Rotational Motion

Circular Motion Fundamentals

Angular Quantities

Quantity	Symbol	SI Unit	Relation to Linear
Angular displacement	$\theta$	rad	$s = r\theta$
Angular velocity	$\omega$	rad/s	$v = r\omega$
Angular acceleration	$\alpha$	rad/s $^2$	$a_t = r\alpha$

Angular Velocity

\omega = \frac{\Delta\theta}{\Delta t}

For uniform circular motion, $\omega$ is constant.

Period and Frequency

T = \frac{2\pi}{\omega}, \quad f = \frac{1}{T} = \frac{\omega}{2\pi}

Where $T$ is the period (time for one revolution) and $f$ is the frequency (revolutions per second).

Relation to Linear Speed

V = r\omega = \frac{2\pi r}{T} = 2\pi rf

Example

A CD rotates at $200\mathrm{ rpm}$ . Find the angular velocity in rad/s and the linear speed of a Point $5\mathrm{ cm}$ from the centre.

\omega = 200 \times \frac{2\pi}{60} = \frac{400\pi}{60} = 20.9\mathrm{ rad/s}

V = r\omega = 0.05 \times 20.9 = 1.05\mathrm{ m/s}

Centripetal Acceleration

An object in uniform circular motion has a constantly changing velocity (direction changes), so it Is always accelerating toward the centre of the circle.

Magnitude

A_c = \frac{v^2}{r} = \omega^2 r = \frac{4\pi^2 r}{T^2}

Direction

Always directed toward the centre of the circular path (radially inward).

Key Points

Centripetal acceleration changes the direction of velocity, not its magnitude.
If the centripetal force is removed, the object moves in a straight line (tangent to the circle) by Newton”s first law.
The word “centripetal” means “centre-seeking.”

Centripetal force is NOT a new force — it is the NET force toward the centre provided by existing Forces (gravity, tension, friction, normal force, etc.). Never include “centripetal force” as a Separate force on a free-body diagram.

Centripetal Force

Magnitude

F_c = ma_c = \frac{mv^2}{r} = m\omega^2 r

Direction

Always directed toward the centre of the circle.

Common Examples

Situation	Centripetal Force Provided By
Car turning on a flat road	Friction between tyres and road
Car on a banked curve	Horizontal component of normal force
Satellite in orbit	Gravitational force
Object on a string (horizontal circle)	Tension in the string
Conical pendulum	Horizontal component of tension
Motorcyclist in vertical circle	Combination of weight and normal reaction

Horizontal Circular Motion

Object on a String

For an object of mass $m$ on a string of length $r$ moving in a horizontal circle at speed $v$ :

T = \frac{mv^2}{r}

Where $T$ is the tension in the string (horizontal).

Conical Pendulum

A mass $m$ on a string of length $L$ traces a horizontal circle of radius $r$ at angle $\theta$ to The vertical.

Vertical: $T\cos\theta = mg$

Horizontal: $T\sin\theta = \dfrac{mv^2}{r}$

Dividing: $\tan\theta = \dfrac{v^2}{rg}$

The radius: $r = L\sin\theta$

The period: $T_p = 2\pi\sqrt{\dfrac{L\cos\theta}{g}}$

Example

A $0.5\mathrm{ kg}$ mass on a string of length $1\mathrm{ m}$ moves in a horizontal circle at $3\mathrm{ m/s}$ . Find the angle the string makes with the vertical and the tension.

\tan\theta = \frac{v^2}`\{rg}` = \frac{9}{r \times 9.81}

Also $r = L\sin\theta = \sin\theta$ So:

\tan\theta = \frac{9}{9.81\sin\theta}

\frac{\sin\theta}{\cos\theta} = \frac{0.917}{\sin\theta}

\sin^2\theta = 0.917\cos\theta

1 - \cos^2\theta = 0.917\cos\theta

Let $u = \cos\theta$ : $u^2 + 0.917u - 1 = 0$ .

