Identification of Absorption Features in an Extrasolar Planet Atmosphere

Published 2007 May 11 © 2007. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation T. Barman 2007 ApJ 661 L191 DOI 10.1086/518736

1538-4357/661/2/L191

Abstract

Water absorption is identified in the atmosphere of HD 209458b by comparing models for the planet's transmitted spectrum to recent, multiwavelength, eclipse-depth measurements (from 0.3 to 1 μm) published by Knutson et al. A cloud-free model that includes solar abundances, rainout of condensates, and photoionization of sodium and potassium is in good agreement with the entire set of eclipse-depth measurements from the ultraviolet to near-infrared. Constraints are placed on condensate removal by gravitational settling, the bulk metallicity, and the redistribution of absorbed stellar flux. Comparisons are also made to the Charbonneau et al. sodium measurements.

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10.1086/518736