Some aspects of the chaotic diffusion of Trojan asteroids

Details Some aspects of the chaotic diffusion of Trojan asteroids Some aspects of the chaotic diffusion of Trojan asteroids

May 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002padeu..12...33s&link_type=abstract

2nd Workshop of Young Researchers in Astronomy & Astrophysics, Publications of the Astronomy Department of the Eötvös University

Astronomy and Astrophysics

Astrophysics

Scientific paper

A recently developed mapping model for the 1:1 resonance has been used to investigate the long term dynamics of Jupiter's Trojans. It has been found that the indirect planetary perturbations destabilize the outer part of the stability region, where there is a 13:1 secondary resonance. A conjecture has been risen up that this region might serve as a natural boundary of stability for the Trojan asteroids.

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