserve">1.) </s>
          <s xml:space="preserve">à ce poids, comme ſa <lb />proportionnelle OV de (hyp.) </s>
          <s xml:space="preserve">7 {1/4} à Cm + Cn -
</s>
          <pb facs="0185" n="133" />
          <s xml:space="preserve"><fw type="head">DE M. BORELLI.</fw>
Cλ - Cp: </s>
          <s xml:space="preserve">Donc cette même puiſſance E eſt à ce <lb />
<ptr xml:id="note-0185-01a" corresp="note-0185-01" type="noteAnchor" />
poids, comme 7. </s>
          <s xml:space="preserve">{1/4} à 15. </s>
          <s xml:space="preserve">{1919081693413745<unclear reason="illegible" />0578881.</s>
          <s xml:space="preserve">/705<unclear reason="illegible" />00000000000000000000.</s>
          <s xml:space="preserve">}; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">par con-<lb />ſèquent la valeur de cette puiſſance étant (hyp.) <lb /></s>
          <s xml:space="preserve">de 7. </s>
          <s xml:space="preserve">{1/4} liv. </s>
          <s xml:space="preserve">ce même poids eſt auſſi juſtement de <lb />15. </s>
          <s xml:space="preserve">{5919081692@137450@78881.</s>
          <s xml:space="preserve">/70500000000000000000000.</s>
          <s xml:space="preserve">} liv. </s>
          <s xml:space="preserve">c’eſt-à-dire, de 15. </s>
          <s xml:space="preserve">livres, &amp; </s>
          <s xml:space="preserve"><lb />un peu plus de cinq ſeptiémes de livre. </s>
          <s xml:space="preserve">Ce qu’il faloit <lb />trouver.</s>
          <s xml:space="preserve" />
        </p>
        <floatingText>
          <body>
            <div type="float">
              <note xml:space="preserve" xml:id="note-0185-01" corresp="note-0185-01a" place="margin">DES POIDS <lb />ſoutenus avec <lb />des cordes ſeu-<lb />lement.</note>
            </div>
          </body>
        </floatingText>
      </div>
      <div type="section">
        <head xml:space="preserve">FIN.</head>
        <head xml:space="preserve">AU RELIEUR.</head>
        <p rend="italics">
          <s xml:space="preserve">LE S neuf planches au pied deſquelles on voit Projet, <lb />doivent ètre reliées ſelon l’ordre de leurs chifres immé-<lb />diatement à la fin de la Méchanique; </s>
          <s xml:space="preserve">en ſorte que le quart <lb />du papier où il n’y a rien, ſoit enfermé dans le livre, &amp; </s>
          <s xml:space="preserve">que <lb />l’autre quart où ſont les figures, puiſſe, en les dépliant, en <lb />ſortir tout entier, pour ſervir à tous les endroits de cette Mé-<lb />chanique où l’on en aura beſoin. </s>
          <s xml:space="preserve">Pour les quatre autres plan-<lb />ches, au pied deſquelles on voit Examen, elles doivent auſſi <lb />être reliées de la même maniére à la fin de l’Examen que voicy <lb />de M. </s>
          <s xml:space="preserve">Borelli.</s>
          <s xml:space="preserve" />
        </p>
      </div>
      <div type="section">
        <head xml:space="preserve">A PARIS,</head>
        <p>
          <s xml:space="preserve">De l’Imprimerie dela Veuve Clement Gaſſe, 1687.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0186" />
      </div>
      <div type="section">
        <head xml:space="preserve">EXTRAIT DV PRIVILE’GE</head>
        <head rend="italics" xml:space="preserve">du Roy.</head>
        <p>
          <s xml:space="preserve"><hi rend="small caps">PAr</hi> Lettres Patentes du Roy, données à Ver-<lb />ſailles 19. </s>
          <s xml:space="preserve">jourde Juin 1687. </s>
          <s xml:space="preserve">ſignées par le Roy <lb />en ſon Conſeil, <hi rend="small caps">Galloys</hi> &amp; </s>
          <s xml:space="preserve">ſcellées. </s>
          <s xml:space="preserve">Il eſt permis <lb />à <hi rend="small caps">Jean</hi> <hi rend="small caps">Boudot</hi> Libraire à Paris, d’imprimer un <lb />livre intitulé Projet d’une nouvelle Méchanique, avec un <lb />Examen de l’Opinion de M. </s>
          <s xml:space="preserve">Borelli, ſur les propriétez des <lb />Poids ſuſpendus par des Cordes, par M. </s>
          <s xml:space="preserve">V * * * * * * * en <lb />tel volume, marge, &amp; </s>
          <s xml:space="preserve">caractére, en autant de volumes, <lb />&amp; </s>
          <s xml:space="preserve">tout autant de fois que bon luy ſemblera, pendant <lb />le tems de huit années conſécutives, à commencer <lb />du jour qu’il aura été achevé d’imprimer pour la <lb />premiére fois. </s>
          <s xml:space="preserve">Et défenſes ſont faites à toutes ſortes <lb />de perſonnes d’imprimer ledit livre, d’en vendre n’y <lb />diſtribuër d’autre impreſſion que de celle dudit <lb /><hi rend="small caps">Boudot</hi>, ou de ceux qui auront ſon droit, à peine <lb />de mil livres d’amende, &amp; </s>
          <s xml:space="preserve">de tous dèpens, dom-<lb />mages &amp; </s>
          <s xml:space="preserve">intérêts, &amp; </s>
          <s xml:space="preserve">de confiſcation des Exemplaires <lb />contrefaits, ainſi qu’il eſt porté plus au long dans ledit <lb />Privilége.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">Regiſtré ſur le Livre de la Communauté des Li-<lb />braires &amp; </s>
