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CBSE Class 10 Science Light Reflection and Refraction Notes

How These Notes Will Help You

 

Light — Reflection and Refraction is one of the most calculation-intensive chapters in CBSE Class 10 Science, and it is also one of the most reliably high-scoring ones for students who prepare it well. The chapter combines conceptual understanding (how and why light behaves the way it does at different surfaces) with numerical problem-solving (mirror formula, lens formula, magnification, power of lenses). Many students find the sign convention confusing, or get mirror and lens image positions mixed up — and these are exactly the kinds of errors that cost marks in board exams. These notes are specifically designed to prevent those mistakes.

 

Every formula in this chapter is presented with both a derivation of its meaning and a worked numerical so you can see exactly how it is applied. The sign convention (New Cartesian System) is explained once, clearly, and then applied consistently throughout every formula and every worked example — so you never have to guess which direction is positive or negative. The image formation tables for concave mirrors, convex mirrors, convex lenses, and concave lenses cover every possible object position, giving you a complete reference for diagram questions and for questions that ask 'describe the image formed when...'. These tables are built directly from the NCERT syllabus and CBSE exam patterns.

 

What You Get in These Notes

✅  New Cartesian Sign Convention explained once, clearly — applied consistently throughout every formula

✅  Complete image formation tables for all 4 optical devices — covers every object position tested in board exams

✅  Mirror formula and lens formula both derived from meaning, then applied in fully worked numericals

✅  Magnification formula for both mirrors and lenses — with sign interpretation (erect vs inverted)

✅  Power of a lens — definition, formula, unit, and combination of lenses formula with worked examples

✅  Refraction — Snell's Law, refractive index, glass slab, total internal reflection explained with clarity

✅  Complete comparison tables: concave vs convex mirror, convex vs concave lens, mirror vs lens formula

✅  Common mistakes section, key definitions summary, and practice questions (1M / 3M / 5M) with numericals

 

Who are these notes for? These notes are written for CBSE Class 10 students who want to master the numerical and conceptual aspects of this chapter. They are particularly useful for students who understand the ray diagrams but lose marks on formula-based questions due to sign convention errors, and for students who find it difficult to remember which image is formed at which object position. The notes are equally useful as a first-read and as a revision reference.

 

How to use these notes: Read the sign convention section first and ensure it is clear before moving to formulas. For each worked numerical, cover the solution and attempt it yourself before checking. After reading the image formation tables, test yourself by closing the table and drawing a ray diagram for a random object position — this is the most effective revision method for this chapter.

 


FutureTopper offers free CBSE Class 10 Math and Science question banks, 2026–27. Blue-yellow theme with icons and bold text. Limited time offer.

1. Introduction — What is Light?

 

Light is a form of electromagnetic radiation that is visible to the human eye. It travels in straight lines (called rays) in a uniform medium, at a speed of approximately 3 × 10⁸ m/s in vacuum — the fastest speed possible in the universe. Light does not need a medium to travel; it can propagate through vacuum, unlike sound. When light travels from one medium to another, or encounters a surface, its behaviour changes — and the two most important behaviours are reflection (bouncing off a surface) and refraction (bending as it passes from one medium to another).

 

Key Topics in This Chapter

• Reflection of Light — laws of reflection, plane mirror, spherical mirrors

• Concave Mirror — image formation at all object positions, uses

• Convex Mirror — image formation, uses

• Mirror Formula and Magnification — numericals

• Refraction of Light — laws of refraction, Snell's Law, refractive index

• Refraction through glass slab — lateral displacement

• Lenses — convex (converging) and concave (diverging) lenses

• Convex Lens — image formation at all object positions

• Concave Lens — image formation

• Lens Formula, Magnification, and Power of a Lens — numericals

 

2. Reflection of Light

 

Reflection is the phenomenon in which light bouncing off a surface returns to the original medium. It occurs at all surfaces — polished, rough, transparent, or opaque — but the type of reflection depends on the surface. Smooth, polished surfaces (like mirrors) produce regular (specular) reflection where parallel rays remain parallel after reflection. Rough surfaces produce diffuse (irregular) reflection where parallel rays scatter in all directions — this is actually how we see most objects.

 

2.1 Laws of Reflection

 

The laws of reflection are universal — they apply to every reflecting surface, whether plane, concave, or convex, and whether the surface is a mirror, water, or polished metal.

 

LAW 1:  The angle of incidence = The angle of reflection

        ∠i  =  ∠r

        (both angles measured from the NORMAL to the surface at the point of incidence)

 

LAW 2:  The incident ray, the reflected ray, and the normal to the surface

        at the point of incidence all lie in the SAME PLANE.

