Lecture 4 Flashcards

1
Q

Hadeon eon

A

“Hellish”
Planets just formed and still many planetoids
Heavy bombardment period

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2
Q

Late heavy bombardment

A

Caused by re-arrangement of planetary orbits during Hadeon eon
Late planetismals swallowed by planets

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3
Q

Earth structure

A

Core: Dense, iron and nickel core. Molten outside.

Mantle: Silicates and less dense rocks with pockets of partly molten rocks. Most of earth’s volume.

Crust/lithosphere: Outer skin consisting of igneous rocks (granite and basalt).

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4
Q

Differentiation

A

Separation of minerals by density

Heavy sink, lighter rise

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5
Q

Sources of heat in earth causing differentiation

A
  1. Impacts
  2. Gravitational energy in centre
  3. Radioactive decay of elements (Currently what keeps interior hot)
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6
Q

Processes caused by earth’s interior heat

A
  1. Volcanism: Release of gas trapped in interior and extrusion of igneous rock.
  2. Plate tectonics: Movement + recycling of rocks.
  3. Magnetic field: Shielding of atmosphere from cosmic energetic particles.
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7
Q

Escape velocity

A

More massive bodies = Larger escape velocity = Harder for gas to escape

(If planet too hot, light atoms will evaporate and fly out of atmosphere)

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8
Q

Solar wind

A

Strips off atmosphere with energetic particles from Sun.

Earth has magnetic field to protect atmosphere.

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9
Q

What is found in Earth’s atmosphere?

A
Nitrogen
Oxygen 
Water vapour
Argon
Carbon dioxide
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10
Q

Where is the earth’s magnetic field generated?

A

Core

Rapid rotation of metals causes electric current

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11
Q

Requirements for magnetic field

A

1) Molten, metallic (conductive) core
2) Rapid or moderately rapid rotation
3) Convection within globe

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12
Q

Tectonic plates

A

Moved by convection motions in mantle

Moves few cm per year

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13
Q

Continental drift

A

Alfred Wagner

Used to be one big continent

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14
Q

Subduction zone

A

Where seafloor crust material sinks under plates

Important for auto-regulation of climate

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15
Q

Seafloor crust and continental crust

A

Seafloor crust: High density, heavy igneous rock (basalt), 5-10 km thick

Continental crust: Low density, light rocks (granite), 20-70 km thick

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16
Q

Why no plate tectonics on Mercury, Venus and Mars?

A
  • High surface temp may have baked out water from crust

- Thicker crust may resist fracturing

17
Q

Greenhouse effect

A

Greenhouse gases trap and absorb infrared radiation leaving surface
(CO2 absorbs and spits out IR light, which warms up atmosphere)

18
Q

Positive or negative feedback?

More greenhouse gases -> Hotter atmosphere -> More greenhouse gases released from oceans

A

Positive

19
Q

Positive or negative feedback?

More snow snd ice -> Cooler atmosphere -> More snow and ice

A

Positive

20
Q

Positive or negative feedback?
Hotter surface temp -> More water vapour -> More clouds -> More sunlight reflected back into space -> Cooler surface temp

A

Negative

21
Q

CO2 cycle

A

1) Atmospheric CO2 dissolves in rain water
2) Acidic rain erodes and dissolves rocks. Minerals (silicate) carried by rivers to oceans
3) Dissolved oceanic CO2 reacts w/ silicate rocks to form carbonate rocks
4) Carbonate rocks pushed into mantle and heated in subduction zones. Gases (CO2) released back into atmosphere by volcanoes.
5) Back to 1)

22
Q

How does temp affect CO2 cycle?

A

High temp -> Faster weathering -> Strong CO2 removal

Low temp -> Weaker weathering -> Atmospheric CO2 buildup

(Negative feedback)

23
Q

Weakness of CO2 cycle

A

1) Has delay time of 400,00 years
2) Very slow, possibly taking millions of years
3) Prone to instabilities

24
Q

Snowball Earth

A
  • Happened 2.4-2.2 Gyr and 750-580 Myr ago

- Glaciers went down to equator and oceans froze 1 km deep

25
Q

Hypothesis for 2nd snowball earth

A

Continental drift happened to gather all continents near equator
Weathering could continue despite glaciers (more CO2 removal)
Weak greenhouse effect (low CO2) and lots of glaciers (reflection)

Become positive feedback