By the end of this chapter you'll be able to…

  • 1Apply laws of reflection
  • 2Distinguish concave and convex mirrors
  • 3Use mirror and lens formulas
  • 4Calculate magnification
  • 5Understand refractive index and Snell's law
💡
Why this chapter matters
Foundation of optics. Used in spectacles, cameras, microscopes, telescopes. Indian C.V. Raman heritage.

Before you start — revise these

A 5-minute refresher here will save you 30 minutes of confusion below.

Light - Reflection and Refraction — Class 10 Science

"Light: the messenger that brings the universe to our eyes."

1. About the Chapter

This chapter explores how light BEHAVES:

  • Reflection (bouncing back)
  • Refraction (bending in different media)
  • Mirrors (spherical: concave, convex)
  • Lenses (concave, convex)
  • Formulas for mirror/lens

Why Important

  • All optics: spectacles, microscopes, cameras
  • Visual perception
  • Indian Raman Effect heritage

2. Reflection of Light

Definition

When light strikes a surface and BOUNCES BACK.

Laws of Reflection

  1. Angle of incidence = Angle of reflection (i = r)
  2. Incident ray, normal, reflected ray are all in the same plane.

Types of Reflection

  • Regular (specular): smooth surfaces; clear images. Examples: mirrors.
  • Diffuse: rough surfaces; scattered. Examples: paper, walls.

3. Spherical Mirrors

Two Types

1. Concave Mirror (curves inward — like inside of bowl)

  • Converges parallel rays to a focal point
  • Magnifies image when object close

2. Convex Mirror (curves outward — like back of spoon)

  • Diverges parallel rays
  • Always forms small, virtual image

Important Terms

  • Centre of Curvature (C): centre of the sphere
  • Radius of Curvature (R): distance from C to surface
  • Pole (P): midpoint of mirror
  • Focus (F): where parallel rays converge (or appear to)
  • Focal Length (f): distance from pole to focus
  • f = R/2 (for spherical mirrors)

Sign Conventions

  • All distances measured from POLE
  • Distances in DIRECTION OF INCIDENT LIGHT: positive
  • Distances AGAINST direction of incident light: negative
  • Heights ABOVE principal axis: positive
  • Heights BELOW principal axis: negative

Mirror Formula

1/v + 1/u = 1/f

where:

  • u = object distance
  • v = image distance
  • f = focal length

Magnification

m = h'/h = −v/u

where:

  • h' = image height
  • h = object height
  • m positive: erect; m negative: inverted

4. Image Formation by Concave Mirror

Depends on OBJECT POSITION:

Object PositionImage PositionImage TypeSize
At infinityAt FReal, invertedHighly diminished
Beyond CBetween F and CReal, invertedDiminished
At CAt CReal, invertedSame size
Between C and FBeyond CReal, invertedMagnified
At FAt infinityHighly magnified
Between F and PBehind mirrorVirtual, erectMagnified

Uses

  • Shaving mirror (close object: erect, magnified)
  • Dentist's mirror
  • Headlights (object at focus: parallel beam)
  • Solar concentrator
  • Astronomical telescope

5. Image Formation by Convex Mirror

ALWAYS:

  • Virtual (behind mirror)
  • Erect
  • Diminished
  • Smaller than object

Uses

  • Rear-view mirror (wide field of view)
  • Security mirrors in shops
  • Vehicle side mirrors

6. Refraction of Light

Definition

Bending of light when passing from one medium to another.

Why Does It Happen?

Light travels at DIFFERENT SPEEDS in different media.

  • Vacuum/air: ~3 × 10⁸ m/s
  • Water: ~2.25 × 10⁸ m/s (slower)
  • Glass: ~2 × 10⁸ m/s (even slower)

Laws of Refraction

  1. Incident ray, refracted ray, and normal — all in SAME PLANE
  2. sin(angle of incidence) / sin(angle of refraction) = constant

The constant = REFRACTIVE INDEX (n) of the second medium with respect to the first.

