NCERT Science Notes - Class 10
Chapter - 10 | The Human Eye and the Colourful World

Welcome to AJs Chalo Seekhen. This webpage is dedicated to Class 10 | Science | Chapter - 10 | The Human Eye and the Colourful World. In this chapter, students explore into how we perceive light and colors. This chapter explains the intricate workings of the human eye, detailing its structure and function in vision. It delves into the phenomena of light refraction, dispersion, and how we see colors. Students also learn about common optical defects and their corrections. The chapter beautifully connects the science of light with the wonder of the colorful world we experience, enriching students' understanding of both physiology and optics.

NOTES

10.0 - The Role of Light and Lenses in the Human Eye

You've already studied how light refracts through lenses and how lenses form images of different sizes, positions, and types. These ideas help us understand the structure and function of the human eye, which has its own lens that lets us see objects around us by bending light.

In this chapter, we’ll connect these ideas to understand:

  1. The Role of the Eye's Lens – How it helps us focus light to see clearly.
  2. Vision Correction with Lenses – How lenses in glasses correct eyesight issues.
  3. Natural Optical Phenomena – Such as rainbows, the splitting of light into colors, and why the sky appears blue.
Let’s dive into these topics using what you know about light and lenses to explore the science behind how we see and the fascinating effects of light in nature.

10.1 - The Human Eye

The human eye is one of our most important sense organs. It allows us to see the world around us and enjoy the colors of everything we observe. While we can use our other senses, like touch, smell, taste, or hearing, to identify objects, only our eyes can truly help us see colors.


The Eye as a Camera

The human eye functions like a camera. It has a lens system that focuses an image onto a light-sensitive surface called the retina.


How Light Enters the Eye

Light enters through a clear, thin membrane called the cornea. The cornea forms a transparent bulge on the eye’s surface and is responsible for most of the light bending, or refraction, as it enters the eye.


The Structure of the Eye

  • The eyeball is round and measures about 2.3 cm in diameter.
  • Behind the cornea lies the iris, a dark, muscular structure. It controls the size of the pupil, the small opening that lets light enter the eye.
  • The pupil adjusts to control the amount of light: it expands in low light and contracts in bright light.

Focusing Light on the Retina

The eye lens further adjusts the focus to ensure a clear image of objects at different distances. The lens creates an upside-down, real image on the retina.


The Retina and Vision

The retina is a delicate layer with many light-sensitive cells. When light hits these cells, they create electrical signals. These signals travel to the brain through the optic nerve. The brain then interprets the signals, flipping the image so we see objects as they are.

This complex and precise system is what enables us to see the beautiful and colorful world around us.


10.1.1 - Power of Accommodation

The eye lens is made of a jelly-like material and can change its shape slightly, thanks to the ciliary muscles around it. This flexibility allows the eye to adjust its focus for objects at different distances. This ability to adjust the focal length of the eye lens is called accommodation.

  • Seeing Distant Objects: When the ciliary muscles are relaxed, the lens becomes thinner, increasing its focal length. This allows us to see distant objects clearly.
  • Seeing Nearby Objects: When focusing on closer objects, the ciliary muscles contract, making the lens thicker and decreasing its focal length, allowing us to see nearby objects more clearly.

Least Distance of Distinct Vision
If you hold an object too close, the eye feels strain, and the image may appear blurry. The minimum distance at which we can see objects clearly and without strain is called the least distance of distinct vision or the near point. For a young adult with normal vision, this distance is about 25 cm.


Far Point of the Eye
The far point is the farthest distance at which an object can be seen clearly by the eye. For a normal eye, this point is considered to be infinity. Thus, a person with normal vision can see objects clearly from 25 cm to infinity.


Cataract
In older adults, the eye’s crystalline lens may turn cloudy, a condition known as cataract. This cloudiness can partially or completely obstruct vision, but it can usually be corrected through cataract surgery to restore sight.


