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Spitzer Observations of the Thermal Emission from WASP-43b

ASTROPHYSICAL JOURNAL, no. 2 (2014)

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eclipsesplanets and satellites: atmospheresplanets and satellites: individual (WASP-43b)techniques: photometric

Abstract

WASP-43b is one of the closest-orbiting hot Jupiters, with a semimajor axis of a = 0.01526 +/- 0.00018 AU and a period of only 0.81 days. However, it orbits one of the coolest stars with a hot Jupiter (T-* = 4520 +/- 120 K), giving the planet a modest equilibrium temperature of T-eq = 1440 +/- 40 K, assuming zero Bond albedo and uniform p...More

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