Refraction and Snell's Law Revision Notes | A Level AQA Physics
Snell's law is n₁ sin θ₁ = n₂ sin θ₂, where n is refractive index and angles are measured from the normal. Free AQA notes and 13 questions answered.
Updated 12 Sept 2026 · Revise Right Team
Refraction and Snell's Law is part of Refraction, diffraction and interference in A Level AQA Physics.
5 min
Reading time
13
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A Level AQA
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What this lesson covers
Snell's law is n₁ sin θ₁ = n₂ sin θ₂, where n is refractive index and angles are measured from the normal. Free AQA notes and 13 questions answered.
Define refractive index and calculate it using the ratio of the speed of light in a vacuum to the speed of light in a substance
Apply Snell's law at a boundary between two media to calculate angles of refraction or refractive indices
Explain why light changes direction when it crosses a boundary between media of different refractive indices
Recall that the refractive index of air is approximately 1 and use this to simplify Snell's law calculations
Key ideas to keep in view
Use this lesson to stay inside Refraction, diffraction and interference while connecting the detail back to the wider Waves topic.
Refractive index: A dimensionless ratio that describes how much slower light travels in a substance compared to in a vacuum. Defined as n = c / c_s, where c is the speed of light in a vacuum and c_s is the speed of light in the substance.
Snell's law: A relationship governing refraction at a boundary between two media: n_1 sin θ_1 = n_2 sin θ_2, where n_1 and n_2 are the refractive indices of the two media and θ_1 and θ_2 are the angles of incidence and refraction measured from the normal.
Normal: An imaginary line drawn perpendicular to a surface at the point where a ray meets it. All angles in refraction problems are measured from the normal, not from the surface itself.
Angle of refraction: The angle between the refracted ray and the normal on the transmitted side of a boundary. It differs from the angle of incidence whenever the two media have different refractive indices.
Revision notes
Read the core explanations from Refraction and Snell's Law before testing yourself from memory.
1. Why Light Bends at a Boundary
Picture a ray of light travelling through air and then entering a glass block at an angle. The moment it crosses the surface, it changes direction — bending towards the normal as it slows down. That bending is refraction, and understanding it precisely is what this lesson is about.
The key physical reason is straightforward: light travels at different speeds in different materials. When a wavefront hits a boundary at an angle, one side of the wavefront slows down before the other, causing the whole wavefront to pivot. The result is a change in direction.
This is directly analogous to a car driving from tarmac onto mud at an angle — the wheel that hits the mud first slows down, and the car turns. The physics of refraction follows exactly the same geometry.
2. Refractive Index — Quantifying How Much Light Slows
To describe how much a material slows light, physicists use the refractive index, given the symbol $n$. It is defined as the ratio of the speed of light in a vacuum, $c$, to the speed of light in the substance, $c_s$.
Because light can never travel faster than $c$, the value of $c_s$ is always less than or equal to $c$. This means $n$ is always greater than or equal to 1. A higher refractive index means light travels more slowly in that material and bends more when it enters.
This approximation matters enormously in calculations. When one medium is air, Snell's law simplifies considerably — you will see this in action shortly. For now, commit this to memory: $n_{\text{air}} \approx 1$.
Some typical values worth knowing: glass has $n \approx 1.5$, water has $n \approx 1.33$, and diamond has $n \approx 2.4$. These numbers tell you that light travels roughly half as fast in diamond as it does in a vacuum.
3. Snell's Law — The Equation That Governs Refraction
Knowing that light bends at a boundary is useful, but to actually calculate angles and indices you need Snell's law. It connects the refractive indices of two media to the angles the ray makes with the normal on each side of the boundary.
The equation tells you something elegant: the product $n \sin \theta$ is conserved across a boundary. If $n_2 > n_1$ (light entering a denser medium), then $\sin \theta_2 < \sin \theta_1$, so $\theta_2 < \theta_1$ — the ray bends towards the normal. If $n_2 < n_1$ (light entering a less dense medium), the ray bends away from the normal.
When one medium is air ($n_1 = 1$), Snell's law becomes $\sin \theta_1 = n_2 \sin \theta_2$. This is the form you will use most often in AQA questions, so recognise it quickly.
4. Worked Calculations Using Snell's Law
Theory only becomes useful when you can execute it under exam conditions. The following worked examples cover the two most common question types: finding an angle of refraction and finding a refractive index. Work through each step before revealing the next — that active engagement is what builds exam fluency.
