Earth´s Early Atmosphere
- Theories on the development of Earth’s atmosphere have developed over time as instrumental analysis has improved
- The surface of the early Earth was molten for millions of years during which time there was no atmosphere surrounding the planet
- Eventually cooling began to take effect and allow for molten materials to slowly solidify forming land masses
- Volcanoes formed on the land masses and released gases from the Earth’s interior through violent eruptions
- Earth’s gravity prevented the gases from escaping into outer space and they formed the atmosphere
- Analysis of the minerals in the earth's crust enables scientists to deduce the gases present millions of years ago that helped form those minerals
- It is thought that the atmosphere at that moment in Earth’s history was similar to that of Venus or Mars today which consist mainly of CO2
- During a period of intense volcanic activity, large amounts of carbon dioxide and water vapour were released, as well as nitrogen, hydrogen, ammonia, methane and other gases.
- The early atmosphere therefore contained mainly CO2 and water vapour
- There was little or no oxygen present
Volcanoes spewed out water, carbon dioxide and other gases from the Earth’s interior
- While the surface of the Earth was still very hot the large quantities of water vapour remained in the gaseous state
- When conditions cooled sufficiently, the water vapour later condensed and fell to the surface of the Earth, forming the oceans
- Carbon dioxide is a water soluble gas (it is the gas used in fizzy drinks) and dissolves readily
- When the water vapour condensed large amounts of CO2 dissolved in the oceans
- Carbonate substances were precipitated during this process which later formed sediments
Examiner Tip
For this topic you should be able to describe how the atmosphere and oceans came about.