origin and structure of the earth marshak – chapter 1 (plus an introduction to chapter 2)

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Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

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Page 1: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Origin and Structureof the Earth

Marshak – Chapter 1(plus an introduction to Chapter 2)

Page 2: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

The Earth is part of the solar system and thus most likely formed at the same time…

So, what do we know about the solar system and it’s structure?

These are the observations which are needed to come up with an idea (hypothesis) for how the solar system (and Earth) formed.

Page 3: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Formation of the solar system and differentiation of Earth

• Hypotheses must satisfy observations: planets orbit sun in one direction, axes of rotation nearly perpendicular to orbit, most planets rotate in same direction as orbit about sun, >99% solar system mass in sun, ~99% solar system angular momentum in planets

• Inner Terrestrial - Mercury, Venus, Earth, Mars• Outer Jovian - Jupiter, Saturn, Uranus, Neptune, Pluto?• Terrestrial – dense, rocky, >3 g cm3, Mg, Fe, Si, K, Ca,

metals combined with O• Jovian - “gassy” <~1.5 g cm3, ice, H, He, CH4 methane CO2

• Asteroid belt between Mars and Jupiter, source of meteorites

Page 4: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Origin of our Solar System: The Nebular Hypothesis

Page 5: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)
Page 6: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)
Page 7: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)
Page 8: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

The Sun is ~99% of the mass of the solar system

~99% of the angular momentum is in the planets

Inner planets are rocky and dense – terrestrial planets

Outer planets are gassy – gas giant planets

We know the Earth is composed of layers – Why?

Page 9: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Planetary Differentiation• Why?

– There is a motive• Layers of different chemical composition can have

different density, and gravity provides a driving force whereby planets can lower their potential energy by sorting the denser material towards the center.

– There is a means• Solids are hard to sort mechanically, but liquids are

easily separated gravitationally. Partial or complete melting allows large-scale differentiation.

– There was an opportunity• Heating beyond the melting point of most components of

undifferentiated solar material during planet formation is inevitable for bodies above a certain size (> approx. 1,000 km radius) that formed early enough or fast enough.

Page 10: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Chemical Differentiation of the Earth

Early Earth Earth Today

Early Earth likely entirely molten – gravitational segregationof dense metals (mostly Fe) to the center is the result.

Page 11: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Origin of the moon by planetary impact on Earth

This occurred ~4.5 billion years ago (4.5 Ga) (very early in Earth history as age is only ~4.6 Ga)

Page 12: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Whole Earth has significant Fe - due to the core

However, outer layers of Earth are much different

Page 13: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Earth’s crust (thin outer layer) mostly Si and O

Earth’s mantle (between core and crust) issimilar to the crust, but with lower Si, and higher Fe and Mg

Page 14: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Introduction to Plate Tectonics

Page 15: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

• Plate Tectonics: Structure of Earth’s surface is largely caused by the formation, movement, and destruction of large rigid plates…

• Major conclusions of Plate Tectonics:– The lithosphere (outermost shell of Earth) is composed of 13 or

more large rigid plates and numerous smaller ones

– The plates move with respect to one another and thus continents are mobile (imbedded in plates)

– Continents are relatively old, ocean basins relatively young

– Geologic activity (earthquakes, volcanoes) is concentrated along the boundaries between plates

Page 16: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

January 20, 2011 – Earthquakes in the past 5 yearsfrom www.iris.edu

Page 17: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Earthquakes mark outline of Earth’s tectonic plates.

Page 18: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Known volcanoes of the world – do the locations look familiar?from the Smithsonian Global Volcanism Project

Page 19: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Note that earthquakesand volcanoes generallyoccur in the same locations.

Where are Earths largemountains found?

Are all of these generallyfound in the same places?

Page 20: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Earth’s outermost layer comprises plates which move relative to each other.These movements are now measured by GPS and VLBA techniques.

