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In this paper we show an example of a young asteroid cluster located in a dynamically stable region, which was produced by partial disruption of a primitive body about 30 km in size. We estimate its age to be only 1.9 ± 0.3 Myr; thus, its post‐impact evolution should have been very limited. The large difference in size between the largest object and the other cluster members means that this was a...
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