Abstract
The motions of asteroids in the secular resonance v6 are investigated by a simple analytical model. By using this model, it is found that eccentricities of asteroids may become very large (e ~ 0.8) when asteroids are in or near this resonance. These large increases in eccentricity are also confirmed by the numerical integrations. The strongly depopulated region in the asteroidal belt, which corresponds to the position of the secular resonance v6, is explained well by this analytical model.
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© 1988 Kluwer Academic Publishers
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Yoshikawa, M. (1988). The Motions of Asteroids in the Secular Resonance v6 : An Analytical Model and Numerical Calculations. In: Roy, A.E. (eds) Long-Term Dynamical Behaviour of Natural and Artificial N-Body Systems. NATO ASI Series, vol 246. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-3053-7_26
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DOI: https://doi.org/10.1007/978-94-009-3053-7_26
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-7873-3
Online ISBN: 978-94-009-3053-7
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