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Light – Reflection and Refraction – Class 10 Science Chapter 9 Notes & NCERT PDF

Class 10ScienceChapter 9NCERT book: Science - Class 10

Notes and a simple summary of Chapter 9 of the NCERT Class 10 Science book, with the official chapter PDF, flashcards, an MCQ quiz and an AI tutor for your doubts.

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Chapter 9: Light – Reflection and Refraction

Introduction

We see an object when light reflected from it reaches our eyes. A small source of light casts a sharp shadow of an opaque object, which shows that light travels in a straight line — a ray of light. (The book notes that when an obstacle is very small, light bends around it — diffraction — and that modern quantum theory treats light as neither purely a wave nor a particle.) In this chapter we use the straight-line (ray) model to study reflection by spherical mirrors and refraction by glass slabs and lenses.

Key Concepts

1. Laws of Reflection

(i) The angle of incidence is equal to the angle of reflection.
(ii) The incident ray, the normal at the point of incidence and the reflected ray all lie in the same plane.

These laws hold for all reflecting surfaces, including curved ones. A plane mirror gives an image that is virtual, erect, the same size as the object, as far behind the mirror as the object is in front, and laterally inverted.

2. Spherical Mirrors — the vocabulary

  • Concave mirror – reflecting surface curved inwards (faces the centre of the sphere). Converges light.
  • Convex mirror – reflecting surface curved outwards. Diverges light.
  • Pole (P) – centre of the reflecting surface.
  • Centre of curvature (C) – centre of the sphere of which the mirror is a part. It is not on the mirror; it is in front of a concave mirror and behind a convex mirror.
  • Radius of curvature (R) – distance PC.
  • Principal axis – line through P and C; it is normal to the mirror at P.
  • Principal focus (F) – point where rays parallel to the axis meet (concave) or appear to diverge from (convex) after reflection.
  • Focal length (f) – distance PF.
  • Aperture – diameter of the reflecting surface.
  • For mirrors of small aperture, R = 2f — so F lies midway between P and C.

    In Activity 9.2, a concave mirror focuses sunlight into a bright spot that can burn paper; that spot is a real image of the Sun, and its distance from the mirror gives the approximate focal length.

    3. Rules for Ray Diagrams (mirrors)

    Use any two of these:

  • A ray parallel to the principal axis passes through F after reflection (concave), or appears to come from F (convex).
  • A ray through F (concave) or directed towards F (convex) emerges parallel to the principal axis.
  • A ray through C (concave) or directed towards C (convex) is reflected back along the same path — it falls along the normal.
  • A ray striking the pole obliquely is reflected obliquely, making equal angles with the principal axis.
  • 4. Image Formation by a Concave Mirror (Table 9.1)

  • Object at infinity → image at F; highly diminished, point-sized; real and inverted.
  • Object beyond C → image between F and C; diminished; real and inverted.
  • Object at C → image at C; same size; real and inverted.
  • Object between C and F → image beyond C; enlarged; real and inverted.
  • Object at F → image at infinity; highly enlarged; real and inverted.
  • Object between P and F → image behind the mirror; enlarged; virtual and erect.
  • Uses of concave mirrors: torches, search-lights and vehicle headlights (powerful parallel beams); shaving mirrors; dentists' mirrors (large image of teeth); solar furnaces.

    5. Image Formation by a Convex Mirror (Table 9.2)

  • Object at infinity → image at F behind the mirror; highly diminished, point-sized; virtual and erect.
  • Object anywhere between infinity and P → image between P and F behind the mirror; diminished; virtual and erect.
  • Uses of convex mirrors: rear-view (wing) mirrors in vehicles — they always give an erect, diminished image and have a wider field of view. The book mentions a convex mirror in a wall of Agra Fort that shows the full image of the Taj Mahal.

    6. New Cartesian Sign Convention

  • The pole P (or the optical centre O of a lens) is the origin; the principal axis is the x-axis.
  • The object is always placed to the left, so light falls from the left.
  • Distances to the right of the origin are positive; to the left, negative.
  • Heights above the axis are positive; below, negative.
  • Consequences: for a real object u is always negative; f of a concave mirror is negative, f of a convex mirror is positive.

    7. Mirror Formula and Magnification

    Mirror formula: 1/v + 1/u = 1/f
    Magnification: m = h′/h = −v/u

    A negative m means the image is real and inverted; a positive m means virtual and erect.

