IF. Satelks. 



DiRantia a Saturno = 2,688 Idiain- Ann. d) 



Tenipas Period. = 336691'', 

 unde tn — ^6S4,626,r^ 0,93054277» 

 Hincfi2=o, Orbita erit Hyperbola direfta, 



cujus 4 Ax. Transv. = 1585,740 = 0.433899 

 ^ Ax. Conjug, = 4995,736 = 1.366962 

 Excentricitas = 5241,66 = i. 434173 

 Dift. Perili. = 3655,626 = 1.000274. 



Si s =: 180*, Trajeftoria erit Ellipfis retrograda , 



cujus 4 Ax. Major = 1831.915 = 0.501259 



i Ax. Minor = 193,080 = 0.052832 



Excentr. = 1821,711 = 0.498467 



Dift. Aph. = 365 3, 62-:^ = 0.999726 



Dift. Per. = 10,204 ~ 0.002782 



Temp. Period, = 10 A. C. 168 659'. . 



Si s = 94°.7'.5o" vel aSs^.^s^.io'', Trajeftoria erit Pa- 

 rabola direfta : 



cujns Dift. Per. = 1556,6496 = 0.425811 

 Inclinatio Radii veftoris ad axin = 98°.3i'-42". 



Si » = i5P'.3i'.3i'' ve! 20i°.28'29'', raotus a diiefto 

 inutatur in Retrogradum, & vicisfim. 



V. Satelks. 



Diftantia a Saturno = 3.752 4dia,in. Annuli 

 Tempus Period. = 3903 ii"i 



Un. 



d) Bradlsjns quidem hujns Satellitis diftmiliam ponit = 

 2-,6sf ^Lyiim. Annnli; a ier.ipore vero Periodico SrJ:'litif illam 

 tffe = 2 iig conjlat. De cetero krrc djffergnna parvi admodiira 



ep pj.pmsnti in coiufuJtonihiii\ 5;;^' indc deducuniur. 



