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

  • 1State Snell's law and define refractive index
  • 2Explain total internal reflection and its applications
  • 3Apply the lens formula and find magnification
  • 4Calculate the power of a lens in dioptres
  • 5Identify and correct myopia and hypermetropia
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Why this chapter matters
Optics explains how light refracts and how lenses form images — the basis of spectacles, cameras, microscopes and optical fibres. It is a high-scoring chapter in the TN SSLC exam with reliable numericals and ray diagrams.

Before you start — revise these

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

Optics — Class 10 Science (Samacheer Kalvi)

TN State Board (Samacheer Kalvi) Class 10 Science, Physics — Chapter 2. How light bends, lenses form images, and how vision defects are corrected.


1. About this chapter

This chapter studies the refraction (bending) of light, the refractive index, total internal reflection, image formation by lenses, and the human eye with its common defects of vision.

2. Refraction and refractive index

  • Refraction: the change in direction of light as it passes from one transparent medium to another due to a change in speed.
  • Laws of refraction (Snell's law):
    1. The incident ray, refracted ray and normal lie in the same plane.
    2. sin i / sin r = constant = n (refractive index).
  • Absolute refractive index: n = c / v (speed of light in vacuum ÷ speed in medium). Denser medium → higher n → light bends towards the normal.
  • Glass slab: the emergent ray is parallel to the incident ray but laterally displaced.

3. Total internal reflection (TIR)

When light travels from a denser to a rarer medium and the angle of incidence exceeds the critical angle (C), it is completely reflected back.

  • Condition: ray goes denser → rarer, and i > C.
  • n = 1 / sin C.
  • Applications: mirage, brilliance of diamond, optical fibres, and total-reflecting prisms.

4. Lenses

TermFormulaNotes
Lens formula1/v − 1/u = 1/fsign convention applies
Magnificationm = h'/h = v/u+ve = erect/virtual, −ve = inverted/real
Power of a lensP = 1/f (in metres)unit dioptre (D); convex +, concave −
  • Convex (converging) lens: thicker at the middle; convex lens can form real or virtual images.
  • Concave (diverging) lens: always forms a virtual, erect, diminished image.

5. The eye and defects of vision

  • The eye focuses light on the retina; the ciliary muscles change the lens focal length (accommodation).
  • Myopia (short sight): distant objects blurred; image forms before the retina; corrected by a concave lens.
  • Hypermetropia (long sight): near objects blurred; image forms behind the retina; corrected by a convex lens.
  • Presbyopia: loss of accommodation with age; corrected by bifocal lenses.

6. Worked examples

Example 1. Light travels at 2×10⁸ m s⁻¹ in glass. Find its refractive index. (c = 3×10⁸) n = c/v = 3×10⁸ / 2×10⁸ = 1.5.

Example 2. A convex lens has focal length 20 cm. Find its power. P = 1/f = 1/0.20 = +5 D.

Example 3. The critical angle of a medium is 30°. Find its refractive index. n = 1/sin C = 1/sin 30° = 1/0.5 = 2.

7. Common mistakes

  • Mistake: Forgetting the sign convention in the lens formula. Fix: Distances measured against the incident light are negative; use the convention consistently.
  • Mistake: Using f in cm for power. Fix: Power needs f in metres (P = 1/f).
  • Mistake: Swapping myopia and hypermetropia corrections. Fix: Myopia → concave lens; hypermetropia → convex lens.

8. Practice (book-back style)

  1. State Snell's law of refraction.
  2. Define refractive index and write n = c/v.
  3. What is total internal reflection? Give two applications.
  4. A lens has power −2 D. Find its focal length and type.
  5. Name and correct the two common defects of vision.

9. Answer key

  1. sin i / sin r = constant (n); incident, refracted rays and normal are coplanar.
  2. Ratio of speed of light in vacuum to that in the medium; n = c/v.
  3. Complete reflection of light at a denser–rarer boundary when i > C; optical fibre, mirage (also diamond brilliance).
  4. f = 1/P = 1/(−2) = −0.5 m = −50 cm; concave (diverging) lens.
  5. Myopia → concave lens; hypermetropia → convex lens.

10. Quick revision

  • Physics Ch 2 · refraction, refractive index, TIR, lenses, eye.
  • Snell: sin i/sin r = n; n = c/v; denser → bends towards normal.
  • TIR: denser→rarer and i > C; n = 1/sin C.
  • Lens: 1/v − 1/u = 1/f; m = v/u; P = 1/f (D).
  • Myopia → concave; hypermetropia → convex.