 

Normal = line perpendicular to the reflecting surface at the point where light strikes.

 

2.2 Plane Mirror — Image Characteristics

 

A plane mirror is a flat, smooth reflective surface. The image formed by a plane mirror is one of the simplest to understand and forms the baseline for understanding spherical mirror images.

 

Plane Mirror — Image Properties (Memorise All 6)

1. Virtual — image cannot be obtained on a screen; formed behind the mirror

2. Erect — right-side up (same orientation as the object)

3. Laterally inverted — left and right are swapped (left hand appears as right hand)

4. Same size as object — magnification = +1

5. As far behind the mirror as the object is in front

6. Image distance = Object distance  (|v| = |u|)

 

3. Spherical Mirrors

 

A spherical mirror is a mirror whose reflecting surface is part of a hollow sphere. The two types — concave (reflecting surface on the inner curved side) and convex (reflecting surface on the outer curved side) — behave very differently and are used for different purposes.

 

3.1 Key Terms and Definitions

 

Term

Symbol

Definition

Centre of Curvature

C

Centre of the sphere of which the mirror is a part. Located in front of concave mirror, behind convex mirror.

Radius of Curvature

R

Radius of sphere of which mirror is part. R = 2f (twice the focal length).

Pole

P

Midpoint / geometric centre of the reflecting surface of the mirror.

Principal Axis

Imaginary straight line passing through C, F, and P — the axis of symmetry.

Focus (Principal Focus)

F

Point where all rays parallel to principal axis converge (concave) or appear to diverge from (convex) after reflection.

Focal Length

f

Distance from Pole (P) to Focus (F) along the principal axis. f = R/2.

Aperture

Diameter of the reflecting surface. Larger aperture = more light collected.

 

Key relationship:  R  =  2f   →   f  =  R / 2

 

For CONCAVE mirror:  f is NEGATIVE (focus in front of mirror — same side as object)

For CONVEX mirror:   f is POSITIVE (focus behind mirror — opposite side to object)

(Using New Cartesian Sign Convention — see Section 3.2)

 

3.2 New Cartesian Sign Convention

 

The New Cartesian Sign Convention is essential for using the mirror formula and lens formula correctly. Every sign error in a numerical comes from not applying this convention carefully. Learn it once, apply it everywhere.

 

New Cartesian Sign Convention — The Complete Rules

1. All distances are measured from the POLE (P) of the mirror (or optical centre of lens).

2. Distances measured in the DIRECTION OF INCIDENT LIGHT are POSITIVE (+).

3. Distances measured AGAINST the direction of incident light are NEGATIVE (−).

4. Heights measured UPWARD from the principal axis are POSITIVE (+).

5. Heights measured DOWNWARD from the principal axis are NEGATIVE (−).

 

Incident light travels LEFT TO RIGHT (standard convention):

  → Objects are placed to the LEFT of the mirror → object distance u is always NEGATIVE

  → For CONCAVE mirror: f is NEGATIVE, R is NEGATIVE

  → For CONVEX mirror: f is POSITIVE, R is POSITIVE

 

MEMORY AID: Object is ALWAYS to the left → u is ALWAYS negative for mirrors.

 

3.3 Rules for Drawing Ray Diagrams (Spherical Mirrors)

 

Only two of the three rules are needed to locate an image. Always choose the two that are easiest to draw for the given object position.

 

Rule

Incident Ray

Reflected Ray

Rule 1

Parallel to the principal axis

Passes through F (concave) or appears to come from F (convex)

Rule 2

Passes through F (concave) or directed toward F (convex)

Emerges parallel to the principal axis

Rule 3

Passes through C (or directed toward C for convex)

Retraces its path back through C (reflects along same line)

 

3.4 Image Formation by Concave Mirror

 

The position and nature of the image formed by a concave mirror depends entirely on where the object is placed relative to F and C. This table is one of the most frequently tested items in CBSE board exams — in diagram questions and in 'describe the image' questions.

 

Object Position

Image Position

Image Size

Image Nature

Uses

At infinity (∞)

At F (focal point)

Highly diminished (point image)

Real, Inverted

Reflecting telescopes, solar furnaces

Beyond C (beyond 2f)

Between F and C

Diminished (smaller than object)

Real, Inverted

Used in rear-view mirrors — NO; this is concave.

At C (at 2f)

At C (at 2f)

Same size as object

Real, Inverted

Used in ERG machines (medical)

Between C and F

Beyond C (beyond 2f)

Enlarged (magnified)

Real, Inverted

Projectors, headlights (object at F gives parallel beam)

At F

At infinity (∞)

Highly enlarged

Real, Inverted

Searchlights, vehicle headlights (parallel beam produced)

Between F and P

Behind the mirror

Enlarged (magnified)

Virtual, Erect

Shaving/make-up mirrors, dental mirrors (magnified upright image)

 

Concave Mirror — Key Facts for Board Exam

• Only when object is BETWEEN F and P does concave mirror give a VIRTUAL, ERECT image.

