l.o: to know what the earth’s atmosphere was like in the past and what it is like now. starter:...
TRANSCRIPT
L.O: To know what the earth’s atmosphere was like in the past and
what it is like now.
Starter: What does the air we live in consist of?
Our atmosphere has Our atmosphere has remained the same in the remained the same in the
last 200million yearslast 200million years
Carbon0.04%
dioxide Oxygen21%
Nitrogen78%
Others (Argon)0.9% and trace others
The Earth was formed about 4500 million years ago.
The very first atmosphere mainly consisted of hydrogen and helium gases.
Frozen giant planets like Saturn and Jupiter still have atmospheres like this. However on the warmer, smaller Earth these light gases were largely lost into space.
Smaller planet = less gravity (couldn’t hold on to the gases)
Saturn
Jupiter
EarthHelium
HydrogenSpace
During the first billion years on Earth there was intense volcanic activity. This produced the next early atmosphere.
It would have contained large quantities of carbon dioxide (CO2), along with methane (CH4) , and ammonia (NH3) and steam
This is rather like the atmosphere on Mars and Venus today.
The Earth’s atmosphere would also have contained water vapour which condensed to form the oceans.
Venus
CO2 CH4 NH3 steam
Mars
EarthCO2, CH4, NH3, H20
Carbon dioxide reacted with rocks and much became trapped in them.
The evolution of algae some 3000 million years ago, and subsequently plants which successfully colonised the Earth’s surface, led us towards the present atmosphere.
Their photosynthesis replaced carbon dioxide with oxygen.
Over a period of time billions of tonnes of carbon dioxide became locked up in fossil fuels.
Photosynthesis increased
oxygen levels
CO2 + ROCK
CO2 + Water Oxygen + Glucose
EarthCO2 decreases, O2 Increases, H20, CH4, NH3
As oxygen levels rose atmospheric ammonia (NH3) reacted with oxygen(O2) to form water(H2O) and nitrogen (N2)O2 + NH3 H20 + N2
As oxygen levels rose atmospheric methane (CH4) reacted with oxygen (O2) to form water and carbon dioxideO2 + CH4 H20 + CO2
Also, living organisms, including denitrifying bacteria, broke down nitrogen compounds releasing more nitrogen into the atmosphere.
And so the atmosphere headed towards a composition that has remained fairly constant for the last 200 million years.
Earth
EarthO2 increases, H20 increases, NH3 decreasesN2 increases
CH4 decreases
Oxygen normally exists as pairs of atoms (O2).
Oxygen can, however, turn into another form that has three atoms joined together. This is ozone (O3).
As oxygen levels rose, so did the amount of ozone.
This layer of ozone in the atmosphere filters out harmful ultraviolet rays from the sun. This will have allowed new organisms to evolve and survive.
3O2 2O3
Oxygen ozone
Earth
Harmful UV rays stopped
with ozone layer
Harmful UV rays reach Earth’s surface
without ozone layer
AD 2006The city of London and oxygen levels are stabilised at about 21% of the atmosphere. The oxygen level hasn’t changed for 200 million years.
Ox conc 21.0%
4 Billion years 3 Billion years 2 Billion years 1 Billion years Present day
Carbondioxide
Methane Ammonia Oxygen Nitrogen Others
Present day atmosphere contains 78% nitrogen, 21% oxygen, 1% noble gases and about 0.03% CO2
Gases
Explanation
Pictures
Evolution of the earth’s atmosphere
Answer the questions on the worksheet
1. What was the main gas in the atmosphere around 3500M years ago?
2. Where did this gas come from?
3. What process led to reduction in CO2 levels?
4. What gas protects life from harmful UV radiation?
5. What % of the present atmosphere is oxygen?
Carbon dioxide
Volcanoes
Photosynthesis
Ozone
21%
Activity