Paleoproterozoic Tectonic Evolution of the Trans-North China Orogen: Toward a Comprehensive Model
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Dairy Syncline Mine Project Record of Decision
United States Department of Agriculture U.S. Forest Service Caribou-Targhee National Forest Final Record of Decision Dairy Syncline Mine Project, Caribou County, Idaho April 2020 Forest Service – Caribou-Targhee National Forest – April 2020 In accordance with Federal civil rights law and U.S. Department of Agriculture (USDA) civil rights regulations and policies, the USDA, its Agencies, offices, and employees, and institutions participating in or administering USDA programs are prohibited from discriminating based on race, color, national origin, religion, sex, gender identity (including gender expression), sexual orientation, disability, age, marital status, family/parental status, income derived from a public assistance program, political beliefs, or reprisal or retaliation for prior civil rights activity, in any program or activity conducted or funded by USDA (not all bases apply to all programs). Remedies and complaint filing deadlines vary by program or incident. Persons with disabilities who require alternative means of communication for program information (e.g., Braille, large print, audiotape, American Sign Language, etc.) should contact the responsible Agency or USDA’s TARGET Center at (202) 720-2600 (voice and TTY) or contact USDA through the Federal Relay Service at (800) 877-8339. Additionally, program information may be made available in languages other than English. To file a program discrimination complaint, complete the USDA Program Discrimination Complaint Form, AD- 3027, found online at http://www.ascr.usda.gov/complaint_filing_cust.html and at any USDA office or write a letter addressed to USDA and provide in the letter all of the information requested in the form. To request a copy of the complaint form, call (866) 632-9992. -
Tectonic Features of the Precambrian Belt Basin and Their Influence on Post-Belt Structures
... Tectonic Features of the .., Precambrian Belt Basin and Their Influence on Post-Belt Structures GEOLOGICAL SURVEY PROFESSIONAL PAPER 866 · Tectonic Features of the · Precambrian Belt Basin and Their Influence on Post-Belt Structures By JACK E. HARRISON, ALLAN B. GRIGGS, and JOHN D. WELLS GEOLOGICAL SURVEY PROFESSIONAL PAPER X66 U N IT ED STATES G 0 V ERN M EN T P R I NT I N G 0 F F I C E, \VAS H I N G T 0 N 19 7 4 UNITED STATES DEPARTMENT OF THE INTERIOR ROGERS C. B. MORTON, Secretary GEOLOGICAL SURVEY V. E. McKelvey, Director Library of Congress catalog-card No. 74-600111 ) For sale by the Superintendent of Documents, U.S. GO\·ernment Printing Office 'Vashington, D.C. 20402 - Price 65 cents (paper cO\·er) Stock Number 2401-02554 CONTENTS Page Page Abstract................................................. 1 Phanerozoic events-Continued Introduction . 1 Late Mesozoic through early Tertiary-Continued Genesis and filling of the Belt basin . 1 Idaho batholith ................................. 7 Is the Belt basin an aulacogen? . 5 Boulder batholith ............................... 8 Precambrian Z events . 5 Northern Montana disturbed belt ................. 8 Phanerozoic events . 5 Tectonics along the Lewis and Clark line .............. 9 Paleozoic through early Mesozoic . 6 Late Cenozoic block faults ........................... 13 Late Mesozoic through early Tertiary . 6 Conclusions ............................................. 13 Kootenay arc and mobile belt . 6 References cited ......................................... 14 ILLUSTRATIONS Page FIGURES 1-4. Maps: 1. Principal basins of sedimentation along the U.S.-Canadian Cordillera during Precambrian Y time (1,600-800 m.y. ago) ............................................................................................... 2 2. Principal tectonic elements of the Belt basin reentrant as inferred from the sedimentation record ............ -
GEOLOGIC FRAMEWORK, TECTONIC EVOLUTION, and DISPLACEMENT HISTORY of the ALEXANDER TERRANE Georgee
