The Changing Face of the Extrasolar Giant Planet HD 209458b

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Published 2003 March 20 © 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation James Y-K. Cho et al 2003 ApJ 587 L117 DOI 10.1086/375016

1538-4357/587/2/L117

Abstract

High-resolution atmospheric flow simulations of the tidally locked extrasolar giant planet HD 209458b show large-scale spatio-temporal variability. This is in contrast to the simple, permanent day/night (i.e., hot/cold) picture. The planet's global circulation is characterized by a polar vortex in motion around each pole and a banded structure corresponding to approximately three broad zonal (east-west) jets. For very strong jets, the circulation-induced temperature difference between moving hot and cold regions can reach up to ~1000 K, suggesting that atmospheric variability could be observed in the planet's spectral and photometric signatures.

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10.1086/375016