Final answer:
The velocity with which an object hits the Earth is given by (GM/R)¹/², derived from energy conservation principles equating gravitational potential and kinetic energies.
Step-by-step explanation:
The velocity with which an object m hits the Earth is given by the formula derived from equating kinetic energy to gravitational potential energy. Using the formula for gravitational potential energy (U = -GMm/R) and kinetic energy (K = 1/2 mv²), and setting them equal for an object falling from rest far away (ignoring air resistance), we get:
1/2 mv² = GMm/R
By canceling out the mass m from both sides and solving for v, we obtain:
v = (2GM/R)¹/²
This corresponds to option A: (GM/R)¹/².