Kinetic Theory

Kinetic Theory: Atomic and Molecular Explanation of Pressure and Temperature

We have developed macroscopic definitions of pressure and temperature. Pressure is the force divided by the area on which the force is exerted, and temperature is measured with a thermometer. We gain a better understanding of pressure and temperature from the kinetic theory of gases, which assumes that atoms and molecules are in continuous random motion.

A green vector v, representing a molecule colliding with a wall, is pointing at the surface of a wall at an angle. A second vector v primed starts at the point of impact and travels away from the wall at an angle. A dotted line perpendicular to the wall through the point of impact represents the component of the molecule’s momentum that is perpendicular to the wall. A red vector F is pointing into the wall from the point of impact, representing the force of the molecule hitting the wall.

When a molecule collides with a rigid wall, the component of its momentum perpendicular to the wall is reversed. A force is thus exerted on the wall, creating pressure.

The figure above shows an elastic collision of a gas molecule with the wall of a container, so that it exerts a force on the wall (by Newton’s third law). Because a huge number of molecules will collide with the wall in a short time, we observe an average force per unit area. These collisions are the source of pressure in a gas. As the number of molecules increases, the number of collisions and thus the pressure increase. Similarly, the gas pressure is higher if the average velocity of molecules is higher. The actual relationship is derived in the "Things Great and Small" feature below. The following relationship is found:

\(\text{PV}=\cfrac{1}{3}\text{Nm}\overline{{v}^{2}},\)

where \(P\) is the pressure (average force per unit area), \(V\) is the volume of gas in the container, \(N\) is the number of molecules in the container, \(m\) is the mass of a molecule, and \(\overline{{v}^{2}}\) is the average of the molecular speed squared.

What can we learn from this atomic and molecular version of the ideal gas law? We can derive a relationship between temperature and the average translational kinetic energy of molecules in a gas. Recall the previous expression of the ideal gas law:

\(\text{PV}=\text{NkT}.\)

Equating the right-hand side of this equation with the right-hand side of \(\text{PV}=\cfrac{1}{3}\text{Nm}\overline{{v}^{2}}\) gives

\(\cfrac{1}{3}\text{Nm}\overline{{v}^{2}}=\text{NkT}.\)

Making Connections: Things Great and Small—Atomic and Molecular Origin of Pressure in a Gas

The figure below shows a box filled with a gas. We know from our previous discussions that putting more gas into the box produces greater pressure, and that increasing the temperature of the gas also produces a greater pressure. But why should increasing the temperature of the gas increase the pressure in the box? A look at the atomic and molecular scale gives us some answers, and an alternative expression for the ideal gas law.

The figure shows an expanded view of an elastic collision of a gas molecule with the wall of a container. Calculating the average force exerted by such molecules will lead us to the ideal gas law, and to the connection between temperature and molecular kinetic energy. We assume that a molecule is small compared with the separation of molecules in the gas, and that its interaction with other molecules can be ignored. We also assume the wall is rigid and that the molecule’s direction changes, but that its speed remains constant (and hence its kinetic energy and the magnitude of its momentum remain constant as well). This assumption is not always valid, but the same result is obtained with a more detailed description of the molecule’s exchange of energy and momentum with the wall.

Diagram representing the pressures that a gas exerts on the walls of a box in a three-dimensional coordinate system with x, y, and z components.

Gas in a box exerts an outward pressure on its walls. A molecule colliding with a rigid wall has the direction of its velocity and momentum in the \(x\)-direction reversed. This direction is perpendicular to the wall. The components of its velocity momentum in the \(y\)- and \(z\)-directions are not changed, which means there is no force parallel to the wall.

