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A Nongray Theory of Extrasolar Giant Planets and Brown Dwarfs

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Burrows, A., Marley, M., Hubbard, W. B., Lunine, J. I., Guillot, T., Saumon, D., Freedman, R., Sudarsky, D., Sharp, C.·1997·The Astrophysical Journal

Abstract

We present the results of a new series of nongray calculations of the atmospheres, spectra, colors, and evolution of extrasolar giant planets (EGPs) and brown dwarfs for effective temperatures below 1300 K. This theory encompasses most of the mass/age parameter space occupied by substellar objects and is the first spectral study down to 100 K. These calculations are in aid of the multitude of searches being conducted or planned around the world for giant planets and brown dwarfs and reveal the exotic nature of the class. Generically, absorption by H 2 at longer wavelengths and H 2 O opacity windows at shorter wavelengths conspire to redistribute flux blueward. Below 1200 K, methane is the dominant carbon bearing molecule and is a universal diagnostic feature of EGP and brown dwarf spectra. We find that the primary bands in which to search are Z (~1.05 μm), J (~1.2 μm), H (~1.6 μm), K (~2.2 μm), M (~5 μm), and N (~10 μm), that enhancements of the emergent flux over blackbody values, in particular in the near infrared, can be by many orders of magnitude, and that the infrared colors of EGPs and brown dwarfs are much bluer than previously believed. In particular, relative to J and H , the K band flux is reduced by CH 4 and H 2 absorption. Furthermore, we conclude that for T eff 's below 1200 K most or all true metals may be sequestered below the photosphere, that an interior radiative zone is a generic feature of substellar objects, and that clouds of H 2 O and NH 3 are formed for T eff 's below ~400 and ~200 K, respectively. This study is done for solar-metallicity objects in isolation and does not include the effects of stellar insulation. Nevertheless, it is a comprehensive attempt to bridge the gap between the planetary and stellar realms and to develop a nongray theory of objects from 0.3 M J ("Saturn") to 70 M J (~0.07 M ☉ ). We find that the detection ranges for brown dwarf/EGP discovery of both ground- and space-based telescopes are larger than previously estimated.

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Metadata

Authors
Burrows, A., Marley, M., Hubbard, W. B., Lunine, J. I., Guillot, T., Saumon, D., Freedman, R., Sudarsky, D., & Sharp, C.
Venue
The Astrophysical Journal
Published
1997-12-20
Volume
491
Issue
2
Pages
856-875
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W1985663566
Cited by
1,390
References
4
FWCI
39.15
Type
journal article
Language
en
Open access
bronze

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CoChat. (2026). Citation check: A Nongray Theory of Extrasolar Giant Planets and Brown Dwarfs. https://app.cochat.ai/papers/10.1086/305002
The paper
Burrows, A., Marley, M., Hubbard, W. B., Lunine, J. I., Guillot, T., Saumon, D., Freedman, R., Sudarsky, D., & Sharp, C. (1997). A Nongray Theory of Extrasolar Giant Planets and Brown Dwarfs. The Astrophysical Journal. https://doi.org/10.1086/305002

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