1Big from small
In 1827 Robert Brown watched tiny grains released from pollen, floating in water, through a microscope. They never stopped jiggling. Water molecules, far too small to see, hit each grain from all sides millions of times a second; at any instant one side gets a few more hits, so the grain is kicked at random. This Brownian motion is direct evidence that molecules exist and never stop moving.
Kinetic theory explains a whole gas from its molecules, each obeying Newton's laws: their hits on the walls make the pressure, and how fast they move on average sets the temperature.
2The assumptions
- A gas has a huge number of molecules (about in a mole), so averages are steady.
- They move at random, equally in every direction, in straight lines between collisions.
- They are tiny: their own volume is negligible next to the space between them.
- Collisions with each other and with the walls are perfectly elastic: no kinetic energy is lost.
- There are no forces between molecules except during a collision.
- A collision takes almost no time compared with the time between collisions.
How empty is a gas? In air a molecule is about 0.3 nm across, but its neighbours are about 3.3 nm away. The molecules fill only about 0.04% of the space, which is why a gas is so easy to squeeze.
- Random motion: the average velocity is zero, but the average speed is not.
- No forces: no potential energy between molecules; all the energy is kinetic.
- Elastic collisions: the total kinetic energy stays the same at a fixed temperature, though single molecules speed up and slow down.
3One molecule, one wall
A molecule of mass moves towards a wall with velocity and bounces back elastically. Its momentum changes from to , so the wall gets a kick of . It must cross the box and come back, a distance , before hitting that wall again, which takes .
4Pressure of a gas
Add up molecules in a cube of side : . Dividing by the wall's area gives .
Where the ⅓ comes from: . The motion is random, so the three averages are equal and each is one third of . The wall feels only the x part.
5What temperature is
Kinetic theory gives ; the gas law gives . They describe the same gas, so :
- Per mole: . For moles: (the translational kinetic energy).
- It depends only on : heavy or light, at the same temperature every molecule has the same average kinetic energy.
- At 300 K it is about J; doubling the kelvin temperature doubles it.
6Mass and the rms speed
At the same temperature light molecules move faster: . If oxygen has 400 m/s, hydrogen (16 times lighter) has m/s.
7Real gases
At low pressure and high temperature molecules are far apart and fast, and a gas is nearly ideal. At high pressure their own size matters (there is less free space than ). At low temperature they are slow, and small attractions pull them together; cool and squeeze enough and the gas becomes a liquid.
Summary
Key ideas
- Brownian motion shows that molecules exist and never stop moving.
- Kinetic theory explains pressure and temperature from the motion of molecules obeying Newton's laws.
- Ideal gas: many molecules, random motion, negligible size, elastic collisions, no forces between collisions, instant collisions.
- A gas is mostly empty space: in air the molecules fill about 0.04% of the volume.
- The average velocity of the molecules is zero, but their average speed is not.
- One molecule gives a wall a kick of 2mvₓ every 2L/vₓ, an average force of mvₓ²/L.
- Random motion makes the three directions equal, which gives the factor ⅓ in P = ⅓ρv²rms.
- Pressure is two thirds of the kinetic energy per unit volume.
- The average kinetic energy of a molecule is 3/2 kT: temperature measures molecular motion.
- At the same temperature all gases have the same average kinetic energy per molecule, so lighter molecules move faster.
- v_rms = √(3RT/M), with M in kg/mol.
- Real gases depart from ideal behaviour at high pressure and low temperature.
Every equation
- Kick on the wall
- Force of one molecule
- Pressure
- Pressure and density
- Equal directions
- Energy density
- KE per molecule
- KE per mole
- KE of n moles
- rms speed
- Molecule mass
- Boltzmann constant
- Van der Waals
- Compressibility