Plate Tectonic Presentation

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    Plate Tectonics

    RAKESH ROSHAN RANA

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    Structure of the Presentation

    Interior of EarthPlate

    Evolution of Plate Tectonic Theory

    Type of Plate MarginsEvidence

    Cause

    Post-Pangea TectonicsSupercontinent CycleDiscussions & Remarks

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    Interior of the Earth

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    One of the earliest discoveries of seismology was a discontinuity at a depth of 2900 km where the

    velocity of P-waves suddenly decreases. This boundary is the boundary between the mantle and

    the core and was discovered because of a zone on the opposite side of the Earth from an

    Earthquake focus receives no direct P-waves because the P-waves are refracted inward as a result

    of the sudden decrease in velocity at the boundary. This zone is called a P-wave shadow zone.

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    This discovery was followed by the discovery of an S-wave shadow zone. The S-wave shadow zone occurs

    because no S-waves reach the area on the opposite side of the Earth from the focus. Since no direct S-waves

    arrive in this zone, it implies that no S-waves pass through the core. This further implies the velocity of S-wave

    in the core is 0. In liquids m = 0, so S-wave velocity is also equal to 0. From this it is deduced that the core, or at

    least part of the core is in the liquid state, since no S-waves are transmitted through liquids. Thus, the S-wave

    shadow zone is best explained by a liquid outer core.

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    Have a Look

    Distribution of Continents

    Mid-ocean Ridges

    Trenches

    Orogenic Belts

    Deformation

    Metamorphism

    Volcanism

    Earthquakes

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    Plate

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    Development of Continental Drift

    Lots of people had noticed that the coastlines

    of Africa and South America are similar

    Frank Taylor (1910)

    Alfred Wegener (1912) Die Entstehung Der

    Kontinente Und Ozeane

    1. How we know plate tectonics happens

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    Fit ofContinents

    Across the

    Atlantic

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    The PermianIce Age

    Problem

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    WegenersTheory

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    Dating

    the

    Breakup

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    Frank Taylor

    In somerespects, Taylors

    ideas were more

    modern than

    Wegeners

    Taylor always

    thought

    Wegener hadstolen credit

    from him

    1. How we know plate tectonics happens

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    Frank Taylor

    Recognizedrole of Mid-

    Atlantic Ridge

    Never

    reconstructed

    the continents

    like Wegener

    did

    1. How we know plate tectonics happens

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    Confirmation of Continental Drift

    World War II technology

    International Geophysical Year (IGY) 1957-58

    Worldwide Standardized Seismic Network1963-

    1. How we know plate tectonics happens

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    The Geomagnetic

    Reversal Time

    Scale

    1. How we know plate tectonics happens

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    Discovery of Sea-Floor Spreading

    1. How we know plate tectonics happens

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    Sea-Floor

    Spreading

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    Where Does Ocean Crust Go?

    Hugo Benioff, 1954

    1. How we know plate tectonics happens

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    Benioffs Interpretation

    1. How we know plate tectonics happens

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    Benioffs Interpretation Updated

    1. How we know plate tectonics happens

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    PLATESPlate Area (km2) Plate Area (km2)

    Pacific 103,300,000 Scotia 1,600,000

    North American 75,900,000 Burma microplate 1,100,000

    Eurasian 67,800,000 Fiji microplates 1,100,000

    African 61,300,000 Tonga microplate 960,000

    Antarctic 60,900,000 Mariana microplate 360,000

    Australian 47,000,000 Bismark microplate 300,000

    South American 43,600,000 Juan de Fuca 250,000

    Somali 16,700,000 Solomon microplate 250,000

    Nazca 15,600,000South Sandwichmicroplate

    170,000

    Indian 11,900,000 Easter microplate 130,000

    Philippine 5,500,000Juan Fernandezmicroplate

    96,000

    Arabian 5,000,000 Rivera microplate 73,000

    Caribbean 3,300,000 Gorda microplate 70,000

    Cocos 2,900,000 Explorer microplate 18,000

    Caroline microplate 1,700,000 Galapagos microplate 12,000

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    What Drives It: Convection

