# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1040780814:0302 # Permalink to this reading: https://leibnizlegible.com/page/1040780814:0302?run=74 # Title: [Astronomiae Physicae & Geometricae Elementa] Astronomiæ Physicæ & Geometricæ Elementa (shelfmark Leibn. Marg. 124) # Folio 284, page id 1040780814:0302 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1040780814&page=302 # Source image: https://digitale-sammlungen.gwlb.de/content/1040780814/jpgs/default/00000302.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 56 lines, status machine # Lines: 56 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. 284. ASTRONOMLA PAESTCA quadraturam in D perVeNtO, MIN Cranescit (quoniaM SR, SL, a proinde etiam e S A, tunc aequales funt) et proinde Vis per illam ubique exposita nulli hic sunt effectus: Satelles isitur E reliquis Viribus agitatus areas per radium rectorem temporibus provortio- nales nunc describit. DAMLVerO F quadranteM DB peFAOFAL, SM deticit ab sNr, X Vis perturbans deseriptionem areae per radium rectorem TE, quo minus sit tempori provortionalis, quae est uE MN, dircctionem ab m versus Nsiro ab L vertus r (hoc est, in consequen tia) habet, ac proinde motum Satellitis in illo quadrante accelerat: Post oppositionem vero in B, L. F tendit in antecedentiam, motum. que retardat, doncc in quadratura ad c Craneseat rUESUS M N, eju que proinde effectus ceslent. Pursus, cum Vis mn perturbans de scrixtionem area quam radius FE verrit, ne SC. HXC (IE teMPOTI proportionalis, in transitu Satellitis à c ad a, vel d D ad B, perpetuo augeatur e in c ac B Sic maxima, e hinc rursuS perpetuo diminu- atur donee Satelles perveniat in D vel c ubi cranelcit; patet Sd tellitis sic perturbati motum esse relocistimum (caereris paribus) in Syysiis B d c, tardissimum in Ouadraturis c e D. 1. F. D. PROPOSITTOTI. dem positis, Satellitis L. Orbita circa Primaruin ldese a (caeteris paribus) macis curva est in e D Quadraturis cum 50lb, quam in SyZysiis C B. Cum enim Satelles L. relocius moreatur in SYLy SIIS qua Ouadraturis, minus deslectet a recto tramite, quem ri insitâ (ola de scriberet, in illis quam in hisce; hoc es, Satellitis Orbita minus curra est in Conjunctione e Oppotitione quam in Ouadraturis. Sed et majorhac Curredo ex alia etiam causa provenit: Vis ut MN (de qua PrOP. PTXC.) in Conjunctione e Oppositione ad c _ B Contra ria eA Vi, qua Corpus Y trahit E, adeoque illam minuit: MinUS CrSO UESCTUE L VertuS Y ad a e B quam ad c e D; minusque Propterea a recto tramite deslectet in illis quam in hilco. Satellitis isitur Via currior cAt in Ouadraturis c es D quam in Syzysiis B eC. GiOROLLARFOM. teris parIbuS) lonsius recedere a Primario r in Ouadraturis quam in Syzygiis. HIOc pacto Satellitis Orbita circa Primarium F. I. Z liptica quati ft, cujus centrum Primarius occupat; major Aris Ouadrata Solis inter- Jacet, minor Syzysias: sic enim Orbita currior est illic quam hic. Atque augmen- tum celeritatis Satellitis prope Syzreias di- verlum erit in Orbita hac, ab illo quod fuis. Tet in Orbita circulari Prop. praec. quia Visut MN Satellitis motum accelorantis aut retar- dantis directio alia cM in hranc, alia in illam. LtD. L1. la pradicts seguuur SatelluemE, (Ca. conc euir loco de tur S e