Chapter 6- Earth evolution and Earth structure Flashcards

(67 cards)

1
Q

solar system

A

consists of the sun, planets, moons, comets, and asteroids

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2
Q

sun

A

a star composed of hydrogen and helium, largest object in the solar system, making up 99.8% of the total mass of the solar system

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3
Q

Planet

A

a sizeable objects orbiting a star, massive enough to have it’s own gravity

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4
Q

moon

A

/natural satellite, body that orbits a planet

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5
Q

asteroids

A

rocky objects which failed to form a planet

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6
Q

meteorites

A

rock fragments which fall to earth from space

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7
Q

comet

A

composed of ice and dust. outer layer melts into water vapour as it gets closer to the sun

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8
Q

Density/Composition/Comparison of metallic meteorites

A

7.0-8.0 gcm-3. Iron and nickle with some sulfur and silicon. Similar to Earth’s core

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9
Q

Density/Composition/Comparison of stony meteorites

A

3.0-3.7 gcm-3, silicate minerals similar to peridotite, similar to Earth’s mantle. high porosity

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10
Q

Protoplanetary disc

A

rotating disc of dense gas and dust surrounding a newly formed stars

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11
Q

Planetisimals

A

solid objects in protoplanetary discs

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12
Q

protoplanet

A

moon-sized planetary body that formed within a protoplanetary disc

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13
Q

Impact crater

A

-circular with a rim of broken rock built up of ejected material
-quartz grains may be shocked or even melted
-rock strata are tilted
-material at depth is broken up
-ejected material is in an inverted sequence

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14
Q

Elastic rebound theory

A

-two parts of a solid/brittle/competent rock are under stress from opposing forces
-the body of the rock is deformed and put under strain
-energy applied is stored as elastic strain energy
-deformation continues until the stress is more than the strength of the rock and it snaps
-the two parts of the rock suddenly move relative to each other and there is displacement along the fault
-elastic strain energy that was stored is transmitted through the earth by seismic waves

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15
Q

stress

A

the force per unit area acting on/within a body

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16
Q

strain

A

the change in shape of a body in response to stress

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17
Q

seismometer

A

a device which receives seismic vibrations and converts them into a signal which can be transmitted and recorded

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18
Q

seismogram

A

paper or electronic record made by a seismograph

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19
Q

seismograph

A

a device which receives and records seismic vibrations

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20
Q

P wave properties

A

-primary, travel fastest and arrive first
-push, longitudinal/compressional waves, can travel through any type of material
-pressure, particles move together and apart (compression and rarefaction) longitudinal

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21
Q

S waves

A

-secondary, travel at 60% the speed of P waves
-Shear, the particle movement is sideways in a shearing motion, making it transverse (cannot travel through liquid)
-several, times larger in amplitude than P waves

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22
Q

L waves

A

-particles oscillate in a circular movement so the wave looses energy quickly with long distance
-travel on the surface
-low frequency, long duration, and large amplitude make them the most destructive
-long, longest wavelength of all the waves
-last, travels slower than P and S waves and arrives last

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23
Q

Formula for velocity of a P wave

A

Velocity = square root of ( (incompressibility + 3/4 rigidity) / (density) )

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24
Q

formula for velocity of an S wave

A

Velocity = Square root of ( rigidity/density )

