Metamorphic core complex

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Metamorphic core complexes are exposures of deep crust exhumed in association with largely amagmatic extension. They form, and are exhumed, through relatively fast transport of middle and lower continental crust to the Earth's surface. During this process, high-grade metamorphic rocks (eclogite-, granulite- to amphibolite- facies) are exposed below low-angle detachment faults (mylonite shear zones) that show ductile deformation on the lower side (footwall) with amphibolite- to greenschist-facies syndeformational metamorphism, and ductile-brittle to brittle deformation on the upper-side (hanging-wall) with tilted geometries.

Descriptions[edit]

are characterized by a generally heterogeneous, older metamorphic-plutonic basement terrane overprinted by low-dipping lineated and foliated mylonitic and gneissic fabrics. An unmetamorphosed cover terrane is typically attenuated and sliced by numerous subhorizontal younger-on-older faults. Between the basement and cover terranes is a decollement and/or steep metamorphic gradient with much brecciation and kinematic structural relationships indicating sliding or detachment.

The decollement is also called a detachment fault.

Metamorphic core complexes form as the result of major continental extension, when the middle and lower continental crust is dragged out from beneath the fracturing, extending upper crust. Movement zones capable of producing such effects evolve in space as well as with time. Deforming rocks in the footwall are uplifted through a progression of different metamorphic and deformational environments, producing a characteristic sequence of (overprinted) meso- and microstructures.

Location[edit]

The core complex model was first developed in the cordillera of western North America, with northern cordilleran core complexes being Eocene in age, while those in Arizona to the south are younger. Core complexes are thought to be found in the Aegean, Anatolia, Iran, Tibet, north China, Slovakia (Janak et al. 2001), Venezuela-Trinidad (Miocene), and New Zealand. The youngest core complex is found in eastern New Guinea.

Core complexes on other planets[edit]

A feature at the center of Artemis Corona on Venus has been suggested as a metamorphic core complex (Spencer 2001). This could be the largest metamorphic core complex in the solar system.

See also[edit]

References[edit]

  • Coney, P.J. (1980). Cordilleran metamorphic core complexes. In Crittenden, M.D., Coney, P.J., and Davis, G.H. "Cordilleran Metamorphic Core Complexes". GSA Memoir (Geological Society of America) 153: 7–34. 
  • Janák, M.; Plašienka, D.; Frey, M.; Cosca, M.; Schmidt, S. TH.; Lupták, B.; Méres, Š. (February 2001). "Cretaceous evolution of a metamorphic core complex, the Veporic unit, Western Carpathians (Slovakia): P–T conditions and in situ40Ar/39Ar UV laser probe dating of metapelites". Journal of Metamorphic Geology 19 (2): 197–216. doi:10.1046/j.0263-4929.2000.00304.x. 
  • Lister, G.S.; Davis, G.A. (1989). "The origin of metamorphic core complexes and detachment faults formed during Tertiary continental extension in the northern Colorado River region, U.S.A.". J. Struct. Geol. 11: 65–94. doi:10.1016/0191-8141(89)90036-9. 
  • Spencer, J. E. (2001). "Possible giant metamorphic core complex at the center of Artemis Corona, Venus". Geological Society of America Bulletin 113 (3): 333–345. doi:10.1130/0016-7606(2001)113<0333:PGMCCA>2.0.CO;2. ISSN 0016-7606. 

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