Circular Motion
Motion of a particle along a circular path with constant or variable speed. Study each concept with live diagrams and full derivations, then test yourself with past questions.
Uniform Circular Motion
A periodic motion along a circular path with constant speed. The speed never changes — only the direction of motion turns continuously around the centre. For one full revolution of period $T$ and frequency $f$:
$$v = \dfrac{2\pi r}{T} = 2\pi r f$$- Speed and kinetic energy remain constant.
- Velocity, force and acceleration are constant in magnitude but change direction continuously.
- Work done is zero, because the force is always $\perp$ to the displacement.
- Force & acceleration always point towards the centre, $\perp$ to the velocity (angle $=90^\circ$).
Non-Uniform Circular Motion
Velocity changes in both magnitude and direction, so the particle has both tangential and radial acceleration.
$$a_t = \dfrac{dv}{dt}, \qquad a_c = \dfrac{v^2}{r}, \qquad a = \sqrt{a_t^2 + a_c^2}$$Motion of a Cyclist
- Turning without inclination: friction supplies the centripetal force. $$\dfrac{mv^2}{r}=\mu mg \;\Rightarrow\; v_{max}=\sqrt{\mu r g}$$
- Leaning at angle $\theta$ to the vertical, the horizontal component of the ground reaction provides the centripetal force: $$\tan\theta = \dfrac{v^2}{rg}$$
Condition for skidding
When the centripetal force required for the turn is greater than the frictional force the tyres can provide, skidding occurs. If $\mu$ is the coefficient of friction between the road and the tyre, the limiting friction (frictional force) is $f = \mu R$, where the normal reaction $R = mg$, so $\;\therefore f = \mu (mg)$.
Step 1 — Skidding requirement
For skidding, centripetal force $>$ frictional force:
$$\frac{mv^2}{r} > \mu (mg) \;\;\Rightarrow\;\; \frac{v^2}{rg} > \mu$$Step 2 — Relate to the angle of banking
But $\dfrac{v^2}{rg} = \tan\theta$, therefore:
i.e. when the tangent of the angle of banking is greater than the coefficient of friction, skidding occurs.
Body in a Vertical Circle
- Energy conservation: $v_A^2 - v_C^2 = 4gr$.
- Critical speeds: lowest $v_A=\sqrt{5gr}$, top $v_C=\sqrt{gr}$.
- If $v_A \le \sqrt{2gr}$ the body oscillates; if $\sqrt{2gr} < v_A < \sqrt{5gr}$ it leaves the circular path before reaching the top.
Full derivation — tension & critical speeds
A body of mass $m$ is whirled on a string of length $r$ in a vertical circle. Let A be the lowest point, C the highest point, and P a general point where the string makes an angle $\theta$ with the downward vertical.
Step 1 — Tension at a general point
At P, the net force towards the centre is the tension minus the radial component of the weight, and this must equal the centripetal force:
$$T - mg\cos\theta = \frac{mv^2}{r} \;\;\Rightarrow\;\; T = \frac{mv^2}{r} + mg\cos\theta$$Step 2 — Tension at special points
Substituting $\theta = 0^\circ,\ 90^\circ,\ 180^\circ$:
$$T_A = \frac{mv_A^2}{r} + mg \;(\text{max}), \qquad T_{horiz} = \frac{mv^2}{r}, \qquad T_C = \frac{mv_C^2}{r} - mg \;(\text{min})$$Step 3 — Energy conservation from A to C
Rising from bottom to top lifts the body a height $2r$. Mechanical energy is conserved:
$$\frac{1}{2}mv_A^2 = \frac{1}{2}mv_C^2 + mg(2r) \;\;\Rightarrow\;\; v_A^2 = v_C^2 + 4gr \tag{1}$$Step 4 — Condition to complete the circle
The string must stay taut at the top, i.e. $T_C \ge 0$:
$$\frac{mv_C^2}{r} \ge mg \;\;\Rightarrow\;\; v_C \ge \sqrt{gr}$$Step 5 — Minimum speed at the bottom
Putting the minimum top speed $v_C^2 = gr$ into (1):
$$v_A^2 = gr + 4gr = 5gr$$Step 6 — Difference of extreme tensions
$$T_A - T_C = \frac{m(v_A^2 - v_C^2)}{r} + 2mg = \frac{m(4gr)}{r} + 2mg = 6mg$$With the critical speeds, the bottom tension itself is $T_A = \dfrac{m(5gr)}{r} + mg = 6mg$, while the top tension just reaches zero.
