Unit 4: Geophysics Part 1: Plate Tectonics.

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Presentation transcript:

Unit 4: Geophysics Part 1: Plate Tectonics

Section 1: Continental Drift

Continental drift: an idea before its time Alfred Wegener First proposed hypothesis, 1915 Continental drift hypothesis Supercontinent called Pangaea began breaking apart about 200 million years ago Continents “drifted” to present positions Continents “broke” through the ocean crust

Pangaea approximately 200 million years ago Figure 7.2

Continental drift: an idea before its time Wegener’s continental drift hypothesis Evidence used by Wegener Fit of South America and Africa Fossils match across the seas Rock types and structures match Ancient climates Main objection to Wegener’s proposal was its inability to provide a mechanism (what causes them to move?)

Jigsaw Evidence

Similar mountain ranges on different continents Figure 7.7

Paleoclimatic evidence for continental drift Figure 7.8

The fossils of mesosaurus are separated by an ocean The fossils of mesosaurus are separated by an ocean. Mesosaurus couldn’t swim, so in order for this dinosaur to be on two separate continents, they must have been together at one time.

Section 2: Plate Tectonics

Plate tectonics: the extended theory More encompassing than continental drift Associated with Earth’s rigid outer shell Called the lithosphere Consists of several plates (about 20) Plates are moving slowly Largest plate is the Pacific plate Plates are mostly beneath the ocean

Plate tectonics: the extended theory Asthenosphere Exists beneath the lithosphere Hotter and weaker than lithosphere Allows for motion of lithosphere Plate boundaries All major interactions among plates occur along their boundaries

Plate tectonics: the extended theory Plate boundaries Types of plate boundaries Divergent plate boundaries Two plates move apart Mantle material upwells to create new seafloor Ocean ridges and seafloor spreading Oceanic ridges develop along well-developed boundaries Along ridges, seafloor spreading creates new seafloor

Divergent boundaries located along oceanic ridges Figure 7.11

Plate tectonics: the extended theory Plate boundaries Types of plate boundaries Divergent plate boundaries Continental rifts form at spreading centers within a continent Convergent plate boundaries Plates collide, an ocean trench forms, and lithosphere is subducted into the mantle

The East African rift – a divergent boundary on land Figure 7.13

Plate tectonics: the extended theory Plate boundaries Types of plate boundaries Convergent plate boundaries Oceanic–continental convergence Denser oceanic slab sinks into the asthenosphere Pockets of magma develop and rise Continental volcanic arc forms Examples include the Andes, Cascades, and the Sierra Nevadan system

An oceanic–continental convergent plate boundary Figure 7.15 A

Plate tectonics: the extended theory Plate boundaries Types of plate boundaries Convergent plate boundaries (destructive margins) Oceanic–oceanic convergence Two oceanic slabs converge and one descends beneath the other Often forms volcanoes on the ocean floor Volcanic island arc forms as volcanoes emerge from the sea Examples include the Aleutian, Mariana, and Tonga islands

An oceanic–oceanic convergent plate boundary Figure 7.15 B

Mariana Trench Deepest trench in the ocean Formed where two oceanic plates collide Actual deepest spot is known as the “Challenger Deep” At 36,000 feet, it is tall enough that Mt. Everest could fit into it if it was wide enough! http://en.wikipedia.org/wiki/Challenger_Deep

Plate tectonics: the extended theory Plate boundaries Types of plate boundaries Convergent plate boundaries (destructive margins) Continental–continental convergence When subducting plates contain continental material, two continents collide Can produce new mountain ranges such as the Himalayas

A continental–continental convergent plate boundary Figure 7.15 C

The collision of India and Asia produced the Himalayas Figure 7.16 A

The collision of India and Asia produced the Himalayas Figure 7.16 C

Plate tectonics: the extended theory Plate boundaries Types of plate boundaries Transform fault boundaries Plates slide past one another No new crust is created or destroyed Transform faults Most join two segments of a mid-ocean ridge Aid the movement of oceanic crustal material

Section 3: Evidence for Plate Tectonics

Testing the plate tectonics model Evidence from ocean drilling Some of the most convincing evidence confirming seafloor spreading has come from drilling directly into ocean-floor sediment Age of deepest sediments Thickness of ocean-floor sediments verifies seafloor spreading

Testing the plate tectonics model Hot spots and mantle plumes Caused by rising plumes of mantle material Volcanoes can form over them (Hawaiian Island chain) Mantle plumes Long-lived structures Some originate at great depth, perhaps at the mantle–core boundary

The Hawaiian Islands have formed over a hot spot Figure 7.21

Testing the plate tectonics model Evidence for the plate tectonics model Paleomagnetism Probably the most persuasive evidence Ancient magnetism preserved in rocks Paleomagnetic records show Earth’s magnetic field reversals Recorded in rocks as they form at oceanic ridges

Paleomagnetic reversals recorded by basalt flows Figure 7.27

Measuring plate motion By using hot spot “tracks” like those of the Hawaiian Island–Emperor Seamount chain Using space-age technology to directly measure the relative motion of plates Very Long Baseline Interferometry (VLBI) Global Positioning System (GPS)

Directions and rates of plate motions Figure 7.28

What drives plate motion Several models have been proposed Plate–mantle convection Convection: the transfer of heat through the movement of heated material

Where does the energy come from that causes the convection current? Heat from within the Earth, due to: Radioactive decay of elements within the earth Heat left over from the Earth’s original formation

Layering at 660 km Figure 7.30 A

Whole-mantle convection Figure 7.30 B

Several mechanisms contribute to plate motion Figure 7.29

Plate tectonics into the future Present-day motions have been extrapolated into the future some 50 million years Areas west of the San Andreas Fault slide northward past the North American plate Africa collides with Eurasia, closing the Mediterranean and initiating mountain building Australia and New Guinea are on a collision course with Asia

A possible view of the world 50 million years from now Figure 7.31