The history

The history of speed, velocity and acceleration

From Aristotle's falling stones to satellites that clock your bike ride: 2,300 years of learning what 'how fast' means.

For two thousand years people followed Aristotle: heavy things fall faster, and motion needs a push. Oxford scholars in the 1330s and Galileo in the 1600s learned to treat speed as a number that changes, and to measure how quickly it changes. Newton linked acceleration to force, speedometers and radar put speed on every road, and Einstein showed that one speed, light's, can never be reached.

2,300+
years
19
moments
6
people
12
places

c. 1335

Mean speed rule

William Heytesbury and the Merton Calculators, England

c. 1350s

Velocity–time graph

Nicole Oresme, France

1604

Law of fall (distance ∝ time²)

Galileo Galilei, Italy

1888

Speedometer patent

Josip Belušić, Croatia

1896

Speeding fine

Walter Arnold, England

1899

Car over 100 km/h

Camille Jenatzy, La Jamais Contente

1949

Radar speeding tickets

Connecticut State Police, USA

c. 350 BCEWhy do things move?

400 BCE – 1299

Why do things move?

Aristotle's picture of motion rules, with a few thinkers like Philoponus testing it by dropping things.

350 BCE

c. 350 BCE

Heavier things fall faster, says Aristotle

AristotleAthens, Greece

In his Physics, Aristotle taught that a moving thing needs a mover to keep it going, and that heavier bodies fall faster than light ones. It matched everyday sights like a falling leaf, and it ruled for nearly 2,000 years.

Why it mattered. It set the puzzle every later thinker had to solve: what speed and falling really are.

517

c. 517

A drop test against Aristotle

John PhiloponusAlexandria, Egypt

The Alexandrian scholar John Philoponus wrote that if you drop two weights, one many times heavier, the difference in their fall times is very small. He argued that moving things carry an 'impetus' given to them.

Why it mattered. It was the first recorded doubt, based on dropping things, that heavier means faster.

1300 – 1599

Speed becomes a number

Oxford's Merton scholars and Nicole Oresme treat speed as a quantity that changes, and draw it as a graph.

1335

c. 1328–1350

The Oxford Calculators measure motion

Thomas Bradwardine, William Heytesbury, Richard Swineshead, John DumbletonMerton College, Oxford, England

A group of Merton College scholars began treating speed as a quantity that can change from instant to instant. Heytesbury's rules of about 1335 include the mean speed rule: speeding up steadily, you cover the same distance as moving the whole time at the speed you had halfway through.

Why it mattered. The mean speed rule is s = ½ (u + v) t, three centuries before Galileo tested it.

1350

c. 1350s

Motion drawn as a graph

Nicole OresmeParis, France

Nicole Oresme drew a changing speed as a line of heights over time, so that the area of the shape stood for the distance covered. With it he proved the Merton rule with a simple triangle and rectangle.

Why it mattered. It is the first velocity–time graph, and the idea that the area under it is the distance.

1580 – 1700

Uniform acceleration

Galileo measures falling and rolling, defines acceleration, and Newton ties it to force.

1586

Two lead balls from a church tower

Simon Stevin and Jan Cornets de GrootDelft, Netherlands

Stevin and de Groot dropped two lead balls, one ten times heavier than the other, about 30 feet onto a board from the New Church tower in Delft. The two thuds sounded as one.

Why it mattered. A real, recorded experiment against Aristotle, years before the more famous Pisa story.

1604

16 October 1604

Distance grows with time squared

Galileo GalileiPadua, Italy

In a letter to his friend Paolo Sarpi, Galileo stated that a falling body covers distances that grow as the square of the time: 1, 4, 9, 16. He was timing balls rolling down gentle slopes, which slow the fall enough to measure.

Why it mattered. It is the first statement of s = ½ a t² tested against measurements.

1638

Uniform acceleration is defined

Galileo GalileiLeiden (printed), from Arcetri, Italy

In Two New Sciences Galileo defined uniformly accelerated motion as one that gains equal amounts of speed in equal times. He timed bronze balls rolling down a grooved ramp with a water clock, and showed all bodies would fall together without air.

Why it mattered. It is the definition of acceleration still taught today: a = Δv ÷ Δt.

1644

Motion carries on in a straight line

René DescartesAmsterdam, Netherlands

In his Principles of Philosophy, Descartes wrote that a moving body keeps moving in a straight line unless something stops or turns it, and that going round a circle needs something pulling inwards.

