Modeling the Formation of Clouds in Brown Dwarf Atmospheres

Details Modeling the Formation of Clouds in Brown Dwarf Atmospheres Modeling the Formation of Clouds in Brown Dwarf Atmospheres

2002-05-13

arxiv.org/abs/astro-ph/0205192v3

Astrophys.J. 586 (2003) 1320-1337; Erratum-ibid. 595 (2003) 573

Astronomy and Astrophysics

Astrophysics

25 pages; 8 figures. We have added considerable detail describing the physics of the cloud model. We have also added discussio

Scientific paper

10.1086/377199

Because the opacity of clouds in substellar mass object (SMO) atmospheres depends on the composition and distribution of particle sizes within the cloud, a credible cloud model is essential for accurately modeling SMO spectra and colors. We present a one--dimensional model of cloud particle formation and subsequent growth based on a consideration of basic cloud microphysics. We apply this microphysical cloud model to a set of synthetic brown dwarf atmospheres spanning a broad range of surface gravities and effective temperatures (g_surf = 1.78 * 10^3 -- 3 * 10^5 cm/s^2 and T_eff = 600 -- 1600 K) to obtain plausible particle sizes for several abundant species (Fe, Mg2SiO4, and Ca2Al2SiO7). At the base of the clouds, where the particles are largest, the particle sizes thus computed range from ~5 microns to over 300 microns in radius over the full range of atmospheric conditions considered. We show that average particle sizes decrease significantly with increasing brown dwarf surface gravity. We also find that brown dwarfs with higher effective temperatures have characteristically larger cloud particles than those with lower effective temperatures. We therefore conclude that it is unrealistic when modeling SMO spectra to apply a single particle size distribution to the entire class of objects.

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