# Leibniz Legible — https://leibnizlegible.com # Page: https://leibnizlegible.com/page/1032774592:0013 # Permalink to this reading: https://leibnizlegible.com/page/1032774592:0013?run=74 # Title: [Tabularum Astronomicarum Pars Prior De Motibus Solis Et Lunae, Nec-Non De Positione Fixarum Ex ipsis Observationibus deductis] Tabularum Astronomicarum Pars Prior De Motibus Solis Et Lunæ, Nec-Non De Positione Fixarum Ex ipsis Observationibus deductis (shelfmarks Leibn. Marg. 164, Stück 1; Leibn. Marg. 164) # Folio - , page id 1032774592:0013 # Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1032774592&page=13 # Source image: https://digitale-sammlungen.gwlb.de/content/1032774592/jpgs/default/00000013.jpg # Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 37 lines, status machine # Lines: 37 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. R A. F A7 lum per cubum quadrantis muralis, scd etiam porcacilis cripedalis. Ouamris altieudo meridiana Sirii non (uperet 25 gradus. cujus alticudinis retractio posita cst 2 18, non ideo ni- nus cerra erie differentia cemporis incer transicum Sirii ee reliquarum fixarum aut planccarum, cum retractio actra cantum in verticalibus circulis, quorum unus est moridia- nus, accollat; nullam autem paciatur inxqualicatem in tervallum temporis medii incer appulsus ad meridianuim; quod in gradus convertum cum debita correctione alcen sionales disterentias ostendie, ex quibus, rariis modis de d rariis temporibus inter le, ac praelereim cum Sirio com paratis, e propter motum proprium actixarum correctis. consticuta aliunde alcentione recta sirii exguisicarum obser- vacionum ope, alcensionem rectam stellarum praecipuarum de planctarum eandem deduxi. Affixarum quae distane polo quinquaginta gradibus circiter, ex aqualibus alcitu- dinibus ad ortum ex ad occalum mediationem caeli colle- si, cum eam caeli regionem quadrans muralis non respi- ceret, carumque alcentiones rectas in cundem catalo sum cum reliquis conjeci. Farum cciam declinationes ex alcicudinibus meridianis habitis opc quadrancis cripedalis, cujus est dirilioexquilita comparatilque cum alticudinibus jam antca a D. Picard obferratis, de lxepe iceraris, debitaque retractionis quan- titace imminuris; asecutus Tum. Adjeci praeterca longicudines e laticudines Aellarum prima magnicudinis aliarumque nonnullarum ex Trigo nometrix deductas calculo, qui alcentionibus rectis de de- clinationibus obferratis innititur. Optima ex vera cabularum condendarum ratio ad pla- necarum motus decerminandos ex nudis obserrationibus deducenda videbatur. FIOc Crat commune Astronomo- rum vocum, Ced res ipla _ difficilis _ ardua in CKCCuTIOC iplis vila est, ad fctitiosigitur motus Greometricos contu- gerunt, in quibus nescio quid subtilicatis e acuminis in-