# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1041163592:0423 # Permalink to this reading: https://leibnizlegible.com/page/1041163592:0423?run=74 # Title: [Philosophiae Naturalis Principia Mathematica] Philosophiæ Naturalis Principia Mathematica (shelfmark Leibn. Marg. 166) # Folio 389, page id 1041163592:0423 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1041163592&page=423 # Source image: https://digitale-sammlungen.gwlb.de/content/1041163592/jpgs/default/00000423.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 42 lines, status machine # Lines: 42 recognised, mean confidence 0.91 # 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. 1II PRINCIDIA MATHEMATICA. EFOD. LXVL,) quam in ipsius aphelio. Acque hae sune inaequali. L1 cates insioniores ab AArOnOmIS HOTaTA. Sunc etiam alix quaedam nondum obserrata inxqualitates, qui- bus motus l. unares adeo perturbantur, uc nulla hactenus legc ad Regulam aliquam certam reduei potuerint. Velocitates enim seu motus horarii Aporeei et Nodorum Lunx, et corundem aequati- ones, uc es dillerencia incer Lccentricicatem maximam in Syzygiis ee minimam in Ouadraturis, ec inaequalicas quae Variatio dicitur, augentur ac diminuuntur annuatim (per Corol. F4. PrOp. LXVL.) in triplicata ratione diametri apparentis Solaris. Et Variatio Pra- terea ausetur vel diminuitur in duplicata ratione temporis in- ter quadraturas quam proxime (per Corol. 1. ec 2. LCm. X. ee COrOl. 16. Prop. LXVI. Lib. l.) Scd haec inxqualicas in calculo Atronomico, ad Protthaphaerelin Lunae reterri Colet, et cum ca contundi. PROPOSITIO ZXIII. PROBLEMA V. Motus inaequales Satellitum fovis e Saturni a motibus Luna ribus derivare. Ex mocibus Lunxe noltrx motus analogi Lunarum seu Satelli- cum foris sic derirantur. Mocus medius Nodorum Sacellitis ex- timi Torialis, est ad motum medium Nodorum Lunxe nostra, in Fa- tione compolita ex ratione duplicata temporis. Periodici Perrre circa Solem ad cempus periodicum fovis circa Solem, de ratione simplici cemporis periodici Sacellitis circa Jorem ad tempus perio. dicum Lunx circa Terram: (per COrOl. 16. PFOP. LXVI.) adcoquo annis centum conticit Nodus iste 8e. 24. in ancecedencia. NIOFUS medii Nodorum Sacellicum inceriorum unt ad motum hujus, uE illorum tempora periodica ad cempus periodicum hujus, per idem Corollarium, de inde dantur. Motus autem Ausis Satellitis cu- jusque in consequentia, eA ad mocum Nodorum iplius in antece. dentia, uc motus Apogaei Lunae nostrae ad hujus mocum Nodo- rum, (per idem Corol.) se inde datur. Diminui tamen debet MOTUS Ausis sic inventus in ratione 5 2d 9 vel I ad 2 circiter, ob causam quam hic exxonere non vacat. Aequationes maximae No- dorum e Auxis Sacellicis cujusque Pere sune ad aequationes maxi- mas Nodorum et augis Lunxe respectire, ut mocus Nodorum et Aueis Satellicum tempore unius revolutionis aequationum prio. rUMs LERFIVS. GHIIIIHIEIIIEIIMIIIMSHAMISMIIIIIIII