Answer:

Step-by-step explanation:
The initial mechanical energy of the object, when it is suspended at a height h above the planet of radius R and mass M, is just gravitational potential energy, so

When the object reaches the ground, its mechanical energy is now sum of its kinetic energy Kf and its new gravitational potential energy Uf:

Since the mechanical energy is conserved, we can write
Ei = Ef
So we can write
![\frac{GMm}{R+h] =(1)/(2)mv^2 + (GMm)/(R)]()
from which we can find an expression for v, the speed of the object when it hits the ground:
