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The reason that graphs of asteroid rotation rates lack the expected statistical tail associated with high rotational rates is that
• Athe greater the speed in which an asteroid spins the more likely it is to cohere
• Bthe weak forces in asteroids displaying such a high rotational rate would not be able to prevent the asteroid from falling apart
• Casteroids are not being subjected to a uniform distribution of random collisions
• Dmost monolithic asteroids, upon colliding with other asteroids, are able to sustain such a high rate of rotation
• Efor the most part, the asteroids surveyed were less than 150 meters in diameter and thus far less likely to be rubble-piles, which are better able to sustain the impact from collisions

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