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Glarus overthrust fault - david martineau

3/30/2015

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Figure 1 (left) shows the location of Glarus fault in google maps. Figure 2 (right) shows a zoomed satellite view on the region in which the Glarus fault is located. 
The Swiss Alps are both magnificient and impressive, luring lots of tourists every year. Apart from drawing tourists, this fairly new mountain range also attracts many geologists. A distinct line (as seen in Figure 5) seperating two rock layers outcrops at numerous locations in the Swiss Alps; this is known as the Glarus Overthrust Fault. The Glarus Thrust is located in the eastern part of the Alps of Switzerland. The thrust is exposed over a large area in the Canton of Glarus, St. Gallen and Graubünden regions.  
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Figure 3: Picture of the Hausstock peak, cleary showing a fault line and labeling different rock units (Gasser, Brok, 2008)
A thrust fault is simply a low-angle reverse fault, especially if that fault extends for several to hundreds of kilometers such as the Glarus Thrust (Fossen, 2010). Since a thrust fault dips at a low angle, it is possible for compression to push older rock sequences above younger ones. According to Herwegh et al., the Glarus Thrust dates back to the Oligocene-Miocene age, roughly 35 to 5 millions years ago. The fault separates the Glarus nappe from its footwall with a total displacement of at least 30 to 40 km (2006). As shown in Figure 3, the top of the Hausstock peak constitutes of Verrucano rocks, which form the base of the Helvetic Nappes. These rocks consists of rhyolitic and spilitic layered volcanic rocks, as well as red beds and conglomerates, dating back to the Permian (299 to 251 Ma)  (Raumer, Neubauer, 1993). The Verrucano beds can be seen at the base of the Helvetic nappes in some areas but in others, can overlie folds and younger rock strata (Herwegh et al., 2006). The Helvetic Nappes and Subhelvetic Units, overthrust the Wildflysh Nappe and the North Helvetic Flysch (NHF), hence known as Infrahelvetic complex. The NHF consists mainly of turbiditic sandstones and slates dating back to the Early Oligocene (roughly 34 Ma) (Gasser, Brok, 2008). The Glarus fault is an important feature in the geological world because it is shows a very clear example of a thrust fault where the nappe contact is extremely clear and is also visible in three-dimensions. Furthermore is has played a role in the history of geology, as it was not always clear that thrusting was the answer to this phenomenon (Buckingham et al., 2013). 
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Figure 4: Geological map of the Glarus fault (Herwegh et al., 2006)
In the geological map of the Glarus Overthrust (Figure 4), the thrust line seems to somewhat follow the topography (circles around the peaks, observable even though the geological map does not include contour lines). This is caused by the fault dipping at a low angle. When the rock beddings are horizontal or nearly horizontal, their contacts will also be horizontal. Therefore, on a topographic map, the bedding contacts will run parallel to the contour lines (UOregon, 2010). This is also true for faults, explaining why the fault line seems to follow topography. On this map, the dark line with arrows is the Glarus fault line. The darkest layer is the Permian Verrucano rocks, while the white layer is the younger, Oligocene Flysch units. The Flysch Units in this map refer to the NHF as well as the Wildflysch Nappe. The flysch units contain many folds and other deformations. The map shows that the Helvetic Nappe, which contains the Verrucano rocks as well as Mesozoic-Cenezoic sediments, overlay the Infrahelvetic complex, which inclides the Flysch units, a Mesozoic cover and a crystalline basement. The older Helvetic Nappe overlays the Infrahelvetic complex along the thrust line, showing that the thrust fault was responsible for this displacement. The numbers on this map are irrelevant for the purpose of this text, they simply correspond to stops visited by Herwegh et al. in 2006. 
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Figure 5: The Glarus Thrust seen from the Tschingelhorner region (Imper, 2011)
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Figure 6: Profile of Glarus Thrust showing erosion of the overthrusted rock sequence (Verrucano) (Imper, 2011)
In Figure 5, the Flysch rocks are the brownish rocks underneath the darker coloured rocks (Verrucano). As mentioned ealier, the Flysch rocks are sedimentary rocks and contain shale and sandstone. Also, in the Tschingelhorner region, a limestone level dating back between 100 and 150 ma can be identified between both rock layers. This limestone layer would have also been brought with the Verrucano rocks along the fault. Figure 6 shows the cross-section profile between Tschingelhorner and Charpf. The Verrucano rocks are exposed in the regions of Tschingelhorner and Charpf but are missing in the area in between (surroundings of Elm). This valley was formed by erosion, which is why the Verrucano rocks are missing. By looking at Figure 6, it is easy to observe that both of the Verrucano outcrops on either side are part of the same bed and would have been connected prior to erosion. The surrounding rocks around the Glarus fault are also caracterized by folds such as in the Flysch rocks (Imper, 2011). 
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Figure 7: View of the Glarus Thrust in Tschingelhoren, showing thrusting as well as deformation in units (Herwegh et al., 2006)
The deformation that took place in the Infrahelvetic Complex occured in three phases. During the first phase, the Sardona and Blattengrat Nappes slid onto the NHF. The Sardona and Blattengrat Nappes consist of Late Cretaceous and Eocene limestones, marls and marine sandstones. This phase could have occured by gravity sliding. In the second phase, the Infrahelvetic Complex was subjected to folding. The third phase is the development of the Glarus Thrust. The Glarus thrust is an out-of-sequence thrust, where a minimum displacement of 35 km which formed a steep crenulation cleavage below the thrust. Another theory is that the Sardona and Blattengrat Nappes were not caused by gravity sliding but by compressional tectonics. This could have thrusted and folded the NHF Unit. Also this theory suggests that the Glarus thrust was first displaced between 25 to 30 km and was later followed by another 5 to 10 km displacement. The Infrahelvetic complex would have been folded during the first displacement and would have developed its steep crenulation cleavage during the second displacement (Gasser, Brok, 2008). Figure 3 shows an example of this folding in the NHF. Figure 7 shows the Verrucano rock layer thrusted over the Quinten Formation (Qu). Underneath the Ofen (middle), the Qu displays a large syncline fold with parasticic folds which have been destroyed by the Glarus Thrust. On the left of the picture, there is a large recumbent fold which consists of Mesozoic and Cretaceous sediments. There is also an alteration zone between some of the Verrucano and Flysh Units contacts that can be observed. This alteration zone was caused by the friction heat released when the thrust was displaced (Herwegh et al., 2008). 
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Figure 8: Schematic diagram of an overthrust formation (Buckingham et al., 2013)
According to Buckingham et al., the stress which caused the Glarus Oversthrust, was the formation of Alps. The Alpine Orogeny is thought to have been formed by two different orogenies; one during the Cretaceous and one during the Tertiary. The formation of the Alps was caused by the collison of the European continent and the Adriatic continent, after subducting the ocean basins in between, like the Tethys Ocean. There is still shortening in the eastern part of the Alps today (Froitzheim, 2012). The Glarus Thrust was formed during the second part of the orogeny. This collision caused enough stress to push the older rock layers (Verrucano), along the low-angle thrust fault, above the younger sequences. Figure 8 shows an example of how overthrusts are formed, causing older rocks to lie on top of younger ones. The large white arrows show the direction of compression. As the figure illustrates, the fault has to be dipping at a low-angle. If it was not, the compression would simple cause a reverse fault and this inversion in rock layers could not be observed.


References:

Buckingham, Thomas, Walker Simon, Jurg Meyer, and Harry Keel. "Swiss Tectonic Arena Sardona." Unesco World Heritage, v3.0. 7 Aug. 2013. Print.

Fossen, Haakon. Structural Geology. Cambridge: Cambridge UP, 2010. Print.

Froitzheim, Nikolaus. "Geology of the Alps Part 1: General remarks; Austroalpine nappes." Structural Geology. University of Bonn, Germany. 27 Mar. 2012. PDF.  
<http://www.steinmann.uni-bonn.de/arbeitsgruppen/strukturgeologie/lehre/wissen-gratis/geology-of-the-alps-part-1-general-remarks-austroalpine-nappes>.



Gasser, Deta, and Bas Brok. "Tectonic Evolution of the Engi Slates, Glarus Alps, Switzerland." Swiss Journal of Geosciences 101 (2008): 311-22. Print.

Herwegh, Marco, Jean-Pierre Hürzeler, O. Adrian Pfiffner, Stefan M. Schmid, Rainer Abart, and Andreas Ebert. "The Glarus Thrust: Excursion Guide and Report of a Field Trip of the Swiss Tectonic Studies Group (Swiss Geological Society, 14.–16. 09. 2006)." Swiss Journal of Geosciences: 323-40. Print.

Imper, David. "Elm-Linthal: Crossing the Richetlipass." Federal Office of Topography Swisstopo. Swisstopo, 15 Feb. 2011. Web. 30 Mar. 2015. <http://www.swisstopo.admin.ch/internet/swisstopo/en/home/topics/geology/viageoalpina/VGA_Sardona.parsys.000101.downloadList.80281.DownloadFile.tmp/stage0610elmlinthalen.pdf>.

Raumer, J. F. Von. Pre-Mesozoic Geology in the Alps. Berlin: Springer-Verlag, 1993. Print.

University of Oregon. "Outcrop Patterns." Structural Geology. 2010. Web. 29 Mar. 2015. <http://pages.uoregon.edu/millerm/Srpatterns.html>.




