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JEE Main Physics Optics 2027: Mirrors, Lenses, Young's Double Slit & Polarization

Ray optics and wave optics in one guide: mirror and lens formulas, prisms, total internal reflection, YDSE, diffraction and Brewster's law with worked examples.

Edurack

September 28, 2026

JEE Main Physics Optics 2027: Mirrors, Lenses, Young's Double Slit & Polarization

Optics is two chapters in one: ray optics, where geometry and sign convention rule, and wave optics, where interference and diffraction decide. Both halves are formula-friendly, and once you fix the sign convention, most numericals become mechanical.

In ray optics, sign convention is the entire game. Choose one and never switch mid-problem.

Chapter at a Glance

SnapshotDetail
NTA unitUnit 16 of 20 — Optics
Priority (trend-based)Moderate
Typical question styleSign-convention numericals in ray optics, formula MCQs in wave optics
Best first stepFix the sign convention once, then practise mirror and lens problems

Priority reflects past-paper trends, not an official NTA weightage.

What the NTA Syllabus Covers

  • Reflection, spherical mirrors and mirror formula
  • Refraction at plane and spherical surfaces, thin lens and lens maker's formula, total internal reflection, magnification, power, lenses in contact, prism
  • Microscope and astronomical telescope with their magnifying powers
  • Wave optics: Huygens' principle, Young's double slit experiment, coherent sources, single-slit diffraction, polarization, Brewster's law and Polaroids

Master These Topics

1. Mirrors and Lenses with Cartesian Sign Convention

Measure distances from the pole or optical centre, positive along the direction of incident light.

  • Mirror: 1/v + 1/u = 1/f, magnification m = −v/u
  • Thin lens: 1/v − 1/u = 1/f, magnification m = v/u
  • Lens maker's formula: 1/f = (n − 1)(1/R₁ − 1/R₂)
  • Power P = 1/f with f in metres, in dioptres. Lenses in contact: P = P₁ + P₂.

Worked example (mirror): An object is 30 cm from a concave mirror with f = −10 cm. Then 1/v = 1/f − 1/u = −1/10 + 1/30 = −2/30, so v = −15 cm. Magnification m = −v/u = −(−15)/(−30) = −0.5. The image is real, inverted and half the object's size.

Worked example (lens): A convex lens with f = +20 cm and an object at u = −30 cm: 1/v = 1/20 − 1/30 = 1/60, so v = 60 cm and m = v/u = −2, real, inverted and twice as large.

Trap: A concave mirror has negative f and a convex lens has positive f in Cartesian convention. Mixing the two conventions is the most common source of wrong answers.

2. Refraction, TIR and Prism

Snell's law: n₁ sinθ₁ = n₂ sinθ₂. Total internal reflection needs light going from denser to rarer medium beyond the critical angle: sinC = 1/n. For n = 4/3 (water), sinC = 0.75, so C ≈ 49°.

For a thin prism, deviation is δ = (n − 1)A. For a general prism at minimum deviation, n = sin((A + δ_m)/2) / sin(A/2).

3. Young's Double Slit Experiment

Fringe width is β = λD / d, where D is the screen distance and d is slit separation. Bright fringes occur where path difference is nλ, dark where it is (n + ½)λ.

Worked example: λ = 600 nm, D = 1 m, d = 1 mm. Then β = 6 × 10⁻⁷ × 1 / 10⁻³ = 6 × 10⁻⁴ m = 0.6 mm.

For single-slit diffraction of slit width a, the central maximum has width 2λD / a.

4. Polarization

Only transverse waves can be polarized, which is evidence that light is a transverse wave. At the Brewster angle, reflected light is completely plane polarized: tanθ_B = n. For glass with n = 1.5, θ_B ≈ 56°.

5. Optical Instruments

For an astronomical telescope in normal adjustment, M = f₀ / f_e. A compound microscope has magnification roughly (L/f₀)(D/f_e), where D = 25 cm is the least distance of distinct vision.


Common Traps to Avoid

  • Using the mirror formula for a lens or the reverse.
  • Forgetting that the object distance u is negative in Cartesian convention.
  • Mixing up fringe width with fringe position.
  • Applying Brewster's law without checking that the light travels from the rarer to the denser medium.

60-Second Revision Sheet

  • Mirror 1/v + 1/u = 1/f; lens 1/v − 1/u = 1/f
  • Lens maker 1/f = (n − 1)(1/R₁ − 1/R₂)
  • TIR sinC = 1/n; Brewster tanθ_B = n
  • YDSE β = λD/d; single-slit central width 2λD/a

Your Study Plan

  1. Day 1: reflection, mirrors, sign convention practice.
  2. Day 2: lenses, combinations, lens maker's formula and power.
  3. Day 3: refraction, TIR, prism and optical instruments.
  4. Day 4: wave optics (YDSE, diffraction, polarization), timed set.

Practice Optics Questions Free → (opens in a new tab)


Continue Your Physics Journey


Frequently Asked Questions

Which is more important for JEE Main, ray optics or wave optics?

Both appear. Ray optics gives numerical problems, while wave optics gives quick formula-based questions, especially on YDSE and polarization.

What is the condition for total internal reflection?

Light must travel from a denser to a rarer medium and strike the boundary at an angle larger than the critical angle.

Ready to put this into practice?

See the matching test series on Edurack.

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