- Deformation Bands
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Deformation bands are small faults with very small displacements. In the past, these bands have been called Luder's bands or braided shear fractures.[1][2] They often proceed large faults. They develop in porous rocks, like sandstone. Material in a deformation band has a much smaller grain size, poorer sorting, and a lower porosity than the original sandstone. They can restrict and/or change the flow of fluids like water and oil. They are common in the Colorado Plateau.[3] Good examples form in the Entrada Sandstone in the San Rafael Swell in Utah.[4] The Mars Reconnaissance Orbiter showed deformation bands in Capen Crater, located in the Arabia quadrangle. The bands represent failure by localized frictional sliding. Deformation bands are present in a variety of porous rock types such as sandstones, limestones, siltstones, poorly welded volcanic tuffs, and breccias. The Cataclastic and compactional kind of bands often form seals and prevent the flow of liquids like water or oil. In their formation grains shift their packing and are crushed.[5][6]
References
- ^ Schultz, R. 2009. Fractures and Deformation Bands in Rock: A Field Guide and Journey into Geologic Fracture Mechanics. Oxford University Press
- ^ http://www.springerlink.com/content/r70236158556gww32/
- ^ http://folk.uib.no/nglhe/Utah.html
- ^ Schultz, R. 2009. Fractures and Deformation Bands in Rock: A Field Guide and Journey into Geologic Fracture Mechanics. Oxford University Press
- ^ http://mars.jpl.nasa.gov/mro/gallery/press/20080918c.html
- ^ Schultz, R. and R. Siddharthan. 2005. A general framework for the occurrence and faulting of deformation bands in porous granular rocks. Tectonophysics: 411. 1-18.
Categories:- Structural geology
- Geology stubs
- Mars stubs
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