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๐ŸŽฏโญ INTERACTIVE LESSON

Rotational Dynamics and Angular Momentum

Learn step-by-step with interactive practice!

Rotational Dynamics and Angular Momentum - Complete Interactive Lesson

Part 1: Angular Momentum (L = Iฯ‰)

๐ŸŒ€ Angular Momentum

Part 1 of 7 โ€” L=Iฯ‰L = I\omega

Just as linear momentum p=mvp = mv describes the "quantity of motion" in a straight line, angular momentum L=Iฯ‰L = I\omega describes the "quantity of rotational motion."

Defining Angular Momentum

For a rigid body rotating about a fixed axis:

L=Iฯ‰L = I\omega

Where:

  • LL = angular momentum (kgโ‹…m2/s)(kg\cdot m^{2}/s)
  • II = rotational inertia (kgโ‹…m2)(kg\cdot m^{2})
  • ฯ‰\omega = angular velocity (rad/s)

For a Point Mass

A particle of mass mm moving in a circle of radius rr:

L=mvrL = mvr

(since I=mr2I = mr^2 and ฯ‰=v/r\omega = v/r, so L=mr2โ‹…v/r=mvrL = mr^2 \cdot v/r = mvr)

Direction and Sign

Like torque, angular momentum follows a sign convention:

  • CCW rotation โ†’ L>0L > 0 (positive)
  • CW rotation โ†’ L<0L < 0 (negative)

Units

[L]=kgโ‹…m2/s[L] = \text{kg}\cdot\text{m}^2\text{/s}

Linear-Rotational Analogies

LinearRotational
Mass mmRotational inertia II
Velocity vvAngular velocity ฯ‰\omega
Momentum p=mvp = mvAngular momentum L=Iฯ‰L = I\omega
Force FFTorque ฯ„\tau
F=maF = maฯ„=Iฮฑ\tau = I\alpha
F=dp/dtF = dp/dtฯ„=dL/dt\tau = dL/dt

Key Insight

Angular momentum is large when:

  • The object has a large rotational inertia (lots of mass far from axis)
  • The object spins fast (large ฯ‰\omega)

A massive, slowly spinning flywheel can have the same LL as a tiny, rapidly spinning top.

Angular Momentum Quiz ๐ŸŽฏ

Angular Momentum Calculations ๐Ÿงฎ

  1. A solid disk (M=4M = 4 kg, R=0.5R = 0.5 m) spins at ฯ‰=10\omega = 10 rad/s. What is its angular momentum? (inkgโ‹…m2/s)(in kg\cdot m^{2}/s)

  2. A particle of mass 0.5 kg moves at 8 m/s in a circle of radius 2 m. What is its angular momentum? (inkgโ‹…m2/s)(in kg\cdot m^{2}/s)

  3. A flywheel has L=200L = 200 kgโ‹…m2/skg\cdot m^{2}/s and I=25I = 25 kgโ‹…m2kg\cdot m^{2}. What is its angular velocity? (in rad/s)

Angular Momentum Concepts ๐Ÿ”

Exit Quiz โ€” Angular Momentum Basics โœ…

Part 2: Conservation of Angular Momentum

๐Ÿ”„ Newton's Second Law for Rotation

Part 2 of 7 โ€” ฯ„net=Iฮฑ\tau_{\text{net}} = I\alpha

Newton's Second Law F=maF = ma has a rotational analogue: net torque equals rotational inertia times angular acceleration.

The Rotational Second Law

ฯ„net=Iฮฑ\tau_{\text{net}} = I\alpha

This is the most important equation in rotational dynamics. It tells us:

  • A net torque causes angular acceleration
  • More rotational inertia means less angular acceleration for the same torque
  • The angular acceleration is in the same direction as the net torque

Equivalent Form

ฯ„net=ฮ”Lฮ”t\tau_{\text{net}} = \frac{\Delta L}{\Delta t}

Net torque equals the rate of change of angular momentum โ€” the direct analogue of F=dp/dtF = dp/dt.