If the molecule’s velocity changes in the \(x\)-direction, its momentum changes from \(–{\text{mv}}_{x}\) to \(+{\text{mv}}_{x}\). Thus, its change in momentum is \(\text{Δ}\text{mv}\phantom{\rule{0.20em}{0ex}}\text{= +}{\text{mv}}_{x}–(–{\text{mv}}_{x})=2{\text{mv}}_{x}\). The force exerted on the molecule is given by

\(F=\cfrac{\text{Δ}p}{\text{Δ}t}=\cfrac{2{\text{mv}}_{x}}{\text{Δ}t}\text{.}\)

There is no force between the wall and the molecule until the molecule hits the wall. During the short time of the collision, the force between the molecule and wall is relatively large. We are looking for an average force; we take \(\text{Δ}t\) to be the average time between collisions of the molecule with this wall. It is the time it would take the molecule to go across the box and back (a distance \(2l)\) at a speed of \({v}_{x}\). Thus \(\text{Δ}t=2l/{v}_{x}\), and the expression for the force becomes

\(F=\cfrac{2{\text{mv}}_{x}}{2l/{v}_{x}}=\cfrac{{\text{mv}}_{x}^{2}}{l}\text{.}\)

This force is due to one molecule. We multiply by the number of molecules \(N\) and use their average squared velocity to find the force

\(F=N\cfrac{m\overline{{v}_{x}^{2}}}{l},\)

where the bar over a quantity means its average value. We would like to have the force in terms of the speed \(v\), rather than the \(x\)-component of the velocity. We note that the total velocity squared is the sum of the squares of its components, so that

\(\overline{{v}^{2}}=\overline{{v}_{x}^{2}}+\overline{{v}_{y}^{2}}+\overline{{v}_{z}^{2}}\text{.}\)

Because the velocities are random, their average components in all directions are the same:

\(\overline{{v}_{x}^{2}}=\overline{{v}_{y}^{2}}=\overline{{v}_{z}^{2}}\text{.}\)

Thus,

\(\overline{{v}^{2}}=3\overline{{v}_{x}^{2}},\)

or

\(\overline{{v}_{x}^{2}}=\cfrac{1}{3}\overline{{v}^{2}}.\)

Substituting \(\cfrac{1}{3}\overline{{v}^{2}}\) into the expression for \(F\) gives

\(F=N\cfrac{m\overline{{v}^{2}}}{3l}\text{.}\)

The pressure is \(F/A,\) so that we obtain

\(P=\cfrac{F}{A}=N\cfrac{m\overline{{v}^{2}}}{3\text{Al}}=\cfrac{1}{3}\cfrac{\text{Nm}\overline{{v}^{2}}}{V},\)

where we used \(V=\text{Al}\) for the volume. This gives the important result.

\(\text{PV}=\cfrac{1}{3}\text{Nm}\overline{{v}^{2}}\)

This equation is another expression of the ideal gas law.

We can get the average kinetic energy of a molecule, \(\cfrac{1}{2}{\text{mv}}^{2}\), from the right-hand side of the equation by canceling \(N\) and multiplying by 3/2. This calculation produces the result that the average kinetic energy of a molecule is directly related to absolute temperature.

\(\overline{\text{KE}}=\cfrac{1}{2}m\overline{{v}^{2}}=\cfrac{3}{2}\text{kT}\)

The average translational kinetic energy of a molecule, \(\overline{\text{KE}}\), is called thermal energy. The equation \(\overline{\text{KE}}=\cfrac{1}{2}m\overline{{v}^{2}}=\cfrac{3}{2}\text{kT}\) is a molecular interpretation of temperature, and it has been found to be valid for gases and reasonably accurate in liquids and solids. It is another definition of temperature based on an expression of the molecular energy.

It is sometimes useful to rearrange \(\overline{\text{KE}}=\cfrac{1}{2}m\overline{{v}^{2}}=\cfrac{3}{2}\text{kT}\), and solve for the average speed of molecules in a gas in terms of temperature,

\(\sqrt{\overline{{v}^{2}}}={v}_{\text{rms}}=\sqrt{\cfrac{3\text{kT}}{m}},\)

where \({v}_{\text{rms}}\) stands for root-mean-square (rms) speed.

Example: Calculating Kinetic Energy and Speed of a Gas Molecule

(a) What is the average kinetic energy of a gas molecule at \(\text{20}\text{.}0\text{º}\text{C}\) (room temperature)? (b) Find the rms speed of a nitrogen molecule \(({\text{N}}_{2})\) at this temperature.

Strategy for (a)

The known in the equation for the average kinetic energy is the temperature.

