Planetary motion around an object driven by nongravitational forces.

Authors: Söderholm,  L. H. S.
Document Type: Article
Pubstate: Published
Journal: Nuovo Cimento
Volume: 108 B   1109-1113
Year: 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.