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The San Rafael Swell by Lorraine Hamel

3/30/2015

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The San Rafael Swell lies in Emery County and northern Wayne County in central Utah (Figure 1 shows the exact delimitations of the San Rafael Swell) (Gilluly 1928, Freeman et al. 2008). It is a broad, asymmetrical, anticline stretching about 50 km long and 120 km wide (Jeffrey et al. 2011). The major axis of the anticline, from south to north, first trends north-northeast. Then, it abruptly turns east-northeast in the central part of the swell, and then north-northeast again. The San Rafael Swell has elevations ranging from 4000 to 7000 feet above sea level. Beds over the eastern edge of the swell have elevations ranging from 4000 to 6000 feet above sea level and dip steeply eastward. These beds are dominated by a monoclinal fold with a central limb dipping eastward as well (Freeman et al. 2008, Johnson & Johnson 2000). Beds over the center and on the west edge of the uplift dip gently westward with a dip angle of two to five degrees west, and have elevations ranging from 6000 to 7000 feet above sea level (Freeman et al. 2008, Hawley et al. 1968). See Figure 2 for a picture of a portion of the San Rafael Swell.

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Figure 1. San Rafael Swell Specific Delimitations http://files.geology.utah.gov/maps/geomap/30x60/pdf/ofr-404.pdf

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Figure 2. Portion of San Rafael Swell, "The Reef" Section (Johnson & Johnson 2000)
Differential erosion from resistance in different sedimentary rocks has carved the San Rafael Swell into a distinctive topography (Gilluly 1928). Exposed sedimentary rocks from the uplift range in age from the Carboniferous to Jurassic periods (Bartsch-Winkler et al. 1990). The inner part of the San Rafael Swell, called Sinbad Country, is underlain mainly by rocks of Permian and Triassic age. This section is of low relief. The outer part of the swell is a steep ridge, called the Reef. It is formed mainly of resistant sandstone of the Glen Canyon Group of Triassic and Jurassic age. The Carmel Formation of Middle and Late Jurassic age and younger strata are exposed outside the Reef, while the oldest rocks exposed in the San Rafael Swell crop out in the deep canyons of Straight Wash and the San Rafael River; they are probably of Early Permian and Pennsylvanian age  (Hawley et al. 1968). The central limb is characterized morphologically by Navajo Sandstone (Johnson & Johnson 2000). This can be seen in the following geologic map and profiles (Figure 3 and Figure 4).

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Figure 3. Geologic Map and Cross-Section of San Rafael Swell http://written-in-stone-seen-through-my-lens.blogspot.ca/2011/08/flight-plan-part-i-geology-of-san.html

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Figure 4. Cross-Section of San Rafael Swell http://www.lemkeclimbs.com/san-rafael-swell.html

Most of the rocks of the San Rafael Swell have been uplifted, crossfolded, and involved in nearly-vertical-sided collapse. Deformation in the region happened in Precambrian, Paleozoic, and Mesozoic time. Frequent deformation, uplift, intrusion, and faulting could have occurred in zones of weakness throughout this geologic time interval (Bartsch-Winkler et al. 1990). Many high-angle faults cut the sedimentary rocks. Most are normal faults, but a few reverse faults are also present. High-angle faulting probably started around the time of folding in earliest Tertiary time but reached maximum proportions later in the Tertiary. A few faults may be older than early Tertiary (Hawley et al. 1968).

Bibliography

Delaney, Paul T. and Anne E. Gartner. 1997. "Physical Processes of Shallow Mafic Dike Emplacement Near the San Rafael Swell, Utah." Geological Society of America Bulletin 109 (9): 1177-1192. http://gsabulletin.gsapubs.org/content/109/9/1177.short

Hawley, C.C., R. C. Robeck, and H. B. Dyer. 1968. "Geology, Altered Rocks And Ore Deposits of The San Rafael Swell Emery County, Utah" U.S. Department of the Interior, U.S. Geological Survey http://pubs.usgs.gov/bul/1239/report.pdf

Jeffery, D. L., J. L. Bertog, and J. R. Bishop. 2011. "Sequence Stratigraphy of Dinosaur Lake: Small Scale Fluvio-Deltaic Stratal Relationships of a Dinosaur Accumulation at the Aaron Scott Quarry, Morrison Formation, San Rafael Swell, Utah." Palaios 26 (5): 275-283. http://palaios.sepmonline.org/content/26/5/275.short

Johnson, K. M. and A. M. Johnson. 2000. "Localization of Layer-Parallel Faults in San Rafael Swell, Utah and Other Monoclinal Folds." Journal of Structural Geology 22 (10): 1455-1468. http://www.sciencedirect.com/science/article/pii/S0191814100000468

Bartsch-Winkler, Susan, Robert P. Dickerson, Harlan N. Barton, Anne E. McCafferty, V.J.S. Grauch, Hayati Koyuncu, Keenan Lee, Joseph S. Duval, Steven R. Munts, David A. Bemjamin, Terry J. Cclose, David A. Lipton, Terry R. Neumann, and Spencee Willett. 1990. "Mineral Resources of the San Rafael Swell Wilderness Study Areas, Including Muddy Creek, Crack Canyon, San Rafael Reef, Mexican Mountain, and Sids Mountain Wilderness Study Areas, Emery County, Utah." U.S. Geological Survey, U.S. Bureau of Mines http://pubs.usgs.gov/bul/1752/report.pdf

Gilluly, James. 1928. "Geology and Oil and Gas Prospects of Part of the San Rafael Swell, Utah." Contributions to Economic Geology http://pubs.usgs.gov/bul/0806c/report.pdf

Freeman, Michael L., David L. Naftz, Terry Snyder, and Greg Johnson. 2008. "Assessment of Nonpoint Source Chemical Loading Potential to Watersheds Containing Uranium Waste Dumps Associated with Uranium Exploration and Mining, San Rafael Swell, Utah." U.S. Department of the Interior, U.S. Geological Survey http://pubs.usgs.gov/sir/2008/5110/pdf/sir20085110.pdf

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March 30th, 2015

3/30/2015

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The Muddy mountain thrust: louis Warnock

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The Muddy Mountain Thrust was formed by a thrust sheet and is located in Southern Nevada, between Las Vegas and the Valley of Fire, in the Buffington Window (see fig. 1). It is oriented roughly in the east-west direction, overthrusting towards the east. The overthrust extends a minimum of 210 km, from the Clark Mountains to the Muddy Mountains. It is to be highlighted that its strike is offset by the Las Vegas shear zone. Palezoic carbonates are found thrusting above younger Mesozoic Sandstone (see fig. 2) and the thrust sheet itself is thought to be between 24 and 40 km in width, although some estimates are as large as 80 km (see fig 1). Its minimum thickness is constrained to 4-5 km; 2-2.5 km of dolomite/limestone and 2-2.5 km of sandstone. Therefore, considering the range of widths and thicknesses of the thrust sheet, its area is at least 3800 km2 (Brock & Engelder 1977). 

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                                     Figure 1.  Geological map of the Muddy Mountain thrust (Fossen, 2015) 

Below the fault plane is Jurassic Aztec sandstone composed of medium-to-fine grained and well-rounded quartz (eolian sandstone). It is red-brick in color, although bleaching is observed in some instances near the fault. In some parts, the thrust moves across a sandstone which has filled topographic depression through surface erosion; the grain size of this sandstone is similar to that of the Aztec sandstone below it, although the sorting is poorer and the grains are show more angularity (Brock & Engelder, 1977). This sandstone is referred to as molasse by Cayeux (1929). Erosional pockets filled by the molasse and channel cuts in the Aztec sandstone is fluvial, indicated that the faulting must have been near-surface; however, the molasse is some distant away from the leading edge of the thrust, meaning erosional depressions must have been filled before the thrusting. The contact between the molasse and the erosional surface of the Aztec sandstone is parallel to the fault line.

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        Figure 2.  Cross-sectional view of the Muddy Mountain overthrust

The thrust was measured to have a dip of 55˚ north in the northern sector (Brock & Engelder, 1977). Several elements of the structure are evidence for thrusting: an increase in intensity of microfractures parallel to and at small angle of contact, a cataclastic decrease in grain size as we approach the contact, an increase in the degree of induration, a loss of well-defined beddings and an increase color contrasts in the sandstone and shearing of dolomite in the upper crust. The zone of deformation (that is, fracturing and cataclasis) associated with the faulting extends as much as 75 m down into the Aztec Sandstone and more than 100 m up into the Goodsprings Dolomite. In the overthrust sheet, there is presence of brecciation and shattered carbonates measuring up to 5 m with gauge injections around them (Brock & Engelder, 1977). In the lower plate, cataclastic deformation has caused angular clasts with finer and more poorly sorted grains than the undeformed sandstone (Graph 1). Microfracturing positively correlates with cataclasis in the sandstone. The zones of induration (cemented sandstone) range from 1 to 5 m in thickness, and the cementation occurs at 10 to 15 m from the contact, although it is also shown in areas as far as 50 m away from the contact (Brock & Engelder, 1977). The induration is caused by lithostatic stress of the thrusting load above. Fractures with low-angle to contact line are associated with this induration. The shortening direction of the deformation bands in the Aztec Sandstone is analogous to that of the Cordilleran thrust belt.
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                                                 (Brock & Engelder, 1977)
The deformation is strongly localized to the thrust zone. A planar contact with a narrow gouge zone is visible for several hundred meters of outcrop (see fig 3). This gauge has a thickness which ranges between 3 and 30 cm and was generated by cataclasis and a high mobility, allowing it to flow in cracks of upper layer. Less than 30% of the grains are larger than 100 micrometers; thus, the gauge is fine-grained (Brock & Engelder, 1977). As many as three foliated gauge layers appear within the more granular material, representing shear zones and indicating differential movement and relative slip in the upper plate; the microfracture orientations in the quartz gouge and the cataclastic sandstone next to a shear fracture gives an indication of the orientation of the stress field in which the gouge was formed (parallel to the maximum principal stress). The shear displacement along the fault is restricted to a gouge zone 5 to 20 cm thick at the fault contact. The fault gauge is injected into dolomite cracks of upper layer, which contains the largest percentage of fragments of less than 25 micrometers (Brock & Engelder, 1977). Either the injection promotes further cataclastic deformation, or this flow process acts as a barrier against coarser fractions. The quartz gauge strongly reduces frictional resistance, promoting strike-slip motion. The presence of widely distributed band populations and of compactional bands in the porous sandstone indicate the contractional nature of the deformation (Fossen, 2015) .

