Abstract
Based on the ideas of Lyapunov’s method, we construct a family of symmetric periodic solutions of the Hill problem averaged over the motion of a zero-mass point (a satellite). The low eccentricity of the satellite orbit and the sine of its inclination to the plane of motion of the perturbing body are parameters of the family. We compare the analytical solution with numerical solutions of the averaged evolutionary system and the rigorous (nonaveraged) equations of the restricted circular three-body problem.
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Original Russian Text © M.A. Vashkov’yak, 2006, published in Pis’ma v Astronomicheskiĭ Zhurnal. 2006, Vol. 32, No. 10, pp. 787–795.
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Vashkov’yak, M.A. Periodic solutions of the singly averaged hill problem. Astron. Lett. 32, 707–715 (2006). https://doi.org/10.1134/S1063773706100069
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DOI: https://doi.org/10.1134/S1063773706100069