Annotation
In the framework of the limited planar circular three-body problem it is shown that asteroids, which are unstable according to Hill, nevertheless can have stable orbits in the case of the first-order resonances. The limits and periods of changes in the eccentricities have been calculated for asteroids of the Hilda group.
© 2016 Publisher M.V.Lomonosov Moscow State University
Authors
I.A. Gerasimov, N.V. Rakitina
Sternberg State Institute of Astronomy, Moscow State University, Leninskie Gory, Moscow, 119992, Russia
Sternberg State Institute of Astronomy, Moscow State University, Leninskie Gory, Moscow, 119992, Russia
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