Long-term evolution of the asteroid orbits at the 3:1 mean motion resonance with Jupiter (planar problem)
Astrophysics
2009-11-11 v1
Abstract
The 3:1 mean-motion resonance of the planar elliptic restricted three body problem (Sun-Jupiter-asteroid) is considered. The double numeric averaging is used to obtain the evolutionary equations which describe the long-term behavior of the asteroid's argument of pericentre and eccentricity. The existence of the adiabatic chaos area in the system's phase space is shown.
Keywords
Cite
@article{arxiv.astro-ph/0610025,
title = {Long-term evolution of the asteroid orbits at the 3:1 mean motion resonance with Jupiter (planar problem)},
author = {Vladislav Sidorenko},
journal= {arXiv preprint arXiv:astro-ph/0610025},
year = {2009}
}
Comments
17 pages, 20 figures