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Figure 4.             Principal stresses acting on the Aztec                                 Sandstone (Fossen, 2015)

The thrusting is related to the Cretaceous to early Paleogene Sevier orogeny of the North American Cordilleran thrust system. In the early stages of the Muddy Mountains development, contraction was occurring at shallow burial depths, causing compactional bands (see fig 4): shear-enhanced compaction bands (SECB) and pure compaction bands (PCB) in the porous parts of the sandstone. Later, thinner and more offset cataclastic shear bands (CSB) would reflect a higher degree of cataclasis associated with shearing in a less porous medium, where the shear stress is generated by friction on the fault (Fossen 2015). The presence of SECBs and PCBs supports the idea that low differential stress is related to this contractional regime. Experimentally, it has been shown that locally the deformation is lithologically controlled (i.e. grain size and porosity), whereas the stress path depends on the overburdern; it is the contraction (the compaction) that results in well distributed bands in the Aztec Sandstone (Soliva et al., 2013). Thrusting occurred slowly and was near-surface.
Works cited
Brock, William G., and Terry Engelder. "Deformation associated with the movement of the Muddy Mountain overthrust in the Buffington window, southeastern Nevada." Geological Society of America Bulletin 88.11 (1977): 1667-1677.

Fossen, H., Zuluaga, L.F., Ballas, G., Soliva, R., Rotevatn, A., Contractional
deformation of porous sandstone: insights from the Aztec Sandstone, SE Nevada, USA, Journal of Structural Geology (2015), doi: 10.1016/j.jsg.2015.02.014.

Soliva, R., Schultz, R.A., Ballas, G., Taboada, A., Wibberley, C., Saillet, E., Benedicto, A., 2013. A model of strain localization in porous sandstone as a function of tectonic setting, burial and material properties; new insight from Provence (southern France). Journal of Structural Geology 49, 50-63.

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March 30th, 2015

3/30/2015

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THe Himalayan Frontal Thrust by thomas St-Laurent

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Figure 1. Himalayas
The Himalayan mountain range is one of the biggest mountain ranges of the world. It spans 2900 km across Nepal and India. Notably, Mount Everest (shown by a white triangle), with a peak above 9 km in altitude, the highest point on the Earth, is in the Himalayan mountain Range.

The Himalayan Frontal Thrust, also known as Himalayan Frontal Fault, is the youngest and most active fault of the Himalayas. The three main Himalayan faults are the Himalayan frontal thrust, the Main Boundary Thrust and the Main Central Thrust (not shown).
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Figure 2. Himalayan Frontal Thrust and Main Bounday Thrust ( 6 )
This immense mountain range has a long history. To understand how it came to be, we have to travel back to Pangea, the supercontinent.

About 225 Ma, the landmass that we know today as India was still attached to what is today known as Africa. Over the next 25 million years, the Indian tectonic plate slowly broke off of Africa and headed north to Asia. Fast forward to 80 Ma; the Indian land mass, moving at a speed varying from 15 to 20 cm/yr, is nearly six and a half thousand kilometer away from the Eurasian tectonic plate. Over the next 70 million years, the Indian plate finished its voyage across the ocean and 10 Ma, collided with the Eurasian plate.
Once the two tectonic plates collided this caused enormous stress on the two plates. “Neither continental plate could be subducted due to their low density/buoyancy. This caused the continental crust to thicken due to folding and faulting by compressional forces.” (1) In this way we can understand that there was crustal shortening in the north-south direction. With all that landmass under stress from all directions, the landmass went in the only possible direction to relieve the stress, skyward, at a rate of “1 cm per year” (2). This process is still happening, the two plates are still being pushed into each other. However, erosion from the melting of icecaps dampens the growth of the mountains.

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Figure 3. Indian-Eurasian Collision (1)
For a more in depth animation of the formation of the Himalayan Mountains, consult: http://www.geolsoc.org.uk/Plate-Tectonics/Chap3-Plate-Margins/Convergent/Continental-Collision

The initial collision of the two tectonic plates occurred while there was still a sea separating the Asian and Indian land masses. Once these two tectonic plates collided, the velocity of the Indian plate decreased significantly to 5 cm/yr. As the two land masses approached each other, the sea floor sediments were compressed and brought to the surface with the thickening of the crust. The two land masses officially collided when the sea was completely drained. Since the initial collision, several enormous earthquakes occurred to relieve this stress. The main central thrust was formed upon this initial collision and over the next few million years the main boundary thrust was created. “The initiation age of the [Himalayan Frontal Thrust] is constrained between 500 and 100 Ka.” (3) The Himalayan Frontal Thrust is the youngest and thus the most active out of the Himalayan Thrusts. “The [Main Central Thrust] is mainly inactive […] and the [Main Boundary Fault] in localized areas exhibits neotectonic acticity.” (3)

We know The Himalayan Frontal Thrust itself is a NW-SE trending thrust fault where the hanging wall is pushed up the footwall. The Frontal Thrust is the boundary between the Sub-Himalaya, often called Siwalik layer, and the north Indian plains. “A slip rate of ≥ 13.8 ± 3.6 mm/yr on the [Himalayan Frontal Thrust] has been estimated on the basis of a radiocarbon date, […] assuming an average fault dip of NE 30°” (3). This is thrusting the Siwalik layer above and onto the Ganges plains. The Siwalik layer is made up of Cenozoic sediments and consists mostly of animal fossils, elephants and horses, to name a few, that made up the wildlife at the time. The northern plains consists of the youngest sediments and the youngest layer of the Himalayan region.
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Figure 4. Geological Cross section of Himalayan region (4)
The Himalayan Frontal thrust was originally thought to be a blind fault. An apparent anticline could be seen following a certain line, with shortening in a direction perpendicular to said line. An age disconformity could also be seen, with the older layer on top. With these indications, geologists explained the deformation by a blind thrust. However, recently, researchers from the Center of Neotectonic Studies of the University of Nevada, the Department of Geological Sciences of San Diego State University and the Wadia Institute of Himalayan Geology of Dehra Dun have shown evidence for traces of the exposed Himalayan Frontal Thrust. These researchers have found that at many sites along the Himalayan Frontal Thrust, namely, Rampur Ganda, Lal Dhang and Ramnagar, “trench exposures and vertical separations of 9-13 m are interpreted to indicate about 13 – 26 m of coseismic slip during the last earthquake.” (5) By analyzing these locations, these geologists have been able to date the simultaneous fracture to 1413 ± 9 A.D5. This indicates that a powerful earthquake caused more slip along the fault at this date. A few earthquakes have occurred in the last century, “the 1905 Kangra earthquake, 1934 Bihar-Nepal earthquake, and 1950 Assam earthquake.” (5) However, little is recorded of the surface rupture that happened during these earthquakes. The aforementioned geologists believe “that the earthquake recorded in the trenches is larger than historical earthquakes and indicate a potential for sections of the [Himalayan Frontal Thrust to rupture simultaneously along lengths of the [Himalayan Frontal Thrust]” (5)

                This is quite an important observation since the fault is still active, geologists and geophysicists will be better suited to study the Himalayan Frontal Thrust. They will then be able to make predictions about potential seismic activity in the area. Similarly, with a better understanding of the geology of the fault scientists, could make better estimations of what the Himalayas will look like in the near and distant future.
Works Cited

http://pubs.usgs.gov/gip/dynamic/himalaya.html (2)

http://www.geolsoc.org.uk/Plate-Tectonics/Chap3-Plate-Margins/Convergent/Continental-Collision (1)

http://www.iisc.ernet.in/currsci/jun102004/1554.pdf (3)

https://www.himalayanclub.org/hj/66/9/geologic-formation-of-the-himalaya/ (4)

http://cires1.colorado.edu/~bilham/HimalayanEarthquakes/Himalayan_thrust.pdf  (5)

http://suvratk.blogspot.ca/2010/10/going-hiking-in-lesser-himalayas.html  (6)

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The Champlain Thrust - Cam Roy

3/30/2015

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Fig. 1 - Approximate fault trace of the Champlain Thrust Fault, running from near the Canadian border to the Catskill Plateau (VGS 2003)
Vermont is best known for its bucolic countryside, cows, hippies and Champ, the friendly monster of massive Lake Champlain. While most visitors to the Green Mountain State pass their time skiing or eating Ben and Jerry’s, geologists flock to an outcrop on the shores of Lake Champlain, near Burlington. Lone Rock Point offers the best glimpse of the Champlain Thrust – an approximately 200 mile thrust fault that was active around 450 million years ago (Vermont Geological Survey, 1998).

Thrusts are low angle faults where the hanging wall is displaced over the footwall, created under contractional tectonic regimes (Fossen, 2010). In the case of the Champlain Thrust, compressional stress was the result of the Taconic Orogeny, a mountain-building process that formed the Green Mountains from 500-400 million years ago. Skiers can thank the Taconic Orogeny event for Jay Peak, Mount Mansfield, Mont Ellen and Killington Peak, among many others. As the North American continent was subducted under the oceanic crust (as the ancient Iapetus Ocean closed), an accretionary prism formed. Thrust faults developed in this accretionary prism (Fig. 2) due to the high compressive stress, most prominently the Champlain Thrust (Stanley 1987).


