CALCVLVS ECLIPSIS SOLK. 3^^ 



Pro corredlionibus inueniendis producatur 3 A Tab, IV. 

 iti 2 vt fit Aszii^ vnde diftaatia O A augetur ^^S- '°- 

 particttk ?^^JL2 



Log. P =1:3.4430028 

 Log. cof.G A^— 7. 6098 5 30 



i.o5a855* 

 Log. IIrz=3.5<539555 crgohaeccorredlio =0,003.« 



7.4889003» 



Deindc ducatur eclipticae parallek A x -rz x ^ 

 qua diftantia O A augetur parricula x cof. B O A , 

 quae ergo corred:io erit -f- o, 791. x. Denique ad 

 A X normaliter rurfum ducatur Aj zizy qua diftan- 

 tia O A itidem augetur particula y fm. B O A zr 

 -i-o, 612.J', quocirca diftantia centrorum correda 

 erit 



1925, (J-{- 0,003. -s-f-o, 791. jp-H-Oj^fia^ liiiac (i 

 fumma femidiametrorum ^-|-/^n 19(53.0 augmen* 

 tum ^ requirat aequatio finalis erit 



37. 4-1-^ — o, 003. s-}-o?79i- x-i-Q\6i2.j 



cx initio autem conctufimus hanc acquationem 



5o— ^ — o^ &(Ji.2J-f-o, 83<^. .i:~o,-548.x 



quarum fumma a eorredioie S liberata erit 



^7. 4=10, 8^4. 2+ 1. 621:, X 4- Oj, q6^./. 



II. 



