Lecture 3: Plate Tectonics 1

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Plate Tectonics 1
September 10, 13,700,002,008
The earth history of our planet
for the last 4.2 Ga:
slow cooling
Slow cooling of the
earth
mantle temperatures
have declined
from 1580 degC
to 1375 degC
in the last 4.5 billion
years
Sources of heat
initial heat
radioactive decay
gravitational settling
All sources are dying away …
Evolution of earth in last 4 Ga
Is primarily consequence of the cooling
process
Key character of cooling is
“Convection”
Convection
cold
cold cold
cold
cold cold
Conditions Necessary for Convection
cold
cold
cold
cold
cold
1) Gravity.
2) A fluid that experiences changes in density as its temperature
changes.
3) A heat source within or at the bottom of the fluid.
Results of Convection
cold
cold
cold
cold
cold
1) Heat is transferred from bottom to top of fluid (flux of heat)
2) The fluid circulates
3) regions of upwelling & downwelling, divergence and
convergence (i.e. flux of fluid)
Convection with Lithosphere
cold
cold
cold
cold
cold
1) Lithosphere is cold, stiff, brittle region at top
2) Subduction zone: downwelling, convergence of plates
3) Ridge: upwelling, divergence of plates
Lithosphere in 3D
700 km
Comparison of Convection in Atmosphere and Solid Earth
Phenomenon
Atmosphere
Mantle
Material
Air
Mg-Fe silicate rock
“Peridotite”
Driving force
Bouyancy
Bouyancy
What changes
density
Temperature
& water content
Temperature
& depletion
Heat source
Sunlight
Radioactive decay
Rate of heat
transsport
1000 watts/m2
0.1 watts/m2
Phenomenon
Atmosphere
Mantle
Speed
1 m/s
3x109 cm/year
1 cm/year
6 deg-C/km
1 deg-C/km
Lapse rate
Coriollis important Yes
No
Phase change
Peridotite melts
to make magma
Water condenses
to make rain
After phase change Dry air
is heavier
Depleted peridotite
is lighter
Phenomenon
Atmosphere
Mantle
Effects of flow
Wind makes
ocean waves
& sand dunes
Flowing mantle
moves continents
Small scale
Features
Tornadoes
Mantle plumes
Human viewpoint
From the bottom
From the top
Comparison of Convection in Atmosphere and Solid Earth
Magma is Solid Earth’s
version of “rain”
Rain vs. magma
rain …
rising moist air
adiabatically cools
crosses vapor-liquid
phase boundary
water droplets form
are negatively bouyant
and fall down as rain
Leaves dry air behind
magma …
rising undepleted mantle
adiabatically cools
crosses solid-liquid
phase boundary
liquid rock droplets form
are positively bouyant
and rise up as magma
Leaves depleted mantle
behind
Lithosphere – brittle top of part of the
earth – is a key feature of our planet
that makes its style of convection
different than “bubbling soup”
Lithosphere: about
100 km thick
asthenopshere: about
600 km thick;
vigorous convection
Deeper mantle is
more viscous and
convects more slowly
Brittle Material
cracks or faults instead of flows
Please memorize
these fault configurations and names
Crustal Movements
measured through GPS
Schematitic GPS
velocities of the ground
10 mm per year
Schematic earth
“Plates”
Really spherical caps
Large sections of the
lithosphere sliding over
the lithosphere
Schematic map
Plate 3
Plate 1
Plate 2
Schematic map
The plate boundaries
are regions of active
tectonism
All motions are a type
of rotation or spinning
of the cap about a pole
of rotation
Schematic map
Lithosphere is organized into
plates that rigidly move
Measured with GPS
Inferred from geology
Four Plates in this Diagram
Divergent Plate Boundaries
plates are moving apart
Is a gap created as they move apart?
Convergent Plate Boundaries
plates are colliding
What happens to the excess material?
Transform Plate Boundaries
plates are sliding past one another
Is a gap created as they move apart?
Plate Motion in the Past
http://www.ucmp.berkeley.edu/geology/anim1.html
Earth Scientists have worked out the history of the earth’s plate
motions for the most recent a billion years or so of earth history
but the farther back in time
the more crudely the plate configuration is known
Why Melting?
(The Mantle’s Rain)
Geological evidence for extension is very common at divergent
plate boundaries
on the sea floor at a divergent boundary
Geological evidence for volcanism is very
common at divergent plate boundaries (e.g. this
sea floor hot spring)
Divergent
plate
boundary in
the ocean is
called a
mid-ocean
ridge
5000 km
200
Ma
0 Ma
200
Ma
Flank
old & cool
Crest
young & hot
Flank
old & cool
Thermal Contraction
Ridge Crest: Hot Lithosphere: 1300C
Ridge Flank: Cold Lithosphere: 800C
Change in temperature: 500C
Thickness of lithosphere 100 km = 105 m
Thermal contraction coefficient of rock: 310-5 per C
Thermal contraction: 310-5  105  500 = 1500 m
Ridge flank should be about 1500 meters below the crest
Depth-Age Relationship
Shape of ridge is explained by cooling
of initially hot lithosphere emplaced at
ridge axis
If you know the age of a patch of sea
floor, you can predict its depth to
amazing accuracy!
Ridge crests – young – little sediment
Flank – old – thick sediment
Mid-Atlantic
Ridge
Divergent Plate Boundary on a Continent
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