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First teaching 2023

First exams 2025

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Average Kinetic Energy of a Molecule (SL IB Physics)

Revision Note

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Average Kinetic Energy of a Molecule

  • We think of an ideal gas as molecules that collide elastically in random motion
  • When the molecules collide, momentum and energy are conserved
    • We assume that, when the molecules are not in contact, no forces act between them
  • This means they have no potential energy
    • Therefore, the internal energy U of an ideal, monatomic gas is equal to its average kinetic energy if the molecules are far enough apart
  • The average kinetic energy, Ek for one molecule is equal to:

E subscript k space equals space 1 half m v squared space equals space space 3 over 2 k subscript B T

  • Where:
    • Ek = average kinetic energy of one molecule (J)
    • v = mean square speed of one molecule (m s–1)
    • m = mass of one molecule (kg)
    • kB = Boltzmann constant
    • T = temperature of the gas (K)
  • A consequence of this equation is that a greater gas temperature means a greater average kinetic energy of the particles
  • Since the total internal energy is the total kinetic energy, the internal energy of a gas U is defined as:

U space equals space 3 over 2 N k subscript B T

  • Where:
    • U = internal energy (J)
    • N = number of molecules

  • The relation to the amount of substance is:

U space space equals space 3 over 2 n R T 

  • Where:
    • = number of moles
    • R = ideal gas constant
  • When heat is transferred to a fixed volume of gas, the internal energy increases and hence, so does the temperature, since the equations show that

U space proportional to space T

  • This is only relevant for monatomic gases. Examples include:
    • Helium
    • Neon
    • Argon
  • A monatomic (one atom) molecule only has translational energy, whilst a diatomic (two-atom) molecule has both translational and rotational energy

Translation and rotational KE, downloadable AS & A Level Physics revision notes

A diatomic molecule has both rotational and translational kinetic energy

Worked example

600 J of thermal energy is transferred to 3 g of helium gas kept at a constant volume in a cylinder.

Helium has a mass number of 4.

Calculate the temperature of the gas.

Answer:

Step 1: List the known quantities

  • Thermal (internal) energy, U = 600 J
  • Molar mass of helium, mr = 4 g mol–1 (from its mass number)
  • Mass of helium gas, m = 3 g

Step 2: State the relevant equation

U space equals space 3 over 2 n R T

Step 3: Calculate the number of moles of the gas

m subscript r space equals fraction numerator space m over denominator n end fraction space space space rightwards double arrow space space space n space equals fraction numerator space m over denominator m subscript r end fraction
n space equals space 3 over 4 space equals space 0.75 space moles

Step 4: Rearrange the internal energy for the temperature, T

T space equals fraction numerator space 2 U over denominator 3 n R end fraction 

Step 5: Substitute in the values

T space equals space fraction numerator 2 space cross times space 600 space over denominator 3 space cross times space 0.75 space cross times space 8.31 end fraction space equals space 64 space straight K

Exam Tip

Calculations involving moles, molar mass and number of molecules are common in this topic. You should be confident with converting between these quantities for all calculations in thermal physics.

Remember the combination 'nRT' and 'NkBT' is also in the ideal gas equation. This shows how all the equations link together.

If you are using the equation E subscript k space equals space 3 over 2 k subscript B T , remember this is only for one molecule, so you will need to multiply it by the total number of molecules for a whole gas.

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Ashika

Author: Ashika

Ashika graduated with a first-class Physics degree from Manchester University and, having worked as a software engineer, focused on Physics education, creating engaging content to help students across all levels. Now an experienced GCSE and A Level Physics and Maths tutor, Ashika helps to grow and improve our Physics resources.