AP Physics C: Mechanics ›  Unit 6

Unit 6 Energy and Momentum of Rotating Systems

Angular momentum is conserved. Figure skaters — and satellites — know this. Unit 3 and Unit 4's tools come back, rebuilt for anything that spins.

📋 10–15% AP Exam Weighting🕐 ~13–19 Class Periods📺 6 Episodes✅ Progress Check 6
EP.6.1

Rotational Kinetic Energy

K = ½mv² had a rotational twin waiting all along: K_rot = ½Iω². A rolling object carries both kinds at once.

K_rot = ½Iω²K_tot = K_trans + K_rotSame object, two motions
🕐 2–3 class daysOpen lesson →
EP.6.2

Torque and Work

Force times distance becomes torque times angle. The rotational work-energy theorem falls straight out of the same logic as Unit 3.

W = ∫τ dθΔK_rot = W_netRotational work–energy theorem
🕐 2–3 class daysOpen lesson →
EP.6.3

Angular Momentum and Angular Impulse

L = r × p for a particle, or L = Iω for a rigid body — two ways of describing the same conserved quantity that keeps a spinning system spinning.

L = r × pL = Iωτ_ext = dL/dt
🕐 3–4 class daysOpen lesson →
EP.6.4

Conservation of Angular Momentum

Zero net external torque means L never changes — even if I does. That's how a figure skater speeds up just by pulling their arms in.

Στ_ext = 0 ⇒ L constantI₁ω₁ = I₂ω₂Shape-changing systems
🕐 2–3 class daysOpen lesson →
EP.6.5

Rolling

Rolling without slipping links v_cm and ω exactly. The instant a system slips, that link breaks — and friction starts stealing energy.

v_cm = rωa_cm = rαRolling vs. slipping
🕐 2–3 class daysOpen lesson →
EP.6.6

Motion of Orbiting Satellites

Circular orbits keep everything constant; elliptical ones trade kinetic and potential energy back and forth while angular momentum holds steady. Escape velocity is just the point where total energy hits zero.

U_g = −GMm/rE_total = −GMm/2r (circular)v_esc = √(2GM/r)
🕐 3–4 class daysOpen lesson →
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