Abstract
We report here recent work on the long term evolution of an asteroid near the 3:1 resonance with Jupiter, for planar motion, by making use of a mapping model (Hadjidemetriou, 1993). Some additional results are also included. The mapping is four dimensional and is a model for the Poincaré mapping, on a surface of section, of the elliptic restricted three body problem, near the 3:1 resonance, defined at the times t n = nT, where T is the period of Jupiter in its orbit.
This is a preview of subscription content, log in via an institution.
Buying options
Tax calculation will be finalised at checkout
Purchases are for personal use only
Learn about institutional subscriptionsReferences
Hadjidemetriou, J.D.:1993, Asteroid motion near the 3:1 resonance, Celest. Mech. (to appear)
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1993 Springer Science+Business Media Dordrecht
About this paper
Cite this paper
Hadjidemetriou, J.D., Voyatzis, G. (1993). Long-Term Evolution of Asteroids Near a Resonance. In: Bois, E., Oberti, P., Henrard, J. (eds) Interactions Between Physics and Dynamics of Solar System Bodies. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1902-3_7
Download citation
DOI: https://doi.org/10.1007/978-94-011-1902-3_7
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-4840-8
Online ISBN: 978-94-011-1902-3
eBook Packages: Springer Book Archive