• Pixel-art sticker of Warmet, personifying Planetary Equilibrium Temperature, with the caption “Farther Out, Colder Me.”

IndexRelativity & CosmosSticker

Warmet

Planetary Equilibrium Temperature Physics

\[T_{\text{eq}} = T_\star \sqrt{\frac{R_\star}{2 d}}\,(1 - A)^{1/4}\]
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Meet Warmet, a rocky planet who balances the sunlight he soaks up with the heat he gives off. With 30 percent reflected, Earth's equilibrium temperature comes out about 255 K, or −18 °C. The real average of 288 K shows a 33 K greenhouse effect. Pixel-art kiss-cut sticker in 2, 3, 4 and 6 inches; equation, symbols and sources in the physics panel below.

Size
Surface

Flat $6 shipping worldwideMade to order, ships in 2–5 business days

Details

Size3″ × 3″

3″ × 3″ kiss-cut sticker.

Shipping

Flat $6 shipping on every order, worldwide, whatever's in it.

Delivery times & where we ship

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.

Full refund & replacement policy

The physics

Meet Warmet, a rocky planet who balances the sunlight he soaks up with the heat he gives off.

A planet warms until it radiates away as much energy as it absorbs. Some sunlight is reflected straight back, measured by the albedo A. The rest heats the planet, which then glows in the infrared.

Balancing the two gives T_eq = T★√(R★/2d)(1 − A)^¼. For the Earth, the Sun's surface is 5772 K, its radius is 6.96 × 10⁸ m, the distance is 1.50 × 10¹¹ m and A ≈ 0.30. That gives about 255 K, or −18 °C.

The real average is about 288 K, or 15 °C. The extra 33 K is the greenhouse effect, from gases that trap some of the outgoing infrared.

Astronomers use this formula to guess whether newly found planets around other stars might be warm enough to hold liquid water. Without this natural warming, the average surface would sit well below freezing.

Equations

\[T_{\text{eq}} = T_\star \sqrt{\frac{R_\star}{2 d}}\,(1 - A)^{1/4}\]
Symbols
SymbolMeaningUnit
\(T_{\text{eq}}\) equilibrium temperature of the planet \(\mathrm{K}\)
\(T_\star\) surface temperature of the star \(\mathrm{K}\)
\(R_\star\) radius of the star \(\mathrm{m}\)
\(d\) distance from the star \(\mathrm{m}\)
\(A\) albedo \(\mathrm{dimensionless}\)