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Thermal Mirage

Heat Refraction Physics

\[n\cos\alpha = \text{constant}\]
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Meet Thermal Mirage. Hot air over a road is thinner, so light travels slightly faster in it. Skylight skimming the road bends up into your eye, and you see the sky below the horizon: the puddle is sky. On the mug: n cos α = constant. Pixel-art full-wrap black ceramic mug in 11 or 15 oz; equation, symbols and sources in the physics panel below.

Shipping calculated at checkout by destinationMade to order, ships in ~10 days

Details

Size & material11oz · 15oz

Black glossy ceramic mug with a C-handle. Lead- and BPA-free.

  • 11oz: 0.33 l
  • 15oz: 0.44 l
CareDishwasher & microwave safe

Dishwasher safe (top rack) or hand wash. Microwave safe.

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Made to order: about 10 days of production and handling before it ships.

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The physics

Hot air near a road has a lower refractive index, so shallow sky rays bend upward and the sky appears below the horizon. With 30 K of heating only rays within about 0.4° of the road turn back.

Thermal Mirage paints a puddle on a dry road, and the puddle is sky.

The refractive index of air depends on its density: n − 1 is proportional to density, the Gladstone–Dale rule, with n − 1 ≈ 2.9×10⁻⁴ at standard conditions. Hot air over a sunlit road is thinner, so its index is slightly lower and light travels slightly faster in it.

In air layered by temperature, a ray obeys n cos α = constant, the formula on this mug, where α is its angle above the horizontal. A ray from the sky heading shallowly down toward the road enters ever lower-index air, flattens out and bends back up into your eye. You see the sky below the horizon, shimmering like water. This is an inferior mirage.

A worked number: if the air at the road is about 30 K hotter than the air at eye height, the index differs by about 2.5×10⁻⁵, and only rays within α_max ≈ √(2Δn) ≈ 0.4° of the road can turn back. That is why the puddle always sits far ahead.

“Come closer,” says Thermal Mirage. “I'll keep moving the water.”

Equations

\[n\cos\alpha = \text{constant}\]
\[n - 1 = K\rho\]
\[\alpha_{max} \approx \sqrt{2\,\Delta n}\]
Symbols
SymbolMeaningUnit
\(n\) refractive index of air \(\mathrm{dimensionless}\)
\(\alpha\) angle of the ray above the horizontal \(\mathrm{rad}\)
\(K\) Gladstone–Dale constant of air \(\mathrm{m³/kg}\)
\(\rho\) air density \(\mathrm{kg/m³}\)
\(\alpha_{max}\) largest ray angle that can be turned back \(\mathrm{rad}\)
\(\Delta n\) refractive-index difference between cool and hot air \(\mathrm{dimensionless}\)

Source Gladstone, J. H. & Dale, T. P. (1863). Researches on the refraction, dispersion, and sensitiveness of liquids. Philosophical Transactions of the Royal Society of London 153, 317–343.doi.org/10.1098/rstl.1863.0014 (opens in a new tab)