When ฯ„net=0\tau_{\text{net}} = 0:

ฮ”Lฮ”t=0โ‡’L=constant\frac{\Delta L}{\Delta t} = 0 \Rightarrow L = \text{constant}

No net torque โ†’ angular momentum is conserved!

Applying ฯ„=Iฮฑ\tau = I\alpha

Example 1: Spinning a Wheel

A solid disk (M=5M = 5 kg, R=0.4R = 0.4 m) has a tangential force of 2020 N applied at its rim.

  • I=12MR2=12(5)(0.16)=0.4I = \frac{1}{2}MR^2 = \frac{1}{2}(5)(0.16) = 0.4 kgโ‹…m2kg\cdot m^{2}
  • ฯ„=FR=(20)(0.4)=8\tau = FR = (20)(0.4) = 8 Nยทm
  • ฮฑ=ฯ„/I=8/0.4=20\alpha = \tau/I = 8/0.4 = 20 rad/s2rad/s^{2}

Example 2: Pulley Problem

A mass mm hangs from a string wrapped around a pulley (mass MM, radius RR, solid disk). The tension in the string provides the torque:

ฯ„=TR=Iฮฑ=12MR2โ‹…aR\tau = TR = I\alpha = \frac{1}{2}MR^2 \cdot \frac{a}{R}

Combined with mgโˆ’T=mamg - T = ma, you can solve for both aa and TT.

Rotational Newton's Second Law Quiz ๐ŸŽฏ

Rotational Dynamics Calculations ๐Ÿงฎ

  1. A solid cylinder (M=8M = 8 kg, R=0.25R = 0.25 m) has a net torque of 5 Nยทm applied. What is ฮฑ\alpha? (inrad/s2)(in rad/s^{2})

  2. A wheel (I=2I = 2 kgโ‹…m2kg\cdot m^{2}) starts from rest and a constant torque of 6 Nยทm is applied for 4 seconds. What is the final angular velocity? (in rad/s)

  3. A disk (I=0.5I = 0.5 kgโ‹…m2kg\cdot m^{2}) decelerates from 40 rad/s to rest in 8 seconds. What is the magnitude of the braking torque? (in Nยทm)

Round all answers to 3 significant figures.

Rotational Dynamics Review ๐Ÿ”

Exit Quiz โ€” Rotational Second Law โœ…

Part 3: Ice Skater & Spinning Examples

โšก Rotational Kinetic Energy

Part 3 of 7 โ€” KErot=12Iฯ‰2KE_{\text{rot}} = \frac{1}{2}I\omega^2

A spinning object has kinetic energy due to its rotation โ€” even if its center of mass isn't moving. This rotational kinetic energy follows the same pattern as translational KE.

Rotational Kinetic Energy

KErot=12Iฯ‰2KE_{\text{rot}} = \frac{1}{2}I\omega^2

Compare with translational: KEtrans=12mv2KE_{\text{trans}} = \frac{1}{2}mv^2

LinearRotational
12mv2\frac{1}{2}mv^212Iฯ‰2\frac{1}{2}I\omega^2

Units

KErotKE_{\text{rot}} is measured in joules (J), just like any other form of energy.

Total Kinetic Energy for Rolling Objects

An object that both translates and rotates has:

KEtotal=12mvcm2+12Iฯ‰2KE_{\text{total}} = \frac{1}{2}mv_{\text{cm}}^2 + \frac{1}{2}I\omega^2

For rolling without slipping (v=Rฯ‰v = R\omega):

ShapeKEtotalKE_{\text{total}}
Hoop12mv2+12mv2=mv2\frac{1}{2}mv^2 + \frac{1}{2}mv^2 = mv^2
Disk12mv2+14mv2=34mv2\frac{1}{2}mv^2 + \frac{1}{4}mv^2 = \frac{3}{4}mv^2
Solid sphere12mv2+15mv2=710mv2\frac{1}{2}mv^2 + \frac{1}{5}mv^2 = \frac{7}{10}mv^2

Work-Energy Theorem for Rotation

The work done by a torque:

W=ฯ„โ‹…ฮธW = \tau \cdot \theta

The work-energy theorem:

Wnet=ฮ”KErot=12Iฯ‰f2โˆ’12Iฯ‰i2W_{\text{net}} = \Delta KE_{\text{rot}} = \frac{1}{2}I\omega_f^2 - \frac{1}{2}I\omega_i^2

Power

The rotational power (rate of doing work):

P=ฯ„ฯ‰P = \tau\omega

This is analogous to P=FvP = Fv in linear motion.

