Class 10 Science · Chapter 9

Light – Reflection and Refraction

Spherical mirrors, ray diagrams, mirror formula, refraction, refractive index, lenses, lens formula and power.

NCERT Science (Textbook for Class X)CBSE Class 10 13 min read

1. Chapter at a Glance

We see objects because light from them enters our eyes. Light travels in straight lines (very small objects can bend it, but for everyday optics we use straight-line rays). When light falls on a polished surface it reflects; when it passes from one transparent medium into another it refracts (bends). This chapter studies images formed by spherical mirrors and spherical lenses using ray diagrams, the New Cartesian sign convention, the mirror and lens formulae, magnification, refractive index and the power of a lens — a numerical-heavy chapter for board exams.

What you will learn
  • Laws of reflection; terms for spherical mirrors; f = R/2.
  • Ray diagrams and image tables for concave and convex mirrors; uses.
  • Sign convention, mirror formula and magnification.
  • Refraction through a glass slab; laws of refraction; refractive index.
  • Convex and concave lenses, lens formula, magnification and power.

2. Reflection of Light

Laws of reflection: (i) the angle of incidence equals the angle of reflection; (ii) the incident ray, the normal at the point of incidence and the reflected ray lie in the same plane. These laws apply to all reflecting surfaces, including curved ones. A plane mirror forms a virtual, erect image of the same size, as far behind the mirror as the object is in front, and laterally inverted.

Spherical mirrors — terms

  • Concave mirror: reflecting surface curved inwards (faces the centre of the sphere). Convex mirror: reflecting surface curved outwards.
  • Pole (P): centre of the reflecting surface. Centre of curvature (C): centre of the sphere of which the mirror is a part (in front for concave, behind for convex). Radius of curvature (R): distance PC.
  • Principal axis: line through P and C. Principal focus (F): point where rays parallel to the axis meet after reflection (concave) or appear to diverge from (convex). Focal length f = PF.
  • For mirrors of small aperture: R = 2f.

Rules for ray diagrams (any two are enough)

  1. A ray parallel to the principal axis passes through (or appears to come from) F after reflection.
  2. A ray through F (or directed towards F) becomes parallel to the axis.
  3. A ray through C (or directed towards C) retraces its path.
  4. A ray incident obliquely at P is reflected obliquely, making equal angles with the axis.
Concave mirror converging parallel rays to a real focus in front and convex mirror diverging them from a virtual focus behind; real-life uses such as torch reflectors, solar cookers, shaving mirrors, rear-view and road-bend security mirrors; image formation by a concave mirror for object beyond C, at C, between C and F, between F and P, and by a convex mirror
Spherical mirrors: focus, uses and image formation. The small ray sketches are schematic; use the table below for exact positions.
Object position (concave mirror)Image positionSizeNature
At infinityAt FHighly diminished, point-sizedReal, inverted
Beyond CBetween F and CDiminishedReal, inverted
At CAt CSame sizeReal, inverted
Between C and FBeyond CEnlargedReal, inverted
At FAt infinityHighly enlargedReal, inverted
Between P and FBehind the mirrorEnlargedVirtual, erect

Convex mirror: object at infinity → image at F behind the mirror, point-sized; object anywhere between infinity and P → image between P and F behind the mirror, diminished, virtual and erect.

Uses: concave — torches, searchlights and vehicle headlights (parallel beam), shaving and dentists' mirrors (enlarged image), solar furnaces. Convex — rear-view mirrors of vehicles, because they always give an erect image and have a wider field of view.

3. Sign Convention, Mirror Formula and Magnification

New Cartesian sign convention: the pole is the origin and the principal axis is the x-axis; the object is placed to the left; distances measured along the incident light (to the right) are positive, against it (to the left) negative; heights above the axis are positive, below negative. So for a concave mirror f is negative; for a convex mirror f is positive; object distance u is always negative.

