Results of numeric integrations of orbits of (5026) Martes and 2005 WW113 asteroid pair
Abstract
The orbital dynamic of very young asteroid pair (5026) Martes and 2005 WW113 is studied by numerical integrations. We discover strong resonant perturbations of the larger member of pair (5026) Martes by the mean motion resonance 3:11 with Earth. The unbounded secondary (2005 WW113) moved far from the resonance and is not perturbed.
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