AQA · A-Level · Physics

    Course version: 7408 · Version from Sept 2016

    General shape of black-body curves, use of Wien’s displacement law to…

    Full specification wording

    Classification by temperature, black-body radiation (A-level only): General shape of black-body curves, use of Wien’s displacement law to estimate black-body temperature of sources.

    A black body absorbs all incident radiation and emits a continuous spectrum whose shape depends only on absolute temperature.

    Checked against the AQA 7408 specification (opens in a new tab) on .

    • Point 2 of 4
    • 4 key terms

    Study notes

    From the checked teaching notes for this specification point.

    The idea

    A black body absorbs all incident radiation and emits a continuous spectrum whose shape depends only on absolute temperature. Plotting intensity against wavelength gives a curve that rises steeply to a single peak then falls away at long wavelengths; hotter bodies peak at shorter wavelengths and have greater total intensity, so curves for different temperatures never cross. Wien’s displacement law states λmaxT = 2.9 × 10⁻³ m K, where λmax is the peak wavelength in metres and T is thermodynamic temperature in kelvin. To estimate a source’s temperature, read λmax from the curve or spectrum, convert to metres, then divide the constant by λmax.

    For example: A star peaking at 5.0 × 10⁻⁷ m gives T = 2.9 × 10⁻³ ÷ 5.0 × 10⁻⁷ = 5800 K.

    What earns the marks

    • States that a black body absorbs all incident radiation and emits a continuous spectrum depending only on its absolute temperature.
    • Describes the curve shape: intensity rises with wavelength to a single maximum, then decreases at longer wavelengths, with no crossing of curves for different temperatures.
    • States Wien’s displacement law as λmaxT = 2.9 × 10⁻³ m K and identifies λmax as the wavelength of peak intensity.
    • Converts a peak wavelength into metres and divides the constant by it to estimate T, or rearranges to find λmax from T.
    • Explains that a higher temperature gives a shorter peak wavelength and a greater area under the curve, linking this to total emitted power.
    • Uses correct units: λmax in m, T in K, and the constant in m K.

    Common mistakes and how to put them right

    • Using the wavelength in nanometres or micrometres directly in Wien’s law.

      Put it right: The error is failing to convert to metres, so the correction is to multiply by 10⁻⁹ or 10⁻⁶ before dividing.

    • Treating the peak wavelength as the maximum intensity value.

      Put it right: The error is confusing the x-coordinate of the peak with the y-coordinate, so the correction is to read λmax from the wavelength axis.

    • Assuming curves for different temperatures cross or that a cooler body can have a shorter peak wavelength.

      Put it right: Remember that higher temperature always shifts the peak to shorter wavelength.

    Exam tips

    • Sketch the axes with wavelength on the x-axis and intensity on the y-axis, label the peak and mark λmax clearly before substituting numbers.
    • Show the rearrangement of λmaxT = 2.9 × 10⁻³ m K explicitly, then substitute values with units so the kelvin unit follows through.
    • When comparing two sources, quote both peak wavelengths and state the inverse relationship: the shorter λmax corresponds to the higher temperature.

    Try the lesson

    The start of the Classification by temperature, black-body radiation (A-level only): General shape of black-body curves, use of Wien’s displacement law to estimate black-body temperature of sources. lesson, made from checked teaching notes for this specification point.

    Have a go first

    A black-body curve shows how the intensity of radiation emitted varies with wavelength. As the temperature of a black body increases, what happens to the wavelength at which the curve reaches its peak?

    Listen

    A black body absorbs all incident radiation and emits a continuous spectrum whose shape depends only on absolute temperature. Plotting intensity against wavelength gives a curve that rises steeply to a single peak then falls away at long wavelengths; hotter bodies peak at shorter wavelengths and have greater total intensity, so curves for different temperatures never cross. Wien’s displacement law states λmaxT = 2.9 × 10⁻³ m K, where λmax is the peak wavelength in metres and T is thermodynamic temperature in kelvin. To estimate a source’s temperature, read λmax from the curve or spectrum, convert to metres, then divide the constant by λmax. For example, a star peaking at 5.0 × 10⁻⁷ m gives T = 2.9 × 10⁻³ ÷ 5.0 × 10⁻⁷ = 5800 K. A strong answer earns marks for these points. States that a black body absorbs all incident radiation and emits a continuous spectrum depending only on its absolute temperature. Describes the curve shape: intensity rises with wavelength to a single maximum, then decreases at longer wavelengths, with no crossing of curves for different temperatures. States Wien’s displacement law as λmaxT = 2.9 × 10⁻³ m K and identifies λmax as the wavelength of peak intensity. Converts a peak wavelength into metres and divides the constant by it to estimate T, or rearranges to find λmax from T. A common slip: Assuming curves for different temperatures cross or that a cooler body can have a shorter peak wavelength. Instead, remember that higher temperature always shifts the peak to shorter wavelength. Exam tip: Sketch the axes with wavelength on the x-axis and intensity on the y-axis, label the peak and mark λmax clearly before substituting numbers.

    Key words

    Say what each word means before you turn the card.

    Black body

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    Wien's displacement law

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    Peak wavelength

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    Intensity–wavelength curve

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    See every definition
    Black body
    Absorbs all incident radiation and emits a continuous spectrum whose shape depends only on absolute temperature.
    Wien's displacement law
    States λmaxT = 2.9 × 10⁻³ m K, where λmax is the peak wavelength in metres and T is thermodynamic temperature in kelvin.
    Peak wavelength
    The wavelength of peak intensity, read from the curve or spectrum and converted to metres to estimate a source's temperature.
    Intensity–wavelength curve
    Rises steeply to a single peak then falls away at long wavelengths, with hotter bodies peaking at shorter wavelengths and curves never crossing.

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