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
Key Equations
Moment of Inertia of a Rod
Find the moment of inertia of a uniform rod of mass kg and length m about: (a) its center, (b) one end.
(a) About center: kg·m².
(b) About one end (distance m from CM):
Check: kg·m² ✓
Exercises
7 problemsA uniform rod has kg and m. Find its moment of inertia (in kg·m²) about its center.
Using the parallel axis theorem, find (in kg·m²) for the same rod ( kg, m) about one end.
A solid disk has kg and m. Find its moment of inertia (in kg·m²) about its symmetry axis.
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Upgrade to Pro →A solid sphere ( kg, m) rotates at rad/s. Find its rotational kinetic energy (in J).
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Upgrade to Pro →A gyroscope has spin angular momentum kg·m²/s and its CM is m from the pivot. Find the precession rate (in rad/s). Mass of gyroscope: kg.
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Upgrade to Pro →A thin ring of mass kg and radius m rotates about its symmetry axis. Find its moment of inertia (in kg·m²).
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Upgrade to Pro →A rod ( kg, m, ) is pivoted at one end and released from horizontal. Find its angular acceleration (in rad/s²) at the moment of release.
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Upgrade to Pro →Key Takeaways
- The moment of inertia tensor generalizes scalar ; principal axes diagonalize it.
- Parallel axis theorem: — 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 : heavier, slower, longer-armed tops precess faster.