lecture 24. forces stabilizing climate, carbonate-silicate cycle
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Lecture 24. Forces Stabilizing Climate, Carbonate-Silicate Cycle. reading: Chapter 4. Forces Stabilizing Climate. Presence of an atmosphere What happens on the Moon? How does an atmosphere stabilize climate during day and night? What happens when you have a ticker atmosphere? - PowerPoint PPT PresentationTRANSCRIPT
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reading: Chapter 4
Lecture 24. Forces Stabilizing Climate, Carbonate-Silicate Cycle.
Forces Stabilizing Climate
1. Presence of an atmosphereWhat happens on the Moon?How does an atmosphere stabilize climate during day and night?
What happens when you have a ticker atmosphere?What happens when you have a thinner atmosphere?
Seasons are Caused by Tilt (also called Obliquity)
ecliptic = plane of thesolar system
More solar radiation in the summerLess solar radiation in the winter
Earth’s tilt angle: 23.5˚
Forces Stabilizing Climate, cont.
2. Having a large Moon
Moon very large compared to the Earth and other Moons.The Moon stabilizes the tilt of the Earth.This stabilizes the seasons.
animation
Forces Stabilizing Climate, cont.
Mars:Currently Mars’ tilt is 25˚No large Moons (2 tiny Moons: Deimos and Phobos)Tilt is highly variable - chaotic.Tilt varies between 0-60˚ on timescales of tens of
thousands of years/millions of years
ecliptic = plane of thesolar system
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Mars at High and Low Tilt Angles
today
high tilt angle
low tilt angle
Forces Stabilizing Climate, cont.
3. The Carbonate-Silicate Cycle
Unique feature of the Earth -is a result of:
a. plate tectonicsb. volcanismc. having oceans
Where does most CO2 come from?
} having a geologically active planet
Plate Tectonics
Forming Carbonate Rocks
CO2 + H2O ---> H2CO3 (carbonic acid, dissolved in rainwaterand in the oceans)
Ca2+ + H2CO3 ---> CaCO3 + 2H+ (limestone + acid)
Where is most of the CO2 in the Earth?1x tiny bit in atmosphere (270 ppm)50x dissolved in the oceans30,000x deposited as carbonate rocks (sedimentary rock)1.7 millionx dissolved in the mantle
If we were to put all carbonate rocks into the atmosphere, wouldhave an atmosphere similar to Venus.
Silicate/Rock Weathering
CaSiO3 + 2H2CO3 ---> Ca2+ + 2HCO3- + SiO2 + H2O
silicate carbonic ions quartz rock acid
Another type of silicate rock:
2KAlSi3O8 + 2H2CO3 + 9H2O ---> 2K+ + 2HCO3- + 4H4SiO4 + Al2Si2O5(OH)4
feldspar carbonic ions quartz clay acid
Acid weathering of rocks produces ions (Ca2+, K+, Fe2+, Mg2+, etc.).Ions washed into rivers and the oceans (ocean salinity).Clays and quartz are produced.Ions combine with H2CO3 to produce limestone.
Forming Carbonate Rocks
CO2 + H2O ---> H2CO3 (carbonic acid, dissolved in rainwaterand in the oceans)
Ca2+ + H2CO3 ---> CaCO3 + 2H+ (limestone + acid)
Today:Much of the limestone is biogenic (coral reefs, shells)Some of the limestone is abiogenic.
Subduction
CaCO3 + SiO2 ---> CaSiO3 + CO2
limestone quartz silicate rock
metamorphic reaction: occurs at high T and P
The Carbonate-Silicate Cycle
1. CO2 outgassing from volcanos (greenhouse gas)2. CO2 dissolves in rain, lakes, streams, turns into carbonic acid3. Carbonic acid reacts with rocks, making ions, quartz, and clay4. Ions and dissolved CO2 reacts to make carbonate rocks5. Carbonate rocks are subducted6. Subducted carbonate rocks turned into CO2
How Does this Cycle Stabilize Climate?
CO2 + H2O ---> H2CO3 (carbonic acid, dissolved in rainwaterand in the oceans)
Ca2+ + H2CO3 ---> CaCO3 + 2H+ (limestone + acid)
At high temperatures, more limestone is precipitated.More CO2 dissolves in the oceans.This cools climate and lower temperatures.
} negative feedback loop
CO2 Constantly Replaced By Subduction
Earth’s Climate Is Obviously Not That Stable
1. The tilt undergoes precession (spinning like a top)Alters how much solar radiation each hemisphere
receives during summer and winter.Cycles: 20,000 years
2. There are small variation in the Earth’s tilt21.5 to 24.5˚Cycles: 40,000 years
3. Small variation (5%) in Earth’s eccentricityChanges the distance to the Sun, higher heating when closer.Cycles: 100,000 years
Milankovitch cycles - couldtrigger ice ages.
reading: Chapter 4
Lecture 25. Snowball Earth vs. Slushball Earth..