• All other positions give REAL, INVERTED images.

• As object moves from infinity toward mirror, image moves from F toward infinity (then virtual).

• At F: image at infinity → parallel beam of light produced (used in searchlights, headlights).

• Uses: Shaving mirror, dental mirror, solar furnace, reflector in torches/headlights.

 

3.5 Image Formation by Convex Mirror

 

A convex mirror always forms a virtual, erect, and diminished image — regardless of where the object is placed. This is because parallel rays, after reflecting from a convex mirror, diverge and never actually meet. Only two object positions are typically asked about in CBSE.

 

Object Position

Image Position

Image Size

Image Nature

At infinity (∞)

At F (behind mirror)

Highly diminished (point image)

Virtual, Erect

Anywhere between infinity and P

Between F and P (behind mirror)

Diminished (smaller than object)

Virtual, Erect

 

Convex Mirror — Why Used as Rear-View Mirror in Vehicles

1. Always gives ERECT (right-side up) image — driver sees correctly oriented view.

2. Always gives DIMINISHED image — wider field of view (see more of the road behind).

3. Always VIRTUAL — driver knows image is behind the mirror; no confusion about distance.

 

Limitation: Objects appear further away than they are (because image is diminished).

That is why rear-view mirrors say: 'Objects in mirror are closer than they appear.'

 

3.6 Mirror Formula and Magnification

 

The mirror formula relates the object distance, image distance, and focal length of a spherical mirror. It applies to both concave and convex mirrors, provided the New Cartesian Sign Convention is applied consistently.

 

MIRROR FORMULA:

 

  1/v  +  1/u  =  1/f

 

where:

  v = image distance (measured from pole P)

  u = object distance (measured from pole P)  [always negative for real objects]

  f = focal length  [negative for concave, positive for convex mirror]

 

Also:  f  =  R / 2  →  R  =  2f

 

MAGNIFICATION (m):

 

  m  =  Height of Image (h')  /  Height of Object (h)  =  −v / u

 

  m > 0 (positive):  Image is ERECT (same side up as object)

  m < 0 (negative):  Image is INVERTED

  |m| > 1:           Image is ENLARGED (magnified)

  |m| < 1:           Image is DIMINISHED (smaller than object)

  |m| = 1:           Image is SAME SIZE as object

 

Worked Numerical 3.1 — Concave Mirror

Problem: An object is placed 20 cm in front of a concave mirror of focal length 15 cm.

Find: (a) image distance (b) magnification (c) nature of image.

 

Given: u = −20 cm (object in front of mirror, negative by sign convention)

       f = −15 cm (concave mirror, negative by sign convention)

 

Using mirror formula:  1/v + 1/u = 1/f

  1/v + 1/(−20) = 1/(−15)

  1/v = 1/(−15) − 1/(−20) = −1/15 + 1/20

  1/v = (−4 + 3)/60 = −1/60

  v = −60 cm

 

Image is 60 cm in front of the mirror (v is negative → real image, same side as object).

 

Magnification: m = −v/u = −(−60)/(−20) = −3

 

Interpretation: m = −3 → Image is INVERTED (negative) and MAGNIFIED by 3× (|m| = 3 > 1).

Nature of image: REAL, INVERTED, ENLARGED (3 times the object size).

 

Worked Numerical 3.2 — Convex Mirror

Problem: An object 6 cm tall is placed 30 cm in front of a convex mirror with R = 40 cm.

Find: image distance, image height, and describe the image.

 

Given: u = −30 cm  (object in front of mirror, negative)

       R = +40 cm  (convex mirror, positive) → f = R/2 = +20 cm

       h = +6 cm   (object is upright, positive)

 

Mirror formula:  1/v = 1/f − 1/u = 1/20 − 1/(−30) = 1/20 + 1/30

  1/v = (3 + 2)/60 = 5/60 = 1/12

  v = +12 cm  (positive → image is behind the mirror → virtual image)

 

Magnification: m = −v/u = −(12)/(−30) = +0.4

Image height: h' = m × h = 0.4 × 6 = +2.4 cm

 

Image is VIRTUAL (behind mirror), ERECT (m positive), DIMINISHED (|m| < 1).

Image height = 2.4 cm (smaller than 6 cm object).

