The history

The history of combustion and conservation of mass

From a million-year-old campfire to the Keeling Curve: how people learned that burning destroys nothing.

People used fire for a million years before anyone knew what it was. For most of the 1700s chemists believed burning released a fire substance called phlogiston. Then scientists started weighing everything, in sealed vessels, and found the opposite: burning takes in part of the air, and not a speck of matter is lost.

1,002,000+
years
20
moments
7
people
12
places

c. 1 million years ago

Secure evidence of fire inside a cave

Wonderwerk Cave, South Africa

1703

First big theory of burning

Georg Ernst Stahl's phlogiston, Prussia

1754

Carbon dioxide identified

Joseph Black, Edinburgh

1771–1772

Oxygen first made

Carl Wilhelm Scheele, Sweden (Priestley independently in 1774)

1756 and 1774

Mass conserved in sealed vessels

Mikhail Lomonosov, St Petersburg; Antoine Lavoisier, Paris

1789

Conservation of mass in a textbook

Antoine and Marie-Anne Lavoisier, Paris

1958

Continuous record of CO₂ in the air

Charles David Keeling, Mauna Loa

c. 1 million years agoFire before chemistry

1000000 BCE – 1600

Fire before chemistry

Early humans learn to keep and use fire long before anyone can say what a flame is.

1000000 BCE

c. 1 million years ago

Ash deep inside a cave

Early humans, probably Homo erectusWonderwerk Cave, Northern Cape

Deep inside Wonderwerk Cave, far from the entrance, scientists found ash from burnt plants and bits of burnt bone in layers about a million years old. Tiny cracks and colours in the bone show it was heated where it lay. It is among the oldest secure signs of people using fire, though some researchers argue for older ones.

Why it mattered. Fire gave early humans warmth, light, safety and cooked food, the first chemistry anyone ever controlled.

500000 BCE

c. 400,000–700,000 years ago (disputed)

Fire at the Peking Man cave?

Homo erectus ("Peking Man"); dug up from the 1920sZhoukoudian, near Beijing

Burnt bones and thick dark layers in the Zhoukoudian caves were long taken as the hearths of Peking Man. A careful study in 1998 found burnt bone but no clear ash or hearths, so whether these people kept fires there is still argued about.

Why it mattered. It shows how hard it is to prove who first tamed fire, and why old claims need testing.

1600 – 1770

Fire as a substance

Chemists explain burning with phlogiston, a fire stuff that escapes in the flame, while careful weighing starts to turn up awkward facts.

1673

Metals that get heavier in the fire

Robert BoyleLondon

Boyle heated lead and tin in sealed glass vessels. When he opened them and weighed the metal's ash, called a calx, it was heavier than the metal. He guessed that particles of fire had passed through the glass and stuck to it.

Why it mattered. A real clue, misread: he opened the vessel before weighing, so air rushed in and the extra weight was really oxygen.

1703

Phlogiston: fire as a substance

Georg Ernst StahlHalle

Building on Johann Becher's ideas, Stahl taught that everything that burns holds a fire substance, phlogiston, which escapes in the flame. Charcoal was almost pure phlogiston; a metal was its calx plus phlogiston. The idea explained a lot and ruled chemistry for most of the century.

Why it mattered. It was the first big theory of burning, and it was wrong in a way that pushed chemists to start weighing things.

1754

1754 (thesis); published 1756

Fixed air: carbon dioxide is found

Joseph BlackUniversity of Edinburgh

Black heated magnesia alba and chalk and weighed them. They lost weight by giving off a gas he called fixed air, the gas we call carbon dioxide. He later found it in the breath and in the gases from burning charcoal.

Why it mattered. Careful weighing showed that a gas could be part of a solid, and gave chemists the first product of burning.

1756

Lomonosov's sealed flasks

Mikhail LomonosovSt Petersburg

Lomonosov repeated Boyle's test but kept the flasks sealed. Heating metal inside them did not change the total weight; only letting air in did. He had already written to Leonhard Euler in 1748 that matter lost in one place is gained in another. His results were recorded in his notes and were little known in Western Europe.

Why it mattered. He reached the conservation of mass years before Lavoisier, though historians still debate how complete his proof was.

1770 – 1800

The oxygen revolution

Oxygen is found three times over, and the Lavoisiers show with sealed vessels and balances that burning is joining with it and that mass is conserved.

1771

1771–1772 (published 1777)

Scheele makes "fire air"

Carl Wilhelm ScheeleUppsala

Scheele, a pharmacist, heated mercury oxide, saltpetre and other substances and collected a gas that made things burn fiercely. He called it fire air. His book describing it was held up at the printer until 1777, so others were credited first.

Why it mattered. He was probably the first to make oxygen, a reminder that discoveries often happen twice.

