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A time-dependent radiative model for the atmosphere of the eccentric transiting planets

Published online by Cambridge University Press:  01 May 2008

Nicolas Iro  and
Drake Deming
Nicolas Iro
Affiliation:
NASA GSFC Planetary Systems Laboratory code 693.0, Greenbelt, MD 20770, USA email: nicolas.iro@nasa.gov; leo.d.deming@nasa.gov LESIA Observatoire de Paris-Meudon, 92190 Meudon Cedex, FRANCE
Drake Deming
Affiliation:
NASA GSFC Planetary Systems Laboratory code 693.0, Greenbelt, MD 20770, USA email: nicolas.iro@nasa.gov; leo.d.deming@nasa.gov
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Abstract

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We present a time-dependent radiative model for the atmosphere of the transiting planets that takes into account the eccentricity of their orbit. We investigate the temporal temperature and flux variations due to the planet-star distance variability. We will also discuss observational aspects with Spitzer measurements.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S253: Transiting Planets , May 2008 , pp. 516 - 519
Copyright
Copyright © International Astronomical Union 2009

References

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