 

4. Refraction of Light

 

Refraction is the bending of light as it passes from one transparent medium to another. It occurs because light travels at different speeds in different media — the denser the medium, the slower light travels in it. When light enters a denser medium (e.g., from air to glass), it slows down and bends toward the normal. When it enters a less dense medium (e.g., from glass to air), it speeds up and bends away from the normal.

 

Refraction is responsible for a wide range of everyday phenomena — the apparent bending of a straw in a glass of water, the twinkling of stars, the formation of a rainbow, the operation of a lens in glasses or a camera, and the working of optical fibres in telecommunications.

 

4.1 Laws of Refraction (Snell's Law)

 

LAW 1:  The incident ray, the refracted ray, and the normal to the interface

        at the point of incidence all lie in the SAME PLANE.

 

LAW 2 (SNELL'S LAW):  The ratio of the sine of the angle of incidence

        to the sine of the angle of refraction is a constant for a given

        pair of media and a given colour of light:

 

        sin i / sin r  =  n₂₁  =  n₂ / n₁  =  constant

 

where:  i  = angle of incidence (in medium 1)

        r  = angle of refraction (in medium 2)

        n₁ = refractive index of medium 1

        n₂ = refractive index of medium 2

        n₂₁ = refractive index of medium 2 with respect to medium 1

 

4.2 Refractive Index

 

Definition: The refractive index of a medium is a dimensionless number that describes how much slower light travels in that medium compared to its speed in vacuum. A higher refractive index means light travels more slowly in that medium and bends more toward the normal when entering it.

 

Absolute Refractive Index (n) of a medium:

 

  n  =  Speed of light in vacuum (c)  /  Speed of light in medium (v)

  n  =  c / v

  n  =  3 × 10⁸ m/s  /  v

 

Snell's Law (extended form):

  n₁ × sin i  =  n₂ × sin r

  (This form makes calculations easier — use this version in numericals)

 

Also: n₂₁  =  n₂ / n₁  =  v₁ / v₂  =  λ₁ / λ₂

(speed in medium 1 / speed in medium 2 = refractive index of 2 w.r.t. 1)

 

Medium

Refractive Index (n)

Speed of Light (approx.)

Vacuum

1.000 (exact, by definition)

3.00 × 10⁸ m/s

Air

1.0003 (≈ 1.00 for calculations)

≈ 3.00 × 10⁸ m/s

Water

1.33

2.25 × 10⁸ m/s

Glass (crown)

1.50

2.00 × 10⁸ m/s

Glass (flint)

1.70

1.76 × 10⁸ m/s

Diamond

2.42

1.24 × 10⁸ m/s

 

4.3 Refraction through a Glass Slab — Lateral Displacement

 

When light passes through a glass slab with parallel surfaces, it undergoes refraction at entry (bends toward normal) and again at exit (bends away from normal). Because the surfaces are parallel, the angle of emergence equals the angle of incidence — the emergent ray is parallel to the incident ray but shifted sideways. This perpendicular shift is called lateral displacement.

 

Key Points — Refraction Through Glass Slab

• At entry (air → glass): ray bends TOWARD normal (denser medium, slower speed).

• At exit (glass → air): ray bends AWAY from normal (less dense medium, faster speed).

• Emergent ray is PARALLEL to incident ray (both surfaces are parallel).

• Lateral displacement: the perpendicular distance between incident and emergent rays.

• Lateral displacement INCREASES with: thicker slab, higher refractive index, larger angle of incidence.

• Net deviation of direction = 0° (parallel in, parallel out — just shifted sideways).

 

5. Lenses — Refraction Through Curved Surfaces

 

A lens is a transparent optical device with two curved surfaces (or one curved and one flat) that refracts light. The two main types are the convex (converging) lens, which is thicker at the centre than at the edges, and the concave (diverging) lens, which is thinner at the centre than at the edges. Lenses are used in cameras, microscopes, telescopes, spectacles, magnifying glasses, and projectors.

 

5.1 Key Terms for Lenses

 

Term

Definition

Optical Centre (O)

The central point of the lens. Rays passing through O pass straight through without bending.

Principal Axis

Imaginary line passing through both centres of curvature and the optical centre.

Principal Focus (F)

For convex lens: point where parallel rays converge after refraction. For concave lens: point from which parallel rays appear to diverge after refraction.

Focal Length (f)

Distance from Optical Centre (O) to Principal Focus (F). Positive for convex, negative for concave (by sign convention).

Focal Plane

Plane perpendicular to principal axis passing through F. Objects at infinity form images in the focal plane.

Radius of Curvature

Radius of the sphere of which each lens surface is a part. R = 2f for thin lenses (approx.).

