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High resolution observations of the 2.125-micron feature in Io's spectrum during 1975 and 1976High resolution observations of a weak absorption feature in the Io spectrum, obtained in 1975-1976 indicate that, if this feature is indicative of the presence of a new class of material, it may be the only diagnostic feature in Io's near-IR spectrum that can be distinguished by terrestrial telescopes. It appears unlikely that the absorber is a gas, or that gaseous CO2 contributes to the line shape.
Document ID
19920048524
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
doi:10.1016/0019-1035(92)90048-C
Authors
Larson, Harold P. (NASA Ames Research Center Moffett Field, CA, United States)
Timmermann, Ralf (NASA Ames Research Center Moffett Field, CA, United States)
Fink, Uwe (Arizona, University Tucson, United States)
Date Acquired
August 15, 2013
Publication Date
February 1, 1992
Publication Information
Publication: Icarus
Volume: 95
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Accession Number
92A31148
Funding Number(s)
CONTRACT_GRANT: NAGW-2406
CONTRACT_GRANT: NAG2-206
Distribution Limits
Public
Copyright
Other

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