AP Physics C: Mechanics ›  Unit 2

Unit 2 Force and Translational Dynamics

Newton's laws, free-body diagrams, and every kind of force you'll meet all year — friction, springs, gravity, drag, and circular motion — all traced back to ΣF = dp/dt.

📋 20–25% AP Exam Weighting🕐 ~15–25 Class Periods📺 10 Episodes✅ Progress Check 2
EP.2.1

Systems and Center of Mass

A system can be treated as a single point at its center of mass. For continuous objects, that point comes from an integral, not just an average.

x_cm = Σmᵢxᵢ/Σmᵢλ(x) = dm/dx∫r dm / ∫dm
🕐 1–2 class daysOpen lesson →
EP.2.2

Forces and Free-Body Diagrams

Every force is an interaction between two objects. Draw them as vectors from the center-of-mass dot, and the algebra practically writes itself.

Contact vs. field forcesFree-body diagramsAxis along acceleration
🕐 2–3 class daysOpen lesson →
EP.2.3

Newton's Third Law

Every force comes with a partner, equal and opposite, acting on the other object. Tension and ideal pulleys make this precise.

Paired forcesIdeal string / pulleyTug-of-war physics
🕐 1–2 class daysOpen lesson →
EP.2.4

Newton's First Law

Zero net force means constant velocity — nothing more, nothing less. Balanced in one direction says nothing about what's happening in another.

ΣF = 0Translational equilibriumInertial frames
🕐 1–2 class daysOpen lesson →
EP.2.5

Newton's Second Law

F = ma is the special case. The real law is that net force is the rate of change of momentum — and that version survives everything Unit 4 throws at it.

ΣF = maΣF = dp/dtMulti-body systems
🕐 2–3 class daysOpen lesson →
EP.2.6

Gravitational Force

Every mass pulls on every other mass. Near Earth's surface that collapses into mg — but the inverse-square law underneath never goes away.

F = Gm₁m₂/r²Weight = mgField vs. force
🕐 1–2 class daysOpen lesson →
EP.2.7

Kinetic and Static Friction

Static friction resists up to a maximum; kinetic friction is (almost) constant once things start sliding. Knowing which one applies changes the whole problem.

f_s ≤ μ_s Nf_k = μ_k NSurface interactions
🕐 2–3 class daysOpen lesson →
EP.2.8

Spring Forces

Hooke's law is a restoring force — always pointed back toward equilibrium, always proportional to displacement. This is where oscillations start.

Fₛ = −kxRestoring forceEquilibrium position
🕐 1–2 class daysOpen lesson →
EP.2.9

Resistive Forces

Drag depends on velocity itself, which means the equation of motion becomes a differential equation. Terminal velocity falls out when acceleration finally hits zero.

F ∝ v or v²Differential equationsTerminal velocity
🕐 2–3 class daysOpen lesson →
EP.2.10

Circular Motion

Constant speed doesn't mean constant velocity. Center-seeking acceleration keeps an object turning even when nothing speeds it up or slows it down.

a_c = v²/rCentripetal forceUniform circular motion
🕐 2–3 class daysOpen lesson →
🎓 AP Classroom — Progress Check 2
~30 multiple-choice · 4 free-response · Covers all 10 episodes
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