Modeling Trojan dynamics: diffusion mechanisms through resonances
Abstract
In the framework of the ERTBP, we study an example of the influence of secondary resonances over the long term stability of Trojan motions. By the integration of ensembles of orbits, we find various types of chaotic diffusion, slow and fast. We show that the distribution of escape times is bi-modular, corresponding to two populations of short and long escape times. The objects with long escape times produce a power-law tail in the distribution.
- Publication:
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Complex Planetary Systems, Proceedings of the International Astronomical Union
- Pub Date:
- July 2014
- DOI:
- 10.1017/S1743921314007959
- arXiv:
- arXiv:1508.00450
- Bibcode:
- 2014IAUS..310...96P
- Keywords:
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- Celestial mechanics;
- methods:numerical;
- Astrophysics - Earth and Planetary Astrophysics
- E-Print:
- Published on Complex Planetary Systems, Proceedings of the International Astronomical Union, IAU Symposium, Volume 310, pp. 96-97