Planetary motion around an object driven by nongravitational forces.

Författare: Söderholm,  L. H. S.
Dokumenttyp: Artikel
Tillstånd: Publicerad
Tidskrift: Nuovo Cimento
Volym: 108 B   1109-1113
År: 1993


The perturbation of an elliptic planetary motion around a central object is studied. The central object is assumed to be perturbed by a non-gravitational force, which does not act on the planet. The conserved vectors and the Krylov-Bogoliubov method are used.