 

5.2 Sign Convention for Lenses

 

The same New Cartesian Sign Convention applies to lenses, but with the optical centre (O) as the reference point (instead of the pole for mirrors).

 

Sign Convention for Lenses:

 

  Object is always to the LEFT of lens  →  u is always NEGATIVE

 

  CONVEX (converging) lens:

    f is POSITIVE (focus on the right — transmission side, same as emergent light)

    Real images form on the RIGHT → v is POSITIVE for real images

    Virtual images form on the LEFT → v is NEGATIVE for virtual images

 

  CONCAVE (diverging) lens:

    f is NEGATIVE (focus on the left — same side as object)

    Images always virtual, on same side as object → v is always NEGATIVE

 

5.3 Rules for Drawing Ray Diagrams Through Lenses

 

Rule

Incident Ray

Refracted Ray

Rule 1

Parallel to the principal axis

Passes through F₂ (far focus) for convex; appears to come from F₁ (near focus) for concave

Rule 2

Passes through F₁ (near focus) for convex; directed toward F₂ for concave

Emerges parallel to the principal axis

Rule 3

Passes through Optical Centre (O)

Passes through without any bending (straight line)

 

5.4 Image Formation by Convex Lens

 

Object Position

Image Position

Image Size

Nature

Uses

At infinity (∞)

At F₂ (focal point)

Highly diminished

Real, Inverted

Telescope objective lens

Beyond 2F₁ (beyond 2f)

Between F₂ and 2F₂

Diminished

Real, Inverted

Camera lens (object far, image small on film)

At 2F₁ (at 2f)

At 2F₂ (at 2f)

Same size as object

Real, Inverted

Photocopier at 100% scale

Between F₁ and 2F₁

Beyond 2F₂

Enlarged

Real, Inverted

Film projector (slide/movie projector)

At F₁ (focal point)

At infinity (∞)

Highly enlarged

Real, Inverted

Searchlight / parallel beam production

Between F₁ and O

Same side as object (left of lens)

Enlarged

Virtual, Erect

Magnifying glass, reading lens

 

Convex Lens — Key Pattern

• Object BETWEEN F and O → Virtual, Erect, Enlarged (magnifying glass).

• All other positions → Real, Inverted images.

• At F: image at infinity (parallel beam). Beyond 2F: diminished. At 2F: same size. Between F and 2F: enlarged.

• SAME pattern as concave mirror — if you know one, you know the other.

 

5.5 Image Formation by Concave Lens

 

A concave (diverging) lens always forms a virtual, erect, and diminished image — regardless of object position. This is because diverging lenses cause parallel rays to spread out, and the diverged rays never actually meet — they only appear to diverge from a point on the same side as the object.

 

Object Position

Image Position

Image Size

Nature

At infinity (∞)

At F₁ (same side as object)

Highly diminished (point image)

Virtual, Erect

Anywhere between infinity and O

Between F₁ and O (same side as object)

Diminished

Virtual, Erect

 

Concave Lens vs Convex Mirror — A Useful Parallel

Both concave lenses and convex mirrors ALWAYS produce:

  → Virtual, Erect, Diminished images

  → Images that are between F and the surface/optical centre

 

The key difference: convex mirror REFLECTS light; concave lens REFRACTS light.

Both are used where a wide field of view / smaller representation is needed.

 

5.6 Lens Formula and Magnification

 

LENS FORMULA:

 

  1/v  −  1/u  =  1/f

 

NOTE: Lens formula uses (1/v − 1/u) NOT (1/v + 1/u) like mirror formula.

This is the most common mix-up — memorise the difference.

 

where:

  v = image distance from optical centre O

  u = object distance from optical centre O  [always negative]

  f = focal length  [positive for convex, negative for concave]

 

MAGNIFICATION (m) for Lens:

 

  m  =  h' / h  =  v / u

 

NOTE: For lens, m = v/u (NOT −v/u as for mirrors).

  m > 0: Image is ERECT   |   m < 0: Image is INVERTED

  |m| > 1: Enlarged       |   |m| < 1: Diminished

 

Mirror Formula vs Lens Formula — Critical Difference

MIRROR:  1/v  +  1/u  =  1/f     and    m  =  −v/u

LENS:    1/v  −  1/u  =  1/f     and    m  =   v/u

 

The LENS formula has a MINUS sign between 1/v and 1/u.

The MIRROR magnification has a NEGATIVE sign: m = −v/u.

The LENS magnification has NO negative sign: m = v/u.

 

These two differences cause the majority of formula errors in board exams.

 

Worked Numerical 5.1 — Convex Lens (Magnifying Glass)

Problem: An object is placed 10 cm from a convex lens of focal length 15 cm.

Find image distance, magnification, and describe the image.

