Earth's Interior and Magnetics Flashcards

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1
Q

earth’s internal structure

A
  • Crust – the outer layer of rock that forms a thin skin on Earth’s surface
  • Mantle – thick shell of dense rock that separates the crust above from the core below
  • Core – the metallic central zone of the Earth
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2
Q

how to get direct evidence of earth’s interior

A
  • mining
  • drilling
  • physical samples (kimberlites, xenoliths, opiolites)
  • remotely sensed evidence (deep earth geophysical models: seismic waves, magnetism, gravity)
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3
Q

mining

A
  • Deepest mine in the world: 3.9km deep - TauTona Gold mine

- High temperatures (up to 55 degrees C) and pressure on rocks

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4
Q

drilling

A
  • Take a core sample -> cylindrical section of rock taken with a hollow steel tube called a core drill
  • We’ve drilled up to 12.5km (Kola superdeep borehole)
    • Found water that originated from rock minerals
    • Found microscopic fossils
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5
Q

kimberlites

A
  • Igneous bodies/volcanic rocks formed from mantle melts (>150km deep) that ascend quickly towards earth’s surface and crystallize
  • Gives us a sample of composition of mantle rocks, and diamonds
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6
Q

xenoliths

A
  • Small fragments of crustal or mantle rocks that are picked up again in an ascending magma – evidence for composition, pressures, and temperatures at depths within earth
  • Ex. Peridotite xenolith in basalt
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7
Q

ophiolites

A
  • Slivers of preserved oceanic crust that indicates its structure
  • Sometimes young ocean crust or ocean crust between 2 colliding continents gets “obducted” rather than subducted
  • Sections of ocean crust snipped off and preserved on a continent
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8
Q

studying interior of the earth

A
  • Deep interior of earth must be studied indirectly
    • Direct access to crustal rocks and small upper mantle fragments brought up igneous activity
    • Can only drill so deep (not to the mantle)
  • Geophysics: branch of geology that studies interior of earth
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9
Q

how do we know earth isn’t a uniform solid?

A
  • if it were, P-wave, s-wave, and surface waves would arrive at a station at the same time, and we would compute body wave arrival time at different seismometers
  • but that doesn’t happen -> we get seismic reflection and refraction
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10
Q

seismic reflection

A
  • occurs if there is a contrast in seismic wave velocity. The strength of the reflection depends on contrast in density
  • 2-way travel time is used to calculate distance to reflection surface
  • Seismic waves travel fastest through dense materials (ie. Igneous rocks)
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11
Q

seismic refraction

A
  • bending of seismic waves as they pass from one material to another having different seismic wave velocities
  • Curved energy pathways
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12
Q

evidence for existence of the core

A
  • seismic shadow zones: specific areas on the opposite side of the Earth from large earthquakes do not receive seismic waves
    • P‐wave shadow zone (103°‐142° from epicenter) explained by refraction of waves encountering core‐mantle boundary
    • S‐wave shadow zone (≥103° from epicenter) suggests outer core is a liquid (s-waves can’t travel through liquids)
  • careful observations of P‐wave refraction patterns indicate inner core is solid
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13
Q

evidence for core’s composition

A
  • composition inferred from its calculated density, physical and electro-magnetic properties, and composition of meteorites
  • Iron metal (liquid in outer core and solid in inner core) best fits observed properties
  • Inner core probably solid due to great pressure
  • Probably slowly growing as core cools: about 100 degrees C per billion years
  • Temperature is about 5400 degrees C -> temp. Of surface of the sun
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14
Q

evidence for core-mantle boundary

A
  • boundary/”D” layer is marked by great changes in seismic velocity, density, and temperature
  • Hot core may melt lowermost mantle or react chemically to form iron silicates in this seismic wave ultralow-velocity zone (ULVZ)
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15
Q

geothermal gradient

A
  • Geothermal gradient: temperature increase with depth into earth
  • tapers off sharply beneath lithosphere
  • Due to steady pressure increase with depth, increased temperatures produce little melt except the outer core
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16
Q

evidence for magnetic field

A

1) Earth is rotating – liquid metallic outer core is moving and the electrical charges in it are moving too
2) Convection of material between the (hot) lower boundary (inner core‐outer core) and (cooler) upper boundary (core‐mantle)
- Moving charges induce a magnetic field, which helps drive movement in the outer core

17
Q

magnetic field in outer core

A
  • Outer core probably flowing in large convection currents
  • Fluid channelled into rolls by earth’s spin – magnetic field direction
  • Travel several kms per year – million times faster than mantle convection
  • Moving mantle generates an electrical current which in turn generates earth’s magnetic field – the Dynamo effect
18
Q

ways to measure magnetic field

A

Magnets, compasses, and magnetometers

19
Q

compasses

A
  • A compass needle points in the direction of the horizontal component of the magnetic field where the compass is located
  • The needle is weighted to remain horizontal despite the pull
20
Q

declination vs. inclination

A
  • Declination: the angle made between the Magnetic North at that point and the True North (geographic north) -> varies with latitude and longitude
  • Inclination: angle between the magnetic field’s force line and the surface of the earth -> varies with latitude
21
Q

is the magnetic field fixed?

A
  • Depends on scale of thinking
  • Changes recorded through geological time and observed in the rock record (Paleomagnetism)
  • Magnetic minerals record the orientation of the magnetic field at the time of formation of minerals
  • Older rocks contain magnetic minerals that show significant variations in terms of polarity (which way was North) and orientation
22
Q

magnetic striping

A

tells us that convergent boundaries are spreading

23
Q

recording variations in earth’s magnetic field; polar wander

A
  • “normal”: same as today
  • “reversed”: opposite direction
  • Polar wander: over shorter timescales we can observe the movement of the Earth’s geomagnetic North pole (up to 10s of kms per year)
24
Q

what do magnetic anomalies tell us?

A

Useful in near surface studies to make inferences about subsurface structures and rocks