232 De Causa PHysrca FLuxus 
critque 3x35 Vd'—$6Gdx — 133 dx +24G x 
ot 3X 35  d? s : : 
& x — coran quod fi in denominatore pro 
Ï - 15 Vd “+ = 
« fcribatur valor vero propinquus Fe prodibit valor ma 
3X35 Vd : FANt he 
56G—88Y eritque x: d::15#:8G—27 
quèm proximè. Diverfà pauld ratione prodit x — ïs L 
gis accuratus 
165 VV d . ; 7 
+ Ge » EC. quam feriem producere non eft difficile , 
fi operz prætium videbitur. In Prop. VI. quefivimus figu- 
ram aquæ orbem lunarem complentis ex atione Solis oriun- 
dam. HÂc correétione adhibita, & cæteris retentis ut priùs, 
Axis minor figuræ foret ad majorem ut 46.742 ad 47.742) 
quæ parüm differt àratione quam in ea Propofitione exhi- 
vi re PTLS hib Prop. VIII. ded 
selPLEs . Series quam exhibuimus in Prop. . deducitur per 
ie | ea pee IL Si CA a. CB—ECP—e CF 
= c. Cf=f. Cg=g. Sint ÂACM, À Cm Seétiones quæ- 
vis folidi per rectam 4 C (quæ normalis eft plano BPbp) 
tranfeuntes. Arcus mu centro C radio Cm defcriptus, 
occurrat rex CM in, & occurrant ordinatæ MW”,mu 
Axi Bbhin 7” & v, & circulo BKbin K & k. Sit C4: 
— CM: = x, feu x diftantia focià centro in figura 4 CM, 
fit L Logarithmus quantitatis 4 pre ; & ultima ratio 
— x 
gravitatis particulæ À in fruflum planis 4 CM, À Cm ter- 
minatum ad gravitatem in fruftum Sphæræ centro C ra- 
dio C A defcriptæ iifdem planis contentum, erit ea 3 CM 
x L—x ad x per Prop. II. Gravitas igitur particulæ in 
: . CM XL— x, mu 3CMXxmu  3— 
folidum erit ut /2 - x f — x L— x 
x5 x3 
3CKXKkXCP SES : 
= es XL PE x Dre SIT CT 
. ts e? 
4. Éritque # + Bmx =CM = 4 — x. 
br— e? 
br 
= 0 — x, = Ge €? mme XX 
Unde e: + 
