Answer:
T = approximately 24 hs.
Explanation:
In order to keep the satellite over a fixed point on the equator, as the earth rotates, the satellite must have the same angular velocity that Earth has, which means that it must have a period equal to the time used by Earth to complete an entire rotation on itself, which is almost exactly 24 Hs.
Mathematically, this can be obtained taking into account that the force that keeps the satellite in orbit is the centripetal force, which is actually the gravitational force exerted by Earth, so we can write the following equality:
Fg = Fc ⇒ G*ms*me / (re +rsat)² = ms*ω²*(re +rsat)
By definition, ω =ΔФ / Δt
For a complete revolution, ΔФ = 2*π, and Δt = T (period of the rotation),
so we can replace ω by (2*π/T), solving then for T:
T= 86,313 sec. (24 hs are exactly 86,400 sec, so the value is actually very close to the theorical one).
