Home / A-Level Physics 9702 / Topic 12 revision notes
Download PDFA-Level Physics 9702 contents

Motion in a circle

A-Level Physics 9702 · Topic 12 revision notes · A2

Radians and angular speed, then the centripetal acceleration and force that turn velocity without changing its size, applied to real examples.

7 definitions to learn word for word, 13 equations in their own column, 6 diagrams and graphs. Read it, cover it, test yourself.

  1. 12.1a Radians and angular displacement
  2. 12.1b Angular speed
  3. 12.2a Centripetal acceleration and centripetal force
  4. 12.2b Applying circular motion
Definitions (mark-scheme wording)EquationsExam traps

12.1aRadians and angular displacement

Definitions

Radian
the angle subtended at the centre of a circle by an arc equal in length to the radius.
Angular displacement (θ)
the angle through which an object has turned about the centre of the circle, measured in radians.

Key points

  • A full circle is 2π rad = 360°; so 1 rad ≈ 57.3°.
  • Degrees to radians: multiply by π/180.
  • Arc length s = rθ only works with θ in radians.
  • Small angles (θ in rad): sin θ ≈ tan θ ≈ θ.
θ r s θ = s / r s = r: 1 rad
Angle in radians = arc length / radius. When s = r, θ = 1 rad.

Watch out!

  • Calculator in the wrong mode: set it to radians for any angle from θ = s/r or ωt.

12.1bAngular speed

Definitions

Angular speed (ω)
the rate of change of angular displacement (angle turned per unit time).
Period (T)
the time taken for one complete revolution.
Frequency (f)
the number of revolutions per unit time.

Key points

  • Every point on a rigid rotating body has the same ω.
  • Linear (tangential) speed increases with radius: v = rω.
  • Uniform circular motion: constant speed, constant ω, but changing velocity (direction changes).
  • Convert rev min-1 to rad s-1: multiply by 2π, divide by 60.
AB v2v ω same ω, v ∝ r
A rotating disc: points A and B turn through the same angle in the same time (same ω), but B at larger radius moves faster (v = rω).

Watch out!

  • ω must be in rad s-1, not rev s-1 or degrees per second.
  • Radius r is measured from the centre of the circle, not the diameter.

12.2aCentripetal acceleration and centripetal force

Definitions

Centripetal acceleration
the acceleration of an object moving in a circle, directed towards the centre of the circle.
Centripetal force
the resultant force on an object moving in a circle, directed towards the centre of the circle.

Key points

  • At constant speed the velocity changes direction, so the object accelerates (Newton's first law needs a resultant force).
  • Velocity is tangential; force and acceleration point along the radius to the centre.
  • Force is perpendicular to velocity, so it does no work: kinetic energy and speed stay constant.
  • Centripetal force is not an extra force: it is provided by tension, gravity, friction, normal contact or a magnetic force.
  • If the force is removed, the object moves off along the tangent (not outwards along the radius).
r v F, a v F speed constant, velocity not
Uniform circular motion: velocity is tangential; the centripetal force and acceleration point inwards along the radius.
v₁ v₂ Δv Δv (and so a) points to the centre |v₁| = |v₂|, directions differ
Why the acceleration points inwards: the change in velocity Δv = v2 - v1 between two nearby points is directed towards the centre.

Watch out!

  • There is no outward "centrifugal force" on the object. Draw only the real forces; their resultant is inwards.
  • In F = mv2/r, F is the resultant force, not one of the forces added to it.

12.2bApplying circular motion

Key points

  • Method: draw the real forces, find the resultant towards the centre, set it equal to mv2/r.
  • Car on a flat bend: friction between tyres and road provides the centripetal force.
  • Banked track: the horizontal component of the normal force provides it; N cos θ = mg.
  • Mass on a string in a vertical circle: tension is greatest at the bottom, least at the top.
  • At the top, the string stays taut only if v ≥ √(gr); at this minimum speed T = 0 and gravity alone provides the force.
  • Satellites and planets: gravitational force provides the centripetal force (see topic 13).
  • Conical pendulum / aircraft banking: horizontal component of tension or lift provides it.
Tmg Tmg top:T + mg = mv²/r bottom:T - mg = mv²/r
Vertical circle: at the top, tension and weight both act towards the centre; at the bottom, tension must exceed weight.
θ Nmg to centre N cos θ = mg N sin θ = mv²/r
Banked track: the horizontal component of the normal force, N sin θ, provides the centripetal force; N cos θ balances the weight.

Watch out!

  • At the top of a vertical circle, weight helps (T + mg); at the bottom it opposes (T - mg). Do not use the same equation for both.
  • Use the radius to the centre of mass of the object, e.g. string length plus the ball radius if needed.
Back to A-Level Physics 9702 contents · (c) 2026 TheLucidSTEM · thelucidstem.com