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7.4 Conservation of Angular Momentum

6 min readjanuary 29, 2023

Kashvi Panjolia

Kashvi Panjolia

Peter Apps

Peter Apps

Kashvi Panjolia

Kashvi Panjolia

Peter Apps

Peter Apps

Attend a live cram event

Review all units live with expert teachers & students

Enduring Understanding 5.E: The of a system is conserved.

Essential Knowledge 5.E.1: If the exerted on the system is zero, the of the system does not change.

Angular Momentum

is the rotational equivalent to linear momentum and is calculated by using the equation L=Iω, where I is the and ω is the . It is measured in units of kilogram meters squared per second (kgm^/s). is conserved when there are no net external torques on the object(s) in the system.

https://firebasestorage.googleapis.com/v0/b/fiveable-92889.appspot.com/o/images%2FScreen%20Shot%202020-04-14%20at%204.12.54%20PM.png?alt=media&token=fe2fbd8b-c493-4f07-b294-9051e03bf47f

Image courtesy of ScienceABC.

The skater above has a constant in both images. This means the overall of the skater does not change from the first image to the second. The skater pulling their hands in is an internal force (and therefore an internal torque), so is conserved. In terms of I and 𝜔, the first image has a large I and small 𝜔, since the skater's arms are extended outward, meaning more mass is distributed farther away from the axis of rotation, which goes through the center of the skater. If the skater has a higher , then the ω will have to be smaller.

In the second image, the skater has a smaller I and larger 𝜔. The skater has pulled their arms and legs in, so more mass is closer to the axis of rotation. In the equation for , I=MR^2, this means that the will be smaller than before because the radius (R) decreases while the amount of total mass (M) stays the same. If the is smaller, the will be larger to maintain constant . Therefore, the skater is spinning faster in the second image.

Other common situations with the involve collisions and planetary motion.

https://firebasestorage.googleapis.com/v0/b/fiveable-92889.appspot.com/o/images%2FScreen%20Shot%202020-04-14%20at%204.14.16%20PM.png?alt=media&token=12203a2d-719d-4d87-aec8-33e96f3abae3

is conserved in planetary motion because the planets are moving in closed orbits around the sun. A closed orbit is when the planet moves in a repeated pattern and returns to the same point in space after a certain period of time, such as a planet orbiting a star. The of the planet is constant, as the planet is not changing its shape or size, and the of the planet is also constant, as it is moving in a closed orbit.

The is constant because of , which states that planets sweep out equal areas (the purple regions in the image above) in equal amounts of time. In the purple region to the left, the planet still has the same as it does when it passes through the purple region to the right. The planet has a greater linear velocity on the left, since it is closer to the center of the orbit (the star), and the gravitational pull is stronger there. However, the faster is negated by the fact that the planet sweeps out a larger angle than in the purple region to the right. Since the time it takes to pass through the region is the same for both regions, the angular velocity of the planet is the same in both regions.

Note the difference between and . is the velocity that is directly related to distance and time, while is the velocity that relates to angle and time. tells us that the of the planet changes but does not change. Therefore, is conserved. You do not need to know about for the AP exam, but you do need to understand that the of a planet in a closed orbit is conserved.

EXAMPLE: (AP Classroom)

https://firebasestorage.googleapis.com/v0/b/fiveable-92889.appspot.com/o/images%2FScreen%20Shot%202020-04-14%20at%204.15.40%20PM.png?alt=media&token=3f705206-ca2b-492f-bd76-719585f12e1e

The left end of a rod of length d and I of the rod is attached to a frictionless horizontal surface by a frictionless pivot, as shown above. Point C marks the center (midpoint) of the rod. The rod is initially motionless but is free to rotate around the pivot. A student will slide a disk of mass:

https://firebasestorage.googleapis.com/v0/b/fiveable-92889.appspot.com/o/images%2FScreen%20Shot%202020-04-14%20at%204.00.27%20PM.png?alt=media&token=a3f4da7b-bab4-4cfa-bb23-9c47d72b2440

toward the rod with velocity v0 perpendicular to the rod, and the disk will stick to the rod a distance x from the pivot.

a. Immediately before colliding with the rod, the disk’s about the pivot is:

https://firebasestorage.googleapis.com/v0/b/fiveable-92889.appspot.com/o/images%2FScreen%20Shot%202020-04-14%20at%204.23.00%20PM.png?alt=media&token=0e7e8949-ac23-425b-8ddf-5bd8400bfd60

and its with respect to the pivot is:

https://firebasestorage.googleapis.com/v0/b/fiveable-92889.appspot.com/o/images%2FScreen%20Shot%202020-04-14%20at%204.23.48%20PM.png?alt=media&token=55ca9ff8-2d46-4a1f-b170-765f33ced406

Derive an equation for the ω of the rod. Express your answer in terms of d, mdisk, I, x, v0, and physical constants, as appropriate.

