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The detection of a new strong band near 3590 cm(exp -1) (2.79 microns) in the spectrum of IoA strong absorption band at 3590 +/- 20 cm(exp -1) (2.790 +/- 0.015 microns) has been discovered in the spectrum of Io using the Kuiper Airborne Observatory (KAO). The 2 nu(sub 1) + nu(sub 3) combination mode of solid SO2 falls at this position. Since SO2 is abundant on Io it must contribute to the new band. However, a band due to H2O was also predicted near this frequency in Io's spectrum based on laboratory experiments of H2O:SO2 mixed Io ice analogs which were used to assign the two weak, variable features at 3370 and 3170 cm(exp -1) (2.97 and 3.15 microns) to trace amounts of H2O frozen in solid SO2 on Io. The new band probably originates from both SO2 and H2O. Unfortunately, the spectral resolution of the data is insufficient to settle the issue of whether or not there are two resolvable components.
Document ID
19960003658
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Salama, F.
(NASA Ames Research Center Moffett Field, CA, United States)
Allamandola, L. J.
(NASA Ames Research Center Moffett Field, CA, United States)
Sandford, S. A.
(NASA Ames Research Center Moffett Field, CA, United States)
Bregman, Jesse D.
(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)
Date Acquired
September 6, 2013
Publication Date
January 1, 1995
Publication Information
Publication: Astronomical Society of the Pacific, Airborne Astronomy Symposium on the Galactic Ecosystem: From Gas to Stars to Dust, Volume 73
Subject Category
Astronomy
Accession Number
96N13668
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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