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PLATE TECTONICS & CONVECTION. Earth’s Interior The Theory of Plate Tectonics  Earth’s crust and part of the upper mantle are broken up into plates that.

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Presentation on theme: "PLATE TECTONICS & CONVECTION. Earth’s Interior The Theory of Plate Tectonics  Earth’s crust and part of the upper mantle are broken up into plates that."— Presentation transcript:

1 PLATE TECTONICS & CONVECTION

2 Earth’s Interior

3 The Theory of Plate Tectonics  Earth’s crust and part of the upper mantle are broken up into plates that move on a plastic-like layer of the mantle  Earth’s surface is made up of rigid plates known as the Lithosphere. 80 km thick (up to 200 km thick beneath continents), very brittle, easily fractures at low temperature.  These plates “float” over the upper mantle called the Asthenosphere. 250 km thick - solid rock, but it is soft and flows easily (ductile).  There are 7 major plates and about 18 minor plates.  Most of the major plates are located under the continents

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5 What moves the plates? 1. Mantle Convection 2. Ridge Push 3. Slab Pull

6 Mantle Convection What causes these Plates to move? Convection Currents Demonstration

7 Mantle Convection  Mantle Convection Mantle Convection  Convection Current  Any movement of matter that results from differences in density  Differences of density within the earth are caused by differences in temperature  Examples  “Lava” in a lava lamp  Boiling Water  Making popcorn in an air popper  “Hot air rises!”

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9 REVIEW: Earth is HOT EARTH’S FORMATIONRADIOACTIVE DECAY OF ELEMENTS Moving objects have kinetic energy. When objects collide, kinetic energy is converted into thermal energy. When Earth formed, objects in the solar system collided, generating thermal energy. When the earth was molten, it began to separate into layers based on density. Particles of matter had gravitational potential energy, so as gravitational force acted to separate these particles according to density, the particles experienced friction (because they were moving past one another). A byproduct of friction is thermal energy. What is radioactive decay?  Some elements have an unstable nucleus  To become more stable, the nucleus of the radioactive element breaks apart When a nucleus breaks apart, heat is released. The decay of radioactive elements into more stable elements releases heat inside the Earth, making the interior of the Earth hot Radioactive elements have been present within Earth since the Earth was formed and still exist within Earth today, therefore, heat continues to be generated in Earth’s interior.

10 Convection Currents  Convection currents transfer heat through the movement of heated fluid material (i.e. molten rock)  The asthenosphere is heated by the inner and outer core of the Earth. This heat is transferred through the mantle.

11  When materials like solid rock are heated, they expand and become less dense  Hot, less dense plastic-like material rises, coming in contact with the lithosphere (crust and uppermost mantle)  It cools at the lithosphere (or Earth’s outermost layer) and becomes more dense causing the material to sink  The constant rotation of the material creates a current that is able to pull the plates

12 How Plates Move CONVECTION CURRENTS IN ASTHENOSPHERE

13 Forces Causing Plate Motion Rising mantle material at mid-ocean ridges creates the potential for plates to move away from the ridge Moves lithosphere in opposite directions away from a mid-ocean ridge Ridge Push When tectonic plates collide, the denser plate (slab) will sink in to the mantle As a slab sinks, it pulls on the rest of the plate with a force called slab pull Slab Pull

14 RIDGE PUSH Human Demonstration - Dominoes

15 SLAB PULL Table Cloth Demonstration

16 Ridge Push

17 Slab Pull

18 WHY DOES THE OCEANIC CRUST GO UNDER THE CONTINENTAL CRUST? Density!!!

19  Mostly Basalt  High in Iron (5-10%)  Low in Silica (45-60%)  Young (0-200 myo)  New rock formed at MOR  Thin (8-10 km thick)  Dense (3.0 g/cm 3 )  Mostly Granite  Low in Iron (2-5%)  High in Silica (65-75%)  Sits on top of Oceanic  Old (up to 4 byo)  Thick ( km thick)  Low Density (2.7 g/cm 3 ) Oceanic CrustContinental Crust


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