← Year 10 Earth and space

Where does the sunlight go?

The sun is Earth's main energy source. Some sunlight is reflected straight back to space and the rest is absorbed and warms the planet. How much is reflected (the albedo) depends on the surface: ice reflects most, oceans and forests absorb most.

Fresh snow reflects about 80% of the sunlight that hits it. The open ocean reflects about 6%. When sea ice melts, that difference matters for the whole planet.

To understand climate, start with the energy coming in.

WidthMore contexts, same idea.
EngageCommit to a prediction before you test anything. A wrong guess is fine: it shows you what to look for.

Engage: does all sunlight warm the Earth?

Sunlight reaches the Earth. What happens to it?

ExploreTry it on the board and compare what happens with your prediction.

Explore: change the surfaces

Click a surface to change it, or use the buttons. Watch the white reflected arrows and the absorbed energy.

Try it yourselfYour edits are saved in this browser.

Change the surfaces until you have seen the percentage reflected change by at least 30 points.

Use the board. This ticks when you get there.

ExplainUse the particle model to explain what you saw.

Explain: absorbed and reflected

In your book: draw sunlight hitting ice and ocean side by side, with reflected and absorbed arrows of the right sizes.

Reflects most sunlight, or absorbs most?

Fresh snow
Open ocean
Sea ice
Dark forest
Thick white cloud

Arctic sea ice melts and is replaced by open ocean. What happens to the energy absorbed there?

Why does fresh snow reflect most of the sunlight that hits it, while the open ocean absorbs most?

Elaborate TypicalUse the same idea in a new context.

Elaborate: the angle of the sun

The same sunlight hits the equator nearly straight on, but the poles at a low angle. Why do the poles get less energy per square metre?

Elaborate WiderUse the same idea in a new context.

Elaborate: land use

A city replaces grassland with dark roads and roofs. What happens to the local energy budget?

EvaluateLook back at your first ideas and what changed.

Evaluate: look back

Write one sentence: "At first I thought… Now I think… because…"

Revision summary

For teachers

Students identify the sun as Earth's energy source and explain why different surfaces absorb or reflect different proportions of sunlight (albedo) (AC9S10U04, node 1, a hinge node). About 18 minutes.

Open the teacher guide: answers, solutions, slides and a worksheet.

Students will be able to

Before class

A concept tutorial for introducing or revising the idea. Set the width with ?width=minimum, typical (default) or wider.

The hinge is the absorbed–reflected split: without it students can't explain why surface changes alter the energy balance (node 2), or why the greenhouse effect is about outgoing, not incoming, energy (node 3).

Board notes: surface albedos are typical values (ocean 6%, forest 15%, city 12%, grassland 25%, desert 35%, ice and snow 80%). The absorbed figure uses Earth's average incoming sunlight (340 W/m²) for the surfaces shown; the whole planet's 30% includes clouds, which the row doesn't.

Running the lesson

  1. Engage: count how many chose 'all of it warms the Earth'.
  2. Explore: ask which button changed the reflected percentage most.
  3. Explain: the melting ice question is the checkpoint.

The hard part (on purpose)

Linking a surface's albedo to how much energy it absorbs. When a student guesses from shininess, ask what percentage the board gives for that surface.

When students get stuck

Stretch and support

Stretch: Melting ice absorbs more, which warms, which melts more ice. What kind of feedback is that?

Support: Give a table of surfaces to rank by percentage reflected.

Where it leads

Next: energy balance between the spheres (node 2), then the greenhouse effect (node 3).

What each step is for

Now you can
Next lesson4. What keeps Earth's temperature steady?Earth is in energy balance when the energy it absorbs from the sun equals the energy it gives off to space as infrared. Energy moves between the spheres by radiation, conduction and convection, and the oceans store heat. Upset the balance and Earth warms or cools until it is restored.