GRE Physics Companion: Gravitational Potential Energy and Gravitational Potential
For point-mass gravity,
The field is related to potential by
Figure 1. A compact potential strategy: choose the reference zero, write or integrate the potential,
differentiate to recover the field when needed, and use energy conservation for motion.
1 High-value GRE facts
- With zero at infinity, U = −GMm∕r.
- gravitational potential is Φ = U∕m = −GM∕r.
- g = −∇Φ.
- Potential is scalar and superposes algebraically.
- A shell has zero interior field but nonzero constant interior potential.
- A uniform sphere has a quadratic interior potential.
- Near a surface, ΔU ≈ mgh only for small height changes.
- Escape corresponds to the threshold total energy E = 0.
- vesc =
.
- For a system of masses, count each interacting pair once.
Part I: Original GRE-style problems
Problem 1: sign of point-mass potential energy
With U(∞) = 0, the gravitational potential energy of two positive masses at finite separation
is
- positive
- zero
- negative
- imaginary
- undefined
Problem 2: gravitational potential
The gravitational potential of a point mass M is
- −GM∕r
- −GMm∕r
- GM∕r2
- −GM∕r2
- GMm∕r
Problem 3: field from potential
The Gravitational Field is related to gravitational potential by
- g = ∇Φ
- g = −∇Φ
- g = Φr
- g = ∇2Φ
- g = 0 everywhere
Problem 4: interior shell potential
Inside a thin uniform spherical shell of radius R and mass M, the gravitational potential
is
- zero
- −GM∕r
- −GM∕R
- −GMr∕R2
- +GM∕R
Problem 5: uniform-sphere center potential
At the center of a uniform solid sphere,
equals
- −GM∕R
- −3GM∕(2R)
- −GM∕(2R)
- zero
- −2GM∕R
Problem 6: near-surface approximation
The approximation
is best when
- h ≫ R
- h is comparable to R
- |h|≪ R
- g = 0
- the source is nonspherical
Problem 7: escape speed
The minimum Newtonian escape speed from radius r is
- GM∕r
- 2GM∕r

Problem 8: circular versus escape speed
At the same radius,
is
- 1∕2
- 1
- 2
- 2π
Problem 9: equipotential geometry
The equipotential surfaces of an isolated point mass are
- planes
- cylinders
- spheres
- cones
- helices
Problem 10: zero field
At a point where the gravitational field is zero, the gravitational potential
- must also be zero
- must be positive
- need not be zero
- must be infinite
- cannot be defined
Problem 11: scalar superposition
For several point masses, gravitational potential is found by
- vector addition of each potential
- scalar addition of each potential
- multiplying the individual potentials
- averaging the masses first
- adding only the nearest mass
Problem 12: pair counting
For three point masses, the number of distinct pairwise gravitational-potential-energy terms
is
- 1
- 2
- 3
- 6
- 9
Part II: Complete worked solutions
Solution 1
With zero at infinity,
for finite positive r. Answer: (C).
Solution 2
Potential is potential energy per unit test mass:
Answer: (A).
Solution 3
A conservative gravitational field points toward decreasing potential:
Answer: (B).
Solution 4
The shell interior field is zero, so the potential is constant and equals its surface value:
Answer: (C).
Solution 5
For a uniform sphere,
Answer: (B).
Solution 6
The constant-g approximation is accurate when the height change is small compared with the
body’s radius. Answer: (C).
Solution 7
Set the minimum escape energy equal to zero:
Thus
Answer: (B).
Solution 8
Since
Answer: (C).
Solution 9
Point-mass potential depends only on radius, so constant-potential surfaces are spheres. Answer:
(C).
Solution 10
Zero field means zero gradient of potential, not necessarily zero potential itself. Answer:
(C).
Solution 11
Potential is a scalar, so individual potentials add algebraically. Answer: (B).
Solution 12
The distinct pairs are (1, 2), (1, 3), and (2, 3). Answer: (C).
2 GRE checklist
- Keep U and Φ distinct.
- Use the minus sign in both U = −GMm∕r and g = −∇Φ.
- Remember that zero field does not imply zero potential.
- Use mgh only as a local approximation.
- Set E = 0 for the minimum escape condition.
- Count each pair once in system potential energy.
References
References
[1] PhysicsLibrary, M07-04, Gravitational Potential Energy and Gravitational Potential.
[2] PhysicsLibrary, M07-03, Newton’s Shell Theorem and Spherical Mass Distributions.
[3] J. R. Taylor, Classical Mechanics, University Science Books, 2005.