OCR · A-Level · Physics

    Course version: H556 · Version from Sept 2015

    (a) energy levels of electrons in isolated gas atoms

    Full specification wording

    Electromagnetic radiation from stars: (a) energy levels of electrons in isolated gas atoms

    In an isolated gas atom, electrons can occupy only certain allowed energy levels.

    Checked against the OCR H556 specification (opens in a new tab) on .

    • Point 1 of 11
    • 2 key terms

    Study notes

    From the checked teaching notes for this specification point.

    The idea

    In an isolated gas atom, electrons can occupy only certain allowed energy levels. Each level has a definite energy, and the lowest is the ground state. An electron can move to a higher level only by absorbing an amount of energy exactly equal to the difference between the two levels, for example by absorbing a photon of that energy. It can drop to a lower level by emitting a photon with energy equal to the difference. Because the level spacings are fixed, the photons absorbed or emitted have specific energies and therefore specific frequencies and wavelengths, producing line spectra rather than a continuous spectrum.

    What earns the marks

    • Electrons in an isolated gas atom can occupy only discrete allowed energy levels.
    • The lowest allowed level is the ground state and higher levels are excited states.
    • A transition between levels involves absorption or emission of a photon with energy equal to the level difference.
    • The fixed energy differences give rise to line spectra with specific frequencies and wavelengths.

    Common mistakes and how to put them right

    • Thinking electrons can have any energy.

      Put it right: Only discrete energy levels are allowed.

    • Believing any photon can cause a transition.

      Put it right: The photon energy must match the energy difference between levels.

    • Confusing excitation with ionisation.

      Put it right: Excitation moves an electron to a higher level, while ionisation removes it from the atom.

    Exam tips

    • Use the equation ΔE = hf to link photon energy to frequency.
    • Remember that absorption produces dark lines in a spectrum and emission produces bright lines.
    • Check whether the question is about an isolated atom or a solid, because energy bands apply to solids.

    Try the lesson

    The start of the Electromagnetic radiation from stars: (a) energy levels of electrons in isolated gas atoms lesson, made from checked teaching notes for this specification point.

    Listen

    In an isolated gas atom, electrons can occupy only certain allowed energy levels. Each level has a definite energy, and the lowest is the ground state. An electron can move to a higher level only by absorbing an amount of energy exactly equal to the difference between the two levels, for example by absorbing a photon of that energy. It can drop to a lower level by emitting a photon with energy equal to the difference. Because the level spacings are fixed, the photons absorbed or emitted have specific energies and therefore specific frequencies and wavelengths, producing line spectra rather than a continuous spectrum. A strong answer earns marks for these points. Electrons in an isolated gas atom can occupy only discrete allowed energy levels. The lowest allowed level is the ground state and higher levels are excited states. A transition between levels involves absorption or emission of a photon with energy equal to the level difference. The fixed energy differences give rise to line spectra with specific frequencies and wavelengths. Exam tip: Use the equation ΔE = hf to link photon energy to frequency.

    See it

    A flowchart running from top to bottom. The first node is labelled "Ground state (lowest allowed level)". An arrow labelled "Absorbs photon of energy equal to level difference" leads from it to a second node labelled "Higher level (excited state)". A return arrow labelled "Emits photon of energy equal to level difference" leads back from the higher level to the ground state. Both the ground state and the higher level have arrows leading to a third node labelled "Fixed level differences give specific photon energies". From there an arrow leads to a fourth node labelled "Specific frequencies and wavelengths", and a final arrow leads to a fifth node labelled "Line spectra rather than a continuous spectrum".
    It shows an electron moving between the ground state and a higher level by absorbing or emitting a photon, and how the fixed level differences lead to line spectra.

    Key words

    Say what each word means before you turn the card.

    Energy levels

    Try answering aloud or in your head before turning the card.

    Line spectra

    Try answering aloud or in your head before turning the card.

    See every definition
    Energy levels
    In an isolated gas atom, electrons can occupy only certain allowed levels, each with a definite energy.
    Line spectra
    Because the level spacings are fixed, the photons absorbed or emitted have specific energies and therefore specific frequencies and wavelengths, producing line spectra rather than a continuous spectrum.

    Label the diagram

    Some boxes have lost their names. Pick the right name for each number.

    The diagram again, with 2 boxes numbered instead of named. A flowchart running from top to bottom. The first node is labelled "Ground state (lowest allowed level)". An arrow labelled "Absorbs photon of energy equal to level difference" leads from it to a second node labelled "Higher level (excited state)". A return arrow labelled "Emits photon of energy equal to level difference" leads back from the higher level to the ground state. Both the ground state and the higher level have arrows leading to a third node labelled "Fixed level differences give specific photon energies". From there an arrow leads to a fourth node labelled "Specific frequencies and wavelengths", and a final arrow leads to a fifth node labelled "Line spectra rather than a continuous spectrum".
    • 1Box 1

    • 2Box 2

    0 of 2 labelled

    There is more to this lesson

    The full lesson goes on to check your understanding and help you earn the marks. Create a free account to carry on, with your progress saved.

    Carry on with the full lesson

    A week of Premium from your first lesson · Then the free plan continues · No card, no charge

    Test your understanding of Electromagnetic radiation from stars: (a) energy levels of electrons in isolated gas atoms

    Active recall beats re-reading. Take an instant quiz now to test what you’ve learned and lock it into long-term memory.

    Take topic quiz

    A week of Premium from your first lesson · Then the free plan continues · No card, no charge