Find the distance from the center of the earth to a geosynchronous satellite that is located some point along the equator.
The formula for the velocity of a geosynchronous satellite is:
If a geosynchronous satellite is located along the equator from the center of the Earth, the gravitational force will be equal to the centripetal force.
Here, G represents the gravitational constant (6.67×10-11 Nm2/kg2), M represents the mass of the Earth (6×1024 kg), and T represents the time (1 day).
By putting the corresponding values in the equation, we get:
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