Mapping models for the motion of asteroids near a resonance.

Details Mapping models for the motion of asteroids near a resonance. Mapping models for the motion of asteroids near a resonance.

Dec 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990ndpd.conf..219h&link_type=abstract

Comptes-rendus de la table ronde: Nouveaux développements en planétologie dynamique, p. 219 - 227

Other

Minor Planets: Orbit Theory, Minor Planets: Resonances

Scientific paper

A simple mapping model is obtained for the motion of an asteroid near a resonance with Jupiter, assuming a circular orbit for Jupiter. This mapping has all the main features of the actual system, i.e. the correct values for the fixed points (periodic orbits) and the correct stability indices. The method is applied for the 3:1 resonance, but can be used for the study of motion near any other resonance and also far from resonance.

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