A&A manuscript no. ASTRONOMY (will be inserted by hand later) AND Your thesaurus codes are: ASTROPHYSICS 08 Atmospheric Circulation and Tides of “51Pegb-like” Planets Adam P. Showman1 and Tristan Guillot2 1 University of Arizona, Department of Planetary Sciences and Lunar and Planetary Laboratory, Tucson, AZ 85721; show-
[email protected] 2 Observatoire de la Cˆote d’Azur, Laboratoire Cassini, CNRS UMR 6529, 06304 Nice Cedex 4, France;
[email protected] Submitted 23 March 2001; Accepted 18 January 2002 Abstract. We examine the properties of the atmo- the similar brown dwarfs, for which theoretical models spheres of extrasolar giant planets at orbital distances now reproduce the observations well, even in the case of smaller than 0.1 AU from their stars. We show that these low-temperature objects (Teff ∼ 1000K or less) (e.g. Mar- “51 Peg b-like” planets are rapidly synchronized by tidal ley et al. 1996; Allard et al. 1997; Liebert et al. 2000; interactions, but that small departures from synchronous Geballe et al. 2001; Schweitzer et al. 2001 to cite only a rotation can occur because of fluid-dynamical torques few). However, an important feature of extrasolar plan- within these planets. Previous radiative-transfer and evo- ets is their proximity to a star: The irradiation that they lution models of such planets assume a homogeneous at- endure can make their atmospheres significantly different mosphere. Nevertheless, we show using simple arguments than those of isolated brown dwarfs with the same ef- that, at the photosphere, the day-night temperature dif- fective temperature. This has been shown to profoundly ference and characteristic wind speeds may reach ∼ 500K alter the atmospheric vertical temperature profile (Sea- and ∼ 2kmsec−1, respectively.