The history

The history of the gas laws

From a tube of mercury in Florence to a number fixed forever in 2019: 400 years of learning how gases push, stretch and move.

People once thought air had no weight at all. Then glass tubes, mercury and balloons showed that a gas pushes back when you squeeze it, swells when you heat it, and does both in the same way whatever it is made of. In the end all the rules fitted into one short equation, PV = nRT, and scientists found out why: a gas is a crowd of molecules hitting the walls.

376
years
20
moments
12
people
10
places

1643

Lasting vacuum made in a lab

Evangelista Torricelli, Florence, Italy

1662

Law linking pressure and volume

Robert Boyle and Robert Hooke, Oxford, England

21 November 1783

People fly (hot-air balloon)

Pilâtre de Rozier and the Marquis d'Arlandes, Paris

1 December 1783

Crewed hydrogen balloon flight

Jacques Charles and Nicolas-Louis Robert, Paris

1834

Gas law in one equation

Émile Clapeyron, Paris, France

1860

First law of physics based on chance

James Clerk Maxwell, Aberdeen, Scotland

1874

One gas constant for every gas

Dmitri Mendeleev, St Petersburg (Horstmann in 1873)

1910

Nobel Prize for a gas equation

Johannes Diderik van der Waals, Netherlands

1643 (tested on a mountain in 1648)The weight and spring of air

1643 – 1738

The weight and spring of air

Mercury tubes prove air has weight, Boyle finds that squeezed air pushes back, and the first thinkers link pressure to heat and to tiny moving particles.

1643

1643 (tested on a mountain in 1648)

A sea of air with weight

Evangelista Torricelli; later Blaise Pascal and Florin PérierFlorence, Grand Duchy of Tuscany

Torricelli filled a glass tube with mercury and turned it upside down in a bowl. The mercury fell to about 76 cm and stopped, leaving empty space above it. The weight of the air outside was holding it up. In 1648 Pascal's brother-in-law carried the same tube up the Puy de Dôme in France, and the mercury stood lower at the top.

Why it mattered. It proved that air has weight and pushes on everything, which is what pressure means.

1662

Squeeze the air and it pushes back harder

Robert Boyle, with Robert Hooke; helped by Richard Towneley and Henry PowerOxford, England

Boyle trapped air in the short, closed end of a J-shaped glass tube and poured mercury into the long end. Every time he doubled the push, the trapped air shrank to half its size. Towneley and Power had spotted the same pattern, and Boyle printed the result in the second edition of his book on the "spring of the air".

Why it mattered. It was one of the first laws of nature written as a rule linking two measured numbers: pressure times volume stays the same.

1676

The same law, found again in France

Edme MariotteParis, France

Mariotte, a French priest and scientist, found the same rule on his own and wrote it up in his Discourse on the Nature of Air. He added an important warning: it only works if the temperature does not change. In the same book he coined the word "barometer".

Why it mattered. His warning about temperature pointed the way to the next gas laws.

1702

Heat the air and its push grows

Guillaume AmontonsParis, France

Amontons, who had been mostly deaf since boyhood, built a thermometer that read temperature from the pressure of trapped air. He saw that equal drops in temperature gave equal drops in pressure. If you kept cooling, the pressure would one day reach nothing, which he put at about minus 240 °C.

Why it mattered. It was the first hint that there is a coldest possible temperature, absolute zero.

1738

Pressure is tiny particles hitting the walls

Daniel BernoulliBasel, Switzerland (book printed in Strasbourg)

In his book Hydrodynamica, Bernoulli pictured air as countless tiny particles flying in all directions. Their hits on the walls of a container make the pressure, and faster particles mean a hotter gas. He even showed why this gives Boyle's law.

Why it mattered. It was the first kinetic theory of gases, more than a hundred years before most scientists accepted it.

1783 – 1802

Balloons and heat

Paris goes balloon mad, and the scientists who fly them discover that every gas grows by the same amount when heated.

1783

21 November 1783

People fly for the first time, on hot air

Joseph-Michel and Jacques-Étienne Montgolfier; flown by Jean-François Pilâtre de Rozier and the Marquis d'ArlandesParis, France

The Montgolfier brothers, paper makers from Annonay, built a huge cloth and paper balloon and filled it from a fire. Pilâtre de Rozier and d'Arlandes rode it about 9 km across Paris in some 25 minutes. The brothers thought smoke held a special gas with "levity". In fact, heated air simply spreads out, so the balloon holds less of it and is lighter than the cold air around it.

