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Silicate volcanism on IoThis 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.
Document ID
19860047239
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Carr, M. H.
(U.S. Geological Survey Menlo Park, CA, United States)
Date Acquired
August 12, 2013
Publication Date
March 10, 1986
Publication Information
Publication: Journal of Geophysical Research
Volume: 91
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
86A31977
Funding Number(s)
CONTRACT_GRANT: NASA ORDER W-15788
Distribution Limits
Public
Copyright
Other

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