AP Physics C: Mechanics · Unit 3: Work, Energy, and Power ·  Lesson 3.4

Conservation of Energy

Energy never disappears — it just changes costumes  ·  Approx. 2–3 class days

StarringEi = Ki + Ugi + Usi + WncEf = Kf + Ugf + Usf

Use this as a quick reference for mechanical energy, choosing a system, and the full conservation of energy equation.

Conservation of Energy infographic

🧭 Plot Summary

Everything from Lessons 3.1 through 3.3 converges here. A system's mechanical energy is just kinetic plus potential energy — and the deep promise of this lesson is that energy is never created or destroyed, only converted between forms or transferred across a system's boundary. Choose your system wisely (echoing Lesson 2.1), and you can often set up a single equation — initial energy plus any nonconservative work equals final energy — and solve for whatever's missing, without ever touching kinematics or force diagrams directly.

What you'll do in this lesson

  • Identify what forms of energy a given system can have.
  • Define mechanical energy as the sum of kinetic and potential energy.
  • Explain how energy changes form within a system, or transfers between a system and its surroundings.
  • Choose a system so that conservation of energy applies cleanly.
  • Apply the full conservation of energy equation to solve for unknown quantities.
  • Represent energy transformations using energy bar charts.

Why it matters

Conservation of energy is arguably the single most powerful problem-solving tool in all of mechanics — many problems that look intimidating with forces and kinematics become almost trivial once you track energy instead.

Self-Check Before You Roll On

Check off each item as you get there. These aren't grades — they're your own signal.