Why it mattered. It was the first time people flew freely, and it made the link between heat and gas volume impossible to ignore.

1783

27 August and 1 December 1783

The hydrogen balloon, and a village fights back

Jacques Charles and Nicolas-Louis RobertParis, France

Charles filled a silk balloon with hydrogen made from iron and acid. His first, unmanned balloon came down in the village of Gonesse, where frightened villagers attacked it with pitchforks. On 1 December, Charles and Robert flew in a hydrogen balloon themselves for about two hours, watched by a huge crowd.

Why it mattered. Gas balloons turned the study of gases into something the whole of Paris cared about.

1787

c. 1787 (never published)

Every gas grows by the same amount

Jacques CharlesParis, France

Charles is said to have filled balloons with different gases and warmed them all by the same amount. Each one grew by the same fraction of its size. He never wrote it up, so we only know about it because another scientist gave him the credit later.

Why it mattered. It suggested that all gases follow one rule for heat, whatever they are made of.

1801

1801 (published 1802)

Each gas in a mix pushes on its own

John DaltonManchester, England

Dalton, a teacher who was fascinated by weather, studied how water vapour mixes into air. He found that in a mixture of gases, each gas pushes as if the others were not there. The total pressure is just the sum of the parts. The same year he showed that different gases expand alike when heated.

Why it mattered. It is why divers and doctors can work out how much oxygen is in each breath.

1802

31 January 1802

Charles's law goes public, with credit

Joseph Louis Gay-LussacParis, France

Gay-Lussac measured carefully how gases grow when heated at a steady pressure. He found they all grow by about 1/267 of their size at 0 °C for every degree. He also said that Charles had found this about 15 years earlier, which is why we call it Charles's law.

Why it mattered. The number 267 hid a secret: cool a gas to about minus 267 °C and its volume would, in theory, shrink to nothing.

1811 – 1874

One law for every gas

Avogadro's idea lets gases be counted, Clapeyron joins the rules into one equation, and Mendeleev gives it one constant, R.

1811

1811 (revived at Karlsruhe in 1860)

Equal volumes hold equal numbers

Amedeo Avogadro; later championed by Stanislao CannizzaroTurin, Kingdom of Sardinia (published in Paris)

Gay-Lussac had noticed in 1808 that gases react in simple volumes, like two litres of hydrogen to one of oxygen. Avogadro explained it with a bold guess: equal volumes of any gas, at the same temperature and pressure, hold the same number of particles. Almost nobody listened until Cannizzaro handed out a pamphlet at a big chemistry meeting in Karlsruhe, Germany, in 1860.

Why it mattered. It is the n in PV = nRT: it lets you count particles by measuring a gas.

1834

One equation for every gas

Émile ClapeyronParis, France

Clapeyron, an engineer who had taught in St Petersburg and built early French railways, was explaining Sadi Carnot's ideas about steam engines. To do it, he joined Boyle's law and Gay-Lussac's law into one equation, pv = R(267 + t), and drew engine cycles as loops on a pressure against volume graph. That graph is still used for every engine today.

Why it mattered. It is the ideal gas law almost as we write it now.

1874

One constant for all gases

Dmitri Mendeleev (and August Horstmann in 1873)St Petersburg, Russia

Earlier versions of the gas law used a different constant for each gas. Mendeleev, famous for the periodic table, used Avogadro's idea to write the law for a mole of any gas as pV = RT, with one shared R. His value was within about 0.3% of today's. In Russia the ideal gas law is still called the Clapeyron–Mendeleev equation.

Why it mattered. The single R is what makes PV = nRT work for every gas.

By the numbers

Where is the coldest cold? Absolute zero worked out from gases

Each estimate comes from asking at what temperature a gas would push or fill nothing. Better measurements closed in on minus 273.15 °C.

