AP Physics 1 Unit 6: Energy and Momentum in Rotating Systems
Rotational inertia and rotational kinetic energy
Rotational motion has its own “inertia” and its own form of kinetic energy. You already know how a mass resists changes in its translational motion and how its kinetic energy depends on speed. For rotation, the same ideas apply—but where the mass is located relative to the axis becomes just as important as how much mass there is.
Moment of inertia: the rotational version of mass
Moment of inertia (also called rotational inertia) measures how strongly an object resists changes in its rotational motion about a chosen axis. The key idea is that mass farther from the axis contributes much more to rotational inertia than mass close to the axis.
For a set of point masses, the moment of inertia about a specific axis is
I = \sum m r^2
- I is the moment of inertia about the axis (units: \text{kg}\cdot\text{m}^2).
- m is the mass of a particle.
- r is that particle’s perpendicular distance from the axis.
That r^2 is the whole story: doubling the distance from the axis makes the contribution four times larger. This is why a figure skater’s arms matter so much—mass moved outward drastically increases I.
For continuous objects (disks, rods, spheres), you typically use known formulas rather than doing calculus in AP Physics 1.
Common moments of inertia you are expected to use
These are about axes through the center of mass unless stated otherwise:
| Object | Axis | Moment of inertia I |
|---|---|---|
| Thin hoop (ring) radius R | center, perpendicular to plane | MR^2 |
| Solid disk/cylinder radius R | center, perpendicular to plane | \frac{1}{2}MR^2 |
| Solid sphere radius R | through center | \frac{2}{5}MR^2 |
| Thin rod length L | through center, perpendicular to rod | \frac{1}{12}ML^2 |
| Thin rod length L | about one end, perpendicular to rod | \frac{1}{3}ML^2 |
A common conceptual check: the hoop has a larger I than the disk for the same M and R because more of its mass is at the outer edge.
Changing the axis: the parallel-axis theorem
In real problems, the axis of rotation is often not through the center of mass (a rod pivoted at one end, a disk rotating about an off-center axle). The parallel-axis theorem lets you shift from a center-of-mass axis to a parallel axis a distance d away:
I = I_{cm} + Md^2
- I_{cm} is the moment of inertia about an axis through the center of mass.
- d is the perpendicular distance between axes.
Why it makes sense: shifting the axis makes every bit of mass, on average, farther from the axis—so I must increase.
Rotational kinetic energy
Just as translational kinetic energy is energy of motion due to speed, rotational kinetic energy is energy of motion due to angular speed.
For an object rotating with angular speed \omega about a fixed axis:
K_{rot} = \frac{1}{2}I\omega^2
- K_{rot} is rotational kinetic energy (joules).
- I depends on mass distribution and chosen axis.
- \omega is angular speed in \text{rad/s}.
This mirrors translational kinetic energy:
K_{trans} = \frac{1}{2}mv^2
The analogy is powerful:
- mass m corresponds to moment of inertia I
- speed v corresponds to angular speed \omega
Total kinetic energy for rolling or combined motion
Many rotating-system problems involve objects that both translate and rotate (a rolling wheel, a yo-yo, a bowling ball). In those cases, the total kinetic energy is
K_{total} = \frac{1}{2}Mv_{cm}^2 + \frac{1}{2}I_{cm}\omega^2
Notice the rotational part uses I_{cm} (about the center of mass), not necessarily the moment of inertia about the ground contact point.
Worked example: comparing rotational kinetic energies
Situation: A hoop and a solid disk have the same mass M and radius R. They rotate about their centers with the same angular speed \omega. Which has more rotational kinetic energy?
Reasoning: Since K_{rot} = \frac{1}{2}I\omega^2, the one with larger I has larger K_{rot}.
- Hoop: I = MR^2
- Disk: I = \frac{1}{2}MR^2
So
K_{hoop} = \frac{1}{2}(MR^2)\omega^2
K_{disk} = \frac{1}{2}\left(\frac{1}{2}MR^2\right)\omega^2 = \frac{1}{4}MR^2\omega^2
The hoop has twice the rotational kinetic energy at the same \omega.
