# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1040780814:0397 # Permalink to this reading: https://leibnizlegible.com/page/1040780814:0397?run=74 # Title: [Astronomiae Physicae & Geometricae Elementa] Astronomiæ Physicæ & Geometricæ Elementa (shelfmark Leibn. Marg. 124) # Folio 379, page id 1040780814:0397 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1040780814&page=397 # Source image: https://digitale-sammlungen.gwlb.de/content/1040780814/jpgs/default/00000397.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 50 lines, status machine # Lines: 50 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. HII. SE CTEOMETRFCA E LEMENTA. PROPOSITIO LIX. Onae Maenitudinem definire. Ouoniam Lunx Distantia angulusque sub quo appatet ex Pla cedentibus cognita habentur, hoc est (reterente aBC Lunam, cu. jus centrum L, ∞0 oculum) recta or. e ansulus AOB, husuque proinde semissis AOL; in triansulo r a0 rectansulo ad a inre tur La Luna Semidiameter: vel brevius Sic: Diameter Lunx eAt ad Diametrum Ter ra ut Semidiameter L UMa aPPaFCNSCOS. nita ad notam Luna Parallaxin horizon talem, uti patet. Luna autem ipta est ad Ferram (Der PrOP. XVIII. EI. XH.) in triplicata ratione sux Diametri ad Diametrum Perra, ac proinde detinitur. O. H. V. Sacellitum Torialium ee Saturniorum Magnicudo similiter dofi- nietur ex cognitis Distantia ec ansulo quem quisque subtendit. PROPOSTTTO LX. Vancitatem materiae in Luna definire respectu duantitatis materice in Terra. Delionet s Solem; aBc Orbem magnum, in cuslls circumteren. tia commune centrum graritatis Telluris r e L una L. circumfer- tur, Sicut L ib. I. explicatum eAt. Sit a centrum iltud noto Tempore Nori. lunii cujusdam; B idem illud centrum Prove notum TempUS OuadraLEX eN. er. insequentis: AEque ex datis duo. bus hisce Temporibus dabuntur (ver PFOD. AVTIT. L Ib. TIT.) Solis LOCa Cx punctis a ex B rila: commune enim il. Jud Terra et Luna graritatis centrum (PeF PFOD. LXHT. L ib. T.) ita Orbem masnum peragrat, ut area per radios ad Solem ductos abscilta tine temporibus proportionales. ObTer. ventur Loca Solis et Luna c Tellure in + vila. Noti erso sunt an- Suli B+S, ASF: Sed prius innotuit ASB; ergo non latebit BSF. In triansulo isitur BSt datis angulis BFS, BSF e latere SB (Oebis magni lined ex Sole dueta e positione datd, in Terra Diameeris ex Solis Theoria _ Parallaxi cognita) innotescet e sD latus in iildem notis menturis: Sed ex Luna Theoria nota cA +V Distantia L una a Terra; nOta ersO CA (per F. Dat.) ratio inter YV _ FB, ad eoque inter BF, BI. POTIO, ex Mechanicis notistimum est candem esse rationem graricatis Luna versus longinquum Solem ad gravitatem Terra vertus cundem, hoc est (per CorOL. PrOP. XL. VIT. L ib. T) Ouantitatis materia in Luna ad Ouancitatem materia in Terra, at que rectae B+ ad BV rectam; definita ergo est ratio Ouantitatis ma- cerix in Luna ad Ouancitatem materia in Terra. O. R. F. BbD2 Tem. LatD. L1.