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Spec mapping: OCR H556 Module 5.3 — Circular motion (radian measure; angular displacement, angular velocity and angular frequency; period and frequency; the linear-angular bridge v=rω; sub-strand sits inside Module 5 alongside Oscillations and Gravitational fields). Refer to the official OCR H556 specification document for exact wording.
Circular motion is one of the most elegant topics in A-Level Physics. A body moving in a circle at constant speed is a perfect example of accelerated motion in which the speed is constant but the velocity is changing all the time. Before we can talk about the forces involved, we need a new language — the language of angular quantities: angle measured in radians, angular displacement, angular velocity, frequency and period.
This lesson is the foundation of OCR A-Level Physics A Module 5.3 (Circular motion). Everything else in the topic — centripetal force (lesson 2), simple harmonic motion (lessons 3-5), damping and resonance (lesson 6), and the orbital mechanics of Module 5.4 — depends on being able to move fluently between the linear world (metres and metres per second) and the angular world (radians and radians per second). Many students arrive at A-Level with a hazy notion of "the angle is just a number" — by the end of this lesson we want a sharper picture: an angle is a ratio of two lengths (arc to radius), and that ratio is what makes the calculus of trigonometric functions clean.
You have been using degrees since primary school. Why, at A-Level, do we suddenly switch to radians?
The honest answer is calculus. Differentiating the trigonometric functions gives the neatest possible formulae only when the angle is measured in radians. Specifically, dθdsinθ=cosθ holds only with θ in radians; in degrees the derivative picks up an awkward π/180 factor. Engineers and physicists need those neat formulae, so they use radians by default and leave degrees to navigators, surveyors and carpenters.
The practical answer is arc length. With radians, the relationship between the arc length s, the radius r and the angle θ is simply
s=rθ
No awkward factor of π/180. The radian was invented specifically so this equation would have no fudge factor in it. Compare with the degree formulation s=rθ×π/180, which is correct but cluttered. Once you start chaining equations together (as we shortly will, to derive centripetal acceleration), the cleanness of the radian form pays off enormously.
Exam Tip: Whenever an OCR Physics question gives you an angle without explicitly saying "degrees", assume it is in radians. Make sure your calculator is in radian mode for any circular motion or SHM question. A single forgotten mode-switch destroys whole exam answers and is one of the most expensive silent errors at A-Level.
Imagine a circle of radius r. Mark two radii so that the arc between them has length s. The angle θ between the radii, measured in radians, is defined as
θ=rs
In words: one radian is the angle subtended at the centre of a circle by an arc equal in length to the radius. Because both s and r are lengths, the radian is dimensionless — it is really just a ratio. This is why you can drop the "rad" symbol when the radian is multiplied by a length to produce another length (as in s=rθ): a metre times a (dimensionless) radian is still a metre. Strictly the radian is given its own SI symbol for clarity, but it has no SI base-unit dimensions.
If the arc length equals the radius (s=r), the angle is exactly 1 rad. If the arc length is the full circumference (s=2πr), the angle is 2π rad, which corresponds to 360°.
| Degrees | Radians |
|---|---|
| 360° | 2π |
| 180° | π |
| 90° | π/2 |
| 60° | π/3 |
| 45° | π/4 |
| 30° | π/6 |
| 1° | π/180≈0.01745 rad |
| 1 rad | 180/π≈57.30° |
Conversion rules:
- Degrees → radians: multiply by π/180
- Radians → degrees: multiply by 180/π
Memorise the "boundary" entries (30°,45°,60°,90°,180°,360° and their radian images). The rest you can derive on the fly. Many OCR questions silently expect you to know that π/3=60° when reading an angle off a diagram — getting the conversion wrong then propagates into every later calculation.
Angular displacement θ is the angle, measured in radians, through which a rotating body has turned from some reference direction. It is the angular equivalent of linear displacement s.
Just as linear displacement is a vector, angular displacement is also a vector — by convention, its direction lies along the axis of rotation and its sense is given by the right-hand rule (curl the fingers in the direction of rotation; the thumb gives the angular vector direction). For OCR A-Level purposes you only need to treat angular displacement as a signed scalar: positive for anticlockwise, negative for clockwise (or vice versa, depending on the choice of axis). Vector treatments are reserved for undergraduate mechanics and the "Going further" section below.