What commonly goes wrong here
A frequent mistake is thinking “same mass and same radius means same rotational inertia.” The distribution matters: putting mass at larger radius increases I a lot.
Another common issue is mixing up which axis the given I formula uses. A rod about its center and a rod about its end differ by a factor of 4.
Exam Focus
- Typical question patterns:
- Compare speeds or energies of different rolling objects using their different I values.
- Choose the correct moment of inertia expression for a given axis (center vs end vs shifted).
- Use energy methods with K_{rot} = \frac{1}{2}I\omega^2.
- Common mistakes:
- Using the wrong axis for I (forgetting the pivot is not at the center).
- Treating a hoop and a disk as if they have the same I.
- Forgetting total kinetic energy can include both translation and rotation.
Work, torque, and power in rotational motion
Energy methods become especially useful in rotating systems because forces and torques can vary in time and because rotational plus translational energy can be conserved even when forces look complicated.
Work in rotation: connecting torque to energy
In translation, work is
W = F\Delta x
In rotation, the analogous statement is: a torque does work when it causes angular displacement. For constant torque aligned with the rotation,
W = \tau\Delta\theta
- \tau is torque about the axis.
- \Delta\theta is angular displacement in radians.
This formula is not magic—it comes from the translational idea. A tangential force applied at radius r gives torque \tau = rF (for perpendicular force), and the point of application moves along an arc length s = r\Delta\theta. Then
W = Fs = F(r\Delta\theta) = (rF)\Delta\theta = \tau\Delta\theta
Rotational work-energy theorem
The rotational version of the work-energy theorem is
W_{net} = \Delta K_{rot}
and since K_{rot} = \frac{1}{2}I\omega^2,
W_{net} = \frac{1}{2}I\omega_f^2 - \frac{1}{2}I\omega_i^2
This is especially useful for rotating machinery, pulleys, and any situation where torque acts through an angle.
Power in rotational motion
Power is the rate at which work is done. Rotational power is
P = \tau\omega
This is the rotational analog of P = Fv. It helps you reason about engines and motors: for a given power output, higher angular speed means lower torque and vice versa.
Worked example: torque doing work to spin up a disk
Situation: A solid disk with moment of inertia I = \frac{1}{2}MR^2 starts from rest. A constant torque \tau is applied through an angular displacement \Delta\theta. Find its final angular speed.
Step 1: Use work from torque
W = \tau\Delta\theta
Step 2: Work becomes rotational kinetic energy
\tau\Delta\theta = \Delta K_{rot} = \frac{1}{2}I\omega^2 - 0
Step 3: Solve for \omega
\omega = \sqrt{\frac{2\tau\Delta\theta}{I}}
If you substitute I = \frac{1}{2}MR^2, you get
\omega = \sqrt{\frac{4\tau\Delta\theta}{MR^2}}
Common conceptual pitfall: confusing torque with work
Torque is not energy. A large torque applied through a tiny angle can do little work, while a modest torque applied through many revolutions can do lots of work. On exams, this shows up when students try to compare “how much work” based only on torque values.
Exam Focus
- Typical question patterns:
- Use W = \tau\Delta\theta and \Delta K_{rot} to find final \omega after a torque acts.
- Relate motor power to torque and angular speed using P = \tau\omega.
- Combine rotational work-energy with translational work-energy when an object both rotates and translates.
- Common mistakes:
- Using degrees instead of radians in W = \tau\Delta\theta.
- Treating torque as if it automatically means high energy without considering angular displacement.
- Forgetting that the net work relates to change in kinetic energy (not the work from just one torque if multiple act).
Angular momentum and rotational impulse
Energy tells you about “how much motion” in a scalar sense, but momentum is often the better tool when interactions are short, impulsive, or involve rotation about a pivot. For rotating systems, that tool is angular momentum.
What angular momentum is (and what it measures)
Angular momentum measures how much rotational motion something has about a chosen axis, and how hard it is to change that rotational motion.
For a rigid object rotating about a fixed axis,
L = I\omega
- L is angular momentum about the axis.
