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Tidal evolution in multiple planet systems: application to Kepler-62 and Kepler-186

Emeline Bolmont 1, 2, 3, 4, 5 Sean N. Raymond 1, 2, 3, 4, 5 Leconte Jérémy, Correia Alexandre, Quintana Elisa,
1 ECLIPSE 2014
L3AB - Laboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux, OASU - Observatoire aquitain des sciences de l'univers, LAB - Laboratoire d'Astrophysique de Bordeaux [Pessac], Université Sciences et Technologies - Bordeaux 1
Abstract : A large number of observed exoplanets are part of multiple planet systems. Most of these systems are sufficiently close-in to be tidally evolving. In such systems, there is a competition between the excitation caused by planet-planet interactions and tidal damping. Using as an example two multiple planet systems, which host planets in the surface liquid water habitable zone (HZ): Kepler-62 and Kepler-186, we show the importance and effect of both planetary and stellar tides on the dynamical evolution of planets and on the climate of the HZ planets.
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Submitted on : Thursday, October 30, 2014 - 10:31:50 AM
Last modification on : Friday, November 29, 2019 - 3:28:03 PM

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Emeline Bolmont, Sean N. Raymond, Leconte Jérémy,, Correia Alexandre,, Quintana Elisa,. Tidal evolution in multiple planet systems: application to Kepler-62 and Kepler-186. Proceedings IAU Symposium No. 310: Complex Planetary Systems 07-11 July 2014, Namur, Belgium, 2014, Namur, Belgium. pp.7428. ⟨hal-01078753⟩



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