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Igneous origin for the Na in the cloud of IoMixtures 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.
Document ID
19900051283
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Johnson, Mary L.
(California Inst. of Tech. Pasadena, CA, United States)
Burnett, D. S.
(California Institute of Technology Pasadena, United States)
Date Acquired
August 14, 2013
Publication Date
June 1, 1990
Publication Information
Publication: Geophysical Research Letters
Volume: 17
ISSN: 0094-8276
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0094-8276
Accession Number
90A38338
Funding Number(s)
CONTRACT_GRANT: NAGW-1741
Distribution Limits
Public
Copyright
Other

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