Davide M. answered 02/04/21
Ph.D. in Applied Mathematics and Master Degree in Theoretical Physics
The centripetal force CF ωacting on a object of mass m rotating with angular velocity ω at distance r from the center of the Earth is given by
CF=mωr2
For circular orbits, the centripetal force must be equal to the gravitational force GF given by
GF=γmM/r2
where γ is the gravitational constant (numerical value γ≈6.6·10-11), M is the mass of the Earth (numerical value M≈5.97·1024)
You therefore must impose the above quantity to be equal, thus
mωr2=γmM/r2
and therefore, r=(γM/ω)1/3
In order to obtain the geostationary orbit, you use the angular velocity of the Earth (numerical value ω≈7,2921·10−5).
If you plug in all the numerical values (you can also check that the units will be meters!) you will obtain the geostationary radius r≈4.2·107 m which is roughly 42.000 km.
Best,
Davide