Experimental study of the NaCl-H2O system up to 28 GPa: Implications for ice-rich planetary bodies

Physics of the Earth and Planetary Interiors

Volumn 155, Issue 1-2, 2006, Pages 152-162

  Frank, Mark R ^a   Runge, Claire E ^b,e   Scott, Henry P ^c   Maglio, Steven J ^a   Olson, Jessica ^a   Prakapenka, Vitali B ^d   Shen, Guoyin ^d,f  

^a NORTHERN ILLINOIS UNIVERSITY   (United States)

^b The College of William and Mary   (United States)

^c INDIANA UNIVERSITY SOUTH BEND   (United States)

^d UNIVERSITY OF CHICAGO   (United States)

^e PRINCETON UNIVERSITY   (United States)

^f ARGONNE NATIONAL LABORATORY   (United States)

Author keywords

High pressure; Icy satellites; Impurities; NaCl H2O; Subsurface oceans

Indexed keywords

HIGH PRESSURE EFFECTS; HIGH TEMPERATURE EFFECTS; ICE; RAMAN SPECTROSCOPY; SOLAR SYSTEM; STRUCTURAL GEOLOGY; SYNCHROTRON RADIATION; THERMODYNAMIC PROPERTIES;

ICE-RICH PLANETARY BODIES; ICY SATELLITES; SUBSURFACE OCEANS;

PLANETS;

HIGH PRESSURE; PLANETARY EVOLUTION; SODIUM CHLORIDE;

EID: 33644889642     PISSN: 00319201     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.pepi.2005.12.001     Document Type: Article

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