Newton, Isaac
,
Philosophia naturalis principia mathematica
,
1713
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Apogæo Solis, Variatio maxima eſt 33′. </
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>14″, & in ejus Perigæo
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37′. </
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>11″, ſi modo Eccentricitas Solis ſit ad Orbis magni ſemidia
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metrum tranſverſam ut (16 15/16) ad 1000. </
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LIBER
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TERTIUS.</
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>Hactenus Variationem inveſtigavimus in Orbe non eccentrico,
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in quo utique Luna in Octantibus ſuis ſemper eſt in mediocri ſua
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diſtantia a Terra. </
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<
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>Si Luna propter eccentricitatem ſuam, magis
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vel minus diſtat a Terra quam ſi locaretur in hoc Orbe, Variatio
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paulo major eſſe poteſt vel paulo minor quam pro Regula hic
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allata: ſed exceſſum vel defectum ab Aſtronomis per Phænomena
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determinandum relinquo. </
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PROPOSITIO XXX. PROBLEMA XI.
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Invenire motum borarium Nodorum Lunæ in Orbe circulari.
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<
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>Deſignet
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S
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Solem,
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T
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Terram,
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P
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Lunam,
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NPn
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Orbem Lunæ,
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Npn
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veſtigium Orbis in plano Eclipticæ;
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N, n
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Nodos,
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nTNm
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lineam Nodorum infinite productam;
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PI, PK
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perpendicula de
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miſſa in lineas
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ST,
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perpendiculum demiſſum in planum </
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