# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1040780814:0377 # Permalink to this reading: https://leibnizlegible.com/page/1040780814:0377?run=74 # Title: [Astronomiae Physicae & Geometricae Elementa] Astronomiæ Physicæ & Geometricæ Elementa (shelfmark Leibn. Marg. 124) # Folio 359, page id 1040780814:0377 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1040780814&page=377 # Source image: https://digitale-sammlungen.gwlb.de/content/1040780814/jpgs/default/00000377.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 50 lines, status machine # Lines: 50 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. L. 1D. CF. umbrd usco censcus quodam tenpors punel c ut suunt celebranda cum illud ad Pettt. Supaus Coiclratorem intra hunc circulum constitutum, uc au O. lire polius in Hemi- Ephaerica superficiei illuminata puncio, suol ecta ex o ad planum Disci normalis octendit; inrenienda cst quanta Diametri Solaris parS d Luna LeSatUE pFX. dicto Observatori. Fun- satur recta A0, produ. catur doncc circulo MOX occurrat in M; dico Solis Diametri partem à Luna tectam ese ad Diametrum intesram ut OM ad AM. lam si Obserrator esset in M, Luna nullam prorsus Diametri So- laris partem ab illo teseret: Obserratori rero paulatim versus Pen- umbra centrum a prosredienti. Solaris Diametri pars maior major- que per interpositam Lunam ab illo tesitur, donce tandem illo ad centrum a perrento, Sol totus (hoc cH, ejus Diameter integra) ab c0 tesatur, si modo Solis apparens Diameter Luna Diametrum appa- rentem non excedat, (quod hic suppono, quodque in harum magni- cudinibus medioeribus tere obtinet,) e Luna totalis Vmbra vertex ad Terram usque pertingat, siro circulus penum brOsIS MO X Cen- trum habeat perfecte ex totaliter umbrosum: Ft ideo A Solis Di ameter ut AS in Uncias diridatur, ex data ratione inter A M _E OM, qua ex Loci intra circulum ma x situ dato innotescit, dabuntur Dia- metri Solis Oncix sire Disiti obscurati horumque partes respectu Obervatoris. Ouod h circulo m xa concentricus sit (ut in Ag. Separata) circellus BC rel totaliter umbrosus, vel non mere umbrolis, sed reliquo ob. scurior e quidem aequaliter; hoc es, si Ombrae Lunaris centrum vel ultra Spectatorem procendatur, vel cirra illum delinat, l0c0 rectae as sumenda es in priori calu recta BM Semidiametro. rum AM _ AB differentia; in posteriori en illarum summa: est nempe Solis Diameter interra 2d ejus partem Spectatori ad o a Luna tectam in casu priori uE BM ad OM, in posteriori verO ut CM ad OM. Nam in priori casu Spectator ad B Solem integrum ridebit a Luna tectum, in posteriori Spectator in a politus circa obscuram Lunam circulum e Solari Disco reliduum lucidum videbit, corona instai, cujus visa Latitudo aequatur Semidiametro Solari minuIae SC. midiametro Lunari, eidem nempe cum Semidiametro AD e Luna rila; oportetque ut Spectator in e consticuatur, ut Luna mareinem Solis Discum interius continsentem cernat. Determinata isitur cA in omni casu Feliplis Solaris Ouancitas. G. L. F. PRC _E GTEOMLXRKCA F L EMENTA. centrum pervenerit, sic Novilunium verum. Ponatur a ese Pen per rectam les instituit, ipsumque circulum venumbrosum esse MOX; erit a N itineris Penumbrae pars ea qua facienda cA in- ter hocce temporis punctum ee momentum Conjunctionis verx