# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1040780814:0227 # Permalink to this reading: https://leibnizlegible.com/page/1040780814:0227?run=74 # Title: [Astronomiae Physicae & Geometricae Elementa] Astronomiæ Physicæ & Geometricæ Elementa (shelfmark Leibn. Marg. 124) # Folio 209, page id 1040780814:0227 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1040780814&page=227 # Source image: https://digitale-sammlungen.gwlb.de/content/1040780814/jpgs/default/00000227.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 65 lines, status machine # Lines: 65 recognised, mean confidence 0.85 # 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. AB (0le8 C pU odan UNTC. 259 Vedia rUM AHUI mal et u pC tCs 10I Lib. III. _E CFEOMETRLCLE L LEMEN TA. 209 ratio quadrati semidiametri ad integrum circulum; _ ex OrbiEX specie data, dabitur ratio media distantia B5 seu ca, e etiam semi- axisminoris Be ad excentricitatem SC; e inde ratio triansuli BCS ad radii quadratum; e ex ratione ar- cus altumpti a c ad circumterentia quadrantem aD, dabitur ratio sinu- um eorundem, (c. DC ad OF, Q CON sequentor etiam iptius BC ad aF; HOc CA, Per L. Fl. VI. ratio trianguli BCS ad cc5. In partibus erso quarum circulus continet 360, dantur sc. ctor acc de triangulum ccs, (cui analosum LCS Aiguationis Pars Physica dicitur, ficut AnguIUS SL C Pars Optica;) adeoque horum aggresatum aas trilineum, quod Prop. praeced. ostensum eAt proportionale eAe trilineo ALS, _F prO. inde Anomaliam mediam jure repralentare. Nam s OrDita FI. liptica ABP area tota in 360 partes aequales dirila concipiatur; illius ParS aL. S, nempe Anomalia media Planetae in L, tot ejusmodi partes continebit, quot acs continet partes similes area circularis aBP; adeoque eodem exprimetur nuerO. RursUS, in triangulo cCs, data ratione laterum e0, Cs (Distantia media Planeta à Solc ad Fxcentricitatem) et ansulo comprehenso acs, (allumpei nempe aCCi Complemento ad duos rectos,) dabitur (per XII. Datorum) anou luS aSc; adeoque d aSF Anomalia coxquata, nempe angulus cu- jus tansens PP. eA ad P. C tansentem ansuli asc prius inventi in ratione data Orbita Pemiaxis minoris cB ad semiaxem tajorem cD. Ft cum Anomalia media et vera; per calculum inventa, ci- dem astumpio arcui aa congruant, erunt e inter se congrux; five altera alteri correspondebit. Ft pari modo licet alium quemris arcum altimmere, ex congruas Anomalias (mediam sc. _ veram) inde calculo determinare, quae proinde erune inter se correspondentes. PROPOSEETO, II Ita Anomalia mediâ Planetae, cujus Orbita datur, Momaliam veram e Planetae Distantiam à Sole per calculum invenire, vicissim. Nullam dari calculi methodum directam Prablema hoc solvendi pronunciat Keplerus ad finem Part. IV. Physicae Caelestis. Ouomodo vero methodo indirecta _, ad usus Astronomicos satis accommodatd hujusce Problematis calculus absolri poterit, nunc ostendendum est. In circulo ADP, Orbitam in Aphetio de Perihelis tansente, Tuman. tur Anomalia PXCenEri arCUS aC, Vel ansuli ACC, per CingulOS Sra. dus se excedentes. Ad horum unumquemque (per pracedentem) inreniantur correspondentes Anomatia; media IC. _ Vera. POH conctitum er so, pro Planstx dibita data, Canonem Anomalix me. dia