

v^^s»-r ' 



cuntur variationes in orbitis Planetarum Secunda- 

 riorum Solaribus, poft fubitam Priniarii dellru- 

 dionem. 



L UNA. 



DiftantiaTellurisaSole =23992 Semi diansetrisTeUuriSj 



Lunas a Tellure = 60,28» 

 Tempus Periodicuni Telluris = 3i558i5i",4 

 Lunse = 236oy9i'',jj 



Unde m = 3981O0606J r =z 39,7714. 



Si * = o, Orbita erifc Ellipfis, 

 cujus i Ax, Maj. = 429,497 = 1.079134 

 t Ax. IVlin. = 428,414 = 1.076401 

 Excent. = 30,491 = 0.076609 

 Dift. Aph. = 459,988 = i-i5 5733 

 Dift. Perili. = 399,006 = 1.0025^4 



Temp. Period = 409 .10 .36'.! 6". 



Si 2 = iSo, Orbita erit EUipfis, 

 cujus i- Ax. JVFaj. = 371,59 r = 0.933630 

 I Ax. Min. = 370,720 = 0.931443 

 Excent. = 25,415 = 0.06386 

 Dift. Aph. = 397,006 = 0.99749 

 Dift. Perib. = 346,176 = 0.86977 



Tempus Period = 329 .la .5'.4a". 



Si 2 = 90°, five Tellus evanefceret Luna in Quadra- 

 turis exiftente; Erit orbita Solaris Ellipfis, 



cujus 1 Axis Major = 3Q8.4582 = *.,a«*»* 



4 Axis Minor = 398.2657 = 



Excentr. = 12,389$ = 



Dift. Aph. = 410,8477 = 



Dift. Perih = 386,068? = 



Tempus Period. = 365 .ai j'^*''. 



C a Si 