A car tyre of radius 0.33 m rolls through 12 complete revolutions without slipping. Calculate the distance travelled.
One revolution =2π rad, so 12 revolutions =24π rad.
s=rθ=0.33×24π=24.88 m
Notice how painless the calculation is in radians. In degrees you would have needed 12×360=4320°, then converted to radians anyway. The no-slip rolling condition s=rθ is the same relationship that unwinds string from a pulley, or threads paper through a printer roller: every turn through angle θ delivers an arc length rθ of perimeter. This is the same equation as for a fixed-axis rotation, but applied along the tyre's own rim rather than at a fixed point in space.
A simple pendulum of length L=1.20 m is pulled aside through an angle of 4.5° from the vertical. How far has the bob moved along its arc?
Convert: θ=4.5°×π/180=0.0785 rad.
s=Lθ=1.20×0.0785=0.0942 m=9.4 cm
For small angles, the bob's arc length and its straight-line displacement from equilibrium differ by less than 0.1%. This is exactly the "small-angle approximation" that turns a pendulum into an SHM oscillator — a result we will exploit heavily in lesson 3.
Just as linear velocity is the rate of change of linear displacement, angular velocity ω (the Greek letter omega) is the rate of change of angular displacement:
ω=tθ(uniform circular motion)ω=dtdθ(instantaneous)
The SI unit is radians per second (rad s−1). Numerically ω is a scalar for our purposes, but strictly it is also a vector along the axis of rotation (again, right-hand rule). When OCR writes "the wheel has angular velocity 20 rad s−1" without specifying axis, the magnitude is what they want.
A body that travels once around a circle (θ=2π) in a time T — the period — has angular velocity
ω=T2π
Rearranging,
T=ω2π
The period tells you how many seconds each revolution takes. It is by far the most physically intuitive of the three angular measures: ask anyone how fast a flywheel spins, and they will instinctively reach for "revolutions per minute" — a period-style quantity — rather than ω in rad s−1.
Frequency f is the number of complete revolutions per second, measured in hertz (Hz). Since one revolution takes T seconds, there are 1/T revolutions per second, so
f=T1ω=2πf
You will use ω=2πf constantly, both in circular motion and later in simple harmonic motion. The factor 2π converts "revolutions per second" into "radians per second" — exactly 2π radians per revolution.
If a body moves in a circle of radius r with angular velocity ω, in time t it sweeps through an angle ωt and covers an arc length
s=rθ=r(ωt)
Its linear (tangential) speed is therefore
v=ts=rω
This is arguably the single most important equation in circular motion. It is the bridge between the angular world and the linear world. Memorise it.
| Angular quantity | Linear equivalent | Relationship |
|---|---|---|
| θ (rad) | s (m) | s=rθ |
| ω (rad s−1) | v (m s−1) | v=rω |
| α (rad s−2) | atangential (m s−2) | at=rα |
The last row — angular acceleration α — only matters if the rotation is speeding up or slowing down; for uniform circular motion α=0 and the entire row can be ignored. For OCR you will almost always work in uniform circular motion (constant ω), so the first two rows are the workhorses.
A vinyl record spins at 3331 rpm (revolutions per minute). A speck of dust sits 0.12 m from the centre.
(a) Angular velocity:
3331 rpm =33.33/60=0.556 rev s−1
ω=2πf=2π×0.556=3.49 rad s−1
(b) Period:
T=ω2π=3.492π=1.80 s
Sanity check: 60 s /33.33 rev ≈1.80 s per revolution. ✓
(c) Linear speed of the dust:
v=rω=0.12×3.49=0.419 m s−1
Notice the dust is moving at about 0.42 m s−1, but a speck at 0.06 m from the centre would move at only 0.21 m s−1. Different radii, same angular velocity: v∝r at fixed ω. This is why a car's tyre rim moves faster than its hub even though both share the same wheel.
Estimate the linear speed of a point on the Earth's equator. Take the Earth's radius as 6.37×106 m and its period as 24 hours.