TECTONICS, VOL. 6, NO. 2, PAGES 151-173, APRIL 1987 GEOLOGIC FRAMEWORK, TECTONIC EVOLUTION, AND DISPLACEMENT HISTORY OF THE ALEXANDER TERRANE GeorgeE. Gehrels1 and Jason B. Saleeby Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena Abstract. The Alexander terrane consists of Devonian (Klakas orogeny). The second phase is upper Proterozoic(?)-Cambrian through marked by Middle Devonian through Lower Middle(?) Jurassic rocks that underlie much of Permian strata which accumulated in southeastern (SE) Alaska and parts of eastern tectonically stable marine environments. Alaska, western British Columbia, and Devonian and Lower Permian volcanic rocks and southwestern Yukon Territory. A variety of upper Pennsylvanian-Lower Permian syenitic to geologic, paleomagnetic, and paleontologic dioritic intrusive bodies occur locally but do not evidence indicates that these rocks have been appear to represent major magmatic systems. displaced considerable distances from their The third phase is marked by Triassic volcanic sites of origin and were not accreted to western and sedimentary rocks which are interpreted to North America until Late Cretaceous-early have formed in a rift environment. Previous Tertiary time. Our geologic and U-Pb syntheses of the displacement history of the geochronologic studies in southern SE Alaska terrane emphasized apparent similarities with and the work of others to the north indicate rocks in the Sierra-Klamath region and that the terrane evolved through three distinct suggested that the Alexander terrane evolved in tectonic phases. During the initial phase, from proximity to the California continental margin late Proterozoic(?)-Cambrian through Early during Paleozoic time. Our studies indicate, Devonian time, the terrane probably evolved however, that the geologic record of the along a convergent plate margin. -
Tectonostratigraphic Terrane Analysis of New Brunswick L
Document generated on 09/30/2021 12:46 p.m. Atlantic Geology Tectonostratigraphic terrane analysis of New Brunswick L. R. Fyffe and A. Fricker Volume 23, Number 3, December 1987 Article abstract the URI: https://id.erudit.org/iderudit/ageo23_3art01 The contents of a computerized lexicon database are displayed in the form of a range chart that demonstrate the spartial and temporal relationships of See table of contents lithtostratigraphic units to tectonostratigraphic terrans of New Brunsiwck. The chart provides a reference basis from which to derive the accretionary history of these terrance. Publisher(s) The tectonostratigraphlc zonation of Hew Brunswick ia based upon the Atlantic Geoscience Society uniqueness of the pre-Taconlan stratigraphy within each fault-bounded terrane. From northwest to southeast, the following terranes and cover sequences are recognized: Matapedia Cover. Blmtree Terrane, Mlramichi ISSN Terrane, Frederlcton Cover, St. Croix Terrane, Hascarene Terrane, and 0843-5561 (print) Avalonian Terrane. 1718-7885 (digital) Overstepping of the Matapedia Cover Sequence indicates that the Elmtree and Mlramichi terranes were docked with the North American craton by the Late Explore this journal Ordovician to Early Silurian. The presence of a similar early Paleozoic stratigraphy, tectonic style and major Silurian unconformity in the St. Croix Terrane suggests that it had become docked to the Mlramichi Terrane prior to this subduction-related Taconian event. Cite this article Detritus and a similar fauna in the cover rocks of the St. Croix Terrane provide Fyffe, L. R. & Fricker, A. (1987). Tectonostratigraphic terrane analysis of New evidence that it was docked to the Hascarene Terrane by the Late Silurian. -
The Timing and Location of Major Ore Deposits in an Evolving Orogen" the Geodynamic Context
