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Greenhouse effect

Earth science · Climate

3D cutaway of the greenhouse effect Open the interactive 3D model →

Carbon dioxide is only 0.04 % of the air — so how can it change the temperature of a whole planet?

Sunlight passes through the air and warms the ground. The warm ground then gives off invisible heat rays (infrared). A few gases in the air, such as water vapour and carbon dioxide, catch those heat rays and send some back down, keeping Earth about 33 °C warmer than it would otherwise be.

Earth’s surface is about 33 K warmer than it would be without greenhouse gases because water vapour, carbon dioxide, methane and clouds absorb the infrared radiation emitted by the surface and re-emit part of it back downward. Adding CO₂ makes the atmosphere more opaque to infrared, raising the effective emission level to colder altitudes and creating a radiative forcing of about 5.35 ln(C/C₀) W/m².

Key facts

Incoming solar radiation (global mean)
≈ 340 W/m²
Planetary albedo
≈ 0.29–0.30
Effective emission temperature
≈ 255 K (−18 °C)
Mean surface temperature
≈ 288 K (15 °C)
Back radiation to the surface
≈ 340 W/m²
Forcing for doubled CO₂
≈ 3.7–3.9 W/m²

Parts you can explore (13)

In the 3D model

Rotate and take apart the model, follow a guided tour of what each part does and why it’s needed, change it with a live slider, and test yourself with a short quiz. Free, no sign-up.

Open Greenhouse effect in 3D →

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