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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

Angular Momentum (particle)
L=r×p=mr×v\vec{L} = \vec{r}\times\vec{p} = m\vec{r}\times\vec{v}. For a particle moving in a circle: L=mrv=mr2ωL = mrv = mr^2\omega. Units: kg·m²/s.
Angular Momentum (rigid body)
For a rigid body rotating about a fixed axis: L=IωL = I\omega. This is the most common form used in GP1.
Torque–Angular Momentum Relation
τnet=dL/dt\vec{\tau}_\text{net} = d\vec{L}/dt. Net torque equals the rate of change of angular momentum — the rotational analog of F=dp/dt\vec{F} = d\vec{p}/dt.
Conservation of Angular Momentum
If the net external torque on a system is zero, L\vec{L} is constant: Iiωi=IfωfI_i\omega_i = I_f\omega_f. Conservation holds for each component independently.
Ice Skater Effect
When a spinning skater pulls in their arms, II decreases, so ω\omega must increase to conserve L=IωL = I\omega. Kinetic energy increases (work is done by the skater's muscles).
Angular Impulse
Analog of impulse: τΔt=ΔL\vec{\tau}\Delta t = \Delta\vec{L}. A torque applied for a short time produces a change in angular momentum.

Key Equations

Angular momentum (rigid body)
L=IωL = I\omega
For rotation about a fixed axis.
Angular momentum (particle)
L=mvrsinθ=mr2ωL = mvr\sin\theta = mr^2\omega
θ is the angle between r and v; for circular motion L = mvr.
Conservation of angular momentum
Iiωi=Ifωf(τext=0)I_i\omega_i = I_f\omega_f \quad (\sum\tau_\text{ext} = 0)
Valid when no net external torque acts.
Torque–angular momentum
τnet=dLdt\vec{\tau}_\text{net} = \frac{d\vec{L}}{dt}
Rotational analog of Newton's Second Law in terms of momentum.
Worked Example

Spinning Skater

Problem

A skater spins at 2.0 rad/s with arms extended (Ii=4.0I_i = 4.0 kg·m²). She pulls in her arms, reducing II to 1.5 kg·m². Find her new angular speed.

Solution

No external torque acts (frictionless ice), so LL is conserved:

Iiωi=IfωfI_i\omega_i = I_f\omega_f
ωf=IiωiIf=4.0×2.01.55.3 rad/s\omega_f = \frac{I_i\omega_i}{I_f} = \frac{4.0\times 2.0}{1.5} \approx 5.3 \text{ rad/s}
Answer New angular speed ≈ 5.3 rad/s — faster than before.
Practice

Exercises

7 problems
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Exercise 1 / 7 Free
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An 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.

ω₂ = rad/s
Exercise 2 / 7 Free
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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.

ω_f = rad/s
3 of 7

A spinning skater has Ii=4 kg⋅m2I_i = 4 \text{ kg·m}^2 and ωi=2 rad/s\omega_i = 2 \text{ rad/s}. She reduces II to 1 kg⋅m21 \text{ kg·m}^2. What is her new angular velocity?

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4 of 7

A torque of 6 N⋅m6 \text{ N·m} acts on a spinning body for 3 s3 \text{ s}. What is the change in angular momentum?

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5 of 7

A wheel (I=2 kg⋅m2I = 2 \text{ kg·m}^2) starts from rest. A constant torque of 4 N⋅m4 \text{ N·m} acts for 5 s5 \text{ s}. What is the final angular velocity?

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6 of 7

A figure skater (I1=5 kg⋅m2I_1 = 5 \text{ kg·m}^2) spins at 1.5 rad/s1.5 \text{ rad/s}. She extends her arms, increasing II to 7.5 kg⋅m27.5 \text{ kg·m}^2. What is her new angular velocity?

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7 of 7

A satellite moves at v1=3000 m/sv_1 = 3000 \text{ m/s} at r1=2×107 mr_1 = 2 \times 10^7 \text{ m} from a planet. At r2=1×107 mr_2 = 1 \times 10^7 \text{ m}, what is its speed? (Angular momentum is conserved.)

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Key Takeaways

  • Angular momentum L=IωL = I\omega (rigid body) or L=mvrsinθL = mvr\sin\theta (particle) is a vector quantity.
  • Conservation: Iiωi=IfωfI_i\omega_i = I_f\omega_f when net external torque is zero.
  • Reducing II increases ω\omega and vice versa — this is why a collapsing star spins faster (pulsar formation).
  • τnet=dL/dt\vec{\tau}_\text{net} = d\vec{L}/dt is the most general form of the rotational equation of motion.
  • Angular momentum is conserved independently in each direction.