Module 5: Rotation and Equilibrium
"In the absence of external torques, the angular momentum of a system remains constant. The universe keeps its books very carefully."
— paraphrase of a conservation law
This lesson is where everything in Module 5 converges. Rolling without slipping is not pure rotation and not pure translation — it is both simultaneously, linked by the constraint vcm = Rω. To analyze a rolling object on an incline you need M5L1 kinematics, M5L2 dynamics, and M3 energy conservation — all at once. Then the lesson extends the rotational framework to its most powerful conservation law: angular momentum L = Iω is conserved when net external torque is zero. This is why a gyroscope resists tipping, why a diver can control rotation speed in the air, and why neutron stars spin at extraordinary rates. Conservation of angular momentum is one of the deepest symmetries in physics, and it is accessible to you right now.
The rolling constraint links every kinematic and dynamic quantity:
The rotational analog of linear momentum:
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CC5.3 Analyze rolling motion and apply conservation of angular momentum
★ LO5.3.1 Apply the rolling-without-slipping constraint (vcm = Rω, acm = Rα) to kinematic and dynamic problems
★ LO5.3.2 Calculate the total kinetic energy of a rolling object as the sum of translational and rotational kinetic energy
★ LO5.3.3 Use energy conservation to find the speed of a rolling object at the bottom of an incline
★ LO5.3.4 Predict which of two rolling objects reaches the bottom of an incline first based on their shape factors
★ LO5.3.5 Define angular momentum L = Iω and state its SI units
★ LO5.3.6 Apply the angular impulse-momentum theorem: τnetΔt = ΔL
★ LO5.3.7 Apply conservation of angular momentum to solve problems involving changing moment of inertia
Section 10.8 covers rolling; Chapter 11 introduces angular momentum. Read all four sections — each one introduces a concept you will need in the computational problems.
Video 1 establishes the rolling constraint and total kinetic energy; Video 2 applies energy conservation to the incline race; Video 3 introduces angular momentum and conservation.
Arrange these steps in the correct order for solving a rolling-on-incline problem using energy conservation.
A figure skater is spinning with arms extended. No external torque acts. Sort each action into the correct category.
Each card poses a question about rolling motion or angular momentum. Form your answer first, then check.
The sphere (c = 2/5) arrives before the ring (c = 1) because it stores less energy as rotation. Mass and radius cancel completely: v = √[2gh/(1+c)]. A 10 kg sphere and a 0.1 kg sphere of any radius would tie each other.
With no external torque, L = Iω = constant. Pulling arms in decreases I. Since L is fixed, ω must increase to compensate: ω₂ = I₁ω₁/I₂. Angular momentum is conserved; angular velocity is not. The skater spins faster, but L is unchanged.
Ktrans = ½mv² and Krot = ½Iω² = ½(cMR²)(v/R)² = ½cmv². So Krot/Ktrans = c. For a solid sphere (c = 2/5), Krot = (2/5)Ktrans — rotational KE is 40% of translational KE. Total = (7/5)Ktrans.
When a massive star collapses into a neutron star, its radius shrinks from ~10⁶ km to ~10 km — a factor of ~10⁵. Since L = Iω = cMR²ω is conserved and R drops by 10⁵, ω must increase by ~(10⁵)² = 10¹⁰. A one-month rotation becomes milliseconds. The same physics as the figure skater, scaled to stellar dimensions.
Problem 1 — Rolling Speed at Bottom of Incline
A solid cylinder of mass 3.0 kg and radius 0.10 m rolls without slipping from rest down an incline of height 0.80 m. Find: (a) the speed of the center of mass at the bottom, (b) the angular velocity at the bottom, (c) the translational and rotational kinetic energies.
Given: Solid cylinder → Icm = ½MR², so c = 1/2. h = 0.80 m, starts from rest.
(a) Speed at bottom:
vcm = √[2gh/(1+c)] = √[2(9.8)(0.80)/(1 + 0.5)] = √[15.68/1.5] = √10.45 = 3.23 m/s
(b) Angular velocity:
ω = vcm/R = 3.23/0.10 = 32.3 rad/s
(c) Kinetic energies:
Ktrans = ½mvcm² = ½(3.0)(3.23)² = ½(3.0)(10.43) = 15.65 J
Krot = ½Icmω² = ½(½)(3.0)(0.01)(32.3)² = ½(0.015)(1043) = 7.82 J
Total = 23.47 J ≈ mgh = (3.0)(9.8)(0.80) = 23.52 J ✓ (rounding)
Note: Krot/Ktrans = c = 1/2, as predicted. The cylinder puts half as much energy into spinning as into translating.
Problem 2 — The Incline Race
A solid sphere, a solid cylinder, and a hollow ring all have mass 1.5 kg and radius 0.12 m. They are released simultaneously from rest at the top of a 1.2 m high incline. Find the speed of each at the bottom and rank them.
