Bruce Fegley

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We use thermochemical equilibrium and kinetic calculations to model sulfur and phosphorus chemistry in the atmospheres of giant planets, brown dwarfs, low-mass stars, and extrasolar giant planets (EGPs). The chemical behavior of individual Sand P-bearing gases and condensates is determined as a function of pressure, temperature, and metallicity. Our results(More)
Thermochemical equilibrium calculations of gas abundances and condensation cloud formation are used to model the atmospheric chemistry of Gliese 229B. The calculations , which are analogous to our prior modeling of atmospheric chemistry of the Jo-vian planets in our solar system, predict the abundances of gases which are potentially observable by(More)
  • Citation Lupu, Kevin Zahnle, Mark S Marley, Laura Schaefer, Bruce Fegley, Caroline Morley +5 others
  • 2014
Article is made available in accordance with the publisher's policy and may be subject to US copyright law. Please refer to the publisher's site for terms of use. The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. ABSTRACT It is now understood that the accretion of terrestrial planets(More)
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