Hinc (12 = 0, erit Orbita Solaris Hyperbola direfta, 



cujus 4- Ax. Transv. = 1683,807 = 0.216253 



4- Ax. Conjug. = 8970,191 = 1.205336 



Excentricitas = 9126,957 = i. »36387 



Difl. Per. = 7443,1 j = 1.000134. 



Si a = 180, erit Orbita Ellipfis Retrograda, 



cujus i Ax. IVlajor = 4338,314 = 0.582938 



i Ax. ]VIinor= 3031,058 = 0.407417 



Excentr. = 3101,836 = 0.416927 



Di(t. Aph. = 7441,15 = 0.999865 



Dift. Per. = 1235,478 i^ 0.16601 1 



Tempus Period. = 13 Ann.Comm. 43 .13 .19. 



Si s = ii6°.9.r5 vel. 44J. 50.45, Orbita erit Parabola 



direfta, cujus dift. Periii. = 390,93235 =; o.o^ijjgi, 



& Inclinatio Radii veftoris ad axin == i5 3*.30. 



Si 3 — 130*41' o" vel 329'. 18' o' , Orbita erit Linea 

 refta, & direftio inotus mutabitur 



JJ. Satelles. 



Diftantia a Saturno = 1,694 ^diam. Annuli, 

 Tempus Period. Satellitis =3 118389'j 



Unde m = 5799.077, r= 0,759. 

 Hinc fi 2 = o, Orbita erit Hyperbola direfta, 



cujus 4 Ax. Transv. =3 1637,390 =0.282353 



4- Ax. Conjug. =7354,990 — 1.251060 



Excentricit. =7437,467—1.282526 



Dift. Perih. — 5800,077 ~ 1.000173. 



Si s — 180, Trajeftoria erit Ellipfis retrograda, 



cujus ^ Ax. MHJor =3093,793 =0.533325 



^ Ax. Minor ~ 1498,9^6 — 0.2^8478 



I5xcentr. ~ 2705,284 = 0.466503 



Dift. Aph. -j 5798.077 =0.999828 



Dift.Perih.= 3875^09=0.066822 



Temp. Period. = it Ann. Comm. 175 ,11 .23'. 



Si 



