Refraction and total internal reflection
Light inside a diamond can only get out if it meets the surface within 24.4° of the normal, which is why diamonds sparkle.
Why light bends
A straw in a glass of water looks broken at the surface, and a fish in a tank can seem to be in two places at once. These are effects of refraction, the change of direction of light as it passes from one material into another. OpenStax explains the cause: light changes speed. Light is slower in glass or water than in air because it interacts with the atoms of the material. How much slower is measured by the index of refraction, n = c/v, where c is the speed of light in a vacuum and v its speed in the material. Since light is never faster than c, n is always at least 1.
| Material | Index of refraction n | Speed of light (× 10⁸ m/s) |
|---|---|---|
| Air (0 °C, 1 atm) | 1.000293 | about 3.00 |
| Ice | 1.309 | 2.29 |
| Water | 1.333 | 2.25 |
| Polystyrene | 1.49 | 2.01 |
| Crown glass | 1.52 | 1.97 |
| Flint glass | 1.66 | 1.81 |
| Zircon | 1.923 | 1.56 |
| Diamond | 2.419 | 1.24 |
Why should a change of speed change the direction? OpenStax uses a lawn mower. Push it at an angle from a footpath onto grass: the wheel that reaches the grass first slows down while the other is still on the path, so the mower swings toward the perpendicular. Going from grass back onto the path, the first wheel speeds up and the mower swings away from the perpendicular. Light does the same. Entering a slower material it bends toward the normal; entering a faster one it bends away. The path is exactly reversible, and light that hits the boundary head on, along the normal, goes straight through without bending.
Snell’s law
The exact rule is the law of refraction, or Snell’s law: n₁ sin θ₁ = n₂ sin θ₂, with both angles measured from the normal. OpenStax notes that it is named after the Dutch mathematician Willebrord Snell (1580 to 1626), although Ibn Sahl had found it in 984 and used it in his work On Burning Mirrors and Lenses. In one OpenStax example, light goes from air into a material at 30.0° and continues at 22.0°; then n₂ = sin 30.0° ÷ sin 22.0° = 1.33, the index of water. In another, light enters diamond at 30.0° and bends to only 11.9°: the bigger the change in speed, the bigger the change in direction.
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Total internal reflection
When light goes from a slower material into a faster one, from water into air for example, it bends away from the normal, so the refracted angle is larger than the incident angle. Tilt the incoming ray further and the refracted ray swings toward the surface. At one angle, the critical angle θc, it runs along the surface at 90°. Beyond that no light gets out at all: it is all reflected back inside. OpenStax calls this total internal reflection and gives θc = sin⁻¹(n₂/n₁), which only works when n₁ > n₂. For water to air θc is 48.6°, for polystyrene 42.2°, and for diamond only 24.4°. Going the other way, from air into water, total internal reflection cannot happen.
Total internal reflection is a perfect mirror that needs no silver coating, and it has many uses. In an optical fibre, light enters a thin glass core and keeps striking the side at angles beyond the critical angle, so it is reflected again and again and follows the fibre around bends. A coating of lower index, the cladding, keeps the light in even when fibres touch. OpenStax notes that most telephone and internet traffic now travels as laser light in such fibres, and that bundles of fibres in endoscopes let doctors see inside the body. Binoculars use prisms with total internal reflection instead of mirrors. In a diamond the small critical angle traps light, which bounces around inside and escapes only at a few places: the sparkle.
- Water has n = 1.333. Using c = 3.00 × 10⁸ m/s, what is the speed of light in water, in units of 10⁸ m/s? Two decimal places.
- Light goes from air into a material at 30.0° and refracts to 22.0°. What is the material’s index? Two decimal places.
- Light goes from air into crown glass (n = 1.52) at 45°. What is the angle of refraction? One decimal place.
- What is the critical angle for light going from water (n = 1.333) into air? One decimal place.
- What is the critical angle for diamond (n = 2.419) to air? One decimal place.
- Light passes from water into air at an angle. It bends…
- Away from the normal
- Toward the normal
- Not at all
- Back into the water every time
- Total internal reflection can happen when light goes…
- From glass into air
- From air into water
- From air into glass
- From air into diamond
- A ray hits the surface of water straight on, along the normal. It…
- Goes straight through without bending
- Bends toward the surface
- Is totally reflected
- Splits into two rays at right angles
- What keeps light inside an optical fibre?
