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# Title: Leibniz-Handschriften zur Mathematik LH 35, 13, 3 (shelfmark LH 13, 3)
# Folio 52v, page id 00068200:0106
# Original at the GWLB: https://digitale-sammlungen.gwlb.de/resolve?id=00068200&page=106
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Si motus solis in Ecliptica tam accurate notari
posset, ut mutatio in competentibus horae partibus
esset sensibilis, hinc haberetur loci longitudo. In terra
maximi gnomones accederent. Hora facit in
aqualore 15 gradus  revolutionis; et gradus
in aequatore est ic lecitarum Gemmanicarum
 Lunae MoH) in Eclptica notabilis unasdie. Ancgserentus cum tempore iplunatenit
olonfixtur cum seimeridre solis et
Luna aptior est songitudinibus ideo die
multa de ea Morinus. Etsi autem cursus
ejus nondum perfecte constitutus sit, fortasse
in praviat nondum tabila Theoria, seu causa
posset haberi praxis seu effectus hoc modo:
in certo loco cotidie, quantum licet observentur
lunae appulsus ad fixas, appulsusque momentum
idemque fiat in locis plunb e Et ita ducatur
Linea quo in globo linearo stellato linea
quem luna describit, idque fiat per plures
cunationes, tonec praecise tandem Luna
redeat ad prioresstellas, seu priorem spiratem
repetat. quod fiet ubi ipsius et tervae respectus
ad solem idem fuenit, qui ante. porro hinc
ey
lue quodsi idem fiat in alio ad huc loco,
vel aliis, eo res erit aartior. Nota Hinc
jam colligi poterit, dato loco in terra,
uoodo eo ubi hoc momento spectari
debeat Luna. Et d vicissim  ex datis
lunae locis inter fixas, praesertim in tali
altitudine poli, et tuli distantia a menidre
locus ubi observamus. In globo coelesti utiliter delinea
bitur ubinam ilpsa spectaretur in coelo ex tentio terrre
locus varial pront luna abest a zeuclt. Pera
sunt loco instrumentorio