Thermal Mirage
Heat Refraction Physics
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.
ShippingBy destination
Shipping calculated at checkout by destination.
Made to order: about 10 days of production and handling before it ships.
Returns & replacements21 days
Every item is printed to order, so we can’t accept returns or exchanges for change of mind, or if you ordered the wrong size or colour.
Print defect, misprint, damage or the wrong item? We’ll send a free replacement, or a refund if you prefer. Report it within 21 days of delivery with a photo; no need to send it back.
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.
Equations
| Symbol | Meaning | Unit |
|---|---|---|
| \(n\) | 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)