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Published byChad Walsh Modified over 9 years ago
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Class 1: Plate Tectonics Review Today’s topics: Earth’s compositional layers Plate tectonics: theory & actions
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Earth’s Compositional Layers Atmosphere & Hydrosphere Crust Mantle Core
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Earth’s Atmosphere & Hydrosphere
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Earth’s Crust more dense relatively light CRUST
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Earth’s Mantle MANTLE more dense than crust CRUST
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Earth’s Core highest density CRUST MANTLE CORE
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Earth’s Magnetic Field rocky core Earth Requirements for magnetic field: 1. rotation 2. heat flow, convecting fluid 3. a mobile conductor (iron or metallic hydrogen)
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Global Earthquake Locations
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Global Volcano Locations
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Linking Observations
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Continental Drift
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Continental Drift (movie)
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Ages of the Ocean Floor Ma = Million years ago 1 billion years = 1 Gyr 1 million years = 1 Myr 1 thousand years = 1 kyr
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Fig.4.11a Heat Flow Warm colors = higher heat flow Cool colors = lower heat flow high at ocean ridges
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Global Topography and Bathymetry ocean ridges
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The Puzzle Solved….. earthquake locations volcano locations sea floor age sea floor bathymetry + heat flow too!
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Earth’s Tectonic Plates
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Earth’s Tectonic Plates (movie)
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Lithosphere & Asthenosphere
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Plate Boundaries
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Divergent Plate Boundaries
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Seafloor Spreading (movie)
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Convergent Plate Boundaries 1 2 3
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Seafloor Subduction (movie)
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Transform Plate Boundary strike-slip faulting
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Transform Faulting (movie)
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Plate Boundaries Hotspots
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Fig.4.20 Hot Spots hot spot trail
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Fig.4.22a Hot (not molten) rising plume lithosphere Direction of plate motion Formation of Island Chains V1 melting at base of crust V1
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Fig.4.22a Formation of Island Chains (movie)
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Fig.4.22b Example: The Hawaiian Chain Fixed hot spot
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Earth’s crust is divided into plates Plates move relative to one another at 1-15 cm/yr Plate interiors are largely undisturbed Deformation is concentrated at plate boundaries Consequences: Plate tectonics constantly change Earth’s surface Earthquakes occur mostly at plate boundaries Volcanoes occur mostly at plate boundaries Basic Premise of Plate Tectonics
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1.Examine volcanic rocks Q: what was the source for magma? How do we explore Earth’s interior? 2. Observe seismic waves from earthquakes Q: where are the layers, what are their densities? 3. Examine meteorites Q: what are they made of? like the core? 4. Existence and behavior of geomagnetic field Q: what is the core doing?
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Satellites1 (Moon) Size (radius)6378 km Bulk density5.5 g/cm 3 (4.1 g/cm 3 uncompressed) Surface gravity 9.8 m/s 2 Tectonism, volcanismyes (today) Rotation 1 day Orbit365.25 days Atmosphere 78% N 2, 21% O 2 Surface pressure1 atm Surface temperature 20°C (diurnal, seasonal changes) Plate tectonicsyes Wateryes Earth
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