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Disequilibrium Chemistry in a Brown Dwarf's Atmosphere: Carbon Monoxide in Gliese 229B

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Published 1999 June 4 © 1999. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation Caitlin A. Griffith and Roger V. Yelle 1999 ApJ 519 L85 DOI 10.1086/312103

1538-4357/519/1/L85

Abstract

The distribution of CO in Gliese 229B's atmosphere reveals how disequilibrium processes establish the atmospheric composition. The CO abundance derived from its spectral signature exceeds the equilibrium value by several orders of magnitude. Our investigation of the source for CO considers disequilibrium mechanisms common to planetary atmospheres and concludes that the CO abundance is sensitive to atmospheric dynamics. Convection is not required to explain the observed abundance; instead, the vertical transport rate at ~6 bars may be similar to that in planetary stratospheres.

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10.1086/312103