5^7 



horizontati^ fuit ri:.i",<l)i. Reductis itaque observationibus supra 

 allatis ad centrum Saturni , reperitur : 



Die ^ Martii 

 Eiie ^j —/ 

 Die i| — 



Ex quibus elicitur : 



Dic iQMartii 

 Dic X - 

 Die g — 



Asc. 



reeta obser- 



DecL borealis 





vata t> 



t> 



i8i' 



15" i-,56 



i' i^ 38'',0 8. 



i8i 



10 4.8, 45 





i8i 



6 33, 00 



2 20 2<5, ^4. 



180 



57 5^? 85 



2 24 15, 18. 



Long. |) apparehs 



6'" 0° 14 23 ,42 

 6 o 5 4,98 

 5 29 55 40, 17. 



Lat. bor. -^ 



2° 35 12 ,88. 



2 35 19, 28- 



2 35 23, 37. 



Adhibita correctione longitudinis Saturni ex aberratione luminis 

 ■^ii -f-< iS''''^^, ex Nutatione ~ H- 12 ^^,^5, et correctione latitu- 

 dinis ob aberrationem luminis ~r — o ^,12 non neglecta, prodit: 



Bie r| Martii 

 Dic g — 

 Die g — 



Long. geoc. vera 



6' 0-13' 57^30 

 6 o 4 38, 8<5 



5 ^9 5S 145 05 



Latitudo vera 

 borealis 1p 



2 35 13 ',00. 

 1 35 19^ 40- 

 ^ 3s5 235 45^* 



Unde sequentes tabukfum Saturni correctiones obtinentur; 



Ex 



