Stability of the GJ 876 Planetary System

Details Stability of the GJ 876 Planetary System Stability of the GJ 876 Planetary System

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001pasj...53l..25k&link_type=abstract

Publications of the Astronomical Society of Japan, Vol.53, No. 4, pp. L25-L26

Astronomy and Astrophysics

Astronomy

24

Celestial Mechanics, Mean-Motion Resonance, Methods: Numerical, Planetary Systems: Individual (Gj 876'S Planets)

Scientific paper

The newly discovered planetary system of the GJ 876 is stabilized by a 2:1 mean-motion resonance. We carried out numerical simulations of the GJ 876 planetary system for several sets of initial epochs, and investigated their stability, since this planetary system is very sensitive to an initial epoch because of a large difference between the osculating elements and the mean elements.

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