# Leibniz Legible — https://leibnizlegible.com
# Page: https://leibnizlegible.com/page/1032774592:0126
# Permalink to this reading: https://leibnizlegible.com/page/1032774592:0126?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 106, page id 1032774592:0126
# Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=1032774592&page=126
# Source image: https://digitale-sammlungen.gwlb.de/content/1032774592/jpgs/default/00000126.jpg
# Model: FoNDUE-GD_v2_ft_Leibniz, run 74, 2026-09-06T16:05:13Z — 38 lines, status machine
# Lines: 38 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.

106
modoreperca, productumque diridaeur per mocunt ora
riu viCUM F393 arc. 28. habebuncur 1486 vel 24 46
Suberahenda a rempore veri novilunii pro vero initio cclip-
sis, quod continget 2 22 28 veri vel apparentis temporis.
Ouamvis inicium ccliplis in prima opcracione inventum. à
novilunio z0 non disticerie, nihilominus ad majorem accu-
racionem hanc secundam operationem insticuimus, cujus
beneficio horarius morus lunx a Sole rilus a primo divertus,
eoque accuratior inventus est, ac denique tempus veri ini-
tii ccliplis, paulo dirertum à primo dabitur.
Z==II. Proprer correctiones ultimo loco inrentas, ma-
nifectum est cempus maximae obscuraeionis in priori caleu-
lo inventum medix ccliplinon conrenire; led media cclip-
sis erit momentum medium incer inicium et finem, quod
in hilce ccliplibus nullius csEMOMenEi. AE VetO cenpus ma-
Xinix obscurationis, quod in observando nunquam explo-
racissimum habebitur, quale primo inrentum est opc per-
Dendicularis L T rerinebimus: uc inde quanca siE maxima
obscurario definiatur. Scd oportet ut punctum Y quod cst
occursus perpendicularis LY ductae ad balim crianguli siE
in ipsa basi non producta, ut in hoc exemplo in triangulo
GLR inventum est: secus enim si perpendicularis L. T du-
cta ad balim prioris erianguli CI R cadac exera triangulum,
decerminacio cemporis maxima obscuracionis in alECrO
trianoulo crie inveltioanda.
Ecto punctum q in superticie cerra policio loci propoliti
cempore maximae obscurationis, et punctum r locus centri
umbrae lunae in orbita Cur eodem cempore. Poitur cum cem-
pus maxima obscurationis locopro-
polico invento in puncto q vertante.
invencum Fuerit 3 34 53 RFF. Z2 peF
primam regulam reperietur angulus
Parallacticus P C 943 46 45, et
Parallaxis loci in gnempe C944 13
vel 2641
LLIIL. Sed In llalsoe ein
DSVS TABDE ARVMI.