Snell's Law

n₁ sin θ₁ = n₂ sin θ₂

For light entering DENSER medium: bends TOWARDS normal. For light entering RARER medium: bends AWAY from normal.

Refractive Index

n = c / v

where:

  • c = speed of light in vacuum
  • v = speed in medium

Examples (n values)

  • Air: 1.0003 ≈ 1
  • Water: 1.33
  • Glass: 1.5
  • Diamond: 2.42

Total Internal Reflection

When light goes from denser to rarer medium at angle > critical angle, it reflects entirely back.

  • Used in OPTICAL FIBRES
  • Sparkling of diamonds
  • Mirage

7. Refraction by Spherical Lenses

Types

1. Convex Lens (thicker in middle): CONVERGING

  • Focuses parallel rays to focal point

2. Concave Lens (thinner in middle): DIVERGING

  • Spreads parallel rays apart

Important Terms

Same as mirrors: optical centre, focal length, etc.

Lens Formula

1/v − 1/u = 1/f

(Note: different sign from mirror formula.)

Magnification (for lens)

m = h'/h = v/u

(Positive sign, unlike mirror.)

Power of a Lens

P = 1/f (in diopters)

where f is in METRES.

  • Convex lens: positive power
  • Concave lens: negative power

Combining Lenses

P = P₁ + P₂ + ...


8. Image Formation by Lenses

Convex Lens (similar pattern to concave mirror):

Object PositionImageType
At infinityAt FReal, inverted, diminished
Beyond 2FBetween F and 2FReal, inverted, diminished
At 2FAt 2FReal, inverted, same size
Between F and 2FBeyond 2FReal, inverted, magnified
At FAt infinity
Between F and centreSame side as objectVirtual, erect, magnified

Concave Lens

ALWAYS forms virtual, erect, diminished image.

Uses

Convex lens:

  • Magnifying glass
  • Camera
  • Microscope (objective)
  • Spectacles for hyperopia (far-sighted)

Concave lens:

  • Spectacles for myopia (near-sighted)
  • Peephole

9. Human Eye (Brief; covered in next chapter)

  • Cornea: outer transparent layer
  • Iris: coloured (controls pupil size)
  • Pupil: opening
  • Lens: convex; focuses light
  • Retina: back of eye; light-sensitive cells
  • Optic nerve: sends signals to brain

(Detailed in Chapter 10.)


10. Worked Examples

Example 1: Concave Mirror

An object is placed 30 cm from a concave mirror of focal length 10 cm. Find image distance and magnification.

Using mirror formula: 1/v + 1/(-30) = 1/(-10)

  • 1/v = -1/10 + 1/30 = -3/30 + 1/30 = -2/30
  • v = -15 cm

Magnification: m = -v/u = -(-15)/(-30) = -0.5

Image is REAL (v negative for concave mirror in this convention), INVERTED, HALF size.

Example 2: Refractive Index

Light enters water (n=1.33) from air. Speed in water?

  • n = c/v
  • 1.33 = (3×10⁸) / v
  • v = 3×10⁸ / 1.33 ≈ 2.25 × 10⁸ m/s

Example 3: Lens Formula

A convex lens of f = 20 cm produces image at v = 30 cm. Find object distance.

1/v - 1/u = 1/f 1/30 - 1/u = 1/20 1/u = 1/30 - 1/20 = -1/60 u = -60 cm

Object is 60 cm from lens (on negative side).

Example 4: Power of Lens

A lens has focal length 25 cm. Find its power.

  • P = 1/f = 1/0.25 = +4 diopters (convex)

11. Common Mistakes

  1. Concave vs convex confusion

    • CONCAVE mirror: curves INWARD (like bowl interior). CONVERGES.
    • CONVEX mirror: curves OUTWARD (like back of spoon). DIVERGES.
    • For LENSES, it's reversed: convex lens converges; concave lens diverges.
  2. Sign convention errors

    • Strict rules. Memorise. Distances behind mirror/in front of lens — be careful with signs.
  3. Mirror vs lens formula

    • Mirror: 1/v + 1/u = 1/f
    • Lens: 1/v − 1/u = 1/f
  4. Refractive index value

    • Always ≥ 1 for media (vacuum is 1; all media > 1).
  5. Magnification sign

    • Negative m = inverted image. Positive m = erect.

