# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1040780814:0249 # Permalink to this reading: https://leibnizlegible.com/page/1040780814:0249?run=74 # Title: [Astronomiae Physicae & Geometricae Elementa] Astronomiæ Physicæ & Geometricæ Elementa (shelfmark Leibn. Marg. 124) # Folio 231, page id 1040780814:0249 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1040780814&page=249 # Source image: https://digitale-sammlungen.gwlb.de/content/1040780814/jpgs/default/00000249.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 79 lines, status machine # Lines: 79 recognised, mean confidence 0.80 # 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. OniS Tetur 110 L 1Nal 1atio st Dit De AUII indet 1 t JeM. Situ montsa stan P ret Iu intet motilus apD iptae Di vatiol IaMG i suibe B tit poliviti inab a) t1 Ol L ib. TII. A DTHOMETRICA LLEMENTA. ad utus Asronomicos, unde istronomicum dicitur; hoc ergo adhi- bendum esset: Atqui ad medium ex dato apparente determinandum Locus Solis et necesarius; ergo ille praeterpropter crat prius inve niendus, Tempus apparens, quasi medium fuisset, adhibendo, ut Temporis Aquatio inveniatur. FIdc vero semel inventa, e appa- rente Tempore ad Astronomicum reducto, ad Tempus iltud (idem quod propolitum est momentum, sed numero ad ingrectum in Ta- Dulas apto expresum) guaratur (per eandem Prop. XVT.) Solis LOcuS, de Distantia Telluris à Solo, qua patet esse vera d correcta. Non absimiliter Problematis hujus conrersum construetur, Tem- Pusque inrenietur, quo Sol d Tellure risus datum Locum tenebit. S F C TIO De recauor Planetarum Primariorum Orbitis determi- nandis, e horum cum e Sole, tum eellure spectatorum Pheoria condenai. PROCOSILIO LIL. DOsitionem Lineae Loaorum Prois Lhanclara ipsius Planetae minare. in Nodo versantis a Sele Distantium per observationes deter. commodacto Lelctats Solem; I Orbitam lelluris, cujus lOcusS; n Lineam Nodorum Plaliela Propolci. Sitque primum Perra in T, et ex hac obterretur Planeta in Lcliptica, ideoque in Nodo (uo, puta P: nunquam enim Planeta in Felipriea ridebitur d Fellure in Feliptica plano ver- Tante, niti cum infi- Cliptica plano ctiam Fuerit. Pot inte sram rerolutionem obserretur Planeta in eodem Nodo, cum Terra ad+ pervene. rit. Ducta intelli- santur rectae ST, PF, item St, PT se mutuo intersecantes in x puncto. inter oblelrattones intersecto, esTP oblerrata lilongatio llancta a Sole, e latus sr Distantia Telluris a Sole in obserratione prima: inVemItus ergo SX; ec ideo xt, Cu cala 3t Vam eulo d Sole in obserratione secunda: Rursus, in triansulo +XP datur an- sulus Xe angulo FXS in prori aqualis, a ansul s L In Figuris binis ad binos casus superioris de inferioris Planeta ac In triangulo srx dantur ansuli rSF ex Theoria Perra d Tempore Satio Planeta à Sole secundo obserrata, e latus +x modo inven- cum; e proinde itremetus Lallo et. DeluC, In triangulo StP datis laceribus FS, FP, cum angulo compreheno PtS, inrenietur SP tlatlla