STEP 1: Identify applicable equations -

  • The question mentions and . We may also need because a collision is mentioned. can be calculated using L=Iω for the rod and L=mvr for the disk about the pivot point since the disk is moving in a straight-line motion.

https://firebasestorage.googleapis.com/v0/b/fiveable-92889.appspot.com/o/images%2FScreen%20Shot%202020-04-14%20at%204.25.57%20PM.png?alt=media&token=7e5d1d00-d1d2-486d-8c75-b6f79a77f5c4

STEP 2: Set up your . This statement is very similar to any other conservation statement you have written, such as for energy or linear momentum. Before the collision, the rod is at rest and the disk is the only object in the disk-rod system that is moving, so we only calculate the of the disk on the left side of the equation. After the collision, the disk sticks to the rod and both objects move together with a final ω, so we combine the for the two objects on the right. Now, we simply solve for ω by dividing both sides by the combined post-collision .

https://firebasestorage.googleapis.com/v0/b/fiveable-92889.appspot.com/o/images%2FScreen%20Shot%202020-04-14%20at%204.26.33%20PM.png?alt=media&token=cb640615-d025-4280-824b-e690b06e211f

Your answer should be:

https://firebasestorage.googleapis.com/v0/b/fiveable-92889.appspot.com/o/images%2FScreen%20Shot%202020-04-14%20at%204.27.07%20PM.png?alt=media&token=1d09ff51-3dda-456d-bad2-719ea7ddb188

b. Consider the collision for which your equation in part (a) was derived, except now suppose the disk bounces backward off the rod instead of sticking to the rod. Is the of the rod when the disk bounces off it greater than, less than, or equal to the of the rod when the disk sticks to it?

_____Greater than _____Less than _____Equal to

Briefly explain your reasoning.

CORRECT ANSWER: Greater than

REASONING: When the disk hits the rod, it transfers to the rod. This is an internal collision so is conserved before and after the collision. When the disk bounces off the rod, its changes from positive to negative. This is a larger change in its momentum than when it was brought to rest by sticking to the rod. Since the total momentum is constant, the rod must gain more to balance out the now negative momentum of the disk. Since the rod has more but the same , analyzing the equation L=Iω tells us that the of the rod must increase to create the increase in , so the final will be greater than the original final , when the disk stuck to the rod.

🎥Watch: AP Physics 1 - Unit 7 Streams

Key Terms to Review (13)

Angular momentum

: Angular momentum refers to the rotational equivalent of linear momentum. It describes how fast an object rotates around an axis and depends on its mass distribution and rotational speed.

Angular Speed

: Angular speed refers to how fast an object is rotating or spinning around a fixed axis. It is measured in radians per second (rad/s).

Angular Velocity

: Angular velocity refers to the rate at which an object rotates or moves in a circular path. It is measured in radians per second (rad/s).

Conservation of Angular Momentum

: The conservation of angular momentum states that the total angular momentum of a system remains constant if no external torques act on it. In other words, the spinning motion of an object will not change unless an external force is applied.

Conservation of Momentum

: Conservation of momentum states that in any closed system where no external forces act, the total momentum before an event equals the total momentum after the event. Momentum refers to mass in motion.

Kepler's 2nd Law

: Kepler's 2nd Law states that as a planet moves around its elliptical orbit, it sweeps out equal areas in equal time intervals. This means that planets move faster when they are closer to the Sun and slower when they are farther away.

L=Iω

: L=Iω represents the angular momentum of an object. It is equal to the moment of inertia (I) multiplied by the angular velocity (ω).

Linear Velocity

: Linear velocity refers to the rate at which an object changes its position in a straight line. It is calculated by dividing the change in displacement by the change in time.

Moment of Inertia

: Moment of inertia measures an object's resistance to changes in its rotational motion. It depends on both the mass distribution and the axis of rotation.

mvr (Momentum of a Point Mass)

: The momentum of a point mass, represented by mvr, is the product of an object's mass (m) and its velocity (v) in a specific direction. It quantifies the motion and impact of an object.

Net external torque

: Net external torque represents the sum total effect produced by all external torques acting on an object or system. It determines the rate at which an object's angular momentum changes.

Post-collision angular speed

: The post-collision angular speed refers to the rotational speed of an object after a collision or interaction with another object. It describes how fast an object is rotating after the collision has occurred.

Rotational Inertia

: Rotational inertia, also known as moment of inertia, is a measure of an object's resistance to changes in its rotational motion. It depends on both the mass and distribution of mass around the axis of rotation.

