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SIO15-18: Lecture 4 Plate Tectonics SIO15-18: Lecture 4 Plate Tectonics

SIO15-18: Lecture 4 Plate Tectonicsigppweb.ucsd.edu/~gabi/sio15/pdfs/Lecture04-presentation.pdf · SIO15-18: Lecture 4 Plate Tectonics • lith. formed at MORs • lith. consumed

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Page 1: SIO15-18: Lecture 4 Plate Tectonicsigppweb.ucsd.edu/~gabi/sio15/pdfs/Lecture04-presentation.pdf · SIO15-18: Lecture 4 Plate Tectonics • lith. formed at MORs • lith. consumed

SIO15-18: Lecture 4 Plate Tectonics

SIO15-18: Lecture 4 Plate Tectonics

Page 2: SIO15-18: Lecture 4 Plate Tectonicsigppweb.ucsd.edu/~gabi/sio15/pdfs/Lecture04-presentation.pdf · SIO15-18: Lecture 4 Plate Tectonics • lith. formed at MORs • lith. consumed

SIO15-18: Lecture 4 Plate Tectonics

https://igppweb.ucsd.edu/~gabi/sio15

SIO15-18: Lecture 4 Plate Tectonics

•  Monday before class•  folders outside of lecture hall•  submit by first letter of FAMILY NAME•  email submissions not accepted!•  Q&A blog on class website!! HOMEWORK PAGE•  emailed questions on weekends may not be answered

Page 3: SIO15-18: Lecture 4 Plate Tectonicsigppweb.ucsd.edu/~gabi/sio15/pdfs/Lecture04-presentation.pdf · SIO15-18: Lecture 4 Plate Tectonics • lith. formed at MORs • lith. consumed

SIO15-18: Lecture 4 Plate Tectonics

SIO15-18: Lecture 4 Plate Tectonics

Page 4: SIO15-18: Lecture 4 Plate Tectonicsigppweb.ucsd.edu/~gabi/sio15/pdfs/Lecture04-presentation.pdf · SIO15-18: Lecture 4 Plate Tectonics • lith. formed at MORs • lith. consumed

SIO15-18: Lecture 4 Plate Tectonics

SIO15-18: Lecture 4 Plate Tectonics

Lithosphere

•  cool and strong but brittle•  zone of Eqs/volcanoes

Asthenosphere

•  warm, soft, ductile

Image: S. Marshak “Earth, Portrait of a Planet”

Page 5: SIO15-18: Lecture 4 Plate Tectonicsigppweb.ucsd.edu/~gabi/sio15/pdfs/Lecture04-presentation.pdf · SIO15-18: Lecture 4 Plate Tectonics • lith. formed at MORs • lith. consumed

SIO15-18: Lecture 4 Plate Tectonics

Why do continents have roots?What keeps the lithosphere afloat?

SIO15-18: Lecture 4 Plate Tectonics

2 counteracting forces

•  gravity•  buoyancy

isostatic equilibrium

•  forces are balanced•  body floats Image: S. Marshak “Earth, Portrait of a Planet”

!  rigid lithosphere floats on soft asthenosphere!  asthenosphere reacts to imbalance (flows)

Page 6: SIO15-18: Lecture 4 Plate Tectonicsigppweb.ucsd.edu/~gabi/sio15/pdfs/Lecture04-presentation.pdf · SIO15-18: Lecture 4 Plate Tectonics • lith. formed at MORs • lith. consumed

SIO15-18: Lecture 4 Plate Tectonics

Which of the previously 9 planets in our solar systemis now a dwarf planet?

POPQUIZ #1

YOUR FULL NAME AND STUDENT ID#

WRITE DOWN ONLY 1 WORD!

SIO15-18: Lecture 4 Plate Tectonics

•  lithosphere is broken up into 12 major plates •  move about (a few cm per year)•  driven by mantle convection •  divergent

•  convergent•  transform

Image: P. Abbott “Natural Disasters”

Mendocino Triple Junction

Page 7: SIO15-18: Lecture 4 Plate Tectonicsigppweb.ucsd.edu/~gabi/sio15/pdfs/Lecture04-presentation.pdf · SIO15-18: Lecture 4 Plate Tectonics • lith. formed at MORs • lith. consumed

SIO15-18: Lecture 4 Plate Tectonics

a little bit like this

Image: S. Marshak “Earth, Portrait of a Planet”

