Stability of the 3:1 Resonance Locking in the 55 Cancri Planetary System

Details Stability of the 3:1 Resonance Locking in the 55 Cancri Planetary System Stability of the 3:1 Resonance Locking in the 55 Cancri Planetary System

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.1289m&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.1289

Physics

1

Scientific paper

The most crowded extrasolar planetary system discovered so far is the
one around 55 Cancri with four planets. We applied Laskar's frequency
map analysis which yields a quantitative measure for the stability of
the system.

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