The potential energy \( U \) of an object of mass \( m \) placed at a distance \( R \) from the center of the Earth (i.e., on the surface of the Earth) is given by the gravitational potential energy formula:
\[
U = -\frac{GMm}{R}
\]
Where:
- \( G \) is the gravitational constant,
- \( M \) is the mass of the Earth,
- \( m \) is the mass of the object,
- \( R \) is the radius of the Earth.
Thus, the correct answer is:
\[
\boxed{(A) \, -\frac{GMm}{R}}
\]