7.4 Conservation of Angular Momentum

7.4 Conservation of Angular Momentum The conservation of angular momentum states that if no external torque acts on a system, its total angular momentum remains constant. Angular momentum ( 𝐿 L) is defined as: 𝐿 = 𝐼 𝜔 L=Iω where 𝐼 I is the moment of inertia and 𝜔 ω is the angular velocity. When the moment of inertia changes, such as in figure skaters pulling their arms inward, the angular velocity adjusts to conserve 𝐿 L: 𝐿 initial = 𝐿 final or 𝐼 1 𝜔 1 = 𝐼 2 𝜔 2 L initial ​ =L final ​ orI 1 ​ ω 1 ​ =I 2 ​ ω 2 ​ This principle explains phenomena like spinning objects, planetary motion, and gyroscopic stability, highlighting the interplay between rotational inertia and angular velocity.

7.4 Conservation of Angular Momentum


Enduring Understanding 5.E

The angular momentum of a system is conserved.

Essential Knowledge

  • 5.E.1: If the net external torque exerted on a system is zero, the angular momentum of the system does not change.


Angular Momentum

Angular momentum is the rotational equivalent of linear momentum and is given by:

Where:

  • : Angular momentum (kg⋅m²/s).

  • : Moment of inertia (kg⋅m²).

  • : Angular velocity (rad/s).

Angular momentum is conserved when there are no net external torques acting on the system. This principle applies to various scenarios, such as spinning ice skaters and planetary motion.

7.4 Conservation of Angular Momentum


Example: Ice Skater

When a skater pulls their arms in, they reduce their moment of inertia . To conserve angular momentum, their angular velocity increases. Conversely, extending their arms increases , causing to decrease.

  • Initial State: Large , small .

  • Final State: Small , large .

This demonstrates how changes in mass distribution affect rotational speed while maintaining constant angular momentum.


Conservation in Planetary Motion

Angular momentum is conserved in planetary motion because planets move in closed orbits around the Sun. Kepler’s Second Law explains that planets sweep out equal areas in equal time intervals, maintaining constant angular velocity .

Key Points:

  • Linear Velocity vs Angular Velocity:

    • Linear velocity changes as a planet approaches or recedes from the Sun.

    • Angular velocity remains constant to conserve angular momentum.

  • Gravitational Influence:

    • Planets move faster when closer to the Sun (greater linear velocity).

    • Angular momentum is conserved despite these changes.


Example Problem: Rod and Disk System

Scenario: A disk of mass slides towards a rod (length , rotational inertia ) and sticks to it at a distance from the pivot. The system rotates after the collision.

Part (a): Derive Post-Collision Angular Speed

  1. Identify Equations:

    • Angular momentum of disk before collision: .

    • Angular momentum of rod-disk system after collision: .

  2. Set Conservation Statement:

  3. Solve for :


Part (b): Disk Bounces Off Rod

Question: Is the post-collision angular speed greater, less than, or equal to the speed when the disk sticks?

Answer: Greater than

Reasoning:

  • When the disk bounces off, it reverses direction, resulting in a greater change in angular momentum compared to when it sticks.

  • To conserve total angular momentum, the rod gains additional angular momentum.

  • Since and is constant, the increase in angular momentum causes an increase in .


Practice Problems

Problem 1:

A disk with mass 0.5 kg, radius 0.2 m, and angular velocity 4 rad/s. Calculate its angular momentum. ()

  • Solution:

  • Answer: 0.04 kg⋅m²/s

Problem 2:

A rod (length 1 m, mass 2 kg) rotates about its end. Find the angular momentum if . ()

  • Solution:

  • Answer: 2 kg⋅m²/s

Problem 3:

A skater reduces their radius by half while spinning. How does their angular velocity change?

  • Solution:

    • Initial angular momentum: .

    • Final moment of inertia: .

    • Since is constant: .

  • Answer: Angular velocity quadruples.

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