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Kinetic Theory of Gases · Lesson 6 of 6

Mean Free Path, Real Gases and the Atmosphere

15 min read3 ideas5 checks2 figures to playBy Asheshanand Acharya
What you will learn 0 / 3
Mean free path
Look around
Breathless in Leh

Travellers who fly into Leh, in Ladakh, are told to rest for a day before they walk far. Climbing a few stairs leaves them breathless. Dal takes forever to cook in an open pot, so every kitchen there uses a pressure cooker. The town is \(3.5\,\text{km}\) above the sea, and the air there is thin.

you will find the air pressure at Leh from one formula and the temperature of the air. You will also see why a pressure cooker is needed there.

How far between collisions?

Light an agarbatti at one end of a room. Its molecules move at about \(500\,\text{m/s}\), yet the smell takes a minute or more to cross the room. The reason is collisions. A molecule moves in a straight line only until it strikes another molecule, then leaves in a new direction. Its path is a zigzag, and its progress across the room is slow. The average length of a straight stretch between collisions is the mean free path \(\lambda\).

definition 3.3
Mean free path

The mean free path \(\lambda\) of a gas molecule is the average distance it travels between two successive collisions with other molecules.

Treat the molecules as balls of diameter \(d\). Two molecules collide if their centres come within \(d\) of each other. So a moving molecule strikes every molecule whose centre lies inside a cylinder of radius \(d\) around its path. In a time \(t\) it moves a distance \(vt\) and sweeps a cylinder of volume \(\pi d^2 vt\). If there are \(n\) molecules per unit volume, it meets \(n\pi d^2 vt\) of them.

Dividing the distance \(vt\) by the number of collisions gives \(\lambda = 1/(\pi d^2 n)\). This treats the other molecules as standing still. They move too. On average, one molecule moves relative to another at \(\sqrt2\) times its own speed. So collisions come \(\sqrt2\) times as often, and the exact result has \(\sqrt2\) in the denominator. With \(n = p/kT\) from the ideal gas equation, \(\lambda\) can be written with the pressure and the temperature.

RememberMean free path
\[ \lambda = \dfrac{1}{\sqrt2\,\pi d^2 n} = \dfrac{kT}{\sqrt2\,\pi d^2 p} \]
Holds whenan ideal gas of molecules of diameter \(d\), all of one kind.
Symbols\(\lambda\) mean free path, \(d\) diameter of a molecule, \(n\) number of molecules per unit volume, \(k\) Boltzmann constant, \(T\) absolute temperature, \(p\) pressure
Units\(\lambda\) and \(d\) in m, \(n\) in m⁻³, \(p\) in Pa

For air at \(300\,\text{K}\) and \(1\,\text{atm}\), take \(d = 3 \times 10^{-10}\,\text{m}\) and \(n = 2.45 \times 10^{25}\,\text{m}^{-3}\). Then \(\pi d^2 = 2.83 \times 10^{-19}\,\text{m}^2\) and \(\sqrt2\,\pi d^2 n = 9.8 \times 10^6\,\text{m}^{-1}\). So \(\lambda = 1.0 \times 10^{-7}\,\text{m}\), about \(0.1\,\mu\text{m}\). That is \(340\) molecular diameters. A molecule makes \(\bar v/\lambda\) collisions each second, the collision frequency. With an average speed of \(468\,\text{m/s}\), that is about \(4.6 \times 10^9\) collisions every second.

One molecule's free paths through a crowdA snapshot of a crowd of gas molecules, with one molecule followed as it moves. It travels in a straight line until it strikes another molecule, then leaves in a new direction, so its path is a zigzag of 20 free paths of very different lengths. A counter gives the number of free paths so far and their average length. The average wanders at first and then settles near 100 nanometres, the mean free path. free paths completed: 0 average free path: not yet
Fig 6.1One molecule followed through a crowd of others. Press play. Each straight stretch ends in a collision. The twenty free paths range from \(21\) to \(267\,\text{nm}\), yet their running average settles near \(100\,\text{nm}\), the mean free path.

Watch the counter in Fig 6.1. The first few free paths give an average that swings from \(21\,\text{nm}\) to over \(100\,\text{nm}\). As more paths are added, the average steadies near \(100\,\text{nm}\). No single free path equals \(\lambda\). The mean free path is a property of the crowd, like the average height of a class.

The formula also shows how \(\lambda\) changes. At a fixed temperature, \(\lambda\) is inversely proportional to the pressure. In a vacuum chamber at \(10^{-3}\,\text{atm}\) it grows to \(0.1\,\text{mm}\). At a fixed pressure, \(\lambda\) is proportional to \(T\), because a hotter gas at the same pressure is less crowded. Bigger molecules have shorter free paths, as \(1/d^2\).

CheckpointUnanswered

The pressure of a gas is halved while its temperature is held fixed. What happens to the mean free path of its molecules?

