OCR · A-Level · Physics
Course version: H556 · Version from Sept 2015
Superposition: (2) a diffraction grating.
A diffraction grating has many equally spaced parallel slits, with the grating spacing d equal to the reciprocal of the number of lines per metre.
Checked against the OCR H556 specification (opens in a new tab) on .
- Point 10 of 10
- 3 key terms
Study notes
From the checked teaching notes for this specification point.
The idea
A diffraction grating has many equally spaced parallel slits, with the grating spacing d equal to the reciprocal of the number of lines per metre. When monochromatic light passes through the grating, sharp maxima occur at angles θ given by d sin θ = nλ, where n is the order of the maximum. The zeroth-order maximum is at θ = 0°, and higher orders appear symmetrically on both sides. To determine wavelength, the angle θ for a chosen order is measured, often by finding the positions of the maxima on a screen or using a spectrometer, and λ = d sin θ / n. For example, with 300 lines per millimetre, d = 1 / (300 × 10³ m⁻¹) = 3.33 × 10⁻⁶ m; if the first-order maximum is at 10.0°, then λ = 3.33 × 10⁻⁶ m × sin 10.0° = 5.79 × 10⁻⁷ m. The many slits make the maxima very sharp, so angles can be measured precisely.
What earns the marks
- States that the grating spacing d equals the reciprocal of the number of lines per metre.
- Uses d sin θ = nλ, identifying n as the order of the maximum.
- Measures the angle θ for a chosen order, for example by locating the first-order maximum on a screen or with a spectrometer.
- Converts lines per millimetre to lines per metre and then to d in metres before calculating.
- Explains that the large number of slits produces sharp, bright maxima, improving precision.
- Recognises that the zeroth-order maximum is at θ = 0° and higher orders appear symmetrically.
Common mistakes and how to put them right
Using d as the number of lines per metre rather than its reciprocal.
Put it right by calculating d = 1 / N, where N is lines per metre.
Forgetting to convert lines per millimetre to lines per metre.
Put it right: Multiply by 10³ before taking the reciprocal.
Using the angle in degrees directly in a calculator set to radians, or vice versa.
Put it right by checking the calculator mode matches the angle unit.
Confusing the order n with the number of slits.
Put it right: n is the order of the maximum, an integer such as 1, 2 or 3.
Exam tips
- Write d = 1 / N and convert N to lines per metre before substituting into d sin θ = nλ.
- Measure the angle to the first-order maximum on both sides and average to reduce alignment error.
- Check that sin θ ≤ 1; if the calculated value exceeds 1, that order does not exist for the given wavelength.
- Quote the wavelength in metres or nanometres with a consistent unit and sensible significant figures.
Try the lesson
The start of the Superposition: (2) a diffraction grating. lesson, made from checked teaching notes for this specification point.
Listen
A diffraction grating has many equally spaced parallel slits, with the grating spacing d equal to the reciprocal of the number of lines per metre. When monochromatic light passes through the grating, sharp maxima occur at angles θ given by d sin θ = nλ, where n is the order of the maximum. The zeroth-order maximum is at θ = 0°, and higher orders appear symmetrically on both sides. To determine wavelength, the angle θ for a chosen order is measured, often by finding the positions of the maxima on a screen or using a spectrometer, and λ = d sin θ / n. For example, with 300 lines per millimetre, d = 1 / (300 × 10³ m⁻¹) = 3.33 × 10⁻⁶ m; if the first-order maximum is at 10.0°, then λ = 3.33 × 10⁻⁶ m × sin 10.0° = 5.79 × 10⁻⁷ m. The many slits make the maxima very sharp, so angles can be measured precisely. A strong answer earns marks for these points. States that the grating spacing d equals the reciprocal of the number of lines per metre. Uses d sin θ = nλ, identifying n as the order of the maximum. Measures the angle θ for a chosen order, for example by locating the first-order maximum on a screen or with a spectrometer. Converts lines per millimetre to lines per metre and then to d in metres before calculating. A common slip: Using d as the number of lines per metre rather than its reciprocal. Instead, calculating d = 1 / N, where N is lines per metre. Exam tip: Write d = 1 / N and convert N to lines per metre before substituting into d sin θ = nλ.
Key words
Say what each word means before you turn the card.
Grating spacing
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Order of the maximum
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Grating equation
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See every definition
- Grating spacing
- The distance between adjacent slits, equal to the reciprocal of the number of lines per metre.
- Order of the maximum
- An integer n in d sin θ = nλ, with the zeroth-order maximum at θ = 0° and higher orders appearing symmetrically on both sides.
- Grating equation
- The relation d sin θ = nλ giving the angles θ at which sharp maxima occur when monochromatic light passes through the grating.
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