# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1041163592:0214 # Permalink to this reading: https://leibnizlegible.com/page/1041163592:0214?run=74 # Title: [Philosophiae Naturalis Principia Mathematica] Philosophiæ Naturalis Principia Mathematica (shelfmark Leibn. Marg. 166) # Folio 180, page id 1041163592:0214 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1041163592&page=214 # Source image: https://digitale-sammlungen.gwlb.de/content/1041163592/jpgs/default/00000214.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. +80 PHITLOSOPMILE NATDRALIS Corol. 5. Fadem ralene ubi attractio oritur a Sphaerae utriusque vircute actractira, mutuo exercita in Sphaeram alteram. Nam viri- bus ambabus seminatur atrractio, provortione servata. Corol. 6. Si hujusmodi Sphaera aligua circa alias quiescentes re- volvancur, singulae circa singulas, sintque dictantixe inter centra re- volrencium ec quielcentium proportionales quielcentium diame- eris; aequalia crunt Tempora periodica. Corol. 7. FF vicissim, Si Tempora periodica sunt aequalia; dictan- tiae crunt proportionales diametris. Corol. 8. Eadem omnia, quae superius de motu corporum circa umbilicos Conicarum Sectionum demonstraca lune, obtinene ubi Sphaera actrahens, Formae ec conditionis cujulris jam descriptae, l0. catur in umbilico. Corol. 9. VE _ ubi srrantia lune etiam SphXrA aFETAhENECS, COn- dicionis cujulris jam descripex. PROPOSITTO LHRVII TTTEOREMA XXXVII. Si ad sincula Sphaerarum puncta tendant vires centripetae, propor- tionales distantiis punctorum a corporibus attractis: dico quod vis composita, qua Sphaerae duae se mutuo trahent, est ut di- stantia inter centra Sphaerarum. Cas. 1. Sit AF. BF SphEra, S centrum ejus, F corpusculum aE- cractum, P ASB axis Sphaera Per centrum corpusculi Eran(ICMS, L P, ef plana duo quibus Sphaera se catur, huic axi perpendicularia ex hinc inde aequalicer distantia 2 centro Sphaerae; C e interlectio nes planorum ec axis, ec II pun- ctum quodris in plano F F. Pun- Eti TIvis centripeta in corpusculum P, secundum lineam F IV exer. cita, est uc distantia PFI; Xc (per Legum C Orol. 2.) Secundum li- neam F C, Peu vertus centrum S, ut lonsitudo PCF. Igieur pun- ctorum omnium in plano P F, hoc est plani torius vis, qua corpuI- culum P trahitur versus centrum S, est ut numerus punctorum ductus in distanciam PG: id est, ut contencum sub plano ip(0 P F ec distancia illa PC. Ec similiter ris plani ef, qua corpulculum P DF MOZV 1. 9 et etaltlec