Worked example: Finding the Angle of Refraction (Air to Glass)
A ray of light travels from air into a glass block. The angle of incidence is 40°. The refractive index of the glass is 1.50. Calculate the angle of refraction. [3 marks]
$n_1 \sin \theta_1 = n_2 \sin \theta_2$ — [M1] Stating the correct relationship earns the method mark.
$n_1 = 1$ (air), $\theta_1 = 40°$, $n_2 = 1.50$, $\theta_2 =?$ — Label each quantity before substituting. This prevents sign and index errors.
$\theta_2 = \sin^{-1}(0.4285) = 25.4°$ — [A1] Answer to 3 significant figures, consistent with the data given.
Answer: $\theta_2 = 25.4°$ (the ray bends towards the normal, as expected when entering a denser medium)
Notice the sanity check built into that answer: the refracted angle (25.4°) is smaller than the incident angle (40°), which is exactly what you expect when light enters a medium with a higher refractive index. If your answer gave a larger angle, that would signal an error in the rearrangement.
Worked example: Finding the Refractive Index of a Substance
A ray of light passes from air into an unknown liquid. The angle of incidence is 55° and the angle of refraction is 38°. Calculate the refractive index of the liquid. [3 marks]
$n_1 \sin \theta_1 = n_2 \sin \theta_2$ — [M1] Always start by stating the relationship.
$n_1 = 1$ (air), $\theta_1 = 55°$, $\theta_2 = 38°$, $n_2 =?$ — The ray travels from air into the liquid, so medium 1 is air.
$\sin 55° = 0.8192$, $\quad \sin 38° = 0.6157$ — Compute each sine value separately to avoid arithmetic slips.
$n_2 = \frac{0.8192}{0.6157} = 1.33$ — [A1] The result is dimensionless and greater than 1, consistent with a refractive index. This value matches water closely.
Answer: $n_2 = 1.33$ (dimensionless)
5. Snell's Law Between Two Non-Air Media
So far, one medium has always been air. AQA questions can also involve a boundary between two materials where neither is air — for example, light passing from glass into water. The full form $n_1 \sin \theta_1 = n_2 \sin \theta_2$ handles this without modification; you substitute both refractive indices directly.
Worked example: Refraction at a Glass–Water Boundary
Light travels from glass (n = 1.50) into water (n = 1.33). The angle of incidence in the glass is 45°. Calculate the angle of refraction in the water. [3 marks]
$n_1 \sin \theta_1 = n_2 \sin \theta_2$ — [M1] The same equation applies regardless of whether air is involved.
$n_1 = 1.50$, $\theta_1 = 45°$, $n_2 = 1.33$, $\theta_2 =?$ — Medium 1 is glass (where the ray starts); medium 2 is water (where it is going).
$1.50 \times \sin 45° = 1.33 \times \sin \theta_2$ — [M1] Both refractive indices are substituted correctly.
$\sin 45° = 0.7071$, so $1.50 \times 0.7071 = 1.0607$ — 1.50 multiplied by 0.7071: 1.5 × 0.7071 = 1.0607.
$\theta_2 = \sin^{-1}(0.7974) = 52.9°$ — [A1] The angle is larger than 45°, confirming the ray bends away from the normal when moving from glass to water (lower n).
Answer: $\theta_2 = 52.9°$
This result connects back to the earlier principle: moving from a higher to a lower refractive index always increases the angle. The full form of Snell's law handles every case — air-to-glass, glass-to-water, or any other pairing — with identical method.
6. Required Practical — Measuring the Refractive Index of Glass
The refractive index equation and Snell's law are not just theoretical tools — they can be verified directly in the laboratory. The standard AQA approach uses a glass block, a ray box, and a protractor to measure angles of incidence and refraction, then applies Snell's law to determine $n$.
The graphical method is more reliable than using a single pair of angles because it averages out random errors across multiple measurements. A best-fit straight line through the origin reduces the effect of any one anomalous reading.
7. Exam Technique and Common Mistakes
Refraction questions are reliable mark-scorers once you know the traps. The following guidance consolidates the most common errors seen in AQA mark schemes and explains exactly how to avoid them.
