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High-resolution infrared spectroscopy of Io and possible surface materialsA comparison of new spectra of Io with laboratory-simulated frosts confirms that the dominant materials on Io are SO2 frost in conjunction with a spectrally neutral material presumed to be sulfur. While the 4-micron region spectra are largely explainable in these terms, attention is drawn to a shoulder in the spectrum at 4.04 microns that is suggestive of adsorbed SO2 gas; two shallow, unidentified bands are also noted at 3.85 and 3.91 microns. The isotopic ratios of oxygen and sulfur appear to be normal. The absence of distinct bands in the new spectra in the 5-micron region limits the abundance of sulfate and sulfite compounds.
Document ID
19890046417
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Howell, Robert R.
(Hawaii, University Honolulu, United States)
Nash, Douglas B.
(California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)
Geballe, Thomas R.
(Groningen, Rijksuniversiteit, Netherlands; Edinburgh, Royal Observatory, U.K. Infrared Telescope Unit, Hilo HI, United States)
Cruikshank, Dale P.
(NASA Ames Research Center Moffett Field, CA; Hawaii, University, Honolulu, United States)
Date Acquired
August 14, 2013
Publication Date
March 1, 1989
Publication Information
Publication: Icarus
Volume: 78
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Accession Number
89A33788
Funding Number(s)
CONTRACT_GRANT: NAGW-1276
Distribution Limits
Public
Copyright
Other

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