10.2 - Defects of Vision and Their Correction

When the eye loses its ability to focus on objects at various distances, this is called a refractive defect. It can lead to blurred vision and discomfort. There are three main refractive defects of the eye:


1. Myopia (Near-sightedness)

  • Definition: Myopia is a condition where a person can see nearby objects clearly but struggles to see distant objects distinctly.
  • Far Point: The farthest point a myopic person can see clearly is closer than infinity.
  • Cause: Myopia can occur due to:
    • Excessive curvature of the eye lens.
    • Elongation of the eyeball.
  • Effect on Vision: In myopia, the image of distant objects forms in front of the retina rather than on the retina itself.
  • Correction: A concave lens is used to correct myopia. It diverges light rays, helping focus the image directly on the retina.
  • Question:
    • Q: What type of lens is used to correct myopia, and why?
    • A: A concave lens is used because it diverges light rays, adjusting the focal point onto the retina.

2. Hypermetropia (Far-sightedness)
  • Definition: Hypermetropia is a condition where a person can see distant objects clearly but finds it difficult to focus on nearby objects.
  • Near Point: For hypermetropic individuals, the near point is farther than the normal near point of 25 cm.
  • Cause: This defect arises when:
    • The focal length of the eye lens is too long.
    • The eyeball is too short.
  • Effect on Vision: The image of close objects forms behind the retina rather than directly on it.
  • Correction: A convex lens is used to correct hypermetropia, converging light rays to focus on the retina.
  • Question:
    • Q: Explain how hypermetropia can be corrected.
    • A: Hypermetropia is corrected with a convex lens, which converges light rays so they focus on the retina.

3. Presbyopia
  • Definition: Presbyopia is the gradual loss of the eye's ability to focus on nearby objects, typically due to aging.
  • Cause: It occurs due to:
    • Weakening of ciliary muscles.
    • Decreased flexibility of the eye lens.
  • Near Point: The near point of vision moves further away as presbyopia progresses.
  • Correction: Bifocal lenses or progressive lenses are used. Bifocal lenses have:
    • A concave (upper) section for distance vision.
    • A convex (lower) section for near vision.
  • Additional Corrections: Contact lenses and surgical options are available for people with presbyopia.
  • Question:
    • Q: Why do older adults often need bifocal lenses?
    • A: Due to presbyopia, where both near and distant vision may be affected, bifocals provide sections for both distance and near correction.

Think It Over: Eye Donation

Our Eyes Can Live After Death

  • By donating eyes, a person can help a blind individual gain sight, even after passing away.
  • In the developing world, about 35 million people are blind; around 4.5 million suffer from corneal blindness, which can be cured with donated corneas.
  • 60% of those with corneal blindness are children under the age of 12, highlighting the impact of eye donation.


Eye Donation
  1. Who Can Donate:
    • Donors can be of any age or gender.
    • People with glasses, cataract surgery history, diabetes, hypertension, or asthma can still donate.
    • Donors should not have any communicable diseases like AIDS, Hepatitis B or C, rabies, acute leukemia, tetanus, cholera, meningitis, or encephalitis.
  2. Time Sensitivity:
    • Eyes should be removed within 4-6 hours of death.
    • Notify the nearest eye bank immediately after death so they can take timely action.
  3. Eye Removal Process:
    • The eye bank team can remove the eyes at home or a hospital.
    • Removal takes only 10-15 minutes and does not cause any disfigurement.
  4. The Eye Bank’s Role:
    • Eye banks collect, evaluate, and distribute donated eyes, ensuring they meet strict medical standards.
    • Unsuitable eyes are used for research and medical education.
    • The identities of both donors and recipients are kept confidential.
  5. Impact of Donation:
    • One pair of donated eyes can restore vision to up to four corneal blind individuals.


10.3 - Refraction of Light Through a Prism

Understanding Light Refraction in a Prism

  • In a rectangular glass slab, the emergent ray is parallel to the incident ray but slightly displaced.
  • A triangular prism is different: it has two triangular bases and three rectangular lateral surfaces that are inclined at angles to each other.
  • The angle between the two lateral faces of a prism is called the angle of the prism.


