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SRMP Dynamic Earth Curriculum - American Museum of Natural ...

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Science Research Mentoring Program<strong>Dynamic</strong> <strong>Earth</strong>Session Eight: Theory <strong>of</strong> Plate TectonicsACTIVITY: GeoworldAnalysis <strong>of</strong> hypothetical planet with plate tectonics. http://serc.carleton.edu/sp/library/guided_discovery/examples/geoworld.html This is a free resource; users should email the author indicatingwhere and how the lab is being used. This course divides the lab into two parts. As part <strong>of</strong> Lesson 8,students complete a modified version <strong>of</strong> Part 1, sections A,B,C,F,and G. Parts 2 and 3 are assigned ashomework.Hand out worksheet and materials (highlighters, rulers, calculators). Read through the instructionsand make sure students understand the key showing the reversals <strong>of</strong> Geoworld’s magnetic field overtime. Note that thickness in the key does not match thickness on the map; students need to considerthe relative thickness <strong>of</strong> each layer.Students work individually or in pairs. Start by working slowly though the first calculations insection A as a class. Make sure students understand how to calculate the rates, since they’ll need todo so as part <strong>of</strong> their homework. Discuss answers as a class. Students who finish early can work onsections F and G.Possible bodies to view:Body Features <strong>Dynamic</strong> ProcessesCallistoCraters, crater line, craterconcentric wrinklesNo volcanoes, or tectonicfeatures! Crust, salty ocean layer,not completely differentiated(shutdown <strong>of</strong> convection)Mercury Craters, streaks Has been geologically inactive forbillions <strong>of</strong> yearsMoon Craters, smooth areas Some shield volcanoes, volcanicdomes, presence <strong>of</strong> waterGanymedeStarburst patterns, some small craters,large slabs <strong>of</strong> darker materialEvidence <strong>of</strong> faulting / riftsEuropaMarsStreaks and scratches, some smallridgesCratered regions, large canyons,volcanoes, polar capsSmooth, young surface;tectonically active (water-icesurface) – possibly driven by warmplumes <strong>of</strong> water rising form deepinside the moonWas once tectonically active(straight line along Tharsis region);likely extinct nowIo Volcanoes See VenusVenus (Radar, then Elevation) Dendritic patterns, volcanoes Uniformly buoyant lithosphere(instead <strong>of</strong> negatively buoyant);melt-down 750 Ma (periodic),covering much <strong>of</strong> surface withvolcanism <strong>of</strong> some form© 2013 <strong>American</strong> <strong>Museum</strong> <strong>of</strong> <strong>Natural</strong> History. All Rights Reserved. 35

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