Downloaded from http://sp.lyellcollection.org/ by guest on September 26, 2021 The timing and location of major ore deposits in an evolving orogen" the geodynamic context DEREK J. BLUNDELL Department of Geology, Royal Holloway, University of London, Egham, Surrey TW20 OEX, UK (e-mail: d. blundell@gl, rhul.ac, uk) Abstract: Although it is possible to identify the potential controls on mineralization, the problem remains to identify the critical factors. Very large mineral deposits are rare occurrences in the geological record and are likely to have resulted from the combination of an unusual set of circumstances. When attempting to understand the mineralization processes that occurred to form a major ore deposit in the geological past, especially the reasons why the deposit formed at a particular time and location within an evolving orogenic system, it is instructive to look at mineralization in modern, active subduction complexes. There it is possible to measure and quantify the rates at which both tectonic and mineralizing processes occur. In a complex subduction system, regions of extension develop. For example, subduction hinge retreat is a process that creates extension and generates heat from the upwelling of hot asthenosphere ahead of the retreating slab, producing partial melting, magmatism and associated mineraliza- tion. Seismic tomography not only images mantle as it is now, but subduction slab anomalies can be interpreted in terms of the past histo12¢ of subduction. This can be used to test tectonic plate reconstructions. Tectonic and magmatic events occur rapidly and are of short duration so that many are ephemeral and will not be preserved. -
Post-Collisional Mantle Delamination in the Dinarides Implied
www.nature.com/scientificreports OPEN Post‑collisional mantle delamination in the Dinarides implied from staircases of Oligo‑Miocene uplifted marine terraces Philipp Balling1*, Christoph Grützner1, Bruno Tomljenović2, Wim Spakman3 & Kamil Ustaszewski1 The Dinarides fold‑thrust belt on the Balkan Peninsula resulted from convergence between the Adriatic and Eurasian plates since Mid‑Jurassic times. Under the Dinarides, S‑wave receiver functions, P‑wave tomographic models, and shear‑wave splitting data show anomalously thin lithosphere overlying a short down‑fexed slab geometry. This geometry suggests a delamination of Adriatic lithosphere. Here, we link the evolution of this continental convergence system to hitherto unreported sets of extensively uplifted Oligocene–Miocene (28–17 Ma) marine terraces preserved at elevations of up to 600 m along the Dinaric coastal range. River incision on either side of the Mediterranean‑Black Sea drainage divide is comparable to the amounts of terrace uplift. The preservation of the uplifted terraces implies that the most External Dinarides did not experience substantial deformation other than surface uplift in the Neogene. These observations and the contemporaneous emplacement of igneous rocks (33–22 Ma) in the internal Dinarides suggest that the Oligo‑Miocene orogen‑wide uplift was driven by post‑break‑of delamination of the Adriatic lithospheric mantle, this was followed by isostatic readjustment of the remaining crust. Our study details how lithospheric delamination exerts an important control on crustal deformation and that its crustal signature and geomorphic imprint can be preserved for millions of years. Te infuence of deep-seated processes on deformation patterns and rates in collisional orogens is unequivo- cally accepted, yet challenging to quantify. -
Arc Magmas Sourced from Mélange Diapirs in Subduction Zones Horst R
Arc magmas sourced from mélange diapirs in subduction zones Horst R. Marschall a;b;∗ John C. Schumacher c aDepartment of Geology & Geophysics, Woods Hole Oceanographic Institution, Woods Hole, MA 02543, USA bDepartment of Earth and Planetary Sciences, American Museum of Natural History, New York, New York, USA cDepartment of Earth Sciences, University of Bristol, Wills Memorial Building, Queen’s Road, Bristol BS8 1RJ, UK Abstract At subduction zones, crustal material is recycled back into the mantle. A certain proportion, however, is returned to the overriding plate via magmatism. The magmas show a characteristic range of compositions that