Activity 10.1: Observing Refraction in a Prism

To study how light refracts in a triangular glass prism:

  1. Set up the Activity:
    • Pin a sheet of white paper to a drawing board.
    • Place a triangular glass prism on it with its triangular base on the paper. Outline the prism with a pencil.
    • Draw a line PE inclined to one refracting surface (e.g., surface AB).
  2. Inserting Pins:
    • Fix two pins (P and Q) on line PE.
    • Look through the other face (AC) to see the images of pins P and Q.
    • Fix two more pins (R and S) so that pins R, S, and the images of P and Q appear in a straight line.
  3. Tracing and Joining Lines:
    • Remove the pins and prism.
    • Join points E and F where line PE and the emergent line intersect the prism boundary.
    • Draw perpendiculars to AB and AC at points E and F, respectively.
    • Label ∠i as the angle of incidence, ∠r as the angle of refraction, and ∠e as the angle of emergence.
  4. Observations:
    • The incident ray PE enters from air to glass at surface AB, bending toward the normal.
    • At surface AC, as the ray exits from glass to air, it bends away from the normal.
    • The peculiar shape of the prism causes the emergent ray to bend at an angle to the direction of the incident ray.
  5. Angle of Deviation:
    • The angle between the direction of the incident ray and the emergent ray is called the angle of deviation (∠D).
    • Measure ∠D to observe how the prism alters the path of light.

Key Definitions and Concepts:
  1. Angle of the Prism:
    • The angle formed by the two lateral faces of a triangular prism.
  2. Angle of Deviation (∠D):
    • The angle formed between the incident ray and the emergent ray after light passes through a prism.
  3. Refraction in Prism vs. Glass Slab:
    • In a glass slab, the emergent ray is parallel to the incident ray.
    • In a prism, the emergent ray is not parallel but deviated from the original path.

Questions and Answers:
  1. What is the angle of the prism?
    A: The angle between the two lateral faces of a triangular prism.

  2. What causes the angle of deviation in a prism?
    A: The peculiar shape of the prism causes the emergent ray to bend at an angle to the incident ray, resulting in an angle of deviation (∠D).

  3. How does light refract in a prism differently from a glass slab?
    A: In a glass slab, the emergent ray is parallel to the incident ray, but in a prism, the emergent ray deviates from the incident ray’s direction.

  4. Why does the light ray bend toward the normal when entering the prism?
    A: The light ray bends toward the normal as it moves from a less dense medium (air) to a denser medium (glass), due to the change in speed.


10.4 - Dispersion of White Light by a Glass Prism

Introduction to Dispersion

  • The stunning colors of a rainbow are produced by the dispersion of white light from the Sun.
  • Dispersion is the process by which white light is separated into its component colors when it passes through a medium like a prism.

Activity 10.2: Observing Dispersion with a Prism

To observe how a prism disperses white light:
  1. Setup:
    • Take a thick cardboard sheet and create a small hole or narrow slit in the middle.
    • Position the cardboard to allow sunlight to pass through the slit, forming a narrow beam of white light.
  2. Using the Prism:
    • Place a glass prism in the path of the beam so that the light strikes one of its faces.
    • Slowly turn the prism until the light that emerges appears on a nearby screen.
  3. Observations:
    • You will see a band of colors on the screen, indicating that the prism has dispersed the white light.
    • The sequence of colors observed will be: Violet, Indigo, Blue, Green, Yellow, Orange, and Red.
    • The acronym VIBGYOR can help remember this sequence.
  4. Understanding the Spectrum:
    • The band of colors produced by the prism is known as its spectrum.
    • Although not all colors may be individually distinct, the colors present are clearly recognizable.

Why Dispersion Occurs
  • Different colors of light bend at different angles when passing through the prism due to their varying wavelengths.
  • Red light bends the least, while violet light bends the most. This variation allows each color to emerge along separate paths, creating a spectrum.

Historical Context
  • Isaac Newton was the first to use a prism to obtain the spectrum of sunlight.
  • He attempted to further split the colors of the spectrum using a second prism but found no additional colors.
  • By inverting the second prism, he allowed all colors of the spectrum to pass through, resulting in a beam of white light emerging from the other side.
  • This experiment led him to conclude that sunlight consists of seven distinct colors.

