# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/00068029:0003 # Permalink to this reading: https://leibnizlegible.com/page/00068029:0003?run=73 # Title: Leibniz-Handschriften zur Mathematik LH 35, 5, 11 # Folio 2r, page id 00068029:0003 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=00068029&page=3 # Source image: https://digitale-sammlungen.gwlb.de/content/00068029/jpgs/default/00000003.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 73, 2026-08-27T15:28:38Z — 43 lines, status machine # Lines: 43 recognised, mean confidence 0.93 # 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. de via centri coravitatis quoddem Theorema calculi differentiali ponamus spatium ABdC A. frg. 1. generari motu motu rectae AB inter movendum decresen tis seu post se partes sin rlinquente ita ut AB relicen AIH Tonsferatur in 1C1L. er 1C1L, reticta 1 C2H ransferatur in 2C2L et ita porrv. patet primo semper tantundem aequili disten sumto puncto E, medio inter A et B, et ducta recti EF parallela ipsi rectae Bd ago centrum gravitalis rectae AB t vel partum ejus ulrunque motu transpositam seu hucc illua relictarum semper manere in recta EF. Nam semper tantundem aequali distantia infra quam suum est, neque enim mulatio fit quod ad distantian ab EA, sed quoad destan tiam ab AB. J Interim qua Ase semper motu procedit necesse est et centrum gravitulis. recta EF semper procedere, mius tamen quam EF Bd. quia EB ducta in diam centri EM dat aream ABd est. minorem utique rectonsito ABd eergo EM minor quod Bd. Sed quanta sit id sic in vestigabium. Novissima portio rciaquenda sit 3C3C cujus centrum NV. quaeratur caeterorum omnium ut A1H. ICrA. 2C3HH. centrum gravitatis P. Jugatur N. eut punctum medi ips quae secetur in g ita ut sit Q N ad p in ratione pondens ipsorm A1A. CrH. 2ChH, ad pondus 2 C3L. idque erit lom centr gnravitatis omnum, qui et cadet in li recta EF, ergo Net secabit EF in y. Hinc puter 5. 3CyL, sit infinite parva, fore noetra infinite parvam ergo ad habendasm punctum q. in recta EF sufficerehabere p. momentam seu recton EZ esse distantian centri gra vitalis vimrum differentiarum ipius axis partia axis AIH, (C2H, ZC3H at, AH, seu momentum earum id est ipsar 1C2 dutras in 1AIC erc. distahilias ab laxes qu quae utique patet spatium ABd 3 complepe sed CA ut in ida finum linea ceperatuur sit AB feratur motu limlar) et inter inu coceucentri vendum deficiat, tunc tentum Gravitatis ipsius et partum ejus ert linea curva