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Hyperion's Dark Material: Rotational VariationWe present two new dark material spectra of Hyperion compared with previously published dark material spectra of Hyperion and Iapetus. A 0.67-micron absorption feature is seen in one of the two new spectra. This suggests possible mineralogical differences across the surface of this Saturnian satellite. Additional information is contained in the original extended abstract.
Document ID
20020046197
Acquisition Source
Headquarters
Document Type
Conference Paper
Authors
Jarvis, K. S.
(Lockheed Martin Corp. Houston, TX United States)
Vilas, F.
(NASA Headquarters Washington, DC United States)
Buratti, B. J.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Hicks, M. D.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA United States)
Gaffey, M. J.
(North Dakota Univ. Grand Forks, ND United States)
Date Acquired
August 20, 2013
Publication Date
April 1, 2002
Publication Information
Publication: Lunar and Planetary Science XXXIII
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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