# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1041163592:0397 # Permalink to this reading: https://leibnizlegible.com/page/1041163592:0397?run=74 # Title: [Philosophiae Naturalis Principia Mathematica] Philosophiæ Naturalis Principia Mathematica (shelfmark Leibn. Marg. 166) # Folio 363, page id 1041163592:0397 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1041163592&page=397 # Source image: https://digitale-sammlungen.gwlb.de/content/1041163592/jpgs/default/00000397.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 41 lines, status machine # Lines: 41 recognised, mean confidence 0.90 # 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. PRINCIPTA MATHIEMATICA. PROPOSITIOMI THEOREMA HI. Vim qua Luna retinetur in Orbe suo respicere Terram, e esse re- ciproce ut quadratum distantiee locorum ab ipsius centro. Patet altertionis pars Prior per PhenOmenON sextuM, et PrOPO- policionem secundam vel tertiam Libri primi: de pars posterior per mocum cardissimum Lunaris Apogei. Nam motus ille, qui lingulis revolutionibus eA graduum eantum trium ex minutorum erium in consequentia, contemni potest. Patet enim (per Corol. I. PFOP. XLV. Lib. I.) quod s dictantia LUINX a CeNErO PCFEX SIC ad Lemidiametrum PCrEX UE D ad F; vis a qua motus talis oriatur lIE rCCIPROCC VE D2, 4, id cA, reciproco ut ca ipsius D dignitas cu- jus index est 224, hoc est, in ratione distancix paulo majore quam duplicata inverse, scd quae partibus 593 propius ad duplicatam quam ad criplicatam accedit. Oritur vero ab actione Solis (uri Dotthac dicetur) et proprerea hic neglisendus eAt. Actio Solis quatenus Lunam distrahie a Ferra, est ut distantia Lunxe a Terra quamproxime; ideoque (per ca quae dicuntur in C Orol. 2. Prop. ZLV. Lib. I.) es ad Lunae vim centripetam ut 2 2d 357,45 circi- Ter, Peu L ad 17845. Et neslecta Solis vi cantilla, vis reliqua qua Luna retinetur in Orbe erit reciproce ut D2. Id quod eriam plenius constabir conterendo hanc vim cum vi Gravitatis, vE AC in PropOCriOnE sEGUentE. Corol. Si vis centripeta medioeris qua Luna retinetur in Orbe, augeatur primo in racione 17745 ad 27825, deinde criam in rati- one duplicata semidiameeri Perrae ad medioerem dictantiam centri Lunae a centro Terrae: habebitur vis centripeta Lunaris ad super- siciem Terrae, polito quod vis illa descendendo ad superticiem TErrA Perpetuo auseatur in reciproca alcicudinis ratione du- plicata. PROPOSITIOIV. THEOREMA WV. Lunam gravitare in Terram, e vi gravitatis retrahi semper a motu rectilineo, es in Orbe suo retineri. Liunae distantia medioeris a Ferra in Syzygiis est Pemidiameero- rum cerrestrium, secundum plerosque AAtronomorum 59, secun- dum Pendelinum 60. secundum Copernicum 603, et sccundum Ty- A ad ehonem L IBEK TRXTIVS. GIIHIIMIIIBHIHMBBIIBI