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    Pea-soup analogy

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    Other Causes

    Differential rate of motion

    Earth Slope

    Heat Gradient

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    How Plates Move

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    The Plate Tectonics Model

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    The Plate Tectonics Model

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    Plate motions

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    Plate Motions

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    Divergent boundary

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    Magnetic

    Stripes in

    theFAMOUS

    Area

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    Anatomy of a Mid-Ocean Ridge

    Con ergent bo ndar

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    Convergent boundary

    Subduction

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    Terrane Accretion

    Transform boundary

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    Transform boundary

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    Mass Construction and Destruction

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    Relationship between plate tectonic

    setting and structural style:

    Tectonic SettingStressState

    Types of Structures Examples

    Divergent plates extension normal faults, roll overanticlines, tilted blocks

    North Sea, Red Sea,Basin and Range

    Convergent plates compression thrust faults, folds,faulted folds

    Andes, Zagros Mts(Iran), Canadian

    Rockies

    Transform plate boundaries strike-slipstrike-slip faults,

    compressional andextensional flower

    structures

    San Andreas fault,Alpine Fault (New

    Zealand).

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    Terranes in

    Western NorthAmerica

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    A h T i

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    Archean Tectonics Archean Crust formed 4.4 to 2.5 billion years ago.

    The formation of these cratonic nucleii marks thetransition from an early Earth that was so hot andenergetic that no remnants of crust were preserved, toa state where crustal preservation became possible.

    Most of the cratons are attached to a high velocitymantle root that extends to depths of at least 200 km(King, 2005).

    These cratonic roots are composed of stiff and

    chemically buoyant mantle material (Section 11.3.1) whose resistant qualities have

    contributed to the long-term survival of the Archeancontinental lithosphere (Carlson et al., 2005).

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    The beginning of the Archean Eon approximately

    coincides with the age of the oldest continental crust.A conventional view places this age at approximately

    4.0 Ga, which coincides with the age of the oldest rocks found

    so far on Earth: the Acasta gneisses of the Slave craton in

    northwestern Canada (Bowring & Williams, 1999).However, >4.4 Ga detrital zircon minerals found in the Yilgarn

    craton of Western Australia (Wilde et al., 2001) suggest that

    some continental crust may have formed as early as 4.44.5

    Ma, although this interpretation is controversial (Harrison et al.,

    2005, 2006; Valley et al., 2006).

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    PRECAMBRIAN HEAT FLOW

    The majority of terrestrial heat production comes from thedecay of radioactive isotopes dispersed throughout the core,

    mantle, and continental crust.

    Heat flow in the past must have been considerably greater than

    at present due to the exponential decay rates of these isotopes.For an Earth model with a K/U ratio derived from

    measurements of crustal rocks, the heat flow in the crust at 4.0

    Ga would have been three times greater than at the present day

    and at 2.5 Ga about two times the present value (Mareschal &

    Jaupart, 2006). For K/U ratios similar to those in chondritic meteorites, which

    are higher than those in crustal rocks, the magnitude of the

    decrease would have been greater.

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    Heat Flow with TimeFig. Variation of

    surface heat flowwith time. Solidline, based on achondritic model;

    dashed line,based on a K/Uratio derived fromcrustal rocks

    (McKenzie &Weiss, 1975).

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    In Many of the cratons includes an abundance of high

    temperature/low pressure metamorphic mineral assemblages and

    the intrusion of large volumes of granitoids, suggestrelatively high (500700 or 800C) temperatures in

    the crust during Archean times, roughly similar to those which

    occur presently in regions of elevated geotherms.

    By contrast, geophysical surveys and isotopic studies of mantle

    nodules suggest that the cratonic mantle is strong and cool and

    that the geotherm has been relatively low since the Archean Some

    of the most compelling evidence of cool mantle lithosphere comes

    from thermobarometric studies of silicate inclusions in Archean

    diamonds, which suggest that temperatures at depths of 150200 km during the Late Archean were similar to the

    present-day temperatures at those depths (Boyd et al.,

    1985; Richardson et al., 2001).

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    Proterozoic Tectonics

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    Supercontinent Cycle