Tidal Dissipation and Eccentricity Pumping: Implications for the Depth of the Secondary Eclipse of 55 Cnc e - Archive ouverte HAL
Communication Dans Un Congrès Année : 2014

Tidal Dissipation and Eccentricity Pumping: Implications for the Depth of the Secondary Eclipse of 55 Cnc e

Emeline Bolmont
Franck Selsis
  • Fonction : Auteur
Sean N. Raymond
F. Hersant
  • Fonction : Auteur
  • PersonId : 853119
A. S. Maurin
  • Fonction : Auteur
J. Pericaud
  • Fonction : Auteur

Résumé

We use the super-Earth 55 Cnc e (Fischer et al. 2008) as a case-study to address an observable effect of tidal heating. This transiting short-period planet belongs to a compact multiple system with massive planets. We investigate whether planet-planet interactions can force the eccentricity of this planet to a level that would affect the eclipse depth observed with Spitzer.

Dates et versions

hal-00944217 , version 1 (10-02-2014)

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Citer

Emeline Bolmont, Franck Selsis, Sean N. Raymond, J. Leconte, F. Hersant, et al.. Tidal Dissipation and Eccentricity Pumping: Implications for the Depth of the Secondary Eclipse of 55 Cnc e. Exploring the Formation and Evolution of Planetary Systems 2014, 2013, Victoria, British Columbia, Canada. pp.393-394, ⟨10.1017/S174392131300906X⟩. ⟨hal-00944217⟩
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