A Time-Dependent Radiative Model for the Atmosphere of the Eccentric Exoplanets

Details A Time-Dependent Radiative Model for the Atmosphere of the Eccentric Exoplanets A Time-Dependent Radiative Model for the Atmosphere of the Eccentric Exoplanets

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010apj...712..218i&link_type=abstract

The Astrophysical Journal, Volume 712, Issue 1, pp. 218-225 (2010).

Astronomy and Astrophysics

Astronomy

8

Planets And Satellites: Individual: Hd 80606B Hd 17156B, Radiative Transfer

Scientific paper

We present a time-dependent radiative model for the atmosphere of extrasolar planets that takes into account the eccentricity of their orbit. In addition to the modulation of stellar irradiation by the varying planet-star distance, the pseudo-synchronous rotation of the planets may play a significant role. We include both of these time-dependent effects when modeling the planetary thermal structure. We investigate the thermal structure and spectral characteristics for time-dependent stellar heating for two highly eccentric planets. Finally, we discuss observational aspects for those planets suitable for Spitzer measurements and investigate the role of the rotation rate.

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