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Asked in NEET 2005 · Energy of an orbiting satellite
For a circular orbit of radius r, the centripetal condition gives (mv²)/r=(GMm)/(r²).
So the kinetic energy is K=1/2mv²=(GMm)/(2r).
The potential energy is U=-(GMm)/r.
Comparing magnitudes, |U|=2K.
K/(|U|)=1/2.
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