Si » =J57*29'-3S" vel. 302'.3o'.2j, Orbita erifc Parabo- 

 la diredia, 



cujus Dift. Per. =: 987,0275 =50873930 

 Inclinafcio Radii veci:oris ad axin = 4i°-39'59- 



Motus femper direftus nianebit. 



VII Satelles. 



Diftantia a Saturno = 25,348 4'^''''m. Ann. 



Tempus Periodicnm = 6854023; 

 unde m=: 387-55'' *" = 2.8574942763. 

 Hinc fi 2 =5 o, Orbita Solaris erit Ellipfis direfta , 

 cujus ^ Ax. Major = 2247>o8o = 5.79815? 

 i Ax. Minor = 1263,027 = 4.102837 

 Excentricitas = 1858,529 = 4 795577 

 Dift. Apii. = 4105,609 = ic. 593934 

 Dift. Perih. = 388>55i= 1.002580 

 Tercpus Period. 411 A. C. 198''. 23* 40'. 



Si 2 = 90°, Orbita itidem Ellipfis erit direfta, 

 cujus ^ Ax. Maj. = 441,6416 = 1.139571 

 |. Ax. Min. = 414,0867 = 1.068471 

 Excent. = 153,5561 = 0.396222 

 Dift. Aph. = 595.1977 = 1.535793 

 Dift. Perih, = 283,0855 = 0.743345 



d h 



Temp. Period. = 35. A C. 313 9 57'48". 



«. 



Si s= 980*. Orbita Solaris itidem erit Ellipfis direfta, 

 cujus i Ax. Maj. >= 244,880 = 0.631864 

 t Ax. Min. t= 199,738 = 0.515385 

 Excent. t= 141,671 = 0.3655 5 f 

 Dift. Aph. i= 386,551 = 0.997419 

 Dift. Perih. t= 103,309 = 0.366309 



_ , d h , 



Temp. Period. =1 14 A. C. 25» .33 o. 



Or» 



