Suppose that the Earth is fixed and that the orbit of the Moon around the Earth is approximately circular. If the radius of the Moon's orbit is R= 384,000 km and its period is T= 27.3 days, estimate the mass of the Earth.
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Let the mass of the moon be m and the mass of the earth be M. r=the radius of the moon's orbit.

Gravitational force between the moon and earth = GMm/r2,

where G=6.67×10-11Nm2/kgand r=384000000=3.84×108m.

The circular motion creates a centripetal force on the moon=mv2/r, where v is the velocity in orbit.

These two forces are equal and opposite:

GMm/r2=mv2/r. The length of the orbit is 2πr and the moon takes time T (orbital period) to travel a complete orbit, therefore T=2πr/v, so v=2πr/T. The centripetal force is 4π2rm/T2.

GMm/r2=4π2rm/T2, M=4π2r3/(GT2), r3=5.66231×1025m3, T=27.3 days=2358720 seconds, T2=5.56356×1012 s2.

M=(4π2)(5.66231×1025)/(6.67×10-11×5.56356×1012)=6.02386×1024kg.

So the mass of the earth is 6.024×1021 metric tonnes approx.

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