# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1040780814:0263 # Permalink to this reading: https://leibnizlegible.com/page/1040780814:0263?run=74 # Title: [Astronomiae Physicae & Geometricae Elementa] Astronomiæ Physicæ & Geometricæ Elementa (shelfmark Leibn. Marg. 124) # Folio 245, page id 1040780814:0263 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1040780814&page=263 # Source image: https://digitale-sammlungen.gwlb.de/content/1040780814/jpgs/default/00000263.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 55 lines, status machine # Lines: 55 recognised, mean confidence 0.88 # 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. (ib Plare rieuII Spec A, C ria. et Lib. IIl. CE GTEOMETRTCA LLEMENTA. in plano Orbis planctarii recta L. N ad S N perpendicularis; juncta P. N exit (Per Convers. PrOp. XI. F.L. XI.) eidem SN etiam perpendicularis. In triansulo sI. N rectansulo ad e dantur SI. ex NSC; unde dabi- tur latus L. N. In criansulo LF N rectansulo ad F. danu LatuS L. N modo inventum et ansuluS L. NP, qui (per Des. VI. FL. XI.) aequalis eAt Inclinationi Orbis planctarii ad Felipticam, per PrOP. XX. in- rentae; danturisItUr L. F. es P N. In Triansulo POrrO L. FS rectangulo ad F. dantur latera L. F _ L.5; ideoque datur latus SF, Distantia Dlanetae à Sole Curiata. In triansulo F.S N praeter rectum ad N dantur es Cx prius inventum P N; dabitur ergo ansulus ES N, Planeta L onsitudo FTeliocentrica in FCliprica à Nodo e computata: Sed datur Nodi Locus in Licliptica; quare ee Plancta Locus Heliocentricus in Feliptica notus erit. Rursus, in triansulo r5F data cA sr ab initio, e modo inventa cA SF; datur etiam an- sulus TSF, (aequalis Cumma vel differentia datorum angulorum TSN, F.SN, Quia tres rectae ST, SF, S N sunt in plano Rcliptica,) qui ec Ansulus Commutationis dicitur: Lit propterea dantur reliqua, nempe angulus T F. S Parallaxis Orbis mincupatus, e S PP Flonea- tio Planetae à Sole; hoc e, politio rectae TP. sive Planeta LOCuS Geocentricus in Feliptica, ec ejusdem re magnitudo. Denigue, in triansulo TEI. rectangulo ad F. dantur latera PF. eC F L; inNO. celcent isitur rL. Dittantia Planetae a Terra ex angulus L. Y P. P1a neta Latitudo Gieocentrica. S I C T IO IV De lanetarum P. loncatione maxima à Sole, Directione, Statione Retrogradatione. PROPOSITIO XXXVI. At Clanera oncationem à Sole maximam, e dato superiore visam, ejusque lempus determinare. Sit SSol, TP Plancta remotioris Orbita, re PrOPOII. LuCaLuL utcunque propioris Planeta radius rector SV, atque huic normalis VT remotioris Orbita occurrens in T, qua Proinde (per XVT. FI. HIT.) Orbitam circularem ve continset in v. Interior in V a Solemaxi- me elonsatus superiori in r ridebitur: Nam recta ab alio quovis Orbitae er puncto (ut V) ad ducta minorem ansulum cum rS Compre. hendet. In criansulo isitur rus rectansulo ad v datur laterum ST, SV (datorum nempe Planetarum Distantiarum a Sole) ratio; inno- retcunt isitur reliqui anguli FoY, SxV, quorum tiic ett Planela 24.5 Llonsatio