The Human Eye and the Colourful World

Accommodation, defects of vision, prisms, dispersion, atmospheric refraction and scattering.

Chapter Notes

Based on NCERT Class 10 Science, Chapter 10

10.1 The human eye

  • Light enters through the cornea, passes the pupil (its size is controlled by the iris) and is focused by the eye lens on the light-sensitive retina.
  • The retina's rods and cones send signals through the optic nerve to the brain.
  • The ciliary muscles change the curvature — and therefore the focal length — of the eye lens. This ability is called the power of accommodation.
  • The least distance of distinct vision for a normal young eye is about 25 cm and the far point is infinity.
Near point ≈ 25 cm Far point = infinity
Board-style practice questions

Q1.What is the power of accommodation of the eye? What is the near point of a normal eye?

2 marks

10.2 Defects of vision and their correction

  • Myopia (near-sightedness): the image forms in front of the retina; distant objects look blurred. Corrected with a concave lens of suitable power.
  • Hypermetropia (far-sightedness): the image forms behind the retina; near objects look blurred. Corrected with a convex lens.
  • Presbyopia: with age the ciliary muscles weaken and the near point recedes; bifocal lenses (concave upper, convex lower) are used.
Correcting power: P = 1/f, with f in metres (negative for myopia)

Watch it happen — Eye Defect Corrector

Controls

100 cm

Live result

Required lens
Concave
Focal length
-100cm
Power
-1D
Corrective lens ray pathRequired lens: Concave
rays diverge — virtual image
Click to start animation

A concave lens shifts the image of a distant object to the defective far point.

Board-style practice questions

Q1.A person cannot see objects beyond 1.5 m clearly. Name the defect and find the power of the corrective lens.

3 marks

10.3–10.4 Prism, dispersion and the rainbow

  • A ray passing through a glass prism bends towards the base and the total bending is measured by the angle of deviation.
  • White light splits into its seven colours (VIBGYOR) on passing through a prism because each colour bends by a different amount — red least, violet most. This splitting is dispersion.
  • Newton showed that a second inverted prism recombines the spectrum back into white light.
  • A rainbow forms when sunlight is refracted, internally reflected and refracted again by raindrops acting as tiny prisms.

Watch it happen — Prism Dispersion Lab

Controls

60 °

Live result

Refractive index
1.523
Minimum deviation δ
39.19°
Deviation39.19
Dispersion through a prismRefractive index: 1.523
white light splits — violet bends most
Click to start animation

Violet has the largest refractive index, so it deviates the most — that's why it lies at the bottom of a spectrum.

Board-style practice questions

Q1.What is dispersion of white light? Why do different colours bend differently in a prism?

2 marks

10.5 Atmospheric refraction

  • Air layers of different density refract light continuously, which makes stars twinkle — the apparent position of a star keeps changing slightly.
  • Planets do not twinkle because they are extended sources: the variations from all their points average out.
  • The Sun is visible about 2 minutes before actual sunrise and 2 minutes after sunset because of atmospheric refraction; the Sun also appears flattened near the horizon.

10.6 Scattering of light

  • The Tyndall effect is the scattering of light by colloidal particles, which makes the path of a beam visible in smoke or a fine mist.
  • Fine particles scatter shorter (blue) wavelengths more strongly, so the clear sky looks blue; on the Moon there is no atmosphere, so the sky looks black.
  • At sunrise and sunset light travels through much more air, most of the blue is scattered away and the Sun appears reddish. Danger signals are red because red scatters least and travels furthest.

Watch it happen — Tyndall & Sky Colour

Controls

450 nm
1 ×

Live result

Relative scattering
5.86× red
Perceived sky
Blue (noon)
Scattering5.86
Scattering of light (Tyndall effect)Relative scattering: 5.86 × red
shorter wavelengths scatter most
Click to start animation

Blue light scatters ~5.5× more than red, so the sky looks blue overhead and red at sunset.

Board-style practice questions

Q1.Why is the sky blue and why does the sun appear reddish at sunrise and sunset?

3 marks