1774

1 August 1774

Priestley's candle burns brighter

Joseph PriestleyBowood House, Wiltshire

Priestley focused sunlight with a large lens onto red mercury calx. A gas came off in which a candle burned with a dazzling flame and a mouse lived longer than in ordinary air. He called it dephlogisticated air and told Lavoisier about it in Paris that October.

Why it mattered. Priestley found oxygen but kept the phlogiston theory; Lavoisier saw what it really meant.

1774

Tin in a sealed retort

Antoine LavoisierParis

Lavoisier heated tin in sealed glass vessels and weighed everything before and after. The total did not change. When he broke the seal, air rushed in, and the weight rose by exactly what the tin had gained.

Why it mattered. The metal was taking something out of the air, not losing phlogiston: the key experiment behind this box's first chapter.

1777

1777 (published 1780)

A new theory of burning

Antoine LavoisierParis

In a paper on combustion in general, Lavoisier argued that burning, rusting and breathing are all a substance joining with part of the air. He named that part oxygène, "acid maker", because he wrongly thought all acids contained it.

Why it mattered. It replaced phlogiston with the idea we still use: burning is joining with oxygen.

1783

1782–1783

Breathing is slow burning

Antoine Lavoisier and Pierre-Simon LaplaceParis

Lavoisier and Laplace put a guinea pig in an ice calorimeter and measured the heat it gave out and the fixed air it breathed out. Burning charcoal to make the same amount of that gas gave nearly the same heat. Breathing, they concluded, is a slow combustion.

Why it mattered. It linked the flame and the body, the idea behind this box's chapter on fat and breath.

1788

Marie-Anne Lavoisier answers the phlogistonists

Marie-Anne Paulze LavoisierParis

Marie-Anne Lavoisier translated Richard Kirwan's Essay on Phlogiston from English into French, adding notes that took its arguments apart. She kept the laboratory's records, took part in experiments and hosted scientists from across Europe.

Why it mattered. Her work spread the new chemistry, though she was rarely credited in her lifetime.

1789

The law in a textbook

Antoine Lavoisier, with drawings by Marie-Anne LavoisierParis

Lavoisier's Traité élémentaire de chimie stated that nothing is created in any operation, of art or of nature: the same quantity of matter exists before and after. It listed 33 elements and used a new, logical naming system. Marie-Anne drew its 13 plates of apparatus. Five years later Lavoisier was guillotined in the Revolution.

Why it mattered. It is often called the first modern chemistry textbook, and it made conservation of mass the ground rule of chemistry.

1800 – today

Flames at work, and their cost

Safety lamps, candle lectures and engines put combustion to work, and measurements show where all that carbon goes.

1815

A flame that can't escape

Humphry DavyRoyal Institution, London

Coal mines were full of firedamp, methane, which exploded when miners' candles lit it. Davy wrapped the flame in fine iron gauze. The gauze soaks up heat so fast that flame can't pass through it to the gas outside.

Why it mattered. It saved many lives, and showed that a flame needs heat as well as fuel and oxygen.

1848

1848; published 1861

The Chemical History of a Candle

Michael FaradayRoyal Institution, London

In Christmas lectures for young people, Faraday burned candles and caught what came off. He showed that the wax turns into water and carbon dioxide, using oxygen from the air, and that we do the same when we breathe. He gave the lectures again in 1860, and they became a famous book.

Why it mattered. It is still one of the best explanations of combustion ever written for young people.

1876

The four-stroke engine

Nikolaus OttoDeutz, near Cologne

Otto built an engine that sucked in fuel and air, squeezed it, burned it and pushed out the exhaust, in four strokes of the piston. Squeezing the mixture before lighting it made it far more efficient than earlier gas engines.

Why it mattered. Nearly every petrol car and motorbike engine still works this way.

1905

Energy has mass

Albert EinsteinBern

In a short paper, Einstein showed that anything that gives out energy E loses mass E ÷ c². For burning, the loss is about one part in ten billion, far too small to weigh.

Why it mattered. It is the one tiny exception to Lavoisier's law, and it matters only in nuclear reactions.

1958

March 1958

Measuring the CO₂ we make

Charles David KeelingMauna Loa Observatory, Hawaii

Keeling began measuring carbon dioxide in the air with great precision, high on a Hawaiian volcano. His record, the Keeling Curve, rises every year, with a small wobble as plants grow and die with the seasons.

Why it mattered. It shows the conservation of mass on a planetary scale: the carbon we burn does not vanish, it stays in the air.

1975

Catalytic converters arrive

Carmakers, under the US Clean Air ActUnited States

From the 1975 models, most new petrol cars in the US got catalytic converters to meet new limits on carbon monoxide and unburnt fuel. They needed unleaded petrol, because lead ruins the catalyst. Three-way converters that also clean NOx followed a few years later.

Why it mattered. They cut the poisons from incomplete burning, though every gram of fuel carbon still leaves as CO₂.

2014

December 2014

Where does lost fat go?

