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Origin of the Earth's Atmosphere

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Origin of the Earth's Atmosphere 1. Hot Why? - Primordial heat, collisions and compression during accretion, decay of short-lived radioactive elements – PowerPoint PPT presentation

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Title: Origin of the Earth's Atmosphere


1
Origin of the Earth's Atmosphere
1. Hot
Why? - Primordial heat, collisions and
compression during accretion, decay of
short-lived radioactive elements
Consequences - Constant volcanism, surface
temperature too high for liquid water or life as
we know it, molten surface or thin, unstable
basaltic crust.
2. Atmosphere - early atmosphere probably
completely different in composition (H2, He)
3. Cooling
Primordial heat dissipated to space
Condensation of water (rain), accumulation of
surface water.
Accumulation of new atmosphere due to volcanic
out gassing
2
Evolution of the Atmosphere
Atmosphere - Envelope of gases that surrounds the
Earth. Used by life as a reservoir of chemical
compounds used in living systems. Atmosphere has
no outer boundary, just fades into space. Dense
part of atmosphere (97 of mass) lies within 30
km of the Earth (so about same thickness as
continental crust).
3
First Atmosphere
1. Composition - Probably H2, He
2. These gases are relatively rare on Earth
compared to other places in the universe and were
probably lost to space early in Earth's history
because
a.Earth's gravity is not strong enough to hold
lighter gases
b.Earth still did not have a differentiated core
(solid inner/liquid outer core) which creates
Earth's magnetic field (magnetosphere Van
Allen Belt) which deflects solar winds.
3. Once the core differentiated the heavier
gases could be retained
4
Second Atmosphere
Produced by volcanic out gassing
No free O2 at this time (not found in volcanic
gases).
Gases produced were probably similar to those
created by modern volcanoes (H2O, CO2, SO2, CO,
S2, Cl2, N2, H2) and NH3 (ammonia) and CH4
(methane)
5
Addition of O2 to the Atmosphere
Today, the atmosphere is 21 free oxygen. How
did oxygen reach these levels in the atmosphere?
Oxygen Production
a. Photochemical dissociation - breakup of water
molecules by ultraviolet
b. Photosynthesis - CO2 H2O sunlight
organic compounds O2 - produced by
cyanobacteria, and eventually higher plants -
supplied the rest of O2 to atmosphere.
6
Chemical Composition Today - Nitrogen (N2)- 78,
Oxygen (O2)- 21, Carbon Dioxide (CO2) - 0.03 ,
plus other miscellaneous gases (H2O for one).
7
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