Physics
Scientific paper
Apr 2010
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010eas....42..315m&link_type=abstract
EAS Publications Series, Volume 42, 2010, pp.315-331
Physics
Scientific paper
This chapter is a review of the dynamics of two-planet systems. It includes the study of averaged models of both secular and resonant planetary configurations. The introduction describes our understanding of long-term planetary behavior and stability. The next section introduces the presently known sample of 31 extra-solar systems and the classification of these systems with respect to their dynamical behavior. Their secular dynamics are described in Section [see full textsee full textsee full textsee full text], where we also introduce the main techniques commonly used for exploring dynamical features. We conclude this section by describing the effects of the proximity of a secular system to mean-motion resonances. Finally, phenomena related to mean-motion resonances are presented in Section [see full textsee full textsee full textsee full text].
Beauge Christian
Ferraz-Mello Sylvio
Michtchenko Tatiana A.
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