# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/00068532:0130 # Permalink to this reading: https://leibnizlegible.com/page/00068532:0130?run=74 # Title: Leibniz-Handschriften zur Physica LH 37, 3 # Folio 67v, page id 00068532:0130 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=00068532&page=130 # Source image: https://digitale-sammlungen.gwlb.de/content/00068532/jpgs/default/00000130.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 44 lines, status machine # Lines: 44 recognised, mean confidence 0.92 # 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. conatus AC, BC, concurcunt in C certio Circuli. Quod si id non sit tentum grovitilis sed aliud G, sit tamen C in directine ipsius G, perinde est ac sicentum p. quoque esset in G si ei sit baculus BCG, et sit impulsus in BC, grave autem sit in altero extremo G. An idem est at si impulsus fieret in FG paralleta ipsi BC sed hinc porro sequitur, si motus ille directus in lineaB oriatur excirculari circa centim M, interesse itium gravesit in C an vero in G. quia C vecti MFB accu incumbet hi B at G inF, propius ad centrum. Hinc etsi MB et Ns sint aequalet si tamen centrum grav. sit in G. multum interest, utrum centrum motus sit x, an M, quia cungis ab N abest quam b M. Hoc prima ponte non apparebat. at huc video non posse tuto motus circulares pro conptibus rectiliners substitui, etsi illiee circulare, quoque sint rectitiali in tangente si obe baculi (BC G grave G impellatur linea BC perinde est quasi impulsus factus curvr vi ponderis g. fuisset linea FG, quia in hac linea dit ipsum grave c 1 tendit 1C si A incurrat in B et C. ita tamen ut tantum tangat B, quid fiet. summa virium data est A VP + BCe + (G ((A) = v (B) (B) = e celeulas et directio centri grav. (C) (C7 = n commuris manet, seu quadratum ejus ductum in Aggregatum Manere etiam debet eadem vic respectiva, Si ope horum determinari res potestr ut intertior determi abrti detaitum eadem prodibunt quae prodirent si ponamus esse intervalum inter B et C, sed utcunque exiguum. Nam sed ea ratione semper quiescet A pust iclum si B et C non colae- reant oft sed quid si Cohaereant 2 tunc omnis vis respectiva redibit ad solum conatum discedendi centri BC ab A. Ergo haec duo confunti non debent. Sed s. non cohareant pars vis respectivae redacta erit ad recessum inter B et B et C. Si globus A symul tangat erlobos aequales plures C. et feriatur a globo B, post ictum quiescent B et A, mojusque oonis erit translatus in globos C. rug. C. 1. Lum Erjo puto idem esse si A incurrat in Cec aequales, sumamus duos samtum et consideremus quid fulam. debet eadem esse celentuusum vis in summa a qua si detraratur vis centri gravitatis lestatit vis ictus quem examinemus. Videbum et auide prodeat, si paulo ante attiuut (quam d