ACEpath
Select Subject
Select Unit

Formula For Rotational Ke

Krot=12Iω2K_{rot} = \frac{1}{2}I\omega^2

  • Energy of rotation
  • Depends on moment of inertia and angular velocity
  • Analogs of translational KE: 12mv2\frac{1}{2}mv^2
  • Important for rolling and spinning objects

Total Kinetic Energy Of Rolling Objects

Ktotal=Ktrans+Krot=12mv2+12Iω2K_{total} = K_{trans} + K_{rot} = \frac{1}{2}mv^2 + \frac{1}{2}I\omega^2

  • For rolling without slipping: v=rωv = r\omega
  • K=12mv2+12(mr2)(vr)2=12mv2(1+Imr2)K = \frac{1}{2}mv^2 + \frac{1}{2}(mr^2)\left(\frac{v}{r}\right)^2 = \frac{1}{2}mv^2\left(1 + \frac{I}{mr^2}\right)
  • K=12mv2(1+β)K = \frac{1}{2}mv^2\left(1 + \beta\right) where β=I/(mr2)\beta = I/(mr^2)
  • Solid sphere: β=2/5\beta = 2/5, hollow sphere: β=2/3\beta = 2/3, cylinder: β=1/2\beta = 1/2

Races On Inclines

  • Objects with different shapes roll down incline
  • Faster object reaches bottom first (has larger acceleration)
  • Depends on β=I/(mr2)\beta = I/(mr^2)
  • Smaller β\beta -> larger acceleration
  • Results independent of mass and radius

Angular Momentum Of Rigid Bodies

L=IωL = I\omega

  • Rotational analog of linear momentum (p=mvp = mv)
  • Vector quantity: direction along rotation axis
  • Units: kg - m2/s
  • Conserved when τnet=0\tau_{net} = 0

Angular Momentum Of Particles

L=mvrL = mvr_\perp (for point particle)

  • Perpendicular distance from reference point to velocity line
  • Depends on choice of reference point
  • Conserved when net external torque = 0

Change In Angular Momentum

ΔL=τnetΔt\Delta L = \tau_{net}\Delta t

  • Net torque causes change in angular momentum
  • Analogous to impulse-momentum theorem
  • Important for rotational collisions

Conditions For Angular Momentum Conservation

  • Net external torque on system = 0
  • Internal torques cancel (action-reaction pairs)
  • System isolated from external rotational influences
  • Can hold even during collisions

Changing Moment Of Inertia Example Skater

  • Iiωi=IfωfI_i\omega_i = I_f\omega_f
  • Skater pulls arms in: II decreases, ω\omega increases
  • Angular momentum conserved (no external torque)
  • Used by figure skaters, divers
  • Demonstrates conservation in action

Planetary Orbits

  • Planets sweep out equal areas in equal times (Kepler's 2nd Law)
  • Conservation of angular momentum
  • L=mvr=constantL = mvr = \text{constant} (approximately circular orbits)
  • Explains why orbits are stable