This looks like the translational momentum formula p = mv. The analogy continues:
- m corresponds to I
- v corresponds to \omega
- p corresponds to L
For a particle moving past an axis, angular momentum depends on the “lever arm”:
L = mvr
This scalar form applies when the motion is perpendicular and you’re focusing on magnitude about a point/axis. More generally, angular momentum is a vector and depends on direction, but AP Physics 1 usually emphasizes the right-hand rule and sign conventions qualitatively rather than full vector algebra.
Why the choice of axis matters
Angular momentum is always “about something.” The same object can have different angular momentum values depending on which axis you choose.
- A spinning disk has a clear axis through its center.
- A moving particle has angular momentum about an axis if its line of motion does not pass through the axis.
On exam problems, the “best” axis is usually the pivot point or a point where external torques vanish (so you can use conservation).
Torque is the cause of changes in angular momentum
In translation, net force changes momentum:
F_{net} = \frac{\Delta p}{\Delta t}
In rotation, net torque changes angular momentum:
\tau_{net} = \frac{\Delta L}{\Delta t}
If net torque is constant over a time interval,
\Delta L = \tau_{net}\Delta t
This is the rotational analog of the impulse-momentum theorem. The quantity \tau\Delta t is called angular impulse.
Connecting torque, angular acceleration, and angular momentum
If the moment of inertia is constant (rigid object about a fixed axis), then combining L = I\omega with \tau_{net} = \frac{\Delta L}{\Delta t} gives
\tau_{net} = I\alpha
This is the rotational analog of F_{net} = ma.
A subtle but important point: \tau_{net} = I\alpha assumes I is constant. In some conservation problems (like a skater pulling in arms), I changes, and then it’s better to use conservation of L than torque-acceleration.
Worked example: angular impulse from a brief torque
Situation: A wheel has moment of inertia I and initially rotates at \omega_i. A brake applies a constant opposing torque of magnitude \tau for time \Delta t. Find the final angular speed.
Step 1: Write the angular impulse-momentum relation
\Delta L = \tau_{net}\Delta t
If the torque opposes rotation, it is negative in your sign convention. Using magnitudes with a sign choice:
I\omega_f - I\omega_i = -\tau\Delta t
Step 2: Solve
\omega_f = \omega_i - \frac{\tau\Delta t}{I}
This mirrors the translational result v_f = v_i - \frac{F\Delta t}{m}.
Common misconception: “torque causes rotation”
More precisely, net torque causes changes in rotational motion. If an object is rotating at constant angular speed and net torque is zero, it keeps rotating (Newton’s first law in rotational form). Students often look for a torque any time something is spinning, but steady rotation does not require a torque.
Exam Focus
- Typical question patterns:
- Use L = I\omega for a rigid object and relate changes in L to applied torque over time.
- Choose an axis to make external torque zero, then apply conservation of angular momentum.
- Compare angular momentum before and after an impulsive interaction (hit, grab, collision).
- Common mistakes:
- Using \tau = I\alpha in situations where I changes (skater pulling arms in).
- Forgetting that angular momentum depends on the chosen axis.
- Dropping sign conventions: clockwise vs counterclockwise matters for L and \tau.
Conservation of angular momentum in rotating systems
Conservation laws are powerful because they let you predict motion without tracking every force in detail. Angular momentum is conserved when the net external torque on a system is zero (or negligible) about the chosen axis.
The conservation principle
If
\tau_{ext,net} = 0
then
L_i = L_f
This can apply to:
- a person changing body configuration on a frictionless turntable
- a collapsing star spinning faster as it shrinks
- collisions where external torques about a pivot are negligible during a short interaction
Why “about the chosen axis” is not just a detail
A system can have zero external torque about one axis but not about another. On AP problems with a pivot, the pivot point is often the best axis because the external force from the pivot passes through the pivot, producing zero torque about that point.
That’s not because the pivot force is small—it can be huge. It’s because its lever arm about the pivot is zero.
Configuration changes: the skater effect
A classic conservation-of-angular-momentum scenario is a rotating person pulling arms in.
- Pulling arms in decreases I.
- If external torque is negligible, L = I\omega stays constant.
- Therefore \omega must increase.
Mathematically,
I_i\omega_i = I_f\omega_f
so
\omega_f = \frac{I_i}{I_f}\omega_i
If I_f is smaller, \omega_f is larger.
