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The 2.5-5.0 micron spectra of Io - Evidence for H2S and H2O frozen in SO2The present analysis of IR spectra of Io in the 2.5-5.0 micron region with laboratory data on plausible surface ices gives attention to four unidentified features exhibiting spatial and temporal band strength variations; these fall close to the fundamental stretching modes in H2S and H2O, respectively. It is suggested that the 3.85- and 3.91-micron bands in the Io spectra can be accounted for by the absorption of the S-H stretching vibration in H2S clusters and isolated molecules in an SO2-dominated ice. The observations resemble the transmission spectra of SO2 ices that contain about 3 percent H2S and 0.1 percent H2O.
Document ID
19900035858
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Salama, F.
(NASA Ames Research Center Moffett Field, CA, United States)
Allamandola, L. J.
(NASA Ames Research Center Moffett Field, CA, United States)
Witteborn, F. C.
(NASA Ames Research Center Moffett Field, CA, United States)
Cruikshank, D. P.
(NASA Ames Research Center Moffett Field, CA, United States)
Sandford, S. A.
(NASA Ames Research Center Moffett Field, CA, United States)
Date Acquired
August 14, 2013
Publication Date
January 1, 1990
Publication Information
Publication: Icarus
Volume: 83
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Accession Number
90A22913
Distribution Limits
Public
Copyright
Other

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