SIMBAD references

2011ApJ...733....8G - Astrophys. J., 733, 8 (2011/May-3)

Tidal evolution of a secularly interacting planetary system.

GREENBERG R. and VAN LAERHOVEN C.

Abstract (from CDS):

In a multi-planet system, a gradual change in one planet's semimajor axis will affect the eccentricities of all the planets, as angular momentum is distributed via secular interactions. If tidal dissipation in the planet is the cause of the change in semimajor axis, it also damps that planet's eccentricity, which in turn also contributes to the evolution of all the eccentricities. Formulae quantifying the combined effects on the whole system due to semimajor axis changes, as well as eccentricity damping, are derived here for a two-planet system. The CoRoT 7 system is considered as an example.

Abstract Copyright: ∼

Journal keyword(s): celestial mechanics - planetary systems - planets and satellites: dynamical evolution and stability - planet-star interactions

Simbad objects: 2

goto Full paper

goto View the references in ADS

To bookmark this query, right click on this link: simbad:2011ApJ...733....8G and select 'bookmark this link' or equivalent in the popup menu