Upload
rakesh-roshan-rana
View
224
Download
0
Embed Size (px)
Citation preview
8/6/2019 Plate Tectonic Presentation
1/55
Plate Tectonics
RAKESH ROSHAN RANA
8/6/2019 Plate Tectonic Presentation
2/55
Structure of the Presentation
Interior of EarthPlate
Evolution of Plate Tectonic Theory
Type of Plate MarginsEvidence
Cause
Post-Pangea TectonicsSupercontinent CycleDiscussions & Remarks
8/6/2019 Plate Tectonic Presentation
3/55
Interior of the Earth
8/6/2019 Plate Tectonic Presentation
4/55
8/6/2019 Plate Tectonic Presentation
5/55
8/6/2019 Plate Tectonic Presentation
6/55
8/6/2019 Plate Tectonic Presentation
7/55
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.
8/6/2019 Plate Tectonic Presentation
8/55
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.
8/6/2019 Plate Tectonic Presentation
9/55
8/6/2019 Plate Tectonic Presentation
10/55
8/6/2019 Plate Tectonic Presentation
11/55
Have a Look
Distribution of Continents
Mid-ocean Ridges
Trenches
Orogenic Belts
Deformation
Metamorphism
Volcanism
Earthquakes
8/6/2019 Plate Tectonic Presentation
12/55
Plate
8/6/2019 Plate Tectonic Presentation
13/55
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
8/6/2019 Plate Tectonic Presentation
14/55
Fit ofContinents
Across the
Atlantic
8/6/2019 Plate Tectonic Presentation
15/55
The PermianIce Age
Problem
1. How we know plate tectonics happens
8/6/2019 Plate Tectonic Presentation
16/55
WegenersTheory
1. How we know plate tectonics happens
8/6/2019 Plate Tectonic Presentation
17/55
Dating
the
Breakup
1. How we know plate tectonics happens
8/6/2019 Plate Tectonic Presentation
18/55
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
8/6/2019 Plate Tectonic Presentation
19/55
Frank Taylor
Recognizedrole of Mid-
Atlantic Ridge
Never
reconstructed
the continents
like Wegener
did
1. How we know plate tectonics happens
8/6/2019 Plate Tectonic Presentation
20/55
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
8/6/2019 Plate Tectonic Presentation
21/55
The Geomagnetic
Reversal Time
Scale
1. How we know plate tectonics happens
8/6/2019 Plate Tectonic Presentation
22/55
Discovery of Sea-Floor Spreading
1. How we know plate tectonics happens
8/6/2019 Plate Tectonic Presentation
23/55
Sea-Floor
Spreading
1. How we know plate tectonics happens
8/6/2019 Plate Tectonic Presentation
24/55
Where Does Ocean Crust Go?
Hugo Benioff, 1954
1. How we know plate tectonics happens
8/6/2019 Plate Tectonic Presentation
25/55
Benioffs Interpretation
1. How we know plate tectonics happens
8/6/2019 Plate Tectonic Presentation
26/55
Benioffs Interpretation Updated
1. How we know plate tectonics happens
8/6/2019 Plate Tectonic Presentation
27/55
8/6/2019 Plate Tectonic Presentation
28/55
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
8/6/2019 Plate Tectonic Presentation
29/55
What Drives It: Convection
8/6/2019 Plate Tectonic Presentation
30/55
Pea-soup analogy
8/6/2019 Plate Tectonic Presentation
31/55
Other Causes
Differential rate of motion
Earth Slope
Heat Gradient
8/6/2019 Plate Tectonic Presentation
32/55
How Plates Move
8/6/2019 Plate Tectonic Presentation
33/55
The Plate Tectonics Model
8/6/2019 Plate Tectonic Presentation
34/55
The Plate Tectonics Model
8/6/2019 Plate Tectonic Presentation
35/55
Plate motions
8/6/2019 Plate Tectonic Presentation
36/55
Plate Motions
8/6/2019 Plate Tectonic Presentation
37/55
Divergent boundary
8/6/2019 Plate Tectonic Presentation
38/55
Magnetic
Stripes in
theFAMOUS
Area
8/6/2019 Plate Tectonic Presentation
39/55
Anatomy of a Mid-Ocean Ridge
Con ergent bo ndar
8/6/2019 Plate Tectonic Presentation
40/55
Convergent boundary
Subduction
8/6/2019 Plate Tectonic Presentation
41/55
Terrane Accretion
Transform boundary
8/6/2019 Plate Tectonic Presentation
42/55
Transform boundary
8/6/2019 Plate Tectonic Presentation
43/55
Mass Construction and Destruction
8/6/2019 Plate Tectonic Presentation
44/55
8/6/2019 Plate Tectonic Presentation
45/55
8/6/2019 Plate Tectonic Presentation
46/55
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).
8/6/2019 Plate Tectonic Presentation
47/55
Terranes in
Western NorthAmerica
8/6/2019 Plate Tectonic Presentation
48/55
A h T i
8/6/2019 Plate Tectonic Presentation
49/55
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).
8/6/2019 Plate Tectonic Presentation
50/55
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).
8/6/2019 Plate Tectonic Presentation
51/55
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.
8/6/2019 Plate Tectonic Presentation
52/55
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).
8/6/2019 Plate Tectonic Presentation
53/55
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).
8/6/2019 Plate Tectonic Presentation
54/55
Proterozoic Tectonics
8/6/2019 Plate Tectonic Presentation
55/55
Supercontinent Cycle