The satellite is in circular motion, and the only force acting on it is the gravity exerted from the Earth:

where

is the gravitational constant,

is the Earth's mass, m is the mass of the satellite and r is the radius of the circular orbit.
Since it is a circular motion, this force acts as centripetal force,

:

where v is the satellite's speed.
But the speed is also equal to the distance covered in one revolution (which is the circumference:

) divided by the time needed to cover one revolution (which is the period T=6560 s):

By replacing this into the previous formula and simplifying ,we get

And re-arranging and substituting the values, we find the radius of the orbit:
![r= \sqrt[3]{ (T^2 G M)/(4 \pi^2) } = 7.57 \cdot 10^7 m=7570 km](https://img.qammunity.org/2019/formulas/physics/college/dptz712zza5la55xfb77ztbgx7yrg7y41i.png)