Huygens, Christiaan, Christiani Hugenii opera varia; Bd. 1: Opera mechanica

Table of figures

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[81] Fig. 4.N Q K C Q D L R E P F A Q G M Q Q H B Q
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[82] Pag. 136.TAB. XIX.Fig. 1.D C X B Y E R I Q L S N K P A TF G Y M H O
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[83] Fig. 2.X C D A T E R I Q L S N K P B Y
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[84] Fig. 3.F G K C D I E M A B D
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[85] Fig. 4.D K E F L B A H G C E
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[86] Fig. 5.D C K L F E A G H D B
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[87] Fig. 6.C D K F L E H G A D B
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[88] Pag. 142.TAB. XX.Fig. 1.D L F K A E G H C L K F D B
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[89] Fig. 2.D F K L C H E G A K F L D B
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[90] Fig. 3.L D C A E H G B L D
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[91] Fig. 4.D L C E A X V G H L D B
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[92] Fig. 5.T F K A V Q Z D E O B X P C Y f I G M L R N S H
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[93] Fig. 6.K E A H C L D F G B
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[94] Pag. 154.TAB. XXI.Fig. 1.G E G O A K L Q Q M M H F R R N N B D L K C P S V X Z Y X V T
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[95] Fig. 3.F A D E B C G H
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[96] Fig. 2.G E Ω O Ω S A S Q Q M M R R N X F N V P Φ Δ V B C K D Z
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[97] Pag. 156.Fig. 2.S F Z V O V L A Q Q M M I R R N N X T X K E K Y H G P B C D
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[98] Fig. 1.F H A E G B C
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[99] Fig. 3.C B A E D
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[100] Fig. 4.E F E D D D V O B A N C K H
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[101] Fig. 5.D D D E F E B A C H K
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[102] Pag. 160.Fig. 1.F D D @ N A L C H K M
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[103] Fig. 2.D D D F B A L C H K
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[104] Fig. 3.C A B
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[105] Fig. 4.B A K C E D G
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[106] G D E C A K B
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[107] G D K C A B
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[108] Fig. 5.K B K A C E D F
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[109] Fig. 6.Q B Q O N A C E D R P F
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[110] Pag. 164.Fig. 1.G B O N C R P F
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8552CHRISTIANI HUGENII
Ponatur grave C è quiete dimiſſum, certo tempore,
11De de-
SCENSU
GRAVIUM.
TAB. IV.
Fig. 3. quod dicatur F, vi gravitatis tranſire ſpatium C B. Ac
rurſus intelligatur idem grave accepiſſe alicunde motum quo,
ſi nulla eſſet gravitas, transiret pari tempore F motu æqua-
bili lineam rectam C D. Accedente ergo vi gravitatis non
perveniet grave ex C in D, dicto tempore F, ſed ad pun-
ctum aliquod E, recta ſub D ſitum, ita ut ſpatium D E
ſemper æquetur ſpatio C B, ita enim, & motus æquabilis,
& is qui à gravitate oritur ſuas partes peragent, altero alte-
rum non impediente. Quamnam vero lineam, compoſito il-
lo motu, grave percurrat, cum motus æquabilis non recta
ſurſum aut deorſum ſed in obliquum tendit, è ſequentibus
definiri poterit. Cum vero deorſum in perpendiculari con-
tingit motus æquabilis C D, apparet lineam C D, acce-
dente motu ex gravitate, augeri recta D E. Item, cum ſur-
ſum tendit motus æquabilis C D, ipſam C D diminui recta
D E, ut nempe, peracto tempore F, grave inveniatur
ſemper in puncto E. Quod ſi, utroque hoc caſu, ſeorſim,
uti diximus, duos motus conſideremus, alterumque ab al-
tero nullo modo impediri cogitemus, hinc jam acceleratio-
nis gravium cadentium cauſam legesque reperire licebit. Et
primum quidem duo iſta ſimul oſtendemus.
PROPOSITIO I.
ÆQualibus temporibus æquales celeritatis par-
tes gravi cadenti accreſcere, & ſpatia æqua-
libus temporibus ab initio deſcenſus emenſa, augeri
continue æquali exceſſu.
Ponatur grave aliquod, ex quiete in A, primo tempore
22TAB. V.
Fig. 1. lapſum eſſe per ſpatium A B, atque ubi pervenit in B, ac-
quiſiviſſe celeritatem qua deinceps, tempore ſecundo, mo-
tu æquabili, percurrere poſſet ſpatium quoddam B D. Sci-
mus ergo ſpatium ſecundo tempore peragendum majus fore
ſpatio B D, quia vel ceſſante in B omni gravitatis

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