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Atmospheres of Extra-solar Planets and Brown Dwarfs
Published online by Cambridge University Press: 19 September 2017
Abstract
Brown dwarfs have masses intermediate to stars and planets, but their atmospheres can span planetary plasma conditions as they cool over time. They are more directly observable than the currently known extra-solar planets. In this paper, we provide a brief summary of the atmospheric properties of brown dwarfs, and apply this knowledge to predict the thermal and spectral properties of extra-solar planets.
- Type
- Extrasolar Planets
- Information
- Symposium - International Astronomical Union , Volume 213: Bioastronomy 2002: Life Among the stars , 2004 , pp. 119 - 122
- Copyright
- Copyright © Astronomical Society of the Pacific 2004