Evolution of Our Atmosphere

Earth’s atmosphere has changed dramatically over billions of years. The atmosphere we have today was formed through volcanic activitylife processes, and chemical reactions.

 


Stage 1: Early atmosphere (like Mars or Venus)

  • The early Earth was covered in volcanoes, which released gases
  • The atmosphere was mostly carbon dioxide (CO) with very little or no oxygen
  • It also contained nitrogenwater vapour, and small amounts of methane and ammonia
  • Very similar to the atmospheres of Mars and Venus today
 

Stage 2: Water vapour condensed to form oceans

  • As Earth cooled, water vapour condensed and formed the oceans
  • CO dissolved into the oceans and formed carbonates
  • Some carbon was locked into sedimentary rocks and fossil fuels
 

Stage 3: Life begins – oxygen increases

  • Algae and plants evolved and carried out photosynthesis:
    CO
    + HO O + glucose
  • This reduced carbon dioxide levels and released oxygen
  • Over time, oxygen levels increased, allowing animals to evolve
 

Stage 4: Atmosphere today

Today’s atmosphere is made up of:

  • ~78% nitrogen
  • ~21% oxygen
  • ~1% other gases (argon, carbon dioxide, etc.)
 

💡 Human activities (like burning fossil fuels and deforestation) are now changing the atmosphere again, increasing carbon dioxide levels.

Questions 

  1. What gas was most abundant in the early atmosphere?
  2. What formed when water vapour condensed?
  3. What process started adding oxygen to the atmosphere?
  4. Name one place where carbon is now ‘locked away’.
  5. What percentage of the atmosphere is nitrogen today?

Summary 

  • The early atmosphere was rich in carbon dioxide with no oxygen
  • Volcanic activity and cooling formed the oceans
  • Photosynthesis by algae and plants increased oxygen and reduced CO
  • Carbon became locked in sedimentary rocks and fossil fuels
  • Today’s atmosphere is mainly nitrogen (78%) and oxygen (21%)