Greenhouse Effect
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Global Climate: the Earth's thermostat
For at least the past 1/2 billion years, the temperature
of Earth's atmosphere has
remained close to 25 C. Why?
The "greenhouse effect"
Certain constituents of Earth's
atmosphere are opaque to infrared radiation.
Most
important: H2O and CO2

The atmosphere is mostly
transparent to solar radiation, which heats the ground.
The ground re-radiates this heat
as infrared, which is partially blocked by the opacity
of greenhouse gasses.
The role of H2O is
complex - the most important greenhouse gas, but clouds, etc.
More CO2
-> more trapping of heat -> warmer temperatures
What is the thermostat?
The carbon cycle:

On
timescales longer than 100,000 years or so,
- CO2 combines with H2O in
air to form carbonic acid H2CO3
- carbonic acid reacts with silicate minerals in rock (chemical
weathering)
- the products of weathering are
transported to the oceans
- where they are used by plankton to produce CaCO3 (calcium
carbonate)
and
SiO2 (silica) shells
- These organisms die, sink to the
bottom of the ocean, and become sediments
- Sediments are subducted by plate
techtonic motions and melted
- Volcanism at mid-ocean ridges
and volcanoes release CO2 back
into the atmosphere
On shorter timescales, photosynthesis
removes CO2 from
the atmosphere and delivers
it to sediments
as well.
Seawater can "buffer" changes in
atmospheric CO2.
The rate of chemical weathering doubles
for each 10° C increase in temperature
Warmer temperatures lead to more
evaporation -> more rain, increasing weathering
Warmer temperatures lead to more
vegitation -> more CO2
removal
The thermostat:

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The Earth's climate is kept, more or less, at a constant temperature.
warming -> faster removal
of CO2 from the atmosphere
-> less CO2
-> cooling
cooling ->
slower removal of CO2 from the atmosphere
-> more CO2
-> warming
This process occurs on geologic timescales (100,000 years or more) and
is responsible
for returning the Earth to its natural equilibrium temperature.
What can cause a deviation?
Change in solar radiation striking Earth:
The sun is now 50% or so brighter than it
was just after the formation of the Earth.
Clouds or dust can block solar
radiation from striking Earth, reducing solar heating
Changing reflectivity of the
ground
ocean vs.
continent, snow/ice vs. rock
Change in
atmospheric composition:
Increased/decreased
photosynthesis
Volcanism
Fires
release/uptake of gasses
dissolved
in the oceans