) 
( m 
335 
nominationes prius indicatas T, Sc S (unt maiïaer 
Telluris , Lunæ & Solis , B' diftantia Telluris a So- 
le variabilis & ?/i inclinatio orbitæ lunaris ad. edi- 
T + L . 
pticam. Ponendo jam* in hac aequatione ^ k 
. " , SS 
.ni<- "^ 5 ’ S , 
- I fere, ^ -f ^ = v, — = ~ — sPiCof ttwz), 
ubi B eft diftantia media Solis a Tellure, A excen- 
tricitas orbitæ Telluris , & tt differentia inter m'o- 
tum Telluris in longitudinem & motum aphelii 
Telluris, nec non per Theoremata Newtoni vel 
S' I 
Hugenii — — fere, quoniam magis ac- 
B 
. 178 
curata determinatio ipfius ~ noftro non' infèrvit in- 
ftituto, proveniet ddt tdz^ + 
^ 3 k d 
'im^kdz^ ^ ^ n^dz^ 
— (Cof. 2Z’— 2pz) d 
4 
6 tt 
4- — -f&cO-h 
k ^ 
2 t 6 tt 
3 d2i^'(Co(. 2 Z — ■ 2 ?2z) ^ I 
4 
r I 
±t lOt^ 
H- &cc.)-{-2kdz 
a’ Ä 
9 fj2 dz ^ . Cof. 2; ' — nz 
8 « 
/T o- V VA 3 ^4 
-h &c. ) . ( 
g ? vv. 
3 Sin. 22; — 2 7 / 2 i f i 
t 6 tt 
— — .. 
k^ 
+ 
3//^ .Sin. 2 ; — nz 
SB 
■(7- 
2t ^ 6?n^dz^ 
- + &C. )} . 
4 ‘ 
' /- 
