Steven Dutch, Natural and Applied Sciences, University
of Wisconsin - Green Bay
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The asteroid was only discovered in 1998 and was photographed by the Japanese probe Hayabusa in 2005. The asteroid is not round because its gravity is far too feeble to pull it into a round shape. Its peanut shape suggests it may be a contact binary, that is, two small asteroids held in direct contact by their gravity. Contact binaries are completely impossible for large planets and moons because their gravity would pull them together into a single sphere. But tiny asteroids have such feeble gravity they can be pulled together enough to touch but not be completely merged.
Itokawa appears to be a loosely compacted pile of rocky rubble. It may have been shattered by an impact and some of the fragments were gathered up by the remnant asteroid.



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Created 17 December 2007, Last Update 28 December 2007
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