17 ^ t^' 

 Tcmpus Pcriodicum invcnitur pcr rcgulana 



Keplcri = T/^Tcmp. Per. 7^ x ^ Ax. major = 



Difl:. 7/1 a o 



r^ 



37433683» X 9 99^33477' = 13990501", 6 = 



19*6,0333 

 4 Annix Comm. 159'^. 6^30'. 16". 



Quo habeatur diftancia Satellitis ab oppoficione 

 fivc z, ut orbitx Solarcs Hypcrbolica: dcfinant, & 

 EllipticK incipiant, h. e. ubi orbita Solaris crit Pa- 



rabola, ponendus eft Cof. % - • — — q. pr. (§. IV. 



^ ^278646 1 ^ ^^^ ^^^,^ 2'.9", & fubftitucn. 



% X 0.78646 

 do hunc pro z, proque m & r asfumendo corum 

 valores 1926,0333 & 0,78646 in cxprcsfionc Cof 2; = 



— Ij+^; propius obtinctur x. 



rm 



V^i + m^+awiCots ar 



= I04°,i'.48", idquein noftro cafii absquc omni cr- 

 rore fenfibili. Invcnto vcro x. habetur per §. III ».*• M 

 = fin. 2g-.i8'38"»- & D= i925,7(,07, Diftantia Pe- 

 rihelii = M^ = 461,525, angulus ylS/? ($. 111.«. 3- 

 Fig. 2) five inclinatio axeos SR Parabol^ ad ra- 

 dium veaorcm ^A =180° — »2= «8o — 5H*-37-'i7' 

 = 131. 23.43. Tendit vero in hoc pun£lo Satelles 

 verfus Perihelium , & orbita Solaris erit Elliptica 

 ad 58°37'-i7" ab utraque parte conjunftionis. 



VOL. VII. C ^'f- 