- Total internal reflection at the core’s surface
- A silver coating
- Diffraction
- The fibre absorbing light at the edges
- Diamond has n = 2.419. Light enters it from air at 30.0°. What is the angle of refraction? One decimal place.
- Light changes speed between materials; n = c/v.
- Snell’s law: n₁ sin θ₁ = n₂ sin θ₂, angles from the normal.
- Into a slower material: toward the normal. Into a faster one: away.
- From n₁ > n₂ beyond θc = sin⁻¹(n₂/n₁): total internal reflection (water 48.6°, diamond 24.4°).
Sources for this course (16)
- OpenStax College Physics 2e (openstax.org/books/college-physics-2e): 25.2 The Law of Reflection (θr = θi, diffuse vs mirror reflection, image as far behind the mirror)
- 25.3 The Law of Refraction (Roemer 1676 data -> 2.26 × 10⁸ m/s, about 25% low; Michelson rotating mirrors with a fixed mirror 35 km away, 0.04%; c = 2.99792458 × 10⁸ m/s; n = c/v; Table 25.1 air 1.000293, water 1.333, ice 1.309, crown glass 1.52, flint 1.66, polystyrene 1.49, zircon 1.923, diamond 2.419; Snell's law; 30.0° -> 22.0° gives 1.33; air to diamond 30.0° -> 11.9°; zircon 1.56 × 10⁸ m/s; Ibn Sahl 984; Snell 1580 to 1626; lawn-mower analogy)
- 25.4 Total Internal Reflection (mirror more than 90%; θc = sin⁻¹(n2/n1); polystyrene 42.2°, water 48.6°, diamond 24.4°; fibre optics, cladding; corner reflectors on bicycles and on the Moon; binoculars)
- 25.5 Dispersion (Kamal al-Din al-Farisi 1267 to 1319, camera obscura and a water-filled glass vessel; Theodoric of Freiberg; Ibn al-Haytham; about six rainbow colours; Table 25.2 n at 660/610/580/550/470/410 nm; violet bent most; rainbow seen looking away from the Sun; secondary rainbow from two reflections; lasers disperse little)
- 25.6 Image Formation by Lenses (ray tracing rules, P = 1/f in diopters, 1/do + 1/di = 1/f, m = −di/do, 0.750 m object and f = 0.500 m -> 1.50 m and m = −2.00, magnifier do 7.50 cm -> di −30.0 cm and m = 4.00, Table 25.3 three cases)
- 26.1 Physics of the Eye (cornea and lens act as one thin lens, most bending at the cornea, cornea n 1.38, lens-to-retina 2.00 cm, near point 25 cm, power 50.0 D to 54.0 D, hair 1.20 × 10⁻² cm at 60.0 cm)
- 27.3 (Young 1801)
- NASA science.nasa.gov/eclipses/geometry (umbra, penumbra; typical umbral path may be less than 50 miles wide, penumbra a thousand miles or more) and nasa.gov image article Diagram of Umbra and Penumbra (umbra shrinks, penumbra grows away from the Sun)
- NASA Visible Light page (Newton 1665 prism experiment, 380 to 700 nm)
- Royal Society, Fara 2015 commentary on Newton (1672) New Theory about Light and Colours (royalsocietypublishing.org/rsta/article/373/2039/20140213)
- NIST Meter page (Evenson group 299 792 456.2 ± 1.1 m/s; 1983 definition fixes c = 299 792 458 m/s) and NIST J. Res. 1972 measurement (tf.nist.gov/general/pdf/527.pdf)
- APS News July 2010, Fizeau (Galileo lanterns; Roemer 1676; Fizeau 1849, 313 300 km/s, about 5% high)
- Wikipedia Fizeau's measurement (8633 m, 720 notches, 25.2 turns per second -> 313 274 304 m/s, 4.5% high) and Speed of light (Galileo proposal 1638; Foucault 1862 298 000 ± 500 km/s, −0.60%; Michelson 1926 299 796 ± 4 km/s)
- Baez and DESY "How is the speed of light measured?" (same table)
- NASA Moon Fact Sheet (mean distance 384 400 km)
- IAU 2012 astronomical unit 149 597 870 700 m.
Checked: 2026-10-17