# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1040780814:0284 # Permalink to this reading: https://leibnizlegible.com/page/1040780814:0284?run=74 # Title: [Astronomiae Physicae & Geometricae Elementa] Astronomiæ Physicæ & Geometricæ Elementa (shelfmark Leibn. Marg. 124) # Folio 266, page id 1040780814:0284 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1040780814&page=284 # Source image: https://digitale-sammlungen.gwlb.de/content/1040780814/jpgs/default/00000284.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 50 lines, status machine # Lines: 50 recognised, mean confidence 0.95 # Machine transcription. Not an edition. Errors are expected: about 8% character error rate on Latin and French lines, higher on German. # Licence: CC BY 4.0, Leibniz Legible. Machine output: do not ingest it as verified text; keep this provenance with the text. # Wording rule: say "the machine reads it as …", never "Leibniz wrote". # After the first blank line: the recognised lines in reading order, one per line. 266 ASTRONOMLE PAYSTCA Lib. III. tionem rectae Sr ad Pa: Onde Ouantitas Mrateria in S ost ad Onan. titarem Materia in P in ratione composita ex triplicata ratione sv ad ead duplicata ratione Temporis periodici Satellitis a circa P ad Tempus periodicum Primarii r circa Solem. Vtraque autem com- Donens ratio datur; nempe ratio sr ad e a per praemistuum Lemma, ipla Tempora periodica per obserrationem: non latebit isitur ratio composica; nempe ratio Ouantitatis Materia in Sole ad Ouan. titatem Materix in Primario P. Frinc invenietur ratio Ouanticatis Materia in Planetis tribus Sa- tellitio donatis; inveniendo sc. rationem Ouantitaris Mlateria in il- lorum unoquoque ad Ouantitatem Materix in Solc. SCHOLTOM. Similiter inrenietur ratio Graritatis Acceleratricis in Superticie Solis ad Graritarem Acceleratricem in Puperficie cujurris Planetae Satellitem habentis. HTabentur enim ratio Crravitatis in superticie Solis ad Craritatem in V, duplicata sc. rationis Dictantia sr ad Semidiametrum Solis ex praecedentibus cognita, et ratio Gravi tatis in r versus solem ad Graritatem in A vertuS Planetam, in- renta ut supra; item ratio Graritatis in a ad Graritatem in Cuper. ficie Planeta e, duplicata nota rationis quam habet Semidiameter Planeta ad Distantiam Satellitis à Primario. Liguet iam rationem ex tribus hisce notis rationibus compositam eandem ese cum ra- tione Craritatis in superticie Solis ad Graritatem in superticie Pla neta P. Et hinc rursus, ex aquo, determinabitur rario CTravitatis in superticie unius Planctae ad Graritatem in superticie alteriuS, si uterque Satellite saudet. PROPOSITIO ZLIX. Dvenire rationem Densitatis Sols ad Densitatem Planetae eu Ljusvis Primarii, circa quem Satelles revolvitur. Si duo COrpOra A _ B sinE ejusdem magnicudinis, patet quanti- tatem materiae in a eAe ad quancitatem materiae in B ut dentitas iptius a ad densitatem ipsus e: FF si ejusdem Fuerint densitatis, quantitas materix in a est ad quantitatem materia in B ut COrPO. ris a magnitudo ad magnitudinem corporis B: EF isitur, licet neque magnitudines neque dentitates aequentur, ratio quantitatis materiae in a ad quantirarem materia in B componitur ex directa ratione densitatum ec directa ratione masnitudinum corundem. Unde ratio densitatis corporis a ad densitatem corporis B compo. nitur ex ratione quantitatis materia in a ad quantitatem materia in B, _ ratione masnitudinis corporis B ad magnitudinem corporis A; hoc cA (in casu praesenti) Densitas Solis est ad Denlitatem Planeta in ratione composita ex ratione Ouantitatis Materia in Sole ad Ouantitatem Materia in dicto Plancta, _ ratione MaSHI tudinis Planeta ad Magnicudinem Solis. Sed (per PTOP. PFaC.) da cur componentium rationum prior, s Planera Satellite saudet; dri it