# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1041163592:0447 # Permalink to this reading: https://leibnizlegible.com/page/1041163592:0447?run=74 # Title: [Philosophiae Naturalis Principia Mathematica] Philosophiæ Naturalis Principia Mathematica (shelfmark Leibn. Marg. 166) # Folio 413, page id 1041163592:0447 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1041163592&page=447 # Source image: https://digitale-sammlungen.gwlb.de/content/1041163592/jpgs/default/00000447.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 43 lines, status machine # Lines: 43 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. PRINCTPTA MATETEMAETEA. 4 13 cus medius Nodorum circulo tori respondens. Et motus Nodo- L. IBEK rum, quo cempore Sol vergit ab N ad , CA act 1961. 49. 3. 55. TERTIVS. ut arca NA Z ad circulum cOrUM. IIaec ita se habene, ex Hypochesi quod Nodus horis singulis in locum priorem retrahitur, lic ue Sol anno toro completo ad No- dum cundem redeat a quo Cub inicio digrestus fuerac. Verum per motum Nodi AC uE Sol cicius 2d NTOdum ROVENEAEUE, et compu- eanda jam es abbreviatio temporis. Cum Sol anno toro conticiae 360 gradus, ec Nodus motu maximo codem. tempore conticeret 395r. 38. 71. 50, Tcu 39,6355 gradus; et motus: mediocris Nodi in loco quovis N ic ad ipsius motum mediocrem in Ouadraturis SuIS, UE A Z 9 ad ATg: erit motus Solis ad morum Nodi in NV, ut 360 AT9 ad 39,63554Z9; id elt,. ut 9,0827646 A. T9 2d A2, 9. Onde si circuli corius circumferencia N An diridatur in particu- a5 aequales Aa tempus quo Sol percurrac parriculam A a, s cir- culus quielceret, erit ad tempus quo percurrit eandem parri culam. Si circulus una cum Nodis circa cenerum Y revolvatur, reciprOCC UE 9,0827646 ATg ad 9, 0827646 ATg + AZ 9. Nam cempus est reciproce ut relocitas qua particula percurritur, de haec relocitas est summa relocicatum Solis et Nodi. Igieur A cem- Dus, quo Sol absque motu Nodi perCurrCret arcum NV A, exPO- natur per Sectorem NI A, _ Particula tempOrIS qUO PCTCUEFCRCE arcum quam minimum Aa exponatur per Sectoris particulam ATa; ex (perpendiculo aY in NVn demisto) si in AZ capiatur aZ, ejus longitudinis ut sic rectangulum dZ in Z V ad Sectoris parciculam AT a ue AZ9 2d 9,0827546 ATg + AZ 9, id CAt, uE AC aZ 2d 2 AZ uE AT g 2d 9,0827646 AF9 + AZ g; rectangu- lum aZ in Q Y delignabit decrementum temporis ex moru Nodi Oriundum, TeMPOTC EOTO quo arCUS Aa PCFCUrrIEUF. EC Si pun- ctum a tansit Curvam NdCn arca curvilinca Nd Z crit decre- MENEUM FOTuM, quo temPOrC arCUS EOtuS N A percurritur; et propterea excessus Sectoris N AY supra aream N d Z erit tempus illud Eorum. F.F quoniam motus Nodi cempore minore minor cst in ratione cemporis, debebit etiam arca Aa Y Z diminui in cadem ratione. Id quod AcE si capiatur in AZ longitudo eZ, guxe BF ad lonsitudinem AZ ut A29 ad 9,0827646 ATg + AZ g. Sic enim rectangulum e. Z in Z Y erit ad aream AZ Ta ut decremen- tum temporis quo areus A PCrCUrRItUT, ad tempuS EOtuM quo Percurreretur A Nodus quielceret: EF propterea rectangulum illud respondebit decremento motus NVodi. EF S punctum e tansaE Curram