Introduction Lecture 1 - The Earth System Flashcards

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1
Q

Summarise the Stone Age

A

-Lasted 3.4 million years
-Humans learned how to use stones
-Facilitated hunting and other tasks

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2
Q

Summarise the Bronze Age

A

-Started around 6000-3000BC
-Humans learned how to extract metal from rocks (copper and tin to make bronze)

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3
Q

Summarise the Iron Age

A

-Started around 1200BC
-Humans start extracting iron to make steel tools
-Ended around 200BC-100AD

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4
Q

Summarise the Industrial Age

A

-Lasted from 1760-1970
-Fueled by coal mining which allowed us to harness steam energy; power tools and running water
-Population increased but so too did pollution
-This began anthropogenic climate change

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5
Q

Summarise the Oil Age

A

-1901-present
-Oil extraction to fuel economy; the world is now dependent on oil

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6
Q

Summarise the Space Age

A

-1957-present
-Lunar and potentially Martian exploration
-Satellite data is a huge industry and critical for resource management and mitigation/ planning of natural disasters

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7
Q

Summarise the Information Age

A

-1970-present
-Extraction of rare earths for computers and new technology
-Economy driven by IT
-The rise of AI and machine learning

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8
Q

Summarise the Big Bang

A

-First atoms (protons and neutrons formed in the first second)
-Hydrogen, helium and small amounts of lithium and berillium are formed

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9
Q

Summarise the first Star Formation

A

-Gasses come together under gravity
-Heat and pressure fuses hydrogen atoms to create helium (nuclear fusion)
-This fusion produces heavier elements all the way up to iron

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10
Q

Summarise the first Star Deaths

A

-Some stars go supernova and produce the rest of the elements in the periodic table
-Some of these heavier elements allow planet building and therefore life

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11
Q

Summarise the Formation of the Earth

A

-Asteroids and protoplanets collide to form a primitive Earth
-Asteroid impacts, planet formation and radioactive elements provide heat
-Planetary differentiation occurs
-Water is brought to Earth by asteroids and condenses due to Earth’s position inside the habitable zone

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12
Q

Explain Planetary Differentiation

A

-Heavier metals like iron and nickel sink to form the Earth’s core
-Lighter elements rise upwards, cool and condense to form the Earth’s crust

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13
Q

Explain how we obtained knowledge of the Earth’s interior

A

-Seisimic body waves (P and S) can travel through liquids (P waves also through solids)
-Changes in density cause the waves to refract
-Density increases with depth in the Earth

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14
Q

Outline the main layers of the Earth

A

-Crust
-Mohorovicic Discontinuity
-Lithosphere
-Asthenosphere
-Transition Zone
-Core (Outer and Inner)

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15
Q

Describe the Crust

A

-Outermost layer of the solid Earth
-Oceanic crust is basaltic, 1-10km thick
-Continental crust is granitic, 30-80km thick

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16
Q

Describe the Mohorovicic Discontinuity

A

-The boundary between the crust and mantle

17
Q

Describe the Lithosphere

A

-This contains the crust and the rigid upper mantle

18
Q

Describe the Asthenosphere

A

-Plastic (able to be molded and shaped)
-This is below the lithosphere

19
Q

Describe the Transition Zone

A

-The boundary between the upper and lower mantle, around 660km deep
-Here, seismic waves change direction

20
Q

Describe the Core (Inner and Outer)

A

Outer: -Liquid
-2900-5100km deep
-Earth rotation and
convection currents here
create the Earth’s magnetic
field

Inner: -Solid
-5100-6371km deep
-Single massive crystal of
iron and nickel

21
Q

What is meant by Uniformitarianism?

A

-Natural laws and processes remain constant across space and time

22
Q

Summarise the Rock Cycle

A

-Sediments come together through compaction and cementation to from sedimentary rocks
-Sedimentary rocks become metamorphic when exposed to heat and pressure
-Metamorphic rocks are melted into magma, and then condense to form igneous rocks
-Over time, igneous, metamorphic and sedimentary rocks are broken down, through weathering and erosion, to form sediments once more