For 'explain' questions on refraction, the mark scheme consistently rewards a two-part answer: state that the speed of light changes at the boundary, then link this to the change in direction. A response that only says 'light bends' without explaining why will not access the higher marks.
Refraction and Snell's law underpin several further topics in the AQA specification, including total internal reflection and optical fibres. The core skill you have built here — correctly applying $n_1 \sin \theta_1 = n_2 \sin \theta_2$ with careful labelling of media and angles — transfers directly to those topics without modification.
Sources and content standards
Published by Revise Right. Use the official specification reference to check the requirements for your course. Content updated: 2026-09-12.
Snell's law states that n₁ sin θ₁ = n₂ sin θ₂, where n₁ and n₂ are the refractive indices of the two media and θ₁ and θ₂ are the angles the ray makes with the normal on each side of the boundary. When the first medium is air, with n = 1, it simplifies to sin θ₁ = n₂ sin θ₂.
What is the refractive index of air?
The refractive index of air is approximately 1, because the speed of light in air is almost identical to its speed in a vacuum. Calculations treat air as n = 1 exactly, which simplifies Snell's law to sin θ₁ = n₂ sin θ₂.
What is refractive index?
Refractive index n is the ratio of the speed of light in a vacuum, c, to the speed of light in a substance: n = c ÷ (speed in the substance). It is always greater than or equal to 1, and a higher value means light travels more slowly in that material. Air has n ≈ 1, glass about 1.5, water about 1.33 and diamond about 2.4.
How do you calculate the refractive index of a liquid?
To calculate refractive index, rearrange Snell's law to n₂ = n₁ sin θ₁ ÷ sin θ₂. For light passing from air into a liquid with an angle of incidence of 55° and an angle of refraction of 38°, n₂ = sin 55° ÷ sin 38° = 0.8192 ÷ 0.6157 = 1.33, which matches water closely.
How do you calculate the angle of refraction?
To calculate the angle of refraction, use Snell's law to find sin θ₂, then take the inverse sine. For light entering glass (n = 1.50) from air at 40°, sin θ₂ = sin 40° ÷ 1.50 = 0.6428 ÷ 1.50 = 0.4285, so θ₂ = 25.4°, smaller than the incident angle because the ray bends towards the normal.
Why does light refract?
Light refracts because it travels at different speeds in different materials. When a wavefront hits a boundary at an angle, one side of the wavefront slows down before the other, so the whole wavefront pivots and changes direction. Entering a higher refractive index, the ray bends towards the normal; entering a lower one, it bends away from the normal.
Can refractive index be less than 1?
A refractive index cannot be less than 1, because light can never travel faster than c, its speed in a vacuum. Refractive index is c divided by the speed of light in the substance, and that speed is always less than or equal to c, so n is always at least 1.
When does light bend towards the normal?
Light bends towards the normal when it enters a medium with a higher refractive index, because n sin θ is conserved across the boundary, so a larger n means a smaller angle. When it enters a medium with a lower refractive index, such as from glass into water, it bends away from the normal.
What is the car analogy for refraction?
Refraction is like a car driving from tarmac onto mud at an angle: the wheel that hits the mud first slows down and the car turns. In the same way, one side of a light wavefront slows down before the other at a boundary, so the whole wavefront pivots and changes direction.
What are the refractive indices of glass, water and diamond?
Typical refractive indices are about 1.5 for glass, 1.33 for water and 2.4 for diamond. A higher refractive index means light travels more slowly in that material and bends more when it enters, so light in diamond travels roughly half as fast as in a vacuum.
How do you use Snell's law for light going from glass into water?
Snell's law handles a glass–water boundary with both refractive indices substituted directly. For light from glass (n = 1.50) into water (n = 1.33) at 45°, 1.50 × sin 45° = 1.33 × sin θ₂, so sin θ₂ = 0.7974 and θ₂ = 52.9°, bending away from the normal.
How do you measure the refractive index of a glass block?
The refractive index of glass is measured with a glass block, a ray box and a protractor, measuring angles of incidence and refraction and applying Snell's law. A graphical method with a best-fit straight line through the origin is more reliable than a single pair of angles, because it averages out random errors.
Does refractive index have units?
Refractive index has no units: it is the ratio of the speed of light in a vacuum to the speed of light in the substance, so the units cancel and the result is dimensionless. A calculated value such as 1.33 should always be greater than 1.