Evolution of continents

Continents are made and deformed by plate motion

Continents are older than ocean rocks

Lithosphere floats on a viscous layer below the continents

Tectonics of North America

Shields

central, older portions of continents

low elevation and relatively flat

basement complex of metamorphic and igneous rocks

Stable Platforms

shields covered with a series of horizontal sedimentary rocks

many transgressions and regressions

sedimentary rocks are now preserved in large basins

Mountain belts

relatively narrow zones of folded, compressed rocks with associated magmatism

formed at convergent plate boundaries

two major active belts: Cordilleran (Rockies-Andies) and Alps-Himalaya

older examples include Appalachians and the Urals

Appalachian Mountains - eroded because they formed during assembly of Pangaea more than 270 m.y. ago. Consists of

Plateau - undeformed but uplifted sedimentary rocks

Valley and Ridge - folded and faulted sedimentary rocks

Blue Ridge - intensely deformed metamorphic complex

Piedmont and Coastal Plain - intensely deformed metamorphic complex with igneous intrusions

Multiple zones because Applachians formed from multiple collisions.

 

North American Cordillera - Complex geologic history from multiple episodes of deformation and magmatism over the past 500 million years. Includes Rocky Mountains, Basin and Range, and Sierra Nevada mountains. Western margin of U.S. was a subduction zone which was converted to a transform fault starting about 30 Ma as the Farallon plate completely subducted and a middle ocean ridge and a subduction zone met.

How Continents Grow

Magmatic differentiation: magma transferred to continents at subduction zones

Continental accretion: buoyant fragments of continents attached to continents as the result of plate motions

Accretion of Fragments

Accretion of Island Arcs

Accretion Along Transform Fault

Accretion by Continental Collision/Rifting

Suspect Terranes of Western North America - Multiple accretions of older island arcs, oceanic plateaus, oceanic crust, and marine sedimentary rocks during the subduction and eventual disapperance of Farallon plate

How Continents are Modified

The Himalayan Orogeny

60-40 Ma - The Indian Plate subducts under the Eurasian Plate. Passive margin on Northern India and active margin on Southern Asia

40-20 Ma - India subcontinent collides with Tibet and breaks along the Main Central Thrust fault. Passive and active margin sediments are folded, uplifted and partially eroded. Plastic thickening of southern edge of Asian continent

20-10 Ma - A second thrust fault forms, lifting the first fault. Himalayas mountains from from folded and faulted sediments and crust. Ganges plain subsides and fills with sediments from erosion of Himalayas. Tibetan Plateau forms from plastic thickening of southern edge of Asian continent.

Formation of Appalachian and Urals Mountains during assembly of Pangea

510 Ma - after breakup of Rodina supercontinent, U.S is part of Laurentia continent

450 Ma (Taconic orogeny) - Laurentia collides with island arcs

400 Ma ( Acadian and Caledonian orogenies) - Laurentia collides with Baltica and forms contintent of Laurussia.

340 Ma (Variscan orogeny) - Collision of Laurussia and Gonawana starts in what is now Europe

300 Ma (Appalachian, Ural and Hercynian orogenies) - collision of Laurussia and Gonawana continues between what is now Europe and Africa and extends into what is now North America, Siberia collides with Laurussia forming the Ural mountains.

270 Ma - Assemby of Pangaea is complete.

Wilson Cycle - Edges of many cratons have experienced multiple episodes of a plate tectonic cycle

Rifting during breakup of a supercontinent

Passive margin cooling and sediment accumulation as ocean basin opens

Active margin volcanism and terrane accretion during subduction and ocean closure

Orogeny during continent-continent collision that forms next supercontinent

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