11-THE HUMAN EYE AND THE COLOURFUL WORLD

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CHAPTER – 11 THE HUMAN EYE AND THE COLOURFUL WORLD:

CHAPTER – 11 THE HUMAN EYE AND THE COLOURFUL WORLD Class :- X Subject :- SCIENCE Name :- Manish Yadav Add me as friend on facebook cutemanish66@gmail.com

THE HUMAN EYE:

THE HUMAN EYE

The human eye:- The human eye is the sense organ which helps us to see the colourful world around us. The human eye is like a camera. Its lens system forms an image on a light sensitive screen called retina. The eye ball is almost spherical in shape with a diameter of about 2.3cm. Light enters the eye through a transparent membrane called cornea. Behind the cornea is a muscular diaphragm called iris which has an opening called pupil. The pupil controls the amount of light entering the eye. The eye lens helps to focus the image of objects on the retina. The ciliary muscles helps to change the curvature of the lens and to change its focal length. :

The human eye:- The human eye is the sense organ which helps us to see the colourful world around us. The human eye is like a camera. Its lens system forms an image on a light sensitive screen called retina. The eye ball is almost spherical in shape with a diameter of about 2.3cm. Light enters the eye through a transparent membrane called cornea. Behind the cornea is a muscular diaphragm called iris which has an opening called pupil. The pupil controls the amount of light entering the eye. The eye lens helps to focus the image of objects on the retina. The ciliary muscles helps to change the curvature of the lens and to change its focal length. Working of the eye:- The eye lens forms a real inverted image of the object on the retina. The light sensitive cells in the retina then produce electrical signals which are carried by the optic nerves to the brain. The brain processes the information and sends the message to the eye and then we see the object.

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POWER OF ACCOMMODATION :- The ability of the eye lens to see both near and distant objects by adjusting its focal length is called the power of accommodation of the eye The eye lens is composed of a fibrous jelly like material. Its curvature can be changed to some extent by the ciliary muscles. The change in the curvature of the eye lens can change its focal length. When the muscles are relaxed, the lens becomes thin and its focal length increases and when the muscles contract, the lens becomes thick and its focal length decreases. Near point :- The minimum distance at which the eye can see objects clearly is called the least distance of distinct vision or near point. For a normal eye it is 25cm. Far point :- The farthest distance upto which the eye can see objects clearly is called the far point of the eye. For a normal eye it is between 25cm and infinity.

DEFECTS OF VSION AND THEIR CORRECTON:

DEFECTS OF VSION AND THEIR CORRECTON 1) MYOPIA OR NEAR SIGHTEDNESS :- Myopia is a defect of vision in which a person can see nearby objects clearly but cannot see distant objects clearly because the image is formed in front of the retina. This may be due to:- i) Increase in curvature of the eye lens ii) Increase in the length of the eye ball It can be corrected by using a suitable concave lens. Myopic eye Correction using concave lens

2) HYPERMETROPIA OR FAR SIGHTEDNESS :-:

2) HYPERMETROPIA OR FAR SIGHTEDNESS :- Hypermetropia is a defect of vision in which a person can see distant objects clearly but cannot see nearby objects clearly because the image is formed behind the retina. This may be due to:- i) Decrease in curvature of eye lens ii) Decrease in the length of the eye ball It can be corrected by using a suitable convex lens. Hypemetropic eye Correction using convex lens

3) PRESBYOPIA:

3) PRESBYOPIA Presbyopia is a defect of vision in old people in which they are not able to see nearby objects clearly due to the increase in the distance of near point. This is due to the weakening of the ciliary muscles and decrease in the flexibility of the eye lens. It can be corrected by using suitable convex lens. Sometimes they are not able to see both nearby and distant objects clearly. It can be corrected by using bifocal lenses consisting of both concave and convex lenses. The upper part is concave for correction of distant vision and the lower part is convex for correction of near vision.

