To solve this problem we will apply the concepts related to the balance of Forces, in this case the centripetal force of the body must be equal to the gravitational force exerted by the moon on it.
The gravitational force is given by the function
Here
G = Gravitational Universal constant
M = Mass of the planet
m = Mass of the satellite
r = Radius(orbit)
Now the centripetal force is given as
Here
m = mass of satellite
v = Velocity of satellite
r = Radius (orbit)
Since there must be balance for the satellite to remain in the orbit
The velocity depends on the mass of the planet and the orbit, and not on the mass, so if the orbit is maintained, the velocity will be the same: 946m/s