The gravitational attraction between the Earth and the satellite provides the centripetal force that keeps the satellite in circular motion:

where
m is the satellite mass
v is its speed
r is its distance from the Earth's center
G is the gravitational constant
M is the Earth's mass
Re-arranging the formula, we get

The satellite orbits at a distance equal to one Earth's radius (R) above the surface. This means that its distance from the Earth's center is twice the Earth radius:

Therefore, its velocity is
