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Io - Longtudinal distribution of sulfur dioxide frostA longitudinal variation in the distribution of SO2 frost on Io is examined. Twenty spectra of Io (0.26 to 0.33 micrometer) are presented and a strong ultraviolet absorption is found shortward of 0.33 micrometer. The abundance of frost is greatest at orbital longitudes 72 to 137 degrees. Longitudes 250 to 323 degrees are least abundant in SO2. Comparisons are made with a Voyager color relief map, which suggest that SO2 frost is in greatest concentration in the white areas of Io and other sulfurous materials are in greatest concentration in the red areas.
Document ID
19810027841
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Nelson, R. M.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Lane, A. L.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Matson, D. L.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Fanale, F. P.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Nash, D. B.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Johnson, T. V.
(California Institute of Technology, Jet Propulsion Laboratory, Pasadena Calif., United States)
Date Acquired
August 11, 2013
Publication Date
November 14, 1980
Publication Information
Publication: Science
Volume: 210
Subject Category
Lunar And Planetary Exploration
Accession Number
81A12245
Funding Number(s)
CONTRACT_GRANT: NAS7-100
Distribution Limits
Public
Copyright
Other

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