 

Given: u = −10 cm (object to left of lens, negative)

       f = +15 cm (convex lens, positive)

 

Lens formula:  1/v − 1/u = 1/f

  1/v − 1/(−10) = 1/15

  1/v + 1/10 = 1/15

  1/v = 1/15 − 1/10 = (2 − 3)/30 = −1/30

  v = −30 cm  (negative → image on same side as object → VIRTUAL)

 

Magnification: m = v/u = (−30)/(−10) = +3

 

Image is VIRTUAL (v negative), ERECT (m positive), ENLARGED by 3× (|m| = 3 > 1).

This is the magnifying glass configuration (object between F and O).

 

Worked Numerical 5.2 — Concave Lens

Problem: A concave lens has focal length 25 cm. Object placed 40 cm from lens.

Find image position and magnification.

 

Given: u = −40 cm, f = −25 cm (concave lens, negative)

 

1/v − 1/u = 1/f

  1/v − 1/(−40) = 1/(−25)

  1/v + 1/40 = −1/25

  1/v = −1/25 − 1/40 = (−8 − 5)/200 = −13/200

  v = −200/13 ≈ −15.4 cm

 

v is negative → image is on the SAME SIDE as object (left of lens) → VIRTUAL image.

Magnification: m = v/u = (−15.4)/(−40) = +0.385

 

Image is VIRTUAL, ERECT, DIMINISHED (m ≈ +0.39, so image is about 39% of object size).

 

6. Power of a Lens

 

The power of a lens is a measure of its ability to converge or diverge a beam of light. A lens with a shorter focal length bends light more strongly and therefore has greater power. Power is used extensively in the field of optometry — the power printed on spectacle prescriptions is the power of the corrective lens.

 

POWER OF A LENS:

 

  P  =  1 / f

 

where f is the focal length in METRES.

 

  Unit of power: DIOPTRE (D)   [1 dioptre = 1 m⁻¹]

 

  CONVEX lens: f is POSITIVE → Power is POSITIVE

  CONCAVE lens: f is NEGATIVE → Power is NEGATIVE

 

COMBINATION OF LENSES (lenses placed in contact):

 

  P_total  =  P₁  +  P₂  +  P₃  + ...

 

  (The total power is the algebraic sum of individual powers)

  Equivalent focal length: 1/f = 1/f₁ + 1/f₂ + ...

 

Worked Numerical 6.1 — Power and Combination of Lenses

Problem: Two lenses — one convex of focal length 20 cm and one concave of focal length 40 cm

— are placed in contact. Find: (a) total power, (b) equivalent focal length.

 

Convex lens: f₁ = +20 cm = +0.20 m → P₁ = 1/0.20 = +5.0 D

Concave lens: f₂ = −40 cm = −0.40 m → P₂ = 1/(−0.40) = −2.5 D

 

(a) Total power:  P = P₁ + P₂ = 5.0 + (−2.5) = +2.5 D

 

(b) Equivalent focal length:  f = 1/P = 1/2.5 = 0.40 m = 40 cm

 

The combination acts as a CONVEX lens (P positive) of focal length 40 cm.

 

Power — Quick Reference

Power unit = Dioptre (D) = m⁻¹

Convex lens → Positive power (e.g., +3.5 D)

Concave lens → Negative power (e.g., −2.0 D)

Short focal length → HIGH power (bends light strongly)

Long focal length → LOW power (bends light weakly)

 

Spectacle prescriptions: +ve power = convex lens = treats hypermetropia (far-sightedness)

                         −ve power = concave lens = treats myopia (near-sightedness)

 

7. Comparison Tables — High-Value Board Exam Content

 

7.1 Concave Mirror vs Convex Mirror

 

Feature

Concave Mirror

Convex Mirror

Reflecting surface

Inner (hollow) side — curves inward

Outer side — curves outward

Type

Converging mirror

Diverging mirror

Focus

Real focus — in front of mirror

Virtual focus — behind mirror

Focal length sign

-ve (negative)

+ ve (positive)

Image (generally)

Can be real or virtual

Always virtual, erect, diminished

Image when object beyond F

Real, inverted

Virtual, erect (always)

Image when object between F and P

Virtual, erect, enlarged

Virtual, erect, diminished

Uses

Shaving mirror, dental mirror, solar furnace, torch reflector, telescope

Rear-view mirror in vehicles, security mirrors in shops

 

7.2 Convex Lens vs Concave Lens

 

Feature

Convex Lens

Concave Lens

Shape

Thicker at centre, thinner at edges

Thinner at centre, thicker at edges

Type

Converging lens

Diverging lens

Focus

Real focus — on transmission side

Virtual focus — on same side as object

Focal length sign

+ve (positive)