Energy is not necessarily conserved in this process. The person does internal work (muscles) to pull arms inward, often increasing rotational kinetic energy:
K_{rot} = \frac{1}{2}I\omega^2
Even though L stays constant, K_{rot} can change.
Worked example: turntable and person
Situation: A person stands on a frictionless rotating platform. Initially, the person and platform rotate together at \omega_i with total moment of inertia I_i. The person pulls their arms in, reducing the total moment of inertia to I_f. Find \omega_f and compare kinetic energies.
Step 1: Conserve angular momentum
I_i\omega_i = I_f\omega_f
\omega_f = \frac{I_i}{I_f}\omega_i
Step 2: Compare rotational kinetic energies
Initial:
K_i = \frac{1}{2}I_i\omega_i^2
Final (substitute \omega_f):
K_f = \frac{1}{2}I_f\left(\frac{I_i}{I_f}\omega_i\right)^2 = \frac{1}{2}\frac{I_i^2}{I_f}\omega_i^2
Because I_f < I_i, you get K_f > K_i. The extra energy comes from internal work done by the person.
Collisions and sticking: when energy is not conserved but angular momentum may be
A big AP Physics 1 theme is: momentum-like quantities can be conserved in collisions even when kinetic energy is not.
For rotational collisions, the same idea applies.
If two objects interact briefly and the net external torque about your axis is negligible during that short time, then angular momentum about that axis is conserved:
L_i = L_f
But if they stick together or deform, kinetic energy is typically not conserved.
Worked example: a putty ball hits a rotating disk
Situation: A disk of moment of inertia I_d rotates at \omega_i. A small lump of putty of mass m is dropped onto the disk and sticks at radius r from the center. Assume negligible external torque about the disk axis. Find the new angular speed.
Step 1: Compute initial angular momentum
Putty is dropped vertically (no initial angular momentum about the axis if dropped straight down with no tangential component), so
L_i = I_d\omega_i
Step 2: Compute final moment of inertia
The putty acts like a point mass at radius r:
I_{putty} = mr^2
Total final moment of inertia:
I_f = I_d + mr^2
Step 3: Conserve angular momentum
I_d\omega_i = (I_d + mr^2)\omega_f
\omega_f = \frac{I_d}{I_d + mr^2}\omega_i
The rotation slows because I increased.
What goes wrong: mixing conservation laws incorrectly
A very common error is to conserve rotational kinetic energy in sticking collisions. If objects stick, mechanical energy is usually not conserved because some energy becomes thermal, sound, or deformation.
Another error is to conserve angular momentum when there is a significant external torque about the chosen axis (for instance, friction from the ground on a system that is not symmetric, or a pivot that is not the axis you’re taking moments about).
Exam Focus
- Typical question patterns:
- Configuration change (skater, collapsing object): use I_i\omega_i = I_f\omega_f.
- Rotational “stick” collision: conserve L about the axis, then compute \omega_f.
- Identify when angular momentum is conserved by analyzing external torque about a chosen point.
- Common mistakes:
- Assuming kinetic energy is conserved in inelastic rotational interactions.
- Conserving L about the wrong axis (choosing an axis where external torques are not zero).
- Forgetting to include the added mr^2 contribution to I_f for a stuck mass.
Rolling motion: linking rotation and translation
Rolling is where Unit 6 often feels most “real world.” Wheels, balls, cylinders—many objects both translate and rotate. The key is learning when you can connect linear and angular quantities, and when friction does (and does not) remove mechanical energy.
Rolling without slipping: the no-slip condition
Rolling without slipping means the point of contact between the object and the surface is instantaneously at rest relative to the surface.
That requirement creates a simple relationship between the center-of-mass speed v_{cm} and angular speed \omega for an object of radius R:
v_{cm} = \omega R
Similarly, for accelerations (when rolling without slipping is maintained):
a_{cm} = \alpha R
These relationships are constraints, not general truths for all rotation. They only apply when rolling without slipping is actually happening.