U = \frac{-0.917 + \sqrt{0.841 + 4}}{2} = \frac{-0.917 + 2.200}{2} = 0.642

$\theta = \arccos(0.642) = 50.1\degree$ .

T = \frac`\{mg}`{\cos\theta} = \frac{0.5 \times 9.81}{0.642} = 7.64\mathrm{ N}

Vertical Circular Motion

For an object moving in a vertical circle, the speed varies (it is fastest at the bottom, slowest at The top) because gravity does work.

At the Bottom of the Circle

T - mg = \frac{mv_{\mathrm{bottom}}^2}{r} \implies T = mg + \frac{mv_{\mathrm{bottom}}^2}{r}

At the Top of the Circle

T + mg = \frac{mv_{\mathrm{top}}^2}{r} \implies T = \frac{mv_{\mathrm{top}}^2}{r} - mg

Minimum Speed at the Top

For the object to complete the full circle, $T \ge 0$ at the top:

\frac{mv_{\mathrm{top}}^2}{r} \ge mg \implies v_{\mathrm{top}} \ge \sqrt`\{gr}`

Energy Conservation in Vertical Circles

\frac{1}{2}mv_{\mathrm{bottom}}^2 = \frac{1}{2}mv_{\mathrm{top}}^2 + mg(2r)

V_{\mathrm{bottom}}^2 = v_{\mathrm{top}}^2 + 4gr

For minimum speed at the top ( $v_{\mathrm{top}} = \sqrt{gr}$ ):

V_{\mathrm{bottom}} = \sqrt{5gr}

Example

A $0.3\mathrm{ kg}$ ball on a string of length $0.8\mathrm{ m}$ is swung in a vertical circle. Find The minimum speed at the bottom for the ball to complete the circle.

V_{\mathrm{bottom}} = \sqrt{5gr} = \sqrt{5(9.81)(0.8)} = \sqrt{39.24} = 6.26\mathrm{ m/s}

Banked Curves

Without Friction

For a car on a banked curve at angle $\theta$ with radius $r$ at speed $v$ :

Vertical: $N\cos\theta = mg$

Horizontal: $N\sin\theta = \dfrac{mv^2}{r}$

Dividing: $\tan\theta = \dfrac{v^2}{rg}$

The ideal (no friction needed) speed:

V = \sqrt{rg\tan\theta}

With Friction

When friction is present, the car can travel at speeds above or below the ideal speed. Friction acts Up the slope (to prevent sliding down) or down the slope (to prevent sliding up).

Torque

Definition

Torque (moment of force) is the rotational equivalent of force:

\tau = Fd\sin\theta = Fr_\perp

Where:

$F$ is the force
$d$ is the distance from the axis (pivot) to the point of application
$\theta$ is the angle between the force and the line from pivot to application point
$r_\perp = d\sin\theta$ is the perpendicular distance from the axis to the line of action (moment arm)

SI Unit

The unit of torque is $\mathrm{N}\cdot\mathrm{m}$ (newton-metre).

Torque and Angular Acceleration

Newton’s second law for rotation:

\tau_{\mathrm{net}} = I\alpha

Where $I$ is the moment of inertia and $\alpha$ is the angular acceleration.

Equilibrium Conditions

For an object in static equilibrium:

Translational: $\sum \vec{F} = 0$ (no net force)
Rotational: $\sum \tau = 0$ (no net torque)

The second condition must hold about ANY axis.

Example

A uniform beam of mass $10\mathrm{ kg}$ and length $4\mathrm{ m}$ is supported at its ends. A $20\mathrm{ kg}$ mass hangs $1\mathrm{ m}$ from the left end. Find the support forces.

