CALCVLVS ECLIPSIS SOLIS. 3<^3 



O A O rr 37". i<J' AO=:i<Jo8, 5 



G3Az=i5. 55 Log.OOz:3.o87<J7!^i 



30A— 21. 21 Lfin. 0^0=9.7821324. 



I, ,11,, 



A03=r53. 50 Log.V3:3 3o55 397 



AOA — 32. 29 Vzi:202o, 8. 



Ad correc^ioHes rnireniendas continuetur 3 A Tab. III. 

 iii «, "vt fit A 2; t=: ^ , hinc diftantia O A minne- ^'S 8. 

 tur particula y cof. O A O. 



Log. P=z3,4aS55io . 



LQg.cQDO A0=9- 900 8 1 8 1 



r- — hi«e ergo nafcitur corrcdio^ 



3.3293^91 Z.^ .je, ^ 



Log.n = 13. 5(^34811 ' ,T 



Log.Pg-.GAO __p^ .^^ j g ^ ^Q^ 



Deinde ob ang. A O A rr 32°. 29^ ducatur 

 eclipticae parallela A a*zi:xH- o, 591. 0, qui cor- 

 ret^ione diftantia O A minuitur particuk Ax eof. 

 A O A =z,o y 843 x: H- c, 4.97. 0. Tertio deBique 

 fumta Aj zz>' — o, 055. , inde drftantia O A au- 

 getur particula Aj fin. AOA — o, 537.J/— 0.030.9. 



Vera igitur diftantia centrorum erit 



2020,8 — 0,583,2— 0,843. a'H- 0.5 37/.J— 0,5 27. d 



fummae femidiametrorum 1963,4.^-^ aequanda 

 fieque habebitur : 



57,4-^:10,5 83, 2;4-o.,845.^-C^^537.j4-0,5a7-^- 

 . Zz 2 ^ Finis 



