V 1805. Die 2. 



== 535 == 



Aprilis N. St. 



o^ 44' 57",802 



— 3- 



— — - 



48 3<^?23p. 



— 4. 



— — 



52 14, 541. 



— 5. 





$s 53,248. 



— 7. 





I 3 10,5)61. 



t. s. 



Ex quibus, posita obliquitatc apparenti ecclipticae 

 concluditur , 



23 ^l 57 7 8 



Long. 







observ. 



Correctio tabul. 

 solar. 



O^ 12- 



13 



3Q%i^ 



— 9,59 



13 



1 2 



3+7 <^8 



^ 8,4^ 



14 



1 1 



32, 66 



— II, 33 



15 



10 



32, 60 



— 10, 14 



17 



8 



22, 27 



— II, 24 



Die a. Aprilis 



— 3 



— •4 



• ' — 5 



— 7 



Hincque correctio longitudinis Soiis media prodit zz: — 10^15 

 quam in computo positionuni geocentricarum ^ et ^ adhibere 

 placuit. 



Notandum adhuc vcnit, decliaation?s infra rclatas pa- 

 rajlaxi affectss esse, His praemissis ad observationes planeta- 

 rum exponendas progredior. 



Observationes Cereris. 



K 1804. 



Die 8. Sept. N. St. 



— 14. — — 



_ 16. — ~ 



Tcmpus solare 

 medium 



13 44 33 >4 



13 



13 



Asc. recta 5 

 observata 



13 42^3i',28 



15 58, 8 '12 42 32, 19 



6 39, 8 12 20 39, 8 8 



Decl. ^australis 



jo 55 o ,.53 

 II 30 15, 18 

 II 41 26, 14 



A' 1SQ4. 