Key formulas & results

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

Snell's law
sin i / sin r = n
Refractive index of medium 2 w.r.t. medium 1.
Absolute refractive index
n = c / v
c = speed in vacuum, v = speed in medium.
Critical angle
n = 1 / sin C
For total internal reflection (denser to rarer).
Lens formula
1/v − 1/u = 1/f
Use the sign convention.
Magnification
m = h'/h = v/u
Sign shows nature of image.
Power of a lens
P = 1/f (f in metres)
Unit dioptre; convex +, concave −.
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Common mistakes & fixes

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

WATCH OUT
Ignoring the sign convention in the lens formula
Distances against the incident light are negative; apply the convention consistently.
WATCH OUT
Using focal length in cm for power
Power needs f in metres: P = 1/f.
WATCH OUT
Swapping the corrections for myopia and hypermetropia
Myopia → concave lens; hypermetropia → convex lens.

Practice problems

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

Q1EASY· Concept
Define the refractive index of a medium.
Show solution
The ratio of the speed of light in vacuum to its speed in the medium, n = c/v.
Q2EASY· Numerical
Light travels at 2×10⁸ m s⁻¹ in glass. Find its refractive index (c = 3×10⁸).
Show solution
n = c/v = 3×10⁸/2×10⁸ = 1.5.
Q3MEDIUM· Numerical
A convex lens has focal length 20 cm. Find its power.
Show solution
P = 1/f = 1/0.20 = +5 D.
Q4MEDIUM· Numerical
The critical angle of a medium is 30°. Find its refractive index.
Show solution
n = 1/sin C = 1/sin30° = 1/0.5 = 2.
Q5MEDIUM· Concept
What is total internal reflection? State its conditions and two applications.
Show solution
Complete reflection at a denser–rarer boundary when i > C. Conditions: ray from denser to rarer medium and i > critical angle. Applications: optical fibres, mirage (also diamond's brilliance).
Q6HARD· Application
Name the two common defects of vision and their corrections.
Show solution
Myopia (short sight) — image before retina, corrected by a concave lens; Hypermetropia (long sight) — image behind retina, corrected by a convex lens.

5-minute revision

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

  • Physics Chapter 2 of Samacheer Kalvi Class 10 Science.
  • Snell's law: sin i/sin r = n; n = c/v.
  • Denser medium → light bends towards the normal.
  • TIR: denser→rarer and i > C; n = 1/sin C.
  • Lens: 1/v − 1/u = 1/f; m = v/u; P = 1/f (dioptre).
  • Myopia → concave lens; hypermetropia → convex lens.

Tamil Nadu (TNBSE) marks blueprint

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

Typical chapter weightage: 5-9 marks across MCQ, short answer and numerical/diagram questions

Question typeMarks eachTypical countWhat it tests
MCQ11-2Definitions and refractive index
Short Answer2-31-2TIR, eye defects, ray diagrams
Numerical2-31n, power of lens, lens formula
Prep strategy
  • Learn Snell's law and n = c/v
  • Practise power and lens-formula numericals
  • Memorise TIR conditions and applications
  • Draw ray diagrams for myopia and hypermetropia

Where this shows up in the real world

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

Spectacles and contact lenses

Correcting myopia and hypermetropia uses concave and convex lenses.

Optical fibre communication

Total internal reflection guides light signals over long distances.

Cameras and microscopes

Convex lenses form the images used in imaging instruments.

Exam strategy

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

  1. Write Snell's law / lens formula before substituting
  2. Convert focal length to metres for power
  3. Label ray diagrams neatly for full marks
  4. State TIR conditions precisely

Going beyond the textbook

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

  • Derive the relation n = 1/sin C for the critical angle.
  • Trace the path of light through a glass slab and mark the lateral shift.

Where else this chapter is tested

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

TN SSLC Class 10 Public ExamHigh
Foundation / NTSE PhysicsMedium
School unit testsHigh

Questions students ask

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

Diamond has a very high refractive index and small critical angle, so light entering it undergoes repeated total internal reflection before emerging, producing its sparkle.

The dioptre (D), where power P = 1/f with the focal length f measured in metres. Convex lenses have positive power, concave lenses negative.
Verified by the tuition.in editorial team
Last reviewed on 2 June 2026. Written and reviewed by subject-matter experts — read about our process.
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