High pressure cosmochemistry of major planetary interiors: Laboratory studies of the water-rich region of the system ammonia-water

Details High pressure cosmochemistry of major planetary interiors: Laboratory studies of the water-rich region of the system ammonia-water High pressure cosmochemistry of major planetary interiors: Laboratory studies of the water-rich region of the system ammonia-water

May 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pggp.rept..133.&link_type=abstract

In NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1986 p 133-135 (SEE N87-23341 16-91)

Physics

Geophysics

Planets, Geology, Geophysics, Solar System, Evolution, Laser Methods, Formation, Interior, Petrology, Geochemistry, Pressure, Geomagnetism, Troilite, Laboratory Studies, Water, Ammonia, Experiments, Core, Heating, Regolith, Temperature, Gravity Properties, Analysis, Polarity, Origin, Symmetry, Magnetic Fields, Magnetic Properties, Mars, Planetesimals, Nebula, Meteorites, Chondrules, Accretion, Adsorption, Mantle, Boundaries, Magnetization, Moon, Convection, Terrestrial Planets, Chemistry, Crust, Calcium Car

Scientific paper

Several studies relative to high pressure cosmochemistry of major planetary interiors are summarized. The behavior of gas-ice mixtures at very high pressures, studies of the phase diagram of (NH3)x (H2O)1-x at pressures to 5GPa and temperatures from 240 to 370 K, single crystal growth of ammonia dihydrate at room temperature in order to determine their structures by x-ray diffraction, spectroscopy of chemical reactions during shock compression in order to evaluate how the reactions affect the interpretation of equation of state data obtained by shock methods, and temperature and x-ray diffraction measurements made on resistively heated wire in diamond anvil cells in order to obtain phase and structural data relevant to the interiors of terrestrial planets are among the studies discussed.

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