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Sulfur volcanoes on IoWidespread volcanism on Jupiter's satellite Io, if it occurred over the age of the solar system, would quickly reduce the inventory of most common volatiles needed to drive such volcanism. One exception is the volatile element sulfur. It is therefore postulated that sulfur is the driving volatile for Ionian volcanism. Its presence is consistent with a carbonaceous-chondrite-like bulk composition for the original material that formed Io 4.5 billion years ago. The ubiquity of sulfur on Io today demonstrates the importance of this element in the processes that formed its surface.
Document ID
19790059796
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Consolmagno, G. J.
(Harvard-Smithsonian Center for Astrophysics Cambridge, Mass., United States)
Date Acquired
August 9, 2013
Publication Date
July 27, 1979
Publication Information
Publication: Science
Volume: 205
Subject Category
Lunar And Planetary Exploration
Accession Number
79A43809
Funding Number(s)
CONTRACT_GRANT: NGR-22-007-269
Distribution Limits
Public
Copyright
Other

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