6.1589437; unde Log. - 0,4921014, cm (1 



addatur Log. (i + i^2) = Oj38377J6,4, eric Log i/J 

 = o.874877054> & ^ = 56,2023. Qui valor, fi pro i 



D-hd-tV2D.D-\-d fl2^\no- 

 fubftituatur in — n ^ a \ ^^ / 



vus prodibit ipfius valor = 57,i49; & hoc iterum 

 fubftituto erit^= 57,166, qux miilefima partefemi- 

 diametri Jovis a vera diftantia d non differt. O- 

 mnium Satellitum, qui remotius a Jove,circa ipfum, 

 ceu Primarium, fuos abfolvunt gyros, orbitae So- 

 lares ubivis erunt Ellipticae, & qu idem motu fem- 



m + l + \/ 2m.m-\-\ 



ner dire£lo, nam r = j lem- 



^ m — I 



per eft major unitate, (§. IV. n. 3.). 



Simili modo inveniri potcft diftantia d a Plane- 

 ta Primario, intra quam orbitac Solares Satellitum fem- 



r — I i/m-^i 

 per forent Hyperbolicse, ponendo fcilicet y 



— ffj -t- I -\-\/ 2m,m — i 

 — \/i, unde r= 



m -f I 



D -h d 



,-D + ,+ l/an.D^i -Tv/^| calculumque 

 27T1 ^^ ^^ J ^^ 



