Astronomy and Astrophysics – Astronomy
Scientific paper
Apr 1994
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994cemda..58..353d&link_type=abstract
Celestial Mechanics and Dynamical Astronomy (ISSN 0923-2958), vol. 58, no. 4, p. 353-370
Astronomy and Astrophysics
Astronomy
14
Celestial Mechanics, Circular Orbits, Orbit Calculation, Orbital Mechanics, Particle Trajectories, Perturbation Theory, Radiation Pressure, Satellite Orbits, Two Body Problem, Gravitational Fields, Thrust Vector Control
Scientific paper
The motion has been studied of a particle in a gravitational field perturbed by radiation pressure. By combining the formulation in the physical space variables with the KS variables we obtained explicit evidence for the existence of a surface of stable circular orbits with centers on an axis through the primary body. Furthermore, the effects of a sharp shadow on the two-dimensional unstable parabolic orbits were investigated. It was found that they do not survive the introduction of a shadow.
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