A diffraction grating is like a giant “mirror” made of many, many tiny slits (usually thousands per centimetre). When light hits these slits, it spreads out and interferes with itself, creating bright and dark spots. Think of it as a musical instrument where each slit is a note; when the notes line up, you hear a clear tone (a bright spot). This property lets us measure the colour (wavelength) of light.
When a light wave passes through two adjacent slits, the waves travel slightly different distances before they meet. The extra distance is called the path difference and is given by:
\$\,d\,\sin\theta = m\,\lambda\,\$
If you know any three of these values, you can solve for the fourth. In a typical experiment we measure the angle \$\theta\$, we know \$d\$ from the grating’s specification, and we pick an order \$m\$ (usually \$m=1\$). Then we calculate \$\lambda\$.
Suppose a grating has 1200 lines mm⁻¹ and the first‑order bright spot appears at an angle of \$12^\circ\$. What is the wavelength of the light?
First, find \$d\$:
\$\,d = \dfrac{1}{1200}\,\text{mm} = 8.33\times10^{-4}\,\text{mm} = 8.33\,\mu\text{m}\,\$
Now use the formula with \$m=1\$:
\$\,\lambda = d\,\sin12^\circ = 8.33\,\mu\text{m}\,\times 0.2079 \approx 1.73\,\mu\text{m}\,\$
This wavelength (1730 nm) is in the infrared, so the light source is not visible. If we had measured a smaller angle, we would get a visible colour.
| Order \$m\$ | Angle \$\theta\$ (°) | Wavelength \$\lambda\$ (nm) |
|---|---|---|
| 1 | 12 | 1730 |
| 2 | 24 | 865 |
| 3 | 36 | 577 |