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[parent] GRE Physics Companion: Gyroscopes, Precession, and Nutation

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GRE Physics Companion: Gyroscopes, Precession, and Nutation

The fundamental relation is

|--------|
τ  = dL-.|
------dt--
(1)

For steady precession of a fixed-magnitude angular-momentum vector,

|------------|
τ  = Ω  ×  L.|
-------p------
(2)

For a rapidly spinning heavy top,

|------------|
|      M gℓ  |
|Ωp ≃  -----.|
-------I3ω3--
(3)

PIC

Figure 1. A compact strategy for gyroscope problems: identify the angular-momentum direction, compute the torque about the pivot, use the vector precession relation, and distinguish steady precession from nutation.

1 High-value GRE facts

  1. A torque perpendicular to angular momentum primarily changes its direction.
  2. Steady vector precession satisfies τ = Ωp × L.
  3. Fast gravitational precession scales inversely with spin angular momentum.
  4. Faster spin usually means slower gravitational precession.
  5. Spin, precession, and nutation are distinct motions.
  6. Nutation is variation of the inclination angle.
  7. Exact heavy-top motion generally contains both precession and nutation.
  8. For the symmetric top, ϕ and ψ are cyclic coordinates.
  9. Nutation turning points occur at E = Ueff(𝜃).
  10. A forced precessing rotor exerts an equal and opposite gyroscopic reaction torque on its support.

Part I: Original GRE-style problems

Problem 1: perpendicular torque

A torque remains perpendicular to a constant-magnitude angular momentum vector. Its primary effect is to change

  1. only the mass
  2. the direction of angular momentum
  3. the moment of inertia only
  4. the center of mass position only
  5. gravitational acceleration

Problem 2: steady precession magnitude

If the angle between Ωp and L is 𝜃, then

  1. τ = ΩpL
  2. τ = ΩpL sin 𝜃
  3. τ = Ωp∕L
  4. τ = L∕Ωp
  5. τ = ΩpL cos 2𝜃

Problem 3: fast heavy top

For a rapidly spinning heavy top,

Ωp
(4)

is approximately

  1. I3ω3∕(Mgℓ)
  2. Mgℓ∕(I3ω3)
  3. MgℓI3ω3
  4. g∕ω32
  5. ω3

Problem 4: effect of doubling spin

Within the fast-top approximation, doubling ω3 changes Ωp by a factor of

  1. 1∕4
  2. 1∕2
  3. 1
  4. 2
  5. 4

Problem 5: gravity torque

A top has center of mass distance ℓ from its pivot and inclination 𝜃 from vertical. The gravity torque magnitude is

  1. Mgℓ
  2. Mgℓ cos 𝜃
  3. Mgℓ sin 𝜃
  4. Mg∕ℓ
  5. I3ω3

Problem 6: nutation

Nutation refers to

  1. spin about the symmetry axis
  2. oscillation of the inclination angle
  3. translation of the pivot
  4. constant angular momentum magnitude
  5. zero torque

Problem 7: cyclic spin coordinate

For the heavy symmetric top,

p ψ
(5)

equals

  1. I3ω3
  2. Mgℓ
  3. I1𝜃
  4. I1ϕ
  5. zero necessarily

Problem 8: precession rate from constants

For the symmetric top,

˙ϕ
(6)

equals

  1. (pϕ − pψ cos 𝜃)∕(I1 sin 2𝜃)
  2. pϕ∕I3
  3. pψ∕I1
  4. Mgℓ∕I1
  5. zero

Problem 9: nutation turning point

At a nutation turning point,

  1. 𝜃 = 0
  2. ϕ = 0 necessarily
  3. ω3 = 0 necessarily
  4. pψ = 0
  5. gravity vanishes

Problem 10: stable steady precession

In the effective-potential picture, stable steady precession occurs at

  1. a local maximum of Ueff
  2. a local minimum of Ueff
  3. any turning point
  4. Ueff = 0 only
  5. infinite energy

Problem 11: reaction torque

A rotor is forced to precess with angular velocity Ω and angular momentum L. The torque exerted by the rotor on its support is

  1. Ω × L
  2. −Ω × L
  3. L × L
  4. zero always
  5. Ω ⋅ L

Problem 12: torque-free symmetric body

For an ideal torque-free symmetric body, the angle between its symmetry axis and the inertial angular-momentum vector is

  1. constant
  2. always zero
  3. always increasing
  4. always decreasing
  5. undefined

Part II: Complete worked solutions

Solution 1

From

dL = τ dt,
(7)

a perpendicular torque produces a perpendicular increment in angular momentum. To first order the magnitude is unchanged and the direction turns. Answer: (B).