Natural Phenomenon: The Rainbow
  • A rainbow is a natural spectrum seen in the sky, formed by the dispersion of sunlight through tiny water droplets after rain.
  • The water droplets function like small prisms, refracting and dispersing sunlight, reflecting it internally, and refracting it again upon exiting the droplet.
  • A rainbow is always formed in a direction opposite to that of the Sun.
  • Rainbows can also be observed on sunny days when looking through a waterfall or water fountain with the Sun behind you.

Key Definitions and Concepts:
  1. Dispersion:
    • The splitting of white light into its component colors when passing through a medium such as a prism.
  2. Spectrum:
    • The band of colors produced when white light is dispersed, consisting of the sequence VIBGYOR (Violet, Indigo, Blue, Green, Yellow, Orange, Red).
  3. Angle of Refraction:
    • The angle at which different colors of light bend when passing through a prism, affecting the resulting spectrum.
  4. Rainbow:
    • A natural spectrum appearing in the sky, caused by the dispersion of sunlight through water droplets, often observed after rain.

Questions and Answers:
  1. What is dispersion?
    A: Dispersion is the process of splitting white light into its component colors when passing through a medium like a prism.
  2. What is the sequence of colors observed in a spectrum produced by a prism?
    A: The sequence of colors is Violet, Indigo, Blue, Green, Yellow, Orange, and Red (VIBGYOR).
  3. How did Isaac Newton contribute to our understanding of light dispersion?
    A: Isaac Newton was the first to use a prism to obtain the spectrum of sunlight and demonstrated that sunlight is made up of seven colors.
  4. How is a rainbow formed?
    A: A rainbow is formed by the dispersion of sunlight through tiny water droplets, which act like prisms, refracting and reflecting the light to produce a spectrum in the sky.

10.5 - Atmospheric Refraction

Definition: Atmospheric refraction is the bending of light rays as they pass through the Earth’s atmosphere, which has varying density and refractive index.

1. Wavering of Objects in Hot Air

  • Observation: When looking at objects above a fire or radiator, you may notice a wavering or flickering appearance.
  • Cause: The air just above the heat source is hotter and less dense than the cooler air above it. Hot air has a lower refractive index compared to cooler air.
  • Effect: The fluctuating conditions of the air cause the apparent position of the object to change, creating the illusion of wavering.
Question: What causes the wavering of objects seen above a fire?
  • Answer: The wavering is caused by atmospheric refraction, as hot air is less dense and has a different refractive index than cooler air, resulting in a fluctuating apparent position of objects.

2. Twinkling of Stars
  • Definition: The twinkling of stars is a phenomenon caused by atmospheric refraction of starlight.
  • Explanation: As starlight enters the Earth's atmosphere, it continuously refracts due to the varying refractive index of the atmosphere.
  • Effect:
    • The atmosphere bends starlight toward the normal, causing the star to appear slightly higher than its actual position, especially when viewed near the horizon.
    • The apparent position of the star fluctuates due to changing atmospheric conditions, leading to a flickering effect in brightness—sometimes appearing brighter and at other times fainter.
Question: Why do stars twinkle?
  • Answer: Stars twinkle because their light undergoes continuous refraction in the Earth's atmosphere, which has a varying refractive index. This causes the apparent position of the star to shift slightly, resulting in a flickering effect.

3. Why Don’t Planets Twinkle?
  • Explanation: Planets are much closer to Earth than stars, making them appear as extended sources of light rather than point sources.
  • Effect: Since a planet can be seen as a collection of many point-sized light sources, the variations in light from these sources average out, resulting in no noticeable twinkling effect.
Question: Why do planets not twinkle like stars?
  • Answer: Planets do not twinkle because they are closer to Earth and appear as extended sources of light. The light from different parts of a planet averages out, minimizing variations in brightness.

