If you're seeing this message, it means we're having trouble loading external resources on our website.

If you're behind a web filter, please make sure that the domains *.kastatic.org and *.kasandbox.org are unblocked.

## High school physics

### Course: High school physics>Unit 7

Lesson 7: Conservation of angular momentum

# Conservation of angular momentum review

Review how angular momentum is conserved if there is no external torque applied to a system.  Specific scenarios are highlighted: system changing it rotational inertia, orbiting bodies, and rotational collisions.

## Key terms

Term (symbol)Meaning
Conservation of angular momentumAngular momentum is constant for a system with no net external torque.

## Equations

EquationSymbol breakdownMeaning in words
${L}_{i}={L}_{f}$${L}_{i}$ and ${L}_{f}$ are the total initial and final angular momentum.Total initial angular momentum equals the total final angular momentum for a system with no net external torque. Commonly called the conservation of angular momentum.

## Applying the conservation of angular momentum

### Objects can change their shape and still conserve angular momentum

Angular momentum depends on the rotational velocity of an object, but also its rotational inertia. When an object changes its shape (rotational inertia), its angular velocity will also change if there is no external torque.
An example is when an ice skater spins and changes her rotation velocity by holding her arms outwards or pulling them inwards (see Figure 1 below).
When she pulls her arms in, her rotational inertia is reduced. Since there is no external net torque on the ice skater, her angular momentum remains constant because her angular velocity magnitude increases.

### Orbital systems such as our solar system have angular momentum conserved

A system of planets orbiting a star has no net external torque, so its angular momentum is constant. As a planet travels along an elliptical orbit, its speed reduces when it is further away from the star, and increases its speed as it approaches the star as seen in Figure 2.
This keeps the angular momentum about the star constant by adjusting the variables of $v$ and $r$ for the angular momentum equation below:
$L=mvr$
This scenario of orbiting objects is discussed with more detail in the next lesson.

### Rotational collisions conserve angular momentum

When objects collide without a net external torque, the angular momentum is constant. The two objects exert equal, but opposite angular impulses upon each other to maintain the total angular momentum of the colliding system. An example of this would be a ball colliding with a stick that rotates about its end as shown in Figure 3.