REFRACTION OF LIGHT THROUGH A GLASS PRISM:

REFRACTION OF LIGHT THROUGH A GLASS PRISM When a ray of light passes through a glass prism, it gets bent twice at the air-glass interface and glass-air interface. The emergent ray is deviated by an angle to the incident ray. This angle is called the angle of deviation . Incident ray Refracted ray Emergent ray D i r i r Air Glass Glass Air Glass prism

DISPERSION OF WHITE LIGHT BY A GLASS PRISM:

DISPERSION OF WHITE LIGHT BY A GLASS PRISM When a beam of white light is passed through a glass prism, it is split up into a band of colours called spectrum . This is called dispersion of white light. The spectrum of white has the colours violet, indigo, blue, green, yellow, orange and red (VIBGYOR). The red light bends the least and the violet light bends the most. Beam of white light Spectrum R O Y G I B V Glass prism

RECOMBINATION OF THE SPECTRUM OF WHITE LIGHT PRODUCES WHITE LIGHT:

RECOMBINATION OF THE SPECTRUM OF WHITE LIGHT PRODUCES WHITE LIGHT R V V R R When a beam of white light is passed through a glass prism, it is split up into its component colours. When these colours are allowed to fall on an inverted glass prism it recombines to produce white light. V White light White light Glass prisms

RAINBOW FORMATION:

RAINBOW FORMATION A rainbow is a natural spectrum appearing in the sky after a rain shower. It is caused by the dispersion of sunlight by the tiny water droplets present in the atmosphere. The water droplets act like small prisms. Due to the dispersion of sunlight and internal reflection by the water droplets we see the rainbow colours. Sunlight Raindrop Red Violet Dispersion Internal reflection Observer

ATMOSPHERIC REFRACTION:

ATMOSPHERIC REFRACTION Atmospheric refraction is due to the gradual change in the refractive index of the atmosphere. The refractive index of the atmosphere gradually increases towards the surface of the earth because the hot air above is less dense than the cool air below. So light gradually bends towards the normal. Twinkling of stars:- is due to the atmospheric refraction of star light and due to the changing in the position of the stars and the movement of the atmosphere. So the light from the stars is sometimes brighter and sometimes fainter and it appears to twinkle. Planets are closer to the earth than stars. The light from stars are considered as point source of light and the light from planets are considered as extended source of light. So the light from the planets nullify the twinkling effect. Apparent position Real position Eye Star Increasing refractive index

ADVANCE SUNRISE AND DELAYED SUNSET:

Earth Observer Sunrise Sunset Apparent position Apparent position Atmosphere ADVANCE SUNRISE AND DELAYED SUNSET The sun is visible to us about 2 minutes before sunrise and about two minutes after sunset due to atmospheric refraction. The apparent flattening of the sun’s disc at sunrise and at sunset is also due to atmospheric refraction. Horizon Horizon

SCATTERING OF LIGHT:

SCATTERING OF LIGHT TYNDALL EFFECT:- When a beam of light passes through a colloidal solution, the path of light becomes visible due to the scattering of light by the colloid particles. This is known as Tyndall effect. The earth’s atmosphere contains air molecules, water droplets, dust, smoke etc. When sunlight passes through the atmosphere the path of the light becomes visible due to the scattering of light by these particles. The colour of the scattered light depends upon the size of the scattering particles. Very fine particles scatter blue light. Larger particles scatter different colours of light.

WHY IS THE COLOUR OF THE CLEAR SKY BLUE ?:

WHY IS THE COLOUR OF THE CLEAR SKY BLUE ? The fine particles in the atmosphere have size smaller than the wave length of visible light. They can scatter blue light which has a shorter wave length than red light which has a longer wave length. When sunlight passes through the atmosphere, the fine particles in the atmosphere scatter the blue colour more strongly than the red and so the sky appears blue. If the earth had no atmosphere there would not be any scattering of light and the sky would appear dark. The sky appears dark at very high altitudes.

COLOUR OF THE SUN AT SUNRISE AND SUNSET:

COLOUR OF THE SUN AT SUNRISE AND SUNSET At sunrise and at sunset the sun is near the horizon and the light from the sun travels through the thicker layers of the atmosphere and longer distance through the atmosphere. Near the horizon most of the blue light and shorter wave lengths are scattered away by the particles of the air and the red light and longer wave lengths reaches our eyes. So the sun appears reddish at sunrise and sunset. Observer Sun near horizon Sun overhead Blue light scattered away Sun appears reddish Atmosphere Earth

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