OCR · A-Level · Physics
Course version: H556 · Version from Sept 2015
(g) transmission diffraction grating used to determine the wavelength of…
Full specification wording
Electromagnetic radiation from stars: (g) transmission diffraction grating used to determine the wavelength of light
A transmission diffraction grating has many equally spaced parallel slits.
Checked against the OCR H556 specification (opens in a new tab) on .
- Point 7 of 11
- 3 key terms
Study notes
From the checked teaching notes for this specification point.
The idea
A transmission diffraction grating has many equally spaced parallel slits. Monochromatic light passing through the grating produces sharp maxima at angles given by d sin θ = nλ, where d is the grating spacing, n is the order and λ is the wavelength. To determine wavelength, measure the angle θ for a known order n and calculate λ = d sin θ / n. The grating spacing d equals 1 divided by the number of lines per metre. Because the maxima are sharp, the angle can be measured precisely, giving an accurate wavelength. A spectrometer or optical bench with a protractor measures the angle between the zero-order and nth-order maxima.
What earns the marks
- A transmission diffraction grating consists of many equally spaced parallel slits.
- Light passing through the grating produces sharp maxima at angles satisfying d sin θ = nλ.
- The grating spacing d is the reciprocal of the number of lines per metre.
- Wavelength is determined by measuring the angle θ for a known order n and using λ = d sin θ / n.
- The sharpness of the maxima allows precise angle measurement and therefore accurate wavelength determination.
Common mistakes and how to put them right
Using the number of lines per millimetre directly as d instead of converting to metres and taking the reciprocal.
Measuring the angle between adjacent orders rather than between the zero-order and the nth-order maximum.
Forgetting to divide by n when calculating wavelength from d sin θ = nλ.
Confusing the grating spacing d with the slit width of a double slit.
Put it right: In a grating d is the distance between adjacent slits.
Exam tips
- Always convert lines per millimetre to lines per metre before calculating d = 1/N.
- Measure the angle from the zero-order maximum to the centre of the nth-order maximum, not between two non-zero orders.
- Use a large number of lines and a high order where possible to increase the angle and reduce percentage uncertainty in θ.
Try the lesson
The start of the Electromagnetic radiation from stars: (g) transmission diffraction grating used to determine the wavelength of light lesson, made from checked teaching notes for this specification point.
Listen
A transmission diffraction grating has many equally spaced parallel slits. Monochromatic light passing through the grating produces sharp maxima at angles given by d sin θ = nλ, where d is the grating spacing, n is the order and λ is the wavelength. To determine wavelength, measure the angle θ for a known order n and calculate λ = d sin θ / n. The grating spacing d equals 1 divided by the number of lines per metre. Because the maxima are sharp, the angle can be measured precisely, giving an accurate wavelength. A spectrometer or optical bench with a protractor measures the angle between the zero-order and nth-order maxima. A strong answer earns marks for these points. A transmission diffraction grating consists of many equally spaced parallel slits. Light passing through the grating produces sharp maxima at angles satisfying d sin θ = nλ. The grating spacing d is the reciprocal of the number of lines per metre. Wavelength is determined by measuring the angle θ for a known order n and using λ = d sin θ / n. Exam tip: Always convert lines per millimetre to lines per metre before calculating d = 1/N.
Key words
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Transmission diffraction grating
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Grating spacing
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Order
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See every definition
- Transmission diffraction grating
- Consists of many equally spaced parallel slits, through which monochromatic light passes to produce sharp maxima.
- Grating spacing
- The distance between adjacent slits, equal to 1 divided by the number of lines per metre.
- Order
- The value n in d sin θ = nλ, used with a measured angle θ to determine the wavelength.
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