In the case of a stationary circular rotation of a satellite of mass m, the Moon’s gravitational force (gravity) Fg and the centrifugal force Fc act on it, they balance each other (Fg=Fc).
where v - speed of the spacecraft, m - mass of the spacecraft, R - radius of the moon, h - height of the spacecraft above the surface of the moon.
G – gravitational coVnstant, M - the mass of the Moon
Equating forces and using the formula for speed
(T- rotation period):
"h=8.7*10^7 m"
"h>>R"
Too far from the moon, this is impossible
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