Newton, Isaac
,
Philosophia naturalis principia mathematica
,
1713
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<
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>Reſiſtentia quam patitur a Fluido ſruſtum Co
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nicum, qua ratione fiat minima 299, 30 </
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>Reſiſtentiæ minimæ Solidum 300, 15. </
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S.
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<
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>Satellitis</
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<
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>Jovialis extimi elongatio maxima heliocentrica
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a centro Jovis 370, 35 </
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Hugeniani
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elongatio maxima heliocentrica a
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centro Saturni 371, 5 </
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>Satellitum </
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<
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>Jovialium tempora periodica & diſtantiæ a
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centro Jovis 359, 12 </
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<
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>Saturniorum tempora periodica & diſtantiæ a
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centro Saturni 360, 1 </
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<
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>Jorialium & Saturniorum inæquales motus
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a motibus Lanæ derivari poſſe oſſenditur
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III, 23 </
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>Saturni </
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>diſtantia a Sole 361, 1 </
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>ſemidiameter apparens 371, 9 </
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>ſemidiameter vera 371, 14 </
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<
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>vis attractiva quanta ſit 370, 33 </
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<
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>pondus corporum in ejus ſuperficie 371, 19 </
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<
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>denſitas 371, 37 </
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<
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>quantitas materiæ 371, 27 </
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<
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>perturbatio a Jove quanta ſit 375, 16 </
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<
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>diameter apparens Annuli quo cingitur 371, 8 </
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>Sectiones Conicæ, qua lege vis centripetæ ten
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dentis ad punctum quodcunQ.E.D.tum, deſcri
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buntur a corporibus revolventibus 58, 20 </
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>Sectionum Conicarum deſcriptio Geometrica </
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>ubi dantur Umbilici I, Sect. </
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>4 </
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>ubi non dantur Umbilici I, Sect. </
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>5. ubi dan
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tur Centra vel Aſymptoti 87, 9 </
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<
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>Seſquiplicata ratio definitur 31, 40 </
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>Sol </
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<
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>circum Planetarum omnium commune gravi
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tatis centrum movetur III, 12 </
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<
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>ſemidiameter ejus mediocris apparens 371, 12 </
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>ſemidiameter vera 371, 14 </
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<
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>parallaxis ejus horizontalis 370, 33 </
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<
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>parallaxis menſtrua 376, 4 </
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<
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>vis ejus attractiva quanta ſit 370, 33 </
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<
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>pondus corporum in ejus ſuperficie 371, 19 </
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<
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>denſitas ejus 371, 37 </
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>quantitas mater æ 371, 27 </
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<
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>vis ejus ad perturbandos motus Lunæ 363,
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15: III, 25 </
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>vis ad Mare movendum III, 36 </
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>Soaorum </
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>natura explicatur II, 43, 47, 48, 49, 50 </
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<
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>propagatio divergit a recto tramite 332, 9,
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fit per agitationem Aeris 343, 1 </
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<
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>velocitas computo colligitur 343. 8, paulu
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lum major eſſe debet Æſtivo quam Hyber
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no tempore, per Thecriam 344, 11 </
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>ceſſatio fit ſtatim ubi ceſſat motus corporis
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ſonori 344, 29
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<
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>augmentatio per tubos ſtenterophonicos
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344, 32 </
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<
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>Spatium </
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<
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>abſolutum & relativum p. </
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>6, 7 </
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<
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>non eſt æqualiter plenum 368, 16 </
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>Sphæroidis attractio, cujus particularum vires
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ſunt reciproce ut quadrata diſtantiarum
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198, 21 </
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>Spiralis quæ ſecat radios ſuos omnes in angulo
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dato, qua lege vis centripetæ tendenti ad
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centrum Spiralis deſcribi poteſt a corpore
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revolvente, oſtenditur I, 9: II, 15, 16 </
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>Spiritum Q.E.D.m corpora pervadentem & in
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corporibus latentem, ad plurima naturæ phæ
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nomena ſolvenda, requiri ſuggeritur 484, 17 </
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>Stellarum fixarum </
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<
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>quies demonſtratur 376, 18 </
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<
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>radiatio & ſcintillatio quibus cauſis referendæ
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ſint 467, 38 </
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<
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<
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>Stellæ Novæ unde oriri poſſint 481, 5 </
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<
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>Subſtantiæ rerum omnium occultæ ſunt 483, 22 </
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T.
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<
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>Tempus abſolutum & relativum p. </
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<
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>5, 7 </
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<
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>Temporis Æquatio Aſtronomica per Horolo
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gium oſcillatorium & Eclipſes Satellitum Jo
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vis comprobatur 7, 15 </
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<
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<
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>Tempora periodica corporum revolventium in
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Ellipſibus, ubi vires centripetæ ad umbilicum
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tendunt I, 15 </
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>Terræ </
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<
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>dimenſio per
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Picartum
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378, 11, per
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Caſſinum
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378, 21, per
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Norwoodum
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378, 28 </
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<
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<
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>figura invenitur, & proportio diametrorum,
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& menſura graduum in Meridiano III,
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19, 20 </
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<
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<
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>altitudinis ad Æquatorem ſupra altitudinem ad
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Polos quantus ſit exceſſus 381, 7: 387, 1 </
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<
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>ſemidiameter maxima, minima & mediocris
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387, 10 </
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<
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<
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>globus denſior eſt quam ſi totus ex Aqua con
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ſtaret 372, 31 </
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<
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<
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>globus denſior eſt ad centrum quam ad ſuper
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ficiem 386, 1 </
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<
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<
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>molem indies augeri veroſimile eſt 473, 18
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481, 13 </
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<
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<
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>axis nutatio III, 21 </
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<
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<
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>motus annuus in Orbe magno demonſtratur
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III, 12, 13: 478, 26 </
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<
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<
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>Eccentricitas quanta ſit 421, 15 </
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<
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<
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>Aphelii motus quantus ſit 376, 33. </
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<
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V.
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<
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>Vacuum datur, vel ſpatia omnia (ſi dicantur
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eſſe plena) non ſunt æqualiter plena 328, 18:
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368, 25 </
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