Ammonia-water volcanism on icy satellites - Phase relations at 1 atmosphere

Details Ammonia-water volcanism on icy satellites - Phase relations at 1 atmosphere Ammonia-water volcanism on icy satellites - Phase relations at 1 atmosphere

Dec 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992icar..100..556k&link_type=abstract

Icarus (ISSN 0019-1035), vol. 100, no. 2, p. 556-574.

Mathematics

Logic

69

Ammonia, Icy Satellites, Phase Transformations, Satellite Atmospheres, Water, Phase Diagrams, Volcanoes

Scientific paper

Ammonia-water-rich solutions have been rheologically implicated in the formation of thick viscous extrusions on Uranian and Neptunian satellites. Ammonia-rich liquids are not noted to be an inevitable product of partial melting in ammonia-bearing satellites. In addition to important rheological effects, the dissolved S and C compounds in ammonia-water and other aqueous fluids may control the colors and albedos of resurfaced icy satellites.

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