scholarly journals Transport Pressure Mark Mechanisms in the Late Cretaceous-Early Eocene Conglomerates, Northwestern Wyoming

Author(s):  
James Steidtmann

In spite of rather intensive investigation into the origin of the Harebell (Late Cretaceous), Pinyon (Paleocene) and Pass Peak (Early Eocene) conglomerates in Jackson Hole and adjacent areas certain critical questions remain unanswered. The great thickness, coarseness and lateral extent imply an ancient source of considerable size and relief relatively near to present day Jackson Hole. Evidence for such a source is, however, equivocal and previous workers do not agree on its location. An even more perplexing question concerns the mechanisms by which such a huge volume of cobbles and boulders was transported from the source, wherever it was, to its depositional site. Such a system implies the existence of ancient alluvial fans on a scale unknown in modern environments.

2012 ◽  
Vol 4 (1) ◽  
Author(s):  
Márton Veress ◽  
István Németh ◽  
Roland Schläffer

AbstractThe effects of the intensive rainfall episodes in the years 2009 and 2010 in the Kőszeg Mountains were investigated. Channel profiles were constructed at various times during these periods, which were used to describe the channel changes. We measured the length of the incised and filled sections on multiple occasions. We could establish the degree and the direction of the changes using this data. The sediment veneer that developed in the area of Kőszeg town was mapped and its conditions of development were examined. The erosion and accumulation landforms developed during these years were classified and described. These forms are the following: rills, gullies, alluvial fans and sediment veneer. We distinguished and characterised those which had previously formed, but they were changed or increased (the channels). We established the conditions under which the sediment veneer can develop, furthermore those conditions which can increase the chance of the formation of this landform. These conditions are the following: the high density of roads in the catchment areas of valleys leading to settlements, the great thickness of superficial deposit, and the steep slope of the surface of the catchment area. We created theoretical classification of the morphological environment where the development of sediment veneer may happen and identified settlements with structures which promote or prevent the development of the sediment veneer. We determined the probability of the development of the sediment veneer at some settlements in Kőszeg, and suggestions have been given to decrease the chance of the development of this sediment veneer.


Geosciences ◽  
2019 ◽  
Vol 9 (9) ◽  
pp. 381 ◽  
Author(s):  
Claudio Robustelli Test ◽  
Andrea Festa ◽  
Elena Zanella ◽  
Giulia Codegone ◽  
Emanuele Scaramuzzo

The strong morphological similitude of the block-in-matrix fabric of chaotic rock units (mélanges and broken formations) makes problematic the recognition of their primary forming-processes. We present results of the comparison between magnetic fabric and mesoscale structural investigations of non-metamorphic tectonic, sedimentary, and polygenetic mélanges in the exhumed Late Cretaceous to early Eocene Ligurian accretionary complex and overlying wedge-top basin succession in the Northern Apennines (northwest Italy). Our findings show that the magnetic fabric reveals diagnostic configurations of principal anisotropy of magnetic susceptibility (AMS) axes orientation that are well comparable with the mesoscale block-in-matrix fabric of mélanges formed by different processes. Broken formations and tectonic mélanges show prolate and neutral-to-oblate ellipsoids, respectively, with magnetic fabric elements being consistent with those of the mesoscale anisotropic “structurally ordered” block-in-matrix fabric. Sedimentary mélanges show an oblate ellipsoid with a clear sedimentary magnetic fabric related to downslope gravitational emplacement. Polygenetic mélanges show the occurrence of a cumulative depositional and tectonic magnetic fabric. The comparison of field and laboratory investigations validate the analysis of magnetic features as a diagnostic tool suitable to analytically distinguish the contribution of different mélange forming-processes and their mutual superposition, and to better understand the geodynamic evolution of subduction-accretion complexes.