Checkpoint · numericUnanswered

Air molecules have an average speed of \(500\,\text{m/s}\) and a mean free path of \(100\,\text{nm}\). What is the average time between two collisions of one molecule, in nanoseconds?

ns± 2 %
Real gases and van der waals

When a gas is not ideal

Two assumptions of the ideal gas fail when a gas is squeezed hard or cooled. The molecules do have a size, and they do pull on one another when close. At ordinary pressures neither matters, because the molecules fill less than a thousandth of the space and are far apart. At a hundred atmospheres they fill a few percent of the space and are close neighbours. A gas that departs from \(pV = nRT\) is a real gas.

The departure is measured by the compressibility factor \(Z = pV/nRT\). For an ideal gas \(Z = 1\) at every pressure.

The compressibility factor of a real gasThe compressibility factor Z, equal to pV divided by nRT, is plotted against pressure up to 300 atmospheres. For an ideal gas Z is 1 at every pressure, a flat dashed line. For a real gas Z first dips below 1, to 0.8 at A near 100 atmospheres, where the attraction between molecules lowers the pressure. It returns to 1 at B near 200 atmospheres and rises above 1 at C, where the size of the molecules dominates.501001502002503000.511.5Op (atm)Z A B C ideal gas real gas
Fig 6.2The compressibility factor \(Z = pV/nRT\) of a real gas against pressure, beside the flat line \(Z = 1\) of an ideal gas. At A the real gas dips to \(Z = 0.8\): attraction dominates. At B the two effects cancel. At C the size of the molecules dominates and \(Z\) rises above \(1\).

Fig 6.2 shows both effects. At moderate pressure, A, the attraction between molecules wins. A molecule about to strike the wall is pulled backwards by the others behind it, so it strikes more gently. The pressure is lower than the ideal value and \(Z < 1\). At high pressure, C, the size of the molecules wins. They cannot enter the space the others fill, so the gas resists squeezing and \(Z > 1\).

RememberThe van der Waals equation
\[ \left(p + \dfrac{an^2}{V^2}\right)(V - nb) = nRT \]
Holds whena real gas, approximately, over a wide range of pressure and temperature; for \(a = b = 0\) it becomes \(pV = nRT\).
Symbols\(p\) measured pressure, \(V\) volume of the vessel, \(n\) number of moles, \(a\) constant for the attraction between molecules, \(b\) volume occupied by the molecules of one mole, \(R\) gas constant, \(T\) absolute temperature
Units\(a\) in Pa m⁶/mol², \(b\) in m³/mol

Johannes van der Waals made two corrections in 1873. The molecules cannot move into the space the others occupy, so the free volume is \(V - nb\). The constant \(b\) is about four times the volume of the molecules in one mole. The attraction lowers the measured pressure by an amount proportional to \((n/V)^2\). So \(an^2/V^2\) is added back to \(p\). The units follow: \(an^2/V^2\) is a pressure, so \(a\) is in Pa m⁶/mol², and \(nb\) is a volume, so \(b\) is in m³/mol.

ExampleCarbon dioxide squeezed into a litre

One mole of carbon dioxide fills a \(1.00\,\text{L}\) vessel at \(300\,\text{K}\). For carbon dioxide \(a = 0.364\,\text{Pa m}^6/\text{mol}^2\) and \(b = 4.27 \times 10^{-5}\,\text{m}^3/\text{mol}\). Find the pressure from the ideal gas equation and from the van der Waals equation.

Reveal one step at a time and finish the rest yourself.

A real gas is nearly ideal under two conditions. At low pressure the molecules are far apart, so their size and their attraction hardly matter. At high temperature the molecules move so fast that the weak attraction barely bends their paths. Below a certain temperature, the critical temperature \(T_c = 8a/27Rb\), squeezing turns a gas into a liquid. For carbon dioxide \(T_c = 304\,\text{K}\), just \(31\,^\circ\text{C}\). Oxygen and nitrogen have \(T_c\) near \(-119\,^\circ\text{C}\) and \(-147\,^\circ\text{C}\), so they could not be liquefied until they were first cooled below these temperatures.

CheckpointUnanswered

At moderate pressures a real gas has \(Z = pV/nRT\) less than \(1\). Which effect is responsible?

The barometric formula
Maths you need

The weight of the air

The air near the ground is squeezed by the weight of all the air above it. Climb a little, and there is less air above you, so the pressure falls. In the unit on fluids you met \(dp = -\rho g\,dh\) for a liquid, whose density is fixed. Air is different. Its density is proportional to its pressure, \(\rho = pM/RT\), so the thin air higher up weighs less and the pressure falls more and more slowly. This part uses \(g = 9.8\,\text{m/s}^2\), as the atmosphere needs, and \(M = 0.029\,\text{kg/mol}\) for air.

Deriving \(p = p_0\,e^{-Mgh/RT}\) step 1 of 5
1

\[ dp = -\rho g\,dh \]

Why. a thin layer of air of thickness \(dh\) and unit area weighs \(\rho g\,dh\). The pressure below it exceeds the pressure above it by that weight.