Rotational KE Quiz ๐ŸŽฏ

Rotational KE Calculations ๐Ÿงฎ

  1. A wheel (I=4I = 4 kgโ‹…m2kg\cdot m^{2}) spins at 10 rad/s. What is its rotational KE? (in J)

  2. A solid sphere (mass 3 kg, radius 0.1 m) spins at 20 rad/s (not translating). What is its rotational KE? (in J, round to 3 significant figures)

  3. A torque of 8 Nยทm acts through an angle of 25 rad on a wheel. How much work is done? (in J)

Energy Concepts ๐Ÿ”

Exit Quiz โ€” Rotational KE โœ…

Part 4: Angular Impulse

๐Ÿ”’ Conservation of Angular Momentum

Part 4 of 7 โ€” No External Torque โ†’ LL is Conserved

Just as linear momentum is conserved when there is no external force, angular momentum is conserved when there is no external torque.

The Conservation Law

If ฯ„net,ย ext=0\tau_{\text{net, ext}} = 0, then:

Li=LfL_i = L_f Iiฯ‰i=Ifฯ‰fI_i \omega_i = I_f \omega_f

What Counts as "No External Torque"?

External torque is zero when:

  • No external forces act on the system
  • External forces act at the axis of rotation (r=0r = 0)
  • External forces are parallel to the axis

Key Consequence

If II decreases โ†’ ฯ‰\omega must increase (and vice versa) to keep LL constant.

ฯ‰f=IiIfฯ‰i\omega_f = \frac{I_i}{I_f} \omega_i

Important Distinction

Angular momentum is conserved, but rotational kinetic energy is generally NOT conserved when II changes:

KEf=12Ifฯ‰f2=IiIfร—12Iiฯ‰i2=IiIfKEiKE_f = \frac{1}{2}I_f\omega_f^2 = \frac{I_i}{I_f} \times \frac{1}{2}I_i\omega_i^2 = \frac{I_i}{I_f} KE_i

If II decreases, KEKE increases โ€” the energy comes from internal work (muscles, etc.).

Rotational Collisions

When two rotating objects interact (e.g., a disk drops onto a turntable), angular momentum is conserved:

I1ฯ‰1+I2ฯ‰2=(I1+I2)ฯ‰fI_1\omega_1 + I_2\omega_2 = (I_1 + I_2)\omega_f

Example

A disk (I1=2I_1 = 2 kgโ‹…m2kg\cdot m^{2}, ฯ‰1=10\omega_1 = 10 rad/s) has a ring (I2=3I_2 = 3 kgโ‹…m2kg\cdot m^{2}, initially at rest) dropped on top:

2(10)+3(0)=(2+3)ฯ‰f2(10) + 3(0) = (2 + 3)\omega_f ฯ‰f=20/5=4ย rad/s\omega_f = 20/5 = 4 \text{ rad/s}

Note: KE is NOT conserved (this is an inelastic rotational "collision").

Conservation Quiz ๐ŸŽฏ

Conservation Calculations ๐Ÿงฎ

  1. A turntable (I=0.5I = 0.5 kgโ‹…m2kg\cdot m^{2}) spins at 8 rad/s. A 2 kg block of clay (I=mr2I = mr^2, r=0.3r = 0.3 m) is dropped on it. What is the final ฯ‰\omega? (in rad/s, round to 3 significant figures)

  2. A skater with I=4I = 4 kgโ‹…m2kg\cdot m^{2} and ฯ‰=6\omega = 6 rad/s pulls in her arms to I=1.5I = 1.5 kgโ‹…m2kg\cdot m^{2}. What is her new ฯ‰\omega? (in rad/s)

  3. In problem 2, by what factor does her KE increase? (round to 3 significant figures)

Conservation Concepts ๐Ÿ”

Exit Quiz โ€” Conservation of Angular Momentum โœ…

Part 5: Rotational Kinetic Energy

โญ Figure Skater & Collapsing Star Examples

Part 5 of 7 โ€” Conservation in Action

The conservation of angular momentum produces some of nature's most dramatic phenomena โ€” from figure skaters spinning faster to neutron stars rotating hundreds of times per second.

