The Helpful Chemist

Topic 09

Chemistry of the Atmosphere

Where our atmosphere came from, how it changed, and what we're doing to it now.

4 lessons

Chemistry of the AtmosphereEvolution of the Atmosphere

Chemistry of the Atmosphere

Lesson 01 of 04

Evolution of the Atmosphere

Chemistry of the Atmosphere2 videos

Key Concepts

  • Earth's atmosphere composition
  • Nitrogen (78%)
  • Oxygen (21%)
  • Argon (approx. 1%)
  • Carbon dioxide (0.04% = 400 ppm)
  • Parts per million (ppm)
  • Atmospheric scale and structure
  • Stable atmosphere over 200 million years
  • Noble gases: neon, helium, krypton
  • Atmospheric composition
  • Volcanic outgassing
  • Evidence from Mars and Venus
  • Carbon dioxide dissolution
  • Carbonate rock formation
  • Photosynthesis equation
  • Photosynthetic bacteria
  • Rise of oxygen
  • Geological timescale

Video 1

Lesson notes

Before you can understand how the atmosphere has changed, you need to know what it's made of today. This video gives you the three main gases and their percentages in a form you can use in any question — as fractions, percentages, ratios, or parts per million — and explains why that composition has barely changed in 200 million years. Short, focused, and exactly what the GCSE specification asks you to recall.

What You Will Learn

00:12How thick the Earth's atmosphere is and why only the first few kilometres sustain human life.

02:20What the three main gases in today's atmosphere are and their approximate percentages.

02:33Why nitrogen at 78% is the most abundant atmospheric gas, not oxygen.

02:51What argon's role is and its approximate 1% share.

02:58Why carbon dioxide at only 0.04% is significant despite its small proportion.

03:19What parts per million (ppm) means as a unit and how to relate it to percentages.

05:17How long the current atmospheric proportions have been approximately stable.

05:31How to express atmospheric composition as fractions, percentages, ratios, and ppm.

Video 2

Lesson notes

Take a journey back 4.6 billion years and watch Earth's atmosphere transform from a volcanic mix of methane, ammonia, and water vapour into the nitrogen-oxygen balance we breathe today. This video walks you through each stage — from the cooling oceans locking away carbon dioxide to photosynthesis flooding the air with oxygen — and connects each change to the chemistry behind it. Essential viewing before tackling air pollution or the carbon cycle.

What You Will Learn

00:58How to describe the composition of the present-day atmosphere and identify which gases make up the remaining 1%.

02:58Why scientists cannot be certain about the exact sequence of events in the atmosphere's development 4.5 billion years ago.

04:22Why evidence from Mars and Venus supports the idea that Earth's early atmosphere was high in carbon dioxide.

06:08How volcanic activity released gases to form Earth's early atmosphere, which was mostly carbon dioxide and water vapour.

07:58How the formation of oceans caused CO₂ levels to fall by dissolving into seawater and forming carbonate rocks.

09:11What the word and symbol equations for photosynthesis are and how photosynthetic bacteria transformed the atmosphere.

10:44How to write a structured six-mark exam answer explaining the development of Earth's atmosphere.

Course Topics
General Introduction
Working Scientifically
Atomic Structure
Bonding & Structure
Quantitative Chemistry
Chemical Changes
Energy Changes
Rate of Reaction
Organic Chemistry
Chemical Analysis
Earth's Atmosphere
Using Resources