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25
focus
origin of the earthquake
26
epicentre
point on the earth's surface directly above the focus
27
shadow zone
an area where earthquake waves are not recorded (103-142 from epicentre on either side)
28
intensity
measure of surface damage caused by an earthquake
29
mercalli scale
measures the intensity of an earthquale based on the effects felt in the area
30
magnitude
measure of the amount of strain energy released by an earthquake
31
richter scale
logarithmic scale that measures magnitude of an earthquake
32
moment magnitude scale
measures magnitude and leverage on two sides of the fault in an earthquale
33
partial melting
occurs when a small proportion (1-5%) of a rock melts, surrounding the solid crystals reduces the rigidity of the rock, enabling it to behave as rheid
34
lithosphere
rigid layer of the crust and upper mantle
35
rheid
non-molten solid that deforms by viscous or plastic flow
36
low velocity zone
characterized by low seismic velocities, below 100km
37
asthenosphere
layer of the mantle below the lithosphere
38
lithophile
aluminium, calcium, potassium, magnesium, sodium, chlorine, oxygen, silicon very reactive, combine readily with oxygen to form oxides (commonly)
39
siderophile
cobalt, gold, iron, nickle high density transition metls, combine with iron easily, found deeper in the crust so less common on the surface
40
chalcophile
silver, copper, mercury, lead, sulfur, tin, zinc combine with sulfur to form high density sulfides crustal abundance is increased by secondary enrichment
41
atmosphiles
nitrogen, noble gases, hydrogen, carbon liquids/gases found at/above the surface
42
Kimberlites
fine crystal size, ultramafic igneous rocks
43
ophiolite suite
section of oceanic crust and upper mantle broken off and attached to the edge of a continent during plate movement
44
peridotite
an ultramafic igneous rock composed of olivine and pyroxene
45
Direct evidence of the composition of the earth
-Crust beneath our feet -mines and boreholes -volcanoes bringing magma up from depth -ophiolite suites -deep boreholes-
46
Cases studies for superdeep boreholes
-Project Mohole, an attept to reach the moho layer, failed due to increasing costs -Kola superdeep borehole, aimed for 15km, reached 12,200 m at which point the temperature was higher than expected (300'C) and the rock was too plastic for the drillbit to be effective
47
Indirect evidence of the structure of the earth
Density Gravity surveys (gravity anomalies and isostasy)
48
isostasy
theoretical state of equilibrium between the Earth's lithosphere and asthenosphere such that the litho 'floats' at an elevation that depends on its thickness and density. The less dense continents rise to a higher elevation than the denser ocean floors, although the pressure exerted on the asthenosphere is the same
49
Isostatic rebound
rising up on land masses that were once depressed by ice sheets
50
subduction
process where one section of the lithosphere is forced down beneath another
51
slab pull
process where cold dense section of lithosphere sinks into the mantle
52
hot spot
area of high heat flow over a mantle plume
53
thermal flux
measures in watts/square meter or milliwatts/square metre rate of heat energy transfer
54
advection
thermal energy is transferred through a medium by a fluid important close to mid ocean ridges where sea water is drawn down into the crust and replaces rising hydrothermal fluids
55
convection
thermal energy is transferred by a substance (fluid/rheid) due to buoyancy differences within the substance hot material expands, density reduces, and material rises whilst colder denser material sinks under the influence of gravity important in the mantle, atmosphere and ocean more efficient than conduction or advection
56
conduction
thermal energy is transferred through a substance with no overall movement of the substance energy is transferred from atom to atom down the thermal gradient slower than advection or convection
57
why is the interior of the earth hot
heat and formation of the earth radioactive decay
58
electromagnetic surveys
an alternating current is passed through a primary transmitting coil, a magnetic field is induced and spreads into the ground inducing a secondary current in any underground material that can act as a conductor the current sets up an alternating secondary magnetic field, which is detected by the secondary receiving coil
59
seismic tomography
builds up a 3d model by analysing the behaviour of seismic waves as they pass through sections of a body
60
continental roots
tomography models of continents show that at depth under mountain ranges the seismic velocity is higher than expected. supports the theory of isostasy suggesting mountains have cold roots which extent into the mantle
61
curie point
temperature above which magnetic materials loose their permanent magnetism. around 500'C
62
remanent magnetism
recorded in rocks due to their alignment of magnetic minerals according to the earths magnetic field at the time of their formation
63
palaeomagnetism
ancient magnetism preserved in rocks
64
magnetometer
an instrument which detects the strength and direction of the magnetic field
65
magnetic inclination
angle of dip of the lines of a magnetic field
66
origin of the earths magnetic field
the temperatures of the core are above the curie point so can't be a permanent magnet temperature difference between the inner core (5700) and the outer core (3500) induces convection currents in the liquid outer core. the move mass of molten iron generates electricity which induces magnetism, generating more electricity and so on balance between generation and destruction allows the earth to maintain a continuous magnetic field
67