This mini-lesson walks you through the whole of Cambridge IGCSE Topic 3 — Waves: the general properties shared by every wave, how light reflects and refracts, the electromagnetic spectrum, and how sound travels.
Work through each screen, answer the questions as you go (some are wordy, some are calculations) and collect ⭐ stars. Supplement-only content is flagged with a Supplement badge. Press Start when you're ready.
3.1 General properties
What a wave is
A wave transfers energy from one place to another without transferring matter. As a wave passes, the particles only oscillate about a fixed point — they don't travel along with the wave.
Amplitude — the distance from the rest (equilibrium) position to the maximum displacement.
Wavelength (λ) — the distance from one point on a wave to the same point on the next wave.
Frequency (f) — the number of waves passing a point each second, measured in hertz (Hz).
Period (T) — the time for one complete wave to pass.
Wavefront — a line joining points that are all in the same part of their oscillation (e.g. all crests).
Watch out: a floating cork bobs up and down as ripples pass — it doesn't get carried to the shore. That's the key idea: waves carry energy, not matter.
3.1 General properties
Transverse vs longitudinal
Waves come in two kinds, sorted by the direction the particles vibrate compared to the direction the wave travels.
Transverse: particles vibrate at right angles to the wave. Longitudinal: particles vibrate along the wave.
In a transverse wave the vibration is at right angles to the direction of travel (peaks and troughs). In a longitudinal wave the vibration is along the direction of travel (compressions and rarefactions).
Quick check
Which type of wave?
?A sound wave moves through air as a series of compressions and rarefactions. The air particles vibrate back and forth along the same line the sound travels. What kind of wave is this?
3.1 General properties
The wave equation
Speed, frequency and wavelength are tied together for every wave:
v = f λwave speed (m/s) = frequency (Hz) × wavelength (m)
And frequency and period are reciprocals of each other:
T = 1 / fperiod (s) = 1 ÷ frequency (Hz)
Worked example
A water wave has frequency 5 Hz and wavelength 0.4 m.
v = f λ = 5 × 0.4 = 2 m/s
Its period: T = 1 ÷ f = 1 ÷ 5 = 0.2 s
Rearranging: f = v ÷ λ and λ = v ÷ f. Cover the symbol you want in the triangle to find which way to divide.
Calculate
Your turn — wave speed
1A wave on a rope has a frequency of 8 Hz and a wavelength of 0.25 m. Calculate its speed.
m/s
Hint: v = f λ = 8 × 0.25.
Calculate
Your turn — rearranging
2A sound wave travels at 340 m/s with a frequency of 170 Hz. Calculate its wavelength.
m
Hint: rearrange v = f λ to λ = v ÷ f = 340 ÷ 170.
Calculate
Your turn — period
3A vibrating tuning fork produces a wave of frequency 250 Hz. Calculate the period of the wave.
s
Hint: T = 1 ÷ f = 1 ÷ 250.
3.1 General properties
Reflection, refraction & diffraction
In a ripple tank you can watch wavefronts behave in three ways:
Reflection — waves bounce off a barrier. The angle of incidence = angle of reflection; speed, frequency and wavelength are unchanged.
Refraction — waves change speed when they pass into shallower water. Frequency stays the same, so the wavelength changes and the wavefronts bend.
Diffraction — waves spread out after passing through a gap or around an edge.
SupplementSupplement — diffraction is greatest when the gap is about the same size as the wavelength. A wide gap diffracts only a little at the edges; a narrow gap spreads the waves into strong semicircles.
3.2 Light
Reflection & the plane mirror
The law of reflection says the angle of incidence equals the angle of reflection, both measured from the normal (the line at 90° to the surface).
The image you see in a plane mirror is:
Upright and the same size as the object.
The same distance behind the mirror as the object is in front.
Virtual (the light only appears to come from behind the mirror) and laterally inverted.
Watch out: always measure angles from the normal, never from the mirror surface itself.
3.2 Light
Refraction through glass
When light enters a denser medium (air → glass) it slows down and bends towards the normal. Leaving the glass it speeds up and bends away from the normal.
Entering denser glass, the ray bends towards the normal, so angle r is smaller than angle i.
Misconception: refraction happens because the wave's speed changes, not because the glass "pulls" the light. The frequency stays the same; the wavelength changes.
Quick check
Which way does it bend?
?A ray of light passes from water into air at an angle to the normal. Air is the less dense medium. What happens to the ray?
3.2 Light · Supplement
Refractive index Supplement
The refractive index n measures how much a material bends light. From Snell's law:
n = sin i / sin rrefractive index = sin(angle of incidence) ÷ sin(angle of refraction)
It is also the ratio of the speed of light in a vacuum to the speed in the medium — a bigger n means a slower, more strongly bending medium.
Worked example
Light hits glass at i = 50° and refracts to r = 30°.
n = sin 50° ÷ sin 30° = 0.766 ÷ 0.500 = 1.53
Calculate · Supplement
Your turn — refractive index Supplement
4A ray enters a transparent block at an angle of incidence of 45° and refracts to an angle of 28°. Calculate the refractive index. (sin 45° = 0.707, sin 28° = 0.469.)
Hint: n = sin i ÷ sin r = 0.707 ÷ 0.469.
