• Pixel-art sticker of Coastor, personifying Hohmann Transfer, with the caption “Burn, Coast, Burn Again.”

IndexRelativity & CosmosSticker

Coastor

Hohmann Transfer Physics

\[t = \pi\sqrt{\frac{a^3}{G M}}\]
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Meet Coastor, a spacecraft who saves fuel by burning, coasting and burning again. A Hohmann transfer stretches one circular orbit into an ellipse touching the next. From Earth to Mars the coast takes about 0.71 years, roughly 259 days, with launch windows about every 26 months. 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 Coastor, a spacecraft who saves fuel by burning, coasting and burning again.

To move from one circular orbit to a bigger one, the most fuel-efficient simple route is a Hohmann transfer. The spacecraft fires its engine once to stretch its orbit into an ellipse that just touches the outer orbit. It then coasts halfway round that ellipse without using fuel, and fires again at the far side to round out into the new circle.

The coasting time is half the period of the transfer ellipse, t = π√(a³/GM), where a is the ellipse's semi-major axis. From Earth at 1 AU to Mars at about 1.52 AU, a ≈ 1.26 AU, and Kepler's third law gives a trip of about 0.71 years, roughly 259 days.

The planets must be lined up correctly before launch, so these windows to Mars open only about every 26 months.

Walter Hohmann described the idea in 1925, long before spaceflight. Many real Mars missions follow paths close to it.

Equations

\[t = \pi\sqrt{\frac{a^3}{G M}}\]
Symbols
SymbolMeaningUnit
\(t\) transfer time \(\mathrm{s}\)
\(a\) semi-major axis of the transfer ellipse \(\mathrm{m}\)
\(G\) Newtonian constant of gravitation \(\mathrm{N·m²/kg²}\)
\(M\) mass of the central body \(\mathrm{kg}\)