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Abstract

Collisions in the asteroid belt frequently lead to catastrophic breakups, where more than half of the target's mass is ejected into space. Several dozen large asteroids have been disrupted by impacts over the past several billion years. These impact events have produced groups of fragments with similar orbits called asteroid families. Here we report the discovery of a very young asteroid family around the object 1270 Datura. Our work takes advantage of a method for identification of recent breakups in the asteroid belt using catalogs of osculating (i.e., instantaneous) asteroid orbits. The very young families show up in these catalogs as clusters in a five-dimensional space of osculating orbital elements.
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This manuscript is based upon work supported by NASA's Planetary Geology and Geophysics program and the Czech Grant Agency.

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Published In

Science
Volume 312 | Issue 5779
9 June 2006

Submission history

Received: 13 February 2006
Accepted: 3 April 2006
Published in print: 9 June 2006

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Authors

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David Nesvorný*
Department of Space Studies, Southwest Research Institute, 1050 Walnut Street, Suite 400, Boulder, CO 80302, USA.
David Vokrouhlický
Department of Space Studies, Southwest Research Institute, 1050 Walnut Street, Suite 400, Boulder, CO 80302, USA.
William F. Bottke
Department of Space Studies, Southwest Research Institute, 1050 Walnut Street, Suite 400, Boulder, CO 80302, USA.

Notes

* To whom correspondence should be addressed. E-mail: [email protected]

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