Conical Pendulum
Full derivation — speed, tension & time period
A bob of mass $m$ hangs from a string of length $l$ and is whirled so that it traces a horizontal circle of radius $r$ while the string sweeps a cone of semi-vertical angle $\theta$. The bob is a depth $h$ below the point of suspension, so $r = l\sin\theta$ and $h = l\cos\theta$.
Step 1 — Resolve the tension
Two forces act on the bob: the weight $mg$ (down) and the string tension $T$ (along the string). Resolving $T$ vertically and horizontally:
$$T\cos\theta = mg \tag{1}$$ $$T\sin\theta = \frac{mv^2}{r} \tag{2}$$(1) holds because the bob stays at a constant height; (2) because the horizontal component must supply the centripetal force of the circular motion.
Step 2 — Divide (2) by (1)
$$\tan\theta = \frac{v^2}{rg} \;\;\Rightarrow\;\; v = \sqrt{rg\tan\theta}$$A faster bob therefore swings out to a larger angle $\theta$.
Step 3 — Magnitude of the tension
Squaring and adding (1) and (2), using $\sin^2\theta+\cos^2\theta=1$:
$$T^2 = (mg)^2 + \left(\frac{mv^2}{r}\right)^2 \;\;\Rightarrow\;\; T = m\sqrt{g^2 + \frac{v^4}{r^2}}$$Step 4 — Time period
One revolution covers the circumference $2\pi r$ at speed $v$:
$$t = \frac{2\pi r}{v} = \frac{2\pi r}{\sqrt{rg\tan\theta}} = 2\pi\sqrt{\frac{r}{g\tan\theta}}$$Substituting $r = l\sin\theta$ and $\tan\theta = \dfrac{\sin\theta}{\cos\theta}$:
$$t = 2\pi\sqrt{\frac{l\sin\theta\cos\theta}{g\sin\theta}}$$As $\theta \to 90^\circ$, $\cos\theta \to 0$: the required speed $v \to \infty$ and $t \to 0$ — the string can never become horizontal.
Centripetal & Centrifugal Force
- Centripetal force is real and acts radially inward: $F_c=\dfrac{mv^2}{r}$.
- Centrifugal force is a pseudo force felt in the rotating frame, directed radially outward — it is what presses a car passenger against the door on a turn.
- Release the string and the stone flies off tangentially, along its instantaneous velocity.
High-Yield Points
Derivation — particle slipping off a smooth sphere
A particle starts from rest at the top of a smooth (frictionless) sphere of radius $R$ and slides down the outside. Let P be a point where the radius to the particle makes an angle $\theta$ with the upward vertical; the particle has then descended a height $R(1-\cos\theta)$.
Step 1 — Speed from energy conservation
The surface is smooth, so mechanical energy is conserved between the top and P:
$$\frac{1}{2}mv^2 = mgR(1-\cos\theta) \;\;\Rightarrow\;\; v^2 = 2gR(1-\cos\theta) \tag{1}$$Step 2 — Radial (centripetal) equation at P
The component of gravity along the radius, less the normal reaction $N$, provides the centripetal force:
$$mg\cos\theta - N = \frac{mv^2}{R} \tag{2}$$Step 3 — Condition for leaving the surface
The particle leaves the sphere where the contact is lost, i.e. $N = 0$:
$$mg\cos\theta = \frac{mv^2}{R} \;\;\Rightarrow\;\; v^2 = gR\cos\theta \tag{3}$$Step 4 — Equate (1) and (3)
$$gR\cos\theta = 2gR(1-\cos\theta) \;\;\Rightarrow\;\; \cos\theta = 2 - 2\cos\theta \;\;\Rightarrow\;\; \cos\theta = \frac{2}{3}$$Step 5 — Height above the centre
The height of P above the centre of the sphere is $h = R\cos\theta$, so:
The particle therefore flies off after dropping a vertical height $\dfrac{R}{3}$ from the top.
Challenge Questions
These higher-order questions go a step beyond the past-paper set — combining energy, friction and vector ideas from circular motion. Try each one before revealing the answer.