GRE Physics Companion: Gravitational Fields, Superposition, and Continuous Mass
Distributions
The Gravitational Field of a point mass is
when the source is at the origin.
For several masses,
Figure 1. A compact field strategy: identify the source geometry, choose the correct density,
exploit symmetry, integrate only surviving components, and check limiting behavior.
1 High-value GRE facts
- Gravitational field has units N∕kg = m∕s2.
- Field is force per unit test mass.
- Point-mass field magnitude is GM∕r2.
- Fields add as vectors.
- dm = λdℓ for a line.
- dm = Σ dA for a surface.
- dm = ρdV for a volume.
- Symmetry should be used before integration.
- A uniform ring has zero field at its center.
- Far from a localized source, the leading field usually approaches point-mass form.
Part I: Original GRE-style problems
Problem 1: field units
The SI units of gravitational field are
- N
- N m
- N∕kg
- kg∕N
- kg m∕s
Problem 2: field and force
At a fixed point in a gravitational field, the test mass is doubled. The gravitational field at that
point
- doubles
- halves
- remains unchanged
- becomes zero
- reverses direction
Problem 3: midpoint field
Two equal masses are placed symmetrically on opposite sides of the origin. The field at the origin
is
- toward the left mass
- toward the right mass
- zero
- twice one field
- undefined
Problem 4: line density
For a thin rod with line density λ, the correct mass element is
- dm = λdV
- dm = λdA
- dm = λdℓ
- dm = dℓ∕λ
- dm = λr2 dr
Problem 5: ring center
The gravitational field at the exact center of a uniform ring is
- GM∕a2
- 2GM∕a2
- zero
- infinite
- GM∕a
Problem 6: ring far field
Far along the axis of a ring of total mass M, its field approaches
- GM∕z
- GM∕z2
- GM∕z3
- a constant
- zero identically
Problem 7: infinite-line scaling
The field magnitude of an infinite uniform line mass scales with perpendicular distance r
as
- r
- constant
- 1∕r
- 1∕r2
- 1∕r3
Problem 8: infinite-sheet field
The magnitude of the field of an infinite uniform sheet with surface density Σ is
- GΣ∕r2
- 2πGΣ
- 4πGΣr
- GΣ∕r
- zero
Problem 9: disk far field
A finite uniform disk observed at distances much larger than its radius behaves to leading order
like
- an infinite sheet
- an infinite line
- a point mass with the disk’s total mass
- zero mass
- a dipole only
Problem 10: ring near center
For small axial displacement z from the center of a uniform ring,
is approximately proportional to
- 1∕z2
- 1∕z
- a constant
- −z
- z2
Problem 11: density dimensions
Volume mass density has units
- kg∕m
- kg∕m2
- kg∕m3
- N∕m3
- m3∕kg
Problem 12: symmetry
For a point on the symmetry axis of a uniform ring, transverse field components
- add constructively
- cancel in pairs
- are larger than the axial component
- are undefined
- produce a torque only
Part II: Complete worked solutions
Solution 1
By definition,
so the units are
Answer: (C).
Solution 2
The field is created by the source masses and is independent of the test mass. Answer:
(C).
Solution 3
The two equal field vectors have equal magnitude and opposite direction. Answer:
(C).
Solution 4
A one-dimensional mass model uses
Answer: (C).
Solution 5
Every ring element has a partner producing an equal and opposite field at the center. Answer:
(C).
Solution 6
At z ≫ a,
Answer: (B).
Solution 7
The infinite-line limit gives
Answer: (C).
Solution 8
The infinite-sheet limit of the disk result is
Answer: (B).
Solution 9
Any localized source looks like its total point mass at sufficiently large distance to leading order.
Answer: (C).
Solution 10
For |z|≪ a,
Answer: (D).
Solution 11
volume density is mass per volume:
Answer: (C).
Solution 12
Rotational symmetry pairs transverse components with equal and opposite partners. Answer:
(B).
2 GRE checklist
- Separate field from force.
- Use vectors for superposition.
- Pick λ, Σ, or ρ from source dimension.
- Use symmetry before integration.
- Check center, far-field, and infinite-source limits.
- Verify that a localized extended source approaches point-mass behavior far away.
References
References
[1] PhysicsLibrary, M07-02, Gravitational Fields, Superposition, and Continuous Mass
Distributions.
[2] PhysicsLibrary, M07-01, Newton’s Law of Universal Gravitation.
[3] J. R. Taylor, Classical Mechanics, University Science Books, 2005.