-280 °C-270 °C-260 °C-250 °C-240 °C 17501800185019001950 1702: Guillaume Amontons, from his air thermometer: about −240 °C17021779: Johann Heinrich Lambert: about −270 °C17791802: Gay-Lussac's expansion of 1/266.66 per degree points to about −267 °C18021834: Clapeyron writes pv = R(267 + t)18341848: William Thomson (Lord Kelvin): absolute scale starting at −273 °C1954: Water's triple point fixed at 273.16 K, putting absolute zero at −273.15 °C1954
  1. 1702 Guillaume Amontons, from his air thermometer: about −240 °C
  2. 1779 Johann Heinrich Lambert: about −270 °C
  3. 1802 Gay-Lussac's expansion of 1/266.66 per degree points to about −267 °C
  4. 1834 Clapeyron writes pv = R(267 + t)
  5. 1848 William Thomson (Lord Kelvin): absolute scale starting at −273 °C
  6. 1954 Water's triple point fixed at 273.16 K, putting absolute zero at −273.15 °C

1845 – 1872

Molecules in motion

The gas laws are explained at last: pressure and temperature come from molecules racing about at a spread of speeds.

1845

1845 (printed 1892)

A paper from Bombay called nonsense

John James WaterstonBombay, British India

Waterston, a Scot teaching naval cadets for the East India Company in Bombay, worked out a detailed theory of gases made of moving molecules. He sent it to the Royal Society in London, and a referee wrote that it was "nothing but nonsense". It sat in the archive until Lord Rayleigh found and printed it in 1892, nine years after Waterston died.

Why it mattered. His ideas were right, and the story is still told as a warning about ignoring outsiders.

1857

Heat is molecules on the move

Rudolf Clausius (and August Krönig in 1856)Zürich, Switzerland

A year after August Krönig in Berlin, Clausius published a fuller theory of gases as molecules racing about and bumping into things. He showed how their speed sets the pressure and the temperature, and later worked out how far a molecule travels between bumps. Together they turned Bernoulli's old picture into real physics.

Why it mattered. It explained where PV = nRT comes from: it is just molecules hitting walls.

1860

1859 talk, 1860 paper

Not every molecule moves at the same speed

James Clerk Maxwell, then Ludwig BoltzmannAberdeen, Scotland

Maxwell realised the molecules in a gas have a spread of speeds, a few slow, most in the middle, a few very fast. He worked out the shape of that spread, and it was the first law of physics based on chance. In 1872 Boltzmann in Graz showed why any gas settles into exactly this spread.

Why it mattered. It showed that a gas law is really the average behaviour of trillions of molecules.

1869 – 2019

Real gases and exact numbers

Real gases turn out to bend the rules, van der Waals fixes the law, balloons return, and R becomes an exact number.

1869

Where gas and liquid become one

Thomas AndrewsBelfast, Ireland

Andrews squeezed carbon dioxide at different temperatures. Below about 31 °C, squeezing turned it into a liquid. Above that temperature, no amount of squeezing made a liquid at all. He called this the critical point and described it in the Royal Society's Bakerian Lecture.

Why it mattered. It showed real gases break the ideal gas law, and explained how to turn gases into liquids by cooling them first.

1873

14 June 1873 (Nobel Prize 1910)

A law for real gases

Johannes Diderik van der WaalsLeiden, Netherlands

Van der Waals, a former schoolteacher, fixed the ideal gas law in his PhD thesis. He added two corrections: molecules take up some space, and they pull on each other a little. His equation described gases and liquids together, and Maxwell praised it in the journal Nature.

Why it mattered. It won him the 1910 Nobel Prize in Physics and is still the first step past PV = nRT.

1960

22 October 1960

Hot-air balloons come back

Ed YostBruning, Nebraska

Yost flew the first modern hot-air balloon, with a plastic envelope and a propane burner he designed. The burner heats the air inside, the air expands, some spills out, and the balloon gets lighter. It flew for about 25 minutes. Almost every hot-air balloon today uses his design.

Why it mattered. It is Charles's law you can ride in.

2019

20 May 2019

R becomes exact

General Conference on Weights and Measures (CGPM)Versailles, France (vote in November 2018)

The world's measurement scientists fixed the Boltzmann constant and the Avogadro constant at exact values. Since R is simply one times the other, the gas constant became exact too: 8.31446261815324 joules per mole per kelvin. The kelvin itself is now defined through the Boltzmann constant.

Why it mattered. The constant in PV = nRT is now a fixed part of how the world defines temperature and amount.

Did you know?

Boyle called air's push its "spring", because squeezed air pushes back like a squashed spring.

In France, Boyle's law is usually called Mariotte's law, after Edme Mariotte.

Jacques Charles never published Charles's law. We only know because Gay-Lussac gave him the credit in 1802.

The first hydrogen balloon was attacked with pitchforks by villagers in Gonesse, and the French government then had to tell people that balloons were not monsters.

