Silicate volcanism on Io

Details Silicate volcanism on Io Silicate volcanism on Io

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986jgr....91.3521c&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 91, March 10, 1986, p. 3521-3532.

Physics

69

Io, Planetary Geology, Satellite Surfaces, Silicates, Volcanology, Anomalous Temperature Zones, Basalt, Lithosphere, Magma, Sulfur, Surface Temperature, Jupiter, Satellites, Io, Silicate, Volcanism, Tides, Lithosphere, Loki, Thickness, Energy, Differentiation, Temperature, Depth, Basalt, Melting, Deformation, Transport, Magma, Resurfacing, Surface, Simulations, Plumes, Eruptions, Emissions, Hot Spots, Comparisons, Volcanoes, Volatiles, Reflectivity, Plasma Torus

Scientific paper

This paper is mainly concerned with the nature of volcanic eruptions on Io, taking into account questions regarding the presence of silicates or sulfur as principal component. Attention is given to the generation of silicate magma, the viscous dissipation in the melt zone, thermal anomalies at eruption sites, and Ionian volcanism. According to the information available about Io, it appears that its volcanism and hence its surface materials are dominantly silicic. Several percent of volatile materials such as sulfur, but also including sodium- and potassium-rich materials, may also be present. The volatile materials at the surface are continually vaporized and melted as a result of the high rates of silicate volcanism.

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