Igneous origin for the NA in the cloud of Io

Details Igneous origin for the NA in the cloud of Io Igneous origin for the NA in the cloud of Io

Jun 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990georl..17..981j&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 17, June 1990, p. 981-984.

Physics

11

Igneous Rocks, Io, Jupiter Atmosphere, Satellite Surfaces, Silica Glass, Sodium Compounds, Chemical Reactions, Mass Distribution, Planetary Magnetospheres, Jupiter, Satellites, Io, Sodium, Clouds, Origin, Formation, Surface, Laboratory Studies, Experiments, Sputtering, Simulations, Sulfur, Sem, Silicates, Electron Microscopy, Photomicrographs, Sulfides

Scientific paper

Mixtures of sulfur and Na-bearing silicates were heated in evacuated silica glass capsules to temperatures between 600 C and 950 C. At or above 850 C, Na-silicate glass reacts with elemental S to form a (Na, K) sulfide. Mobilization of this phase may account for the presence of Na and K on the surface of Io, and hence in the material sputtered onto the Jovian magnetosphere.

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