The Keplerian and mean motions. A geomet
β
Y. Maeyama
π
Article
π
1988
π
Springer-Verlag
π
English
β 636 KB
The point of reference to which the mean m o t i o n of the planets against Keplerian m o t i o n can optimally be applied and the behavior of its astronomical functions are analysed mathematically. To the results o f our problem, which was solved by the first and second laws of KEPLER, virtually al