New Cartesian sign convention for concave and convex mirrors with negative distances to the left of the pole and positive to the right; refraction through a rectangular glass slab showing lateral displacement; converging action of a convex lens and diverging action of a concave lens
Sign convention, refraction through a glass slab, and the action of lenses.
Mirror formula and magnification

1/v + 1/u = 1/f    m = h′/h = −v/u

Negative m → real, inverted image; positive m → virtual, erect image. |m| > 1 enlarged, < 1 diminished.

Worked example: an object is 10 cm in front of a concave mirror of focal length 15 cm. u = −10 cm, f = −15 cm. 1/v = 1/f − 1/u = −1/15 + 1/10 = 1/30 → v = +30 cm (behind the mirror, virtual). m = −v/u = −30/(−10) = +3 → erect and three times enlarged.

4. Refraction of Light

A pencil partly in water looks bent; a coin in a bucket appears raised. Light changes speed when it passes obliquely from one medium into another, so it bends. In a rectangular glass slab, light bends towards the normal on entering glass (rarer → denser) and away from the normal on leaving it. The emergent ray is parallel to the incident ray but shifted sideways — lateral displacement. A ray falling along the normal goes straight without bending.

Laws of refraction: (i) the incident ray, refracted ray and normal lie in the same plane; (ii) Snell's law — for a given colour and pair of media, sin i / sin r = constant (the refractive index of the second medium with respect to the first).

Refractive index: n21 = v1/v2 (speed of light in medium 1 / in medium 2). The absolute refractive index nm = c/v, where c = 3 × 108 m/s is the speed of light in vacuum. A medium with larger n is optically denser (light is slower in it). Optical density is not the same as mass density — kerosene (n = 1.44) is optically denser than water (n = 1.33) but lighter.

5. Refraction by Spherical Lenses

A convex (converging) lens is thicker at the middle; a concave (diverging) lens is thicker at the edges. A lens has two centres of curvature (C1, C2), an optical centre (O) through which rays pass undeviated, and two principal foci F1, F2 on either side. Ray rules: a ray parallel to the axis passes through (convex) or appears to come from (concave) the focus; a ray through the focus emerges parallel; a ray through O goes straight.

Ray diagrams for a convex lens with object beyond 2F1, between F1 and 2F1, and between F1 and O (virtual, upright, enlarged image), and for a concave lens with object at infinity, beyond 2F1 and between F1 and O
Image formation by convex and concave lenses, with candle-and-screen examples.
Table of image formation by a convex lens for object beyond 2F1, at 2F1, between F1 and 2F1, at F1, and between F1 and O, with ray diagrams
Convex lens: image for different object positions.
Table of image formation by a concave lens for different object positions; image always between O and F1 on the same side, virtual and upright
Concave lens: the image is always virtual, upright and diminished.
Object position (convex lens)Image positionSizeNature
At infinityAt F2Point-sizedReal, inverted
Beyond 2F1Between F2 and 2F2DiminishedReal, inverted
At 2F1At 2F2Same sizeReal, inverted
Between F1 and 2F1Beyond 2F2EnlargedReal, inverted
At F1At infinityHighly enlargedReal, inverted
Between F1 and OSame side as objectEnlargedVirtual, erect (magnifying glass)

Concave lens: object at infinity → image at F1, point-sized; any other position → between F1 and O, diminished, virtual and erect.

Lens formula, magnification and power

1/v − 1/u = 1/f    m = h′/h = v/u    P = 1/f (f in metres)

SI unit of power: dioptre (D); 1 D = 1 m−1. Convex lens: f and P positive; concave: negative. For lenses in contact, P = P1 + P2 + P3 + …

Worked example: a concave lens of focal length 15 cm forms an image 10 cm from the lens. Find u. v = −10 cm, f = −15 cm. 1/u = 1/v − 1/f = −1/10 + 1/15 = −1/30 → u = −30 cm. m = v/u = −10/−30 = +1/3 (virtual, erect, one-third size). Power of this lens P = 1/(−0.15) ≈ −6.7 D.