Ruben Meerman and Andrew BrownUniversity of New South Wales, Sydney

Meerman, a physicist, and Brown, a chemist, followed every atom in 10 kg of body fat as it is burned. They found that 8.4 kg leaves as carbon dioxide through the lungs and 1.6 kg as water. Many doctors and trainers they surveyed had guessed it turned into energy or heat.

Why it mattered. It is Lavoisier's law applied to your own body: mass lost has to go somewhere.

By the numbers

Carbon dioxide in the air at Mauna Loa, Hawaii

Every tonne of carbon we burn leaves as about 3.7 tonnes of CO₂, and much of it stays in the air. Data: NOAA Global Monitoring Laboratory.

300 parts per million (yearly average)350 parts per million (yearly average)400 parts per million (yearly average)450 parts per million (yearly average) 1960197019801990200020102020 1959: First full year of measurements19591970: 197019701980: 198019801990: 199019902000: 200020002010: 201020102020: 202020202025: 20252025
  1. 1959 First full year of measurements
  2. 1970 1970
  3. 1980 1980
  4. 1990 1990
  5. 2000 2000
  6. 2010 2010
  7. 2020 2020
  8. 2025 2025

Did you know?

Burning 1 kg of carbon makes 3.67 kg of carbon dioxide, because each carbon atom picks up two oxygen atoms from the air.

Priestley told Lavoisier about his new gas over dinner in Paris in October 1774. Lavoisier understood it better than Priestley did.

Antoine Lavoisier was also a tax collector for the king. That job, not his chemistry, got him guillotined in 1794, during the French Revolution.

Most of the mass you lose when you slim down leaves through your lungs, as carbon dioxide.

Einstein's E = mc² means a burning fuel does lose mass, but only about one part in ten billion: no balance has ever seen it.

The people

Who figured it out

Antoine Lavoisier

1743 – 1794 · Chemist and tax official · France

Weighed everything, named oxygen and hydrogen, and made conservation of mass the ground rule of chemistry.

Marie-Anne Paulze Lavoisier

1758 – 1836 · Chemist, translator and illustrator · France

Worked beside Antoine in the lab, translated and rebutted the phlogistonists, and drew the plates of his Traité.

Mikhail Lomonosov

1711 – 1765 · Scientist, poet and founder of Moscow University · Russia

Showed in 1756 that metals heated in sealed flasks don't change the total weight.

Joseph Priestley

1733 – 1804 · Minister and chemist · England

Discovered oxygen in 1774 but defended phlogiston to the end of his life.

Carl Wilhelm Scheele

1742 – 1786 · Pharmacist and chemist · Sweden

Made oxygen first, around 1771–72, but his book came out too late for the credit.

Joseph Black

1728 – 1799 · Physician and chemist · Scotland (born in France)

Found fixed air, carbon dioxide, by weighing what solids lose when heated.

Michael Faraday

1791 – 1867 · Chemist and physicist · England

Explained a burning candle to children so well that his lectures are still in print.

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. Control of fire by early humans Wikipedia
  2. Microstratigraphic evidence of in situ fire in the Acheulean strata of Wonderwerk Cave (Berna et al., 2012) PNAS
  3. Wonderwerk Cave Wikipedia
  4. Evidence for the use of fire at Zhoukoudian, China (Weiner et al., 1998) Science
  5. Phlogiston theory Wikipedia
  6. Georg Ernst Stahl Encyclopaedia Britannica
  7. Joseph Black Encyclopaedia Britannica
  8. Mikhail Lomonosov and the dawn of Russian science Physics Today
  9. Reflections on the nature of genius: on the 300th anniversary of Mikhail Lomonosov (Shiltsev) arXiv
  10. Joseph Priestley and the discovery of oxygen American Chemical Society, National Historic Chemical Landmarks
  11. Carl Wilhelm Scheele Encyclopaedia Britannica
  12. Antoine-Laurent Lavoisier: the Chemical Revolution American Chemical Society, National Historic Chemical Landmarks
  13. Antoine Lavoisier Wikipedia
  14. Marie-Anne Paulze Lavoisier Wikipedia
  15. Traité élémentaire de chimie Wikipedia
  16. Conservation of mass Wikipedia
  17. Davy lamp Wikipedia
  18. The Chemical History of a Candle Wikipedia
  19. Nikolaus August Otto Encyclopaedia Britannica
  20. The Keeling Curve Scripps Institution of Oceanography, UC San Diego
  21. Mauna Loa CO2 annual mean data NOAA Global Monitoring Laboratory
  22. Catalytic converter Wikipedia
  23. When somebody loses weight, where does the fat go? (Meerman and Brown, 2014) BMJ
  24. Robert Boyle Encyclopaedia Britannica
  25. Antoine Lavoisier Encyclopaedia Britannica
  26. Mass–energy equivalence Wikipedia
  27. Greenhouse gas emissions from a typical passenger vehicle US Environmental Protection Agency
  28. Joseph Priestley Encyclopaedia Britannica
  29. Michael Faraday Royal Institution

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