Newton, Isaac
,
Philosophia naturalis principia mathematica
,
1713
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Quadraturis, & ad
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AD
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demittatur perpendiculum
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GH
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: erit
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AH
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ſinus Inclinationis quæſitæ. </
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LIBER
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TERTIUS.</
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<
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>Nam
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GEq
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æquale eſt
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GHq+HEq=BHD+HEq=
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HBD+HEq-BHq=HBD+BEq
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-2
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BHXBE=
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BEq
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+2
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ECXBH
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=2
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ECXAB
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+2
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ECXBH
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=2
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ECXAH.
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Ideoque cum 2
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EC
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detur, eſt
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GEq
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ut
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AH.
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Deſignet jam
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AEg
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duplicatam diſtantiam Nodorum à Quadraturis poſt datum ali
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quod momentum temporis completum, & arcus
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Gg.,
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ob datum
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angulum
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GEg,
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erit ut diſtantia
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GE.
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Eſt autem
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Hh
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ad
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Gg
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ut
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GH
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ad
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GC,
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& propterea
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Hh
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eſt ut contentum
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GHXGg,
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ſeu
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GHXGE
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; id eſt, ut
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(GH/GE)XGEq
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ſeu
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(GH/GE)XAH,
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id eſt,
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ut
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AH
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& ſinus anguli
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AEG
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conjunctim. </
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<
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>Igitur ſi
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AH
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in
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caſu aliquo ſit ſinus Inclinationis, augebitur ea iiſdem incremen
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tis cum ſinu Inclinationis, per Corol. </
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<
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>3. Propoſitionis ſuperioris,
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& propterea ſinui illi æqualis ſemper manebit. </
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<
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>Sed
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AH
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ubi
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punctum
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G
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incidit in punctum alterutrum
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B
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vel
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D
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huic ſinui
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æqualis eſt, & propterea eidem ſemper æqualis manet.
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Q.E.D.
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<
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>In hac demonſtratione ſuppoſui angulum
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BEG,
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qui eſt du
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plicata diſtantia Nodorum à Quadraturis, uniformiter augeri. </
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Nam omnes inæqualitatum minutias expendeve non vacat. </
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<
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>Con
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cipe jam angulum
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BEG
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rectum eſſe, & in hoc eaſe
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Gg
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eſſe
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augmentum horarium duplæ diſtantiæ Nodorum & Solis ab invi
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cem; & Inclinationis Variatio horaria in eodem caſu (per Corol. </
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3. Prop. </
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<
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>noviſſimæ) erit ad 33′. </
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>10′. </
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>33
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iv
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. </
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<
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>ut contentum ſub In
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clinationis ſinu
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AH
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& ſinu anguli recti
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BEG,
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qui eſt dupli
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cata diſtantia Nodorum a Sole, ad quadruplum quadratum radii;
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id. </
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>eſt, ut mediocris Inclinationis ſinus
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AH
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ad radium quadru
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plicatum; hoc eſt (cum Inclinatio illa mediocris ſit quafi 5
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gr.
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8′1/2)
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ut ejus ſinus 896 ad radium quadruplicatum 40000, ſive ut 224
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ad 10000. Eſt autem Variatio tota, ſinuum differentiæ
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BD
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reſpondens, ad Variationem illam horariam ut diameter
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BD
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ad </
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