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In addition to the revision notes for Pressure, Temperature and RMS Speed on this page, you can also access the following Thermodynamics learning resources for Pressure, Temperature and RMS Speed

Tutorial ID | Title | Tutorial | Video Tutorial | Revision Notes | Revision Questions | |
---|---|---|---|---|---|---|

13.7 | Pressure, Temperature and RMS Speed |

In these revision notes for Pressure, Temperature and RMS Speed, we cover the following key points:

- What is rms speed of a gas?
- What is the relationship between pressure temperature and rms speed in a gas?
- Why are the factors affecting the rms speed of ideal gas molecules?
- What is the translational kinetic energy of gas particles?
- What is mean free path of gas molecules?
- What are the factors affecting mean free path of gas molecules?

Molecules of a gas move in every direction within the container; they hit each other and the container walls and then, they bounce back. If we consider the gas as ideal, the collisions between particles can be neglected. Thus, we consider only the elastic collisions of gas molecules with the container walls.

We call the quantity √**v^{2}_{average}** as root mean square speed (v

P = *n × M**/**3V* × v^{2}_{rms}

This formula indicates how a macroscopic quantity such as pressure depends on a microscopic quantity such as the speed of molecules.

As for the rms speed of gas molecules we have

v_{rms} = √*3 × R × T**/**M*

The translational kinetic energy of a gas molecule molecule is

KE = *3**/**2* × k × T

We obtain a very important conclusion based on the last formula:

**"All ideal gas molecules, no matter what kind of gas they belong, have the same translational kinetic energy at a given temperature."**

This means that when we measure the temperature of an ideal gas, we are actually measuring the average translational kinetic energy of its particles.

Molecules of a gas collide continuously with each other; however, they move linearly at constant speed during the time interval between two consecutive collisions.

We use a parameter known as "mean free path" (in symbols, λ) to describe this random motion of gas particles. It represents the average distance travelled by a gas particle between two collisions. Mean free path depends on the following factors:

**1- Density or concentration of gas**. In this case, we express density in terms of concentration of molecules, i.e. as number of molecules per unit volume (in short, ** N/V**) instead of mass per unit volume, as here we are interested on microscopic parameters such as the number of molecules.

Based on this factor, we can say that higher the concentration of particles, smaller their mean free path. Therefore, the molecular mean free path is inversely proportional to gas concentration.

**2- Size of molecules**. Obviously, larger the gas molecules, shorter the mean free path between them. molecules are, the smaller the mean free path. Mean free path λ, should vary (inversely) as the square of the molecular diameter d because the cross section of a molecule - not its diameter - determines its effective target area.

The equation of mean free path of gas molecules is:

λ = *1**/**√***2** × π × d^{2} × *N**/**V*

where N is the total number of gas molecules.

Enjoy the "Pressure, Temperature and RMS Speed" revision notes? People who liked the "Pressure, Temperature and RMS Speed" revision notes found the following resources useful:

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- Thermodynamics Physics tutorial: Pressure, Temperature and RMS Speed. Read the Pressure, Temperature and RMS Speed physics tutorial and build your physics knowledge of Thermodynamics
- Thermodynamics Practice Questions: Pressure, Temperature and RMS Speed. Test and improve your knowledge of Pressure, Temperature and RMS Speed with example questins and answers
- Check your calculations for Thermodynamics questions with our excellent Thermodynamics calculators which contain full equations and calculations clearly displayed line by line. See the Thermodynamics Calculators by iCalculator™ below.
- Continuing learning thermodynamics - read our next physics tutorial: Molar Specific Heats and Degrees of Freedom

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