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Field · Emerged 1738 – 1908

Kinetic Theory of Gases

Can pressure, temperature and heat be explained as the motion of countless invisible molecules?

5 chapters4 min read6 turning points0 open problems

Branched from
Thermodynamics + Classical Mechanics
Branched into
Statistical Mechanics
Figures
Daniel Bernoulli, Rudolf Clausius, James Clerk Maxwell, Katherine Clerk Maxwell, Ludwig Boltzmann, Josef Loschmidt, Albert Einstein, Jean Perrin

In brief

Kinetic theory explains the behaviour of gases from the motion of the molecules they are made of. Pressure is the drumming of molecules on a container's walls. Temperature measures their average energy of motion. Heat is that motion passed from molecule to molecule. With Newton's laws and some statistics, the gas laws, viscosity, diffusion and heat conduction all follow.

The idea was proposed in 1738 and ignored for a century, because the existence of atoms was unproven and many scientists thought it unprovable. Clausius, Maxwell and Boltzmann developed it into a precise theory between 1857 and 1872. Its reliance on probability, and on atoms, remained controversial until 1908, when Jean Perrin's measurements of Brownian motion convinced almost everyone that molecules are real.

Key ideas

Pressure from collisionsEnters 1738

The pressure of a gas is the average force of molecules bouncing off a surface. Doubling the number of molecules in a box doubles the pressure.

Temperature as motionEnters 1857 – 1858

Absolute temperature is proportional to the average kinetic energy of the molecules. At room temperature, air molecules move at about 500 metres per second.

Mean free pathEnters 1857 – 1858

The average distance a molecule travels between collisions, about 70 nanometres in air. It explains why gases mix slowly although their molecules move fast.

Maxwell–Boltzmann distributionEnters 1860

Molecular speeds are not all equal but spread out in a definite pattern set by the temperature. It was the first law of physics stated as a probability distribution.

H-theoremEnters 1872

Boltzmann's proof that collisions drive any gas towards Maxwell's distribution, with a quantity that always decreases, his mechanical version of entropy's increase.

Draws on other domains

Chapter I

Particles in Motion

In 1738 Daniel Bernoulli proposed that air is made of tiny particles flying in all directions, and that its pressure is their impacts on the walls of the container. From this he derived Boyle's law: squeeze a gas into half the volume and the particles hit the walls twice as often. The idea fitted nothing else known at the time. Heat was thought to be a fluid, and atoms were speculation. It was forgotten for over a hundred years.

Chapter II

Speeds and Collisions

After thermodynamics established that heat is energy, the idea returned. In 1857 Rudolf Clausius calculated from measured pressures that air molecules must travel at hundreds of metres per second. The Dutch meteorologist Buys Ballot raised an obvious objection: then a smell released across a room should arrive instantly, yet it takes minutes. Clausius answered with the mean free path. Molecules are so crowded that each collides billions of times a second, and its path is a random zigzag that makes little progress.

In 1860 James Clerk Maxwell took a decisive step. The molecules do not all move at the same speed. Their speeds are spread out in a pattern fixed by the temperature, the first law of physics expressed as a probability distribution. From it he predicted that a gas's viscosity should be the same at any pressure, which seemed absurd. In 1866 he and Katherine Maxwell, whose role in the experiments he acknowledged, measured it in their attic. The prediction held.

Chapter III

Boltzmann and the Second Law

Ludwig Boltzmann wanted more: to derive the second law of thermodynamics from mechanics. In 1872 he wrote an equation for how collisions change the distribution of speeds and proved that a quantity, HH, always decreases until Maxwell's distribution is reached. Josef Loschmidt objected. Newton's laws run equally well backwards, so reversing every molecule's velocity would make HH increase. Boltzmann's answer changed physics. The second law is not absolutely certain but overwhelmingly probable. Entropy-decreasing states are possible, just unimaginably rare. That idea became statistical mechanics.

Chapter IV

A Closer Look: How Fast Is Air?

Kinetic theory gives the typical speed of a molecule from its mass mm and the temperature TT:

vrms=3kBTm,v_{\text{rms}} = \sqrt{\frac{3 k_B T}{m}} ,

where kB=1.38×10−23k_B = 1.38 \times 10^{-23} J/K is Boltzmann's constant. A nitrogen molecule, the main component of air, has mass 28×1.66×10−27≈4.65×10−2628 \times 1.66 \times 10^{-27} \approx 4.65 \times 10^{-26} kg. At room temperature, 300 K:

vrms=3×1.38×10−23×3004.65×10−26≈517 m/s.v_{\text{rms}} = \sqrt{\frac{3 \times 1.38 \times 10^{-23} \times 300}{4.65 \times 10^{-26}}} \approx 517 \text{ m/s} .