The Montgolfier brothers thought smoke contained a special lifting gas. It was really just hot air.

The law that pressure rises with temperature is often named after Gay-Lussac, but Amontons found it about a century earlier.

R is simply the Avogadro constant times the Boltzmann constant. Since 2019 both are exact, so R is exactly 8.31446261815324 J/(mol·K).

John Dalton once settled on minus 3,000 °C as the coldest possible temperature, more than ten times too cold.

The people

Who figured it out

Robert Boyle

1627 – 1691 · Natural philosopher and chemist · Ireland

Showed that squeezing air makes it push back harder, in exact proportion.

Robert Hooke

1635 – 1703 · Experimenter and inventor · England

Built the air pumps and glassware behind Boyle's experiments.

Edme Mariotte

c. 1620 – 1684 · Priest and physicist · France

Found Boyle's law on his own and warned it only holds at one temperature.

Guillaume Amontons

1663 – 1705 · Physicist and instrument maker · France

Mostly deaf from boyhood, he first guessed at a coldest possible temperature.

Jacques Charles

1746 – 1823 · Physicist and balloonist · France

Flew the first crewed hydrogen balloon and found, but never published, Charles's law.

John Dalton

1766 – 1844 · Teacher, chemist and weather watcher · England

Showed each gas in a mixture pushes as if it were alone.

Joseph Louis Gay-Lussac

1778 – 1850 · Chemist and physicist · France

Measured how gases expand, credited Charles, and rose to about 7,000 m in a balloon in 1804.

Amedeo Avogadro

1776 – 1856 · Physicist and lawyer · Italy

Guessed that equal volumes of gas hold equal numbers of particles.

Émile Clapeyron

1799 – 1864 · Engineer · France

Wrote the gas laws as one equation and drew engines as pressure and volume loops.

John James Waterston

1811 – 1883 · Naval instructor and physicist · Scotland (worked in Bombay, India)

Wrote a correct kinetic theory of gases that was rejected as nonsense.

James Clerk Maxwell

1831 – 1879 · Physicist · Scotland

Worked out the spread of speeds of molecules in a gas.

Johannes Diderik van der Waals

1837 – 1923 · Physicist, once a schoolteacher · Netherlands

Fixed the gas law for real molecules that take up space and attract.

Where it happened

10 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. Gas laws Wikipedia
  2. Boyle's law Wikipedia
  3. Robert Boyle, Irish natural philosopher (Scientist of the Day) Linda Hall Library
  4. Discours de la nature de l'air (work by Mariotte) Encyclopaedia Britannica
  5. Edme Mariotte Encyclopaedia Britannica
  6. Evangelista Torricelli Wikipedia
  7. Blaise Pascal Stanford Encyclopedia of Philosophy
  8. Guillaume Amontons Encyclopaedia Britannica
  9. Guillaume Amontons Wikipedia
  10. Montgolfier brothers Wikipedia
  11. Allarme Générale des Habitants de Gonesse (print, 1783) Smithsonian National Air and Space Museum
  12. Jacques Charles Wikipedia
  13. Charles's law Wikipedia
  14. Dalton's law Wikipedia
  15. Joseph Louis Gay-Lussac Wikipedia
  16. Avogadro's law Wikipedia
  17. Stanislao Cannizzaro Wikipedia
  18. Benoît Paul Émile Clapeyron Wikipedia
  19. Why is the universal gas constant represented by R? (Ask the Historian, J. Chem. Educ.) William B. Jensen, University of Cincinnati
  20. Kinetic theory of gases Wikipedia
  21. John James Waterston Wikipedia
  22. Maxwell–Boltzmann distribution Wikipedia
  23. Ideal gas law Wikipedia
  24. Gas constant Wikipedia
  25. Thomas Andrews (scientist) Wikipedia
  26. The Bakerian Lecture: On the continuity of the gaseous and liquid states of matter (1869) Philosophical Transactions of the Royal Society
  27. Johannes Diderik van der Waals Wikipedia
  28. The Nobel Prize in Physics 1910 NobelPrize.org
  29. 2019 revision of the SI Wikipedia
  30. SI defining constants BIPM
  31. Ed Yost Wikipedia
  32. Absolute zero Wikipedia
  33. Kelvin Wikipedia
  34. Hydrodynamica Wikipedia
  35. Robert Hooke, English polymath (Scientist of the Day) Linda Hall Library

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