,>-»^i- 



15 =^^irKJ^ 



laris Ellipticam induerit figuram; qui vero Priru;" 

 rio funt propiores, motum asfumunt retrogradunij 

 orbita Solari adhuc Hyperbolica exfiftente. Plura 

 confeflaria a §. III deduci posfent, fi cui, m.undo 

 huic posfibilium diutius immorandi otium esfet. AI- 

 lata vero quoque vaiere de SatelHtibns, Ci qui finge- 

 rentur, motu retrogrado incedentibus, mutando quan- 

 titatem r a pofitiva iiinegativam , cuivis obvium eft. 



§. V, 



Rem exemplo , a primo Jovis Satellite defum- 



to, illuftrabimus. 



Eft diftantia Jovis a Sole = 114885788 Semid. v. 



Diftantia Primi Satellitis a Jove = 5 965 Semid. ^», 



,. , 11488,788 ^ 



Unde tn — ; = 1926,0333. 



5,965 

 Ulterius eft tcmpus Periodicum ^ = 374336831"= T, 



Tempus Period. I:mi Satellitis = i52853"5476=f, 

 Hinc »" = ^ {§' in.) = 0,78^46. 

 Ponatar primo Satelles in oppofitione five 2 = o & 



Cof2=+i;EritN=— /^^^(§. IV.) = 



r m 



1,78646 1/1927,0333 „ ,, 



-i—- // ;' = 2,»7an , & N^ = 5,162484, 



quod orbitam Solarem fore Hypcrbolam direaam: 



D 



indicat (§. II.), cuius femiaxis Principalis =-; 



iV^ — 3 



= .-r; = = 009,3415, & fcmi-AxiS 



€0!1- 



