Oxidized or Reduced Early Atmospheres of Terrestrial Planets? Magma Ocean Atmosphere Control and the Importance of Metal-Magma Equilibration

Details Oxidized or Reduced Early Atmospheres of Terrestrial Planets? Magma Ocean Atmosphere Control and the Importance of Metal-Magma Equilibration Oxidized or Reduced Early Atmospheres of Terrestrial Planets? Magma Ocean Atmosphere Control and the Importance of Metal-Magma Equilibration

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1260h&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1260

Physics

Scientific paper

Early terrestrial atmospheres are influenced by interactions with magma
oceans, which could impose either oxidizing or reduced conditions. Key
variables include the depth of magma reaction with Fe, and the effect of
pressure on Fe3+/Fe2+ in magmas.

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