High pressure cosmochemistry applied to major planetary interiors: Experimental studies

Details High pressure cosmochemistry applied to major planetary interiors: Experimental studies High pressure cosmochemistry applied to major planetary interiors: Experimental studies

May 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983stin...8324451n&link_type=abstract

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Computer Science

Cosmochemistry, High Pressure, Ice, Phase Diagrams, Planetary Composition, Adiabatic Equations, Compressible Fluids, Infrared Spectra, Vibrational Spectra, X Ray Diffraction

Scientific paper

The infrared spectra of H2O ice VII and D2O ice VII were studied and techniques were developed for measuring adiabats of phases of NH3-H2O to 5 GPa. A mixing system for pressurized fluids was constructed in which liquid solutions of definite compositions can be prepared and loaded reliably into diamond cells in a project which seeks to determine the properties and boundaries of several high pressure phases of the H2-He-H2O-NH3-CH4 system. These data are needed to constrain theoretical models of the interiors of the major planets.

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