-ve (negative)

Power sign

Positive (+)

Negative (−)

Image (generally)

Can be real or virtual (at one position)

Always virtual, erect, diminished

Uses

Magnifying glass, camera, microscope, telescope eyepiece, projector

Spectacles for myopia (near-sightedness), Galilean telescope eyepiece

 

7.3 Mirror Formula vs Lens Formula — Side by Side

 

Aspect

Mirror Formula

Lens Formula

Formula

1/v + 1/u = 1/f

1/v − 1/u = 1/f

Magnification

m = −v/u

m = v/u

Reference point

Pole (P) of mirror

Optical Centre (O) of lens

Real image v sign

Negative (in front)

Positive (on far side of lens)

Virtual image v sign

Positive (behind mirror)

Negative (same side as object)

Concave/Convex f

Concave: f negative; Convex: f positive

Convex: f positive; Concave: f negative

 

8. Common Mistakes to Avoid

 

Mistake

Why It Is Wrong

Correct Approach

Using +u for object distance

Object is always to the LEFT → against incident light direction

u is ALWAYS NEGATIVE for real objects in both mirrors and lenses

Using mirror formula for lenses

Formulas are different

Mirror: 1/v+1/u=1/f  |  Lens: 1/v−1/u=1/f  (note the minus sign for lens)

m = v/u for mirrors

Mirror magnification has a negative sign

Mirror: m = −v/u  |  Lens: m = v/u  (no negative for lens)

Concave mirror f is positive

Concave mirror focus is IN FRONT (real focus)

Concave mirror: f is NEGATIVE. Convex mirror: f is POSITIVE.

Convex lens f is negative

Convex lens focus is on far side (real focus, positive direction)

Convex lens: f is POSITIVE. Concave lens: f is NEGATIVE.

Power unit = cm⁻¹

Power requires focal length in METRES

P = 1/f (metres only). 1 D = 1 m⁻¹. Convert cm to m first!

Saying all mirror images are inverted

Concave mirror with object between F and P gives erect image

Concave: erect only when object between F and P. Convex: always erect.

Confusing lateral displacement with deviation

Glass slab causes shift, not direction change

Emergent ray is PARALLEL to incident ray (same direction) but laterally shifted.

 

9. Key Definitions and Formula Summary

 

Term / Formula

Definition / Value

Reflection

Bouncing of light off a surface back into the original medium

Laws of Reflection

∠i = ∠r; incident ray, reflected ray, normal are coplanar

Refraction

Bending of light as it passes from one medium to another due to change in speed

Snell's Law

n₁ sin i = n₂ sin r  (or sin i / sin r = n₂/n₁ = constant)

Refractive Index (n)

n = c/v = speed of light in vacuum / speed of light in medium

Refractive index of glass

≈ 1.50 (crown glass) to 1.70 (flint glass)

Refractive index of water

≈ 1.33

Centre of Curvature (C)

Centre of the sphere of which the mirror/lens surface is part

Focal Length (f)

Distance from pole (P) or optical centre (O) to focus (F). f = R/2

Concave mirror f

NEGATIVE  (focus in front, real focus)

Convex mirror f

POSITIVE  (focus behind, virtual focus)

Mirror Formula

1/v + 1/u = 1/f  (with sign convention)

Mirror Magnification

m = −v/u = h'/h

Convex lens f

POSITIVE  (focus on far side, real focus)

Concave lens f

NEGATIVE  (focus on near/object side, virtual focus)

Lens Formula

1/v − 1/u = 1/f  (note minus sign — differs from mirror)

Lens Magnification

m = v/u = h'/h  (no negative sign — differs from mirror)

Power of Lens (P)

P = 1/f  (f in metres). Unit: Dioptre (D) = m⁻¹

Convex lens power

POSITIVE (+)  e.g., +2.5 D

Concave lens power

NEGATIVE (−)  e.g., −3.0 D

Combined power

P_total = P₁ + P₂ + P₃ + ...  (algebraic sum)

Lateral Displacement

Perpendicular shift of emergent ray vs incident ray through a glass slab

R = 2f

Radius of curvature = 2 × focal length for both mirrors and lenses

 

10. Key Points to Remember

 

•         u is ALWAYS negative for real objects in both mirrors and lenses (object always to the left of the device).

•         Mirror formula: 1/v + 1/u = 1/f | Magnification: m = −v/u

•         Lens formula: 1/v − 1/u = 1/f | Magnification: m = v/u (no negative sign)

•         Concave mirror f = negative. Convex mirror f = positive.

•         Convex lens f = positive. Concave lens f = negative.

