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5 min read•june 18, 2024
Peter Apps
Kashvi Panjolia
Peter Apps
Kashvi Panjolia
Enduring Understanding 5.E: The angular momentum of a system is conserved.
Essential Knowledge 5.E.1: If the net external torque exerted on the system is zero, the angular momentum 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 moment of inertia and ω is the angular velocity. It is measured in units of kilogram meters squared per second (kgm^/s). Angular momentum is conserved when there are no net external torques on the object(s) in the system.
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 moment of inertia, I=MR^2, this means that the moment of inertia will be smaller than before because the radius (R) decreases while the amount of total mass (M) stays the same. If the rotational inertia is smaller, the angular velocity will be larger to maintain constant angular momentum. Therefore, the skater is spinning faster in the second image.
Other common situations with the conservation of angular momentum involve collisions and planetary motion.
The angular velocity is constant because of Kepler's 2nd Law, 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 angular velocity 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 linear velocity 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 linear velocity and angular velocity. Linear velocity is the velocity that is directly related to distance and time, while angular velocity is the velocity that relates to angle and time. Kepler's 2nd Law tells us that the linear velocity of the planet changes but angular velocity does not change. Therefore, angular momentum is conserved. You do not need to know about Kepler's 2nd Law for the AP exam, but you do need to understand that the angular momentum of a planet in a closed orbit is conserved.
a. Immediately before colliding with the rod, the disk’s rotational inertia about the pivot is:
STEP 1: Identify applicable equations -
_____Greater than _____Less than _____Equal to
Briefly explain your reasoning.
CORRECT ANSWER: Greater than
REASONING: When the disk hits the rod, it transfers angular momentum to the rod. This is an internal collision so angular momentum is conserved before and after the collision. When the disk bounces off the rod, its angular momentum 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 angular momentum to balance out the now negative momentum of the disk. Since the rod has more angular momentum but the same moment of inertia, analyzing the equation L=Iω tells us that the angular velocity of the rod must increase to create the increase in angular momentum, so the final angular velocity will be greater than the original final angular velocity, when the disk stuck to the rod.
🎥Watch: AP Physics 1 - Unit 7 Streams
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5 min read•june 18, 2024
Peter Apps
Kashvi Panjolia
Peter Apps
Kashvi Panjolia
Enduring Understanding 5.E: The angular momentum of a system is conserved.
Essential Knowledge 5.E.1: If the net external torque exerted on the system is zero, the angular momentum 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 moment of inertia and ω is the angular velocity. It is measured in units of kilogram meters squared per second (kgm^/s). Angular momentum is conserved when there are no net external torques on the object(s) in the system.
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 moment of inertia, I=MR^2, this means that the moment of inertia will be smaller than before because the radius (R) decreases while the amount of total mass (M) stays the same. If the rotational inertia is smaller, the angular velocity will be larger to maintain constant angular momentum. Therefore, the skater is spinning faster in the second image.
Other common situations with the conservation of angular momentum involve collisions and planetary motion.
The angular velocity is constant because of Kepler's 2nd Law, 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 angular velocity 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 linear velocity 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 linear velocity and angular velocity. Linear velocity is the velocity that is directly related to distance and time, while angular velocity is the velocity that relates to angle and time. Kepler's 2nd Law tells us that the linear velocity of the planet changes but angular velocity does not change. Therefore, angular momentum is conserved. You do not need to know about Kepler's 2nd Law for the AP exam, but you do need to understand that the angular momentum of a planet in a closed orbit is conserved.
a. Immediately before colliding with the rod, the disk’s rotational inertia about the pivot is:
STEP 1: Identify applicable equations -
_____Greater than _____Less than _____Equal to
Briefly explain your reasoning.
CORRECT ANSWER: Greater than
REASONING: When the disk hits the rod, it transfers angular momentum to the rod. This is an internal collision so angular momentum is conserved before and after the collision. When the disk bounces off the rod, its angular momentum 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 angular momentum to balance out the now negative momentum of the disk. Since the rod has more angular momentum but the same moment of inertia, analyzing the equation L=Iω tells us that the angular velocity of the rod must increase to create the increase in angular momentum, so the final angular velocity will be greater than the original final angular velocity, when the disk stuck to the rod.
🎥Watch: AP Physics 1 - Unit 7 Streams
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