Glass slab Incident ray Emergent ray lateral shift
Through a glass slab the emergent ray is parallel to the incident ray but displaced sideways.

6. Master Table: Formulas

QuantityFormula
Focal length and radiusf = R/2
Mirror formula1/v + 1/u = 1/f
Magnification (mirror)m = h′/h = −v/u
Snell's lawsin i / sin r = n21
Refractive indexn21 = v1/v2; n = c/v
Lens formula1/v − 1/u = 1/f
Magnification (lens)m = h′/h = v/u
PowerP = 1/f (m); unit dioptre

7. Master Summary Table

Devicef signCan form real image?Virtual image is
Concave mirrorNegativeYesEnlarged (object between P and F)
Convex mirrorPositiveNoAlways diminished
Convex lensPositiveYesEnlarged (object between F1 and O)
Concave lensNegativeNoAlways diminished

Chart — absolute refractive indices of some media (NCERT values):

Air1.0003
Water1.33
Kerosene1.44
Crown glass1.52
Diamond2.42

8. Mind Map

Light
Reflection
  • Laws; plane mirror
  • Concave, convex; R = 2f
Mirror maths
  • Sign convention
  • 1/v + 1/u = 1/f; m = −v/u
Refraction
  • Glass slab, Snell's law
  • n = c/v
Lenses
  • 1/v − 1/u = 1/f; m = v/u
  • P = 1/f (D)

9. Tips and Tricks

Smart ideas
  • Mirror formula has + (1/v + 1/u); lens formula has − (1/v − 1/u).
  • Mirror m has a minus (−v/u); lens m has none (v/u).
  • “Concave Converges, conVEX diVErges” for mirrors; for lenses it is the opposite: convex converges.
  • Always convert f to metres before finding power.
  • Real images are always inverted; virtual images are always erect.
Common mistakes
  • Forgetting the negative sign of u.
  • Using cm in P = 1/f.
  • Saying a convex mirror can form a real image.
  • Assuming optically denser means heavier.

10. Important One-liners

  • Angle of incidence equals angle of reflection.
  • For small-aperture mirrors, R = 2f.
  • Convex mirrors are used as rear-view mirrors.
  • Concave mirrors are used in torches and as shaving mirrors.
  • Light bends towards the normal entering a denser medium.
  • Emergent ray from a glass slab is parallel to the incident ray.
  • Speed of light in vacuum is 3 × 108 m/s.
  • Diamond has refractive index 2.42.
  • A convex lens used as a magnifier has the object between F and O.
  • 1 dioptre is the power of a lens of focal length 1 m.

11. Exam-pattern Questions with Detailed Answers

Q1Easy

The focal length of a concave mirror is 20 cm. Its radius of curvature is:

  1. 10 cm
  2. 20 cm
  3. 40 cm
  4. 80 cm
Show answer

R = 2f = 40 cm.

Answer: (C)

Q2Easy

Which mirror gives a wider field of view? Where is it used?

Show answer

Convex mirror — rear-view mirrors of vehicles and security mirrors at road bends.

Answer: Convex mirror; rear-view mirrors

Q3Easy

Find the power of a convex lens of focal length 50 cm.

Show answer

f = +0.5 m; P = 1/0.5 = +2 D.

Answer: +2 D

Q4Medium

Assertion (A): A ray of light passing through the optical centre of a lens goes undeviated. Reason (R): Near the optical centre the two faces of the lens are almost parallel, like a thin glass slab.

  1. Both true; R explains A
  2. Both true; R does not explain A
  3. A true, R false
  4. A false, R true
Show answer

A thin parallel slab gives negligible lateral shift, so the ray continues straight.

Answer: (A)

Q5Medium

An object 4 cm high is placed 25 cm in front of a concave mirror of focal length 15 cm. Find the position, nature and size of the image.