•         Concave mirror + Convex lens: Object between F and pole/O → Virtual, Erect, Enlarged image.

•         Convex mirror + Concave lens: ALWAYS Virtual, Erect, Diminished — regardless of object position.

•         Power (P) = 1/f where f must be in METRES. Unit = Dioptre (D).

•         Convex lens/concave mirror: Object at F → image at infinity. Object at 2F → same-size real inverted image.

•         Glass slab: Emergent ray parallel to incident ray but laterally displaced. No net deviation.

•         Refractive index: Water = 1.33; Glass ≈ 1.5; Diamond = 2.42. Higher n = slower speed = more bending.

•         R = 2f: Radius of curvature is always twice the focal length.

 

11. Practice Questions

 

Modelled on CBSE board exam patterns. For numerical questions: write Given, Formula, Substitution, Calculation, Answer (units + description). For diagram questions: label all key points (P, F, C or O, F₁, F₂).

 

11.1 — 1 Mark Questions (VSA)

 

1.       State the relationship between focal length and radius of curvature of a spherical mirror.

2.       Write the sign convention for distances measured in the direction of incident light.

3.       A concave mirror has a focal length of 20 cm. What is its radius of curvature?

4.       Define the power of a lens. What is its SI unit?

5.       A convex lens has focal length +25 cm. What is its power in dioptres?

6.       Which type of mirror is used as rear-view mirror in vehicles and why?

7.       State Snell's Law of refraction.

8.       What is lateral displacement? In which situation does it occur?

 

11.2 — 3 Mark Questions (SA)

 

9.       Draw ray diagrams showing image formation by a concave mirror when the object is (a) at C, (b) between F and P.

10.   An object 4 cm high is placed 30 cm in front of a concave mirror of focal length 20 cm. Find (a) position, (b) size, and (c) nature of the image.

11.   Describe with a ray diagram the image formed by a convex lens when the object is beyond 2F. State two uses of a convex lens in this configuration.

12.   An object is placed at a distance of 60 cm from a convex lens of focal length 20 cm. Calculate the image distance and magnification.

13.   List three differences between a convex mirror and a concave mirror.

14.   Two thin lenses of power +4 D and −2 D are placed in contact. Find (a) combined power, (b) equivalent focal length, and (c) state what type of lens the combination behaves as.

 

11.3 — 5 Mark Questions (LA)

 

15.   (a) State the mirror formula. (b) An object 5 cm tall is placed 25 cm in front of a concave mirror with R = 60 cm. Find the position, size, and nature of the image. Draw a neat ray diagram to verify. (c) What happens to the image as the object is moved from beyond C toward F?

16.   (a) State the laws of refraction. (b) A ray of light passes from air into a glass slab. Explain the changes in speed, wavelength, and direction. (c) Define refractive index. If the speed of light in glass is 2 × 10⁸ m/s, find the refractive index of glass.

17.   (a) Define power of a lens. (b) An object is placed 20 cm from a convex lens of focal length 30 cm. Find the image position and magnification. (c) A doctor prescribes spectacles with lenses of power +1.5 D and −0.5 D for the two eyes. What is the focal length of each lens?

18.   (a) Draw ray diagrams showing image formation by a convex lens for object positions: (i) beyond 2F, (ii) at 2F, (iii) between F and 2F, (iv) between F and O. (b) State the image characteristics for each position.

19.   (a) Derive (state and explain) the lens formula 1/v − 1/u = 1/f. (b) Define magnification for a lens. (c) An object of height 2 cm is placed at 30 cm from a concave lens of focal length 15 cm. Find the image position, image height, and describe the image fully.

 

Board Exam Strategy for Light — Reflection and Refraction

1. ALWAYS write sign convention first in any numerical — u is negative, state f sign clearly.

2. Mirror formula: 1/v + 1/u = 1/f  |  Lens formula: 1/v − 1/u = 1/f  — the minus is critical.

3. Mirror magnification: m = −v/u  |  Lens magnification: m = v/u  — no negative for lens.

4. Power must use f in METRES — always convert cm to m before calculating power.

5. For image nature: check sign of v (positive/negative) AND sign of m (positive/negative).

6. Ray diagrams: draw at least two rays; label all key points (P, F, C for mirrors; O, F₁, F₂ for lenses).

7. Concave mirror and convex lens: Object between F and P/O → Virtual, Erect, Enlarged (exam favourite).

8. Convex mirror and concave lens: ALWAYS virtual, erect, diminished — no exceptions.

9. For 5-mark numericals: Given → Formula → Sign convention statement → Substitution → Answer.

10. Image formation tables are worth memorising: they cover every diagram question possible.

 

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