Angular Momentum
Angular momentum is the rotational analog of linear momentum. Like linear momentum, it is conserved when the net external torque is zero. This principle explains some of the most striking phenomena in mechanics — from a spinning skater to planetary orbits — and is one of the fundamental conservation laws of nature.
Key Concepts
Key Equations
Spinning Skater
A skater spins at 2.0 rad/s with arms extended ( kg·m²). She pulls in her arms, reducing to 1.5 kg·m². Find her new angular speed.
No external torque acts (frictionless ice), so is conserved:
Exercises
7 problemsAn ice skater spins with arms out at ω₁ = 3 rad/s (I₁ = 2 kg·m²). When she pulls her arms in (I₂ = 0.5 kg·m²), angular momentum is conserved. Find her new angular velocity ω₂.
Disc 1 (I₁=4, ω=6 rad/s) couples to stationary disc 2 (I₂=2). Press Couple! to watch angular momentum conserved. Find the final ω.
A spinning skater has and . She reduces to . What is her new angular velocity?
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Upgrade to Pro →A torque of acts on a spinning body for . What is the change in angular momentum?
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Upgrade to Pro →A wheel () starts from rest. A constant torque of acts for . What is the final angular velocity?
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Upgrade to Pro →A figure skater () spins at . She extends her arms, increasing to . What is her new angular velocity?
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Upgrade to Pro →A satellite moves at at from a planet. At , what is its speed? (Angular momentum is conserved.)
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Upgrade to Pro →Key Takeaways
- Angular momentum (rigid body) or (particle) is a vector quantity.
- Conservation: when net external torque is zero.
- Reducing increases and vice versa — this is why a collapsing star spins faster (pulsar formation).
- is the most general form of the rotational equation of motion.
- Angular momentum is conserved independently in each direction.