The Figure Skater

A figure skater begins a spin with arms extended:

  • Ii=4.0I_i = 4.0 kgโ‹…m2kg\cdot m^{2}, ฯ‰i=3\omega_i = 3 rad/s
  • L=Iiฯ‰i=12L = I_i\omega_i = 12 kgโ‹…m2/skg\cdot m^{2}/s

She pulls her arms in:

  • If=1.2I_f = 1.2 kgโ‹…m2kg\cdot m^{2}
  • ฯ‰f=L/If=12/1.2=10\omega_f = L/I_f = 12/1.2 = 10 rad/s

Speed increase: ฯ‰f/ฯ‰i=10/3โ‰ˆ3.3ร—\omega_f/\omega_i = 10/3 \approx 3.3\times faster!

Energy Analysis

  • KEi=12(4.0)(9)=18KE_i = \frac{1}{2}(4.0)(9) = 18 J
  • KEf=12(1.2)(100)=60KE_f = \frac{1}{2}(1.2)(100) = 60 J
  • Energy increase: 60โˆ’18=4260 - 18 = 42 J

Where does the extra 42 J come from? Internal work by the skater's muscles pulling her arms inward against the centripetal acceleration.

The Collapsing Star

When a massive star runs out of fuel, its core collapses from roughly the size of the Sun (Rโˆผ7ร—108R \sim 7 \times 10^8 m) to a neutron star (Rโˆผ104R \sim 10^4 m).

Before collapse

  • Ri=7ร—108R_i = 7 \times 10^8 m, rotation period Tiโ‰ˆ30T_i \approx 30 days

After collapse

  • Rf=104R_f = 10^4 m
  • IโˆMR2I \propto MR^2, so If/Ii=(Rf/Ri)2=(104/7ร—108)2โ‰ˆ2ร—10โˆ’10I_f/I_i = (R_f/R_i)^2 = (10^4/7 \times 10^8)^2 \approx 2 \times 10^{-10}

By conservation: ฯ‰f=(Ii/If)ฯ‰i\omega_f = (I_i/I_f)\omega_i

ฯ‰fโ‰ˆ5ร—109ร—ฯ‰i\omega_f \approx 5 \times 10^9 \times \omega_i

The period goes from ~30 days to milliseconds! This explains why pulsars (rotating neutron stars) spin incredibly fast.

Other Examples

  • Helicopter tail rotor: prevents the body from spinning (reaction to main rotor torque)
  • Cat righting reflex: cats change their body shape mid-air to reorient
  • Diver's tuck: pulling into a tuck position reduces II, increasing spin rate

Real-World Angular Momentum Quiz ๐ŸŽฏ

Application Calculations ๐Ÿงฎ

  1. A diver (I=14I = 14 kgโ‹…m2kg\cdot m^{2} extended) rotates at 2 rad/s. She tucks to I=3.5I = 3.5 kgโ‹…m2kg\cdot m^{2}. What is her angular velocity while tucked? (in rad/s)

  2. What is the ratio of her tucked KE to her extended KE?

  3. A merry-go-round (I=800I = 800 kgโ‹…m2kg\cdot m^{2}, ฯ‰=2\omega = 2 rad/s) has a 40 kg child (r=2r = 2 m from center) jump off tangentially. What is the new ฯ‰\omega? (in rad/s, round to 3 significant figures)

Real-World Review ๐Ÿ”

Exit Quiz โ€” Conservation Examples โœ…

Part 6: Problem-Solving Workshop

๐Ÿ› ๏ธ Problem-Solving Workshop

Part 6 of 7 โ€” Angular Momentum Practice

Time to work through challenging problems involving angular momentum, rotational dynamics, and energy.