Why it mattered. It made direction part of motion, the seed of the idea of velocity.

1673

How hard it is to go round

Christiaan HuygensParis, France

In Horologium Oscillatorium Huygens published his theorems on circular motion: the pull needed grows with the square of the speed and shrinks with the radius, what we now write as v² ÷ r.

Why it mattered. It explains the huge accelerations of fan blades and spinning drums.

1676

Light has a speed

Ole RømerParis Observatory, France

Timing the eclipses of Jupiter's moon Io, Rømer noticed they came late when Earth was far from Jupiter. Light, he concluded, takes time to cross space. His figures implied a speed of roughly 220,000 km/s.

Why it mattered. The fastest speed there is turned out to be finite, and measurable.

1684

Speed at an instant

Gottfried Wilhelm LeibnizLeipzig, Germany

Leibniz published his calculus, a method for finding the rate of change at a single instant. Newton had worked out his own version, 'fluxions', in the 1660s. Instantaneous speed is the limit of distance ÷ time over a vanishing interval.

Why it mattered. It gave a precise meaning to what a speedometer shows.

1687

5 July 1687

Newton ties acceleration to force

Isaac NewtonLondon, England

Newton's Principia set out his three laws of motion. The second says a force produces an acceleration, a = F ÷ m, and the first that without a force velocity stays the same in speed and direction.

Why it mattered. Speed, velocity and acceleration became the language of all mechanics.

1860 – 1960

Speed on the road

Cars, speed limits, speedometers and radar guns make speed something everyone measures.

1896

28 January 1896

The first speeding fine

Walter ArnoldPaddock Wood, Kent, England

Walter Arnold was fined for driving at about 8 mph (13 km/h) where the limit was 2 mph, chased down by a policeman on a bicycle.

Why it mattered. Speed limits made measuring speed a legal matter, not just a scientific one.

1899

29 April 1899

Faster than 100 km/h

Camille JenatzyAchères, near Paris, France

Jenatzy's bullet-shaped electric car La Jamais Contente became the first road vehicle to pass 100 km/h, reaching about 105.9 km/h.

Why it mattered. The first car past a hundred was electric, like today's fastest accelerators.

1902

7 October 1902

The eddy-current speedometer

Otto Schultze (after Josip Belušić's 1888 patent)Berlin, Germany

Croatian inventor Josip Belušić patented an electric speedometer in 1888. Otto Schultze patented the eddy-current speedometer in 1902: a spinning magnet drags an aluminium cup against a spring, turning the needle. Speedometers became standard on cars from about 1910.

Why it mattered. It put instantaneous speed in front of every driver.

1947

1947–1949

Radar catches speeders

John L. Barker Sr. and Ben MidlockGlastonbury, Connecticut, USA

Two engineers at the Automatic Signal Company turned wartime Doppler radar into a speed meter. Connecticut State Police tried it in 1947 and began issuing radar speeding tickets in February 1949.

Why it mattered. The Doppler shift of a reflected wave measures speed directly, with no stopwatch.

By the numbers

The land speed record

The fastest anyone has driven on land, from electric cars in 1898 to a jet car that broke the sound barrier in 1997.

0 km/h500 km/h1000 km/h1500 km/h 1900191019201930194019501960197019801990 1898: Chasseloup-Laubat, Jeantaud electric car18981899: Jenatzy, La Jamais Contente: first over 100 km/h1906: Fred Marriott, Stanley Rocket steam car19061927: Henry Segrave, Sunbeam 1000 hp19271935: Malcolm Campbell, Blue Bird19351947: John Cobb, Railton Mobil Special19471965: Craig Breedlove, Spirit of America – Sonic 119651970: Gary Gabelich, Blue Flame rocket car1983: Richard Noble, Thrust219831997: Andy Green, ThrustSSC: faster than sound1997
  1. 1898 Chasseloup-Laubat, Jeantaud electric car
  2. 1899 Jenatzy, La Jamais Contente: first over 100 km/h
  3. 1906 Fred Marriott, Stanley Rocket steam car
  4. 1927 Henry Segrave, Sunbeam 1000 hp
  5. 1935 Malcolm Campbell, Blue Bird
  6. 1947 John Cobb, Railton Mobil Special
  7. 1965 Craig Breedlove, Spirit of America – Sonic 1
  8. 1970 Gary Gabelich, Blue Flame rocket car
  9. 1983 Richard Noble, Thrust2
  10. 1997 Andy Green, ThrustSSC: faster than sound

1900 – today

Limits and satellites

Einstein sets the ultimate speed limit, the Moon settles the falling myth, and satellites measure velocity everywhere.

