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Radiative equilibrium models of “hot Jupiters”

Published online by Cambridge University Press:  26 May 2016

Cédric Goukenleuque ,
Bruno Bézard  and
Emmanuel Lellouch
Cédric Goukenleuque
Affiliation:
NRC/Goddard Space Flight Center, Planetary Systems Branch, Greenbelt, MD 20770 USA
Bruno Bézard
Affiliation:
Observatoire de Paris-Meudon, 5 Place Jules Janssen, F-92195 Meudon, France
Emmanuel Lellouch
Affiliation:
Observatoire de Paris-Meudon, 5 Place Jules Janssen, F-92195 Meudon, France

Abstract

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We present an extension of our equilibrium model, initially applied to 51 Peg b (Goukenleuque et al. 2000), to other irradiated extrasolar planets with different orbital distances (up to 1 AU). The model yields the mean atmospheric thermal structure and predicts the reflected spectral flux as well as the thermal flux emerging from such planets, in the visible and in the infrared wavelength ranges.

Type
Part III: Structure and atmospheres of planets
Information
Symposium - International Astronomical Union , Volume 202: Planetary Systems in the Universe – Observation, Formation and Evolution , 2004 , pp. 277 - 279
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Goukenleuque, C., Bézard, B., Joguet, B., Lellouch, E., & Freedman, R. 2000, Icarus, 143, 308.CrossRefGoogle Scholar