# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1041163592:0429 # Permalink to this reading: https://leibnizlegible.com/page/1041163592:0429?run=74 # Title: [Philosophiae Naturalis Principia Mathematica] Philosophiæ Naturalis Principia Mathematica (shelfmark Leibn. Marg. 166) # Folio 395, page id 1041163592:0429 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1041163592&page=429 # Source image: https://digitale-sammlungen.gwlb.de/content/1041163592/jpgs/default/00000429.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 42 lines, status machine # Lines: 42 recognised, mean confidence 0.89 # 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. 1II PRTNCIDTA MATHEMATIOA. Solem. Fa componitur ex partibus SM, L. HI, quarum L. M d LIvE ipsus SM ParS L M percurbac motum Lunae, uc in Libri primi FcarI PrOP. FXVI. e ejus Corollariis expotirum cst. OUaFENUS Perr2 ec Luna circum commune graritatis centrum revolvuntur, Pertur- babitur etiam motus Terrae circa cenerum illud a riribus consimi libus; sed summas tam virium quam moruum reterre licet ad Lu- nam, ex Cummas virium per lineas ipsis anal0925 FM ec ML delignare. Vis ML (in medioeri lua quantitate) eA ad vim centripetum, qua Luna in Orbe suo circa Lerram quiescentem ad dittantiam PT revolvi posset, in duplicata ratione temporum periodicorum Luux circa Terram a Terrae circa Solem, (per Corol. 17. PFOD. LXVr. Lib. l.) hoc eA, in duplicata ratione die rum 27. Bor. 7. min. 4.3. 2d dics 365. Bor. 6. min. 9. id est, uE 1000 24 178725, Teu F 2d 17826. Invenimus autem in Propositione quarca quod, A Terra ee Luna circa commune gravitatis centrum revolvancur, carum distantia mediocris ab invicem cric 60= Temi- diametrorum mediocrium Terrae quamproxime. Ec vis qua Luna in Orbe circa Terram quiescentem, ad distantiam P Y Cemidiame- erorum cerrestrium 602 revolri porset, est ad vim, qua codem cempore ad distantiam lemidiameerorum 60 revolvi poset, uE 602 2d 60; _ haec vis ad vim graritatis apud nos ut L ad 60760 quamproxime. Ideoque ris mediocris ML eA ad vim graritaris in superticie Terrae, UE XZ 607 ad 60X60X60X 178+07 seu 1 2d638092,6. Vnde ex proportione linearum Y M, M L. datur etiam vis YMI: et hxe Pune vires Solis quibus Lunx mOtus percurbantur. d. F. I. PROPOSITIO ZXVI. PROBLEMA VII Invenire incrementum horarium areae quam Luna, radio ad Ter ram ducto, in Orbe circulari describit. Diximus aream, quam Luna radio ad Ferram ducto describie, esse cempori proporcionalem, nisi quatenus motus Lunaris ab actione Solis curbatur. Inaequalicatem momenti (vel incremenei horarii) hic inveltisandam proxonimus. Ot compuratio Facilior reddatur, Ensamus orbem Lunae circularem esse, e inaequalitates omnes neslisamus, ca sola excepta, de qua hic asitur. Ob in- gentem vero Solis distantiam, ponamus criam lineas SP, S7 Sbi inricem parallelas esse. Hoc pacto vis L. M reduCCtuE TEPCF FCC. 1 HIIIEIIBMIIIMIIIIEBASIEMEMHIEGAABBIIIIHAIIIIAGHBMSIIIHIIIMINI