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Astronomy

The Runaway Greenhouse Effect: When Ocean Planets Boil Away

Quick fact

Venus is the classic example: it likely experienced a runaway greenhouse effect in the past, and its surface temperature now reaches about 460°C, hot enough to melt lead.

Why this is interesting

We know Earth is warming, but did you know that on some planets, warming can become so extreme that entire oceans boil away? Could our planet ever cross that threshold?

Read the full explanation

Understanding The Runaway Greenhouse Effect: When Ocean Planets Boil Away

The ordinary greenhouse effect warms a planet when gases like carbon dioxide trap heat. But water vapor is itself a powerful greenhouse gas. On a planet with oceans, warming the surface causes more water to evaporate. Since water vapor also traps heat, this leads to even more warming, which evaporates even more water. This positive feedback loop can, under enough solar heating, become unstoppable. The atmosphere thickens with steam until the oceans are completely gone, and the surface pressure and temperature soar. This is the runaway greenhouse: once started, it cannot be stopped by natural means.

A deeper explanation

The equilibrium temperature of a planet depends on a balance between incoming sunlight and outgoing infrared radiation. If greenhouse gases absorb infrared, they raise that equilibrium temperature. Water vapor plays a key role because its concentration in the atmosphere is tied to temperature via evaporation. As the greenhouse effect warms the surface, evaporation adds water vapor, which traps more heat, raising the temperature further, causing yet more evaporation. When this positive feedback overwhelms the negative feedback of increased radiation to space, the runaway begins. The critical threshold—the ‘Komabayashi–Ingersoll limit’—occurs when the greenhouse effect of the added water vapor makes the planet absorb more radiation than it can emit, forcing the surface temperature to rise until the oceans completely evaporate. This marks the inner edge of the habitable zone for ocean planets.

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