Problem-Solving Strategy

  1. Identify the system and check for external torques
  2. If no external torque โ†’ use conservation of LL: Iiฯ‰i=Ifฯ‰fI_i\omega_i = I_f\omega_f
  3. If external torque exists โ†’ use ฯ„=Iฮฑ\tau = I\alpha or ฯ„=ฮ”L/ฮ”t\tau = \Delta L/\Delta t
  4. For energy questions โ†’ compute KE=12Iฯ‰2KE = \frac{1}{2}I\omega^2 before and after
  5. For rolling problems โ†’ remember v=Rฯ‰v = R\omega and total KE=12mv2+12Iฯ‰2KE = \frac{1}{2}mv^2 + \frac{1}{2}I\omega^2

Common AP Scenarios

  • Object drops onto rotating platform (inelastic collision)
  • Person walks on turntable
  • Object changes shape while spinning
  • Atwood machine with massive pulley

Workshop Problems โ€” Set 1 ๐ŸŽฏ

Workshop Calculations ๐Ÿงฎ

  1. A turntable (I=1.2I = 1.2 kgโ‹…m2kg\cdot m^{2}, ฯ‰=6\omega = 6 rad/s) has a ring (I=0.8I = 0.8 kgโ‹…m2kg\cdot m^{2}) dropped on it from rest. Find the final ฯ‰\omega. (in rad/s, round to 3 significant figures)

  2. How much kinetic energy is lost in the collision above? (in J, round to 3 significant figures)

  3. A 60 kg person stands on the edge of a 200 kg, 3 m radius turntable (uniform disk) initially at rest. The person begins walking at 1.5 m/s tangentially (relative to the ground). What is the turntable's angular velocity? (in rad/s, round to 3 significant figures)

Strategy Check ๐Ÿ”

Exit Quiz โ€” Workshop โœ…

Part 7: Synthesis & AP Review

๐ŸŽ“ Synthesis & AP Review

Part 7 of 7 โ€” Angular Momentum

Let's synthesize everything about angular momentum and tackle AP-level questions.

Complete Summary

Angular Momentum

L=Iฯ‰(rigidย body)L=mvr(pointย mass)L = I\omega \quad \text{(rigid body)} \qquad L = mvr \quad \text{(point mass)}

Newton's Second Law (Rotational)

ฯ„net=Iฮฑ=ฮ”Lฮ”t\tau_{\text{net}} = I\alpha = \frac{\Delta L}{\Delta t}

Rotational Kinetic Energy

KErot=12Iฯ‰2KE_{\text{rot}} = \frac{1}{2}I\omega^2

Conservation of Angular Momentum

Ifย ฯ„net,ย ext=0:Iiฯ‰i=Ifฯ‰f\text{If } \tau_{\text{net, ext}} = 0: \quad I_i\omega_i = I_f\omega_f

Key Relationships

  • LL conserved โ†” no external torque
  • When II decreases โ†’ ฯ‰\omega increases โ†’ KEKE increases (internal work done)
  • Rotational "collisions": I1ฯ‰1+I2ฯ‰2=(I1+I2)ฯ‰fI_1\omega_1 + I_2\omega_2 = (I_1 + I_2)\omega_f

AP-Style Questions โ€” Set 1 ๐ŸŽฏ

AP Calculation Practice ๐Ÿงฎ

  1. A solid cylinder (M=10M = 10 kg, R=0.2R = 0.2 m) starts from rest and a constant torque of 4 Nยทm is applied. What is its angular momentum after 5 seconds? (inkgโ‹…m2/s)(in kg\cdot m^{2}/s)

  2. A hoop (mass 2 kg, radius 0.5 m) rolls without slipping at 3 m/s. What is its total kinetic energy? (in J)

  3. A child (m=30m = 30 kg) runs at 4 m/s tangent to the edge of a stationary merry-go-round (uniform disk, M=100M = 100 kg, R=2R = 2 m) and jumps on. What is the final angular velocity? (in rad/s, round to 3 significant figures)

Comprehensive Review ๐Ÿ”

Final AP Review โœ