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The Spectral Character of Giant Planets and Brown Dwarfs
A. Burrows, M. Marley, W. B. Hubbard +6
Since October of 1995, employing Doppler spectroscopy astronomers have discovered as many as 20 giant planets and brown dwarfs, including companions to Boo, 51 Peg, …
New Constraints on the Composition of Jupiter from Galileo Measurements and Interior Models
Tristan Guillot, Daniel Gautier, William B. Hubbard
Using the helium abundance measured by Galileo in the atmosphere of Jupiter and interior models reproducing the observed external gravitational field, we derive new constraints on…
Advances in the Theory of Extrasolar Giant Planets and Brown Dwarfs
A. Burrows, D. Sudarsky, C. Sharp +6
We have developed a new non-gray theory of the evolution, spectra, and colors of extrasolar giant planets (EGPs) and brown dwarfs that reveals their exotic nature and uniqueness. W…
A Non-Gray Theory of Extrasolar Giant Planets and Brown Dwarfs
A. Burrows, M. Marley, W. B. Hubbard +6
We present the results of a new series of non-gray calculations of the atmospheres, spectra, colors, and evolution of extrasolar giant planets (EGPs) and brown dwarfs for effective…
Extrasolar Giant Planet and Brown Dwarf Models
A. Burrows, W. B. Hubbard, J. I. Lunine +3
With the discovery of the companions of 51 Peg, 55 Cnc, Boo, And, 70 Vir, 47 UMa, and Gl229, evolutionary and spectral models of gas giants and/or brown dwarfs with…
Liquid metallic hydrogen and the structure of brown dwarfs and giant planets
W. B. Hubbard, T. Guillot, J. I. Lunine +4
Electron-degenerate, pressure-ionized hydrogen (usually referred to as metallic hydrogen) is the principal constituent of brown dwarfs, the long-sought objects which lie in the mas…