Investigation of Light Pressure Influence on Dynamics of Near-Earth Objects with Reverse Motion

Resumo

In this paper we consider the joint influence of secular resonances and light pressure on the long-term orbital evolution of objects with reverse motion in the near-Earth space with semimajor axes of orbits from 15000 to 45000 km. The orbital evolution of each object is considered for three values of the area-to-mass ratio of the object: 0.001, 1, and 10 m²/kg.