NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Laboratory studies of the newly discovered infrared band at 4705.2/cm (2.1253 microns) in the spectrum of Io - The tentative identification of CO2The present evaluation of results from over 120 laboratory experiments relevant to the Trafton et al. (1991) discovery of a 2.1253-micron line in the spectrum of Io demonstrates that this band is produced by neither overtones nor combinations of the fundamental bands of molecules already noted on Io. Since the band's frequency is close to the first overtone of the nu(3) asymmetric stretching mode of CO2, attention is given this molecule's behavior under Io conditions. While pure solid CO2, and CO2 intimately mixed in a matrix of solid SO2 and H2S, generate bands of similar widths, these fall at frequencies lower than the Io band. Attention is given to the possible identification of the Io band with CO2 multimers of 'clusters' on Io.
Document ID
19910052748
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Sandford, Scott A.
(NASA Ames Research Center Moffett Field, CA, United States)
Salama, Farid
(NASA Ames Research Center Moffett Field, CA, United States)
Allamandola, Louis J.
(NASA Ames Research Center Moffett Field, CA, United States)
Trafton, Larry M.
(NASA Ames Research Center Moffett Field, CA, United States)
Lester, Dan F.
(McDonald Observatory; Texas, University Austin, United States)
Date Acquired
August 15, 2013
Publication Date
May 1, 1991
Publication Information
Publication: Icarus
Volume: 91
ISSN: 0019-1035
Subject Category
Astrophysics
Accession Number
91A37371
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available