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ICSEClass 10Physics

Light

Refraction, total internal reflection, lenses, prisms, and scattering.

Chapter 2

Verified Curriculum Topic

What is Light?

Refraction, total internal reflection, lenses, prisms, and scattering.

Light matters because it connects theory, equations, and real physical behaviour. At Class 10 level, students are typically expected to explain concepts precisely, apply laws correctly, and interpret numerical or experimental questions with confidence.

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Summary

The One Thing

Light changes direction when its speed changes between transparent media, and this principle explains refraction, total internal reflection, lens images, prism dispersion and several effects produced by scattering.

Reactions, Processes and Experiments

What happensEquation or processWhat you observeType
Light passes obliquely from one transparent medium into another and changes direction because its speed changes.RefractionFrom a rarer to a denser medium, light bends towards the normal; from a denser to a rarer medium, it bends away from the normal. Its frequency remains unchanged, while its speed and wavelength change.Refraction
The relationship between the angles of incidence and refraction is fixed for a given pair of media.sin i divided by sin r is constantThe incident ray, refracted ray and normal lie in one plane.Laws of refraction
Light passes between two media with refractive indices and .n1 sin i = n2 sin rThe direction of the ray changes according to the refractive indices and the angle of incidence.Snell's law
The refractive index of a medium is determined by comparing the speed of light in vacuum with its speed in that medium.n = c/vA higher refractive index corresponds generally to slower light and greater bending.Absolute refractive index
The refractive index of one medium is compared with that of another medium.n21 = speed of light in medium 1 divided by speed of light in medium 2 = n2/n1The relative refractive index indicates how light speeds differ between the two media.Relative refractive index
Light travels from a denser medium towards a rarer medium and reaches the limiting angle for refraction.sin C = 1/nAt the critical angle, the refracted ray travels along the boundary at 90 degrees to the normal.Critical angle
Light travels from an optically denser medium to an optically rarer medium at an angle greater than the critical angle.Total internal reflectionLight is completely reflected back into the denser medium.Total internal reflection
Light is transmitted through a thin transparent fibre by repeated internal reflection.Repeated total internal reflection in an optical fibreLight follows the fibre, even along curved paths.Optical fibre
Prisms use total internal reflection to redirect light.Total internal reflection in prisms in periscopes and binocularsLight is redirected without requiring a silvered reflecting surface.Application of total internal reflection
Light undergoes repeated internal reflection in a diamond.Total internal reflection in sparkling diamondsDiamonds appear highly brilliant or sparkling.Application of total internal reflection
Light is refracted through changing layers of air near the ground.Mirage formation by total internal reflectionDistant objects or apparent pools of water may appear displaced or inverted.Application of total internal reflection
A ray parallel to the principal axis passes through a convex lens.Refraction by a convex lens: parallel rays pass through the principal focus.The ray converges at the principal focus.Convex-lens refraction
A ray parallel to the principal axis passes through a concave lens.Refraction by a concave lens: parallel rays appear to come from the principal focus.The ray diverges as though it originated at the principal focus.Concave-lens refraction
A convex lens forms images at different positions as the object is moved.Lens formula: 1/f = 1/v - 1/uBeyond 2F: real, inverted and diminished; at 2F: real, inverted and same-sized; between F and 2F: real, inverted and enlarged; at F: no finite real image; between the optical centre and F: virtual, erect and enlarged.Convex-lens image formation
A concave lens refracts light so that the rays diverge.Lens formula: 1/f = 1/v - 1/uFor a real object, the image is always virtual, erect, diminished and between the optical centre and the focus.Concave-lens image formation
The size of a lens image is compared with the size of the object.m = v/uThe value of magnification indicates the relative image size; the image may also be real or virtual and inverted or erect according to the lens arrangement.Magnification
The converging or diverging ability of a lens is calculated.P = 1/fA convex lens has positive power and a concave lens has negative power; power is measured in the dioptre when is in metres.Power of a lens
Two lenses are placed in contact.P = P1 + P2The combined lens has a power equal to the sum of the individual powers.Lenses in contact
The equivalent focal length of two lenses in contact is calculated.1/F = 1/f1 + 1/f2The combination behaves as a single lens with focal length .Equivalent focal length
A prism refracts light through two inclined plane surfaces.Refraction through a prismThe prism deviates light towards its base, and the emergent ray is generally displaced from its original direction.Prism refraction
The least deviation of a ray through a prism is reached.Minimum deviationThe ray path is symmetrical, and the angles of incidence and emergence are equal.Minimum deviation
White light passes through a prism and separates into its component colours.Dispersion by a prismA spectrum is produced; violet deviates the most and red deviates the least.Dispersion
The component colours of white light are arranged according to wavelength.VIBGYORThe order from least to greatest wavelength is violet, indigo, blue, green, yellow, orange and red. Red has the lowest visible frequency and violet the highest.Spectrum
Different colours travel at different speeds in a prism and undergo different deviations.Deviation produced by a prism depends on the angle of the prism, the angle of incidence, the material of the prism and the wavelength of light.Violet is deviated most and red least because refractive index depends on wavelength.Wavelength-dependent deviation
Light is redirected by particles in a medium.ScatteringLight travels in different directions after interacting with particles.Scattering
A beam of light is scattered by colloidal or very fine particles.Tyndall effectThe path of the beam becomes visible.Tyndall effect
Particles much smaller than the wavelength of light scatter incident light.Rayleigh scatteringShorter wavelengths scatter more strongly than longer wavelengths.Rayleigh scattering
Sunlight is scattered by molecules and tiny particles in the atmosphere.Stronger scattering of shorter wavelengthsThe sky appears blue.Atmospheric scattering
Sunlight travels through a longer atmospheric path at sunrise and sunset.Scattering of sunlight through the atmosphereMuch of the blue light is scattered away, leaving the Sun and surrounding sky reddish or orange.Atmospheric scattering
Light is scattered by relatively large water droplets in clouds.Scattering by cloud dropletsDifferent visible wavelengths are scattered nearly equally, so clouds generally appear white.Scattering
Starlight passes through changing layers of Earth's atmosphere.Repeated refraction through changing atmospheric layersStars appear to twinkle.Atmospheric refraction

