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.
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Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 3, pp. 86–91, March, 2019.
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Aleksandrova, A.G., Bordovitsyna, T.V. & Aleksandrov, V.B. Investigation of Light Pressure Influence on Dynamics of Near-Earth Objects with Reverse Motion. Russ Phys J 62, 484–490 (2019). https://doi.org/10.1007/s11182-019-01735-7
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DOI: https://doi.org/10.1007/s11182-019-01735-7