Taking moments about the left end (clockwise positive):

R_{\mathrm{right}} \times 4 - 10g \times 2 - 20g \times 1 = 0

4R_{\mathrm{right}} = 196.2 + 196.2 = 392.4

R_{\mathrm{right}} = 98.1\mathrm{ N}

By vertical equilibrium:

R_{\mathrm{left}} + R_{\mathrm{right}} = 10g + 20g = 294.3\mathrm{ N}

R_{\mathrm{left}} = 294.3 - 98.1 = 196.2\mathrm{ N}

Moment of Inertia

Definition

The moment of inertia $I$ measures an object’s resistance to angular acceleration:

I = \sum m_i r_i^2

For a continuous body:

I = \int r^2\,dm

Common Moments of Inertia

Object	Axis	$I$
Solid cylinder/disk	Central axis	$\dfrac{1}{2}MR^2$
Hollow cylinder	Central axis	$MR^2$
Solid sphere	Diameter	$\dfrac{2}{5}MR^2$
Hollow sphere	Diameter	$\dfrac{2}{3}MR^2$
Thin rod (centre)	Perpendicular through centre	$\dfrac{1}{12}ML^2$
Thin rod (end)	Perpendicular through end	$\dfrac{1}{3}ML^2$
Point mass	At distance $r$	$Mr^2$

Parallel Axis Theorem

For a body of mass $M$ with moment of inertia $I_{\mathrm{cm}}$ about an axis through its centre of Mass:

I = I_{\mathrm{cm}} + Md^2

Where $d$ is the distance between the original axis and the parallel axis through the centre of Mass.

Angular Momentum

Definition

\vec{L} = I\vec{\omega}

For a point mass: $L = mvr = mr^2\omega$ .

SI Unit

$\mathrm{kg}\cdot\mathrm{m}^2/\mathrm{s}$ .

Conservation of Angular Momentum

In a closed system with no external torques:

I_1\omega_1 = I_2\omega_2

Applications

Ice skater spinning: Pulling arms in reduces $I$ So $\omega$ increases.
Diving: Tucking reduces $I$ Increasing angular velocity for flips.
Figure skater: Extending arms increases $I$ Decreasing $\omega$ for a controlled landing.

Example

A figure skater with arms extended has $I = 4.5\mathrm{ kg}\cdot\mathrm{m}^2$ and spins at $2\mathrm{ rad/s}$ . She pulls her arms in, reducing $I$ to $1.5\mathrm{ kg}\cdot\mathrm{m}^2$ . Find Her new angular velocity.

I_1\omega_1 = I_2\omega_2

4.5 \times 2 = 1.5 \times \omega_2

\omega_2 = 6\mathrm{ rad/s}

Her angular velocity triples.

Angular Impulse

\Delta L = \tau \cdot \Delta t

This is analogous to linear impulse: $\Delta p = F \cdot \Delta t$ .

Rotational Kinetic Energy

Formula

E_{k,\mathrm{rot}} = \frac{1}{2}I\omega^2

Total Kinetic Energy of a Rolling Object

For an object that rolls without slipping:

E_k = \frac{1}{2}mv^2 + \frac{1}{2}I\omega^2

Since $v = r\omega$ for rolling without slipping:

E_k = \frac{1}{2}mv^2 + \frac{1}{2}I\frac{v^2}{r^2} = \frac{1}{2}\left(m + \frac{I}{r^2}\right)v^2

Rolling Down an Incline

For an object rolling down a frictionless-free incline (rolling without slipping):

Mgh = \frac{1}{2}mv^2 + \frac{1}{2}I\omega^2

V = \sqrt{\frac{2gh}{1 + \frac{I}{Mr^2}}}

Example

Compare the speeds of a solid sphere, a hollow sphere, and a solid cylinder rolling down the same Incline from the same height.

Solid sphere: $I = \dfrac{2}{5}Mr^2 \implies v = \sqrt{\dfrac{10gh}{7}}$
Hollow sphere: $I = \dfrac{2}{3}Mr^2 \implies v = \sqrt{\dfrac{6gh}{5}}$
Solid cylinder: $I = \dfrac{1}{2}Mr^2 \implies v = \sqrt{\dfrac{4gh}{3}}$

The solid sphere is fastest, followed by the solid cylinder, then the hollow sphere. Objects with More mass concentrated near the centre (smaller $I$ ) roll faster.

