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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
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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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