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Rigid Body Dynamics

A rigid body has six degrees of freedom — three translational and three rotational. The rotational dynamics are governed by Euler's equations for the body-frame angular velocity, and the moment of inertia tensor replaces the scalar mass. Gyroscopic effects and precession emerge naturally.

Key Concepts

Moment of Inertia Tensor
Iij=kmk(rk2δijrkirkj)I_{ij}=\sum_k m_k(r_k^2\delta_{ij}-r_{ki}r_{kj}). For a principal-axis frame, II is diagonal with principal moments I1,I2,I3I_1,I_2,I_3. Angular momentum: L=Iω\vec L=\mathbf{I}\vec\omega.
Euler's Equations
I1ω˙1(I2I3)ω2ω3=τ1I_1\dot\omega_1-(I_2-I_3)\omega_2\omega_3=\tau_1 and cyclic permutations. Written in the body frame where II is diagonal. For a torque-free symmetric top (I1=I2I_1=I_2), these give steady precession of ω\vec\omega around the symmetry axis.
Parallel Axis Theorem
I=Icm+Md2I=I_{\rm cm}+Md^2, where IcmI_{\rm cm} is the moment about the center of mass and dd is the distance to the new axis. Allows computation of II about any parallel axis.
Gyroscopic Precession
A spinning top with angular momentum LL subject to torque τ\tau (from gravity) precesses at Ωprec=τ/L=Mgd/(Iωs)\Omega_{\rm prec}=\tau/L=Mgd/(I\omega_s), where dd is the distance from pivot to CM.

Key Equations

Rotational KE (principal axes)
Trot=12(I1ω12+I2ω22+I3ω32)T_{\rm rot} = \frac{1}{2}(I_1\omega_1^2 + I_2\omega_2^2 + I_3\omega_3^2)
Kinetic energy of rotation in the principal-axis frame.
Parallel axis theorem
I=Icm+Md2I = I_{\rm cm} + Md^2
Moment of inertia about an axis parallel to the CM axis, distance d away.
Precession rate
Ωprec=MgdI3ωs\Omega_{\rm prec} = \frac{Mgd}{I_3\omega_s}
Gyroscopic precession rate of a symmetric top spinning at ωₛ, CM distance d from pivot.
Worked Example

Moment of Inertia of a Rod

Problem

Find the moment of inertia of a uniform rod of mass M=2.0M=2.0 kg and length L=1.2L=1.2 m about: (a) its center, (b) one end.

Solution

(a) About center: Icm=112ML2=112(2.0)(1.44)=0.240I_{\rm cm}=\frac{1}{12}ML^2=\frac{1}{12}(2.0)(1.44)=0.240 kg·m².

(b) About one end (distance d=L/2=0.6d=L/2=0.6 m from CM):

Iend=Icm+Md2=0.240+(2.0)(0.36)=0.240+0.720=0.960 kg⋅m2I_{\rm end} = I_{\rm cm} + Md^2 = 0.240 + (2.0)(0.36) = 0.240 + 0.720 = 0.960\text{ kg·m}^2

Check: Iend=13ML2=13(2.0)(1.44)=0.960I_{\rm end}=\frac{1}{3}ML^2=\frac{1}{3}(2.0)(1.44)=0.960 kg·m² ✓

Answer Icm=0.240I_{\rm cm}=0.240 kg·m², Iend=0.960I_{\rm end}=0.960 kg·m².
Practice

Exercises

7 problems
1 of 7

A uniform rod has M=3.0M=3.0 kg and L=2.0L=2.0 m. Find its moment of inertia (in kg·m²) about its center.

kg·m²
2 of 7

Using the parallel axis theorem, find II (in kg·m²) for the same rod (M=3.0M=3.0 kg, L=2.0L=2.0 m) about one end.

kg·m²
3 of 7

A solid disk has M=5.0M=5.0 kg and R=0.40R=0.40 m. Find its moment of inertia (in kg·m²) about its symmetry axis.

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4 of 7

A solid sphere (M=4.0M=4.0 kg, R=0.20R=0.20 m) rotates at ω=10\omega=10 rad/s. Find its rotational kinetic energy (in J).

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5 of 7

A gyroscope has spin angular momentum L=8.0L=8.0 kg·m²/s and its CM is d=0.15d=0.15 m from the pivot. Find the precession rate Ωprec\Omega_{\rm prec} (in rad/s). Mass of gyroscope: M=0.50M=0.50 kg.

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6 of 7

A thin ring of mass M=2.0M=2.0 kg and radius R=0.50R=0.50 m rotates about its symmetry axis. Find its moment of inertia (in kg·m²).

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7 of 7

A rod (M=2.0M=2.0 kg, L=1.0L=1.0 m, Iend=13ML2I_{\rm end}=\frac{1}{3}ML^2) is pivoted at one end and released from horizontal. Find its angular acceleration α\alpha (in rad/s²) at the moment of release.

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Key Takeaways

  • The moment of inertia tensor generalizes scalar II; principal axes diagonalize it.
  • Parallel axis theorem: I=Icm+Md2I=I_{\rm cm}+Md^2 — always add when moving away from the CM.
  • Euler's equations govern torque-free rotation; asymmetric tops exhibit complex tumbling (Euler's equations are nonlinear).
  • Gyroscopic precession Ω=Mgd/(Iω)\Omega=Mgd/(I\omega): heavier, slower, longer-armed tops precess faster.