Analogy: Linear vs Rotational

Linear Quantity	Rotational Equivalent
Displacement $s$	Angular displacement $\theta$
Velocity $v$	Angular velocity $\omega$
Acceleration $a$	Angular acceleration $\alpha$
Mass $m$	Moment of inertia $I$
Force $F$	Torque $\tau$
Momentum $p = mv$	Angular momentum $L = I\omega$
$F = ma$	$\tau = I\alpha$
$E_k = \frac{1}{2}mv^2$	$E_k = \frac{1}{2}I\omega^2$
$W = Fs$	$W = \tau\theta$
$P = Fv$	$P = \tau\omega$

IB Exam-Style Questions

Question 1 (Paper 1 style)

A car of mass $1200\mathrm{ kg}$ travels around a circular bend of radius $50\mathrm{ m}$ at $15\mathrm{ m/s}$ . Find the minimum coefficient of static friction required.

\frac{mv^2}{r} \le \mu_s mg

\mu_s \ge \frac{v^2}`\{rg}` = \frac{225}{50 \times 9.81} = \frac{225}{490.5} = 0.459

Question 2 (Paper 2 style)

A satellite orbits Earth at an altitude of $400\mathrm{ km}$ in a circular orbit.

(a) Calculate the orbital period.

( $M_E = 5.97 \times 10^{24}\mathrm{ kg}$ , $R_E = 6.37 \times 10^6\mathrm{ m}$ )

R = 6.77 \times 10^6\mathrm{ m}

\frac`\{GMm}`{r^2} = \frac{mv^2}{r} \implies v = \sqrt{\frac`\{GM}`{r}} = \sqrt{\frac{3.98 \times 10^{14}}{6.77 \times 10^6}} = 7669\mathrm{ m/s}

T = \frac{2\pi r}{v} = \frac{2\pi \times 6.77 \times 10^6}{7669} = 5544\mathrm{ s} \approx 92.4\mathrm{ min}

(b) Calculate the centripetal acceleration.

A_c = \frac{v^2}{r} = \frac{5.88 \times 10^7}{6.77 \times 10^6} = 8.68\mathrm{ m/s}^2

Question 3 (Paper 2 style)

A $0.2\mathrm{ kg}$ ball is attached to a string of length $0.8\mathrm{ m}$ and whirled in a Vertical circle.

(a) Find the minimum speed at the top of the circle for the ball to maintain contact.

V_{\mathrm{min}} = \sqrt`\{gr}` = \sqrt{9.81 \times 0.8} = \sqrt{7.85} = 2.80\mathrm{ m/s}

(b) If the speed at the bottom is $8\mathrm{ m/s}$ Find the tension in the string at the Bottom.

T_{\mathrm{bottom}} = mg + \frac{mv^2}{r} = 0.2(9.81) + \frac{0.2(64)}{0.8} = 1.962 + 16 = 17.96\mathrm{ N}

(c) Find the tension at the top.

First find $v_{\mathrm{top}}$ using energy conservation:

\frac{1}{2}mv_{\mathrm{bottom}}^2 = \frac{1}{2}mv_{\mathrm{top}}^2 + mg(2r)

64 = v_{\mathrm{top}}^2 + 9.81(1.6) = v_{\mathrm{top}}^2 + 15.70

V_{\mathrm{top}}^2 = 48.30 \implies v_{\mathrm{top}} = 6.95\mathrm{ m/s}

T_{\mathrm{top}} = \frac{mv_{\mathrm{top}}^2}{r} - mg = \frac{0.2(48.30)}{0.8} - 1.962 = 12.075 - 1.962 = 10.11\mathrm{ N}

Question 4 (Paper 1 style)

A disc of mass $2\mathrm{ kg}$ and radius $0.3\mathrm{ m}$ rotates at $10\mathrm{ rad/s}$ . Find its Rotational kinetic energy.