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Fig. 2 - Diagram of stress that caused the Taconic Orogeny (from Johnson, 1998) CLICK ON IMAGE FOR CLOSER VIEW
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Fig. 3 Sketch of the Champlain Thrust near Lone Rock Point (Stanley 1987)
The east-dipping thrust has shoved older Cambrian rock over younger Ordovician rock to the west (see geologic map - Fig. 2). The phenomenon of older rock overlying younger rock is clearly visible at Lone Rock Point (Fig. 3). The carbonate Cambrian rock (hanging wall) is Dunham Dolostone, visible at many outcrops in the Champlain Valley. The less resistant Ordovician rock (footwall) is a dark gray shale known as the Iberville formation, and also includes flysch and melange. The unconformity between the Ordovician shale and the Cambrian dolostone is striking because the shale has been deformed much more than the more resistant dolostone (University of Vermont, 2010). The exposed fault zone is notably planar and continuous (Stanley, 1987).


The throw of the fault at Lone Rock Point is estimated at 8,850 feet (Vermont Geological Survey, 1998). Moving north from Lone Rock Point, the throw decreases as the fault moves up towards Canada (Stanley 1987). Displacement is taken up by other thrust faults near Philipsburg, Qc., eventually becoming Logan’s Line (which separates the folded Appalachian rocks from the flat Paleozoic sedimentary beds of the St. Lawrence Valley). These other thrust faults are part of the so-called Taconic thrust belt (see Fig. 4). The Champlain Thrust is considered to be the frontal and basal fault of this forward-propogating system of ancient thrusts (Hayman and Kidd, 2002). The throw of the Champlain fault decreases south of Lone Rock Point as well, estimated at 6,000 feet just south of Burlington, tailing off to the south (Stanley, 1987). The trace of the Champlain Thrust is relatively straight and easy to follow north of Burlington. It strikes to the north and dips at approximately 15° to the east (Stanley, 1987). Moving south from Burlington, however, the trace becomes increasingly obscured by higher angle faults that have formed more recently than the original thrust, as evidenced in the geologic map (Fig. 2). 


Displacement along the thrust was originally estimated at 9 miles (Doll et al. 1961). Stanley (1987) bumped up the estimate to 35-50 miles, while Rowley (1982) proposed displacement of 65 miles using a new method based on study of sedimentary sequences across Atlantic-type margin continental shelves.
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Fig. 4 - Geologic map of Vermont (VGS, 1970) Red-Igneous Rocks; Blue-Silurian-Devonian; Pink-Ordovician (i.e. Iberville Shale, "footwall" of thrust fault); Yellow-Cambrian (i.e. Durham Dolostone, "hanging wall" of thrust fault); Orange-Precambrian
Geologists have long been puzzled over certain structures and stratigraphic profiles associated with the Champlain Thrust, and more generally the Taconic Thrust Belt. West-central Vermont is not exactly Structural Geologist Heaven - there is not an abundance of outcrops and it is often hard to differentiate sedimentary facies. Hayman and Kidd (2002) proposed that there has been reactivation of pre-thrusting, flexure-induced normal faults, as well as one post-thrust normal fault (the Mettawee fault) that obscures the original thrust map pattern. The Mettawee fault reduces the map width of the Champlain Fault and decreases the apparent differences in structural level between the Champlain fault and nearby thrust fault systems. The exact age of the Mettawee fault is unknown, although it is believed to have formed some time after the Champlain Thrust but still during the Taconic orogeny event (Hayman and Kidd, 2002).

The Champlain Thrust is a visible reminder of the ancient orogeny that created the Green Mountains. The next time I find myself in Burlington, VT, I think I will make a pilgrimage to Lone Rock Point to admire the dolostone and shale, run my hand along an ancient fault and maybe catch a glimpse of Champ.
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Fig. 4 - Geologic provinces of New England (Hayman and Kidd 2002). All faults are normal except for the Champlain Thrust and the rest of the Taconic thrust belt (including Quebec's Logan Line) CLICK ON IMAGE FOR CLOSER VIEW
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Fig. 5 - Champlain Thrust at Lone Rock Point in Burlington, Vermont, looking east from Lake Champlain. Older Dolostone overlies younger Shale. Photo taken on June 13, 2004. © 2004 Stephen S. Howe. From the Vermont Geological Society
References


Doll, C.G., Cady, W.M., Thompson, J.B. and Billings, M.P. (1961). Centennial geologic map of Vermont Montpelier, Vermont Geologic Survey, scale 1:250,000.

Fossen, H. (2010). Structural Geology. Cambridge: Cambridge University Press.

Gale M. (1998). “Geology of Vermont: Champlain Thrust Fault at Lone Rock Point, Burlington VT”. Vermont Geological Survey. Accessed March 17, 2015. http://www.anr.state.vt.us/DEC/geo/chthrust.htm

Hayman, N. W., & Kidd, W. S. F. (January 01, 2002). Reactivation of prethrusting, synconvergence normal faults as ramps within the Ordovician Champlain-Taconic thrust system. Geological Society of America Bulletin, 114, 476-489.

Johnson, C.W. 1998. The Nature of Vermont: Introduction and Guide to a New England Environment. UPNE, 2nd Edition. ISBN: 0874518563

Rowley, D. B. (August 01, 1982). “New methods for estimating displacements of thrust faults affecting Atlantic-type shelf sequences: With an application to the Champlain Thrust, Vermont.” Tectonics, 1, 4, 369-388.

Stanley, R.S., 1987, “The Champlain thrust fault, Lone Rock Point, Burlington, Vermont”.  Geological Society of America Centennial Field Guide - Northeastern Section.

University of Vermont. “Geologic History of the Champlain Valley” UVM.edu. Accessed March 17, 2015. http://www.uvm.edu/shelburnelandscape/nature/geology.html

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The Moine thrust Belt, Scotland - Jade Sauvé

3/29/2015

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general location of the moine thrust belt

PhotoFigure 1: Google map of Scotland identifying the limits of the Moine Thrust Belt
In 1907, we discovered the Moine Thrust Belt situated in northwest Scotland.  This was truly important scientifically as it was the first thrust belt recognized as such and it substantiated the tectonic plate theory (Wikipedia).  The Moine Thrust Belt, and its associated Moine Supergroup outcrop (Neoproterozoic metamorphic rocks), was formed during the Caledonian orogeny (Kocks et al. 2014) (Johnson 1965).  This mountain building event followed the closure of the Iapetus ocean (Kocks et al. 2014).  There first was an arc-continent collision named Grampian event during the Ordovician (Kocks et al. 2014).  This was followed by an oblique collision of three other proto-continents in the Silurian period (Kocks et al. 2014).  Scotland suffered a great compression as the European plate was carried toward the west above the old Lewisian gneisses present on the Laurentian plate (Wikipedia). The Moine Thrust Belt joins Loch Eriboll, on the north coast of Scotland, to the Sleat peninsula on the Isle of Skye further southwest (see the two red dots on Figure 1) (Wikipedia).
Image credits: By Eric Gaba (Sting – fr:Sting) [GFDL (http://www.gnu.org/copyleft/fdl.html) or CC BY-SA 4.0-3.0-2.5-2.0-1.0 (http://creativecommons.org/licenses/by-sa/4.0-3.0-2.5-2.0-1.0)], via Wikimedia Commons

PhotoFigure 2: Geological map of Northern Scotland Image credit: "Hebridean Terrane" by Mikenorton - Own work. Licensed under CC BY-SA 3.0 via Wikimedia Commons - http///commons.wikimedia.org/wiki/File/Hebridean_Terrane.png#/media/File/Hebridean_Terrane
The Moine Thrust Belt forms the western margin of the Caledonian orogen (see dashed line in Figure 2) (Kocks et al. 2014).  It separates the Hebridean Terrane to the northwest from the Northern Highlands Terrane to the southeast (Wikipedia).  Moine rocks of the Morar group form its top. (Kocks et al. 2014).  Large slabs of Lewisian gneisses lying on top of a conglomerate base mostly characterize these.  Both layers are separated by an unconformity (Wikipedia).  They are formed of unmigmatized psammites with subordinate pelitic horizons (Kocks et al. 2014).  At its most, the width of the thrust belt is 10 km and it is over 190 km long (Wikipedia).  The Highlands of Scotland are full of rolling hills and rugged terraced mountains with steep sides.  Unknown to most people, the mountains close to the Moine Thrust are the vestiges of a much higher reaching mountain belt.  They are formed of complicated layers often characterized by a hard crystalline rock cap at the summit on top of softer sedimentary layers.  We can often find a valley predominantly composed of limestone that goes up and forms sandstone terranes topped by a quartzite cap (Wikipedia).

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Figure 3: Stratigraphy of the Moine Thrust Belt, types of rocks present (Butler 2002)
Many rock types can be found in Northern Scotland.  The basement is made of Lewisian granitic gneiss, a Precambrian metamorphic rock dating from the mid-early Proterozoic to the Archean (3.0-1.7 Ga ago) (Butler 2004).  The Torridonian and Moine Supergroup sediments were deposited on the previously named rock (Butler 2004).  They both date from the late Proterozoic (Butler 2004).  Some Cambro-ordovician rocks are also present because they formed a cover on the foreland basin.  Because their layers were highly differentiated and they possessed a layer-cake nature before the deformation, they can be used to observe the deformation, which was bestowed upon them by the Moine Thrust Belt (Butler 2004). 

