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Greenhouse Effect & Energy Balance

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About this simulation

Explore Earth’s incoming sunlight and outgoing infrared radiation. Change albedo and atmospheric absorption, then watch the surface warm or cool.

What students can explore

  • Keep albedo fixed and increase infrared absorption. What happens before the new equilibrium?
  • One-layer teaching model: sunlight passes through the atmosphere; infrared absorptivity ε also sets emission. OLR=σT⁴(1−ε/2); absorbed sunlight=1361(1−albedo)/4 W/m². Atmosphere adjusts instantly; surface heat capacity is 10 MJ/m²/K. Clouds, convection, oceans and feedbacks are omitted. This is not a climate forecast.

Learning objectives

  1. 1Keep albedo fixed and increase infrared absorption. What happens before the new equilibrium?

Questions teachers ask

Keep albedo fixed and increase infrared absorption. What happens before the new equilibrium?

Less energy initially escapes to space, so the surface warms. Outgoing radiation rises until it matches absorbed sunlight at a higher temperature.

About the model

One-layer teaching model: sunlight passes through the atmosphere; infrared absorptivity ε also sets emission. OLR=σT⁴(1−ε/2); absorbed sunlight=1361(1−albedo)/4 W/m². Atmosphere adjusts instantly; surface heat capacity is 10 MJ/m²/K. Clouds, convection, oceans and feedbacks are omitted. This is not a climate forecast.

Embed this simulation

Drop it into your LMS, blog, or class site — free.

<iframe src="https://kiwibee.io/en/simulations/greenhouse-effect-energy-balance-simulation/embed" title="Greenhouse Effect &amp; Energy Balance | KiwiBee" loading="lazy" allowfullscreen style="width:100%;height:min(70vh,620px);min-height:420px;border:0;border-radius:16px"></iframe>

Continue exploring

From model to evidence

Use a worksheet to capture predictions, observations, and explanations after students explore.

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