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# Title: Leibniz-Handschriften zur Mathematik LH 35, 10, 1
# Folio 9r, page id 00068154:0017
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11 1
Ellipseos muior di apis  distantia socorum e, inor
Exis minor b erit
bb = 99- ee
muxium distantia est ote, minima, q-e lorum medium geo-
metricum est X2b at arithmeticm est =9
 bh + bd = bh+ du =  bd - dh = id
a sol eet liceturbitae
obiba: ba: dh.
0 ob
+b
bo
ib = = dh
di medium arichmeticum
inter do  bd et btr
circumferentia circuli radio id descripta
fere est aequalis circumferentiae
tia Ellipheos cujus diametri
suns do et h, sic tamen ut ircum
ferentia Elliplica sit longior
Tempora periodiceum puli
13769 12
4332
686
d
37
S9
224
15
42
d
V
arcus diurustecipur
3
morae in partibus aequalibeus Eccensrici
observant proportionem intervallorum asole
(Eocentiius quimotu medim metitarcircutus centro sole dscripeus)
planeta absoluto totius circuatus, qua
drante a suo Aphelio praecise mediare habet
habet intervallum a sole inter ma
inir
a
lio
si planeta un una dierum quando est in
periheho distaret a sole partibus 10 in opposita
die inperihelio certum est quod ex sole apparens
ejus promotio (+ incrementu anguli L)  fatura
sit ad apparentiam in perihelio sicut 8I ad
100 (+ in eversa duplicatat
pra porho quae est inter binorum quorumcunque
planetarum tempora periodica est praecise
vediarum
distantiarum Ed est orbium ipsoru attento
tramen hoc quod medium mrithmeticum inter utrumque
diametrum Ellipticae orbitae est paulo minus longiore
hec
. et 10052
5451
166
101E
729
ein non st valde magna, et inmercurio
tulatur ips
9510
8200
1524
100D
724
388
E
8968
4948
82
B2
9
107
8968
19026 ad
9510 atb.
probabile est corpora
planecacim esse ut periodica
tempora
ut mora diumae
Arens diurnimedis
E
1
3