# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1040780814:0368 # Permalink to this reading: https://leibnizlegible.com/page/1040780814:0368?run=74 # Title: [Astronomiae Physicae & Geometricae Elementa] Astronomiæ Physicæ & Geometricæ Elementa (shelfmark Leibn. Marg. 124) # Folio 350, page id 1040780814:0368 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1040780814&page=368 # Source image: https://digitale-sammlungen.gwlb.de/content/1040780814/jpgs/default/00000368.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 53 lines, status machine # Lines: 53 recognised, mean confidence 0.92 # 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. ib. 350 ASTRONOMLE PAYSICA Dos Elenilunium verum risa invenietur. FX invento Des metho- dum supra indicatam motu Luna à Sole horario, determMsabu arcus quo Luna distat a puncto e, ubi Plenilunium rerum celebratus: Sit hic es; ideoque centri Luna Locus ad Tempus datum est 5. Junsatur arcus 05 Luna Disco in m e H, circuloque CDC IN R Occurrens. In triangulo 80P dantur Prater rectum ad 0 latus 80 anguluI. que o~P; unde invenientur latus or (jam supra definitum) et angulus 0r2. In tri angulo rursus oesdantur duo latera PO, PE e angulus interjectus oes; unde dabitur etiam O5 arcus, ex proinde hujus notigu arcus sur differentia oM: Sed datur OR, 8 proinde iplarum oR, om differentia MR data est; omnes nempe in partibus circuli, ut lupra: adeoque, ut in casu priori, Ouantitas Rcliplis in Oneiis DI ametri e Uncia partibus exprecta. Si MR excedat Diametrum Lunx integram (quem casum (che Ma anMCTUM FCFCFE) FclipEs dicitur tot Dieitorum quot Diametrs Luna Uncias mx continet; abusire quidem e impropric, cum proprie loquendo Luna deticere nequeat pluribus Digitis quam ipsa habet in sia Diametro; me autem conslatur ex Luna Semidiametre MS e se distantia minima Centri s ab Ombra marsine cDC, qua (Per lem. Sphaeric.) circuli maximi centra o ec s conjungentis arcus CA. COROLLARTUMI. Hinc Facile determinabuntur Telluris Loca, ex quibus Rclipis Lanaris data Phalis spectari potest. Cum enim ad istam Phasin det cientis Lunx locus ex Prop. hac detur, de hora in dato Loco Telluris; dabitur (per COrOII. XXXVI. Lib. II.) Locus Terra, cui Luna tum et in vertice. Omniaque Loca, qua hinc absunt minus quadrante circuli, hanc ridebunt; qua magis, non videbunt; gua ipso qua- drante, in Florixonte ridebunt. CIOROLLARTUM 2. Ex tribus ultimis Propositionibus Schema Relipsis Lunaris in plano graphice prorrahetur. Cum enim tantilla Caeti Lunaris DarS, quam Ombra (vel etiam Penumbra) Terra una cum Luna ad fi- elipsis Initium illam tangente occupat, pro plano tuto postit ha- beri: Ductis rectis, se decustantibus in ansulo aequali illi quem Via Lunx cum FCliptica comprehendit, Circulos iltos, carumque con curtu Nodum proximum referentibus; sumatur in recta Fclipti cam reterente punctum a communi rectarum concurtu distans tot partibus aequatibus quibusris quot partibus circuli (V. 8. Scrupulis) Centrum Ombrae sive punctum Soli oppositum distat d Nodo; cen ero hoc describatur Circulus Terrx Umbram referens, hujus Semi diametrum toc prius assumptarum aequalium partium faciendo quot scruxulorum in Coelo Ombra Semidiameter revera occupat; ex hoc cenro ducendo rectas lam ad Felipticam quam ad Viam L. W narem De