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The Composition and Evolution of Earth's Atmosphere

Today dry air is about 78% nitrogen, 21% oxygen and about 1% argon, with tiny amounts of carbon dioxide (about 0.04%) and other gases. Earth's early atmosphere came from volcanoes: mostly carbon dioxide and water vapour, with little or no oxygen. As Earth cooled, water vapour condensed into oceans and some CO2 dissolved. Algae and later plants made oxygen by photosynthesis. Carbon was locked away in sedimentary rocks such as limestone and in fossil fuels, so CO2 fell.

🎬 Step-by-step story

  1. Air today: 100 blocks stand for 100%. 78 are nitrogen, 21 are oxygen and 1 is argon and other gases.
  2. Early Earth: volcanoes gave out gases. The air was mostly carbon dioxide and water vapour, with almost no oxygen.
  3. Earth cooled. Water vapour condensed and formed the oceans. Some carbon dioxide dissolved in the sea water.
  4. Algae, and later plants, did photosynthesis. They took in carbon dioxide and gave out oxygen, so oxygen rose.
  5. Carbon got locked in rocks: shells became limestone, and buried living things became coal, oil and gas.
  6. Try it: move the time slider and count the blocks of each colour at each time.

Tip: drag the 3D scene to turn it. Use two fingers to zoom.

🤔 Common doubts, cleared

If nitrogen is 78%, why do we talk about oxygen so much?

We need oxygen to breathe and things need it to burn. Nitrogen is very unreactive, so it mostly just stays in the air. Count the blocks: blue is the biggest group.

Where did the early gases come from?

From inside the Earth, through volcanoes. Watch the volcano in step 2 and the orange CO₂ blocks.

Where did all the water vapour go?

It condensed into liquid water and made the oceans as Earth cooled.

Why did oxygen take so long to build up?

Algae made it slowly, and at first much of it reacted with iron in rocks and the sea. Only after a very long time did it build up in the air. Watch the green blocks grow one by one in step 4.

Is the carbon in limestone really from the air?

Yes. CO₂ dissolved in the sea, sea creatures used it to build calcium carbonate shells, and the shells became limestone. Step 5 shows blocks sinking into the rock layer.

What is in the air today?

The atmosphere is the layer of gas around Earth. For about the last 200 million years its make-up has stayed nearly the same.

These numbers are for dry air. A quick check: nitrogen + oxygen ≈ 99%.

Earth's early atmosphere

Earth is about 4.6 billion years old. In its first billion years there was a lot of volcanic activity. Volcanoes released gases. Scientists think the early air was mostly carbon dioxide with water vapour, some nitrogen and small amounts of methane and ammonia. There was little or no oxygen.

This is a bit like the air of Mars and Venus today, which is mostly CO2.

Why are we not sure?

Nobody was there to measure it, and the evidence (old rocks, gas bubbles in ice, fossils) is limited. So there are different theories. This is a good example of how science uses evidence and changes its ideas.

How oxygen increased

As Earth cooled, water vapour condensed (turned to liquid) and fell as rain. This formed the oceans.

About 2.7 billion years ago, simple algae (tiny green living things in the sea) began to do photosynthesis:

carbon dioxide + water → glucose + oxygen
6CO2 + 6H2O → C6H12O6 + 6O2

Over the next billion years or so, plants appeared too. Oxygen slowly built up until there was enough for animals to live.

How carbon dioxide decreased

CO2 went down in three main ways:

  1. Dissolving in oceans: carbon dioxide dissolves in water and forms carbonates.
  2. Photosynthesis: algae and plants used CO2 to make food.
  3. Locking carbon in rocks: sea creatures used carbonates to build shells and skeletons. These piled up and became sedimentary rocks such as limestone (calcium carbonate). Buried plants became coal; buried tiny sea creatures became crude oil and natural gas.

Fossil fuels are "stored ancient CO2". Burning them returns that carbon to the air.

Try it: model the air with 100 counters

Take 100 beads, buttons or rice grains. Make 78 one colour (nitrogen), 21 another (oxygen) and 1 a third (argon and others). Put them in a jar. Now make a second jar for early Earth: mostly "CO2" counters. Swap counters one by one and say what process changed each one (dissolving, photosynthesis, locking in rock).

Key formulas and definitions

Worked examples

1. A classroom holds 200 m³ of air. Roughly what volume is oxygen?

Oxygen is about 21%. 21% of 200 = 0.21 × 200 = 42 m³.

2. Explain why there was little oxygen in the early atmosphere.

Oxygen in today's air was made by photosynthesis. Before algae and plants existed, nothing made oxygen in large amounts, and volcanoes give out CO₂ and water vapour, not oxygen.

3. Give two ways carbon dioxide left the early atmosphere and say where the carbon went.

1) It dissolved in the oceans, then formed carbonates that sea creatures used for shells; the shells became limestone. 2) Plants used it in photosynthesis; buried plants became coal. So the carbon ended up in sedimentary rocks and fossil fuels.

Common mistakes

Practice quiz

1. About what percentage of dry air is nitrogen?
2. Which gas made up most of Earth's early atmosphere?
3. Where did the oxygen in our air come from?
4. How did the oceans form?
5. Limestone is mainly:

Practice: answer these yourself

Type or choose your answer, then press Check. Use a hint if you are stuck; the full solution appears after you answer.

Frequently asked questions

What is the composition of air?

Dry air is about 78% nitrogen, 21% oxygen, 0.9% argon and 0.04% carbon dioxide, plus tiny amounts of other gases.

What was Earth's first atmosphere made of?

Mostly carbon dioxide and water vapour from volcanoes, with some nitrogen and little or no oxygen.

Why did carbon dioxide decrease?

It dissolved in the oceans, was used by algae and plants in photosynthesis, and was locked up in sedimentary rocks like limestone and in fossil fuels.

Where this is taught

England (GCSE, A level)Year 114.9 Chemistry of the atmosphere
England (GCSE, A level)Year 115.9 Chemistry of the atmosphere

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