atmosphere Flashcards

(5 cards)

1
Q

Timeline of change of the atmosphere

A
  • During first Billion years there was intense volcanic activity
  • Volcanos realsed gasses that formed early atmosphere
  • Gasses where water vapour, carbon dioxide, nitrogen
  • small amounts Methane and Ammonium
  • Earth atmosphere contained little to no oxegen, so very simular to planets like Mars and Venus.
  • Earth cooled down and water vapour developed to form the oceans
  • Some of carbon dioxide dissolved into oceans forming a weak acid
  • This reacted with minearls in the sea to form preciptates
  • Over time this formed sediments of carbonate rock on the seabed
  • Some of carbon dioxide made coral and shells of organisms
  • When they died they formed the sedementry rock limestone, while removing carbon dioxide from atmosphere
  • Level of carbon dioxide began to fall
  • Around 2.7 billion years ago the first Photosynthetic algae evolved in the oceans
  • Proccess of photosynthisis produced oxegen which entered the atmosphere
  • Plants evolved increasing amount of oxegen in atmosphere reaching point where animals could evolve
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2
Q

Pecentage of gasses in the modern atomsphere

A
  • 78% Nitrogen
  • 21% Oxegen
  • 0.04% Carbon dioxide
  • 1 perecent everything else
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3
Q

Early atmosphere

A

Lots of
- Carbon di-oxide
- Water vapour
- Nitrogen
Smaller amounts of
- Methane
- Ammonia

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4
Q

Why can scientist not be certian about the early compositon of the atomosphere

A

The earth is around 4600 million years old, that means scientist cannot be sure about the early atmosphere

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5
Q

How do greenhouse gasses work

A
  • Suns heat energy goes down onto earth in form of shortwave radiaton
  • Passes through atmosphere and hits surface of earth
  • Some of the energy is absorbed and heats up ground
  • Most is remmited or reflected into the atmosphere towards space in form of Longwave radiaton
  • Some energy makes it back to space
  • Most hits particles of Gas in atmosphere, which absorbs energy they then reimmit the energy in random dirrections
  • Some energy remmited towards spave and some towards earth
  • Most energy collides with other gas particles before leaving the atmosphere
  • Proccess repeates keeping heating earth longer than if there was no atmosphere
  • Keeps earth at stable temp
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