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ReportsExposed Water Ice Deposits on the Surface of Comet 9P/Tempel 1
We report the direct detection of solid water ice deposits exposed on the surface of comet 9P/Tempel 1, as observed by the Deep Impact mission. Three anomalously colored areas are shown to include water ice on the basis of their near-infrared spectra, which include diagnostic water ice absorptions at wavelengths of 1.5 and 2.0 micrometers. These absorptions are well modeled as a mixture of nearby non-ice regions and 3 to 6% water ice particles 10 to 50 micrometers in diameter. These particle sizes are larger than those ejected during the impact experiment, which suggests that the surface deposits are loose aggregates. The total area of exposed water ice is substantially less than that required to support the observed ambient outgassing from the comet, which likely has additional source regions below the surface.
1 Science Applications International Corporation (SAIC), Chantilly, VA 20151, USA.
2 University of Maryland, College Park, MD 20742, USA. 3 Belton Space Exploration Initiatives, Tucson, AZ 85716, USA. 4 Delamere Support Services, Boulder, CO 80301, USA. 5 Max Planck Institute for Solar System Research, Katlenburg-Lindau D37191, Germany. 6 Jet Propulsion Laboratory, Pasadena, CA 91109, USA. 7 University of Hawaii, Honolulu, HI 96822, USA. 8 University of Arizona, Tucson, AZ 85721, USA. 9 Brown University, Providence, RI 02412, USA. 10 Cornell University, Ithaca, NY 14853, USA. 11 Space Telescope Science Institute, Baltimore, MD 21218, USA. 12 Ball Aerospace & Technology Corporation, Boulder, CO 80301, USA. 13 Sigma Scientific, Greenbelt, MD 20771, USA. 14 Applied Physics Laboratory, Johns Hopkins University, Laurel, MD 20723, USA. * To whom correspondence should be addressed. E-mail: sunshinej{at}saic.com
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Science. ISSN 0036-8075 (print), 1095-9203 (online)