We know that the Moine Thrust Belt dates back to the Caledonian orogeny, from the end of the Silurian period to the beginning of the Devonian.  Additional precisions can be brought from the U-Pb dating synkinematic unusual igneous intrusions in Southern Assynt (Kocks et al. 2014).  Indeed, the Borrolan complex dates back to 435-425 MA and there is evidence that places the Moine Thrust Belt active at the time of intrusion (Butler 2002).  We can also say that the main displacement occurred from 435-430 MA and that there was only slight movement in early Devonian (Kocks et al. 2014)
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PhotoFigure 4: Duplex
The underlying structures forming the Moine Thrust Belt have not yet been positively identified.  Some theories are able to explain most of what can be observed at the surface.  One such structure is a duplex (Watkins et al. 2014).  A duplex is formed of 2 low dipping thrust faults: the floor thrust deep in the crust and the roof thrust close to the surface.  They are linked by an array of steeper thrust faults called imbricate faults (see Figure 4) (Butler 1982).  Each imbricate fault travels upward in the stratigraphic layers toward the direction of displacement (Butler 2004).  In the Pipe rock formation, the Cambrian quartzites create shortening on the scale of 10's of kilometers by forming duplexes from 1 cm to 10's of meters large (Butler 2000).  However, there are no more imbricate faults south of Assynt until the Torridon area where they return, strongly fracturing Torridonian and Cambrian strata (Butler 2000).  Another aspect that still confuses geologist is that the roof thrust seems to both predate and postdate the imbricate faults (Butler 2004). Evidence pointing toward a roof thrust coming before that array of faults is when the aforementioned thrust is folded by underlying fault culmination (Butler 2004).  However, we can also find proof of the opposite when the roof thrust truncates the imbricate faults (Butler 2004).  This creates a real conundrum because we can find both type of deformation in close physical locations, like at the Glencoul Thrust (Butler 2004)

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Figure 5: Mylonites Image credit: By Woudloper (Own work) [Public domain], via Wikimedia Commons
Mylonites are present everywhere in the Moine Thrust Belt and they can reach 100 meters of thickness in some areas.  They are formed on either side of the thrust by intense shearing and streaking out.  The grains themselves are streaked out and aligned like needles in the direction of sheer (Butler 2002).
The Moine Thrust Belt's movement is constant throughout its three fold systems and all of its active life (Johnson 1965). The trend of the three fold systems is also the same as the Moine Thrust Belt (Johnson 1965).  The fault structure moves west-northwest and it continuously folds and thrusts the slices of foreland units under its power (Butler 2004).  It also crystallizes new minerals during transport, which are simultaneously suffering from vertical flattening (Johnson 1965).  Knowing the original thickness, we can calculate the original length of an outcrop and determine that it shrunk from more than 50 km long to only a few km (Butler 2002).  It was established that structurally higher units were situated to the east.  A mylonitic texture and crystal plastic deformation microstructures are typical of such units (Butler 2002).  To the west, cataclastic fault rocks are more likely to be found (Butler 2002).   This leads to the conclusion that the time sequence at play here is that early, hot, deep and ductile shearing with crystalline plasticity was brought to higher cataclastic faults with brittle faulting and fracture processes (Butler 2002) (Butler 2000). 

It has not yet been determined if the slip on the roof, imbricate and floor thrusts happens simultaneously or not.  It is known that the resulting movement appears to be continuous but a cycle of alternations between roof, imbricate and floor thrusts would also create the effect of a simultaneous movement (Butler 2004).

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Figure 6: Cross-section of the Moine Thrust at Loch Eridoll (Butler 2002)
One of the most interesting parts of the Moine Thrust Belt is situated at Loch Eriboll.  As well as being easily accessible, Loch Eriboll presents a lot of exposed outcrops that reveal key information about the Thrust belt.  We can clearly see the individual thrust and the intermittent flats and ramps that compose the Moine Thrust as well as sheets of Lewisian gneiss and small-scale imbrications of Cambrian stratigraphy (Butler 2000).  Many of these structures can be seen in the Pipe Rock (mostly quartz), which contains markers, trace fossils, for layer-parallel shortening and shear strain.  At Loch Eriboll, many geological layers can be found.  The structurally highest is the Moine Thrust Sheet, which is made of mylonites originating from Moine metasediments, the Lewisian basement and greatly deformed Lewisian slices. Next come mylonites of Lewisian gneiss origin combined to Cambrian quartzites (Butler 2000).  A part of the Lewisian basement was not deformed by the penetrative Caledonian strain.  Thrust sheets comprised of such basement rocks follow the mylonites.  Finally, we can found different imbricated Cambrian sediments at the bottom of the structure (Butler 2000).
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Figure 7: Detailed geological map of the Scottish Highlands By Mikenorton (Own work) [CC BY-SA 3.0 (http://creativecommons.org/licenses/by-sa/3.0) or GFDL (http://www.gnu.org/copyleft/fdl.html)], via Wikimedia Commons
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Figure 8: Detailed geological map of the Scottish Highlands superimposed over a map of Scotland
On the geological map of the Moine Thrust zone (Figures 7 and 8), we can see all the major geological features present in this region. A line punctuated by small triangles represents the thrust belt itself.  A dashed line represents other faults.  The different colors indicate what type of rocks can be found at the surface.  The principal rocks found in this part of Scotland are form the Morar group (dark brown-green). However, in some areas, erosion exposed some older and normally hidden rocks, like the Lewisian basement in dark purple.
References:
Butler, R.W.H., 2004, The Nature of Roof Thrusts in the Moine Thrust Belt, NW Scotland: Implications for the Structural Evolution of          Thrust Belts: Journal of the Geological Society, London, Vol. 5, pp. 849-859.
Butler, R.W.H., 1982, The Terminology of Structures in Thrust Belts: Journal of Structural Geology, Great Britain, Vol. 4, No. 3, pp. 239-245.
Butler, R.W.H., 2000. "The Moine Thrust Belt". Leeds University. Retrieved 2015-03-21
Butler, R.W.H., 2002. "Assynt's Geology". Leeds University. Retrieved 2015-03-21

Christie, J.M., 1965, Moine Thrust: A Reply: The Journal of Geology, Chicago, Vol. 73, No. 4, pp. 677-681.

Johnson, Michael, 1965, The Moine Thrust: A Discussion: The Journal of Geology, Chicago, Vol. 73, No. 4, pp. 672-676.
Kocks, H and 3 others, 2014,
Contrasting magma emplacement mechanisms within the Rogart igneous complex, NW Scotland, record the switch from regional contraction to strike-slip during the Caledonian orogeny: Geological Magazine, Cambridge, Vol. 151, No.5, pp. 899–915.

Various authors, 2007, Moine Thrust Belt: Wikipedia encyclopedia.
Various authors, 2003, Moine Supergroup: Wikipedia encyclopedia.
Watkins, Hannah and 2 others, 2014,
Identifying multiple detachment horizons and an evolving thrust history through cross-section restoration and appraisal in the Moine Thrust Belt, NW Scotland: Journal of structural geology, Aberdeen, Vol. 66, pp. 1-10.

Photo
Old Man of Storr, Skye By Wojsyl, June 2004, Wikicommons
If you want to know more about the geology of the Scottish Highlands, check out this video!
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The hudson valley fold thrust belt

3/29/2015

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The Hudson Valley fold belt is a west-verging fold thrust belt located in Upstate New York. This feature has been heavily studied by local geology students, as road cuts along Route 23 near the town of Catskill give a clear cross section of the entire fold belt. It is bounded by the Catskill mountains to the west and the Hudson river to the east. The belt itself is rather narrow, being on average less than 4 kilometers wide, and is often described in literature as a miniature valley and ridge province. It is difficult to define the westernmost limit of this structure, as west directed displacement can be found a few kilometers away from the westernmost fold in the form of cleavage duplexes. There is some deformed strata the same age as the belt east of the river, which suggests the belt was once wider than its present dimensions. It extends for roughly 80 kilometers between the cities of Kingston to the south and Albany to the north, where it meets the Mohawk River valley.
https://www.google.ca/maps/@42.2662968,-73.8730662,77860m/data=!3m1!1e3?hl=en
Figure 1. Google map of the region containing the Hudson Valley fold belt, which lies between the cities of Albany and Kingston.
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Figure 2: Structures associated with the Hudson Valley fold belt in New Paltz, New York.
http://www.newpaltz.edu/geology/nysga.html

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Figure 3: Sedimentary layers of the Hudson Valley fold belt (Marshak, 1986).

The stratigraphic units found in the fold belt represent sediment deposited by turbidity currents on the continental margin of Laurentia, which would later become North America. The lowest exposed unit is a flysch from the middle Ordovician, which was deformed into tight folds with east dipping axial planes before the younger units of the formation were deposited. This creates what is referred to as the Taconic unconformity, which formed as a result of the Taconic orogeny 440 million years ago. The next two groups are from the lower Devonian and are followed by middle Devonian limestone. Distinguishing rock units of the Helderberg group which follow the Taconic unconformity are the Manlius formation, a laminated micrite deposited in a tidal flat, the Coeymans formation, a lime grainstone from a beach environment, the Kalkberg and New Scotland formations, both lime wakestones, and the Becraft formation, which is also a lime grainstone. Following the Helderberg group is the Tristates group, with both groups originating from a shallow sea that advanced and retreated repeatedly during the lower Devonian.The youngest layers exhibiting deformation are the Bakoven shale and the Mount Marian formation. Based on the coloration of conodont fossils contained in the rocks they appear to have been exposed to a maximum temperature of 200 to 240°C, though it is not known if this occurred during or after the deformation. Most of these rock units are carbonates, with the only significant non-carbonate being the Esopus shale. The largest stratigraphic throw of the Hudson Valley belt is near Kingston, where the Esopus formation was thrusted over the Onondaga limestone.


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Figure 4: The Taconic angular unconformity.
http://hudsonvalleygeologist.blogspot.ca/2012/05/day-6-hudson-valley-fold-thrust-belt.html

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Figure 5: Geological map of the region northwest of Catskill, New York along Route 23 that gives a clear west to east transect of the feature. (Marshak, 1989).