2000 ◽  
Vol 37 (9) ◽  
pp. 1259-1273 ◽  
Author(s):  
M E McMechan

Walker Creek fault zone (WCFZ), well exposed in the western Rocky Mountains of central British Columbia near 54°, comprises a 2 km wide zone of variably deformed Neoproterozoic and Cambrian strata in fault-bounded slivers and lozenges. Extensional shear bands, subhorizontal extension lineations, slickensides, mesoscopic shear bands, and other minor structures developed within and immediately adjacent to the fault zone consistently indicate right-lateral displacement. Offset stratigraphic changes in correlative Neoproterozoic strata indicate at least 60 km of right-lateral displacement across the zone. WCFZ is the southern continuation of the Northern Rocky Mountain Trench (NRMT) fault zone. It shows a through going, moderate displacement, strike-slip fault system structurally links the NRMT and the north-central part of the Southern Rocky Mountain Trench. Strike-slip motion on the WCFZ occurred in the Late Cretaceous to Early Eocene at the same time as northeast-directed shortening in the fold-and-thrust belt. Thus, oblique convergence in the eastern part of the south-central Canadian Cordillera was apparently resolved into parallel northwest-striking zones of strike-slip and thrust faulting during the Late Cretaceous to Early Eocene. The change in the net Late Cretaceous to Early Eocene displacement direction for rocks in the Rocky Mountain trenches from north (56-54°N) to northeast (52-49°N) suggests that the disappearance of strike-slip displacement and increase in fold-and-thrust belt shortening in the eastern Cordillera between 56° and 49°N is largely the result of a north-south change in relative plate motion or strain partitioning across the Cordillera, rather than the southward transformation of right-lateral strike-slip displacement on the Tintina - NRMT fault system into compressional deformation.


1989 ◽  
Vol 26 (2) ◽  
pp. 231-243 ◽  
Author(s):  
Larry S. Lane ◽  
Edward D. Ghent ◽  
Mavis Z. Stout ◽  
Richard L. Brown

Microstructural and petrofabric analyses of mylonites from the Monashee Décollement demonstrate that the hanging wall was displaced eastward over the footwall. Microstructural kinematic indicators include shear-band foliation, asymmetric strain shadows, and S–C fabrics. Quartz c axes locally exhibit asymmetric fabrics that are consistent with the microstructural evidence for sense of shear. The kinematic evidence is reliable because multiple criteria coexist within individual specimens.Metamorphic assemblages from footwall Monashee Complex pelites at the Revelstoke damsite indicate that the peak metamorphic assemblage was sillimanite–K-feldspar–biotite–almandine–quartz ± plagioclase. Biotite–garnet geothermometry and garnet–plagioclase–sillimanite–quartz geobarometry set broad constraints on metamorphic temperatures but closer constraints on pressures, near 650 °C and 630 MPa.Comparison of these data with Late Cretaceous hornblende cooling ages from the same locality indicates that the metamorphism is at least as old as Late Cretaceous. Complex microstructures relating to repeated mylonitization and annealing render difficult the correlation of metamorphic conditions with mylonitic fabrics. Early mylonitic textures predate the metamorphic equilibration and thus are pre-Late Cretaceous in age. Postmetamorphic mylonites are well preserved, but their ages are poorly constrained. The present interpretation favours a Late Cretaceous to Paleocene age relating to compressional tectonics. However, an Early Eocene age relating to extensional shearing cannot be excluded.


2004 ◽  
Vol 23 (2) ◽  
pp. 208-256 ◽  
Author(s):  
David Branagan

The term "Desert Sandstone" was featured on geological maps and in the literature of Australian geology for more than eighty years from 1872. The name was suggested by Richard Daintree (1832-1878) (1868) for what were later described as "a promiscuous lot of sediments that form a dissected tableland in some of the drier portions of the continent" (Howchin, 1918). The name became current, particularly in Queensland, but there were many problems in mapping the unit, which was at first thought to be of Tertiary age, but then became largely accepted as Late Cretaceous.While some geologists thought the unit was of marine origin, others believed it was aeolian, even partly made of volcanic dust, but most geologists thought it was largely lacustrine. In many areas the rock appeared to be highly silicified, and opinions differed as to the source of silicification—a former covering of basalt, or siliceous hot waters from below?Complications arose when Glossopteris, regarded as a Late Palaeozoic fossil, was found in the "Desert Sandstone," and arguments arose about the possibility of this plant having persisted in Australia until the late Mesozoic.The stratigraphic/palaeontological problems were eventually sorted out by detailed mapping, which showed that there were in fact a number of sandstones of similar appearance but quite different ages. It took longer to realise that the apparent uniformity of sedimentary rocks of different ages was largely the result of weathering, which produced the silicified "duricrust" in many parts of inland Australia.The "Desert Sandstone" played an important part in the unravelling of three important lines of earth history in Australia (and there were even repercussions abroad). These were: (a) sedimentation during the Mesozoic and Cainozoic; (b) the clarification of the temporal range (and lateral extent) of the Glossopteris flora; and (c) the weathering processes that produced some of the characteristic scenery of inland Australia.


2017 ◽  
Vol 81 ◽  
pp. 1137-1157 ◽  
Author(s):  
Carlos M. González-León ◽  
Luigi Solari ◽  
Martín Valencia-Moreno ◽  
Mario A. Rascon Heimpel ◽  
Jesús Solé ◽  
...  

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