πŸ”­ Physics β€” Class XII

Ray Optics and Optical Instruments

Reflection, refraction, lenses, mirrors, and the instruments that extend human vision

πŸ“– Chapter 9 ⏱ ~70 min read 🏷️ Optics

Table of Contents

  1. Introduction
  2. Reflection at Spherical Mirrors
  3. Refraction
  4. Total Internal Reflection
  5. Refraction at Spherical Surfaces
  6. Thin Lenses
  7. Prism and Dispersion
  8. Optical Instruments

9.1 Introduction

Nature has endowed the human eye (retina) with the sensitivity to detect electromagnetic waves within a small range of the electromagnetic spectrum. Electromagnetic radiation belonging to this region of the spectrum (wavelength of about 400 nm to 750 nm) is called light. It is mainly through light and the sense of vision that we know and interpret the world around us.

9.2 Reflection at Spherical Mirrors

Spherical mirrors (concave and convex) follow the mirror formula:

1/v + 1/u = 1/f
u = object distance, v = image distance, f = focal length. f = R/2 (R = radius of curvature).

9.3 Refraction

Ray optics and optical instruments
Figure 9.1 β€” Snell's law, thin lens formula, and optical instruments

Refraction is the bending of light as it passes from one medium to another with a different refractive index:

n₁ sin θ₁ = nβ‚‚ sin ΞΈβ‚‚
Snell's Law. n = c/v (refractive index = speed of light in vacuum / speed in medium).

9.4 Total Internal Reflection

Total internal reflection (TIR) occurs when light travels from a denser medium to a rarer medium at an angle greater than the critical angle:

sin C = nβ‚‚/n₁ = 1/n
C = critical angle. All light is reflected back. Used in optical fibres, mirages, diamonds.
πŸ’‘ Applications of TIR

Optical fibres (communication), diamonds (brilliance), mirages (desert illusion), prism binoculars, periscopes with totally reflecting prisms.

9.5 Refraction at Spherical Surfaces

For refraction at a single spherical surface:

nβ‚‚/v βˆ’ n₁/u = (nβ‚‚βˆ’n₁)/R
n₁, nβ‚‚ = refractive indices of object/image space. R = radius of curvature of surface.

9.6 Thin Lenses

The thin lens formula relates object distance, image distance, and focal length:

1/v βˆ’ 1/u = 1/f
u = object distance, v = image distance, f = focal length of lens.
πŸ”΅

Convex (Converging) Lens

Converges parallel rays to focal point. Real or virtual image depending on object position. f > 0.

πŸ”΄

Concave (Diverging) Lens

Diverges parallel rays. Always produces virtual, erect, diminished image. f < 0.

9.7 Prism and Dispersion

A prism deviates light by an angle that depends on the refractive index and the prism angle:

Ξ΄ = (n βˆ’ 1)A (for thin prism)
Ξ΄ = angle of deviation, A = prism angle, n = refractive index. Violet light deviates most, red least.

9.8 Optical Instruments

πŸ”¬

Microscope

m = mβ‚€ Γ— m_e = (D/f_o)(L/f_e). Simple microscope: converging lens held near object. Compound: two lenses for higher magnification.

πŸ”­

Telescope

m = βˆ’f_o/f_e. Large objective collects light from distant objects. Small eyepiece acts as magnifier. Resolving power ∝ 1/d.

⚑ Resolving Power

The minimum angular separation between two point objects that can be distinguished: ΞΈ_min = 1.22Ξ»/d (Rayleigh criterion). Larger aperture d gives better resolving power.

Ch 8 β€” Electromagnetic Waves Ch 10 β€” Wave Optics