Earth and other planets Flashcards

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1
Q

Formation of elements timeline

A
  1. Big bang: Protons and neutrons form followed by H, He and Be
  2. Star formation: Gases come together under gravity, heat/pressure rise and fuse H into He, nuclear fusion produces heavier elements up to Fe
  3. Death of stars: Large stars explode in a supernova, producing last of the heavy elements.
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2
Q

Planet formation, Accretion

A
  1. Rock formation from compression of dust

2. Rocks begin colliding, because of runaway gravity, and combining

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3
Q

Planet formation, Differentiation

A
  1. Heat melts the planet
  2. Heavy elements like Fe and Ni sink to the centre of the molten planet.
  3. Lighter elements rise to the crust
  4. Eventually, the crust cools
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4
Q

During differentiation of a planet, how do the gain enough heat?

A

Formation of the planet itself, asteroid impacts and radioactive elements

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5
Q

Structure of the earth (outside to inside), plus key property of each layer

A

Hydrosphere and atmosphere - Oceans and air
Crust - Solid rock
Mantle - Mostly solid rock, made of silicate minerals
Outer core - Liquid Fe and Ni
Inner core - Solid single crystal of Fe and Ni

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6
Q

4 types of seismic waves

A

Primary, secondary, love and rayleigh

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7
Q

P-waves

A

Faster than s-waves
Travel through solid AND liquid
Particles move in direction of travel
Refract when moving into liquids

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8
Q

What is the name of waves where particles move in the direction of travel?

A

Compressionable waves

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9
Q

S-waves

A

Slower than p-waves
Can’t travel through liquids
Particles move perpendicular to direction of travel

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10
Q

S-waves and imaging the earth’s core

A
  1. S-waves don’t travel through liquid

2. There is an s-wave shadow zone below epicentre suggesting liquid outer core

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11
Q

P-waves and imaging the earth’s core

A
  1. P-waves travel through liquids but refract as they enter them
  2. Another refraction of the waves as they travel through the earth shown by gaps in P-wave shadow zones.
  3. This suggests solid and liquid layers to the core
  4. Because s-waves cannot travel through liquid, and has a larger shadow zone, outer layer must be liquid and the inner solid
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12
Q

Moho discontinuity

A

Boundary between crust and mantle

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13
Q

Lithosphere

A

Consists of crust and rigid mantle

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14
Q

Asthenosphere

A

Consists of soft part of upper mantle, below lithosphere

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15
Q

Transition zone

A

Boundary between upper and lower mantle

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16
Q

Formation of atmosphere

A
  1. Volcanic degassing
  2. Comets and asteroids carrying materials onto earth
  3. Presence of life, i.e. respiration/photosynthesis
17
Q

Definition of a rock

A

Naturally occurring solid composed of at least one mineral

18
Q

Definition of a mineral

A

Solid, ordered crystal structure, naturally occurring, inorganic, characteristic chemical composition

19
Q

Igneous rock

A

Formed from freezing magma

20
Q

Sedimentary rock

A

Forms when rocks are broken down, transported and redeposited

21
Q

Metamorphic rock

A

formed by adding heat and pressure to igneous and sedimentary rock

22
Q

Ages of rock, relative ages: Law of superposition

A

In undeformed stratigraphic sequences the oldest rock is at the bottom

23
Q

Ages of rock, relative ages: Cross cutting

A

If a rock unit crosses across other rocks, that rock must be younger

24
Q

Ages of rock, absolute ages: Radiometric dating

A

Radioactive isotopes half lives can be used to calculate when a rock was formed by observing the ratio of parent to daughter elements

25
Q

Climate definition

A

The weather conditions prevailing in an area, in general, over a long period of time

26
Q

Weather definition

A

State of the atmosphere at a particular place and time