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# Title: Leibniz-Handschriften zur Mathematik LH 35, 15, 6
# Folio 1v, page id 00068208:0002
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HT
Sit semita Lunae sprraus ABCDF. FBr apiatur qua
Luna ex A in B, ex B in C.
ex C in D, ex D in F. et sic
De caeteris R. 6. H. T. Dico
este abiques diversam distantiam
Lunae a polo K, vel polo L.
et nunquam unam distantiam
in aliam coincidere. quod
est manifestum, nam cum
Luna motu suo circulari
AMN diversos semper, live
Almikantarathos, sive parallelas
attingat, punctaque singula circuli Lunae cum punctis
spiralis coincidant, siquidem ab eodem mobili, seu Luna
peragrantur, debet esse abique tam in spirali quam in
circulo Lunae diversa distantiae Lunge à polo. hoc est,
debet esse alia distantia AK, alia BK, alia CR. et sic de
caeteris
Aduerte autem: Licet altera medietas circuli Lunaris NOA
habeat puncta quae sunt in ea distantia aequali a polo cum
punctis primae medietatis AMN, habebitur tamen discrimen
meridianorum ex adcensu vel descensa Lunae, et sic Lunq
ascendens ex M in N, distinguit meridianum MK a meridiano
OK. quoniam Luna ex N descendit ad 0.
olliqe1. quod cum omnes maridiani caeli exarentur in
terrae superficie, siquidem meridianorum omnium plana
centrum terrae geruadunt, habebunt  Singuli meridiani
terrae situm coelestem specificum, sibique specialem; hoc est
specificam distantiam Luna a polo. quod omnino ab Astronomit