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Article
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 |
AbstractThe 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.
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