☰ Contents · Physics

Measuring with a grating and dispersion

Lessons 26–27 · 2 lessons · N. Sh. Turdiyev, K. A. Tursunmetov, A. G. Ganiyev, K. T. Suyarov, J. E. Usarov, A. K. Avliyoqulov. Physics Grade 11, 1st edition. Niso Poligraf Publishing House, Tashkent, 2018
26

Laboratory work: finding the wavelength of light with a diffraction grating

Textbook: pp. 96–97
GoalKnow the method of finding the wavelength of light with a diffraction grating: λ = d·y/(n·x), and calculate the mean value and the errors.
New words
grating constant · panjara doimiysispectral order · spektr tartibiabsolute error · absolut xatolikrelative error · nisbiy xatolik
Explanation

The aim is to measure the wavelength of light with a diffraction grating. Equipment: a grating (with known period d, e.g. 10 μm or 20 μm), an incandescent lamp, a black screen with a narrow slit in the middle and a long rail with a millimetre scale. Looking through the grating at the slit one sees spectra of the 1st, 2nd, … orders on both sides of the slit. We measure the distance y from the slit to the chosen colour's line of order n and the distance x from the grating to the slit screen. For small angles (y ≪ x) sinφ ≈ tanφ = y/x, so from d·sinφ = nλ we get λ = d·y/(n·x). Repeating the measurement for each colour in several orders and on the right and left sides, we find λ_mean, the mean absolute error Δλ = |λ_mean – λ| and the relative error ε = Δλ_mean/λ_mean. We record results in a table. Safety: only a school lamp; do not look at the Sun or at lasers; the teacher connects the lamp to the supply.

Worked examples
d = 10 μm, x = 50 cm. The first-order red line is at y = 3.5 cm: λ = d·y/(n·x) = 10⁻⁵·0.035/(1·0.5) = 7·10⁻⁷ m = 700 nm. In the second order y = 7.0 cm: λ = 10⁻⁵·0.07/(2·0.5) = 700 nm, a consistent result.
Three measurements: 680, 700, 660 nm. λ_mean = (680 + 700 + 660)/3 = 680 nm; deviations 0, 20, 20 nm, Δλ_mean ≈ 13 nm; ε ≈ 13/680 ≈ 2 %.
Class activity

Draw the table template: colour, x (mm), y (mm), n, λ (nm), λ_mean, Δλ, ε. Fill it with the numbers of the example. Do the real work in the school laboratory; at home you may observe the spectrum on a CD with a lamp, but never look straight at the Sun.

Practice
1
Which approximation is used in the experiment and when is it valid?
2
d = 10 μm, n = 1, x = 50 cm, y = 3.5 cm. What is λ in nm?
3
d = 10 μm, n = 2, x = 50 cm, y = 7 cm. What is λ in nm?
4
Why is the central maximum white while spectra form on the sides?