have been explained by three-component mixing in their source regions: hydrous fluids derived from subducted altered oceanic crust and components derived from the thin sedimentary veneer are added to the depleted peridotite in the mantle beneath the volcanoes. However, currently no uniformly accepted model exists for the physical mechanism that mixes the three components and transports them from the slab to the magma source. Here we present an integrated physico-chemical model of subduction zones that emerges from a review of the combined findings of petrology, modelling, geophysics, and geochemistry: Intensely mixed metamorphic rock formations, so-called mélanges, form along the slab-mantle interface and comprise the characteristic trace-element patterns of subduction-zone magmatic rocks. We consider mélange formation the physical mixing process that is responsible for the geochemical three-component pattern of the magmas. Blobs of low-density mélange material, so-called diapirs, rise buoyantly from the surface of the subducting slab and provide a means of transport for well-mixed materials into the mantle beneath the volcanoes, where they produce melt. -
Regional Subduction Zone Models
Subduction III Regional subduction zone modeling Thorsten W Becker University of Southern California Short course at Universita di Roma TRE April 18 – 20, 2011 Reading • King, S. (Elsevier Treatise, 2007) • Billen, M. (Ann Rev, 2009) • Becker & Faccenna (2009) Jarrard (1986) King (2007) Pre - Plate Tectonics Internal deformation of subducted lithosphere. - Isacks & Molnar, 1969 Deep planar fault zone - Elsasser, 1968 Lithospheric thrusting - Plafker, 1965 Mantle Convection Mega-shear to 700 km Crustal-scale thrusting - Holmes, 1944 - Benioff, 1954 - Hess, 1962 1940s 1950s 1960s • Subduction into the mantle was one of the last pieces of the plate tectonics puzzle. Slide courtesy of M. Billen Plate Tectonics: in the SZ Steady-state slab dip: * Newtonian - Stevenson & Turner,1977 * Non-Newtonian Linking slab temp. to - Tovish et al., 1978 mineralogy & petrology * Layered mantle visc. - Peacock, 1990 - Yokokura, 1981 Dynamic topography Corner-flow model. from corner-flow Slab thermal structure - McKenzie, 1969 - Sleep, 1975 -Toksov, 1971; 1973 1960s 1970s 1980s 1970s 1990s • Early analytic models capture major processes. – Force balance on slab. – Slab thermal structure. Slide courtesy of M. Billen Kinematic Slab - Dynamic Wedge 3D, anisotropy implication - Kneller & van Keken, 2007 Non-linear viscosity - Kneller et al., 2007 Compositional & phase: density & viscosity - Gerya & Yuen, 2003 Low viscosity wedge - Honda & Saito, 2003 Wedge/back arc flow Convection in the wedge - Bodri & Bodri, 1978 - Ida, 1983 Temperature-dep. visc. - Toksov & Hsui, 1978 - Honda, 1985 - Eberle, 2001 1970s 1980s 1990s 2000s • Slab & mantle wedge thermal/min./pet. structure. • Fluid transport • Seismic anisotropy. Slide courtesy of M. Billen Observations Plate kinematics & characteristics - Mueller et al., 1997 - Lallemand et al., 2005 Seismic anisotropy - Russo & Silver, 1994 - Fischer et al., 1998 - Long & Silver, 2008 Plate kinematics & characteristics - Jarrard, 1986 Seismic tomography - e.g., van der Hilst, 1997 Arc curvature, slab dip, subduction velocity. -
Western Carpathians, Poland)
Geological Quarterly, 2006, 50 (1): 169–194 Late Jurassic-Miocene evolution of the Outer Carpathian fold-and-thrust belt and its foredeep basin (Western Carpathians, Poland) Nestor OSZCZYPKO Oszczypko N. (2006) — Late Jurassic-Miocene evolution of the Outer Carpathian fold-and-thrust belt and its foredeep basin (Western Carpathians, Poland). Geol. Quart., 50 (1): 169–194. Warszawa. The Outer Carpathian Basin domain developed in its initial stage as a Jurassic-Early Cretaceous rifted passive margin that faced the east- ern parts of the oceanic Alpine Tethys. Following closure of this oceanic basin during the Late Cretaceous and collision of the Inner Western Carpathian orogenic wedge with the Outer Carpathian passive margin