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18 April 2024
 
  » arxiv » astro-ph/0310121

 Article overview


The apsidal corotation in mean motion resonance: the 55 Cancri as an example
Li-Yong Zhou ; Harry J. Lehto ; Yi-Sui Sun ; Jia-Qing Zheng ;
Date 5 Oct 2003
Journal Mon.Not.Roy.Astron.Soc. 350 (2004) 1495
Subject astro-ph
Affiliation1 and 2), Harry J. Lehto (1 and 3), Yi-Sui Sun , Jia-Qing Zheng (Tuorla Observatory, Piikkiö, Finland Department of Astronomy, Nanjing University, China Department of Physics, Turku University, Finland
AbstractThe inner two planets around the 55 Cancri were found to be trapped in the 3:1 mean motion resonance. In this paper, we study the dynamics of this extra-solar planetary system. Our numerical investigation confirms the existence of the 3:1 resonance and implies a complex orbital motion. Different stable motion types, with and without the apsidal corotation, are found. Due to the high eccentricities in this system, we apply a semi-analytical method based on a new expansion of the Hamiltonian of the planar three-body problem in the discussion. We analyse the occurrence of the apsidal corotation in this mean motion resonance and its influence on the stability of the system.
Source arXiv, astro-ph/0310121
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