Quiz 3 Flashcards
Why is Earth so much colder than Venus?
- The albedo is 30%
- atmosphere is 90 times less dense
- atmosphere has 0.04 (96% CO2 on Venus)
- the greenhouse effect is 33°C.
How do we know that Earth was not frozen over its history in spite of much weaker early Sun?
- Evidence from water-deposited sedimentary rocks
- Primitive life dates back to 3.5 billion years
What is the Faint Young Sun Paradox?
It talks about how the early Sun shone 25% to 30% weaker than today along with climate models showing that Earth should have been frozen even with greenhouse gases present.
How does chemical weathering work as a CO2 removal mechanism?
Chemical weathering of silica-rich rocks on the continents removes CO2 from the atmosphere, and part of the carbon is later stored in the shells of marine plankton and buried in ocean sediments.
What is the Snowball Earth hypothesis?
It is located in continents in low latitudes and there is increased rainfall and extreme chemical weathering.
What are the Characteristics of Venus?
- The mean surface temperature 460°C
- it receives 1.93 times more solar radiation
- sulfuric acid clouds reflect 80% of incoming radiation
- receives 50% of radiation received on Earth
- the greenhouse effect is 285°C
What are examples of Greenhouse gases?
CARBON DIOXIDE CO2 (0.04%) METHANE CH4 (0.00018%) WATER VAPOR (~1-3%)
THE GREENHOUSE EFFECT
- The greenhouse gases absorb outgoing IR radiation
- Atmosphere radiates thermal IR radiation towards the surface
- lower troposphere is heated from the Earth’s surface
- greenhouse heating of Earth’s atmosphere is 32°C (Venus’ is 285°C)
- W/o greenhouse heating Earth would be solid frozen
Volcanic input
- The largest reservoir of carbon on Earth is in rocks (on Venus – in atmosphere)
- Major input of CO2 to atmosphere is from volcanic activity and hot springs
- Natural rates of CO2 input and removal are ~ balanced
- W/o this input CO2 will be removed from atmosphere in ~4,000 years
- Volcanic processes are not affected by the atmosphere
Negative feedback from chemical weathering
- When Earth’s climate warms, increased precipitation and vegetation cover increases chemical weathering
- More CO2 removed from the atmosphere, hence moderate cooling
- When Earth’s climate cools, precipitation decreases and vegetation cover becomes more sparse
- More CO2 remains in the atmosphere, hence moderate warming
Earth’s “thermostat”
- The weakness of the early Sun was compensated by much higher concentrations of CO2 due to stronger volcanic activity
- As the Sun brightened, climate warming resulted in more CO2 removed from atmosphere through chemical weathering – cooling effect
Was there a Thermostat Malfunction?
Yes there was, evidence of several glaciations on all continents between 850 and 550 million years ago.
Why are we not using the term “continental drift” suggested by Alfred Wegener in relation to the plate tectonics processes?
Lithospheric plates move across Earth’s surface at rates ranging from 1 to 10 cm per year
Earth’s magnetic field
- Earth’s magnetic field is generated by the rotating fluid outer iron core
- Geomagnetic reversals: randomly distributed; average period 450,000 years
- The last Polarity Reversal happened 780,000 years ago
- Magnetic field protects the atmosphere against depletion by solar winds
Earth’s Crust and Upper Mantle
- Oceanic crust – 5-8 km
- Continental crust – up to 35-40 km
igneous rocks
formed by cooling and solidification of molten rock
magma
general term for molten rock under the surface
lava
molten rock flows on the surface