■,<w^,*_ 



31 :^^ 



Hinc fi 2SO, Orbita Solaris erit Hyperbolica, 



ciijas i Axis Transverfiis = H778,33 = i. 45^84 J 



I Axis Conjugatus = 16003,37 = 1.977953 



Ex<entL"icitas = 19869,70 = 2.45 J968 



Dift. Perihelii = 809 'jS? = 1.000125. 



Si s = 180, Orbita erit EUipfis, 

 cujus 4 Ax. Maj. = 4326,42 = o.j 34761 

 J Ax. Min, = 2134,97 = 0.263891 

 Excentr. = 3762,95; = 0.465 115 

 Dift. Aph. = 8o89)37 = 0.999876 

 Dift. Perih, = 563,47 = 0.069646 



a 



Teinp. Period. = 32 ,6 19 r. 



Si 2 =62°.26'.i4" vel s^^'*.^^'.^^", Orbita erit Parabola', 



cujus Diftantia Perihelii =6792)87 = 0.839632 

 & Inclinatio radii veftoris 'ad axin vel Anomalia = 

 47°.i3'.2i". Motus hujus & fequentium Satellitum 

 femper erit direftus, quoniam *• nbivis > i (§. iV. 3). 



Satelles Ihdus. 

 Tempus Periodicum Siderale Herfchelii asfumo =3 



a d h 



83 '50 tg , 



Tempus vero periodicum interioris ex duobus cogni- 



d h , ., ^ 



tis Satellitibus traditur = 8 »7 1 19 ,3, & masuua 



digresfio = 3 3 ",09; 



nnde m = 6233,6778 & r = i, 78197918« 



Hinc fi 2 = o, Orbita Solaris erit Hyperbola, 



cujus 5- Ax. Transv. = 14246,39 = 2.28 ?39i 

 i Ax. Ccnj. = 14714,50 = 2.360484 

 Excentr. = 20481,10 = 3.285558 



Dift. Perih. = 6^34^7 — 1.000 167. 



Si 



