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Earth's Energy Balance and the Greenhouse Effect, Quantified

A planet settles at the temperature where it radiates away as much as it absorbs, and that calculation gives an Earth well below freezing. The gap between that figure and the real surface temperature is the greenhouse effect, measured rather than asserted.

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What a learner can do afterwards

  • Compute an equilibrium temperature from solar input and albedo, and compare it with the measured surface temperature
  • Explain which gases absorb outgoing radiation and why the main constituents of air do not
  • Read an energy budget diagram and check that the incoming and outgoing terms balance

1 · Read

Earth keeps an energy budget: sunlight streaming in against infrared glowing out. A planet settles at the temperature where those two tallies match. Work the simple model with plain physics and you get a surprise: the balancing number is colder than the world you live in, well below freezing. That gap is not a mistake in your maths. Predict a number, compare it with measurement, and let the mismatch tell you what the model lacks.

The missing piece is the air itself. Earth glows back toward space in infrared, which your eyes cannot see. Gases such as carbon dioxide and methane soak up some of those wavelengths and reradiate in all directions, sending part of the energy back toward the ground. Most of the air lets the glow pass through untouched. A gas holding only a tiny fraction of the sky can still steer the whole climate, because it does the catching.

Try it together

Venus is the same physics pushed to an extreme. It wears air about ninety times thicker than ours, made almost entirely of carbon dioxide beneath permanent cloud. Sunlight filters down as dim red twilight, but the ground's heat cannot easily escape, and the surface roasts near 460 degrees. Deep time agrees: billions of years ago the Sun shone dimmer, yet rocks show liquid water, which the old stronger greenhouse explains.

Good to know

Read any energy diagram with a checker's eye. Start from sunlight, subtract what reflectivity bounces away, and match the rest against outgoing glow. Incoming must equal outgoing, or the planet would heat or cool each year. When the books balance yet the surface stays warmer than the bare number, name the gap: trapped heat returning downward.

Balance sunlight against glow, and the missing warmth names the greenhouse.

2 · Watch

Take it off screen

Print a worksheetA4 with an answer key page for grown-ups. No screen, no internet.

Where it sits

Where this leads

Jobs that lean on this skill. Follow one to see everything it is built on.

Then practise

8 questions wait behind this lesson, each with its answer explained. Every answer feeds the sky: stars light as they are learned, and dim when it is time to come back.

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Earth's Energy Balance and the Greenhouse Effect, Quantified · Science, ages 16 to 17 · LightMySky