I = \frac{1}{2}MR^2 = \frac{1}{2}(2)(0.09) = 0.09\mathrm{ kg}\cdot\mathrm{m}^2

E_k = \frac{1}{2}I\omega^2 = \frac{1}{2}(0.09)(100) = 4.5\mathrm{ J}

Question 5 (Paper 2 style)

A diver has moment of inertia $15\mathrm{ kg}\cdot\mathrm{m}^2$ with arms extended and $4\mathrm{ kg}\cdot\mathrm{m}^2$ in a tucked position. She leaves the board with angular velocity $2\mathrm{ rad/s}$ (arms extended).

(a) Find her angular velocity when tucked.

I_1\omega_1 = I_2\omega_2

15 \times 2 = 4 \times \omega_2 \implies \omega_2 = 7.5\mathrm{ rad/s}

(b) How many complete somersaults can she perform in $1.2\mathrm{ s}$ while tucked?

\theta = \omega_2 \times t = 7.5 \times 1.2 = 9\mathrm{ rad}

Number of somersaults $= \dfrac{9}{2\pi} = 1.43$

She can complete 1 full somersault and is partway through a second.

Summary

Quantity	Formula
Angular velocity	$\omega = \dfrac{v}{r} = \dfrac{2\pi}{T}$
Centripetal acceleration	$a_c = \dfrac{v^2}{r} = \omega^2 r$
Centripetal force	$F_c = \dfrac{mv^2}{r} = m\omega^2 r$
Torque	$\tau = Fr_\perp$
Newton’s second law (rotation)	$\tau = I\alpha$
Angular momentum	$L = I\omega$
Rotational kinetic energy	$E_k = \dfrac{1}{2}I\omega^2$
Conservation of angular momentum	$I_1\omega_1 = I_2\omega_2$

Example

A flywheel starts from rest and accelerates uniformly at $2\mathrm{ rad/s}^2$ for $5\mathrm{ s}$ .

(a) Find the angular velocity after $5\mathrm{ s}$ .

\omega = 0 + 2 \times 5 = 10\mathrm{ rad/s}

(b) Find the number of revolutions made.

\theta = 0 + \frac{1}{2}(2)(25) = 25\mathrm{ rad}

\mathrm{Revolutions} = \frac{25}{2\pi} = 3.98

(c) Find the linear speed of a point $0.3\mathrm{ m}$ from the axis.

V = r\omega = 0.3 \times 10 = 3.0\mathrm{ m/s}

Gravitation and Circular Orbits (Extended)

Orbital Energy

For a satellite of mass $m$ in circular orbit of radius $r$ around a planet of mass $M$ :

E_{\mathrm{total}} = -\frac`\{GMm}`{2r}

E_k = \frac`\{GMm}`{2r}

E_p = -\frac`\{GMm}`{r}

Orbital Speed

V = \sqrt{\frac`\{GM}`{r}}

Orbital Period (Kepler’s Third Law)

T^2 = \frac{4\pi^2}`\{GM}`R^3

$T^2$ is proportional to $r^3$ for all satellites orbiting the same body.

Geostationary Orbits

A geostationary satellite:

Orbits above the equator.
Has a period of 24 hours (matches Earth’s rotation).
Remains above the same point on Earth’s surface.
Orbital radius $\approx 42200\mathrm{ km}$ from Earth’s centre.

Gyroscopic Effects

A spinning gyroscope resists changes to its axis of rotation due to conservation of angular Momentum. This principle is used in:

Navigation systems (gyrocompasses).
Stabilisation of ships and aircraft.
Bicycle stability.
Smartphone orientation sensors.

Precession

When a torque is applied to a spinning object, instead of tipping over, the axis of rotation moves Perpendicular to the applied torque. This is called precession.

The precession angular velocity:

\omega_p = \frac{\tau}{L}

Additional IB Exam-Style Questions

Question 6 (Paper 2 style)

A disc of mass $5\mathrm{ kg}$ and radius $0.2\mathrm{ m}$ rotates about its central axis. A Constant torque of $0.5\mathrm{ N}\cdot\mathrm{m}$ is applied for $4\mathrm{ s}$ Starting from Rest.

