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# Title: Leibniz-Handschriften zur Mathematik LH 35, 15, 6
# Folio 2r, page id 00068208:0003
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concessum est. quamobrem si nota sit ex observatione,
certa distantia Lunae a polo, haec distantia meridianum
in terra specificum indicabit.
Collige 2. quod omnibus astronomis videbitur prorsus
admirabile, scilicet motus Lunaris anomaliam non
polle impedire certitudinem Longitudinum; quod
manifestum est ex dictis; quia si singuli meridiani
habent, uti probatum est, distantiam Lunae apolo sibi
specificam nc necessariam, accidet ut sive tarde moueatur
Luna, sice celeritem, debeat semper et necessario distantia
illa diversa in singulis meridianis reperiri. quod est ab
omni ratione temporis vacare; dque enim volumus
In Mari scire quandonam acadet calis vel talis distantia
a polo, ad hoc et meridianus fuic distantiae proprius
indigetur; sed volumus ut cognita, etiam ex casu,
tali vel tali distantia funae apolo, meridianum illiuo
proprium illico cognoscamus: quod omnino facilé erit
a
assequi postquam singulis meridianis terrae fuerit appropriata
at
distantia Lunae a polo: cuius rei methodum alibi tradimus.
Pollige 4. hoc quod initio diximus, sulicet quod sublato
rimore andmaliae in Luna eliminamus a nobis omnem
motus medii correctionem. quae sand correctio ad nihl
juuat nisi ad habendum, et pronosticandum tempus coniunctionum
Lunarium, vel oppositionum, vel alicuius elongationis
cuncta pi
quae(nullomodo quaerims. qu’a propter remotis illis,
Pit
negletoque ad stellas omni Lunae aspectu, ut solem et
stellis
Hellas a mundo remondmus, exceptis illis quae cum Luna
in ceraem meneiare reperi entu et putemes ingrant