7.4 Conservation of Angular Momentum

6 min readjanuary 29, 2023

Kashvi Panjolia

Kashvi Panjolia

Peter Apps

Peter Apps

Kashvi Panjolia

Kashvi Panjolia

Peter Apps

Peter Apps

Attend a live cram event

Review all units live with expert teachers & students

Enduring Understanding 5.E: The of a system is conserved.

Essential Knowledge 5.E.1: If the exerted on the system is zero, the of the system does not change.

Angular Momentum

is the rotational equivalent to linear momentum and is calculated by using the equation L=Iω, where I is the and ω is the . It is measured in units of kilogram meters squared per second (kgm^/s). is conserved when there are no net external torques on the object(s) in the system.

https://firebasestorage.googleapis.com/v0/b/fiveable-92889.appspot.com/o/images%2FScreen%20Shot%202020-04-14%20at%204.12.54%20PM.png?alt=media&token=fe2fbd8b-c493-4f07-b294-9051e03bf47f

Image courtesy of ScienceABC.

The skater above has a constant in both images. This means the overall of the skater does not change from the first image to the second. The skater pulling their hands in is an internal force (and therefore an internal torque), so is conserved. In terms of I and 𝜔, the first image has a large I and small 𝜔, since the skater's arms are extended outward, meaning more mass is distributed farther away from the axis of rotation, which goes through the center of the skater. If the skater has a higher , then the ω will have to be smaller.

In the second image, the skater has a smaller I and larger 𝜔. The skater has pulled their arms and legs in, so more mass is closer to the axis of rotation. In the equation for , I=MR^2, this means that the will be smaller than before because the radius (R) decreases while the amount of total mass (M) stays the same. If the is smaller, the will be larger to maintain constant . Therefore, the skater is spinning faster in the second image.

Other common situations with the involve collisions and planetary motion.

https://firebasestorage.googleapis.com/v0/b/fiveable-92889.appspot.com/o/images%2FScreen%20Shot%202020-04-14%20at%204.14.16%20PM.png?alt=media&token=12203a2d-719d-4d87-aec8-33e96f3abae3

is conserved in planetary motion because the planets are moving in closed orbits around the sun. A closed orbit is when the planet moves in a repeated pattern and returns to the same point in space after a certain period of time, such as a planet orbiting a star. The of the planet is constant, as the planet is not changing its shape or size, and the of the planet is also constant, as it is moving in a closed orbit.

The is constant because of , which states that planets sweep out equal areas (the purple regions in the image above) in equal amounts of time. In the purple region to the left, the planet still has the same as it does when it passes through the purple region to the right. The planet has a greater linear velocity on the left, since it is closer to the center of the orbit (the star), and the gravitational pull is stronger there. However, the faster is negated by the fact that the planet sweeps out a larger angle than in the purple region to the right. Since the time it takes to pass through the region is the same for both regions, the angular velocity of the planet is the same in both regions.

Note the difference between and . is the velocity that is directly related to distance and time, while is the velocity that relates to angle and time. tells us that the of the planet changes but does not change. Therefore, is conserved. You do not need to know about for the AP exam, but you do need to understand that the of a planet in a closed orbit is conserved.

EXAMPLE: (AP Classroom)

https://firebasestorage.googleapis.com/v0/b/fiveable-92889.appspot.com/o/images%2FScreen%20Shot%202020-04-14%20at%204.15.40%20PM.png?alt=media&token=3f705206-ca2b-492f-bd76-719585f12e1e

The left end of a rod of length d and I of the rod is attached to a frictionless horizontal surface by a frictionless pivot, as shown above. Point C marks the center (midpoint) of the rod. The rod is initially motionless but is free to rotate around the pivot. A student will slide a disk of mass:

https://firebasestorage.googleapis.com/v0/b/fiveable-92889.appspot.com/o/images%2FScreen%20Shot%202020-04-14%20at%204.00.27%20PM.png?alt=media&token=a3f4da7b-bab4-4cfa-bb23-9c47d72b2440

toward the rod with velocity v0 perpendicular to the rod, and the disk will stick to the rod a distance x from the pivot.

a. Immediately before colliding with the rod, the disk’s about the pivot is:

https://firebasestorage.googleapis.com/v0/b/fiveable-92889.appspot.com/o/images%2FScreen%20Shot%202020-04-14%20at%204.23.00%20PM.png?alt=media&token=0e7e8949-ac23-425b-8ddf-5bd8400bfd60

and its with respect to the pivot is:

https://firebasestorage.googleapis.com/v0/b/fiveable-92889.appspot.com/o/images%2FScreen%20Shot%202020-04-14%20at%204.23.48%20PM.png?alt=media&token=55ca9ff8-2d46-4a1f-b170-765f33ced406

Derive an equation for the ω of the rod. Express your answer in terms of d, mdisk, I, x, v0, and physical constants, as appropriate.

