1) earth’s internal heat engine. 2) earth’s magnetic field. 3) intro. to seismology: tools for...

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1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into TODAY’s LECTURE:

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Page 1: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

1) Earth’s internal heat engine.

2) Earth’s magnetic field.

3) Intro. to Seismology: Tools for seeing into the Earth’s interior.

(Chaps. 2-4)

TODAY’s LECTURE:

Page 2: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:
Page 3: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:
Page 4: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Convection in the Mantle Drives Plate Tectonics! But how?

Page 5: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

3 reasons for internal heat:

Earth’s internal heat engineEarth’s internal heat engine

1) from impact during Earth formation 2) radioactive decay of uranium, thorium, potassium

3) heat released as inner core forms

Ways to transfer heat:

1) conduction - motion of atoms

2) convection - mass movement of material

Page 6: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Density:

Defined as the mass of a material, per unit volume.

Usually given in grams per cubic centimeter (g/cm3).

For comparison, the density of water is 1.0 g /cm3

.

Page 7: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Earth’s internal heat engineEarth’s internal heat engine

Hot materials are less dense and rise.Cooler materials are denser and sink.

Page 8: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:
Page 9: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Convecting materials in the Earth’s mantle originate deep, near the core-mantle boundary

Page 10: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Most heat from the deep interior is transferred to the shallow mantle by buoyant masses of

hot, low density material called “plumes”.

Page 11: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Hawaiian Islands

Plumes Create Volcanic Hotspots

Page 12: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Earth’s internal heat engineEarth’s internal heat engine

Cold down-goingmaterial

Hot upwellingMaterial

.

See: MantleUpwelling.MOV

See: MantleDownwelling.MOV

Page 13: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Earth’s internal heat engineEarth’s internal heat engine

See: MantleConvection.MOV

Page 14: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Heat of the upper mantle sets up shallowHeat of the upper mantle sets up shallowconvection cells that drive plate motions.convection cells that drive plate motions.

Page 15: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

There are Three Basic Plate Margin Types: Can You Identify Them?

Page 16: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

See Video:EarthOceanFloors.MOV

Page 17: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Consequences of Plate Motions: Mountain Building

Page 18: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Volcanic Activity

Mt. Mayon, Philippines

Page 19: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Consequences of Plate Motions: Earthquakes!

Page 20: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Convection Also Drives Deep Seafloor Hydrothermal Systems

Page 21: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

The magnetic field is generated by an organized flow of electrons in the molten outer core.

Earth’s magnetic field:Earth’s magnetic field:

Page 22: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Earth’s magnetic field is a dipole with north and south Earth’s magnetic field is a dipole with north and south ends of opposing polarity. The magnetic poles and ends of opposing polarity. The magnetic poles and geographic (rotational) pole are offset by 23.5geographic (rotational) pole are offset by 23.500

Page 23: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Earth-Sun Interactions:(See: Bio_North_America.MOV

& Aurora.Mov)

Page 24: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Earth’s Earth’s magnetic magnetic field:field:

Lines of Lines of magnetic magnetic force are force are ~parallel to ~parallel to the Earth’s the Earth’s surface at surface at the equator, the equator, but are but are vertically at vertically at the poles.the poles.

Page 25: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Earth’s magnetic fieldEarth’s magnetic field

Naturally-occurring magnetic mineral

grains, like the mineral magnetite,

act as tiny bar magnets and become

oriented parallel to the field lines of the Earth’s magnetic field

Page 26: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Moon:

No magnetic field.

No molten outer core.

Page 27: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

MARS: Had a magnetic field early in its history, but not today. How do we know? Remnant magnetism!

Page 28: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Magnetic Reversals:Magnetic Reversals:

Earth’s magnetic field reverses its polarity on an Earth’s magnetic field reverses its polarity on an irregular time scale of a few tens of thousand to irregular time scale of a few tens of thousand to hundreds of thousands of years. hundreds of thousands of years. (see MagFieldRev.MOV)(see MagFieldRev.MOV)

Page 29: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Magnetic reversals are recorded in igneous Magnetic reversals are recorded in igneous rocks by the remnant field orientations rocks by the remnant field orientations frozen into by the magnetic minerals (e.g. frozen into by the magnetic minerals (e.g. magnetite) that crystallize from magma as magnetite) that crystallize from magma as it cools.it cools.

Page 30: 1) Earth’s internal heat engine. 2) Earth’s magnetic field. 3) Intro. to Seismology: Tools for seeing into the Earth’s interior. (Chaps. 2-4) TODAY’s LECTURE:

Magnetic reversals can be dated!Magnetic reversals can be dated!

This is accomplished by using radiometric dating This is accomplished by using radiometric dating methods to date igneous rocks that preserve the methods to date igneous rocks that preserve the

remnant magnetism.remnant magnetism.