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On the effect of X rays on the color of elemental sulfur - Implications for Jupiter's satellite IoAbsorption features arose at 0.42 and 0.52 microns when spectral reflectance measurements were conducted for elemental sulfur allotrope mixtures produced by the exposure of the cyclooctal S(8) allotrope of sulfur to X-rays; while these features due to the presence of short-chain molecules are stable at low temperatures, they fade upon warming of the sample. The hypothesis that X-rays in the Jovian environment would cause other allotropic forms of sulfur to revert to S(8) is contradicted by the fact that these features are not present in S(8) at the same temperature that had not been exposed to X-rays.
Document ID
19900049449
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Nelson, Robert M.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Smythe, William D.
(JPL Pasadena, CA, United States)
Hapke, Bruce W.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Cohen, Alvin J.
(Pittsburgh, University PA, United States)
Date Acquired
August 14, 2013
Publication Date
June 1, 1990
Publication Information
Publication: Icarus
Volume: 85
ISSN: 0019-1035
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0019-1035
Accession Number
90A36504
Distribution Limits
Public
Copyright
Other

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