12. Indian Heritage

C.V. Raman (Indian Physicist)

  • Won NOBEL PRIZE 1930 for the RAMAN EFFECT
  • Discovered that light changes wavelength when scattered by molecules
  • 28 February celebrated as National Science Day in India

Aryabhata

Discussed reflection and refraction in ancient texts.

Modern Indian Optics

  • ISRO uses optical instruments for satellite imaging
  • Indian Astronomical Observatory (Hanle, Ladakh)
  • World-class telescopes built by Indian scientists

13. Conclusion

Light's behaviour follows precise rules:

  • Reflection: angle in = angle out
  • Refraction: bends in new medium (Snell's law)
  • Mirrors and lenses: form images per formulas
  • Sign conventions: critical for problems

Master:

  • Two laws (reflection, refraction)
  • Mirror formula (1/v + 1/u = 1/f) and lens formula (1/v - 1/u = 1/f)
  • Magnification
  • Image formation tables
  • Power of lens

Practice 15+ problems. This is HIGH-MARK chapter for board exam.

Optics: how the world reveals itself to your eyes.

Key formulas & results

Everything you need to memorise, in one card. Screenshot this for revision.

Mirror formula
1/v + 1/u = 1/f
Sign convention important
Magnification (mirror)
m = -v/u = h'/h
Lens formula
1/v - 1/u = 1/f
Magnification (lens)
m = v/u = h'/h
f = R/2
Focal length = half radius of curvature
Snell's law
n₁ sin θ₁ = n₂ sin θ₂
Refractive index
n = c/v
Speed of light in vacuum / speed in medium
Power of lens
P = 1/f (in diopters; f in meters)
Convex +, concave -
⚠️

Common mistakes & fixes

These are the exact errors that cost students marks in board exams. Read them once, save yourself the trouble.

WATCH OUT
Concave vs convex for lens vs mirror
MIRROR: concave converges, convex diverges. LENS: convex converges, concave diverges. (For lenses, it's opposite to mirrors)
WATCH OUT
Mirror formula vs lens formula
Mirror: 1/v + 1/u = 1/f (plus). Lens: 1/v - 1/u = 1/f (minus). Different!
WATCH OUT
Sign convention errors
All distances from POLE. Same direction as incident light = positive. Heights above axis = positive.

NCERT exercises (with solutions)

Every NCERT exercise from this chapter — what it covers and how many questions to expect.

Practice problems

Try each one yourself before tapping "Show solution". Active recall > rereading.

Q1EASY· Mirror
What kind of image is formed by a convex mirror?
Show solution
✦ Answer: Always VIRTUAL, ERECT, DIMINISHED (smaller than object).
Q2EASY· Refraction
What is the refractive index of water?
Show solution
✦ Answer: 1.33. Light is about 1.33 times slower in water than in vacuum.
Q3MEDIUM· Mirror formula
An object is placed 15 cm in front of a concave mirror of focal length 10 cm. Find image distance.
Show solution
Step 1 — Sign conventions. Concave mirror: f = -10 cm (negative) Object in front: u = -15 cm Step 2 — Mirror formula. 1/v + 1/u = 1/f 1/v + 1/(-15) = 1/(-10) 1/v = -1/10 + 1/15 1/v = -3/30 + 2/30 = -1/30 v = -30 cm Step 3 — Interpret. v negative → image is REAL (on same side as object). Image at 30 cm from mirror. Step 4 — Magnification. m = -v/u = -(-30)/(-15) = -2 Image is INVERTED (negative m) and TWICE the size (|m|=2). ✦ Answer: Image at -30 cm (real, inverted, magnified 2x).
Q4HARD· Combined
Find the power of a lens with focal length 50 cm and discuss its use.
Show solution
Step 1 — Convert f to metres. f = 50 cm = 0.5 m Step 2 — Calculate power. P = 1/f = 1/0.5 = 2 diopters Step 3 — Convex or concave? Positive power → CONVEX (converging) lens. Power = +2 D Step 4 — Uses of convex lens. • MAGNIFYING GLASS (when object close) • CAMERA LENS • READING GLASSES for HYPERMETROPIA (far-sightedness) • Microscope and telescope objective lenses Step 5 — Practical application. +2 D is suitable for someone with mild hypermetropia. They cannot see nearby objects clearly. The lens converges light, forming a clear image on retina. Step 6 — Compare to concave lens. Concave lens would have NEGATIVE power. Used for MYOPIA (near-sightedness). Step 7 — Combining lenses. If combined with another lens of power P₂, total: P = P₁ + P₂. Useful in spectacles, eyepieces. Step 8 — Indian eye-care. India has 30M+ visually impaired. Affordable spectacles via Aravind Eye Care. ✦ Answer: P = 1/0.5 = +2 diopters. Convex (converging) lens. Used in: magnifying glasses, cameras, reading glasses for hypermetropia (far-sightedness), microscopes. Compared to concave lens (negative power, for myopia).

