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The August 26, 2011, issue of Science devoted six articles to findings based on dust collected by Hayabusa. Scientists' analysis of the dust from Itokawa suggested that it had probably originally been part of a larger asteroid. Dust collected from the asteroid surface was believed to have been exposed there for about eight million years.
Dust from Itokawa was found to be "identical to material that makes up meteorites." Itokawa is an S-type asteroid whose composition matches that of an LL chondrite.
Read more about this topic: Hayabusa
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