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Stability Mechanism of Planetary System of ν Andromedae

Authors :
Hiroshi Nakai
Hiroshi Kinoshita
Source :
Symposium - International Astronomical Union. 202:202-204
Publication Year :
2004
Publisher :
Cambridge University Press (CUP), 2004.

Abstract

Three planets are detected around ν Andromedae. The stability of Upsilon Andromedae Planetary system is maintained by the co rotation of the pericenters of the two outer planets. If the pericenters of the two outer planets move independently, the planetary system becomes unstable. The corotation of the pericenters is explained by the secular perturbation theory. This corotation is not a secular resonance.

Details

ISSN :
00741809
Volume :
202
Database :
OpenAIRE
Journal :
Symposium - International Astronomical Union
Accession number :
edsair.doi...........b0c0d9aa9bcc9644e95d43e8eb4ae1db
Full Text :
https://doi.org/10.1017/s0074180900217853