Class 10 Science Notes Chapter 10 — The Human Eye and the Colourful World#

The human eye#

Part Function
Cornea Thin transparent front membrane; most of the refraction happens at its outer surface
Iris Dark muscular diaphragm that controls the size of the pupil
Pupil Opening that controls how much light enters (small in bright light, large in dim light)
Eye lens Fine-adjusts the focal length to focus on the retina; forms a real, inverted image
Ciliary muscles Change the curvature, and so the focal length, of the eye lens
Retina Light-sensitive screen with light-sensitive cells; sends electrical signals
Optic nerve Carries signals from the retina to the brain, which sees the image upright
  • Power of accommodation — the eye lens’s ability to change its focal length.
    • Distant object: ciliary muscles relax, the lens gets thinner, and its focal length increases.
    • Near object: ciliary muscles contract, the lens gets thicker, and its focal length decreases.
  • Near point (least distance of distinct vision) of a normal adult eye: 25 cm. Far point: infinity.
  • Cataract — the lens becomes milky and cloudy, causing partial or complete loss of vision. It is treated by surgery.

Defects of vision#

Defect Can see clearly Image forms Causes Corrected with
Myopia (near-sightedness) Near objects only In front of the retina Eyeball too long, or lens too curved Concave lens
Hypermetropia (far-sightedness) Distant objects only; near point is beyond 25 cm Behind the retina Eyeball too short, or focal length too long Convex lens
Presbyopia Not near objects (with age) Behind the retina Ciliary muscles weaken and the lens loses flexibility Convex lens; bifocal lens if both defects
  • A bifocal lens has a concave upper part (distant vision) and a convex lower part (near vision).
  • Defects can also be corrected with contact lenses or surgery.
  • Eye donation: one pair of eyes can give vision to up to four people with corneal blindness. Eyes must be removed within 4–6 hours of death.

Refraction through a prism#

  • A prism has two triangular bases and three rectangular faces. The angle between two side faces is the angle of the prism.
  • Light bends towards the base of the prism.
  • Angle of deviation — the angle between the incident ray (extended) and the emergent ray.

Dispersion#

  • Dispersion — splitting of white light into its colours by a prism.

  • Spectrum — the band of colours: VIBGYOR (violet, indigo, blue, green, yellow, orange, red).

  • Different colours bend by different amounts. Violet bends the most, red the least.

    ROYGBIVWhite lightGlass prismScreen
    Dispersion: a prism splits white light into seven colours. Red bends the least and violet the most.

  • Newton showed that a second, inverted prism recombines the colours into white light, so white light is made of seven colours.

  • Rainbow — dispersion of sunlight by tiny water droplets in the air, which act like small prisms. The droplet refracts and disperses the light, reflects it internally, then refracts it again. A rainbow is always seen in the direction opposite to the sun.

Atmospheric refraction#

The atmosphere’s refractive index changes with temperature and height, so light bends as it passes through.

  • Twinkling of stars: a star is a point source. Starlight bends by changing amounts, so its apparent position and brightness keep changing. Planets do not twinkle, because they are closer and act like a group of point sources whose changes cancel out.
  • Stars look higher than they really are near the horizon.
  • Advance sunrise and delayed sunset: we see the sun about 2 minutes before it actually rises and about 2 minutes after it actually sets.
  • The flickering of objects seen through hot air above a fire is also atmospheric refraction.

Scattering of light#

  • Tyndall effect — scattering of light by colloidal particles, which makes the path of a light beam visible (sunlight through a canopy of trees, a beam in a smoky room).
  • The colour scattered depends on particle size. Very fine particles scatter mainly blue (shorter wavelength); larger particles scatter longer wavelengths.
Observation Reason
Sky is blue Air molecules (smaller than the wavelength of visible light) scatter blue much more than red
Sky looks dark to astronauts in space No atmosphere, so no scattering
Sun is reddish at sunrise and sunset Light travels a longer path through the air; most blue is scattered away, so mainly red reaches us
Danger signals are red Red is scattered least by fog and smoke, so it is seen from far away
Clouds are white Large water droplets scatter all colours equally

Common mistakes#

  • Myopia → concave lens; hypermetropia → convex lens. Do not swap them.
  • Saying red bends the most in a prism. Violet bends the most.
  • Saying planets twinkle. Only stars do.
  • Saying the sky is blue because of dispersion. It is because of scattering.