          <s xml:space="preserve">Imprimeurs de Paris, le 30. </s>
          <s xml:space="preserve">Juillet 1687.</s>
          <s xml:space="preserve" />
        </p>
        <p>
          <s xml:space="preserve">Signé, <hi rend="small caps">Coignard</hi>, Syndic.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">Achevè d’imprimer pour la premiére fois le 30. </s>
          <s xml:space="preserve">Aouſt 1687.</s>
          <s xml:space="preserve" />
        </p>
        <pb facs="0187" />
      </div>
      <div type="section">
        <head rend="italics" xml:space="preserve">FAVTES A CORRIGER.</head>
        <p rend="italics">
          <s xml:space="preserve">PAg. </s>
          <s xml:space="preserve">4. </s>
          <s xml:space="preserve">lig. </s>
          <s xml:space="preserve">20. </s>
          <s xml:space="preserve">AH liſez AK</s>
        </p>
        <p rend="italics">
          <s xml:space="preserve">pag. </s>
          <s xml:space="preserve">9. </s>
          <s xml:space="preserve">ligne 14. </s>
          <s xml:space="preserve">Lemme 3.</s>
          <s xml:space="preserve">, liſez Lemme 3.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">pag. </s>
          <s xml:space="preserve">14. </s>
          <s xml:space="preserve">ligne 11. </s>
          <s xml:space="preserve">poid liſez poids</s>
        </p>
        <p rend="italics">
          <s xml:space="preserve">pag. </s>
          <s xml:space="preserve">17. </s>
          <s xml:space="preserve">ligne 4. </s>
          <s xml:space="preserve">elle ſe liſez elle le</s>
        </p>
        <p rend="italics">
          <s xml:space="preserve">pag. </s>
          <s xml:space="preserve">23. </s>
          <s xml:space="preserve">à la marge Vis-à-vis du problême marquez fig. </s>
          <s xml:space="preserve">19.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">pag. </s>
          <s xml:space="preserve">29. </s>
          <s xml:space="preserve">ligne 22. </s>
          <s xml:space="preserve">AH liſez AD</s>
        </p>
        <p rend="italics">
          <s xml:space="preserve">pag. </s>
          <s xml:space="preserve">35. </s>
          <s xml:space="preserve">à la marge fig. </s>
          <s xml:space="preserve">26. </s>
          <s xml:space="preserve">liſez fig. </s>
          <s xml:space="preserve">26. <lb /></s>
          <s xml:space="preserve">27.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">pag. </s>
          <s xml:space="preserve">38. </s>
          <s xml:space="preserve">ligne 25. </s>
          <s xml:space="preserve">à EF; </s>
          <s xml:space="preserve">liſez HEF; </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">ligne 26. </s>
          <s xml:space="preserve">effacéz ou EHF,</s>
        </p>
        <p rend="italics">
          <s xml:space="preserve">pag. </s>
          <s xml:space="preserve">48. </s>
          <s xml:space="preserve">ligne 31. </s>
          <s xml:space="preserve">points liſez point</s>
        </p>
        <p rend="italics">
          <s xml:space="preserve">pag. </s>
          <s xml:space="preserve">74. </s>
          <s xml:space="preserve">ligne 1. </s>
          <s xml:space="preserve">puiſſnces, liſez puiſſances,</s>
        </p>
        <p rend="italics">
          <s xml:space="preserve">pag. </s>
          <s xml:space="preserve">99. </s>
          <s xml:space="preserve">ligne 14. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">pag. </s>
          <s xml:space="preserve">100. </s>
          <s xml:space="preserve">lignes 5. </s>
          <s xml:space="preserve">16. </s>
          <s xml:space="preserve">&amp; </s>
          <s xml:space="preserve">17. </s>
          <s xml:space="preserve">propotionnelles liſez <lb />proportionelles</s>
        </p>
        <p rend="italics">
          <s xml:space="preserve">pag. </s>
          <s xml:space="preserve">103. </s>
          <s xml:space="preserve">ligne 1. </s>
          <s xml:space="preserve">ces de liſez de ces</s>
        </p>
        <p rend="italics">
          <s xml:space="preserve">pag. </s>
          <s xml:space="preserve">104. </s>
          <s xml:space="preserve">ligne 6. </s>
          <s xml:space="preserve">69. </s>
          <s xml:space="preserve">M. </s>
          <s xml:space="preserve">liſez 69. </s>
          <s xml:space="preserve">de M.</s>
          <s xml:space="preserve" />
        </p>
        <p rend="italics">
          <s xml:space="preserve">pag. </s>
          <s xml:space="preserve">105. </s>
          <s xml:space="preserve">ligne 27. </s>
          <s xml:space="preserve">répoudent, liſez répondent,</s>
        </p>
        <pb facs="0188" />
        <pb facs="0189" />
        <pb facs="0190" />
        <pb facs="0191" />
        <pb facs="0192" />
        <pb facs="0193" />
        <pb facs="0194" />
        <pb facs="0195" />
        <pb facs="0196" />
      </div>
    </body>
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