Annotation
Results from an earlier qualitative analysis on asteroid motion near 2:1 commensurability with Jupiter are compared with those from numerical integration for the equations governing the planar form in the circular restricted three- body problem.
© 2016 Publisher M.V.Lomonosov Moscow State University
Authors
I.А. Gerasimov
Shternberg State Astronornical Institute
Shternberg State Astronornical Institute