vs ■■v#Mr 21 - vT^s^-V ' 



Si s = igo, erit orbita Ellipfis retrograda , 



cujus i Axis Major = 999.33S = o.p88j6 

 ^ Axis Minor = 376,499 = 0.323377 

 Excentricitas = 925;, 699 = 0.480624 

 Dift. Aphelii = 192^,034= 0.999480 

 Uift. Perihelii = 73,636 =0038232 



Tempus Period. = 4 Ann. Comm. 15$ .630'. 



Si 2 = 104° 3', 9" vel. 255°-S7'-Ii", Orbita erit Parabola 

 direfta, cujus Dift.Peiihe]ii= 461,525; = 0.239624, 

 & inclinatio Radii veftoris ad axem = i2i*.3a'43''. 

 Deinde vero orbita femper erit Elliptica. 



Si 2 = i4i°.52',27" vel 2t8°.7'-3?, Orbita erit Linea 

 refta , evanefcente axi minori Ellipfeos., & dire- 

 ftio niotus mutabitur. 



II:dus Satelles. 



Diftantia a Jove = 9,494 |^diam. Jovis, 

 Tempus periodicum = 30682 1'',929; 

 Unde ni = 1210,103 & r = 0.9918566. 

 Hinc fi s = o, O' bita erit Hyperbola direfta, 



cujus \ Axis Transverfus = 594,781 = 0.49« yi 



^ Axis Conjugatus = 1705,126 = 1,40907 



Excentricitas = 1805,884 = 1.49233 



Dift. Perihelii = 1211,103 =1.00082. 



Si S = O, Orbita erit EIJipfi.s retrograda, 



cujus i Axis Major = 604,572 = 0.499624 

 i Axis Minor = 7,017 = 0.005798 

 ExcvjntrititaS = 6041551 = 0.499567 

 Diftantia Aph. = 1209,103 = 0.999191 

 Dift. Perihelii = 0,041 = 0.000056 



Tempus Period. = 4 Ann. Comm. 71 .21 47'. 



Si 



