The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition,...

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The Earths interior structure - Lecture 1 How do we know what’s inside the Earth? samples from inside the Earth (not many) indirect observations of the Earth’s interior seismic, gravity, magnetic, and heat flow measurements today (mostly): seismic studies of Earth’s interior

Transcript of The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition,...

Page 1: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

The Earth’sinterior structure - Lecture 1

How do we know what’s inside the Earth?• samples from inside the Earth (not many)• indirect observations of the Earth’s interior seismic, gravity, magnetic, and heat flow measurements• today (mostly): seismic studies of Earth’s interior

Page 2: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

EARTH’S INTERIOR: SAMPLES

Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4

(page 117)

Page 3: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

KTB borehole -- drilled to a depth of 10 km in GermanyRussians have drilled a 12-km-deep borehole

Page 4: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

Convecting Mantle

Kimberlites: samples of the upper mantle

Page 5: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

Kimberlites: contain samples of the upper mantle (from >150 km deep)

Box 4.4, page 118 (Plummer 1st Canadian edition)

Page 6: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

Mantle xenoliths: samples of the upper mantle from volcanoes

http://www.ees.nmt.edu/condie/MantleXenolith_NM.jpg http://www.calstatela.edu/faculty/acolvil/interior.html

Page 7: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

EVIDENCE FROM SEISMIC WAVES

Plummer 1st Cdn. edition, Ch. 4 pp. 109-112

Page 8: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

Refracted and Reflected Waves

Page 9: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

Fig. 4.01

Seismic Reflection

Page 10: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

Seismic Reflection

T53

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Crustal Seismology: Seismic Reflection

Lithoprobe Seismic ReflectionNovember 2000

Vibroseis trucksStewart-Cassiar HwyNorthwest BC

pp 110-111, Canadian edition of text

Page 12: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)
Page 13: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

Active sourcereflection seismology:

Petroleum industry’sprimary explorationtechnique

Page 14: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

• energy reflects off sharp boundaries between rocks with strong contrasts in density and seismic velocity

• reflection is widely used by oil industry to find hydrocarbon traps in sedimentary basins

Seismic Reflection

Page 15: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

Fig. 4.2

Seismic Refraction

Page 16: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

Fig. 4.3

Page 17: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

Effect of material change on paths of Refracted and reflected waves

layer with slow v

layer with faster v

layer with even faster v

With no change in properties, no refractions, no reflections

Page 18: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

Slower

Faster

Curvature(refraction)

of the energy

Velocitygraduallyincreasingwith depth

seismic raypath bends

Page 19: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

• energy is transmitted through layers and takes a curved path back to the surface without a reflection

• this happens because seismic velocity increases gradually with depth

• seismic velocities in the Earth generally increase with depth due to effects of pressure

Seismic Refraction

Page 20: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

EARTH’S INTERNAL STRUCTURE

Plummer et al. Canadian Edition Ch. 4 pp. 112-119

Page 21: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

Fig. 4.5

Page 22: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

• Earth structure dominantly radial due to – pressure: rearrange atoms to form denser

minerals, for example, in the mantle

– compositional differentiation (denser elements sink to the center)

• main compositional layers are:– crust (0 to 30 km, on average)

– mantle (30 to 2900 km)

– core (2900 to 6370 km)

Earth’s Radial Structure

Page 23: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

• some important rheologic layers are:– solid lithosphere (0 to 150 km)

– gooey asthenosphere (150 to 300 km)

– liquid outer core (2900 to 5150 km)

– solid inner core (5150 to 6370 km)

Earth’s Radial Structure

Page 24: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

Figure 4.6

P-wave velocities in crust and upper mantleMUCH lowervelocities nearEarth’s surface

Page 25: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

Table 4.1 in Canadian edition of text

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Fig. 4.7

P- and S- wave velocities inside the Earth

Page 27: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

• upper mantle (30-660 km)– 8 km/s : peridotite

– seismic velocity variations due to lithosphere, asthenosphere (gooey), olivine phase changes

• lower mantle (660-2900 km)– steady increase in velocity

– probably same composition as upper mantle

Page 28: The Earth s interior structure - Lecture 1 · EARTH’S INTERIOR: SAMPLES Plummer 1st Cdn edition, Ch. 4 pp 107-109, plus Box 4.4 (page 117)

Wait! How do we know this??

We measure the arrival times of different seismic waves, and compare them with what we would expect from calculations for a model Earth.