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Spectrum and atmosphere models of irradiated transiting extrasolar giant planets

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 نشر من قبل Ivan Hubeny
 تاريخ النشر 2008
  مجال البحث فيزياء
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We show that a consistent fit to observed secondary eclipse data for several strongly irradiated transiting planets demands a temperature inversion (stratosphere) at altitude. Such a thermal inversion significantly influences the planet/star contrast ratios at the secondary eclipse,their wavelength dependences, and, importantly, the day-night flux contrast during a planetary orbit. The presence of the thermal inversion/stratosphere seems to roughly correlate with the stellar flux at the planet. Such temperature



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