Consider earth as shown in the figure. The satellite is moving in an east west direction.
We know that earth has rotation. Therefore, let ωe be the angular velocity of earth.
And let ωs be the angular velocity of the satellite.
Lets assume that ‘T′ to be the time period between successive passings about the equator.
We know that, when a satellite is moving in the geostationary orbit of earth, its angular velocity is the same as that of earth’s angular velocity.
So we can write,
ωe=ωs
Now T=2πωrel=2πωe+ωs
T=2π2ωs
For Geostationary satellite 2πωs=24 hr
T=2π×24×hr.2×2π
T=12 hr.