# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1041163592:0431 # Permalink to this reading: https://leibnizlegible.com/page/1041163592:0431?run=74 # Title: [Philosophiae Naturalis Principia Mathematica] Philosophiæ Naturalis Principia Mathematica (shelfmark Leibn. Marg. 166) # Folio 397, page id 1041163592:0431 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1041163592&page=431 # Source image: https://digitale-sammlungen.gwlb.de/content/1041163592/jpgs/default/00000431.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 45 lines, status machine # Lines: 45 recognised, mean confidence 0.90 # 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. I1 PRINOIDIA MATHEMATICA. Tumma senita, id est, ut acceleratio de scriptionis arex CZ P, (CW L LVEK incremencum momenti. Vis qua Luna circa Terram quiescentem YExxIVS. ad distanciam F P, tempore suo periodico CAD BC dierum 27. hor. 7. min. 4.3. rerolvi DoNeE, CHICCrCE UE COrpUS, tempOre CL cadendo, delcriberet lonsitudinem =C F, e velocicarem simul aequireret aequalem relocitatis qua Luna in Orbe suO MOVCTUI. Patet hoc per Corol. 9. Prov. Ir. Lib. l. Cum autem perpen- diculum Xa in T F demissum (IE ipBUS F L ParS certia, e ip. AuS TD seu M L. in Octantibus pars dimidia, vis PL. in Octan- tibus, ubi maxima est, superabie vim MI. in racionc 3 2d 2, adeoque erit ad vim illam, qua Luna tempore luo periodico circa Terram quiescentem revolvi posset, ut 100 4d 3X 178722 Peu TI9T5, et tempore C. F relocitatem generare deberet quae cACE pars igrs velocitatis Lunaris, tempore autem C F A velociratem 100 majorem generaret in ratione C A ad CF (Cu TP. ExPONatuE vis maxima F L. in Octantibus per arcam FRX Rk rectangulo ETPX Pp aequalem. Ec relocitas, quam vis maxima tempore quoris CF gencrare poslet, erit ad relocitatem quam vis omnis minor P.L. eodem tempore generat, ur rectangulum 2T PXC P ad aream RCCF F: TCMPOTE aULEM EOEO C F A, velocitates se- nicae crune ad inricem ue rectangulum =T P XC A ec triangulum TCC, Sive ut arcus quadrantalis C A e radius FP. Ideoque (Per PrOP. IX. Lib. V. Elem.) relocitas PoleriOE, FOtO tempOrO 700 genitas erit pars =19r velocitatis Lune. Hluic Lunae velocitatis quae arexe momento medioeri analosa eA, addatur e auteratur dimidium relocitatis alcerius; ec Ei momentum medioere expona- CuE per numerum 119I5, Tumma 219Y5 + 50 Tcu 11965 exhri- bebie momentum maximum arex in Syzygia A, ac differentia 21915 = 50 (cu 11865 ejusdem momencum minimum in Ouadra- curis. Isitur arex temporibus aequalibus in Syzygiis ec Guadra- curis descripea, sune ad inricem ut 11965 ad 11865. A. d mo- mencum minimum 17865 addatur momentum, quod sIc ad mo- mentorum differentiam 100 uc trapezium FKCC C ad triangu- Jum FCG (vel quod perinde eA, uc quadratum Sinus FR ad quadratum Radii TP, id eAt, uc Pd. ad ZF) e summa extri- bebit momencum arexe, ubi Luna est in loco quoris interme- dio F. Hxec omnia ita se habene, ex Hypocheli quod Sol et Terra qui- elcune, et Luna cempore Synodico dierum 27. Bor. 7. min. 43. re- volvIII. Cum autem periodus Synodica LUnaTIS VerC lC d rum