Estimation of the effect of the moon, sun, and light pressure on the motion of a geostationary satellite

Astronomy and Astrophysics – Astronomy

Scientific paper

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Gravitational Effects, Orbital Mechanics, Pressure Effects, Satellite Perturbation, Synchronous Satellites, Lunar Gravitation, Radiation Pressure, Solar Gravitation, Spherical Coordinates

Scientific paper

Perturbations in the motion of a geostationary satellite due to the attraction of the moon and the sun and those due to light pressure are considered. Formulas are obtained for estimating these perturbations in spherical coordinates. Results of calculations for time intervals of 10, 30, and 90 days are presented. For a period of 30 days, perturbations due to the moon and the sun reach 400 km and 170 km, respectively; perturbations due to light pressure are 9.4 km (without allowance for shadow) and 4.6 km (with allowance for shadow).

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