The fastest possible rate of rotation of a planet is that for which the gravitational force on material at the equator barely provides the centripetal force needed for the rotation. For a planet with a uniform density of 8.8 g/cm3, typical of many planets and asteroids, evaluate the shortest period of rotation.
Rate of rotation?
Centripetal acceleration = (V^2)/R
http://en.wikipedia.org/wiki/Centripetal...
Acceleration due to gravity = GM/(R^2)
http://en.wikipedia.org/wiki/Gravity
At the shortest period of rotation, they are equal so
(V^2)/R = GM/(R^2)
G is the universal gravitational constant.
M is the volume of the sphere of radius R times the density
The period of rotation = distance/velocity = 2(pi)R/V
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