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Waves don’t just travel in straight lines — they spread out whenever they pass through a gap or around an obstacle. Pass light through thousands of tiny, evenly-spaced slits instead of just one, and that spreading becomes precise enough to measure a wavelength to remarkable accuracy.
What you'll be able to do
is the spreading out of a wave as it passes through a gap or around an obstacle. The amount of spreading is most significant when the gap width is comparable to the wavelength of the wave — a gap much wider than the wavelength produces very little noticeable spreading, while a gap comparable to (or smaller than) the wavelength produces substantial diffraction.
Tip — This is why sound (long wavelength) diffracts noticeably around a doorway, letting you hear someone in the next room, while light (very short wavelength) shows almost no visible diffraction through the same doorway.
A consists of a very large number of narrow, evenly-spaced slits. Light passing through produces sharp, well-defined bright maxima at specific angles, where light from every single slit arrives in phase and interferes constructively.
Tip — A grating with MORE lines per mm has a SMALLER slit spacing d, which — from d sinθ = nλ — spreads the maxima out to LARGER angles, giving better separation between wavelengths.
Equation recap
Common mistakes to avoid
Key takeaways
Test yourself
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