    8. Refraction of Light

    Refraction is the change in direction of light when it passes obliquely from one transparent medium to another, because the speed of light changes. Everyday signs: a pencil in water looks bent, a pond looks shallower, letters under a glass slab look raised, a lemon in a glass of water looks bigger. In Activity 9.8 a coin that had just disappeared from view becomes visible again when water is poured into the bowl.

    Glass slab (Activity 9.10): at the air→glass face the ray bends towards the normal; at the glass→air face it bends away. The emergent ray is parallel to the incident ray but laterally displaced, because the bending at the two parallel faces is equal and opposite. A ray falling normally passes straight through.

    Laws of refraction
    (i) The incident ray, the refracted ray and the normal at the point of incidence lie in the same plane.
    (ii) Snell's law: sin i / sin r = constant, for light of a given colour and a given pair of media.

    9. Refractive Index

  • n₂₁ = v₁/v₂ (speed in medium 1 ÷ speed in medium 2); n₁₂ = v₂/v₁.
  • Absolute refractive index: n = c/v, where c = 3 × 10⁸ m s⁻¹.
  • Values from Table 9.3 (no need to memorise): air 1.0003, ice 1.31, water 1.33, alcohol 1.36, kerosene 1.44, crown glass 1.52, diamond 2.42 (the highest in the table).
  • Optical density ≠ mass density. Kerosene (1.44) is optically denser than water (1.33) though it is lighter. Light slows down and bends towards the normal going into an optically denser medium.
  • 10. Spherical Lenses

  • Convex (double convex) lens – thicker in the middle; converging.
  • Concave (double concave) lens – thicker at the edges; diverging.
  • Optical centre (O) – a ray through it passes undeviated.
  • A lens has two centres of curvature (C₁, C₂) and two principal foci (F₁, F₂).
  • Ray rules for lenses: (i) a ray parallel to the axis passes through F₂ after refraction (convex) or appears to diverge from F₁ (concave); (ii) a ray through F₁ (convex), or heading towards F (concave), emerges parallel to the axis; (iii) a ray through O goes straight on.

    11. Image Formation by a Convex Lens (Table 9.4)

  • Object at infinity → image at F₂; point-sized; real and inverted.
  • Object beyond 2F₁ → image between F₂ and 2F₂; diminished; real and inverted.
  • Object at 2F₁ → image at 2F₂; same size; real and inverted.
  • Object between F₁ and 2F₁ → image beyond 2F₂; enlarged; real and inverted.
  • Object at F₁ → image at infinity; highly enlarged; real and inverted.
  • Object between F₁ and O → image on the same side as the object; enlarged; virtual and erect (magnifying glass).
  • Concave lens (Table 9.5): always gives a virtual, erect, diminished image between F₁ and O (at F₁ when the object is at infinity).

    12. Lens Formula, Magnification and Power

    Lens formula: 1/v − 1/u = 1/f
    Magnification: m = h′/h = v/u
    Power: P = 1/f (f in metres); unit dioptre (D), 1 D = 1 m⁻¹

    Convex lens → f and P positive; concave lens → f and P negative. Lenses in contact: P = P₁ + P₂ + P₃ + … (e.g. +2.0 D and +0.25 D give +2.25 D).

    Worked Numericals

    1. Rear-view mirror (Example 9.1). Convex mirror, R = +3.00 m, bus at u = −5.00 m.

    f = R/2 = +1.50 m. 1/v = 1/f − 1/u = 1/1.50 + 1/5.00 = 6.50/7.50 → v ≈ +1.15 m (behind the mirror).

    m = −v/u = −(1.15)/(−5.00) ≈ +0.23 → virtual, erect, diminished.

    2. Concave mirror on a screen (Example 9.2). h = 4.0 cm, u = −25.0 cm, f = −15.0 cm.

    1/v = 1/f − 1/u = −1/15 + 1/25 = −2/75 → v = −37.5 cm (screen 37.5 cm in front).

    m = −v/u = −1.5, h′ = −6.0 cm → real, inverted, enlarged.

    3. Exercise 15. h = 7.0 cm, u = −27 cm, concave f = −18 cm.

    1/v = −1/18 + 1/27 = −1/54 → v = −54 cm; m = −(−54)/(−27) = −2; h′ = −14 cm (real, inverted, twice as large).

    4. Convex lens (Example 9.4). h = 2.0 cm, f = +10 cm, u = −15 cm.

    1/v = 1/f + 1/u = 1/10 − 1/15 = 1/30 → v = +30 cm; m = v/u = −2; h′ = −4.0 cm → real, inverted, enlarged.

    5. Concave lens (Example 9.3). f = −15 cm, v = −10 cm.

    1/u = 1/v − 1/f = −1/10 + 1/15 = −1/30 → u = −30 cm; m = v/u = +1/3 → virtual, erect, one-third size.

