Gravitational Near Earth Surface.

AI Thread Summary
The discussion centers on calculating the minimum mass of a neutron star with a radius of 7 km that rotates at 1000 revolutions per second, ensuring surface material remains in place. The user attempts to solve the problem using the formula but receives feedback indicating a mistake in not cubing the radius value. The correct approach involves applying gravitational equations while considering the effects of rapid rotation. The conversation highlights the importance of careful mathematical application in physics problems. Properly cubing the radius is crucial for accurate results in this context.
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Homework Statement



Certain neutron stars (extremely dense stars) are believed to be rotating at about 1000 rev/s. If such a star has a radius of 7 km, what must be its minimum mass so that material on its surface remains in place during the rapid rotation?

Homework Equations



cramster-equation-201031601226340429448270400007570.gif




The Attempt at a Solution



(7x10^3)(1000*2pi)/6.67*10^-11= 2.0301495

I'm getting it wrong. Any hints why?
 
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You forgot to cube the value of R.

ehild
 
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