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How many stages can Earth be considered to have of atmospheric evolution
Proto-atmosphere
First atmosphere
Second atmosphere
Third atmosphere
Modern atmosphere
What is Earth’s proto-atmosphere
It is the stage following earths accretion and would have had an early atmosphere rich in He and H2 molecules
What would happen to heat within earth
The heat would have resulted in the He and H2 molecules to move rapidly and reach a velocity. While the remaining molecules would have been stripped by solar winds
What would happen during earths first atmosphere
The earths proto-atmosphere He and H2 was removed, it was gradually replaced with volcanic and cometary/meteoritic gasses making it richer in CO2, H2O, N2, NH3, and CH4
What are volcanic gases made of
Roughly 70-90% H2O with the remaining being C-S-N gasses
What would release volatiles trapped in minerals as gases emanating from volcanoes
After differentiation of the inner earth into core and mantle, melting of the mantle would release volatiles due to temperature and pressure
What is another way that some gasses would have been delivered
By comets and carbonaceous chondrites meteorites
The differentiation of the Earth to have a core would allow…
The formation of a magnetic field that helped shield the Earth from solar winds and aid with retaining light gasses in the atmosphere
During the earths second atmosphere what did the atmosphere change from
It gradually evolved to one dominated by N2 and CO2 as the H2O and NH3 levels dropped
Why would the atmospheric H2O lower
It would have lowered as the surface cooled sufficiently to allow stable liquid water (oceans, lakes, streams, groundwater)
What would atmospheric NH3 do to UV
It would’ve lowered as UV rays spilt it into molecules of hydrogen (forming H2) and nitrogen (forming N2)
Why can H2 escape into space easier than N2
H2 is lightweight and can more easily escape into space from Earths gravitational pull whereas N2 is unreactive and stable and able to accumulate in the atmosphere
What happens during the evolution of Earths second atmosphere and into the third
CO2 also transitioned from a major gas to one present only in trace amounts
How much CO2 is found in mars and Venus atmosphere
Mars : 95%
Venus : 96%
What happens as liquid becomes stable at the surface during earths second atmosphere
CO2 could dissolve in water from carbonate and bicarbonate ions, which could react with Ca2+ to form carbonate
Why is CO2 important
Due to greenhouse gas properties that retain heat in the atmosphere making the surface habitable in terms of temperature
What does earths third atmosphere mainly resulted from
It’s evolving biosphere, including the evolution of oxygenic photosynthesis, it has N2 and trace O2
What did Cyanobacteria eventually evolve
The ability to produce O2 and organic C molecules from CO2 and light energy; e allowing the release of O2 into the atmosphere
When did O2 accumulate in the atmosphere
It did not start to accumulate in the atmosphere until ca. 2.3 Ga
What is also a byproduct of the biosphere
N2 is a byproduct of the biosphere
What dominated life on the early earth
Cyanobacteria
What evidence can be found that Cyanobacteria dominated life on the early earth
The form of stromatolites - mound-shaped accumulations of microbial layers that became fossilized
What is the Great Oxidation Event (GOE)
It is geological evidence for the first accumulation of atmospheric O2 at ca. 2.3 Ga in earths iron
What the earths modern atmosphere
0.8 Ga - present
The earths atmospheric O2 remained at or near levels 1% of the present
What happened after 0.8 Ga
O2 started to accumulate to near-modern levels at roughly the time that complex multicellular life evolved
What happened throughout Phanerzonic
The O2 was variable but constrained between ~15% and 35% with current levels at 21%
This evidence comes from ancient charcoal and the presence of giant insects
Why is oxygenating earth’s atmosphere
To allow complex multicellular organisms to breathe and evolve, but also to allow the formation of an ozone layer
How does the ozone (O3) form
In a 2 step reaction in the atmosphere ~30km above the surface
O2 + soler energy
O2 + O
Why is the presence of O3 in the stratosphere important
It filters out harmful UV light from reaching the surface
What is the earths modern atmospheric composition
Nitrogen = 78.08% (78.00%)
Oxygen = 20.95% (21.00%)
Other gasses = 0.97% (1.00%)
Where can aerosol be kept
It can be kept aloft in the atmosphere
What is air pressure and how is it measured
It pushes that air that exerts on its surroundings
It is measured in units called atmospheres (atm) or bars
What is air density and how does it change the weight of the air
It is the total mass of gas molecules per unit of volume
The weight of air at higher elevation compresses air at lower elevations increasing towards the surface
Where is 99% of the atmospheres gases found
Below an elevation of 50km
What happens in high atmosphere
There are very few interactions of gas molecules with each other
What is heat
It is a form of energy. All substances are made of atoms or molecules that are in motion and have kinetic energy. It is defines as the total kinetic energy of all atoms/molecules in a substance
What is temperature
It is measured as the average kinetic energy of individual atoms/molecules in a substance. The faster atoms/molecules vibrate (or move), the higher the temperature
How is heat and temperature related
If heat energy is added to a substance, atoms move faster and the temperature increases
If heat energy is removed from a substance, atoms move slower and temperature decreases
How is heat energy transferred
Radiation
Conduction
Convection
What is radiation
A form of energy transported by electromagnetic waves that does not require a medium to transfer. It is the most important heat transfer for the atmosphere
What is convection
The transfer of heat through matter through molecular collisions, with heat transferred from higher T to lower T. Air is a conductor and the least important for the atmosphere
What is convection
The transfer of heat by mass movement or circulation in a substance. It is important for global heat transfer