Three categories of faults are found in the belt: bedding parallel faults, cross strata faults, and strike-slip and normal faults. Bedding parallel faults are exactly what their name implies: their slip surfaces are parallel to the bedding of both the hanging wall and the footwall strata. No breccia or gouge is present, so these faults must have moved by crack seal extension instead of sliding. Instead, calcite fibers and spar often appear on these fault surfaces. The cross strata faults are also what their name suggests. These faults cut across the bedding planes and displace stratigraphic markers, and are also associated with calcite fibers. Many of these faults form ramp structures typical of thin-skinned deformation. It is thought that many of these faults formed in the later stages of deformation, because they seem to follow the folds that formed early on. The normal faults are represented on the map above as dashed lines and are oblique to the other belts of the fold belt. Their age and mode of formation is not known. On all faults, the hanging wall rocks moved westward relative to the footwall rocks.

There are two scales of folds in the Hudson Valley fold belt: megascopic and mesoscopic. There are ten main megascopic folds in this formation, with amplitudes between 50 and 120 meters and wavelengths of 200 to 800 meters. The synclines of these folds are wider and more symmetrical than the anticlines, and the northwestern limbs are either steep or overturned. The hinges of this series of folds are not always parallel. These folds were formed by the movement of rock over fault bends, regional flexure, and the formation of ramps. The mesoscopic folds (represented on the map) are far smaller, with amplitudes and wavelengths ranging from 1 centimeter to 10 meters. The exact type of fold appears to depend on the rock unit in which they are found, forming chevron folds in the Kalkberg formation and crenulations in the Esopus shale.

North of Kingston, the structures trend north/south to N10°E, while south of the town they change to N30°E. Because of the changes in their structural trend, structures southwest of Kingston are not considered to be part of the belt. This is an example of an orocline, a secondary bend where the curve is caused by the reorientation of preexisting structures. In this case, the older Hudson Valley fold belt structures were reoriented by the Appalachian fold thrust belt to the south.
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Figure 6: Thrust fault duplex along the Hudson Valley fold belt exposed in a quarry. Curved horses can be seen in the photo. The floor thrust is known as the Rondout detachment.
http://web.cortland.edu/gleasong/fdcamp.html

The Hudson Valley fold thrust belt is a good example of thin-skinned deformation, which occurs at a convergent margin where thrust faults appear only in surface rock layers and not in the deeper basement rocks as they do in thick skinned deformation. The deformation history of this feature is believed to be as follows: layer parallel shortening happened before or concurrent with the initial folding and thrusting of the rocks. Ramps began to form through the more competent layers, while detachments formed in the weaker ones. While this was occurring, non-layer parallel shortening occurred as bending and interlayer slip. As the thrusting continued, the rocks were exposed to both pure and simple shear strain. Finally, frictional coupling caused the faults to lock, and instead the strain caused bulk shortening of the rocks. Overall, the strain in this feature expressed itself through faulting, folding, and bedding parallel slip.  
Shortening in the Hudson Valley fold belt occurred above two major detachment faults: the Austin Glen detachment and the Rondout detachment. The Austin Glen detachment is 500 meters below the surface and is not exposed anywhere along the fold belt. The Rondout detachment is stratigraphically higher, and in places where it is exposed it shows west verging mesoscopic folding. It crops out at or right above the post Taconic unconformity, and forms the floor thrust of a duplex. Horses stacked in duplexes are associated with the cross-strata faults, and occur in a variety of sizes.

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Figure 7. Three possible relationships between the Rondout detachment (white) and the Austin Glen detachment (grey). (Marshak, 1986).

In model A, internal shortening occurred in the Austin Glen formation, which lead to the folding of the overlying Rondout detachment. Here, faults do not extend below the Rondout detachment. Model B shows the Rondout detachment as a roof thrust and the Austin Glen detachment as a floor thrust of a duplex system. In model C, ramp faults of the system run all the way through both detachments. In this case, the Rondout detachment is not the basal detachment. 
Video: explanation of the Acadian orogeny. https://www.youtube.com/watch?v=zMtuXPJnhOI


Video explaining the Alleghanian orogeny. https://www.youtube.com/watch?v=fJZy_BCKrIU
Fold belts can appear in a variety of tectonic settings, so not many conclusions can be drawn about the environment of formation. The westward vergence of the HVB could relate it to the westward movement of part of New England relative to the rest of North America. Several theories exist as to how and when this region deformed. Its location between the Acadian foreland basin and the New England Acadian orogeny suggests that it may have formed in the middle Devonian as part of the Acadian orogeny. This mountain building event is associated with the creation of the Laurussian supercontinent and occurred over the Middle to Late Devonian, 380 to 350 million years ago. The Avalon microcontinent traveled along an east-dipping subduction zone and collided with what would later become North America at an oblique angle, forming a mountain chain that stretched from southern Virginia to Newfoundland. Another theory is that it formed as part of the Alleghanian orogeny 320 to 250 million years ago due to its continuity with structures in the central Appalachian mountains. In this orogeny, northwest Africa (at that time part of the Gondwanaland supercontinent) collided with eastern North America and closed the ocean between them, forming Pangaea. By this time, the mountains formed in the Acadian orogeny had been significantly weathered down. In this case movement would have been due either the presence of a transform system that existed on the eastern margin of North America at the time, or the collision between Africa and North America. 

Works Cited:

Burmeister, Kurtis, Marshak, Steven. 2006. Along-strike changes in fold-thrust belt architecture: Examples from the Hudson Valley, New York. Geological Society of America: Field Guide 8.
http://www.friendsofwilliamslake.org/pdfs/burmeister.pdf

Fichter, Lynn S. "The Devonian Acadian Orogeny And Catskill Clastic Wedge." The Geological Evolution of Virginia and the Mid Atlantic Region. James Madison University, 13 Sept. 2000. Web. 28 Mar. 2015.

Fichter, Lynn S. "The Late Paleozoic Alleghanian Orogeny." The Geological Evolution of Virginia and the Mid Atlantic Region. James Madison University, 13 Sept. 2000. Web. 28 Mar. 2015.

Harris, John, Van der Pluijm, Ben. 1997. "Relative timing of calcite twinning strain and fold-thrust belt development; Hudson Valley fold-thrust belt, New York, U.S.A." Journal of Structural Geology, 20 (1): 21-31.

http://www.sciencedirect.com/science/article/pii/S019181419700093X#

Marshak, Steven, Engelder, Terry. 1984. "Development of cleavage in limestone of a fold-thrust belt in eastern New York." Journal of Structural Geology, 7: 345-359

http://www.sciencedirect.com/science/article/pii/0191814185900409

Marshak, Steven. 1986. "Structure and tectonics of the Hudson Valley fold-thrust belt, eastern New York State." Geological Society of America Bulletin, 354-368.
http://gsabulletin.gsapubs.org/content/97/3/354.abstract

Marshak, Steven, Tabor, John. 1989. "Structure of the Kingston orocline in the Appalachian fold-thrust belt, New York." Geological Society of America Bulletin, 683-703

http://gsabulletin.gsapubs.org/content/101/5/683.short

Majerczyk, Chris. 2011. Geology of the Roberts Hill Area in the Hudson Valley Fold-Thrust Belt, Greene County, Eastern New York. Submitted Thesis.
https://www.ideals.illinois.edu/bitstream/handle/2142/29626/majerczyk_chris.pdf?sequence=1
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The Seattle fault zone

