Geo 1012 : Planet Earth : lecture outlines
Climate I: long-term stability
Surface temperature of a planet: distance from the Sun and its albedo
Mean surface temperature of the earth
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Blackbody temperature of the earth : 5° C
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Albedo of the earth: ~ 30%
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Surface temp should be, considering the albedo effect : -25° C
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Actual mean temperature of the earth's surface: +15° C. Why?
Natural Greenhouse effect: today primarily by carbon dioxide and water vapor
Energy from the Sun:: Faint Young Sun Paradox- Problem #1
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25-30% dimmer Sun at the beginning of planet formation
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Positive feed back effects - frozen earth
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Surface temperature of the earth would be below freezing until 2 b.y. ago
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Geologic evidence of liquid water as far back as 3.8 billion years ago
What saved the earth?: Possible solutions
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Albedo lower in the past (practically 0!)
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Greenhouse effect larger in the past
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Solar evolution models might be wrong
Early Greenhouse?
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Possible greenhouse gas: carbon dioxide as an early greenhouse gas
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Needed amount is ~1000 times that today (0.3 bar vs. 3.5 x 10-4 bar today)
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Do we have enough carbon in the earth?
Carbon reservoirs in the earth
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Most of earth’s carbon is locked up in rocks
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Maybe this was available to the atmosphere to increase greenhouse effect
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Vocanic emissions today and in the past
What happens when the Sun gets brighter - Problem #2
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Positive feedback effect-boiling ocean
The record of climate in the earth - always had water, but -----oscillations
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Strong record of extensive glaciations in the last million years
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Ice cover over a substantial portion of the N. American continent
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Evidence from ancient glaciations
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Strong warm climate in the Cretaceous
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No ice caps at poles-temperate climate all the way to the poles
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Why did it not go into a frozen or steamhouse mode?
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The presence of thermostat
Long term stability of the earth's climate: The Earth's Thermostat
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Continental crust made up of K, Na, Mg, Fe, Ca silicates
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Chemical erosion of land : H2O, CO2 , and reactions with Ca-silicate rocks
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Transport of Ca2+, HCO3-, SiO2 ions into the ocean
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Inorganic and organic precipitation of CaCO3 and SiO2 as skeletal parts
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Cycling of products due to plate-tectonics
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Formation of Ca-silicate (rocks) and CO2 and introduction into the atmosphere
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Influences the CO2 content of the atmosphere
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Controlling mechanisms
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plate-tectonics for input of CO2
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Supply of Ca to oceans
Checks and balances - equilibrium
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consequences of input faster than removal as carbonate
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increase in atmospheric CO2
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warmer planet
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wetter planet as warm air holds more water vapor
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more CO2 in soils due to increased plant cover
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more soil mineral dissolution
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increase in rate of input of Ca into oceans
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Removal of CO2 as Calcium carbonate
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less CO2 in the atmosphere and cooling of the planet
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consequences of input lower than removal as carbonate
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decrease of atmosphercic CO2
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cooler planet
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less chemical erosion and less Ca and HCO3- to oceans
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lessened removal as carbonate
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Build up of CO2 in the atmosphere to warm up the planet
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