Why static friction is involved (and why it might do zero work)
Rolling without slipping typically requires static friction, not kinetic friction. Static friction prevents slipping and provides whatever tangential force is needed to enforce v_{cm} = \omega R.
A subtle point that AP Physics 1 loves: in ideal rolling without slipping on a rigid surface, static friction often does no net work on the rolling object because the point of contact does not slide. Energy can still convert between gravitational potential and kinetic forms, but friction is not necessarily dissipating it.
However, static friction can still be essential dynamically—it can be the only horizontal force producing translational acceleration and the only torque producing angular acceleration.
Total kinetic energy of a rolling object
If an object rolls without slipping, it has both translational and rotational kinetic energy:
K_{total} = \frac{1}{2}Mv_{cm}^2 + \frac{1}{2}I_{cm}\omega^2
Using v_{cm} = \omega R, you can express everything in terms of v_{cm}:
K_{total} = \frac{1}{2}Mv_{cm}^2 + \frac{1}{2}I_{cm}\left(\frac{v_{cm}}{R}\right)^2
This makes it clear: for the same center-of-mass speed, an object with larger I_{cm} “stores” more energy in rotation.
Rolling down an incline: who gets to the bottom first?
When objects roll down a ramp without slipping, they accelerate because gravity converts potential energy into kinetic energy. If energy is conserved (no dissipative losses), you can use
Mgh = \frac{1}{2}Mv^2 + \frac{1}{2}I_{cm}\left(\frac{v}{R}\right)^2
Solving for v gives
v = \sqrt{\frac{2gh}{1 + \frac{I_{cm}}{MR^2}}}
This result is extremely useful conceptually:
- If \frac{I_{cm}}{MR^2} is larger, the denominator is larger, so v is smaller.
- So objects with more rotational inertia relative to MR^2 roll down more slowly.
That’s why, for the same M and R, a solid sphere (smaller I_{cm} factor) beats a hoop (larger factor).
Worked example: disk vs hoop rolling down the same height
Situation: A hoop and a solid disk start from rest and roll without slipping down from the same vertical height h. Find the ratio of their final speeds.
Use
v = \sqrt{\frac{2gh}{1 + \frac{I_{cm}}{MR^2}}}
- Hoop: I_{cm} = MR^2, so \frac{I_{cm}}{MR^2} = 1
v_{hoop} = \sqrt{\frac{2gh}{2}} = \sqrt{gh}
- Disk: I_{cm} = \frac{1}{2}MR^2, so \frac{I_{cm}}{MR^2} = \frac{1}{2}
v_{disk} = \sqrt{\frac{2gh}{1 + \frac{1}{2}}} = \sqrt{\frac{2gh}{\frac{3}{2}}} = \sqrt{\frac{4gh}{3}}
Now ratio:
\frac{v_{disk}}{v_{hoop}} = \frac{\sqrt{\frac{4gh}{3}}}{\sqrt{gh}} = \sqrt{\frac{4}{3}}
The disk is faster.
When mechanical energy is not conserved in rolling
Energy conservation works beautifully for ideal rolling without slipping on a rigid surface. But you must be cautious in two common situations:
- Rolling with slipping: kinetic friction does negative work and dissipates mechanical energy.
- Deformable surfaces (soft tires, carpet): rolling resistance can convert mechanical energy to thermal energy even without obvious slipping.
In AP problems, you’re typically told or can assume whether to ignore these losses.
Exam Focus
- Typical question patterns:
- Rolling down an incline: use energy conservation with both translational and rotational kinetic energy.
- Compare final speeds/accelerations of different objects using different I_{cm} values.
- Identify whether friction is static or kinetic and what that implies about energy.
- Common mistakes:
- Using v = \omega R when the object is slipping.
- Assuming friction always removes mechanical energy (static friction in ideal rolling often does no net work).
- Forgetting the rotational kinetic energy term and treating rolling objects like sliding blocks.
Using energy and angular momentum together in multi-step rotation problems
The toughest Unit 6 problems often require you to decide which principle applies in which time interval. A very common structure is:
- Step A: A brief interaction where external torque is negligible → conserve angular momentum.
- Step B: A longer motion with gravity and/or friction constraints → use energy, kinematics, or dynamics.
