# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1040780814:0366 # Permalink to this reading: https://leibnizlegible.com/page/1040780814:0366?run=74 # Title: [Astronomiae Physicae & Geometricae Elementa] Astronomiæ Physicæ & Geometricæ Elementa (shelfmark Leibn. Marg. 124) # Folio 348, page id 1040780814:0366 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1040780814&page=366 # Source image: https://digitale-sammlungen.gwlb.de/content/1040780814/jpgs/default/00000366.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 42 lines, status machine # Lines: 42 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. ASTRONOMLK PHESICA ib. IV 34E nitum LP. Lx HSularum reloccs Casibus ddaplalarum inive ctione patet tempus, quo Llinxe cenerum est in L. puncto Um brae centro proximo, praecedere Tempus Oppositionis verx cele branda cum Luna ad e perrenerit, in casu praesente; hoc est, cum Luna mox superarit Nodum ascendentem, quod obtinet etiam cum mox superarit Nodum descendentem: Sed cum Luna nondum al- secuta cA Nodos, Tempus medix Fclipsis posterius ese Tempore Oppositionis vera; unde constat quando Tempus inter veram OP. potitionem mediamque Reliptin Tempori Oppotitionis addendum Ht quando subducendum, ut conficiatur Tempus media FClip(IS. Artitices rulso Tabulas condunt Temporis, quo L P arCUIS PerCUI ritur, addendi aut substrahendi à Tempore Syrysia vera, ut tat Tempus Fclipsis media aut Obscurationis maxima. Tempus hoc varium est pro raria Notus Lunx à Sole velocitate et varia di Stantia a Nodo. Tabulas hasce, ut prius illas de quibus Schol. PrOP. ZXXVT, ad Sngulos gradus Terminorum Fclipticorum producunt. PROPOSTTIO XZZVIII. indeque Durationem lam interrae Eclipsis quam totalium J’ene brarum definire. deticiens versus Nodum descendentem versere vonatur, patet L. cliptin incipere cum centrum Luna est in a, Luna limbo Umbra limibum ad c (per Prop. IV. Lib. H. Theod.) continsente. In triansulo isitur aT. 0 rectansulo ad L. dantur praeter rectum hypothenula 01. Cumma nempe Semidiametrorum Ombrae _ Luna, ec or. distantia COMPCtENtCM, UE in PFOP. XXXT; unde per analosiam invenie tur tempus requisitum ut Luna à Sole moreatur per areum Cos Fmpus Initii ex Finis Fclipsis Lunae dato Mense contingen tis, item Immersionis totalis Lunae in Vmbram determinare luceh politis quae in praecedente, nis quod in schemate I. Lund nietur isitur arcus AL, adeoque Lempus requilitum ut L una lc (exceCTu mOTUS IUI LuPTa SSLMIH) percurrat; hoc est, Semidura u ariau nciu colasis Immelsens Luna in Vn bram minima centri DmBra a Centro LUnX PFOP. XEXV. inventa; inre tio incesta LcliplS. Sed exprac. Houn CA Tempusmedia R Clip(IS; innotescent isitur ejus M PTIS. 8t de V