Rotational dynamics

MDCAT Physics · Physics · Circular and rotational motion. The idea in plain words, the rules to remember, the mistake to avoid and a worked example, written and checked by Mega Lecture.

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The idea

In rotation, moment of inertia I plays the part that mass plays in straight-line motion. It depends on the mass and on how far that mass is from the axis, so the same body has a different I about a different axis.

A spinning body has rotational kinetic energy ½Iω2 and angular momentum L = Iω. If no external torque acts, L stays constant. So when a body pulls its mass closer to the axis, I falls and ω rises.

A satellite stays in a circular orbit because gravity supplies the centripetal force. Its orbital speed depends only on the radius of the orbit and the mass of the planet, not on the mass of the satellite.

Rules to remember

Common mistake

Students think rotational kinetic energy stays the same when a skater pulls her arms in. Angular momentum stays the same; the kinetic energy increases because she does work in pulling her arms in.

Worked example

A skater spins at 2.0 revolutions per second with a moment of inertia of 4.0 kg m2. She pulls her arms in and her moment of inertia becomes 1.6 kg m2. Find her new rate of spin.

  1. No external torque acts, so angular momentum is conserved: I1ω1 = I2ω2.
  2. The ratio works in any unit of spin rate: 4.0 × 2.0 = 1.6 × new rate.
  3. New rate = 8.0 ÷ 1.6 = 5.0 revolutions per second.

Answer: 5.0 revolutions per second (10π rad s−1).

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