Investigation of the Influence of the Light Pressure on the Stability of Near-Earth Space Object Motion


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Abstract

In this paper we investigate the influence of the light pressure on the motion stability of near-Earth space objects whose orbital semi-major axes change from 8000 to 42400 km. The orbital evolution of each object with area-to-mass ratio in the range from 1 to 70 m2/kg has been considered. In addition, values of the area-tomass ratio have been investigated at which the objects from various zones of the near-Earth space depart from their orbits under the influence of the light pressure and then fall to the Earth.

About the authors

A. G. Aleksandrova

National Research Tomsk State University

Author for correspondence.
Email: aleksann@sibmail.com
Russian Federation, Tomsk

T. V. Bordovitsyna

National Research Tomsk State University

Email: aleksann@sibmail.com
Russian Federation, Tomsk

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