3/23/2015

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1. General Description of the Feature
The Seattle Fault Zone is located in the Seattle metropolitan area in the state of Washington in the United States of America. The approximate location is shown in the embedded Google Map below. The zone is shown within the two dashed lines in Figure 1.1. and is composed of four south dipping thrust faults (Johnson et al., 1994). It is composed of one major fault of a length reaching 45 km - shown in Figure 2.3. - and additional smaller ones. A thrust fault is a type of contractional fault with a low dip angle where the hanging wall relative to the footwall is going up (Fossen, 2010). In this particular case, the Seattle Fault has a high dip angle close to the surface and a low dip value as the fault goes deeper. It falls into the thrust fault cathegory of contractional faults. The faults in the zone trend east-west and are believed to have caused a major earthquake around 900 A.D. which had a magnitude over 7 on the Richter scale (Calvert et al., 2001). Because of this event and the fact that the faults have been active in the past 30 years - according to recent studies - the zone is believed to represent a major seismic hazard (Johnson et al., 1994). The fault zone has been heavily studied in the last 40 years as it goes directly under the City of Seattle - which is the biggest city in the State of Washington  (Information Please, 2007). The exact model describing the relation and motion between the various features is still debated among geologists today (Nelson 2014).
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Figure 1.1. Map of the region which shows an approximation of where the Seattle Fault Zone is located. The zone is within the two dashed lines in the upper part of the image. Adapted from Calvert et al., 2001.
The Seattle Fault Zone is an area that is experiencing contraction, where there is a shortening on the North-South axis (Johnson et al., 1994). The dextral faults on the north and south side of the zone would be the cause this shortening. The area is acting as a restraining transfer zone between the dextral faults (Johnson et al., 1994). The dextral faults would be caused by the subduction of the Juan de Fuca plate and a clockwise rotation of the Cascade arc (more details in section 3). The presence of the faults in the metropolitan area was first mentioned in a 1965 study of the region (Calvert et al., 2001) and is believed to have its origins in late Eocene (40 Ma ago) (Johnson et al., 1994).
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Figure 1.2. A geological map of the region with the Seattle Basin circled in the middle. The legend of on the lower left corner identifies the various rock types present in the region. The major fault is identified with two red arrows. Adapted from Johnson et al., 1994.
The region is composed of a thick layer of Quaternary deposits shown in Figure 1.2. A high resolution geological map of the region is available at this location - a link is provided as there is too much details to be embedded on the web site.
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Figure 1.3. A stratigraphic chart of four different locations in the Seattle Fault Zone. The age and rock unit thickness are labelled on the diagram. Adapted from Johnson et al., 1994.
Figure 1.3 shows the rock units along with their age present at four different locations in the Seattle Fault Zone. The oldest unit shown on the diagram is the Crescent Formation which is made of marine basalt and sedimentary rocks (Johnson et al., 1994). The shaded areas on the chart are sections where the strata was not preserved. On top of the Crescent Formation, layers of sandstone, siltstone and shale are present up until the Narizian strata. The Refugian to Zemorrian strata mark the boundary between marine sedimentary rocks to nonmarine sedimentary rocks (Johnson at al., 1994). The Oligocene portion of the Blakely Formation contains layers of sandstone, siltstone, shale, and conglomerate from a deep-marine environment, and the same types of rocks are found up to the late Miocene era - with the exception that there is no presence of shale (Johnson at al., 1994).
2. Detailed Description of the Structures
The Seattle Fault Zone is defined by 4 south-dipping faults crossing the metropolitan area (Johnson et al., 1994). The faults are shown in Figure 2.1. where they are labeled from 1 to 4. There is one major faults - labelled 3 in Figure 2.1. - and additional smaller faults. The motion of the hanging wall relative to the footwall of the faults is going upward as they are thrust faults. They have dips varying from 65 to 70 degrees near the surface (Johnson et al., 1994). The faults are believed to have dips around 20 degrees at greater depth (Calvert et al., 2001).
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Figure 2.1. A cross-section of one of the interpretations of the Seattle Fault Zone where the four south-dipping faults are visible. The north side of the zone is on the right side of the graph, and the south side of the zone is on the left side of the graph. The numbers on the Y-axis represent the roundtrip time in seconds of the signal they sent to determine the composition of the ground. Adapted from Johnson et al., 1994.
Figure 2.2. shows the four faults along with their projection underground. The different layers are also visible on the image. The faults are listric, and the master ramp is along the northernmost fault - labelled 3 (Jonhson et al., 1994).
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Figure 2.2. The four south dipping thrust faults of the Seattle Fault Zone along with their projection underground. Adapted from Jonhson et al., 1994.
The Seattle Fault Zone is subject to many interpretations, but the four main ones are shown in Figure 2.2. below. The diagrams A, C, and D mainly show the area close to the master fault - and the surface - whereas diagram B includes the potential relation between the Seattle Fault and the Tacoma Fault (Nelson et al. 2014).
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Figure 2.2. The four main models that describe the Seattle Fault along with the various other faults formed by the motion on the fault's master ramp. Adapted from Nelson et al., 2014.
The Seattle Fault Zone contains one major fault that is shown in Figure 2.3. below. The dips and displacement measured along the fault are shown in Table 2.1. The Seattle Fault and Tacoma Fault have a particular relationship as they would be connected and would be forming the boundaries of the Seattle uplift. The Tacoma Fault is composed of multiple faults and folds that are north dipping and east-west striking (Nelson, 2014). If the suggested model where the Tacoma and Seattle faults are connected, and form the Seattle uplift boundaries is right, they would do so at a distance of at least 10 km underground (Nelson 2014).
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Table 2.1. The measurements taken along the Seattle Fault shown in Figure 2.3. above. Adapted from Venturato et al., 2007.
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Figure 2.3. A map showing the various faults in the region. The major fault of the zone is identified as the "Seattle Fault". Adapted from Venturato et al., 2007.
3. Discussion of the Deformation and Motion
The Seattle Fault Zone is experiencing stress from various sources: the subduction of the Juan de Fuca Plate, and the rotation of the Cascade arc. A subduction zone is when two edges of a tectonic plate contact and one goes underneath the other. In this case, the Juan de Fuca Plate goes underneath the Washington state - the North American plate - at a rate of approximately 40 mm/year (Parsons et al., 1999). This movement is creating a clockwise rotation of the Cascade arc (shown in Figure 3.1. on the right) (Parsons et al., 1999). These motions create multiple dextral faults around the Seattle Fault Zone (North and South), which generates restraining bend in the zone. The restraining bend then creates a positive flower structure, which is composed of multiple reverse faults (Fossen, 2010). An example of a positive flower structure is shown in Figure 3.3. A model in Figure 3.2. shows the kinetics creating the shortening in the Seattle Fault Zone.
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Figure 3.1. The overall tectonic setting of the north-west of the United States of America. Adapted from Parsons et al., 1999.
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Figure 3.2. A model showing two strike-slip faults creating a restraining bend which illustrates what could be causing the Seattle Fault. Adapted from Fossen, 2010.
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Figure 3.3. A positive flower structure created within a restraining zone. This is one interpretation of the Seattle uplift. The Seattle Fault (south dipping) connects with the Tacoma Fault (north dipping) and uplifts - in a positive flower like structure - what is in between. Adapted from Fossen, 2010.
These motions results in a current slip-rate of the Seattle Fault equal to 0.5 mm/year, which is believed to be twice the average value it has been in the past 40 millions years (Calvert et al., 2001). The tectonic configuration of the Seattle Fault Zone is shown in Figure 3.2. below. The motion is believed to have started in the late Eocene period and continues to this day.
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Figure 3.4. The tectonic setting of the Seattle Fault Zone where the Juan de Fuca Plate is going under the basement rock of Washington (the North American plate). Additional forces coming from the south are affecting the zone. The Seattle's location is identified with a red arrow on the image. Adapted from Parson et al., 1999.
4. Graphics and Media
2 Minute Geology video about the Seattle Fault. It discuss the basic tectonic activities along with the tsunami believed to have ravaged the Seattle area in 900 A.D.
Short video explaining the tectonic configuration around the Juan de Fuca plate and its movement. It is relevant as it explains the motion of the Juan de Fuca plate relative to the North American Plate (where the Cascade arc resides) - along with the cause of the motion.
Interesting video on the below showing a computer simulation where the tectonic activity produced an earthquake which generated a tsunami. The tsunami spreads on the shores of the metropolitan area. According the to the video description, the simulated earthquake is of magnitude 7.3 on the Richter scale. This is simply to show that Seattle would suffer major damages if such an earthquake were to happen.
5. References
  1. Johnson, S., Potter, C., & Armentrout, J. (1994). Origin and evolution of the Seattle fault and Seattle basin, Washington. In Geology (1st ed., Vol. 22, pp. 71-74). Denver, Colorado: Geological Society of America.
  2. Calvert, A., & Fisher, M. (2001). Imaging the Seattle Fault Zone with high-resolution seismic tomography. In Geophysical Research Letters (12th ed., Vol. 28, pp. 2337-2340). Washington, D.C: American Geophysical Union.
  3. Nelson, A., Personius, S., Sherrod, B., Kelsey, H., Johnson, S., Bradley, L., & Wells, R. (2014). Diverse rupture modes for surface-deforming upper plate earthquakes in the southern Puget Lowland of Washington State. In Geosphere (4th ed., Vol. 10, p. 769–796). Denver, Colorado: Geological Society of America.
  4. Parsons, T., Wells, R., Fisher, M., Flueh, E., & Brink, U. (1999). Three-dimensional velocity structure of Siletzia and other accreted terranes in the Cascadia forearc of Washington. In Journal of Geophysical Research (B8 ed., Vol. 104, pp. 18015-18039). Washington, D.C: American Geophysical Union.
  5. Venturato, A., Arcas, D., Titov, V., Mofjeld, H., Chamberlin, C., & Gonzalez, F. (2007). Tacoma, Washington, tsunami hazard mapping project: Modeling tsunami inundation from Tacoma and Seattle fault earthquakes. In Contribution (Pacific Marine Environmental Laboratory (U.S.)) (Vol. 2984). Seattle, Washington: National Oceanic and Atmospheric Administration.
  6. Fossen, H. (2010). Structural Geology (1st ed.). Cambridge University Press.
  7. Information Please. (2007). Information Please page on Profiles of the 50 Largest Cities of the United States, Section: Seattle, Washington. Retrieved March 29, 2015, from the World Wide Web: http://www.infoplease.com/ipa/A0108609.html
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Linville Falls Fault - Amelia LIndsay-Kaufman

3/22/2015

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The Linville Falls Fault is a thrust fault located near the border between North Carolina and Tennessee, along the towns Linville Falls, Banner Elk, and Boone, in the Blue Ridge Province of the Appalachian Mountains.