1905

30 June 1905 (received)

Nothing catches light

Albert EinsteinBern, Switzerland

In 'On the Electrodynamics of Moving Bodies' Einstein showed that the speed of light is the same for every observer. Velocities then combine as (u + v) ÷ (1 + uv/c²), so nothing with mass can reach c.

Why it mattered. Simple adding of velocities is only an everyday approximation.

1971

2 August 1971

A hammer and a feather on the Moon

David Scott, Apollo 15Hadley Rille, the Moon

Standing on the airless Moon, astronaut David Scott dropped a hammer and a falcon feather together, live on television. They hit the ground at the same moment, as Galileo had said.

Why it mattered. Without air, heavy and light things fall together.

1995

1995–2000

Speed from satellites

US Department of Defense; opened to allWorldwide

The Global Positioning System reached full operation in 1995, and in May 2000 its deliberate degradation for civilian users was switched off. Receivers work out speed from the Doppler shift of satellite signals, which is how phones and sat-navs know yours to a fraction of a km/h.

Why it mattered. Anyone can now measure velocity, with direction, anywhere on Earth.

Did you know?

Since 1983 the metre has been defined by light: the distance light travels in 1/299,792,458 of a second. So the speed of light is exactly 299,792,458 m/s.

1 m/s is exactly 3.6 km/h, because an hour has 3,600 seconds and a kilometre 1,000 metres.

By international rules a car's speedometer may read up to 10% plus 4 km/h too high, but never too low.

The first car to go faster than 100 km/h, in 1899, was electric.

Standing still on the equator, you are moving at about 1,670 km/h as the Earth turns.

The people

Who figured it out

Aristotle

384 – 322 BCE · Philosopher · Greece

His rule that heavier things fall faster lasted nearly two thousand years.

William Heytesbury

c. 1313 – 1372/73 · Logician, Merton College · England

Stated the mean speed rule for uniformly changing motion.

Nicole Oresme

c. 1320 – 1382 · Philosopher and bishop · France

Drew speed against time and read distance from the area.

Galileo Galilei

1564 – 1642 · Physicist and astronomer · Italy

Measured rolling balls, defined uniform acceleration and showed all bodies fall alike without air.

Isaac Newton

1643 – 1727 · Mathematician and physicist · England

Made acceleration the link between force and motion.

Albert Einstein

1879 – 1955 · Physicist · Germany and Switzerland

Showed that velocities do not simply add and that nothing with mass reaches light speed.

Where it happened

12 places, one idea

Sources

Where this comes from

Dates marked “c.” are approximate, and historians sometimes disagree about who was first. If you spot a mistake, tell us.

  1. Aristotle's Physics Stanford Encyclopedia of Philosophy
  2. John Philoponus Stanford Encyclopedia of Philosophy
  3. Oxford Calculators Wikipedia
  4. Mean speed theorem Wikipedia
  5. Nicole Oresme Stanford Encyclopedia of Philosophy
  6. Simon Stevin Wikipedia
  7. Galileo's law of free fall and the 1604 letter to Sarpi Wikipedia
  8. Two New Sciences Wikipedia
  9. Galileo Galilei Encyclopaedia Britannica
  10. Principles of Philosophy (Descartes, 1644) Wikipedia
  11. Horologium Oscillatorium Wikipedia
  12. Rømer's determination of the speed of light Wikipedia
  13. History of calculus: Leibniz, Nova methodus (1684) Wikipedia
  14. Philosophiæ Naturalis Principia Mathematica Wikipedia
  15. Newton's Principia, first edition Cambridge Digital Library
  16. Walter Arnold, first speeding conviction Wikipedia
  17. La Jamais Contente Wikipedia
  18. Speedometer Wikipedia
  19. On the Electrodynamics of Moving Bodies (1905) Wikipedia
  20. Velocity-addition formula Wikipedia
  21. Radar speed gun Wikipedia
  22. The Apollo 15 Hammer-Feather Drop NASA NSSDCA
  23. GPS: Selective Availability GPS.gov (US government)
  24. Global Positioning System Wikipedia
  25. Land speed record Wikipedia
  26. SI base unit: the metre BIPM
  27. Road traffic injuries fact sheet World Health Organization
  28. Speed of light Wikipedia

That's the history. Now see how it works.