\(\overline{\text{KE}}=\cfrac{1}{2}m\overline{{v}^{2}}=\cfrac{3}{2}\text{kT}\)

Before substituting values into this equation, we must convert the given temperature to kelvins. This conversion gives \(T=(\text{20}\text{.}0+\text{273})\phantom{\rule{0.25em}{0ex}}\text{K = 293}\phantom{\rule{0.25em}{0ex}}\text{K}.\)

Solution for (a)

The temperature alone is sufficient to find the average translational kinetic energy. Substituting the temperature into the translational kinetic energy equation gives

\(\overline{\text{KE}}=\cfrac{3}{2}\text{kT}=\cfrac{3}{2}(1\text{.}\text{38}×{\text{10}}^{-\text{23}}\phantom{\rule{0.25em}{0ex}}\text{J/K})(\text{293}\phantom{\rule{0.25em}{0ex}}\text{K})=6\text{.}\text{07}×{\text{10}}^{-\text{21}}\phantom{\rule{0.25em}{0ex}}\text{J}\text{.}\)

Strategy for (b)

Finding the rms speed of a nitrogen molecule involves a straightforward calculation using the equation

\(\sqrt{\overline{{v}^{2}}}={v}_{\text{rms}}=\sqrt{\cfrac{3\text{kT}}{m}},\)

but we must first find the mass of a nitrogen molecule. Using the molecular mass of nitrogen \({\text{N}}_{2}\) from the periodic table,

\(m=\cfrac{2(\text{14}\text{.}\text{0067})×{\text{10}}^{-3}\phantom{\rule{0.25em}{0ex}}\text{kg/mol}}{6\text{.}\text{02}×{\text{10}}^{\text{23}}\phantom{\rule{0.25em}{0ex}}{\text{mol}}^{-1}}=4\text{.}\text{65}×{\text{10}}^{-\text{26}}\phantom{\rule{0.25em}{0ex}}\text{kg}\text{.}\)

Solution for (b)

Substituting this mass and the value for \(k\) into the equation for \({v}_{\text{rms}}\) yields

\({v}_{\text{rms}}=\sqrt{\cfrac{3\text{kT}}{m}}=\sqrt{\cfrac{3(1\text{.}\text{38}×{\text{10}}^{–\text{23}}\phantom{\rule{0.25em}{0ex}}\text{J/K})(\text{293 K})}{4\text{.}\text{65}×{\text{10}}^{\text{–26}}\phantom{\rule{0.25em}{0ex}}\text{kg}}}=\text{511}\phantom{\rule{0.25em}{0ex}}\text{m/s}\text{.}\)

Discussion

Note that the average kinetic energy of the molecule is independent of the type of molecule. The average translational kinetic energy depends only on absolute temperature. The kinetic energy is very small compared to macroscopic energies, so that we do not feel when an air molecule is hitting our skin. The rms velocity of the nitrogen molecule is surprisingly large. These large molecular velocities do not yield macroscopic movement of air, since the molecules move in all directions with equal likelihood. The mean free path (the distance a molecule can move on average between collisions) of molecules in air is very small, and so the molecules move rapidly but do not get very far in a second. The high value for rms speed is reflected in the speed of sound, however, which is about 340 m/s at room temperature. The faster the rms speed of air molecules, the faster that sound vibrations can be transferred through the air. The speed of sound increases with temperature and is greater in gases with small molecular masses, such as helium. (See the figure below.)

In part a of the figure, circles represent molecules distributed in a gas. Attached to each circle is a vector representing velocity. The circles have a random arrangement, while the vector arrows have random orientations and lengths. In part b of the figure, an arc represents a sound wave as it passes through a gas. The velocity of each molecule along the peak of the wave is roughly oriented parallel to the transmission direction of the wave.

(a) There are many molecules moving so fast in an ordinary gas that they collide a billion times every second. (b) Individual molecules do not move very far in a small amount of time, but disturbances like sound waves are transmitted at speeds related to the molecular speeds.

Making Connections: Historical Note—Kinetic Theory of Gases

The kinetic theory of gases was developed by Daniel Bernoulli (1700–1782), who is best known in physics for his work on fluid flow (hydrodynamics). Bernoulli’s work predates the atomistic view of matter established by Dalton.

This lesson is part of:

Temperature, Kinetic Theory, and Gas Laws

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