Solution 2

The magnitude of

Ωp ×  L
(8)

is

ΩpL sin 𝜃.
(9)

Answer: (B).

Solution 3

For rapid spin,

L ≃ I3ω3,
(10)

and gravity gives

Ω  ≃  M-gℓ-.
  p   I3ω3
(11)

Answer: (B).

Solution 4

The precession rate is inversely proportional to spin rate:

       1
Ωp ∝  --.
      ω3
(12)

Doubling spin halves the precession rate. Answer: (B).

Solution 5

τ  = |r   × M  g| = M gℓsin 𝜃.
 g     CM
(13)

Answer: (C).

Solution 6

Nutation is oscillation or variation of the inclination angle

𝜃.
(14)

Answer: (B).

Solution 7

Because

ψ
(15)

is cyclic,

pψ = I3(ψ˙+ ϕ˙cos𝜃 ) = I3ω3.
(16)

Answer: (A).

Solution 8

From

pϕ =  I1ϕ ˙sin2𝜃 + pψ cos𝜃,
(17)

    p  − p  cos𝜃
˙ϕ = --ϕ---ψ-2----.
       I1sin 𝜃
(18)

Answer: (A).

Solution 9

At a turning point of the effective one-dimensional inclination motion,

˙𝜃 = 0.
(19)

Answer: (A).

Solution 10

Stable steady precession requires a stable equilibrium of the inclination coordinate:

U ′eff(𝜃0) = 0,    U ′′eff(𝜃0) > 0.
(20)

Thus it occurs at a local minimum. Answer: (B).

Solution 11

The torque on the rotor is

τ rotor = Ω × L.
(21)

Newton’s third law gives the support torque:

τ support = − Ω × L.
(22)

Answer: (B).

Solution 12

For a torque-free symmetric body,

L
(23)

is fixed in inertial space and the symmetry axis precesses around it with constant inclination. Answer: (A).

2 GRE checklist

  1. Start with τ = dL∕dt rather than memorizing a precession direction.
  2. Use τ = Ωp × L for steady vector precession.
  3. Apply the fast-top formula only when spin angular momentum dominates.
  4. Keep spin, precession, and nutation conceptually separate.
  5. For the symmetric heavy top, exploit the conserved pϕ and pψ.
  6. Use E = Ueff to identify nutation turning points.
  7. Stable steady precession corresponds to a minimum of the effective potential.
  8. Remember the equal-and-opposite reaction torque on a support that forces rotor precession.

References

References

[1]   PhysicsLibrary, M05-11, Euler’s Equations for Rigid Body Rotation.

[2]   PhysicsLibrary, M05-10, Principal Axes and Principal Moments of Inertia.

[3]   J. R. Taylor, Classical Mechanics, University Science Books, 2005.

[4]   H. Goldstein, C. Poole, and J. Safko, Classical Mechanics, 3rd ed., Addison-Wesley, 2002.

[5]   K. R. Symon, Mechanics, 3rd ed., Addison-Wesley, 1971.


"GRE Physics Companion: Gyroscopes, Precession, and Nutation" is owned by bloftin.
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Keywords:  GRE physics, gyroscope, precession, nutation, symmetric top, angular momentum, torque, steady precession, Euler angles, rigid body

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Cross-references: forces, effective potential, formula, equilibrium, angular velocity, energy, heavy symmetric top, oscillation, magnitude, acceleration, position, center of mass, moment of inertia, mass, turning points, spin, angular momentum, nutation, precession, torque, gyroscope, vector, steady precession, relation

This is version 1 of GRE Physics Companion: Gyroscopes, Precession, and Nutation, born on 2026-10-17.
Object id is 1487, canonical name is GREPhysicsCompanionGyroscopesPrecessionAndNutation.
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Classification:
Physics Classification: 45.40.-f (Dynamics and kinematics of rigid bodies)
 45.20.Dd (Newtonian mechanics)

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