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MERITROOT FREE LEARNING · CLASS 10 / PHYSICS

Human Eye and Colourful World

Your chapter workspace for understanding concepts, revising key ideas and practising questions. Choose an available resource below.

PYQs5Formulae4Derivations3
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PYQs

Practise questions grouped by chapter and source year.

Practice questions are organised using the years and labels in our source collection. Work through the solutions with your teacher; these are not a complete official examination paper.

Practice question 1

Source year: 20253 marks

A person cannot see objects distinctly placed within 50 cm from his eyes. Name the defect of vision and the lens used to correct it. Calculate the power of lens required. [CBSE 2025]

Practice question 2

Source year: 20243 marks

Explain why the sun appears reddish at sunrise and sunset. [CBSE 2024]

Practice question 3

Source year: 20233 marks

What is meant by power of accommodation of human eye? How is the range of vision of a normal eye different from that of a person suffering from myopia? [CBSE 2023]

Practice question 4

Source year: 20222 marks

Draw a labelled diagram showing the dispersion of white light through a glass prism. [CBSE 2022]

Practice question 5

Source year: 20212 marks

Why does the sky appear blue on a clear day? Explain with scientific reason. [CBSE 2021]

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Formulae

Revisit important relationships and quick revision formulae.

Least Distance of Distinct Vision

D = 25 cm (for normal eye) Minimum distance at which eye can see clearly

Power for Myopia Correction

P = -1/d (in meters) d = far point distance

Power for Hypermetropia

P = 1/d - 1/D D = 25 cm (least distance of distinct vision)

Range of Vision

Normal eye: 25 cm to infinity Near point: 25 cm Far point: Infinity

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Derivations

Work through the reasoning behind key concepts.

Scattering of Light (Rayleigh Scattering)

Intensity of scattered light ∝ 1/λ⁴ Blue light (shorter wavelength) scatters more than red This explains blue sky and red sunset

Correction of Myopia

For person with far point at distance d: Required focal length: f = -d Power: P = -1/d (concave lens)

Dispersion in Prism

Different wavelengths refract differently Refractive index varies: n ∝ 1/λ Red (longest λ) bends least, Violet (shortest λ) bends most

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