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Tidal evolution of a close-in planet with a more massive outer companion

Published online by Cambridge University Press:  10 November 2011

Adrian Rodríguez ,
Sylvio Ferraz-Mello ,
Tatiana A. Michtchenko ,
Cristian Beaugé  and
Octavio Miloni
Adrian Rodríguez
Affiliation:
Insituto de Astronomia, Geofísica e Ciências Atmosféricas, Rua do Matão 1226, 05508-900 São Paulo, Brazil email: [email protected]
Sylvio Ferraz-Mello
Affiliation:
Insituto de Astronomia, Geofísica e Ciências Atmosféricas, Rua do Matão 1226, 05508-900 São Paulo, Brazil email: [email protected]
Tatiana A. Michtchenko
Affiliation:
Insituto de Astronomia, Geofísica e Ciências Atmosféricas, Rua do Matão 1226, 05508-900 São Paulo, Brazil email: [email protected]
Cristian Beaugé
Affiliation:
Observatório Astronómico, Universidad Nacional de Córdoba, Laprida 854, (X5000BGR) Córdoba, Argentina
Octavio Miloni
Affiliation:
Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La Plata, Paseo del Bosque S/N B1900 FWA, La Plata, Argentina
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Abstract

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We investigate the motion of a two-planet coplanar system under the combined effects of mutual interaction and tidal dissipation. The secular behavior of the system is analyzed using two different approaches, restricting to the case of a more massive outer planet. First, we solve the exact equations of motion through the numerical simulation of the system evolution. We also compute the stationary solutions of the mean equations of motion based on a Hamiltonian formalism. An application to the real system CoRoT-7 is investigated.

Keywords

Celestial mechanics
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S276: The Astrophysics of Planetary Systems: Formation, Structure, and Dynamical Evolution , October 2010 , pp. 508 - 510
Copyright
Copyright © International Astronomical Union 2011

References

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