(a) Find the angular acceleration.

\alpha = \frac{\tau}{I} = \frac{0.5}{\frac{1}{2}(5)(0.04)} = \frac{0.5}{0.1} = 5\mathrm{ rad/s}^2

(b) Find the angular velocity after $4\mathrm{ s}$ .

\omega = 0 + 5 \times 4 = 20\mathrm{ rad/s}

(c) Find the rotational kinetic energy after $4\mathrm{ s}$ .

E_k = \frac{1}{2}I\omega^2 = \frac{1}{2}(0.1)(400) = 20\mathrm{ J}

(d) Find the work done by the torque.

W = \tau\theta = \tau \cdot \frac{1}{2}\alpha t^2 = 0.5 \times \frac{1}{2}(5)(16) = 20\mathrm{ J}

This equals the change in rotational kinetic energy, confirming the work-energy theorem.

Question 7 (Paper 2 style)

A thin rod of mass $2\mathrm{ kg}$ and length $1\mathrm{ m}$ is pivoted at one end and held Horizontally. It is released from rest.

(a) Find the moment of inertia about the pivot.

I = \frac{1}{3}ML^2 = \frac{1}{3}(2)(1) = 0.667\mathrm{ kg}\cdot\mathrm{m}^2

(b) Find the initial angular acceleration.

The torque about the pivot: $\tau = mg \times \dfrac{L}{2} = 2(9.81)(0.5) = 9.81\mathrm{ N}\cdot\mathrm{m}$ .

\alpha = \frac{\tau}{I} = \frac{9.81}{0.667} = 14.7\mathrm{ rad/s}^2

(c) Find the angular velocity as the rod passes through the vertical.

Using conservation of energy (taking the pivot as reference):

Loss of $E_p$ : the centre of mass falls by $\dfrac{L}{2} = 0.5\mathrm{ m}$ .

Mg\frac{L}{2} = \frac{1}{2}I\omega^2

2(9.81)(0.5) = \frac{1}{2}(0.667)\omega^2

9.81 = 0.333\omega^2 \implies \omega = \sqrt{29.4} = 5.42\mathrm{ rad/s}

Question 8 (Paper 1 style)

A horizontal turntable of radius $0.5\mathrm{ m}$ rotates at $3\mathrm{ rad/s}$ . A coin is placed on The turntable at a distance $0.3\mathrm{ m}$ from the centre. If the coefficient of static friction Is $0.4$ Does the coin slip?

A_c = \omega^2 r = 9 \times 0.3 = 2.7\mathrm{ m/s}^2

Required friction: $f = ma_c = m \times 2.7$ .

Maximum available friction: $f_{\max} = \mu_s mg = 0.4m(9.81) = 3.924m$ .

Since $2.7m \lt 3.924m$ The coin does not slip.

For the A-Level treatment of this topic, see Circular Motion.

:::tip Diagnostic Test Ready to test your understanding of Rotational Motion? The contains the hardest questions within the IB specification for this topic, each with a full worked solution.

Unit tests probe edge cases and common misconceptions. Integration tests combine Rotational Motion with other physics topics to test synthesis under exam conditions.

See for instructions on self-marking and building a personal test matrix.

Common Pitfalls

Rounding intermediate answers too early, which compounds errors in multi-step calculations.
Neglecting air resistance or assuming ideal conditions when the question specifies a real-world scenario.
Using the wrong equation from the data sheet — take time to read the full equation, including conditions and variable definitions.
Confusing scalar and vector quantities — always check whether direction matters for the quantity in question.

Cross-References

Topic	Site	Link
[Circular Motion]	A-Level	View
[Circular Motion]	IB	View

Worked Examples

Worked examples demonstrating the application of key concepts are covered in the detailed sub-pages linked above.

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