That is about twice the cruising speed of an airliner, and faster than the speed of sound, about 350 m/s in air. The two are related: sound is a disturbance passed from molecule to molecule, so it cannot outrun the molecules carrying it.

So why does a smell take minutes to cross a room? Each cubic metre of air holds about 2.4×10252.4 \times 10^{25} molecules. With so many, a nitrogen molecule travels only about 70 nanometres, around a thousandth of the width of a human hair, before hitting another. At 500 m/s that means about 7 billion collisions every second, each sending it off in a new random direction. A random walk of NN steps gets only about N\sqrt N steps from its start. So diffusion alone moves a scent molecule only a few millimetres in a second, and in a real room it is mostly carried by air currents.

The same calculation, run backwards, measured the size of molecules. In 1865 Loschmidt combined the mean free path, inferred from viscosity, with the density of liquids to estimate how many molecules a gas contains: the first estimate of what is now Avogadro's number.

Chapter V

Atoms Made Real

Even so, many physicists and chemists around 1900, led by Ernst Mach and Wilhelm Ostwald, regarded atoms as a convenient fiction. Boltzmann, who felt he was fighting alone, took his own life in 1906. Proof came within two years. Albert Einstein had predicted in 1905 how far a pollen-sized particle in water should wander under random molecular impacts. In 1908 Jean Perrin measured it and obtained the number of molecules in a mole. Several other independent methods gave the same value. Ostwald conceded, and atoms became as real as anything in physics. Deriving fluid equations rigorously from the motion of molecules, Hilbert's sixth problem, took much longer. A proof for an idealised gas of hard spheres came only in 2025.

Applications

Where it is used

  • Nuclear engineering

    Separating uranium isotopes

    Lighter molecules move faster at the same temperature. The Manhattan Project's K-25 plant used this to enrich uranium, forcing uranium hexafluoride gas through thousands of porous barriers, each of which slightly favoured the lighter isotope.

    › Sources (1)
    • Rhodes, R. (1986). The Making of the Atomic Bomb. Simon & Schuster.
  • Planetary science

    Why Earth has no hydrogen atmosphere

    In the upper atmosphere, a fraction of molecules in the fast tail of Maxwell's distribution exceed escape velocity. Light hydrogen and helium leak away over geological time, while heavier nitrogen and oxygen stay. The same calculation explains why the Moon has almost no atmosphere.

    › Sources (1)
    • Jeans, J. H. (1916). The Dynamical Theory of Gases. Cambridge University Press.

Open problems

Where the map runs out

Recently resolved

Deriving fluid equations from molecules (Hilbert's sixth problem)

Resolved for an idealised dilute gas of hard spheres by Yu Deng, Zaher Hani and Xiao Ma (2024–25), work cited in Deng's 2026 Fields Medal. Some argue that dense gases and liquids, and realistic forces between molecules, still lie outside it.

Hilbert asked in 1900 for a rigorous derivation of the equations of gases and fluids from the motion of individual molecules. The chain runs from Newton's laws for particles, to Boltzmann's equation, to the equations of fluid flow. Each step is believed, but proving it for realistic time spans has resisted mathematicians for a century.

Why it is hard

Oscar Lanford proved in 1975 that Boltzmann's equation follows from Newton's laws, but only for a tiny fraction of the time between collisions. Extending that to long times means controlling how correlations between molecules build up through repeated collisions, which is exactly where irreversibility comes from. Deng, Hani and Ma did this for hard spheres in 2024 by tracking whole collision histories, and in 2025 carried the chain on to the fluid equations.

What resolving it unlocks

A mathematical account of how reversible molecular motion produces the irreversible behaviour of fluids, answering Loschmidt's objection with a theorem.

› Sources (3)

Further reading

  1. Lindley, D. (2001). Boltzmann's Atom: The Great Debate That Launched a Revolution in Physics. Free Press.

    A popular account of Boltzmann and the fight over atoms.

  2. Brush, S. G. (1976). The Kind of Motion We Call Heat (2 vols.). North-Holland.

    The standard scholarly history of kinetic theory.

  3. Feynman, R. P., Leighton, R. B. & Sands, M. (1963). The Feynman Lectures on Physics, Vol. I, ch. 39–43. Addison-Wesley.

    Kinetic theory explained with Feynman's usual clarity. Free online.