Measuring the speed of light
In 1849 Hippolyte Fizeau timed light over a round trip of about 17 km with a spinning wheel of 720 teeth.
Is light instant?
Switch on a lamp and the room seems to fill with light at once. For a long time many thinkers, including Johannes Kepler and René Descartes, took the speed of light to be infinite, as the American Physical Society notes in its history of the measurement. Galileo was among the first to doubt it. In 1638 he described an experiment in which two people with covered lanterns stand far apart: the first uncovers his lantern, and the second uncovers hers the moment she sees the light. Timing the gap should give the speed. OpenStax notes that such early attempts only showed that light is extremely fast, perhaps instantaneous.
It is easy to see why the lantern test failed. With the lanterns 5 km apart, the light covers 10 km there and back in about 33 millionths of a second, far less than the fraction of a second it takes a person to react. To catch light in the act you need either enormous distances or very fast timing. The first success used enormous distances.
Rømer and the moons of Jupiter
In the 1670s the Danish astronomer Ole Rømer was timing the eclipses of one of Jupiter’s moons as it passed behind the planet. OpenStax describes what he noticed: the moon’s average orbital period, measured from Earth, seemed to change depending on whether the Earth was moving toward Jupiter or away from it. When the Earth was farther away the eclipses came late, and when it was nearer they came early. He concluded that the light was taking time to cross the changing distance. A value calculated from his 1676 data, OpenStax says, is 2.26 × 10⁸ m/s, about 25% below today’s figure, mainly because the size of the Earth’s orbit was not well known then. The important point was that light has a finite speed.
Wheels and mirrors on Earth
The first measurement made entirely on the ground came from Hippolyte Fizeau in 1849. He sent a beam of light through the gaps of a spinning toothed wheel to a mirror 8633 m away and back. At a slow spin the returning light passed through the same gap. As the wheel sped up, a point came where the light that left through a gap came back to find a tooth in the way, and the light seen by the observer dimmed. The wheel had 720 teeth. The light first vanished at 12.6 turns per second, when a tooth had moved into the gap’s place; at twice that speed, 25.2 turns per second, it showed again through the next gap, so the light’s round trip took the time for the wheel to move on by one gap. That gives 2 × 8633 m × 720 × 25.2 per second ≈ 313 000 km/s, about 4.5% too high.
Léon Foucault replaced the wheel with a rotating mirror. Light bounced off the spinning mirror to a fixed mirror and back, and in the meantime the rotating mirror had turned slightly, so the returning beam was shifted by a small measurable angle. In 1862 he obtained 298 000 km/s, within 0.6% of the modern value, using mirrors only about 20 m apart. With the same kind of apparatus he and Fizeau had also shown, around 1850, that light travels more slowly in water than in air, as the wave theory of light predicted. Albert Michelson refined the rotating-mirror method for decades; OpenStax describes his set-up with a fixed mirror 35 km away, and his 1926 result was 299 796 km/s, about 12 parts per million too high.
From measuring c to defining it
By the 1970s lasers with very stable frequencies let scientists measure the frequency and the wavelength of the same light and multiply them, since c = fλ. NIST describes how Ken Evenson’s group in Boulder obtained 299 792 456.2 ± 1.1 m/s, a hundred times more accurate than before. The limit was no longer the measurement of light but the definition of the metre itself, then based on light from krypton atoms. So in 1983 the General Conference on Weights and Measures turned the problem around and defined the metre as the length of the path travelled by light in a vacuum in 1/299 792 458 of a second. Since then the speed of light has been exactly 299 792 458 m/s by definition, and distance is measured with clocks.
A few numbers put the speed in perspective. Light from the Sun, about 149.6 million km away, takes 499 seconds, a little over 8 minutes, to reach us. A laser pulse sent to a reflector on the Moon, 384 400 km away on average, returns about 2.56 seconds later.
- 1638: Galileo describes the covered-lantern test; it cannot detect a delay.
- 1676: Rømer explains early and late eclipses of a moon of Jupiter by light’s travel time.
- 1849: Fizeau’s toothed wheel: about 313 000 km/s.
- 1862: Foucault’s rotating mirror: 298 000 km/s.
- 1926: Michelson’s rotating mirrors: 299 796 km/s.
- 1972: NIST laser measurement: 299 792 456.2 ± 1.1 m/s.
- 1983: The metre is redefined; c = 299 792 458 m/s exactly.
| c in a vacuum | 299 792 458 m/s, exact since 1983 |
| Rømer, 1676 | Jupiter’s moon eclipses: light has a finite speed |
| Fizeau, 1849 | Toothed wheel, 720 teeth, 8633 m: about 313 000 km/s |
| Foucault, 1862 | Rotating mirror: 298 000 km/s |
| Sun to Earth | About 499 s, a little over 8 minutes |
- Fizeau: wheel to mirror 8633 m, 720 teeth, 25.2 turns per second. What speed does 2 × 8633 × 720 × 25.2 give, in units of 10⁸ m/s? Two decimal places.
- How long does sunlight take to reach the Earth from 1.496 × 10¹¹ m away? Use c = 2.998 × 10⁸ m/s and answer in seconds.
- A laser pulse goes to the Moon (384 400 km) and back. How many seconds does the round trip take? Two decimal places, c = 2.998 × 10⁵ km/s.
- Why did Galileo’s lantern experiment fail to measure the speed of light?
- The delay was far shorter than human reaction time
- Light does not travel between hills
- The lanterns were too bright
- Light is slower at night
- What did Rømer use to show that light takes time to travel?
- Eclipses of a moon of Jupiter
- A toothed wheel
- A rotating mirror
- A laser on the Moon
- Since 1983, the speed of light in a vacuum is…
- Exactly 299 792 458 m/s by definition
- Measured again every year
- Exactly 300 000 km/s
- Unknown to better than 1%
- Fizeau’s 313 274 km/s compared with 299 792 km/s: by what percentage was it too high? One decimal place.
- Which result from Foucault’s rotating-mirror work supported the wave theory of light?
- Light travels more slowly in water than in air
- Light travels faster in water
- Light has no speed in water
- Light speed depends on the colour of the mirror
- Rømer’s data gave 2.26 × 10⁸ m/s. By what percentage is that below 3.00 × 10⁸ m/s? Round to a whole number.
- Galileo’s lanterns (1638) could not catch the delay.
- Rømer (1676): Jupiter’s moon eclipses show light has a finite speed.
- Fizeau 1849 (wheel) and Foucault 1862 (mirror) measured c on the ground; Michelson refined it.
- 1983: the metre is defined from light, so c = 299 792 458 m/s exactly. Sunlight takes about 499 s.
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