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Class 9–10 · Physics

Refraction of light

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Refraction of light

n₁n₂ > n₁
Entering higher refractive index bends an oblique ray towards the normal.
Lessons in this chapter
  1. Refraction and optical density
  2. Snell's law
  3. Apparent depth, slabs and prisms
  4. Critical angle and total internal reflection
  5. Lenses and principal rays
  6. Lens images
  7. Lens equation and power
  8. The eye and accommodation
  9. Vision defects
  10. Spectrum and dispersion

Lessons

1

Refraction and optical density

n₁n₂ > n₁
Entering higher refractive index bends an oblique ray towards the normal.

Light changes speed at a boundary. At oblique incidence it bends towards the normal when entering higher refractive index and away when entering lower index. Normal incidence changes speed without changing direction. Optical and mass density are different ideas.

Key relationship

n = c/v

Worked example

c = 3×10⁸, water v ≈ 2.25×10⁸ m/s ⇒ n ≈ 1.33

2

Snell's law

n₁n₂ > n₁
Entering higher refractive index bends an oblique ray towards the normal.

Snell's law relates the sines of angles measured from the normal. Frequency is unchanged across a stationary boundary; speed and wavelength change together. The two rays and normal lie in one plane.

Key relationship

n₁ sin i = n₂ sin r; v = fλ

Worked example

n₁ = 1, n₂ = 1.5, i = 30° ⇒ sin r = 1/3 ⇒ r ≈ 19.5°

3

Apparent depth, slabs and prisms

n₁n₂ > n₁
Entering higher refractive index bends an oblique ray towards the normal.

Refraction makes submerged objects appear shallower. The simple depth ratio applies approximately near normal viewing. A parallel-sided slab produces lateral displacement with parallel emergence; a prism changes the overall direction.

Key relationship

viewed from air near normal: n ≈ real depth/apparent depth

Worked example

Real depth 1.2 m, n = 4/3 ⇒ apparent depth 0.9 m

4

Critical angle and total internal reflection

n₁n₂ > n₁
Entering higher refractive index bends an oblique ray towards the normal.

From higher to lower refractive index, the critical angle produces a refracted ray at 90°. Above it, total internal reflection occurs. Both the index direction and angle condition are necessary. Optical fibres use a higher-index core and lower-index cladding.

Key relationship

sin critical angle = n₂/n₁, n₁ > n₂

Worked example

Glass n = 1.5 to air ⇒ critical angle ≈ 41.8°; i = 50° gives total reflection

5

Lenses and principal rays

n₁n₂ > n₁
Entering higher refractive index bends an oblique ray towards the normal.

In air, ordinary glass convex lenses converge and concave lenses diverge. Parallel rays pass through the far focus of a convex lens or appear from the near focus of a concave lens. A ray through a thin lens's optical centre is approximately undeviated.

Key relationship

convex → convergence; concave → divergence

Worked example

A distant object's parallel rays focus near a convex lens's focal plane.

6

Lens images

n₁n₂ > n₁
Entering higher refractive index bends an oblique ray towards the normal.

For a convex lens, beyond 2F gives a small inverted real image; at 2F, equal size; between F and 2F, enlarged and inverted. Inside F it is upright and virtual. A concave lens gives a real object a smaller upright virtual image.

Key relationship

real image: rays meet; virtual image: backward extensions meet

Worked example

Magnifier: object inside focal distance of convex lens

7

Lens equation and power

n₁n₂ > n₁
Entering higher refractive index bends an oblique ray towards the normal.

With Cartesian signs, a real object has negative u; convex f is positive and concave f negative. Power is reciprocal focal length in metres. Powers approximately add for thin lenses in contact.

Key relationship

1/f = 1/v−1/u; m = v/u; P = 1/f(m), unit D

Worked example

f = +10 cm, u = −30 cm ⇒ v = +15 cm, m = −0.5; P = +10 D

8

The eye and accommodation

n₁n₂ > n₁
Entering higher refractive index bends an oblique ray towards the normal.

The cornea and lens form an inverted real retinal image. The iris controls light through the pupil. Ciliary muscles change lens curvature for near and distant focus. A typical textbook near point is about 25 cm for a young normal eye, with individual variation.

Key relationship

near focus usually requires greater lens power

Worked example

Looking from a distant object to a book changes lens shape rather than moving the retina.

9

Vision defects

n₁n₂ > n₁
Entering higher refractive index bends an oblique ray towards the normal.

Myopia focuses distant objects before the retina and is corrected with a diverging lens. Hyperopia can require a converging lens for near focus. Presbyopia is declining accommodation with age. A professional eye examination determines correction.

Key relationship

myopia: negative correction; hyperopia: positive correction

Worked example

Correcting lens f = −0.5 m ⇒ P = −2 D

10

Spectrum and dispersion

n₁n₂ > n₁
Entering higher refractive index bends an oblique ray towards the normal.

White light contains many frequencies. A prism separates them because refractive index depends on wavelength; ordinary glass bends violet more than red. Rainbows combine refraction, internal reflection and dispersion in droplets.

Key relationship

ordinary glass: nviolet > nred

Worked example

White beam → prism → continuous coloured spectrum

Check your understanding

Try answering first, then open the question to compare your reasoning.

1. Air to glass at oblique incidence: bending direction?

Towards the normal: n increases

2. Does light frequency change across the boundary?

No; speed and wavelength change

3. Lens focal length +0.25 m: power?

P = 1/0.25 = +4 D

4. Usual correcting lens for myopia?

Diverging/concave; negative power

5. Two conditions for total internal reflection?

Higher n to lower n; incidence angle above critical angle

Sources and scope

Original GetReady teaching notes. The 13 core chapters follow the existing site sequence. Physics to save life is an explicitly labelled older-edition supplement. Check your current book and board instructions for examination scope. Illustrations are schematic. Unless stated otherwise, use g = 9.8 m/s². A physics teacher should review content and edition coverage before it is relied on.