5-minute revision

The whole chapter, distilled. Read this the night before the exam.

  • Laws of reflection: i = r; rays/normal in same plane
  • Concave mirror: converges; convex mirror: diverges
  • Mirror formula: 1/v + 1/u = 1/f
  • Magnification (mirror): m = -v/u
  • Refraction: light bends in new medium
  • Snell's law: n₁ sin θ₁ = n₂ sin θ₂
  • Refractive index n = c/v; air ≈1, water 1.33, glass 1.5, diamond 2.42
  • Convex lens: converges; concave lens: diverges
  • Lens formula: 1/v - 1/u = 1/f
  • Power of lens P = 1/f (f in m); diopters
  • Convex lens: positive power; Concave lens: negative power
  • C.V. Raman: Nobel 1930 for Raman Effect (scattering of light)

CBSE marks blueprint

Where the marks come from in this chapter — so you can plan your prep.

Typical chapter weightage: 10-12 marks

Question typeMarks eachTypical countWhat it tests
MCQ13Definitions, types
Short2-32Formulas, applications
Long51Mirror/lens problem with diagram
Prep strategy
  • Memorise formulas
  • Practice sign conventions
  • Master image tables
  • Know refractive index values

Where this shows up in the real world

This chapter isn't just an exam topic — it lives in the world around you.

Indian spectacles

30M+ Indians need vision correction. Aravind Eye Care provides affordable lenses.

Cameras and phones

All cameras use convex lenses. Indian phones (Realme, Xiaomi, OnePlus) use complex multi-lens systems.

C.V. Raman heritage

Bangalore-based Indian Institute of Science where Raman did his Nobel work.

ISRO astronomy

Indian telescopes (Hanle Observatory) use precise optics.

Exam strategy

Battle-tested tips from teachers and toppers for this chapter.

  1. Memorise formulas COLD
  2. Use proper sign conventions
  3. Draw ray diagrams
  4. Verify with image table

Going beyond the textbook

For olympiad aspirants and curious learners — topics that build on this chapter.

  • Aberrations (chromatic, spherical)
  • Total internal reflection (fibre optics)
  • Wave optics (Class 12)
  • Quantum optics

Where else this chapter is tested

CBSE board isn't the only one — other exams test this chapter too.

CBSE Class 10 BoardVery High
Science OlympiadVery High
JEE/NEETVery High

Questions students ask

The real ones — pulled from the Q&A community and tutor sessions.

Light travels SLOWER in denser medium (like water). When it enters water at an angle, the side entering first slows first — causing the ray to BEND. Like a car turning when one wheel hits soft sand. This is REFRACTION, governed by Snell's law.
Verified by the tuition.in editorial team
Last reviewed on 20 May 2026. Written and reviewed by subject-matter experts — read about our process.
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