Snell's Law

Physics
NEET UG
Version 1Updated 22 Mar 2026

Snell's Law, also known as the law of refraction, quantitatively describes the relationship between the angles of incidence and refraction, and the refractive indices of the two media involved, when light or other waves pass through the boundary between two different isotropic media. Formally stated, it dictates that the ratio of the sines of the angles of incidence and refraction is equivalent to…

Quick Summary

Snell's Law, or the law of refraction, describes how light bends when it passes from one transparent medium to another. This bending occurs because light changes its speed in different media. The optical density of a medium is quantified by its refractive index (nn), defined as the ratio of the speed of light in vacuum (cc) to its speed in the medium (vv), i.

e., n=c/vn = c/v. Snell's Law states that for a given pair of media, the product of the refractive index and the sine of the angle of incidence (or refraction) in that medium is constant: n1sinθ1=n2sinθ2n_1 \sin \theta_1 = n_2 \sin \theta_2.

Here, θ1\theta_1 is the angle of incidence in medium 1 (refractive index n1n_1), and θ2\theta_2 is the angle of refraction in medium 2 (refractive index n2n_2). Angles are always measured with respect to the normal (perpendicular line) to the interface.

If light enters an optically denser medium (n2>n1n_2 > n_1), it bends towards the normal (θ2<θ1\theta_2 < \theta_1). If it enters an optically rarer medium (n2<n1n_2 < n_1), it bends away from the normal (θ2>θ1\theta_2 > \theta_1).

This law is fundamental to understanding lenses, prisms, and phenomena like apparent depth and total internal reflection.

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Key Concepts

Refractive Index and Speed of Light

The refractive index (nn) is a crucial property of a medium that dictates how much light slows down when…

Direction of Bending and Optical Density

Snell's Law, n1sinθ1=n2sinθ2n_1 \sin \theta_1 = n_2 \sin \theta_2, directly shows how the direction of bending relates to…

Critical Angle and Total Internal Reflection (TIR)

The critical angle (θc\theta_c) is a special angle of incidence that occurs when light travels from an…

  • Snell's Law:n1sinθ1=n2sinθ2n_1 \sin \theta_1 = n_2 \sin \theta_2
  • Refractive Index:n=c/vn = c/v (where cc is speed of light in vacuum, vv in medium)
  • Relative Refractive Index:n21=n2/n1=v1/v2n_{21} = n_2/n_1 = v_1/v_2
  • Bending:Rarer to denser (n1<n2n_1 < n_2)     \implies bends towards normal (θ2<θ1\theta_2 < \theta_1). Denser to rarer (n1>n2n_1 > n_2)     \implies bends away from normal (θ2>θ1\theta_2 > \theta_1).
  • Critical Angle (for TIR):sinθc=nrarer/ndenser\sin \theta_c = n_{\text{rarer}}/n_{\text{denser}} (occurs when light goes from denser to rarer medium).
  • Apparent Depth:n=Real Depth/Apparent Depthn = \text{Real Depth} / \text{Apparent Depth} (for normal viewing).
  • Unchanged Property:Frequency (ff) remains constant during refraction.
  • Changed Properties:Speed (vv), Wavelength (λ\lambda), Direction (unless θ1=0circ\theta_1 = 0^circ).

N-S-T-A: No Speed Through Air. (Meaning, frequency is constant, speed changes, direction changes, angles are from normal). Or, Snell's Law: Sin Light Angles With Normals. (n1sinθ1=n2sinθ2n_1 \sin \theta_1 = n_2 \sin \theta_2)

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