Jump to: Page Content, Section Navigation, Site Navigation, Site Search, Account Information, or Site Tools.
|
|
Research ArticlesSurface of Young Jupiter Family Comet 81P/Wild 2: View from the Stardust Spacecraft
Images taken by the Stardust mission during its flyby of 81P/Wild 2 show the comet to be a 5-kilometer oblate body covered with remarkable topographic features, including unusual circular features that appear to be impact craters. The presence of high-angle slopes shows that the surface is cohesive and self-supporting. The comet does not appear to be a rubble pile, and its rounded shape is not directly consistent with the comet being a fragment of a larger body. The surface is active and yet it retains ancient terrain. Wild 2 appears to be in the early stages of its degradation phase as a small volatile-rich body in the inner solar system.
1 Department of Astronomy, University of Washington, Seattle, WA 98195, USA.
2 National Aeronautics and Space Administration (NASA) Johnson Space Center, Houston, TX 77058, USA. 3 Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 911098099, USA. 4 NASA Ames Research Center, Moffet Field, CA 940351000, USA. 5 University of Massachusetts, Amherst, MA 010039291, USA. 6 Lockheed Martin Astronautics, Denver, CO, 80201, USA. 7 Planetary and Space Sciences Research Institute, Open University, Milton Keynes MK7 6AA, UK. 8 Max-Planck-Institut für Aeronomie, 37191 Katlenburg-Lindau, Germany. * To whom correspondence should addressed. E-mail: brownlee{at}astro.washington.edu
The editors suggest the following Related Resources on Science sites:In Science Magazine
THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
|
Science. ISSN 0036-8075 (print), 1095-9203 (online)