    6. Speed and power. In glass of n = 1.50, v = c/n = 3 × 10⁸ / 1.50 = 2 × 10⁸ m s⁻¹. A lens of −2.0 D has f = −0.50 m (concave); +1.5 D has f ≈ +0.67 m (convex).

    Formula Sheet

  • R = 2f
  • Mirror: 1/v + 1/u = 1/f; m = −v/u
  • Lens: 1/v − 1/u = 1/f; m = v/u
  • m = h′/h
  • n = c/v; n₂₁ = v₁/v₂; Snell: sin i/sin r = constant
  • P = 1/f (m); P = P₁ + P₂ + …
  • Board Exam Focus

  • Ray diagrams for all six concave-mirror and convex-lens positions (use two rules each).
  • Sign-convention numericals — always write the signs of u, f and h before substituting.
  • Reasoning questions: why convex mirrors for rear-view, why concave mirrors in headlights, why the emergent ray from a slab is parallel.
  • Half of a lens covered with black paper still forms a complete image, only dimmer (Exercise 9).
  • Key Terms

  • Reflection (परावर्तन), Refraction (अपवर्तन)
  • Concave mirror (अवतल दर्पण), Convex mirror (उत्तल दर्पण)
  • Pole (ध्रुव), Centre of curvature (वक्रता केंद्र), Principal focus (मुख्य फोकस)
  • Focal length (फोकस दूरी), Aperture (द्वारक)
  • Real image (वास्तविक प्रतिबिंब), Virtual image (आभासी प्रतिबिंब)
  • Magnification (आवर्धन), Refractive index (अपवर्तनांक)
  • Optical centre (प्रकाशिक केंद्र), Power of a lens (लेंस की क्षमता), Dioptre (डाइऑप्टर)
  • Common Mistakes

  • Forgetting that u is negative for a real object, or taking f of a concave mirror as positive.
  • Using −v/u for lenses (it is +v/u for lenses, −v/u for mirrors).
  • Mixing the formulas: mirror has + (1/v + 1/u), lens has − (1/v − 1/u).
  • Using f in cm in P = 1/f — f must be in metres.
  • Thinking a higher mass density means a higher refractive index (kerosene vs water).
  • Saying a concave lens can form a real image of a real object — it never does.
  • 💡 Key Learning Points

    • ✓State and apply the two laws of reflection and the two laws of refraction (including Snell's law, sin i / sin r = constant).
    • ✓Describe the position, size and nature of images formed by concave/convex mirrors and convex/concave lenses for every object position.
    • ✓Use the New Cartesian Sign Convention with the mirror formula (1/v + 1/u = 1/f) and lens formula (1/v − 1/u = 1/f) to solve numericals.
    • ✓Interpret magnification (m = −v/u for mirrors, m = v/u for lenses): negative m means real and inverted, positive m means virtual and erect.
    • ✓Relate refractive index to the speed of light (n = c/v), and define power of a lens (P = 1/f, in dioptres) with its sign.

    👨‍🏫 Teaching Tips

    • →Start with Activity 9.1 — let students look into both sides of a steel spoon to discover concave and convex mirrors before naming them.
    • →Mark P, F and C with chalk lines (Activity 9.3) and move a candle through each position so students fill in Table 9.1 themselves.
    • →Drill the four ray rules with a 'choose any two' routine; have pairs draw and swap diagrams to check each other.
    • →Before any numerical, make students write a sign line: u = −, f (concave) = −, f (convex) = +, h = + — this prevents most errors.
    • →Do Activity 9.8 (coin in bowl) as a quick demo of refraction; ask students to explain using 'light bends away from the normal'.
    • →Use Table 9.3 to challenge the misconception that denser liquids always bend light more (kerosene vs water).
    • →Cover half a lens with black paper during a demo to show the image is complete but dimmer (Exercise 9).
    • →Link power of lenses to spectacle prescriptions students or family members have — it previews Chapter 10.

    📋 Assessment Questions

    1. Can the student draw correct ray diagrams for a concave mirror with the object beyond C, at C, between C and F, and between P and F?
    2. Can the student solve a mirror or lens numerical with correct signs and state the nature and size of the image?
    3. Can the student explain why convex mirrors are used as rear-view mirrors and concave mirrors in headlights?
    4. Can the student calculate the speed of light in a medium from its refractive index and interpret 'refractive index of diamond is 2.42'?
    5. Can the student convert between power and focal length and identify the lens type from the sign?

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