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Cambridge IGCSE Physics (0625) · Topic 3 — Waves
Mini-Lesson

Waves

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.

energy travels →, but the particles only oscillate up and down

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 (e.g. light) amplitude crest trough wave direction wavelength λ Longitudinal (e.g. sound) compression rarefaction
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.

Supplement Supplement — 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.

glass (denser) air normal i r i > r → bends towards 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)
cladding (less dense) cladding (less dense) in angle > c → TIR
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.

F F object real image
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.

white light red (least bent) violet (most bent)
Red is refracted least, violet most — the order is red, orange, yellow, green, blue, indigo, violet.

Supplement Supplement — 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)
Radio Micro Infrared Visible UV X-ray Gamma ⟵ longer wavelength shorter wavelength ⟶ lower frequency / energy higher frequency / energy
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.
  • Infrared — remote controls, thermal imaging, optical fibres; danger: skin burns.
  • Visible light — vision, photography, illumination.
  • Ultraviolet — security marks, sun-tanning, sterilising; danger: skin cancer and eye damage.
  • X-rays — medical imaging, airport security; danger: ionising, can cause cell mutation.
  • Gamma rays — sterilising equipment, killing cancer cells; danger: highly ionising.

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.

Supplement Supplementultrasound 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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