# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1040780814:0281 # Permalink to this reading: https://leibnizlegible.com/page/1040780814:0281?run=74 # Title: [Astronomiae Physicae & Geometricae Elementa] Astronomiæ Physicæ & Geometricæ Elementa (shelfmark Leibn. Marg. 124) # Folio 263, page id 1040780814:0281 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1040780814&page=281 # Source image: https://digitale-sammlungen.gwlb.de/content/1040780814/jpgs/default/00000281.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 47 lines, status machine # Lines: 47 recognised, mean confidence 0.92 # 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. itol Lib. Ilc. LHEOMETRTOA E, LEMENTA. L05 metrum Terra; eadem nempe (per PFOP. HEVT. T ib. H.) quae eAt inter sinum Distantix apparentis à vertice et sinum Parallaxis. Atqui (per PFOP. XXXV.) datur ratio inter Distantiam Planetae d cen- tro Terrae e ejusdem Distantiam à Sole ad Tempus iltud corni- tum; e (ex superioribus) ad idem Tempus datur ratio Distantia Planetae à Sole ad Orbita Axem majorem ejusque Fxcentricitatem _C: Ft isitur, ex aquo _ per 2. Dat, dabitur ratio iltarum recta- rum ad Terra Diametrum; hoc est, dabuntur omnes ilta Orbita- rum dimetientes recta per Perrx Diametros exprecta. Cumque ex Scholio Prop. XVII. Lib. II. Perra Diameter cognita sit in mensuris notis et tamiliaribus, dabuntur etiam praedicta Orbitarum recta in iisdem. Hinc ad Tempus propositum Distantia Solis de Planetarum pri. mariorum a Terra per Terra Semidiametros aliatre menturas no- tas expresa innoteleunt: Nam ad dictum Tempus distantix istae exprecta in partibus medioeris Distantix Perrx a Sole notae sunt DeT PFOPP. XXXIV. _E XXXV, _ (per hanc) dicta medioeris Distantia Perra à Sole in notis mensuris cognita eAt. SFCTTOV De Magnitudine Densitate Solis Pla- netarum primariorum. PROPOSITIO ZLVI. Olis Planetarum primariorum Maerdea te Contonum est ut hoc loco, post traditam Planctarum Lhcorrat agamus etiam de illorum Nlagnicudine Densitate, ex quibus con- junetim Ouantitas Materia in sinsulis pendet; praesertim cum qua dam in eorum Notu Orbiumque dimentione hinc rectiticanda veniant. Sit horum aliquis aBC, cujus centrue, ue O OcutS ODIet vantis. Junsatur recta op, per quam ductum intelligatur planum secans Solis vel Planetae corpus Sphaericum in ejus circulo maximo BAC. L.x O ducantur rectae hunc tangentes oA, OB, _ jungatur Pa recta. Ansulus a0B idem est cum dicti corporis Diametro apparenti ex o, secatur. que hic bitariam per oe rectam. Obserre. tur haec per methodos Astronomis Patis notas, quo pacto in trianoulo aor noti erunt omnes anguli: nam (PeF PrOP. XVT. LL. TIT.) a eAt rectuS, _ aoP est obserratae Diamerri apparentis lemistis; unde innotescit ratio laterum oP _ AB: Sed (PET PFOD. XLV.) datur ratio inter Terra Semidiametrum ex Ox PI2. neta Distantiam; ex isitur, ex aquo, datur ratio inter Semidiame. tros Terrae _ Planeta; ergo et hujus triplicata etiam est data, nempe