CHEMISTRY OF SILICATE ATMOSPHERES OF EVAPORATING SUPER-EARTHS

@article{Schaefer2009CHEMISTRYOS,
  title={CHEMISTRY OF SILICATE ATMOSPHERES OF EVAPORATING SUPER-EARTHS},
  author={Laura Schaefer and Bruce Fegley},
  journal={The Astrophysical Journal},
  year={2009},
  volume={703},
  pages={L113 - L117}
}
  • L. Schaefer, B. Fegley
  • Published 5 June 2009
  • Geology, Physics, Environmental Science
  • The Astrophysical Journal
We model the formation of silicate atmospheres on hot volatile-free super-Earths. Our calculations assume that all volatile elements such as H, C, N, S, and Cl have been lost from the planet. We find that the atmospheres are composed primarily of Na, O2, O, and SiO gas, in order of decreasing abundance. The atmospheric composition may be altered by fractional vaporization, cloud condensation, photoionization, and reaction with any residual volatile elements remaining in the atmosphere. Cloud… 

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