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.
How rainbows form: refraction, dispersion and reflection inside raindrops, why the colours appear in order, why rainbows are arcs and double rainbows.

A rainbow is sunlight split into its colours by millions of raindrops. The physics combines three things: refraction, reflection and dispersion.
Light leaves each drop at roughly 40–42° to the incoming sunlight, with red at the larger angle and violet at the smaller.
Each colour reaches your eye from drops at a specific angle. Red comes from higher drops and violet from lower ones, so red is on the outside of the arc and violet on the inside: red, orange, yellow, green, blue, indigo, violet.
All the drops sending light to your eye at the same angle form a circle around the point directly opposite the Sun. The ground usually hides the bottom half, so you see an arc. From an aircraft, you can sometimes see a full circle.
Light reflecting twice inside the drops creates a fainter secondary rainbow outside the first, with the colours reversed. The darker band between them is called Alexander’s band.
Stand with the Sun behind you and rain in front, ideally in the morning or late afternoon when the Sun is low.
Refraction follows Snell’s law. Why the sky itself is blue is a different effect, scattering; see why the sky is blue.
No. A rainbow’s position depends on where you stand, so it moves as you move.
Larger raindrops and bright, low sunlight create more vivid rainbows.
Yes. Moonbows form from moonlight, but they’re faint and often look white to our eyes.
Every article is edited by a human and checked against our editorial policy. Spotted a mistake? Tell us.
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.
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.
The Doppler effect explained: why a passing siren changes pitch, the formula, redshift and blueshift of light, and uses in radar, medicine and astronomy.