Master Light Bending, Snell's Law, and Refractive Index Determination
When light travels from one transparent medium to another (like air to glass), it changes direction at the interface - this phenomenon is called refraction. The glass slab experiment is fundamental in optics, helping us understand how lenses, prisms, fiber optics, and even mirages work.
You observe refraction every day: a straw appearing bent in a glass of water, objects at the bottom of a pool appearing closer than they are, or why swimming pools look shallower than their actual depth. Understanding refraction is key to designing eyeglasses, cameras, microscopes, and countless optical instruments.
Swimming pools always appear shallower than they actually are due to refraction! Light from the pool bottom bends away from the normal when entering air, making your brain trace it back to a shallower position. This is why "Never dive in unknown water" is crucial safety advice - what looks like 4 feet might actually be 6 feet deep!
Refraction occurs because light travels at different speeds in different media. Light speed in vacuum is c = 3 Γ 10βΈ m/s, but it slows down in denser materials like glass or water. This speed change causes the light ray to bend.
Vacuum: 3 Γ 10βΈ m/s
Air: ~3 Γ 10βΈ m/s
Water: 2.25 Γ 10βΈ m/s
Glass: 2 Γ 10βΈ m/s
Angle between incident ray and normal (perpendicular) to the surface at the point of incidence
Angle between refracted ray and normal inside the second medium
Ratio of speed of light in vacuum to speed in medium: n = c/v
First Law: The incident ray, refracted ray, and normal all lie in the same plane.
Second Law (Snell's Law): The ratio of sine of angle of incidence to sine of angle of refraction is constant for a given pair of media.
For light traveling from air (nβ β 1) to glass (nβ = n):
Problem: Light enters glass at 60Β° angle of incidence. If refractive index of glass is 1.5, find angle of refraction.
Given: i = 60Β°, n = 1.5, n_air = 1
Solution:
Using Snell's law: nβ sin i = nβ sin r
1 Γ sin 60Β° = 1.5 Γ sin r
0.866 = 1.5 Γ sin r
sin r = 0.866 / 1.5 = 0.577
r = sinβ»ΒΉ(0.577) = 35.3Β°
Light bends toward normal as expected!
When light passes through a parallel-sided glass slab, the emergent ray is parallel to the incident ray but laterally displaced - it shifts sideways. This perpendicular distance between the incident and emergent rays is called lateral displacement.
Even though the emergent ray is parallel to the incident ray, the lateral shift means the light has traveled a longer path through the glass. This causes a slight time delay, which is exploited in optical instruments to create phase differences and interference patterns.
Observations:
| i (degrees) | r (degrees) | sin i | sin r | n = sin i/sin r |
|---|---|---|---|---|
| 30 | 19.5 | 0.500 | 0.334 | 1.50 |
| 40 | 25.4 | 0.643 | 0.429 | 1.50 |
| 50 | 30.7 | 0.766 | 0.511 | 1.50 |
Average n = 1.50 (standard value for glass)
When light travels from denser to rarer medium (glass to air) and angle of incidence exceeds a certain value called critical angle, the light is completely reflected back - no refraction occurs. This is total internal reflection.
Optical Fibers: Light signals travel long distances without loss through repeated total internal reflection
Diamonds: High refractive index (n = 2.42) gives low critical angle (24.4Β°) - causes brilliant sparkle
Mirages: Hot air near ground has lower refractive index - causes total internal reflection of sky light
Prisms: 45-45-90 prisms use TIR to reflect light better than mirrors
Refraction principles are fundamental to countless technologies:
When you look at a fish in water, it appears closer to the surface than it actually is. Due to refraction, apparent depth = real depth / n. For water (n = 1.33), a fish at 4m depth appears to be at only 3m! This is why spear fishing requires aiming below where the fish appears to be.
nβ sin i = nβ sin r - Fundamental equation relating incident and refracted angles
n = sin i / sin r = c/v. Measure of how much light slows in a medium.
Emergent ray parallel to incident ray but laterally displaced. No net deviation.
sin C = 1/n. Beyond this, total internal reflection occurs (denser to rarer medium).
Try our interactive refraction simulator! Trace light rays, adjust angles, measure refractive index, and visualize Snell's law.
Launch Interactive Experiment β