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Class 10 Light: Reflection and Refraction Notes | Class 10 Science

Class 10 Light — Reflection and Refraction covers how light travels, reflects off mirrors, and bends through lenses. Key formulas include the mirror formula (1/v + 1/u = 1/f) and Snell's law (n = sin i / sin r). These concepts form Chapter 10 of the CBSE Class 10 Science syllabus and carry significant weight in board exams.
Class 10 Light: Reflection and Refraction  Notes | Class 10 Science

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eSaral > Class 10 Science Notes > Light: Reflection and Refraction

Light is one of the highest-scoring topics in the CBSE Class 10 Science board exam. Chapter 10 covers two connected phenomena — reflection (light bouncing off surfaces) and refraction (light bending as it changes medium) — and builds every concept from first principles. Students who understand the sign convention, master ray diagrams, and can apply the mirror formula and lens formula without hesitation routinely score full marks on this chapter.

These notes follow the exact CBSE syllabus sequence. Each section gives you the definition, the underlying law, worked examples, and a table or diagram reference so you can revise efficiently. For step-by-step solutions to textbook problems, check the NCERT Solutions on eSaral, which are prepared by IIT Bombay faculty AIR-41 rankers who know exactly which question types appear in board papers.


What is Light and How Does It Behave?

Light is electromagnetic radiation that the human eye can detect. It travels as a transverse wave and also behaves as a stream of energy packets called photons — a property known as wave-particle duality.

Key Physical Properties of Light

Property Value / Description
Speed in a vacuum $3.0 \times 10^8\ \text{m/s}$
Visible wavelength range 400 nm (violet) – 700 nm (red)
Nature Electromagnetic (transverse wave)
Medium required? No — travels through vacuum
Energy packet Photon

What is Rectilinear Propagation of Light?

Rectilinear propagation means light travels in straight lines through a uniform medium. This explains sharp-edged shadows, the working of a pinhole camera, and the formation of solar and lunar eclipses. Light only changes direction in two situations: when it reflects off a surface or refracts as it crosses from one medium to another.

Wave-Particle Duality in Simple Terms

Thomas Young's 1801 double-slit experiment confirmed light's wave nature through interference. Albert Einstein's 1905 explanation of the photoelectric effect confirmed its particle nature. For Class 10, the practical takeaway is that light shows wave behaviour during reflection and refraction, while its photon nature matters more in senior classes and JEE Physics.


What Are the Laws of Reflection?

The two laws of reflection are: (1) the incident ray, reflected ray, and normal at the point of incidence are all in the same plane; and (2) the angle of incidence always equals the angle of reflection ($\angle i = \angle r$). Both angles are measured from the normal to the reflecting surface.

Regular vs. Diffused Reflection

Feature Regular Reflection Diffused Reflection
Surface type Smooth, polished Rough, uneven
Reflected rays Parallel — stay parallel Parallel — scatter in all directions
Image formed Clear and sharp No distinct image
Examples Mirror, calm water Paper, wood, walls

Both types obey the same two laws. In diffused reflection, each individual ray still follows $\angle i = \angle r$ — but because surface normals point in random directions, the outgoing rays scatter.

Plane Mirror Image Characteristics

  • Image is virtual (cannot be projected on a screen)
  • Image is erect (upright)
  • Image is laterally inverted (left-right flipped)
  • Image distance behind the mirror = object distance in front of the mirror
  • Image size = object size (magnification = +1)
Exam Tip: Virtual means the image cannot be caught on a screen. A plane mirror image is always virtual and erect.

Principle of Reversibility of Light

If you reverse the direction of a reflected (or refracted) ray, it retraces its original path exactly. This principle is used in designing periscopes, kaleidoscopes, and multi-lens optical instruments.


Spherical Mirrors and Image Formation

Concave vs. Convex Mirrors — Key Differences

Feature Concave Mirror Convex Mirror
Reflecting surface Inner curved side Outer curved side
Also called Converging mirror Diverging mirror
Focus position In front of a mirror (real) Behind the mirror (virtual)
Image type Real or virtual Always virtual, erect, diminished
Common uses Torches, shaving mirrors, solar cookers Rear-view mirrors

Important Terms

  • Pole (P): Geometric centre of the mirror.
  • Centre of Curvature (C): Centre of the sphere.
  • Radius of Curvature (R): Distance from P to C.
  • Principal Focus (F): Point where rays converge/diverge.
  • Focal Length (f): $f = \frac{R}{2}$

Mirror Formula

The mirror formula is:

$\frac{1}{v} + \frac{1}{u} = \frac{1}{f}$

where $u$ is object distance, $v$ is image distance and $f$ is focal length.

