GRADE 9 · LIGHT PHENOMENA
Refraction and total internal reflection
Refraction law, refractive index and light speed in a medium.
Read the full lesson theory here without an account. In the interactive lesson, the same theory is presented as cards, followed by questions with feedback and practice problems. Your progress is saved.
Understanding step by step
A spoon in a glass seems bent and the bottom seems raised. The objects have not changed; the light's route has. Why does a ray turn at a transparent boundary, and when does it fail to emerge at all?
Different speeds
Transparency does not mean light travels through matter as it does through empty space. Interaction with a medium changes propagation speed. Define absolute refractive index as n = c/v, where c is vacuum light speed and v is its speed in the medium. Ordinary transparent glass has n > 1 and v < c. This ratio describes light of a chosen frequency: the index can differ slightly for different colours.
A number without a unit
If n = 1,5, then c is about one and a half times the speed in the medium: v = c/1,5. It does not mean the light is brighter by that factor. Both speeds use m/s, so n has no unit. c ≈ 3·10⁸ м/с. Greater n means lower speed for this light; at n = 1, its speed is c. The number describes speed; direction depends on how the wave crosses the boundary.
Direction at a boundary
An oblique wavefront does not enter the new medium all at once. One part already travels at the new speed while another still has the old speed, so the front rotates. In a medium of higher n, the ray bends towards the normal; for lower n, away from it. This is a wave explanation of refraction. If the front is parallel to the boundary, all parts change speed together: at normal incidence the ray stays straight even though speed changes.
Law of refraction
The quantitative angle relation is n₁ sin α = n₂ sin β. Subscript 1 refers to the incident medium, 2 to the transmitted medium; α and β are measured from the normal. Rays and normal lie in one plane. If n₁ = n₂, then β = α: no turn. If α = 0, its sine is zero and β is also zero. The law predicts an angle, not just 'towards' or 'away from' the normal.
Checking an angle
Predict before calculating. With incident medium and α unchanged, increasing n₂ reduces β because sin β = (n₁/n₂) sin α. The ray should move closer to the normal. Entering a lower-n₂ medium instead increases the angle, while a refracted ray exists. This check catches swapped indices or angles and explains why one large n alone, without the other medium, cannot determine the turn.
The limiting exit angle
Increase the incidence angle as light leaves higher n for lower n. The refracted ray bends progressively farther from the normal, reaching the boundary direction at β = 90°. This defines critical angle αкр, with sin αкр = n₂/n₁. The ratio must be less than one. If n₁ ≤ n₂, no such limiting angle for total internal reflection exists.
Both conditions together
What happens at α > αкр? The law would require sin β > 1, which no direction can satisfy: there is no propagating refracted ray. In the transparent-media model, total internal reflection occurs. Both conditions are needed: n₁ > n₂ and incidence above the critical angle. Simply going from glass towards air is insufficient: at small angles, some light emerges. A field exists immediately at the boundary, but that belongs to the wave description, not an ordinary outgoing ray.
Applying this to a fibre
An optical fibre's core and cladding have a suitable index relationship. Rays hitting their boundary at suitable angles undergo total internal reflection and are guided along the fibre. Geometry and indices both matter: not every ray is automatically trapped. Frequency stays the same at a stationary boundary; the new speed changes wavelength through v = λν. Refraction should therefore not be explained by a change in source frequency.
From air to glass
Light goes from air, n₁ = 1, into glass, n₂ = 1,5. The incidence angle is 30°. Estimate the refraction angle, given sin 30° = 0,5.
Let's look at an example · 1
First predict: n₂ = 1,5 exceeds n₁ = 1, so the ray in glass must bend towards the normal and β must be less than 30°.
Let's look at an example · 2
Rearrange n₁ sin α = n₂ sin β: sin β = n₁ sin α/n₂ = 1 · 0,5/1,5 = 1/3.
Let's look at an example · 3
An angle whose sine is 1/3 is about 19.5°. This is measured from the normal, just like the given 30°.
Let's look at an example · 4
19.5° is less than 30°: the calculation agrees with the physical prediction for slower propagation in glass.
Check the result
β ≈ 19,5° from the normal. Entering glass bends the ray towards the normal, reducing the original 30° angle.
Key point · 1
n = c/v compares speeds; the ray turns because different parts of an oblique wavefront cross the boundary at different times.
Key point · 2
The refraction law relates both media and angles from the normal; at normal incidence, speed can change without a turn.
Key point · 3
Total internal reflection requires higher n to lower n and incidence above the critical angle.
What comes next
Curved lens boundaries bring rays together to form an image.
Basic Concepts
Refractive index
Absolute refractive index is the ratio of vacuum light speed to light speed in the medium.
A higher refractive index means lower light speed in the medium and usually stronger bending towards the normal.
Refraction of light
Light speed changes between media of different refractive indices. A ray changes direction at oblique incidence; at normal incidence it keeps its direction.
On entering an optically denser medium, a ray usually bends towards the normal.
Total internal reflection
Light is completely reflected when going from an optically denser medium towards a less dense one at an angle above the critical angle.
This is used in optical fibres and prisms; it cannot occur from an optically less dense medium into a denser one.
Physical quantities
Refractive index
nThe ratio of the speed of light in a vacuum to the speed in a medium.
Unit: dimensionless quantity
Speed of light
cSpeed of electromagnetic waves in vacuum.
Unit: meter per second · \frac{\mathrm{м}}{\mathrm{с}}
Speed of light in the medium
vSpeed of propagation of light in a transparent medium.
Unit: meter per second · \frac{\mathrm{м}}{\mathrm{с}}
Angle of refraction
\betaThe angle between the refracted ray and the normal to the surface.
Unit: radian · \mathrm{рад}
Lesson formulas
Law of refraction
n_1\sin\alpha=n_2\sin\betaThe medium's refractive index times the sine of the angle from the normal has the same value on both sides of the boundary.
Physical meaning of refractive index
n=\frac{c}{v}Refractive index gives the factor by which vacuum light speed exceeds the speed in the medium.
Test the relationship
Make a prediction first. The button changes the stated quantity; then compare the result and explore other values.
Reflection and refraction
θотр = θ₁; n₁ sin θ₁ = n₂ sin θ₂
Plane boundary between transparent uniform media; ray optics. Line thickness does not encode power. Under total internal reflection there is no propagating transmitted ray.
At the same incidence angle, n₂ increases from 1.5 to 2. How will the refraction angle from the normal change?
Initial values
Calculated result
- θотр
- 30 °
- θ₂
- 19.47 °
Explaining the result
Angles are measured from the normal. Entering a larger n bends the ray towards the normal. Total internal reflection requires n₁ > n₂ and incidence above the critical angle.
Related formulas
The same formulas in the reference, with symbols and units.
Problems on this topic
Statements, answer options and the walkthrough.