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Colour, prisms and rainbows

Crown glass bends violet light at 410 nm a little more than red light at 660 nm, because its index of refraction is 1.530 for violet and 1.512 for red.

White light is a mixture

In the mid-1660s Isaac Newton let a narrow beam of sunlight into a darkened room through a hole in the window shutter and passed it through a glass prism. A band of colours appeared on the far wall. In a paper published in 1672, which a 2015 commentary in the Royal Society journal Philosophical Transactions calls the foundation of modern optics, he argued that the colours are not added by the prism; white light is a mixture of them, and the prism separates them because each colour is refracted by a slightly different amount. He also showed that a single colour picked out from the band and sent through a second prism stays the same colour.

OpenStax explains the reason. For a given material the index of refraction depends slightly on wavelength: it increases as the wavelength decreases and is greatest for violet. Violet light is therefore bent more than red, and white light fans out into the familiar order from red to violet. Spreading white light into its spectrum this way is called dispersion. More generally, dispersion happens whenever a process changes the direction of light by an amount that depends on wavelength.

White light entering a prism is refracted twice, once at each face. Violet is bent the most and red the least (spread exaggerated).
ColourWaterCrown glassDiamond
Red 660 nm1.3311.5122.410
Orange 610 nm1.3321.5142.415
Yellow 580 nm1.3331.5182.417
Green 550 nm1.3351.5192.426
Blue 470 nm1.3381.5242.444
Violet 410 nm1.3421.5302.458
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White light entering crown glass, with each colour refracted by its own index from OpenStax Table 25.2. The spread is small; try flint glass or diamond, which disperse more.

Colours and wavelengths

We usually name about six colours in a rainbow: red, orange, yellow, green, blue and violet, and sometimes indigo as well. OpenStax stresses that the spectrum is continuous: the names are labels for ranges of wavelength, from about 700 nm for red down to about 400 nm for violet. When the eye receives light of a single wavelength we tend to see one of these colours. The many other hues we can see are the eye’s response to mixtures. Sunlight contains all visible wavelengths and looks white, or very slightly yellow.

Objects get their colours from the light they send back to us. A leaf looks green under sunlight because it reflects more green light than other colours and absorbs much of the rest. Under a light that contains no green, the same leaf looks dark. A filter works in a similar way for light passing through it: a red filter lets red through and absorbs most other colours.

Rainbows

A rainbow is dispersion by water drops. OpenStax describes how light enters a drop, reflects from the back of it and leaves again, refracting both on the way in and on the way out. Since water’s index changes with wavelength, the colours leave at slightly different angles. You only see a rainbow when the Sun is behind you, and each colour reaches your eye from drops at its own angle from the direction of the sunlight, which is why the rainbow is an arc. Two reflections inside the drops make a fainter secondary rainbow above the first. Around 1300, as OpenStax tells, Kamal al-Din al-Farisi in Persia studied this with a large glass vessel of water inside a camera obscura, standing in for a giant raindrop, and Theodoric of Freiberg did similar experiments in Germany; both built on the work of Ibn al-Haytham.

BackgroundDispersion is not always welcome. OpenStax points out that white light sent along an optical fibre would spread out in time, its colours arriving at slightly different moments and blurring one message into the next. Lasers produce nearly a single wavelength, so their light disperses very little, one reason fibre networks use laser light. Astronomers turn the problem around: the dispersion of radio waves from space reveals how much matter they passed through on the way.
  1. Which colour does a glass prism bend the most?
    • Violet
    • Red
    • Green
    • All colours equally
  2. White light enters crown glass from air at 45°. Red has n = 1.512 and violet n = 1.530. By how many degrees do the two refracted rays differ? Two decimal places.
  3. In crown glass, which travels faster?
    • Red light
    • Violet light
    • They travel at the same speed
    • Neither moves in glass
  4. To see a rainbow, where must the Sun be?
    • Behind you
    • In front of you
    • Directly overhead
    • Below the horizon in front of you
  5. What makes the fainter secondary rainbow?
    • Two reflections inside the drops
    • Light passing through two clouds
    • Moonlight
    • Diffraction around the drops
  6. In which year was Newton’s paper on light and colours published?
    • 1672
    • 1801
    • 1543
    • 1905
  7. A leaf looks green in sunlight because it…
    • Reflects more green light and absorbs much of the rest
    • Gives off green light
    • Absorbs green light
    • Bends green light more than other colours
  8. What is the index of refraction of water for red light at 660 nm, from OpenStax Table 25.2?
  9. Why do fibre-optic networks prefer laser light to white light?
    • Laser light is nearly one wavelength, so it disperses very little
    • Lasers are slower
    • White light cannot enter glass
    • Laser light does not reflect
Key points
  • White light is a mixture of colours (Newton, paper of 1672).
  • n rises as wavelength falls, so violet bends more than red: dispersion.
  • Colour names label ranges of a continuous spectrum, about 400 to 700 nm.
  • Rainbow: refraction, one reflection, refraction in drops, Sun behind you; two reflections give the secondary bow.
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