New Cartesian Sign Convention

  • All distances measured from the pole (P)
  • Direction of incident light = positive
  • Opposite direction = negative
  • Concave mirror: $f$ negative
  • Convex mirror: $f$ positive

Magnification Formula

$m = \frac{-v}{u} = \frac{h'}{h}$

Magnification Value Meaning
$m > 0$ Virtual, erect image
$m < 0$ Real, inverted image
$|m| > 1$ Enlarged image
$|m| < 1$ Diminished image
$|m| = 1$ Same size image

How Does Refraction of Light Work?

Refraction is the bending of light when it passes from one transparent medium to another. This bending occurs because light changes speed at the boundary between media.

Laws of Refraction (Snell's Law)

  1. Incident ray, refracted ray and normal lie in the same plane.
  2. For a given pair of media:

    $n = \frac{\sin i}{\sin r}$

What is Refractive Index?

$n = \frac{c}{v} = \frac{3.0 \times 10^8}{v}$

Medium Approximate Refractive Index
Vacuum / Air 1.0
Water 1.33
Glass 1.52
Diamond 2.42

Real-Life Examples of Refraction

  • The pencil appears bent in water.
  • Stars appear to twinkle.
  • The swimming pool appears shallower.
  • Mirages on hot roads.

Check NCERT Solutions for Class 11 Physics


Lenses: Types, Image Formation and Power

Convex vs. Concave Lenses

Feature Convex Lens Concave Lens
Shape Thicker at the centre Thinner at the centre
Effect Converges rays Diverges rays
Focus Real focus Virtual focus
Common Use Magnifying glass, camera Myopia correction

Lens Formula

$\frac{1}{v} - \frac{1}{u} = \frac{1}{f}$

Magnification for Lenses

$m = \frac{v}{u}$

Important: Mirror formula uses addition, while lens formula uses subtraction.

Power of a Lens

Power is the reciprocal of focal length:

$P = \frac{1}{f(\text{in metres})}$

Unit: Dioptre (D)

For lenses in contact:

$P_{total} = P_1 + P_2$

Check NCERT Solutions for Class 12 Physics

Board Exam Tip: Memorize the sign convention, mirror formula, lens formula, magnification formula, refractive index formula, and power formula. These account for most numerical questions asked in this chapter.

Frequently Asked Questions

Find answers to common questions.

What is refractive index and how is it calculated?

Refractive index (n) measures how much a medium reduces the speed of light compared to a vacuum. It is calculated as n = c/v, where c = 3.0 × 10⁸ m/s (speed in vacuum) and v is the speed in the medium. Alternatively, n = sin i/sin r using Snell's law. Diamond has a high refractive index of 2.42, which causes its brilliant sparkle.

What is the difference between a concave and a convex mirror?

A concave mirror has its reflective surface on the inner curved side and converges parallel light rays to a real focus in front of the mirror. A convex mirror has its reflective surface on the outer curved side and diverges rays, forming only virtual, erect, and diminished images. Rear-view mirrors in vehicles are convex; torch reflectors are concave

What are the two laws of reflection?

The first law states that the incident ray, reflected ray, and normal at the point of incidence lie in the same plane. The second law states that the angle of incidence equals the angle of reflection (∠i = ∠r). Both laws hold for every type of reflecting surface — flat, concave, or convex.

What is the mirror formula in Class 10?

The mirror formula is 1/v + 1/u = 1/f, where v is the image distance, u is the object distance, and f is the focal length — all measured from the pole of the mirror using the New Cartesian Sign Convention. This formula applies to both concave and convex mirrors, with sign differences based on the convention

What is the relationship between focal length and radius of curvature?

For any spherical mirror, the focal length (f) is exactly half the radius of curvature (R): f = R/2. This relationship is derived by applying the laws of reflection to a ray parallel to the principal axis. In numericals, if you are given R = 20 cm, the focal length is immediately f = 10 cm.

Why does a pencil appear bent in water?

A pencil appears bent because light rays from the submerged part travel from water (denser medium, n = 1.33) to air (rarer medium, n = 1.0). At the water-air boundary, these rays bend away from the normal. Your eye traces them back as straight lines, making the pencil appear displaced upward — a direct result of refraction.

What is the power of a lens?

Power of a lens is the reciprocal of its focal length measured in metres: P = 1/f. The unit is the dioptre (D). A convex lens has positive power, a concave lens has negative power. An optometrist's prescription of −2.5 D means a concave lens with focal length −0.4 m is needed to correct short-sightedness

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