• Pixel-art sticker of Areala, personifying Kepler's Second Law, with the caption “Equal Areas, Equal Times.”

IndexRelativity & CosmosSticker

Areala

Kepler's Second Law Physics

\[\frac{dA}{dt} = \frac{L}{2m} = \text{const}\]
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Meet Areala, a planet who moves faster near the Sun and slower far away, so the line joining them sweeps equal areas in equal times. Her art shows an ellipse with eccentricity 0.25, the Sun at a focus, and two sectors of equal area. 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 Areala, a planet who speeds up near the Sun and slows down far away, so she always sweeps out equal areas in equal times.

Kepler's second law, published in 1609, says that the line from the Sun to a planet sweeps out equal areas in equal times. Near the Sun the line is short, so the planet must move fast to sweep the same area; far away it moves slowly. Newton later showed that this law is angular-momentum conservation: gravity points straight at the Sun, so it exerts no torque, and the rate of sweeping is fixed at L/(2m).

Earth reaches perihelion in early January, about 147 million kilometres from the Sun, and aphelion in early July, about 152 million. It moves fastest in January, which is one reason northern winter is a few days shorter than northern summer.

In the sticker, the ellipse has eccentricity 0.25, and the two shaded sectors are drawn with equal area: a narrow one far away and a wider one close in.

The law holds for any central force, not only gravity, but breaks down when other bodies tug on the planet.

Equations

\[\frac{dA}{dt} = \frac{L}{2m} = \text{const}\]
Symbols
SymbolMeaningUnit
\(\frac{dA}{dt}\) rate at which the Sun–planet line sweeps area \(\mathrm{m²/s}\)
\(L\) orbital angular momentum of the planet \(\mathrm{kg·m²/s}\)
\(m\) mass of the planet \(\mathrm{kg}\)