What this chapter is about

Chapters 2 and 4 were kinematics — "how to describe motion". Now the key question: why does motion happen? Answer: force. Newton in 1687 stated three laws from which all classical mechanics follows.

Sections

  1. 5.1 — The concept of force and interaction
  2. 5.2 — Newton's first law — inertia
  3. 5.3 — Second law — F=ma
  4. 5.4 — Third law — action and reaction
  5. 5.5 — Weight and mass
  6. 5.6 — Friction
  7. 5.7 — Applications — pulleys, inclined planes
  8. 5.8 — Worked problems
  9. 5.9 — Practice problems
  10. 5.10 — Q&A

Prerequisites

Why this chapter is the heart of physics

\vec F = m\vec a — three letters, but all mechanics rides on it. From falling apples to satellite orbits, from walking to earthquakes — all described by this one equation.

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