RememberThe barometric formula
\[ p = p_0\,e^{-Mgh/RT} = p_0\,e^{-h/H}, \qquad H = \dfrac{RT}{Mg}, \qquad \rho = \rho_0\,e^{-h/H} \]
Holds whenan isothermal atmosphere of one kind of ideal gas, with \(g\) constant; a fair guide to the real air up to about \(10\,\text{km}\).
Symbols\(p\) pressure at height \(h\), \(p_0\) pressure at \(h = 0\), \(M\) molar mass, \(g\) acceleration due to gravity, \(R\) gas constant, \(T\) absolute temperature, \(H\) scale height, \(\rho\) and \(\rho_0\) densities at \(h\) and at \(h = 0\)
Units\(h\) and \(H\) in m, \(M\) in kg/mol

The length \(H = RT/Mg\) is the scale height. For air at \(300\,\text{K}\), \(H = 8.31 \times 300/(0.029 \times 9.8) = 8772\,\text{m}\), about \(8.8\,\text{km}\). Each climb of \(8.8\,\text{km}\) divides the pressure by \(e = 2.72\). Half the air lies below \(H\ln2 = 6.1\,\text{km}\). The scale height is also the height the whole atmosphere would have if its density stayed at the sea-level value. At a fixed temperature the density is proportional to the pressure, so it falls with height in exactly the same way.

Pressure falls exponentially with heightThe pressure of an isothermal atmosphere at 300 kelvin, as a fraction of the sea-level pressure p0, against height up to 20 kilometres, with g = 9.8. The curve is p = p0 times e to the power minus h over H, with a scale height H of 8.8 kilometres. Shimla at 2.2 kilometres has 0.78 of sea-level pressure, Leh at 3.5 kilometres 0.67 and the top of Everest 0.36. A slider moves a point along the curve and reads the height and the pressure. Every 8.8 kilometres of climb divides the pressure by e, about 2.7.51015200.250.50.751Oh (km)p/p0 Leh Everest Shimla h = 3.5 km p/p0 = 0.67 (68 kPa)
SimThe pressure of an isothermal atmosphere at \(300\,\text{K}\), as a fraction of sea-level pressure, against height, with \(g = 9.8\,\text{m/s}^2\). Move the slider and read the pressure. Shimla, Leh and the top of Everest are marked.

Move the slider to \(2.2\,\text{km}\), the height of Shimla: \(p/p_0 = e^{-2.2/8.77} = 0.78\). At Leh, \(3.5\,\text{km}\), it is \(e^{-3.5/8.77} = 0.67\), or \(68\,\text{kPa}\). Each breath at Leh draws in only two thirds of the air, and two thirds of the oxygen, of a breath at the sea. At the top of Everest, \(8.85\,\text{km}\), the formula gives \(0.36\). The measured value is about \(0.33\), because the real air there is far colder than \(300\,\text{K}\).

This pays off the hook. At \(68\,\text{kPa}\) water boils at about \(89\,^\circ\text{C}\) instead of \(100\,^\circ\text{C}\). Dal simmering at \(89\,^\circ\text{C}\) cooks slowly, so kitchens in Leh use a pressure cooker to raise the pressure and the boiling point again. The breathlessness has the same cause: the partial pressure of oxygen falls from \(0.21\,\text{atm}\) at the sea to about \(0.14\,\text{atm}\) at Leh.

Common mistake

The barometric formula assumes one temperature at every height. The real lower atmosphere cools by about \(6.5\,\text{K}\) for every kilometre of climb, so the true pressure falls a little faster than the formula says. The chapter on the first law explains this cooling. The formula also takes \(g\) as constant, which is fair for the first few tens of kilometres.

Checkpoint · numericUnanswered

In an isothermal atmosphere with a scale height of \(8.77\,\text{km}\), at what height is the pressure half of its sea-level value? Give the answer in km.

km± 2 %
CheckpointUnanswered

In an isothermal atmosphere, the pressure falls from \(100\,\text{kPa}\) to \(80\,\text{kPa}\) over the first \(2\,\text{km}\) of climb. What is it after the next \(2\,\text{km}\)?

Story · Rudolf Clausius, 1858
Why smells spread slowly

In 1857 Rudolf Clausius published his kinetic theory, with molecules moving at hundreds of metres per second. The Dutch meteorologist Buys Ballot objected at once. If molecules were so fast, a smell released in one corner would fill a room in an instant, yet it takes minutes. In 1858 Clausius answered with a new idea: the molecules collide so often that each travels only a tiny distance before it turns. He called that distance the mean free path.

Exam traps
  1. Forgetting the \(\sqrt2\) in the mean free path.
    \(\lambda = 1/(\sqrt2\,\pi d^2 n)\). The \(\sqrt2\) comes from the motion of the other molecules.
  2. Using a straight-line fall of pressure with height for the air.
    Air's density falls with its pressure, so the pressure falls exponentially: equal climbs divide it by equal factors.
  3. Adding \(an^2/V^2\) and subtracting \(nb\) the wrong way.
    Attraction lowers the measured pressure, so \(an^2/V^2\) is added to \(p\). The molecules' size lowers the free volume, so \(nb\) is subtracted from \(V\).