Summary
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.
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Söderholm, L.H. Planetary motion around an object driven by non-gravitational forces. Nuov Cim B 108, 1109–1113 (1993). https://doi.org/10.1007/BF02827306
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DOI: https://doi.org/10.1007/BF02827306