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The rainbow: an arc written in every raindrop

The sun at your back, rain ahead of you — and 42 degrees of pure geometry. See how a single drop splits white light, and why the arc always hangs exactly where it hangs.

Everyone has seen one; no one has ever stood next to one. A rainbow is not an object hanging in the air — it is an event played out between three points: the sun, the raindrops and your eye. The figure below has two views: first look inside a single drop, then raise the sun above the horizon and watch what happens to the arc.

Viewing angle (red)
from the antisolar point
Viewing angle (violet)
violet is always tighter
Status
Where the ray hits the drop

Model: geometric optics, a single drop and one internal reflection (primary bow).
Colour dispersion exaggerated ~4× for clarity (in reality it is about 1.7°) — the angle readouts are real.

Fig. 1 — Slide the ray inside the drop, or raise the sun and watch the bow sink below the horizon

A drop like a prism, only round

A ray of sunlight entering a spherical drop goes through three events: it refracts on entry, reflects off the back wall, and refracts again on the way out. At each refraction, violet light bends more than red — water has a slightly higher refractive index for it. White light enters as one ray and leaves as a fan of colours. Move the slider in the DROPLET view: where the ray strikes decides the angle at which the fan leaves the drop.

The key formula
D = 180° + 2α − 4β
D — deviation of the ray · α — angle of incidence · β — angle of refraction (sin β = sin α / n) · the minimum of D gives the rainbow angle: 42.4° (red), 40.7° (violet)

Why 42 degrees, of all things

Drops send light back at all sorts of angles — but not evenly. The formula above has a minimum: around 42° from the antisolar direction, rays from many different impact points pile up into one bright direction. You can see it on the slider: near the minimum, the viewing angle almost stops changing even though the impact point keeps moving. This pile-up — a caustic — is what turns the chaos of a billion droplets into a sharp, luminous circle of radius 42°. We see its slice above the horizon: the arc.

A rainbow is not a thing — it is geometry, private to every eye.

The second bow and the dark band

Some of the light reflects inside the drop not once but twice — and leaves at about 51°. That is the secondary bow: fainter (every reflection costs light) and with the colours reversed, because the extra reflection flips the fan. Between the two bows the sky is noticeably darker — Alexander’s dark band: into that range of angles the drops send no light with either one bounce or two.

The SKY view shows the last piece of the puzzle: the arc’s geometry is chained to the sun. The top of the bow stands at 42° minus the sun’s elevation — which is why the grandest rainbows happen in the morning and towards evening, and at a summer noon, with the sun climbing past 42°, the whole arc slips below the horizon. A garden sprinkler lets you cheat: you can make your own rainbow at any hour, as long as the sun is at your back.

A simplificationWe do pure geometric optics: we ignore interference (the supernumerary bows just inside the main arc), the polarisation of rainbow light, and the fact that large drops flatten while a mist of tiny ones makes a white "fogbow". Refraction and reflection are enough to explain the 42° — and that is the heart of it.

Bibliography (sample)

  1. 1 Descartes — "Les Météores" (1637), appendix to the "Discourse on the Method" — the first geometric explanation of the 42°. gallica.bnf.fr
  2. 2 Nussenzveig, H. M. — "The Theory of the Rainbow", Scientific American 236, 116 (1977). 10.1038/scientificamerican0477-116
  3. 3 Minnaert, M. — "Light and Color in the Outdoors", Springer (1993). 10.1007/978-1-4612-2722-9
  4. 4 OpenStax — "University Physics, Vol. 3: The Nature of Light" (open access). openstax.org
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