PMDC Unit 40 · 4 outcomes

Rotational and Circular Motion

Unit 4 on the PMDC list is the dictionary of turning: angle in radians, angular velocity, and how those link to ordinary linear s, v and a. Stay inside 4.1–4.4.

4.1

Angular displacement

PMDC: Define angular displacement and express it in radians.

Angular displacement is the angle a radius sweeps. In radians it is the arc length divided by the radius. That is why the radian is the natural unit for linking turning to metres.

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Hold these

  • is a ratio of lengths, so the radian is a ‘bare’ number in formulae.
  • Use radians in , not degrees.

4.2

Revolution, degree and radian

PMDC: Define revolution, degree and radian.

One revolution is one full turn: back to the same spoke. A degree cuts that turn into 360 equal slices. A radian cuts it so that the arc equals the radius — 2 of those make a full turn.

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  • 1 = 2 rad
  • / 180)

Hold these

  • Half a turn is rad, not .

4.3

Angular velocity

PMDC: Describe the term angular velocity.

Angular velocity is how fast the angle changes. A steady spinner has constant . Direction (for a wheel) is along the axle by the right-hand rule, but MDCAT mostly wants the size in rad s⁻¹.

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  • unit: rad s⁻¹

Hold these

  • f is revolutions per second. is radians per second. = 2 f.
  • Do not mix rpm into until you convert.

4.4

Linear and angular quantities

PMDC: Find the relations between linear and angular variables: displacements, velocities, and accelerations.

The same turning looks bigger in metres if you sit farther from the centre. Multiply the angular quantity by r to get the linear one. become s, v, al.

These need in radians. The radial (centripetal) acceleration v²/r is extra — it points inward and is not r .

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  • = v² / ² (centripetal, to the centre)

Hold these

  • Farther out, same , larger v.
  • r is along the rim. v²/r is toward the centre. They are different arrows.

Unit 40 formula sheet

Write these until they are cheaper than thinking, then open the quiz.

  • 1 = 2 rad
  • / 180)
  • unit: rad s⁻¹
  • = v² / ² (centripetal, to the centre)