Why Is the Sky Blue? Rayleigh Scattering Explained
Why the sky is blue, explained simply: how sunlight scatters off air molecules, why short wavelengths scatter more, red sunsets and why it isn’t violet.
The Doppler effect explained: why a passing siren changes pitch, the formula, redshift and blueshift of light, and uses in radar, medicine and astronomy.

When an ambulance races past, its siren sounds higher as it approaches and lower as it moves away. The siren doesn’t change; the motion changes the waves reaching you. This is the Doppler effect.
A moving source emits waves while travelling. Ahead of the source, wave crests are bunched together: shorter wavelength, higher frequency. Behind it, they’re spread out: longer wavelength, lower frequency.
For a source moving towards or away from a stationary listener:
f′ = f × v ÷ (v ∓ vₛ)
A siren at 700 Hz approaches at 30 m/s: f′ = 700 × 343 ÷ (343 − 30) ≈ 767 Hz. As it moves away: f′ = 700 × 343 ÷ (343 + 30) ≈ 644 Hz.
Light waves shift too. Objects moving away appear slightly redder (redshift); objects approaching appear bluer (blueshift). Astronomers use this to measure how galaxies move, which revealed that the universe is expanding.
Light’s behaviour also explains why the sky is blue and how rainbows form.
Yes. Motion of the listener also changes the observed frequency.
Everyday speeds are tiny compared with the speed of light, so the shift is extremely small.
The stretching of light to longer wavelengths when a source moves away from the observer.
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Why the sky is blue, explained simply: how sunlight scatters off air molecules, why short wavelengths scatter more, red sunsets and why it isn’t violet.
How rainbows form: refraction, dispersion and reflection inside raindrops, why the colours appear in order, why rainbows are arcs and double rainbows.
Refraction and Snell’s law explained: why light bends between materials, refractive index, n₁ sin θ₁ = n₂ sin θ₂, total internal reflection and a calculator.