4. Advance Sunrise and Delayed Sunset
  • Observation: The Sun appears visible about 2 minutes before actual sunrise and about 2 minutes after actual sunset.
  • Cause: This effect is also due to atmospheric refraction, which bends the light rays from the Sun, allowing us to see it slightly before it crosses the horizon and after it has actually set.
  • Effect:
    • The apparent position of the Sun is different from its actual position.
    • The disc of the Sun appears slightly flattened at sunrise and sunset due to atmospheric refraction.
Question: Why does the Sun appear to rise early and set late?
  • Answer: The Sun appears to rise about 2 minutes early and set about 2 minutes late due to atmospheric refraction, which bends the light rays, altering the apparent position of the Sun relative to the horizon.

10.6 - Scattering of Light

Definition of Scattering of Light:
Scattering of light is the process by which small particles or molecules present in a medium cause light waves to spread out in different directions. This phenomenon is responsible for several natural occurrences, such as the blue color of the sky and the reddening of the sun during sunrise and sunset.


Explanation and Examples:

  • Blue Color of the Sky: This is due to the scattering of shorter wavelengths of light, predominantly blue, by particles in the atmosphere.
  • Color of Water in Deep Sea: Light that penetrates the water scatters, giving it a blue tint as red wavelengths are absorbed at deeper levels.
  • Reddening of the Sun at Sunrise and Sunset: The sun appears red due to the scattering of shorter wavelengths, allowing only the red wavelengths to reach our eyes as the sun is lower on the horizon.

Question:

Why does the path of a beam of light become visible in a colloidal solution but not in a true solution?
Answer:
In a colloidal solution, particles are larger than those in a true solution. This size difference allows the colloidal particles to scatter light, making the path of the beam visible, while in a true solution, the particles are too small to scatter light effectively.

10.6.1 - Tyndall Effect

Definition of Tyndall Effect:
The Tyndall Effect is the scattering of light by particles in a colloid or in a very fine suspension, making the path of the light visible.


Explanation:

  • Atmosphere as a Mixture: The earth’s atmosphere is filled with particles such as smoke, dust, and water droplets. When a beam of light strikes these particles, light scatters, causing the path to become visible.
  • Examples of Tyndall Effect:
    • In a Smoke-filled Room: A beam of sunlight entering through a small hole in a smoke-filled room becomes visible due to scattering by smoke particles.
    • In a Dense Forest Canopy: Sunlight passing through a canopy creates visible beams as water droplets in mist scatter light.

Question:

What type of particles are most effective in scattering blue light, and why?
Answer:
Very fine particles, smaller than the wavelength of visible light, are most effective in scattering blue light. This is because shorter wavelengths, such as blue, are scattered more strongly by small particles.

Question:
Why does the scattered light sometimes appear white?
Answer:
If the size of the scattering particles is large, they scatter light of all wavelengths equally, causing the scattered light to appear white.



10.6.2 - Why is the Colour of the Clear Sky Blue?

Explanation of the Blue Color of the Sky:

  • Size of Atmospheric Particles: Particles in the atmosphere are smaller than the wavelength of visible light, making them efficient at scattering shorter (blue) wavelengths more than longer (red) wavelengths.
  • Wavelength Comparison: Red light has a wavelength about 1.8 times longer than blue light. As a result, blue light is scattered more extensively in the atmosphere, giving the sky its blue color.
Question:
What would the sky look like if Earth had no atmosphere?
Answer:
If there were no atmosphere, there would be no particles to scatter light, so the sky would appear dark, as it does at high altitudes where scattering is minimal.

Additional Information:

  • Red Colour for ‘Danger’ Signals: Red light is used in danger signals because it has a longer wavelength and is scattered the least by fog or smoke, making it visible from a greater distance.
Question:
Why do passengers flying at high altitudes see a dark sky?
Answer:
At high altitudes, there are fewer atmospheric particles to scatter light, making the sky appear dark to passengers.

NCERT Science Notes - Class 10 | Chapter 10 - The Human Eye and the Colourful World

NCERT Science Notes - Class 10 | Chapter 10 - The Human Eye and the Colourful World

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