Posted by kelsey on Thursday, October 30, 2008 at 11:58pm.
Add 4*10^7 m to the radius of the Earth to get the radial distance R from the center of the earth. Call this R.
Solve for the orbital speed V first.
GM/R^2 = V^2/R
G is the universal gravity constant and M is the mass of the earth.
V * P = 2 pi R
(solve for the period P in seconds)
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