Results of numeric integrations of orbits of (5026) Martes and 2005 WW113 asteroid pair
Alexey Rosaev
TL;DR
This study uses numerical integrations to analyze the orbital dynamics of the young asteroid pair (5026) Martes and 2005 WW113, revealing resonant perturbations affecting the larger asteroid but not the secondary.
Contribution
It provides new insights into the resonant interactions and orbital evolution of a young asteroid pair through detailed numerical simulations.
Findings
(5026) Martes experiences strong 3:11 mean motion resonance with Earth.
2005 WW113 is not affected by the resonance and moves away from it.
Resonant perturbations influence the orbital stability of the larger asteroid.
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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Taxonomy
TopicsAstro and Planetary Science · Planetary Science and Exploration · Stellar, planetary, and galactic studies