# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1040780814:0254 # Permalink to this reading: https://leibnizlegible.com/page/1040780814:0254?run=74 # Title: [Astronomiae Physicae & Geometricae Elementa] Astronomiæ Physicæ & Geometricæ Elementa (shelfmark Leibn. Marg. 124) # Folio 236, page id 1040780814:0254 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1040780814&page=254 # Source image: https://digitale-sammlungen.gwlb.de/content/1040780814/jpgs/default/00000254.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 51 lines, status machine # Lines: 51 recognised, mean confidence 0.93 # 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. 2 ASTRONOML A PHYSFCA. alsumpta isitur majore Are Orbita Terra (hre hujus semisse Tellu- ris Distantia media a Sole) habebitur magnitudo Orbita Planeta: penitus isitur determinatur Plancta Orbita. Et Tempus, quando Planeta hic Aphelium tenebat, similiter determinatur, atque idem in Planeta Tellare PrOD. XIV. Factum. Ouoniam Orbitx Planetae Fllipricae Species Tola ex datis determi NatUE, (UIE CX PFOD. XIV. ConStaL,) _ ejus Orbitx maonitudo respectu Orbitx Terra ex comparatione Temporum periodicorum horum Planetarum per praec. concluditur; idem poterit aliunde inserpi. Fa- ciendo nempe ut Orbita certa Speciei (ex tribus Locis Centricis de terminatae) ex Sole ut Umbilico deseripta, transeat per ipsum L0. cum Planeta in linca Nodorum per Prop. XIX. hujus inventum: Fioc namque punctum, in Planeta Orbita datum, tantundem valet ad illius maonitudinem respectu maonitudinis Orbita Terrettris determinandam, acque ejusdem Axis major supra definitus: TRius enim puncti Distantia a Sole in partibus linearum Orbita Telluris determinata cst; potestque alter horum modorum describendi Or- Ditam per alterum examinari et corrigi. Et hinc motus Apsidum cujutris Primarii definietur; nimirum eodem modo quo prius Nodorum motus. PROPOSEEIOZEVI LEMMA. tis umbilico lonsitudine axis majoris, describere Fllipsin per data duo puncta transeuntem. Sit S Figurx describenda umbilicus, ae longitudo axis majoris, L _ duo puncta per quae Flliplis trantire debet. Centro F distantia aequali exceltui rectae ap supra rectam L. S describatur circuluS CF; e timiliter centro distantia aequali excellui rectae ar fupra 18 describatur circulus RF priorem secans in F; exit F FMipseos describenda umbilicus alter: TTisce isitur umbilicis S_ F, C aXC majore aquali recta ap, descripta Fllips erit ea qua quaeritur. Ouoniam enim L. F aqualis CAt AP - LS, CrIt LS F L F aqualis AP. Pari modo AP Xquatur IS F VF: Onde (DeT PFOD. LIT. Lib. tert. Conicorum) Fllipsis umbilicis s d F de- scripca, axem majorem habens aequalem recta aP, transibit per puncta L. 8 l. Facile es ex hujusmodi constructione Cicometrica calculi mo- dum Altronomia accommodatum excositare. Fx datis enim tri bus punctis s, L. _I, hoc eA, ex datis tribus lateribus trianguli ST. I. innoteseunt anguli. RursuS, in triangulo L. IF dantur omnia latera; nempe L. V uEpriuS, L. F ditterentia datarum rectarum AP _ L. S, e IF disterentia iplarum aP, 15; innotescit isitur angulus FL. I: Sed prius notus erat SLV, ergo dabitur angulus SI. F. In triangulo ie1 tur ST. F, Cdatis LS, L F Cum angulO SL. F innOteICet latuS S F dictan- tia focorum, et ansulus L.SF inter L. S positione datam e axem majorem; 1D. lLL d