Titlebook: A Comparison of the Dynamical Evolution of Planetary Systems; Proceedings of the S Rudolf Dvorak,Sylvio Ferraz-Mello Conference proceedings

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G. Cioni,A. Colagrossi,A. Miolaf the basins is found analytically, while the relative area of the basin M. is given by an empirical formula. Further empirical formulae give the exponential decrease of the number of asymptotic orbits that have not yet reached a black hole after . iterations.

lambaste

A canonical form guide to symbolic summationrturbation parameter. According to the results obtained, we conclude that the stickiness effect of tori is caused mainly by the hyperbolic invariant sets near the tori, and the diffusion speed becomes larger when orbits diffuse away from the torus.

委屈

F. Parisi-Presicce,A. Pierantonio, a high percentage of ocean area significantly increases the probability for habitability of planets on stable orbits in extrasolar planetary systems. We show that the systems ε Eridani and 55 Cancri are most promising to find dynamic habitable Earth-like planets, while the system ρ Coronae Borealis is most unpromising.

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https://doi.org/10.1007/1-4020-4466-6Astrometry; Celestial mechanics; Galaxy; Planet; Planetary system; Solar System; solar; stellar

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