# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1041163592:0439 # Permalink to this reading: https://leibnizlegible.com/page/1041163592:0439?run=74 # Title: [Philosophiae Naturalis Principia Mathematica] Philosophiæ Naturalis Principia Mathematica (shelfmark Leibn. Marg. 166) # Folio 405, page id 1041163592:0439 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1041163592&page=439 # Source image: https://digitale-sammlungen.gwlb.de/content/1041163592/jpgs/default/00000439.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 43 lines, status machine # Lines: 43 recognised, mean confidence 0.89 # 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. PRINOIPLA MATHEMATICA. 40 Designet jam. P M arcum; quem Luna dato tempore quam LIvEn minimo describie, ec ML. lincolam quam Luna, impellence vi TEnrIVS. praetata 3TT, eodem tempore describere posset. Junsantue F L MIF, e producantur cx ad m ec l. ubi secent planum l elipeicae; inque Tm demittatur perpendiculum P HI. lC quo- niam recta MC. Parallela est plano Lclipricae, ideoque cum recta mt quae in plano illo jacet concurrere non porest, ex tamen ja- cent hae rectae in plano communi L. MD ml; Parallelae crunt hxe rectae, de propterea similia crune triangula L. MF, Lmp. Jam. cum MP m sic in plano Orbis, in quo Luna in loco F moreba- tur; incidec punctum m in lineam dn per Orbis illius Nodos. N,n ductam. Ec quoniam vis qua lincola L. M genCrATUE, (I tora simul ex semel in loco P imprecta cHet, CfCCreE uE L una moreretur in areu, cujus chorda cAet L. P, aeque adeo EraNS. Ferree Lunam de plano MF mT in planum L P VT; mOrUS an sularis Nodorum a vi illa genicus, aequalis erit angulo mTI. Fst autem nb ad m F UE ML ad MF, adeoque cum MF ob da- cum cempus daca siC, CR mI uE rectangulum M L X M F, id cA, ut rectangulum ITXm P. Ec angulus m FI, si modo angulus E TmD rectus SIC, CAt UE X dC PFOPECrCA UE TX Fn (ob proportionales Tm et m F, TF et PII Im id CAt, adeoque ob datam TP, uE TYX P FI. Ouod A angulus T mh Peu ST N obliguus sic, eric angulus mTV adhuc minor, in rati- one linus anguli ST N ad Radium. FA igitur velocitas NO- dOrUM UE TTZ P FIZ AZ, sive ut contentum sub sinubus crium angulorum TPL, FTN e STN. Si anguli illis Nodis in Ouadracuris ee Luna in Syzygia existen. tibus, recti sine, lineola mi abibie in infinitum, ee angulus mZl eradet angulo m PV aequalis. Hoc aucem in casu, angulus m F est ad angulum F F M, quem Luna eodem tempore motu uo apparente circa Terram deseribit uc 2 ad 59,575. Nam angulus im Fb aequalis est angulo L. F M, id est, ansulo deRexionis Lunx a recto eramite, quem sola vis praetara Solaris 3TF A cum cesta- ret Lunae gravitas dato illo rempore generare pollet; ec angulus P TM aequalis est angulo defexionis Lunae a recto cramite, quem vis illa, qua Luna in Orbe suo recinetur, si cum cellaret vis Sola- rio 3YZ EOAEM LEPOTE SCMETArET LC ha VireS, ut supra dixi MUSs