Joint influence of secular resonances and light pressure on the long-term orbital evolution of objects in the near-earth space bounded by the semi-major axes of orbits from 15000 to 45000 km is considered. The orbital evolution of each object is considered for three area-to-mass ratios: 0.001, 1, and 10 m2/kg. Special attention is given to a search for resonances whose influence increases the eccentricities of near-earth space object orbits and to their joint analysis with the influence of the light pressure force on the object dynamics.
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Translated from Izvestiya Vysshikh Uchebnykh Zavedenii, Fizika, No. 4, pp. 75–80, April, 2018.
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Aleksandrova, A.G., Bordovitsyna, T.V. & Tomilova, I.V. Special Features of the Joint Influence of Low-Order Secular Resonances and Light Pressure on the Motion of Near-Earth Space Objects. Russ Phys J 61, 687–693 (2018). https://doi.org/10.1007/s11182-018-1448-9
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DOI: https://doi.org/10.1007/s11182-018-1448-9