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# Title: Leibniz-Handschriften zur Mathematik LH 35, 9, 2
# Folio 69v, page id 00068126:0138
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lineam circularem propriam aequabili mota abse
olirL
sed corpora palidiora et maxume velidissima
ut ipsi planet
se
re non sunt ad motum erxulare
alligata, unde dessidbunt Elliplicum, qui nascitur
ex circulatione farmonica, seu motu arearum
aequabilium. quando inolestat aqualis accatio
distanitia non servatur
s
interna qob noyl slanee
aliones scuper
oficinior quam nimis  oblongo
molus erit ciircurarisqu nisi s quam glapticas nisin
nisi sit ratio deviationis rendie cclipses planetaria
non multum.
menuim a circulis absunt
s
poeve quaelibet ported e
planeta ia ob circulationem ratmonicam in aethere
deferente sine perturbatione ferantur, currabili nature
invento,, ut perinde moveantur, ac in vacuo
ut tum minir sit libertas quae in vacuo foret si omnis
hrope eadem ses
abesset aesaer
Namaeher in quo fecuuum
ipsis sese accommodat, et post multos conflictus eo
tancum desitum est, ut quioam minimam sibi obstent
Mer et planetae
Itaque in orbe ejusdem planeta materiae crgo
tentie ciciulaentis viela materia bes
vibis hujus figid circulantis velocitas ita temporata est
ipsius planetae motui attemperata est, ut cirguli quos
de circulationes sint distantiis a sole proportionales, quod
t
eo facilius fieri potuit qquo minim co discriment
id confliendo mateur partes diversorum orbium
adeoque conferendo et diversos planetas inter se ista
natura gravitatis efficit circullat circulatione
ut circuli quos materi venti orbin maleriae, aetleriae deferentis
aut etiam ipsus placetaes
partes describuns
verocitatibus ab solvantur
uae eut reciproce in sesquiplicata ratione distan
iarum
Ulnde et etiam fit ut in quavis distantia
maneais aeberea venei aecherer solaris a sole
alium concentricum vicieut
unus orbis contra alteru se tueatur