STEP 1: Identify applicable equations -

  • The question mentions and . We may also need because a collision is mentioned. can be calculated using L=Iω for the rod and L=mvr for the disk about the pivot point since the disk is moving in a straight-line motion.

https://firebasestorage.googleapis.com/v0/b/fiveable-92889.appspot.com/o/images%2FScreen%20Shot%202020-04-14%20at%204.25.57%20PM.png?alt=media&token=7e5d1d00-d1d2-486d-8c75-b6f79a77f5c4

STEP 2: Set up your . This statement is very similar to any other conservation statement you have written, such as for energy or linear momentum. Before the collision, the rod is at rest and the disk is the only object in the disk-rod system that is moving, so we only calculate the of the disk on the left side of the equation. After the collision, the disk sticks to the rod and both objects move together with a final ω, so we combine the for the two objects on the right. Now, we simply solve for ω by dividing both sides by the combined post-collision .

https://firebasestorage.googleapis.com/v0/b/fiveable-92889.appspot.com/o/images%2FScreen%20Shot%202020-04-14%20at%204.26.33%20PM.png?alt=media&token=cb640615-d025-4280-824b-e690b06e211f

Your answer should be:

https://firebasestorage.googleapis.com/v0/b/fiveable-92889.appspot.com/o/images%2FScreen%20Shot%202020-04-14%20at%204.27.07%20PM.png?alt=media&token=1d09ff51-3dda-456d-bad2-719ea7ddb188

b. Consider the collision for which your equation in part (a) was derived, except now suppose the disk bounces backward off the rod instead of sticking to the rod. Is the of the rod when the disk bounces off it greater than, less than, or equal to the of the rod when the disk sticks to it?

_____Greater than _____Less than _____Equal to

Briefly explain your reasoning.

CORRECT ANSWER: Greater than

REASONING: When the disk hits the rod, it transfers to the rod. This is an internal collision so is conserved before and after the collision. When the disk bounces off the rod, its changes from positive to negative. This is a larger change in its momentum than when it was brought to rest by sticking to the rod. Since the total momentum is constant, the rod must gain more to balance out the now negative momentum of the disk. Since the rod has more but the same , analyzing the equation L=Iω tells us that the of the rod must increase to create the increase in , so the final will be greater than the original final , when the disk stuck to the rod.

🎥Watch: AP Physics 1 - Unit 7 Streams

Key Terms to Review (13)

Angular momentum

: Angular momentum refers to the rotational equivalent of linear momentum. It describes how fast an object rotates around an axis and depends on its mass distribution and rotational speed.

Angular Speed

: Angular speed refers to how fast an object is rotating or spinning around a fixed axis. It is measured in radians per second (rad/s).

Angular Velocity

: Angular velocity refers to the rate at which an object rotates or moves in a circular path. It is measured in radians per second (rad/s).

Conservation of Angular Momentum

: The conservation of angular momentum states that the total angular momentum of a system remains constant if no external torques act on it. In other words, the spinning motion of an object will not change unless an external force is applied.

Conservation of Momentum

: Conservation of momentum states that in any closed system where no external forces act, the total momentum before an event equals the total momentum after the event. Momentum refers to mass in motion.

Kepler's 2nd Law

: Kepler's 2nd Law states that as a planet moves around its elliptical orbit, it sweeps out equal areas in equal time intervals. This means that planets move faster when they are closer to the Sun and slower when they are farther away.

L=Iω

: L=Iω represents the angular momentum of an object. It is equal to the moment of inertia (I) multiplied by the angular velocity (ω).

Linear Velocity

: Linear velocity refers to the rate at which an object changes its position in a straight line. It is calculated by dividing the change in displacement by the change in time.

Moment of Inertia

: Moment of inertia measures an object's resistance to changes in its rotational motion. It depends on both the mass distribution and the axis of rotation.

mvr (Momentum of a Point Mass)

: The momentum of a point mass, represented by mvr, is the product of an object's mass (m) and its velocity (v) in a specific direction. It quantifies the motion and impact of an object.

Net external torque

: Net external torque represents the sum total effect produced by all external torques acting on an object or system. It determines the rate at which an object's angular momentum changes.

Post-collision angular speed

: The post-collision angular speed refers to the rotational speed of an object after a collision or interaction with another object. It describes how fast an object is rotating after the collision has occurred.

Rotational Inertia

: Rotational inertia, also known as moment of inertia, is a measure of an object's resistance to changes in its rotational motion. It depends on both the mass and distribution of mass around the axis of rotation.


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AP® and SAT® are trademarks registered by the College Board, which is not affiliated with, and does not endorse this website.


© 2024 Fiveable Inc. All rights reserved.

AP® and SAT® are trademarks registered by the College Board, which is not affiliated with, and does not endorse this website.