radioactive decay and thermal convection

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Radioactive Decay and Thermal Convection

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Radioactive Decay and Thermal Convection
. Thermal structure of the Earth: Heat is a driver for seismological processes. Starting with student experiences. What evidence do they have for Earth’s internal temperature?. Starting with their experiences. - PowerPoint PPT Presentation

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Page 1: Radioactive Decay and      Thermal Convection

Radioactive Decay and Thermal Convection

Page 2: Radioactive Decay and      Thermal Convection

Thermal structure of the Earth: Heat is a driver for seismological

processes

Page 3: Radioactive Decay and      Thermal Convection

What evidence do they have for Earth’s internal temperature?

Starting with student experiences

Page 4: Radioactive Decay and      Thermal Convection

Starting with their experiences

Page 5: Radioactive Decay and      Thermal Convection

Earth’s heat and the age of the Earth• Uniformitarianism (Lyell’s Principles of Geology)

– same geological processes occurring today have existed throughout geologic time

• Darwin (Origin of Species) estimated that it took 300 million years to erode a chalk deposit in southern England

• Lord Kelvin - estimate time from molten state to solidification via cooling– temperature at Earth's core = melting point of rocks– temperature gradient with regard to depth below the surface (1 degree/50’)– thermal decrease through conductivity of rocks*– Estimate of 20 myo to 400 myo)

Page 6: Radioactive Decay and      Thermal Convection

Challenges to Kelvin’s model

• Assumption of a solid Earth • Some argued that the Earth had never been a molten

sphere; rather Earth had formed from the slow accumulation of solid material like asteroids.

• Some attacked Kelvin's assumption about a closed system of dwindling initial heat

• Others offerred the possibility that the then-unknown internal structure of atoms could contain massive amounts of potential energy

Page 7: Radioactive Decay and      Thermal Convection

Where does the heat come from?

• 20% Residual heat from accretion and gravitational collapse

• 80% Radioactive decay– Uranium-238 (4.47 × 109)

– Uranium-235 (7.04 × 108)

– Thorium-232 (1.40 × 1010) – Potassium-40 (1.25 × 109)

Page 8: Radioactive Decay and      Thermal Convection

Average 25oC/km

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Thermal structure

Tufts.edu

Page 10: Radioactive Decay and      Thermal Convection

Earth’s Energy Budget

• Solar Radiation - (99.978%, or nearly 174 petawatts; or about 340 W m-2)

• Geothermal Energy - (0.013%, or about 23 terawatts; or about 0.045 W m-2)

• Tidal Energy – (0.002%, or about 3 terawatts; or about 0.0059 W m-2).

• Waste Heat - (about 0.007%, or about 13 terawatts; or about 0.025 W m-2)

Page 11: Radioactive Decay and      Thermal Convection

How is Earth’s heat released?

• Conduction• Convection• Sketch expected convection in pan

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How to best model mantle material

• Obleck?– Cornstarch and water

• Silly putty?

• What are important criteria for choosing?

Page 14: Radioactive Decay and      Thermal Convection

Convection and Earth’s interior

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• 3D Mantle flow models

Page 21: Radioactive Decay and      Thermal Convection

• 3D Mantle flow models

Page 22: Radioactive Decay and      Thermal Convection

• Mantle convection – Can be imaged using seismic waves– Complex– Sometimes both upper and lower mantle

together– Some subduction zones can be imaged to

base of mantle

Page 23: Radioactive Decay and      Thermal Convection

Reflection on Earth’s interior

• First by yourself, and then with your table, consider 1, 2 or all 3 of the following questions:– What is the difference between the crust and the

mantle?– What is the difference between the lithosphere and

the asthenosphere?– Why are both sets of terms used, and which would

be simplest for your students to understand?

Page 24: Radioactive Decay and      Thermal Convection