Step 1: Understanding the Concept:
When an object is moved through a significant distance relative to Earth's radius, we cannot use the simplified formula $W=mgh$. We must use the change in gravitational potential energy ($U = -GMm/r$). Step 2: Key Formula or Approach:
1. $W = \Delta U = U_f - U_i$
2. $U = -\frac{GMm}{r}$
3. Relationship: $g = \frac{GM}{R^2} \implies GM = gR^2$ Step 3: Detailed Explanation:
1. Initial distance from center: $r_i = R$ (Surface)
2. Final distance from center: $r_f = R + R = 2R$ (at height $R$)
3. Work Done ($W$):
\[ W = \left( -\frac{GMm}{2R} \right) - \left( -\frac{GMm}{R} \right) \]
\[ W = \frac{GMm}{R} - \frac{GMm}{2R} = \frac{GMm}{2R} \]
4. Substitute $GM = gR^2$:
\[ W = \frac{(gR^2)m}{2R} = \frac{mgR}{2} \] Step 4: Final Answer:
The work done is mgR/2.