The rotations of asteroids larger than -40 km in diameter have a distribution close to Maxwellian that suggests that they are either original bodies of the asteroid main belt or its largest, collisionally evolved remnants.
The rotations of asteroids larger than -40 km in diameter have a distribution close to Maxwellian that suggests that they are either original bodies of the asteroid main belt or its largest, collisionally evolved remnants. (en)