Page 21: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

The Theory of Plate TectonicsThe Theory of Plate Tectonics

Earth’s outer layer broken up into 13 major tectonic plates which are made of the crust and uppermost mantle beneath.

Page 22: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Plates may contain oceanic or continental crust or both

contain both continental

and oceanic crust

Some plates

Others are mainly oceanic crust

Page 23: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Earth is Composed of Multiple Layers from Core to Crust.Crust and Upper Mantle (Lithosphere) = Locked Together as Rigid Plate.

In terms of overall radius of Earth the plates are only 1-2%.

Page 24: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

The lithosphere is cold, rigid and solid.What about the asthenospheric mantle beneath?

Page 25: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

The rigid lithosphere slides on the ductile asthenosphere, which is partially molten.

LithosphereLithosphere

AsthenosphereAsthenosphere

Cold, rigid

Hot, ductile

Continental crust(mostly granite)

Oceanic crust (mostly basalt)M

an

tle(m

ostly

oliv

ine

)

Page 26: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Lithosphere and asthenosphere refer to the strength (Is it hot, or is it cold? Is it rigid, or does it flow like toothpaste?)

Lithosphere : Strong, rigid, cold outer shell of rock which includes the crust and part of the upper mantle.

Asthenosphere: The hotter, weak, ductile layer of solid rock below the lithosphere that flows plastically. Analogy – cold toothpaste.

Crust, mantle, and core refer to composition (what is it made of?).

Crust: mostly granite on continents mostly basalt on oceans (we will talk

aboutMantle: made mostly of the mineral olivine these later…)Core: mostly iron and some nickel

Page 27: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

3 Types of Plate Boundaries• divergent• convergent• transform (strike-slip)

transform divergent convergent

Page 28: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Divergent plate boundary• plates move apart• new lithosphere created (oceanic)• volcanism and earthquakes

Page 29: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

convergent plate boundary• plates move towards one another• lithosphere destroyed (oceanic)• volcanism, earthquakes,

mountain belts

Page 30: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Convergent Plate Margins

Ocean-Ocean

Ocean-Continent

Continent-Continent

Page 31: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)
Page 32: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)
Page 33: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Lithosphere created at divergent plate boundariesis destroyed at convergent plate boundaries.

Page 34: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Motion at Plate Boundaries

Page 35: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Hotspot volcanoes are created where a plume of bouyant, hot mantle rises.

Page 36: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Hot Spot Volcano Tracks

Page 37: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

What Forces Drive Plate Tectonics?

Page 38: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Early Earth wasmostly moltendue to:

1) Impact events2) Gravity3) Radioactivity

Page 39: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Earth’s internal heat is still escaping today and is most obviously expressed in volcanic eruptions.

Page 40: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

What role does Earth’s internal heat play in the operation of plate tectonics?

Three modes of heat transfer.

Only convection causes motion.

Page 41: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

How does convection work?

• Within Earth’s interior: - Cold dense rock

sinks in subduction zones.

- Hot, ductile mantle inside rises and convection occurs.

Fig 1.15c

Page 42: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Plate tectonics is caused by convection in the mantle.

In detail there are other driving forces, we willdiscuss these later in the semester…..

Page 43: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Plate Tectonics provides a comprehensive explanation for all of

the major features of the Earth that we can observe.

earthquakes

volcanoes

deep ocean trenches

Island chain from hot spots

Fig 1.10

Page 44: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Plate velocities measured with GPS

Confirms plate tectonic motions beyond reasonable doubt!

Page 45: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)
Page 46: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Mantle tomography – provides images similar to ultrasound.

Page 47: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

Mantle tomography – hot material in red (slower seismic wave velocity), cold material in blue (faster seismic wave velocity).

Earthquake locations shown by white dots.

Clearly shows the subducting oceanic lithosphere (cold) beneath the Japan volcanic arc system (hot).

Page 48: Origin and Structure of the Earth Marshak – Chapter 1 (plus an introduction to Chapter 2)

More detailed image of subduction zone beneath Japan.