Key Terms

  • Refraction: The bending of light as it enters a different transparent medium because its speed changes.
  • Optically denser medium: A medium in which light travels more slowly and generally has a higher refractive index.
  • Optically rarer medium: A medium in which light travels faster and generally has a lower refractive index.
  • Normal: An imaginary line perpendicular to the surface at the point where light strikes it.
  • Angle of incidence: The angle between the incident ray and the normal.
  • Angle of refraction: The angle between the refracted ray and the normal.
  • Laws of refraction: The incident ray, refracted ray and normal lie in one plane; for a given pair of media, sin i divided by sin r is constant.
  • Refractive index: A measure of how much a medium slows and bends light; n = c/v.
  • Snell's law: For two given media, n1 sin i = n2 sin r.
  • Critical angle: The angle of incidence in the denser medium for which the angle of refraction in the rarer medium is 90 degrees.
  • Total internal reflection: Complete reflection of light back into the denser medium when it travels from a denser to a rarer medium and the angle of incidence exceeds the critical angle.
  • Conditions for total internal reflection: Light must travel from an optically denser to an optically rarer medium, and the angle of incidence must be greater than the critical angle.
  • Optical fibre: A thin transparent fibre that transmits light through repeated total internal reflection.
  • Lens: A transparent optical device bounded by two spherical surfaces, or by one spherical and one plane surface, that refracts light.
  • Convex lens: A converging lens thicker at the centre that can form real or virtual images.
  • Concave lens: A diverging lens thinner at the centre that always forms a virtual, erect and diminished image for a real object.
  • Principal axis: The straight line passing through the optical centre and the centres of curvature of a lens.
  • Optical centre: The point near the centre of a thin lens through which a ray passes approximately without deviation.
  • Principal focus: The point on the principal axis where rays parallel to the axis meet, or appear to come from, after refraction.
  • Focal length: The distance between the optical centre and the principal focus.
  • Lens formula: For a thin lens, 1/f = 1/v - 1/u using the Cartesian sign convention.
  • Magnification: The ratio of image height to object height; for a lens, m = v/u.
  • Power of a lens: The ability of a lens to converge or diverge light; P = 1/f when f is measured in metres, with the unit dioptre.
  • Prism: A transparent refracting medium bounded by two plane surfaces inclined at an angle.
  • Angle of prism: The angle between the two refracting faces of a prism.
  • Angle of deviation: The angle between the original direction of the incident ray and the emergent ray.
  • Minimum deviation: The least angle through which a prism deviates a ray; at this position, the path is symmetrical and the angles of incidence and emergence are equal.
  • Dispersion: The splitting of white light into its constituent colours when it passes through a prism.
  • Spectrum: The band of colours obtained when white light is dispersed, commonly remembered as VIBGYOR.
  • Scattering: The redirection of light in different directions by particles in a medium.
  • Tyndall effect: The visible scattering of light by colloidal or very fine particles, making the path of a beam visible.
  • Rayleigh scattering: Scattering by particles much smaller than the wavelength of light; shorter wavelengths scatter more strongly.

Easily Confused

  • Optically denser and optically rarer media: Light travels more slowly in an optically denser medium and faster in an optically rarer medium.
  • Refraction and total internal reflection: Refraction occurs when light enters another medium; total internal reflection returns all the light to the denser medium under the required conditions.
  • Critical angle and total internal reflection: At the critical angle the refracted ray travels along the boundary; total internal reflection occurs only when the angle of incidence is greater than the critical angle.
  • Convex and concave lenses: A convex lens converges light and has positive power; a concave lens diverges light and has negative power.
  • Real and virtual images formed by a convex lens: A real image is formed for object positions beyond the focus, whereas an object between the optical centre and focus produces a virtual, erect and enlarged image.
  • Angle of prism and angle of deviation: The angle of prism is between the refracting faces; the angle of deviation is between the original incident direction and the emergent ray.
  • Dispersion and scattering: Dispersion separates white light into colours through a prism; scattering redirects light in different directions through interaction with particles.
  • Tyndall effect and Rayleigh scattering: The Tyndall effect is the visible scattering by colloidal or very fine particles; Rayleigh scattering specifically concerns particles much smaller than the wavelength of light.
  • Red and violet light in dispersion: Violet has the shortest wavelength and greatest deviation; red has the longest wavelength, lowest visible frequency and least deviation.
  • Lens sign convention and ordinary distance measurement: In the Cartesian convention used in school problems, distances measured in the direction of incident light are usually negative, while distances measured opposite to it are positive.

