# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/00068160:0004 # Permalink to this reading: https://leibnizlegible.com/page/00068160:0004?run=74 # Title: Leibniz-Handschriften zur Mathematik LH 35, 10, 7 # Folio 2v, page id 00068160:0004 # Scan: One image of two folio pages side by side, registered by the library under both labels (also fol. 3r); this page is its left half. # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=00068160&page=4 # Source image: https://digitale-sammlungen.gwlb.de/content/00068160/jpgs/default/00000004.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 48 lines, status machine # Lines: 48 recognised, mean confidence 0.86 # 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. posisa B temporis et ad. ara Vis in centriguga, _ fit est = K: Y. jam R = C g: Y: go vis veninifina elemento seu Triangulo a seu L. interu itu Erc latus rectum est ad: r: jam si vis centripeta seu gravitas sit B m _ FK: L seu LP: YR. seu (si L=d) a D: x fiet descensus integeree ne seu ddr a D a aB = aD r et fiet de dar de dfiet seu adr = LD2. pr - 40: 1. et fiet S ddr = ad Str. = (B far: 12. Et Z av = L St posito D temporis incrementum et ad area seu Triangulem conssans jam vis centrifuga K:Y. Et in casu R aream aequalium est K = ab: Y. (posito radio Y) fiet _vis ceatrifuga a B: ro. rusus vis centripeta seu gravitas n, sit K: L. et L= 2a. posito L esse latus redum fiet primarium, siet. a b: rar seu ad: 2r. jam aar nova vis descendendi integra ova, est diffeaentia vis centripeto et centrifugae et ergo fiet ddr = ad: 2Y = ab. r et fet. dr ddr = Dai SIr: 2r= asdrir, ot fil denque summando dr d Bd, 1: fr = a. r. f Et fier D= ar r: Sar aa et ( seu lequs = (arr. sar- au sit ter sar-aa = e ef v sit r = v + a: a, et dr = 2v dv + a,: a, et fit: E tempus = (2p dv: x F, (ae dv: v sn tempus = 2V + a Lv: v eerum hoc obistat, quod Y radius non incipit ab infinite parvo. Ergo pro Y scribamus Z- h posita h distantias ambilici a vertice et fict dze =dar et daz-dar, et aequatiuo ita stabit 1Z ddque = A a D: 2Z - 27 +s - a 0: Z.h et jum s dq Z hi = S AN: r = fia 1: Y et saZ Z hi = h, - 1 : 7 et fil LF iadque Z - 2 1B. h- a Br (pDh) +0a seu _sta 4z. E. b: s h 2. h - a 2. h + a, = b si sint temporam quadrata ut cubi radiorum, D2= t E h -Z. Ergo 1- fiet. si planetae ferantur in v circa jovem; irculis sintus temporum nquadrata, ut cubi distantiarum erit et tempori sint areis ex etuit centro proportianalia, e sectorm (AB. C1A(B) quadrata ut id est radiorum CA, C) quadrato quadrala, proportionalias ubis suis quod est abstudum. Ergo si moventur in circulis non possunt tempora habere areis proportionalia, quod si habent, necesse est et ae ut non in circulis, sed Eterpsibus ferantur. verunt si planetoer joris ince quales, sntue clegento