Show answer

u = −25, f = −15. 1/v = 1/f − 1/u = −1/15 + 1/25 = (−5 + 3)/75 = −2/75 → v = −37.5 cm (in front, real). m = −v/u = −(−37.5)/(−25) = −1.5; h′ = −1.5 × 4 = −6 cm.

Answer: 37.5 cm in front; real, inverted, 6 cm tall (enlarged)

Q6Medium

The refractive index of diamond is 2.42. What does this mean? Find the speed of light in diamond.

Show answer

Light travels 2.42 times slower in diamond than in vacuum. v = c/n = 3 × 108 / 2.42 ≈ 1.24 × 108 m/s.

Answer: ≈ 1.24 × 108 m/s

Q7Medium

An object is placed 20 cm from a convex lens of focal length 10 cm. Where is the image and what is its nature?

Show answer

u = −20 = 2F1. 1/v = 1/f + 1/u = 1/10 − 1/20 = 1/20 → v = +20 cm. m = v/u = −1.

Answer: At 2F2 (20 cm on the other side); real, inverted, same size

Q8Medium

Two lenses of power +3.5 D and −2.5 D are placed in contact. Find the power and focal length of the combination. Is it converging or diverging?

Show answer

P = 3.5 − 2.5 = +1 D; f = 1/P = 1 m = 100 cm; positive, so converging.

Answer: +1 D, f = 100 cm, converging

Q9Hard

A convex lens forms a real image three times magnified at 60 cm from the lens. Find the object distance and the focal length.

Show answer

Real image → m = −3, v = +60 cm. m = v/u → u = 60/(−3) = −20 cm. 1/f = 1/v − 1/u = 1/60 + 1/20 = 4/60 → f = 15 cm.

Answer: u = −20 cm; f = +15 cm

Q10Hard

Case-based: A student focuses the image of a distant tree on a screen using a lens and finds the screen 25 cm from the lens. (a) Which lens is it? (b) What is its focal length and power? (c) Where should she place a candle to get a same-size image on the screen? (d) Where should the candle be to use this lens as a magnifier?

Show answer

(a) Convex lens (real image on a screen). (b) Distant object → image at F, so f = +25 cm; P = 1/0.25 = +4 D. (c) At 2F, i.e. 50 cm from the lens (image also at 50 cm on the other side). (d) Closer than 25 cm (between F and O).

Answer: Convex; 25 cm, +4 D; candle at 50 cm; within 25 cm for magnifier

Q11Hard

Light enters from air into glass of refractive index 1.5. If the speed of light in air is 3 × 108 m/s, find its speed in glass. What is the refractive index of glass with respect to water (n = 1.33)?

Show answer

v = c/n = 3 × 108/1.5 = 2 × 108 m/s. nglass,water = nglass/nwater = 1.5/1.33 ≈ 1.13.

Answer: 2 × 108 m/s; ≈ 1.13

Q12Hard

A convex mirror used on a car has a radius of curvature of 3.00 m. A bus is 5.00 m from the mirror. Find the position, nature and size of the image.

Show answer

R = +3.00 m → f = +1.50 m; u = −5.00 m. 1/v = 1/f − 1/u = 1/1.5 + 1/5 = (10 + 3)/15 = 13/15 → v ≈ +1.15 m (behind the mirror). m = −v/u = −1.15/(−5) ≈ +0.23.

Answer: 1.15 m behind; virtual, erect, about 0.23 times the size

12. Quick Revision Summary

Revise in 2 minutes
  • Laws of reflection; R = 2f; ray rules through P, F, C.
  • Concave mirror: real images except when object is between P and F; convex mirror: always virtual, erect, diminished.
  • Mirror: 1/v + 1/u = 1/f, m = −v/u; sign convention from the pole.
  • Refraction: towards the normal into a denser medium; Snell's law; n = c/v.
  • Lens: 1/v − 1/u = 1/f, m = v/u; P = 1/f (m) in dioptres; P adds for lenses in contact.