# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1040780814:0232 # Permalink to this reading: https://leibnizlegible.com/page/1040780814:0232?run=74 # Title: [Astronomiae Physicae & Geometricae Elementa] Astronomiæ Physicæ & Geometricæ Elementa (shelfmark Leibn. Marg. 124) # Folio 214, page id 1040780814:0232 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1040780814&page=232 # Source image: https://digitale-sammlungen.gwlb.de/content/1040780814/jpgs/default/00000232.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 52 lines, status machine # Lines: 52 recognised, mean confidence 0.91 # 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. 214 ASTRONOMLE PHESICE Lib. I metrica posterior st anno interro, et tribus minimum annis In- quisitione in Bultialai Astr. Philol. Fundamenta, (ubi altronomia lux omnis fundamenta jecerat, e Problemata praecipua construxe rat:) tamen ulterius non persit Pasanus, quam ad Plancta locum in sua Orbita data ad tempus allienatum ejusque à Sole distantiam determinandum, hoc est, ipla Attronomia principia Aabilienda; omilla omni Altronomid comparatira, in qua, per Geometriam ex colenda, operam tam pulchre collocarerat Celeb. W’ardus. PROPOSTTIO VI Dosita approximatione modo descripia pro satis accurata, (id est, in FEypothesi Wardi,) ex data nomalia media momaliam coaequatam Planetae à Sole Distantiam invenire in Orbita data. PrODONatUE AZ P Planetae Orbita elliprica circa Solem in S Tan- quam Focum consrituta; hujus Aphelium EE a, Perihelium e, AXis major A P: ex data Anomalia media a FF angulo invenienda eAt Anomalia conquata, nempe angulus ASL, e Planeta in L Di Cantia a Sole, Fc. SL; hoc eAt, hujus recta ratio ad FS vel AP. PTOdUCaLUE FL ad B, ut SIt L. B X. Y qualis LS; _ jungatur B5. Ft quo. niam (per PrOP. LIT. Lib. TII. Conic. Apollonii) FF _ L5 Simul aequantur axi Ae, erit eB cidem ap aqualis. Adeoque in triansulo BFS daris la- teribus BF, FS Cum angulo intercePtO DFS, Anomaliae mediae datae AFT. complemento ad duos rectos aut ad quatuor, (prout L est in primo rel Secundo Anomalia Temicirculo,) in- nOTCICenE anguli ESB _E FBS, SIVC L.SB, quorum dicterentia AST CA A nomalia coxquata quaesita. In trianoulo pOrrO P FS ab initio dan- tur angulus L. FS eE latus FS, ec nunc inrentus cA anguluS FST, adeoque d reliquus FL. S; invenietur ergo latus L. S in partibus data distantia FOcorumSF; hoc est, Planeta à Sole Distantia. 9. F. F. In quarendis angulis ESB, FBS in criangulO BFS, ex datis BF, FS cum ansulo BFS; At (per rulgatum Prisonometria Canonem) DF _ FS Timul ad BF dempio FS, Sieut tangens semissis angulorum B_ FSB ad tangentem Temissis difterentia corundem. Sed PF 8 ES Timul aequantur ipsis AP _ FS Timul; e BP dempto rS aequalis AP dempto PS, siro bis SD; e summa ansulorum B _ FSB aqua liS externO ADZ, nempe Anomalia medix; illorum vero disteren tia aequalis FSF Anomalia CORquata. PF isitur summa ipsarum AP e FS Cst ad 2 es, sire illius semissis s a ad hujus semiltem es; hOC elt, dittantia Planeta aphelios ad ejuldem distantiam perihelion, ut tansens dimidix Anomalia media ad tangentem dimidiae Anoma lix coaquatae: in qua analosia primi duo termini sunt constantes in dato Plancta. Simili