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For an object to become round, its gravity must be strong enough to overcome their rigidity. The size at which this occurs is different for each material it could be made of, but by comparing the size of the smallest rounded objects to the largest unrounded objects, a midpoint can be found; the moon Mimas has a mass of around 4 x 1019 kg and is rounded, where many asteroids ranging from 2 x 1019 to 4 x 1019 kg are not so. While this may be due to impacts and not their own characteristics, we could probably place the mass necessary for rounding to begin at somewhere around this mark.

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15y ago

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