334 
' N 
J 
r, f 
o v QJD 
ftitiitis ,i qiias adhibuerat Dom. d' Alembert , & 
quæ lam huic æquationis formæ quam noftro in- 
Itkiuo præcipue funt accommodacæ, dabit æquatio- 
nem abjjjaoc Auctore prolatam -pag. 56 Theorie 
' f ( î;;' -i i ^ . . *( T L) 
dç - la ,L,une , ddvr-\-' v^d zf. -H 
dz (T-{-'L)dz 
4rr : 
Sdz ^ 
■ '/ 2 V \‘ È'^gg 
• J I .1 
+ 
3 Sdz^ Cof. 2 s 
Cof.as — 2/2; 
2 7 ? 
^Sdz"^ .CoC. Z— n Z 2 .(iT-hL). js rdz 
,%v*B'*gg gg -'v’gg 
a S . Sin. 2Z • — 2«« aS. Sin. z — nz 
.--- — . -f, 1-1^ ‘ — 
- = ?•'!' 
3 . 2 7/2"^ dz^ ( T-p L) 
>: 
4^5- 
iS'^ 'r 
« 
S dz , Sin. 2 Z — niz 
2 V^ B' ^ gg 
, 2mm , T -f L.dz^ Çof. 2Z— 2pz " 
^ ^ — 
: . ' 4.?^ 
3 Sdz . Sin! 22; • — 2nz '^Sdvdz . Sin. 22; — 272 z 
zv '^' B'^gg iv '^ ggB ''^ 
2S dv dz S^\r\,z — nz . « v, a 
H r-- ;r — î m qua pro 2i' & g lub- 
Sv ^ ggB '* ^ ^ 
jftituimus nz Sz pz ^ defignantc n rationem* tem- 
poris medii periodici Lunæ ad illud Solis, & p 
rationem motus medii nodi Lunæ ad illum ipfius 
Lunæ, quoniam accuratiore determinatione angu- 
lorum z' & I' non opus fit ad ratiocinia noftra fe- 
queiitia formanda, & in qua æquatione præter de- 
no' 