Learning to “segment” the problem is a core skill.
Choosing the right conservation law
Ask these questions:
Is there significant external torque about my chosen axis during the interaction?
- If no, conservation of angular momentum is on the table.
Is the interaction inelastic (sticking, deformation)?
- If yes, mechanical energy is usually not conserved during the collision-like interval.
Is friction present, and is it doing work?
- Kinetic friction dissipates mechanical energy.
- Static friction may do zero work in ideal rolling constraints.
Is the moment of inertia changing?
- If yes and external torque is negligible, angular momentum conservation is often the simplest route.
Worked example: bullet sticks to a rod pivoted at one end
Situation: A thin rod (mass M, length L) is pivoted frictionlessly at one end and initially at rest. A small bullet (mass m) traveling horizontally at speed v strikes the rod at its free end and sticks. Find the angular speed immediately after impact, then find the maximum height the rod’s center of mass rises (assuming it swings upward afterward without losses).
This is a classic two-part problem.
Part 1: Immediately after impact (angular momentum conserved)
During the short impact, external torque about the pivot is negligible about the pivot because the pivot force produces zero torque about that point. Gravity’s torque during the very brief collision is typically negligible.
Conserve angular momentum about the pivot.
- Initial angular momentum (bullet about pivot): the lever arm is L, so magnitude is
L_i = m v L
- Final angular momentum: rod plus bullet rotate together with angular speed \omega.
Moment of inertia about pivot:
Rod about one end:
I_{rod} = \frac{1}{3}ML^2
Bullet as point mass at radius L:
I_{bullet} = mL^2
Total:
I_f = \frac{1}{3}ML^2 + mL^2
Conservation:
m v L = \left(\frac{1}{3}ML^2 + mL^2\right)\omega
Solve:
\omega = \frac{m v L}{L^2\left(\frac{1}{3}M + m\right)} = \frac{m v}{L\left(\frac{1}{3}M + m\right)}
Part 2: After impact to maximum height (mechanical energy conserved)
After the collision, the rod-bullet system swings upward. If the pivot is frictionless and we ignore air resistance, mechanical energy is conserved during the swing.
Initial energy right after collision is rotational kinetic energy about the pivot:
K_i = \frac{1}{2}I_f\omega^2
At maximum height, rotational speed is zero, so energy is gravitational potential energy increase:
\Delta U = Mg\Delta y_{cm} + mg\Delta y_{bullet}
For a rod pivoted at one end, the center of mass is at \frac{L}{2} from the pivot. If it swings up by angle \theta from vertical-down position, the vertical rise is
\Delta y_{cm} = \frac{L}{2}(1 - \cos\theta)
Bullet at the end rises
\Delta y_{bullet} = L(1 - \cos\theta)
Energy conservation:
\frac{1}{2}I_f\omega^2 = Mg\frac{L}{2}(1 - \cos\theta) + mgL(1 - \cos\theta)
Factor:
\frac{1}{2}I_f\omega^2 = gL(1 - \cos\theta)\left(\frac{M}{2} + m\right)
From here, you can solve for \theta (or directly for the maximum rise if asked). The key learning is not the trig—it’s knowing where to use angular momentum (collision) and where to use energy (swing).
Why this problem is a unit summary without being a “review sheet”
This single scenario forces you to do the most important Unit 6 moves:
- pick the pivot as the angular momentum axis
- treat the collision as inelastic (do not conserve kinetic energy there)
- use mechanical energy conservation afterward
- build the correct moment of inertia for a compound object
Exam Focus
- Typical question patterns:
- Multi-interval problems: conserve L during impact, then conserve energy afterward.
- Compound moment of inertia: add I contributions of multiple parts (rod plus point mass).
- Use the pivot as the axis to eliminate unknown external torques.
- Common mistakes:
- Trying to conserve mechanical energy during the sticking collision.
- Conserving angular momentum about the center of mass instead of about the pivot (introducing external torque from the pivot force).
- Forgetting to add the bullet’s mL^2 to the total moment of inertia.
Angular momentum in systems with translation: choosing a smart reference point
Some AP Physics 1 questions involve an object moving linearly and you’re asked about its angular momentum about a point. These problems are less about heavy computation and more about understanding what angular momentum “counts.”