3.2 Light · Supplement
Total internal reflection Supplement
When light travels from a denser medium towards a less dense one, increasing the angle of incidence eventually reaches the critical angle (c) — where the refracted ray skims along the boundary at 90°. Beyond it, all the light reflects back: total internal reflection (TIR).
n = 1 / sin crefractive index = 1 ÷ sin(critical angle)
In an optical fibre every bounce has an angle greater than the critical angle, so no light escapes.
This is how optical fibres carry light (and data) around bends — used in high-speed communications and in medical endoscopes.
Calculate · Supplement
Your turn — critical angle Supplement
5A type of glass has a critical angle of 42°. Calculate its refractive index. (sin 42° = 0.669.)
Hint: n = 1 ÷ sin c = 1 ÷ 0.669.
3.2 Light
The converging lens
A converging (convex) lens refracts parallel rays so they meet at the principal focus (F). The distance from the lens to F is the focal length.
An object beyond 2F gives a real, inverted, diminished image on the far side — as in a camera.
When the object is further than F, the image is real and inverted (it can be caught on a screen). When the object is closer than F, the image is virtual, upright and magnified — the magnifying-glass effect.
3.2 Light · Supplement
Magnification Supplement
Magnification compares the image size to the object size:
m = image height / object heightmagnification has no units
A magnification greater than 1 means the image is enlarged; less than 1 means diminished.
Worked example
An object 2 cm tall forms an image 6 cm tall.
m = 6 ÷ 2 = 3 (the image is three times larger).
Calculate · Supplement
Your turn — magnification Supplement
6A converging lens forms an image 12 cm tall of an object that is 3 cm tall. Calculate the magnification.
Hint: m = image height ÷ object height = 12 ÷ 3.
3.2 Light
Dispersion of white light
White light is a mixture of colours. A glass prism refracts each colour by a slightly different amount (violet most, red least), spreading them into a spectrum — this is dispersion.
Red is refracted least, violet most — the order is red, orange, yellow, green, blue, indigo, violet.
SupplementSupplement — light of a single frequency (a single colour) is described as monochromatic.
3.3 Electromagnetic spectrum
The electromagnetic spectrum
All electromagnetic (EM) waves are transverse, need no medium, and travel through a vacuum at the same speed:
c = 3 × 10⁸ m/sthe speed of all EM waves in a vacuum (and ≈ in air)
Order to memorise: Radio → Microwave → Infrared → Visible → Ultraviolet → X-ray → Gamma.
Misconception: gamma rays are not faster than radio waves. In a vacuum all EM waves travel at c — gamma simply has a much higher frequency and shorter wavelength.
3.3 Electromagnetic spectrum
Uses & dangers
Radio — TV and radio broadcasting, astronomy, RFID.
Microwaves — satellite TV, mobile phones, microwave cooking. Supplement phones & Wi-Fi use microwaves because they pass through some walls and need only a short aerial.
Pattern: the higher the frequency, the greater the energy. UV, X-rays and gamma are ionising, which is why over-exposure is so harmful.
Quick check
EM spectrum check
?Which statement about the electromagnetic spectrum is correct?
3.4 Sound
Sound waves
Sound is a longitudinal wave made by a vibrating source. It travels as compressions (particles squeezed together) and rarefactions (particles spread apart), and it needs a medium — it cannot travel through a vacuum.
The louder the sound, the larger the amplitude.
The higher the pitch, the greater the frequency.
A healthy human ear hears from 20 Hz to 20 000 Hz.
The speed of sound in air is about 330–350 m/s (much slower than light) and faster in liquids and solids.
Misconception: sound cannot travel through empty space. In a vacuum there are no particles to compress, so a ringing bell inside a vacuum jar falls silent.
3.4 Sound
Echoes & measuring the speed of sound
An echo is sound reflected off a hard surface. You can measure the speed of sound by clapping a known distance from a wall and timing the echo — remembering the sound travels there and back.
Worked example
A clap echoes off a cliff 165 m away after 1.0 s.
Total distance = 2 × 165 = 330 m. Speed = distance ÷ time = 330 ÷ 1.0 = 330 m/s.
SupplementSupplement — ultrasound is sound above 20 000 Hz. It is partly reflected at boundaries, so a transceiver can use the echoes for SONAR depth-finding and for medical scans without ionising radiation.
Calculate
Your turn — speed of sound
7A student stands 170 m from a large wall and claps. The echo returns after 1.0 s. Calculate the speed of sound in air. (Remember the sound travels to the wall and back.)
m/s
Hint: total distance = 2 × 170 = 340 m; speed = distance ÷ time.
Sort it
Name the wave behaviour
Tap the word that describes what is happening to the wave in each case.
Sort it
Longer or shorter wavelength than visible light?
Tap an EM region, then tap the box for whether its wavelength is longer or shorter than visible light.
📻 Longer than visible
⚡ Shorter than visible
Recap
The equations to know
Wave speed: v = f λ
Period: T = 1 ÷ f
Refractive index Supplement: n = sin i ÷ sin r
Critical angle Supplement: n = 1 ÷ sin c
Magnification Supplement: m = image height ÷ object height
Speed of EM waves in a vacuum: c = 3 × 10⁸ m/s
You've covered all four parts of Cambridge IGCSE Topic 3 — general wave properties, light, the electromagnetic spectrum and sound. Press Finish to see your score.
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