•  ductile mantle (video 4a)•  viscosity: resistance to flow (Lecture 2 notes)

SIO15-18: Lecture 4 Plate Tectonics

slab pull ridge push

slab pull more dominant

slab pull

Page 8: SIO15-18: Lecture 4 Plate Tectonicsigppweb.ucsd.edu/~gabi/sio15/pdfs/Lecture04-presentation.pdf · SIO15-18: Lecture 4 Plate Tectonics • lith. formed at MORs • lith. consumed

SIO15-18: Lecture 4 Plate Tectonics

•  lith. formed at MORs•  lith. consumed in subduction zones•  same rate •  plates move a few cm/yr•  earthquakes•  volcanism•  mountain building and other features on Earth’s surface

SIO15-18: Lecture 4 Plate Tectonics

How do we know that plates move sideways?

•  Alfred Wegener, 1915•  continents like jigsaw puzzle•  fossil records match across oceans•  geologic units match across oceans•  apparent polar wander curves don’t match

Page 9: SIO15-18: Lecture 4 Plate Tectonicsigppweb.ucsd.edu/~gabi/sio15/pdfs/Lecture04-presentation.pdf · SIO15-18: Lecture 4 Plate Tectonics • lith. formed at MORs • lith. consumed

SIO15-18: Lecture 4 Plate Tectonics

Shape: like that of bar magnet (dipole)

•  magnetic north 2000 at: 81.5ºN, 111.4ºW

Origin:currents in metallic liquid outer core -> magnetic dynamo

Time Evolution:changing field; reversals

Observables: strength, declination, inclination

SIO15-18: Lecture 4 Plate Tectonics

•  rock freezing from magma record current field•  Earth’s field/rock position change over time (record of magn. field)

Image: S. Marshak “Earth, Portrait of a Planet”

Curie Temperature (~ 500ºC)above: domains align with mag. fieldbelow: domains frozen

Source: Wikipedia

Page 10: SIO15-18: Lecture 4 Plate Tectonicsigppweb.ucsd.edu/~gabi/sio15/pdfs/Lecture04-presentation.pdf · SIO15-18: Lecture 4 Plate Tectonics • lith. formed at MORs • lith. consumed

SIO15-18: Lecture 4 Plate Tectonics

•  freezing rock conserve current magnetic field•  measure inclination and declination in layers of geol. profile•  determine age of layers (fossils, radioactive dating)•  for one location, construct polar wander curve

Image: S. Marshak “Earth, Portrait of a Planet”

SIO15-18: Lecture 4 Plate Tectonics

continental drift (Alfred Wegener 1915)

sea floor observations (Harry Hess 1950s)

What Makes Continents Drift?

-  sea floor deepens away from mid-ocean ridges (MORs)-  sediments thicken away from MORs-  heat flow is greater at MORs than elsewhere-  dredging (ocean rock different from continental rocks)-  earthquakes along MORs -> seafloor cracking

map by Heezen and Tharp

Page 11: SIO15-18: Lecture 4 Plate Tectonicsigppweb.ucsd.edu/~gabi/sio15/pdfs/Lecture04-presentation.pdf · SIO15-18: Lecture 4 Plate Tectonics • lith. formed at MORs • lith. consumed

SIO15-18: Lecture 4 Plate Tectonics

•  mapping of magnetic anomalies (1960s)

-  ship tows magnetometer-  records magnetic anomalies (Earth field+magnetized rock)

-  new lava cools below Curie T-  current magnetic N frozen into rock- rock moves away from ridge-  symmetric patterns

Fig. 4.13

SIO15-18: Lecture 4 Plate Tectonics

•  magnetic anomalies•  ocean deep drilling

Dietmar Mueller, SIO

no oceanic lith. older than 200 Mio yrs -> subduction zones

Fig. 4.14

Page 12: SIO15-18: Lecture 4 Plate Tectonicsigppweb.ucsd.edu/~gabi/sio15/pdfs/Lecture04-presentation.pdf · SIO15-18: Lecture 4 Plate Tectonics • lith. formed at MORs • lith. consumed

SIO15-18: Lecture 4 Plate Tectonics

•  New lithosphere at MOR pushes plates apart•  thickens, cools, gets dense•  loses buoyancy•  more likely to subduct•  sinking slabs pull rest of lithosphere behind it