Planetary motion around an object driven by non-gravitational forces.

Details Planetary motion around an object driven by non-gravitational forces. Planetary motion around an object driven by non-gravitational forces.

Oct 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993ncimb.108.1109s&link_type=abstract

Nuovo Cimento B, Vol. 108, No. 10, p. 1109 - 1113

Physics

Planetary Orbits

Scientific paper

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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