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Figure 1) Approximate location of the Linville Falls Fault in North Carolina, USA

A thrust fault is a fault which has pushed rocks of lower stratigraphic position (usually meaning older rocks) up and over higher (or younger) rocks. Seeing older rock layers on top of younger rock layers is usually a giveaway that a thrust fault has been involved. The Linville Falls Fault is a top-to-northwest thrust fault. Here one billion year old granite of the Grenville Province has been pushed over 700 million year old metamorphosed sandstone. The fault was created during the formation of the Appalachian Mountains about 300 million years ago in the Alleghenian Orogeny when Gondwana collided with Euramerica. (7)

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Figure 2) A map of the geological features surrounding and including the Linville Falls Fault. All of the faults formed in the Alleghenian orogeny except the Burnsville Fault. The four thrust sheets of the Blue Ridge thrust complex are shown. (4)

During the formation of the thrust fault, collisional forces pushed a rock layer called the Blue Ridge thrust complex over 100km to its current location covering Grandfather Mountain. This rock layer forms the hanging wall of the Linville Falls fault. It is composed of alkali feldspar granite overlain by shear zone mylonites, and cranberry gneiss (also part of the Grenville Province). (8) The footwall of the fault consists of autochronous quartzite, which is part of the Grandfather Mountain formation, and quartz-sericite mylonite which was created through shearing. (4) At least 50 km of movement has occurred along the fault. (1) On one edge of the fault there is a thick ductile top-to-northwest shear zone called the Linville Falls Shear Zone, approximately one km wide near Banner Elk and consisting of mylonitic and ultramylonitic rocks with zones that have been cataclastically deformed. (4)

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Figure 3) Relative location of the Linville Falls shear zone (4)

The Linville Falls Fault forms the border of the Grandfather Mountain Window. (figure 2) A window is formed when a layer of rock erodes away in one location to expose a patch of different rocks underneath. (figure 4)  Here, after the Blue Ridge Thrust complex was pushed over Grandfather Mountain by the fault, the peaks of the formation eroded away and in one place a gap eroded all the way through the layer, uncovering the younger rocks underneath. The other faults, such as the Brevard Fault, were formed in the same orogeny (Alleghenian) as the one that created the Linville Falls Fault.  The nearby Linville Falls Gorge arose when the Linville River eroded the softer quartzite out from under the granite and caused the falls to collapse. (7)
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Figure 4) A basic diagram of a window formation
The Blue Ridge Thrust complex, in the hanging wall of the Linville Falls Fault and overlying the Grandfather Mountain Window, consists of stacks of crystalline thrust sheets which can be distinguished from one another by their metamorphic history. They are (in order from structurally lowest to highest) the Pardee Point thrust sheet, the Beech Mountain thrust sheet, the Pumpkin Patch thrust sheet, and the Spruce Pine thrust sheet. (4) A zone of metamorphosed rocks near the sole of the thrust sheet displays many small isoclinal folds with northwest-trending axial planes parallel to foliation in the thrust sheet. (3)

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Figure 5) A geological map showing the orientations and elevations of features surrounding the Linville Falls Fault (4)
The faults in the Blue Ridge Mountains were formed in the Alleghenian Orogeny 320 to 260 million years ago during the late Carboniferous period. The Alleghenian Orogeny is one of the six orogenies making up the formation of the Appalachian Mountains. The mountain building occurred as Pangaea was coalescing, when Africa (at the time part of the supercontinent Gondwanaland) collided with the supercontinent Euramerica. The impact compressed rocks between the two landmasses and forced them up into a mountain chain which at the time was located in the center of the supercontinent. When Pangaea broke up millions of years later, the mountain range split in two. Today we have the Appalachians in North America and the Atlas Mountains in North Africa. The buckling from the collision also created a series of sedimentary folds, perpendicular to the force, bounded by thrust faults which shortened the land by as much as 320 km. The Linville Falls Thrust Fault formed due to the compressional forces in this orogeny. (8) The folds in the Blue Ridge Thrust Sheet are thought to have formed from flattening and passive rotation of earlier folds which originally formed perpendicular to the direction of movement. (3)

Figure 6) An animation showing the break up of Pangaea and the migration of the continents to their current positions. At the beginning of the video it can be seen where North America was connected to Africa. This is where the mountains were originally.
Sources:

(1)    CAROLINA GEOLOGICAL SOCIETY 1997 FIELD TRIP AND ANNUAL MEETING ROAD LOG AND STOP DESCRIPTIONS 
http://carolinageologicalsociety.org/CGS/1990s_files/gb%201997.pdf#page=27

(2)    Significance of lineation and minor folds near major thrust faults in the southern Appalachians and the British and Norwegian Caledonides   Bruce Bryant and John C. Reed Jr.
http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=4629596&fileId=S0016756800058805

(3)    PALEOZOIC STRUCTURAL EVOLUTION OF THE BLUE RIDGE THRUST COMPLEX, WESTERN NORTH CAROLINA  Kevin G. Stewart, Mark G. Adams , and Charles H.Trupe
http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=4629596&fileId=S0016756800058805

(4)    STRUCTURAL RELATIONSHIPS IN THE LINVILLE FALLS SHEAR ZONE, BLUE RIDGE THRUST COMPLEX, NORTHWESTERN NORTH CAROLINA   Charles H. Trupe
http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=4629596&fileId=S0016756800058805

(5)    Geology of the Linville Falls Quadrangle North Carolina  GEOLOGICAL SURVEY BULLETIN 1161-B
http://pubs.usgs.gov/bul/1161b/report.pdf

(6)    Linville Gorge 
http://www.unc.edu/courses/2008spring/geog/006d/001/Class_Readings/Class%20%2313%20-%20April%2021%20(WNC%20-%20Team%20Presentations%20&%20Papers)/Linville%20Gorge_Class%20Paper.pdf

(7)    USGS Valley and Ridge Province
http://web.archive.org/web/20110722154205/http://3dparks.wr.usgs.gov/nyc/valleyandridge/valleyandridge.htm

(8)    CONDITIONS AND TIMING OF METAMORPHISM IN THE BLUE RIDGE THRUST COMPLEX, NORTHWESTERN NORTH CAROLINA AND EASTERN TENNESSEE  Mark G. Adams and Charles H. Trupe http://journals.cambridge.org/action/displayAbstract?fromPage=online&aid=4629596&fileId=S0016756800058805

(9) Image of window: http://upload.wikimedia.org/wikipedia/commons/b/b1/Thrust_system_en.jpg

(10) Video of Pangaea: https://www.youtube.com/watch?v=WaUk94AdXPA
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Aleutian Trench - lucas darroch

3/22/2015

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The Aleutian Trench is part of a subducting zone in the Pacific Ocean connecting Alaska to Kamchatka. The trench is formed where the Pacific plate is being subducted under the North American plate. The boundary is visibly defined on map, see the embedded link below.  
Modelling the large-scale motion of the lithosphere is a fundamental topic in structural geology, plate tectonics is the current thinking to this end. The theory states that the lithosphere is broken up into tectonic plates, the boundary between plates is well defined in an appropriate geological framework [1]. We will investigate the Aleutian Trench, a convergent boundary between the Pacific plate and the North American plate. A map of the earth's major (and some minor) plates is presented in Figure 1. 

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Figure 1: Tectonic plates of the Earth (Wikipedia Online)
In a recent journal, Zahirovic, Sabin, et al analyse a plate motion model and extract topologies in 1 Myr intervals. The model uses paleomagnetic data sampled over the last 200 Myr, present day plate velocities from eight plates, and post-Pangea plate tectonic reconstructions [2]. The embedded link below models the break-up of Pangea using data from Zahirovic, Sabin, et al; the video is hosted by AAAS via Earthbyte.org. The model projects the Pacific plate forming around 190 Myr ago and the Aleutian Trench forming around 40 Myr ago.
Earth's tectonic plates skitter about
When a tectonic plate is subducted, stress builds in the boundary between the two plates. At some critical value of stress, the plates slip against each other and energy is relieved. This large scale displacement (and the mechanical waves which follow) is an earthquake. Figure 2 presents earthquake foci recorded over a ten year period around the Aleutian Islands, the foci are recorded on both plates along the boundary. 
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Figure 2: Larger earthquakes occurring in the Aleutian Islands from 1957-1966. The open circles represent foci underneath the islands, the black triangles represent foci under the trench (Stauder 1968)
During 1980 and 1981, the U.S. Geological Survey completed a reconnaissance along the Aleutian Arc and the Aleutian Trench [3]. The locations investigated are presented in Figure 3, for our investigation we examine the (analysed) section L9-12.
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Figure 3: Map view of the Aleutian Island arc, seismic data is acquired for profiles across the black lines (McCARTHY J.I.L.L. Scholl 1985)
McCARTHY et al. analyse the time and depth section from the seismic survey and build a structural model, these are presented in Figure 4. Relative to the two plates, the contact is a thrust fault over the oceanic crust. An accretion layer of off-scraped sediment forms as the oceanic crust subducts [4]. The faults formed on the oceanic crust suggest that a principle stress is in the direction of general vergence (Anderson fault theory). This is to say that the oceanic crust is extending and active. A master thrust fault runs along the plate boundary, a duplex fault system is forming on the hanging wall. The Pacific and North American plate form a convergent boundary.
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Figure 4: L9-12 seismic survey, data was acquired and processed by the U.S Geological Survey (McCARTHY J.I.L.L. Scholl 1985)
The seismic data was processed at the U.S. Geological Survey marine seismic processing facility in Menlo Parktime [4]. To generate such data sets, elastic waves are introduced to the crust. Bedded surfaces act well as reflectors, sensors are run along the cross section.  Fault planes act as pseudo reflectors, in the depth section they can be seen cutting across the general vergence of the bedding. The time section assumes mild lateral velocity variations and so cannot resolve the faults.
The Aleutian Trench is an active convergent boundary between the Pacific and North American plates. The subduction is continuous, but the internal forces are high in the lithosphere so the displacement is expressed in discrete intervals. The North American plate is thrusting towards the Pacific plate, and the Pacific plate is extending towards the North American plate. This is apparent from the normal faults along the extending oceanic crust and the duplex system on the hanging wall. Relative to each other, the North American and Pacific plates form a contractional margin.

References

  1. Wikipedia contributors. "Plate tectonics." Wikipedia, The Free Encyclopedia. Wikipedia, The Free Encyclopedia, 22 Mar. 2015. Web. 22 Mar. 2015 http://en.wikipedia.org/wiki/Plate_tectonics.
  2. Zahirovic, Sabin, et al. "Tectonic speed limits from plate kinematic reconstructions." Earth and Planetary Science Letters 418 (2015): 40-52.
  3. Stauder, William. "Tensional character of earthquake foci beneath the Aleutian Trench with relation to sea‐floor spreading." Journal of Geophysical Research73.24 (1968): 7693-7701
  4. McCARTHY, J. I. L. L., and David W. Scholl. "Mechanisms of subduction accretion along the central Aleutian Trench." Geological Society of America Bulletin 96.6 (1985): 691-701


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