Tωv=24×3600=86400 s=T2π=864002π=7.27×10−5 rad s−1=rω=6.37×106×7.27×10−5=463 m s−1
So you and your chair are moving eastward at roughly 463 m s−1 (about 1670 km/h) without feeling a thing, because the ground beneath you is moving at exactly the same speed (Galilean relativity, see Newton 1 in the Newton-momentum lesson). At higher latitudes the radius of the circle of latitude is smaller — at 50° N, the effective radius is Rcos50°≈4.10×106 m, and the surface speed drops to ≈298 m s−1. This latitude-dependence has practical engineering importance: rockets are launched eastward and from low latitudes wherever possible, to harvest as much of Earth's rotation as a free initial speed.
Exam Tip: OCR frequently asks candidates to compute the linear speed of a satellite, spinning wheel or ride at a funfair using v=rω. Make sure your angular velocity is in rad s−1, not revolutions per minute. Marks are routinely lost when candidates substitute rpm directly.
A bicycle wheel has diameter 0.66 m. The cyclist pedals at a steady 25 km h−1 on level ground. Find the angular velocity of the wheel in rad s−1 and the period of one rotation.
Convert speed: v=25×1000/3600=6.94 m s−1. Radius r=0.33 m.
ω=rv=0.336.94=21.0 rad s−1
T=ω2π=21.02π=0.299 s
So the wheel completes a full rotation in just under one third of a second, about 3.3 revolutions per second. This is the kind of feel-it estimate that good A-Level physicists develop — when a question gives a speed and a wheel, the period is "fraction of a second", not "many seconds". Anything else suggests an arithmetic slip.
A body moving at constant speed in a circle has a constant ∣v∣ but a continuously changing direction of v. Because velocity is a vector, any change in direction is a change in velocity, and any change in velocity is — by Newton's first law — an acceleration. This is one of the most important conceptual insights in A-Level mechanics, and one that GCSE rarely emphasises.
The velocity vector is always tangential to the circle. At the top of the circle it points one way; a quarter-turn later it points perpendicular to the first. The speed is unchanged, but the velocity is not.
This observation is the gateway to the next lesson, where we will quantify this "changing velocity" as the centripetal acceleration and use Newton's second law to deduce the force required to keep the object in its circular path.
Question (8 marks): A child's roundabout in a playground has radius 1.6 m. It is rotating uniformly, completing one full revolution every 2.5 s. A child sits on a horse fixed to the rim.
(a) Calculate (i) the period T, (ii) the frequency f, and (iii) the angular velocity ω of the roundabout, stating SI units. [3]
(b) Find the linear speed v of the child at the rim. [2]
(c) Without further calculation, describe and explain what happens to (i) the child's angular velocity and (ii) the child's linear speed if she stands up and walks along a radial line from the rim to half-way to the centre. [3]
| Mark | AO | Awarded for |
|---|---|---|
| 1 | AO2 | T=2.5 s with unit (or stated directly) |
| 2 | AO2 | f=1/T=0.40 Hz |
| 3 | AO2 | ω=2π/T=2.51 rad s−1 |
| 4 | AO2 | v=rω used (or v=2πr/T) |
| 5 | AO2 | v=4.0 m s−1 to 2 s.f. |
| 6 | AO1 | Angular velocity unchanged (rigid-body rotation) |
| 7 | AO2 | Linear speed at new radius v′=r′ω=0.80×2.51=2.0 m s−1 |
| 8 | AO3 | Reasoning: same ω for all points on rigid roundabout; v∝r at fixed ω |
AO split: AO1 = 1, AO2 = 6, AO3 = 1.
Mid-band response (4/8):
(a) (i) T=2.5 s. (ii) f=1/T=0.4 Hz. (iii) ω=2π/T=2.51 rad/s.
(b) v=r×ω=1.6×2.51=4.0 m s−1.
(c) The speed drops because she is closer to the centre.
Examiner commentary: The next-band move is to state the principle that all points on a rigid rotating body share the same ω, and only then deduce that v scales with r. Marks 1-5 awarded for the calculation. Marks 6-8 lost — the candidate gives a one-line assertion in (c) but does not separate ω from v, does not name "rigid rotation", and does not state the half-radius numerical answer (≈2.0 m s−1).
Stronger response (7/8):
(a) (i) T=2.5 s. (ii) f=1/T=0.40 Hz. (iii) ω=2π/T=2π/2.5=2.51 rad s−1.
