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Originally published in Science Express on 4 April 2002
Science 10 May 2002:
Vol. 296. no. 5570, pp. 1087 - 1091
DOI: 10.1126/science.1069527

Research Articles

Observations of Comet 19P/Borrelly by the Miniature Integrated Camera and Spectrometer Aboard Deep Space 1 

L. A. Soderblom,1* T. L. Becker,1 G. Bennett,1 D. C. Boice,2 D. T. Britt,3 R. H. Brown,4 B. J. Buratti,5 C. Isbell,1 B. Giese,6 T. Hare,1 M. D. Hicks,5 E. Howington-Kraus,1 R. L. Kirk,1 M. Lee,5 R. M. Nelson,5 J. Oberst,6 T. C. Owen,7 M. D. Rayman,5 B. R. Sandel,4 S. A. Stern,8 N. Thomas,9 R. V. Yelle4

The nucleus of the Jupiter-family comet 19P/Borrelly was closely observed by the Miniature Integrated Camera and Spectrometer aboard the Deep Space 1 spacecraft on 22 September 2001. The 8-kilometer-long body is highly variegated on a scale of 200 meters, exhibiting large albedo variations (0.01 to 0.03) and complex geologic relationships. Short-wavelength infrared spectra (1.3 to 2.6 micrometers) show a slope toward the red and a hot, dry surface (<=345 kelvin, with no trace of water ice or hydrated minerals), consistent with ~10% or less of the surface actively sublimating. Borrelly's coma exhibits two types of dust features: fans and highly collimated jets. At encounter, the near-nucleus coma was dominated by a prominent dust jet that resolved into at least three smaller jets emanating from a broad basin in the middle of the nucleus. Because the major dust jet remained fixed in orientation, it is evidently aligned near the rotation axis of the nucleus.

1 United States Geological Survey, 2255 North Gemini Drive, Flagstaff, AZ 86001, USA.
2 Southwest Research Institute, 6220 Culebra Road, San Antonio, TX 78238, USA.
3 Department of Geological Sciences, University of Tennessee, 306 Geological Sciences Building, Knoxville, TN 37996, USA.
4 Department of Planetary Science, Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ 85721, USA.
5 Jet Propulsion Laboratory (JPL), California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109, USA.
6 DLR Institute of Space Sensor Technology and Planetary Exploration, Rutherfordstrasse, 2D-12489 Berlin, Germany.
7 Institute for Astronomy, University of Hawaii, 2680 Woodlawn Drive, Honolulu, HI 96822, USA.
8 Department of Space Studies, Southwest Research Institute, 1050 Walnut Street No. 426, Boulder, CO 80302, USA.
9 Max-Planck-Institut für Aeronomie, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany.
*   To whom correspondence should be addressed. E-mail: lsoderblom{at}usgs.gov


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THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
The Mass Disruption of Oort Cloud Comets.
H. F. Levison, A. Morbidelli, L. Dones, R. Jedicke, P. A. Wiegert, and W. F. Bottke Jr. (2002)
Science 296, 2212-2215
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