Using v = √[2gh/(1+c)] with g = 9.8 m/s², h = 1.2 m, so 2gh = 23.52 m²/s²:
Solid sphere (c = 2/5):
v = √[23.52/1.4] = √16.80 = 4.10 m/s
Solid cylinder (c = 1/2):
v = √[23.52/1.5] = √15.68 = 3.96 m/s
Hollow ring (c = 1):
v = √[23.52/2.0] = √11.76 = 3.43 m/s
Ranking: Sphere (4.10) > Cylinder (3.96) > Ring (3.43)
Compare to frictionless sliding block (no rotation, c = 0):
v = √[23.52/1.0] = √23.52 = 4.85 m/s — faster than all rolling objects, as expected.
The mass 1.5 kg and radius 0.12 m appeared nowhere in the final answers — they canceled. Replace with any values and the ranking is unchanged.
Problem 3 — Figure Skater: Conservation of Angular Momentum
A figure skater spinning at 2.0 rev/s has a moment of inertia of 4.0 kg·m² with arms extended. She pulls her arms in, reducing her moment of inertia to 1.5 kg·m². Find: (a) her new angular velocity, (b) her initial and final rotational KE, (c) where the extra KE comes from.
Convert: ω₁ = 2.0 rev/s × 2π = 4π rad/s
(a) Conservation of angular momentum (τext = 0):
I₁ω₁ = I₂ω₂
ω₂ = I₁ω₁/I₂ = (4.0)(4π)/(1.5) = 16π/1.5 = 32π/3 ≈ 33.5 rad/s ≈ 5.33 rev/s
(b) Rotational kinetic energies:
K₁ = ½I₁ω₁² = ½(4.0)(4π)² = 2(16π²) = 32π² ≈ 316 J
K₂ = ½I₂ω₂² = ½(1.5)(32π/3)² = ½(1.5)(1024π²/9) = 85.3π² ≈ 842 J
(c) Source of extra kinetic energy:
ΔK = 842 − 316 = 526 J came from the skater's muscles. She did work against the centrifugal tendency of her arms as she pulled them inward. Angular momentum was conserved; energy was not — it was added by biological work.
Problem 4 — Stool + Person: Angular Momentum Transfer
A student (Istudent = 3.0 kg·m²) sits on a frictionless rotating stool (Istool = 0.50 kg·m²) initially at rest. She is handed a spinning bicycle wheel (Iwheel = 0.80 kg·m², ωwheel = 20 rad/s) with its axle pointing upward. She then flips the wheel so its axle points downward. Find the angular velocity of the student + stool.
Before flipping: Total angular momentum (upward positive):
Linitial = Iwheelωwheel + 0 = (0.80)(20) = +16 kg·m²/s (student + stool at rest)
After flipping: Wheel now spins at −20 rad/s (same speed, opposite direction):
Lwheel,final = (0.80)(−20) = −16 kg·m²/s
Conservation (no external torque):
Linitial = Lwheel,final + Lstudent+stool
+16 = −16 + (Istudent + Istool)ω
32 = (3.0 + 0.50)ω = 3.5ω
ω = 32/3.5 ≈ 9.14 rad/s (in the original wheel direction)
The student begins to rotate to compensate for the reversal of the wheel's angular momentum. This is the operating principle of reaction wheels used to orient spacecraft without thrusters.
Problem 5 — Rolling with Energy Conservation: Up a Ramp
A hollow sphere (I = ⅔MR²) rolls without slipping on a flat surface at 4.0 m/s and then encounters a ramp. How high does it rise before momentarily stopping? Compare to a solid sphere at the same speed.
Hollow sphere (c = 2/3):
Total KE at bottom: K = ½(1 + c)mv² = ½(1 + 2/3)(m)(4.0)² = ½(5/3)(m)(16) = (40m/3) J
At top: K = 0, PE = mgh
mgh = 40m/3 ⇒ h = 40/(3 × 9.8) = 1.36 m
Solid sphere (c = 2/5):
K = ½(1 + 2/5)(m)(16) = ½(7/5)(m)(16) = (56m/5) J
h = 56/(5 × 9.8) = 1.14 m
Comparison: The hollow sphere rises higher (1.36 m vs 1.14 m) at the same v because it has more rotational KE stored. At the top, both translational and rotational KE must go to zero — but the hollow sphere had more total KE to begin with for the same vcm.
M5L4 (Static Equilibrium) applies ΣF = 0 and Στ = 0 simultaneously. Make sure you can answer these before continuing:
M5L4 Static Equilibrium is the lesson where torque calculation becomes the central computational skill. The pivot-point strategy you will learn there relies on your fluency with τ = rF sinθ from M5L2.