What Gets Asked

  • Applying refraction rules: Questions may ask whether a ray bends towards or away from the normal when moving between rarer and denser media. The mark-losing error is reversing the direction of bending.
  • Using refractive-index equations: Problems may require , relative refractive index, or Snell's law . A common slip is treating the frequency as changed during refraction; the frequency remains unchanged.
  • Identifying total internal reflection: Students must state both conditions: travel from a denser to a rarer medium and incidence at an angle greater than the critical angle. At , the ray is refracted along the boundary rather than totally internally reflected.
  • Determining lens images: Questions may specify an object's position relative to and . Marks are lost by confusing the image descriptions for positions beyond , at , between and , at , and between the optical centre and .
  • Calculating lens quantities: Questions may use , , , or . The specific risk is using an incorrect sign convention or forgetting that focal length must be in metres for power in dioptres.
  • Explaining prisms and scattering: Questions may ask why violet deviates most, why the sky is blue, why the Sun appears reddish at sunrise and sunset, why clouds appear white, or why stars twinkle. The required distinctions are wavelength-dependent scattering, nearly equal scattering by large cloud droplets, and repeated atmospheric refraction.

Flashcards

Quick quiz

What happens when light travels from an optically rarer medium to an optically denser medium?

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Syllabus-verified

Learning objectives

  • P2.1Define refraction of light and state the laws of refraction.
  • P2.2Define critical angle and total internal reflection, and describe one everyday application, such as an optical fibre.
  • P2.3Describe the formation of images by a convex lens for different object positions, using ray diagrams.
  • P2.4Distinguish between a convex lens and a concave lens in terms of their effect on parallel rays of light.
  • P2.5Explain the dispersion of white light by a glass prism in terms of the different refraction of different colours.
  • P2.6Explain the scattering of light and use it to account for the blue colour of the sky.
Syllabus-verified

Practice questions

Q1. Total internal reflection of light occurs when light travels:1 mark · core
  • A. From a rarer to a denser medium at any angle
  • B. From a denser to a rarer medium at an angle greater than the critical angle
  • C. From a denser to a rarer medium at an angle less than the critical angle
  • D. Through a medium of uniform density

Answer: B

  • 1 mark for selecting B

Total internal reflection occurs only when light travels from a denser to a rarer medium and strikes the boundary at an angle greater than the critical angle for that pair of media.

Q2. An object is placed beyond twice the focal length (2F) of a convex lens. State the nature, position, and relative size of the image formed.3 marks · core

Answer: The image is real and inverted, formed between F and 2F on the other side of the lens, and it is diminished (smaller than the object).

  • 1 mark: image is real and inverted
  • 1 mark: image is formed between F and 2F on the other side of the lens
  • 1 mark: image is diminished (smaller than the object)
Q3. When white light passes through a glass prism, it splits into a spectrum of colours. Explain why this happens, and state which colour is deviated the least.3 marks · core

Answer: White light is made up of several colours, each with a different wavelength. Each colour is refracted by a different amount as it passes through the prism, since the refractive index of glass is slightly different for each wavelength; this causes the colours to separate into a spectrum. Red light, having the longest wavelength, is deviated the least.

  • 1 mark: white light is composed of several colours of different wavelengths
  • 1 mark: each colour is refracted by a different amount due to differing refractive index for each wavelength
  • 1 mark: red is correctly identified as the least deviated colour
Q4. Explain briefly why the sky appears blue during the day.2 marks · core

Answer: Sunlight passing through the atmosphere is scattered by gas molecules and small particles; blue light, having a shorter wavelength, is scattered much more strongly than other colours, so the scattered blue light reaches our eyes from all directions across the sky.

  • 1 mark: sunlight is scattered by molecules/particles in the atmosphere
  • 1 mark: blue light (shorter wavelength) is scattered more strongly than other colours, reaching the eye from all parts of the sky

Key ideas to master

  • Explain the core principle behind Light in clear scientific language.
  • Use the correct equations, symbols, and units when solving numerical questions.
  • Interpret diagrams, graphs, or experiments linked to the topic.
  • Connect conceptual understanding with the final answer instead of memorising formulas alone.

Common exam prompts

  • State the law, principle, or definition behind Light precisely.
  • Apply the relevant equation to a short numerical problem with correct units.
  • Explain a diagram, graph, or experiment related to Light.
  • Distinguish between conceptual understanding and memorised formula use in this chapter.

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Step 2

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Step 3

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Quick answers students usually need

What is Light in ICSE Class 10 Physics?

Refraction, total internal reflection, lenses, prisms, and scattering.

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