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Physics · Ch 3 — Laws of Motion

SUMMARY

SUMMARY

This unit's key results, gathered together:

  • Aristotle held that force is needed to maintain motion; Galileo (and Newton) showed force is needed only to change motion. Mass measures inertia.
  • Newton's first law: with no external force, a body's state of motion is unchanged (this law defines inertial frames).
  • Newton's second law: F⃗=dp⃗/dt\vec F=d\vec p/dt (valid only in inertial frames); for constant mass, F⃗=ma⃗\vec F=m\vec a.
  • Newton's third law: every force has an equal, opposite reaction, acting on the other body.
  • A free body diagram isolates one object's own forces (never the forces it exerts elsewhere).
  • The total momentum of an isolated system is conserved; internal forces cannot change it.
  • Lami's theorem relates three concurrent, coplanar forces via the sines of their opposite angles.
  • Impulse equals the change in momentum, J=∫F dt=ΔpJ=\int F\,dt=\Delta p.
  • Static friction ranges from 00 to μsN\mu_sN; once sliding, kinetic friction is μkN\mu_kN (μk<μs\mu_k<\mu_s); rolling friction is smaller still. …