we will equate the earth's grav force to the centrip force acting on the satellite
GMm/r^2=mv^2/r
where M is the mass of the earth, v the speed of the satellite, r the distance from the center of the Earth, m the mass of the satellite, and G the newtonian grav cst
this gives us:
v^2=GM/r
v=sqrt[GM/r] =
sqrt[6.67x10^(-11)(6x10^24)/(3.67xR)] =
4137.5 m/s
(where R is the radius of the Earth=
6.37x10^6m)