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Spectrophotometry of Io - Preliminary Voyager 1 resultsMultispectral images of Io acquired with the Voyager 1 narrow-angle camera agree with earth-based spectrophotometry to better than 10%. Although the surface materials have general spectral properties similar to various allotropes of sulfur, their ultraviolet (UV) reflectances are much higher. It is likely that varying amounts of SO2 frost mixed with or absorbed on sulfur-rich materials raises the UV reflectance. The possible association with large amounts of SO2 with low temperature forms of sulfur in the white patches on Io is consistent with Io surface models in which SO2 and S exist in thermally stable stratified zones.
Document ID
19810030019
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Soderblom, L.
(U.S. Geological Survey, Branch of Astrogeologic Studies, Flagstaff Ariz., United States)
Johnson, T.
(Geological Survey Flagstaff, AZ, United States)
Kupferman, P.
(Geological Survey Flagstaff, AZ, United States)
Pieri, D.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Morrison, D.
(Hawaii, University Honolulu, Hawaii, United States)
Danielson, E.
(California Institute of Technology Pasadena, Calif., United States)
Smith, B.
(Arizona, University Tucson, Ariz., United States)
Veverka, J.
(Geological Survey Flagstaff, AZ, United States)
Sagan, C.
(Cornell University Ithaca, N.Y., United States)
Cook, A.
(Harvard-Smithsonian Center for Astrophysics Cambridge, Mass., United States)
Date Acquired
August 11, 2013
Publication Date
November 1, 1980
Publication Information
Publication: Geophysical Research Letters
Volume: 7
Subject Category
Lunar And Planetary Exploration
Accession Number
81A14423
Funding Number(s)
PROJECT: PROJECT VOYAGER
Distribution Limits
Public
Copyright
Other

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