Angular momentum of a moving particle about a point
For a particle of mass m moving with speed v, the magnitude of angular momentum about a point is
L = mvr
where r is the perpendicular distance from the point to the particle’s line of motion.
This tells you:
- If the particle heads straight toward the point, r = 0 and L = 0.
- If it passes farther away, L is larger.
Torque from a force depends on lever arm
A force can change angular momentum only if it produces torque about the chosen point. The magnitude of torque is
\tau = rF
when F is perpendicular to the lever arm. More generally, torque depends on the perpendicular component of force.
This is why choosing the pivot point or the center can simplify life: if the force’s line of action goes through your chosen point, torque is zero about that point.
Worked example: when is angular momentum conserved about a point?
Situation: A puck slides on frictionless ice in a straight line. Consider its angular momentum about two different points: point A on the line of motion, and point B off to the side. Is angular momentum conserved about each point?
- About point A: r = 0, so L = 0 at all times. With no external forces, it stays zero.
- About point B: r is constant (the perpendicular distance to the line of motion), v is constant, and m is constant, so L = mvr is constant.
So angular momentum is conserved about both points here, but for different reasons. The important message: with no external force, net external torque about any fixed point is zero, so angular momentum about that point is conserved.
On the other hand, if friction or a force acts, you must check whether that force produces a torque about the point.
Common mistake: using the wrong lever arm
Students often use the direct distance from the point to the particle rather than the perpendicular distance to the line of motion. The formula L = mvr uses the perpendicular distance. If you use the wrong geometry, you’ll get the wrong angular momentum.
Exam Focus
- Typical question patterns:
- Compute or compare L of a moving particle about different points using the perpendicular distance.
- Determine whether a force produces torque about a point (line of action test).
- Conceptual conservation: identify when \tau_{ext,net} = 0 about a chosen point.
- Common mistakes:
- Using the wrong r (not perpendicular).
- Forgetting angular momentum depends on the reference point.
- Assuming “no net force” automatically means “no net torque” without checking the point.
Real-world applications and modeling choices that AP Physics 1 expects
AP Physics 1 is as much about modeling as it is about formulas. Rotating-system problems often require you to state (implicitly or explicitly) what you’re ignoring.
Common modeling assumptions
- Rigid bodies: objects don’t deform, so I is constant unless the configuration changes (like a person moving arms).
- Massless strings and frictionless pulleys (unless told otherwise): simplifies torque and energy analysis.
- No air resistance and negligible axle friction: allows mechanical energy conservation in rolling/swinging.
- Brief collisions: during a short impact, external torques like gravity are often negligible compared with impulsive internal forces.
A useful way to sanity-check answers
- If you increase I while keeping L constant, \omega should decrease.
- If energy is conserved rolling down a height h, your final speed should scale like \sqrt{gh} times a factor less than or equal to \sqrt{2}.
- If an object has bigger I_{cm} relative to MR^2, it should roll more slowly for the same height.
Worked example: why a hoop is “harder to spin up”
Situation: Two objects with equal M and R start at rest. You apply the same torque \tau for the same time \Delta t to each: a hoop and a disk. Which ends with larger \omega?
Use angular impulse:
\Delta L = \tau\Delta t
Starting from rest, L_f = \tau\Delta t.
But L = I\omega, so
\omega = \frac{L}{I} = \frac{\tau\Delta t}{I}
- Hoop: I = MR^2 → smaller \omega
- Disk: I = \frac{1}{2}MR^2 → larger \omega
So the disk spins up faster under the same torque impulse.
Exam Focus
- Typical question patterns:
- Decide what to neglect (air resistance, axle friction) to justify conservation of energy or angular momentum.
- Explain qualitatively how changing I affects \omega and K_{rot}.
- Use proportional reasoning instead of heavy algebra (compare disk vs hoop, sphere vs cylinder).
- Common mistakes:
- Applying conservation laws without stating (or checking) the required condition (zero external torque, no dissipative work).
- Confusing which quantities are conserved in which types of interactions.
- Treating I as an intrinsic property independent of axis choice.