Solubility of molecular hydrogen in silicate melts and consequences for volatile evolution of terrestrial planets

Earth and Planetary Science Letters

Volumn 345-348, Issue , 2012, Pages 38-48

  Hirschmann, M M ^a   Withers, A C ^a   Ardia, P ^a   Foley, N T ^a  

^a University of Minnesota   (United States)

Author keywords

H in core deep melting; Hydrogen; Lunar water; Nebular atmosphere

Indexed keywords

BASALTIC LIQUIDS; CORE FORMATION; EARLY EARTH; FTIR; HIGH PRESSURE; HYDROGEN FUGACITY; HYDROUS MELTS; LOW PRESSURES; MAGMA OCEAN; MAGMATIC VOLATILES; MOLECULAR HYDROGEN; PARTIAL MELT; PARTIAL MELTING; PARTIAL MOLAR VOLUME; REDOX EVOLUTION; SILICATE MELTS; TERRESTRIAL PLANETS; VOLATILE EVOLUTION;

BASALT; EXTRAPOLATION; HYDROGEN; MELTING; PLANETS; SILICATES;

SOLUBILITY;

CONCENTRATION (COMPOSITION); HIGH PRESSURE; HYDROGEN; LOW PRESSURE; LUNAR MANTLE; MARE BASALT; OXIDATION; PARTIAL MELTING; SILICATE MELT; SOLUBILITY; VOLATILE ELEMENT;

EID: 84864067466     PISSN: 0012821X     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.epsl.2012.06.031     Document Type: Article

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