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Identification of water ice on the Centaur 1997 CU26Spectra of the Centaur 1997 CU26 were obtained at the Keck Observatory on 27 October 1997 (universal time). The data show strong absorptions at 1.52 and 2.03 micrometers attributable to water ice on the surface of 1997 CU26. The reflectance spectrum of 1997 CU26 is matched by the spectrum of a mixture of low-temperature, particulate water ice and spectrally featureless but otherwise red-colored material. Water ice dominates the spectrum of 1997 CU26, whereas methane or methane-like hydrocarbons apparently dominate the spectrum of the Kuiper belt object 1993 SC, perhaps indicating different origins, thermal histories, or both for these two objects.
Document ID
20040172653
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Brown, R. H.
(Lunar and Planetary Lab and Steward Observatory, University of Arizona Tucson, AZ 85721, USA. 94035, United States)
Cruikshank, D. P.
Pendleton, Y.
Veeder, G. J.
Date Acquired
August 22, 2013
Publication Date
May 29, 1998
Publication Information
Publication: Science
Volume: 280
Issue: 5368
ISSN: 0036-8075
Subject Category
Lunar And Planetary Science And Exploration
Distribution Limits
Public
Copyright
Other
Keywords
NASA Discipline Exobiology
NASA Center ARC

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