(b) v=rω=1.6×2.51=4.0 m s−1 (to 2 s.f.).
(c) (i) Her angular velocity is unchanged at 2.51 rad s−1 because the roundabout is a rigid body — every fixed point on it rotates at the same ω. (ii) Her linear speed drops because v=rω and r has halved while ω is constant; at r=0.80 m, v=0.80×2.51≈2.0 m s−1.
Examiner commentary: To lift to top-band, the answer would make explicit the vector interpretation — that ω is a property of the rigid body, not of an individual particle — and would note that the child is not in fact a point on the rigid body once she is moving radially, so during her walk her angular velocity does briefly differ from the roundabout's. Marks 1-7 awarded. Mark 8 partial: the candidate has the right answer with reasoning, but the implicit assumption that the child stays locked to the roundabout's ω during the walk is not justified.
Top-band response (8/8):
(a) (i) T=2.5 s. (ii) f=1/T=1/2.5=0.40 Hz. (iii) ω=2πf=2π×0.40=2.513 rad s−1.
(b) The child is fixed to the rim of a rigid rotating body, so v=rω. With r=1.6 m and ω=2.513 rad s−1:
v=1.6×2.513=4.02 m s−1≈4.0 m s−1
(c) (i) Angular velocity of the roundabout itself is unchanged: a rigid body has a single ω that all of its fixed material points share. If the child is standing on the roundabout (not propelling it independently), then at any instant her angular velocity matches the roundabout's at 2.51 rad s−1 — though strictly her path is not a circle of constant radius during the walk, since r(t) is decreasing. After she has come to rest at the new radius, her steady-state ω=2.51 rad s−1 again.
(ii) Linear speed is governed by v=rω. With ω fixed and r halved from 1.6 m to 0.80 m, her linear speed at the new radius is v′=0.80×2.513=2.01 m s−1≈2.0 m s−1.
Examiner commentary: Full marks. The discriminator moves are (1) the principle "rigid body shares a single ω" stated up front; (2) the subtlety that during the walk itself the child's instantaneous angular velocity is not strictly constant — only the steady-state endpoint is. Top-band answers do not just compute; they reason about which idealisation applies and surface its limits. Note also the careful use of 2.513 rad s−1 in working with rounding only at the final answer — this avoids accumulated rounding errors.
Pedagogical observations from teaching A-Level circular motion, with no fabricated examiner-report percentages.
The radian as a ratio of arc to radius is one of the cleanest examples in school physics of why dimensionless angles are the natural choice — and the rabbit hole goes deep.
At undergraduate level, angular velocity is treated as a vector ω along the rotation axis, and the velocity of any material point in a rigid body is given by the elegant cross-product v=ω×r. This single formula contains v=rω as its magnitude (for r perpendicular to ω), but also recovers the direction of v automatically: tangential, perpendicular to both ω and r, sense given by the right-hand rule. This is the standard formulation in Classical Mechanics by John Taylor (chapter 9) and in Mechanics by Kleppner and Kolenkow (a favourite of Cambridge entrance).
A further deep idea: in Lagrangian mechanics, the choice of "generalised coordinate" for a rotating system is naturally the angle θ (rather than the linear position x), and the conjugate "generalised momentum" turns out to be the angular momentum L=Iω, with I the moment of inertia. The conservation of angular momentum then follows from the rotational symmetry of the Lagrangian — a particular case of Noether's theorem, one of the most beautiful results in theoretical physics. (Symmetry under rotation ⇒ angular momentum conservation; symmetry under spatial translation ⇒ linear momentum conservation; symmetry under time translation ⇒ energy conservation.)
Two Oxbridge interview prompts that probe this material:
Recommended reading: Six Easy Pieces (Feynman) Chapter 1 for conceptual clarity; Kleppner and Kolenkow Mechanics Chapter 8 for the rigid-body formulation; Penrose The Road to Reality Chapter 11 for the abstract algebra of rotations and the introduction to SO(3) and quaternions.
Master these five relationships and you will never be stuck on a circular-motion calculation. The next lesson builds directly on them to derive centripetal acceleration — the acceleration required to keep an object moving in a circle.
Reference: OCR A-Level Physics A (H556) specification 5.3 — Circular motion (refer to the official OCR H556 specification document for exact wording).