# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1040780814:0428 # Permalink to this reading: https://leibnizlegible.com/page/1040780814:0428?run=74 # Title: [Astronomiae Physicae & Geometricae Elementa] Astronomiæ Physicæ & Geometricæ Elementa (shelfmark Leibn. Marg. 124) # Folio 410, page id 1040780814:0428 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1040780814&page=428 # Source image: https://digitale-sammlungen.gwlb.de/content/1040780814/jpgs/default/00000428.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 48 lines, status machine # Lines: 48 recognised, mean confidence 0.94 # 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. ASPRONOMLA PAFSICA PROPOSTTTO V Tures Cometae videntur in Temisshaerio versus Solet Glut Delignet SSolem; Y Terram; circulus DE PE centro Taclet spS Fixarum sphaeram, sire illam potius qud visus terminatur. Ouone am Cometa (plendent luce Solis a lere. Rexd, non videbuntur antequam à Sole ita illustrantur, ut Oculos nostros luce ista movere porsnt: e praterca cum Cometa per Caudas suas sint maxime conspicui, has aucem non emittant pri usquam ad Solem incaluerine aliguantu. lum; patet ad utrumris consequendum, opus elle ut Cometa ad detinitam à Solc distantiam accedat. Sit ABCC (phara Soli concentrica ad iltam distantiam deseripta; talis nempe ut nut lus Cometa, proprer illustrationis defectum, rideatur, priusquam intra sphaera hujus superticiem rersetur: Juncta recta Sr produ catur utrinque, donec dicta superticiei occurrat in A e C: Pet Z ducatur planum AP cui ac elt normalis; hoc diridet sphaeram DEFM in duo Hemisphaeria, quorum HFP CA Solem versuS, EDF Soli oppotitum. Cometa omnes in sphaera sesmento BCC eX istentes videbuntur in Fremisphaerio versus Solem; omnes autem qui versantur in segmento Bac ridebuntur in Femisphaerio Sol Oppotito. Patet vero quod segmentum BC C majus eA quam B AC, quia sphaera centrum est in illo: Plures isitur Cometa videbuntur in Fremisphario versus Solem quam in opposito. O. F. D. Sed ec plures primo videbuntur sire detesentur in illo quam in hoc, cum superticiei sphaera pars BCa major sit reliqud BaC: de tesi autem supponuntur quamprimum superticiem hanc attingunt. SCHOL TV M. Ouo minor ponitur sphaera aBCc, hoc ett, quo propius à Sole abese oportet Cometam antequam videatur, eo Cometarum in Fremisphario Solem versus ritorum numerus masis excedit nir merum apparentium in opposito; quoniam tanto masis segmen tum BCc excedit B a C sesmenEuM. EF ob eandem rationem prI mo detectorum numerus in illo quam in hoc maior elt. Si ponatur aBCc ce paulominorem quam sphaera Jovis, sive quod Cometa se prius ridendos non prabeant quam sint Soli paulo pro. piores quam Jupiter, hoc cA, si ponatur sa ipsius s+ guintupla; (nam Toris distantia à Sole excedit quintuplum distantia Felluris, ab eodem;) Segmentum Bec erit propemodum duplum sesmenti BAC, X ideo fere duplo plures Cometa in Fremisphaerio Solem vertus videbuntur quam in Flemisphaerio opposito: At superticies BCC eA tantum se squialtera Superficiei B a C, ideoque dimidio plures illic quam hic primo detesentur. Si aBec sphiaera minor fuerili V. E Flemisphaerio opposito.