at the Cretaceous-Paleocene transition, the Outer Carpathian Basin domain was transformed into a foreland basin that was progressively scooped out by nappes and thrust sheets. In the pre- and syn-orogenic evolution of the Outer Carpathian basins the following prominent periods can be distinguished: (1) Middle Juras- sic-Early Cretaceous syn-rift opening of basins followed by Early Cretaceous post-rift thermal subsidence, (2) latest Creta- ceous-Paleocene syn-collisional inversion, (3) Late Paleocene to Middle Eocene flexural subsidence and (4) Late Eocene-Early Miocene synorogenic closure of the basins. In the Outer Carpathian domain driving forces of tectonic subsidence were syn-rift and thermal post-rift processes, as well as tectonic loads related to the emplacement of nappes and slab-pull. Similar to other orogenic belts, folding of the Outer Carpathians commenced in their internal parts and progressed in time towards the continental foreland. This process was initi- ated at the end of the Paleocene at the Pieniny Klippen Belt/Magura Basin boundary and was completed during early Burdigalian in the northern part of the Krosno Flysch Basin. -
A Geodynamic Model of Subduction Evolution and Slab Detachment to Explain Australian Plate Acceleration and Deceleration During the Latest Cretaceous–Early Cenozoic
A geodynamic model of subduction evolution and slab detachment to explain Australian plate acceleration and deceleration during the latest Cretaceous–early Cenozoic W.P. Schellart1,* 1DEPARTMENT OF EARTH SCIENCES, VRIJE UNIVERSITEIT AMSTERDAM, DE BOELELAAN 1085, 1081 HV AMSTERDAM, NETHERLANDS ABSTRACT During the latest Cretaceous–early Cenozoic, the northern margin of the Australian plate was characterized by a large (4000 km wide) north- to northeast-dipping subduction zone (New Guinea–Pocklington subduction zone) consuming a marginal basin. Geological and geophysical data imply that the subduction zone was active ca. 71–50 Ma, and suggest that it was responsible for plate acceleration from ~1.0 to ~7.3 cm/yr ca. 64–59 Ma, and plate deceleration from ~7.3 to ~0.3 cm/yr at 52–49 Ma. This paper presents a numerical model of buoyancy-driven subduction to test if the rates of Australian plate acceleration and deceleration can be ascribed to the progressive evolution of a subducting slab. The geodynamic model reproduces the first-order plate velocity evolution of the Australian plate, with a transient ~5 m.y. period of acceleration from 2 to 8 cm/yr during upper mantle slab lengthening, an ~5 m.y. period of rapid plate motion (~5–8 cm/yr), and a short, 3.9 m.y., period of plate deceleration, starting with a 2 cm/yr velocity drop during 3.1 m.y. of continental subduction and followed by ~0.8 m.y. of rapid deceleration (4 cm/yr velocity drop) during slab detachment. The geodynamic model demonstrates that plate velocity increases or decreases of ~4–6 cm/yr can occur over a period lasting <1 m.y. -
Isostasy, Dynamic Topography, and the Elevation of the Apennines of Italy ∗ Claudio Faccenna A, , Thorsten W
Earth and Planetary Science Letters 407 (2014) 163–174 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl Isostasy, dynamic topography, and the elevation of the Apennines of Italy ∗ Claudio Faccenna a, , Thorsten W. Becker b, Meghan S. Miller b, Enrico Serpelloni c, Sean D. Willett d a Laboratory Experimental Tectonics, Università Roma TRE, Roma, Italy b Department of Earth Sciences, University of Southern California, Los Angeles, CA, USA c Istituto Nazionale Geofisica e Vulcanologia, Centro Nazionale Terremoti, Bologna, Italy d Department of Earth Sciences, Swiss Federal Institute of Technology, Zurich, Switzerland a r t i c l e i n f o a b s t r a c t Article history: The elevation of an orogenic belt is commonly related to crustal/lithosphere thickening. Here, we discuss Received 19 March 2014 the Apennines as an example to show that topography at a plate margin may be controlled not only by Received in revised form 28 August 2014 isostatic adjustment but also by dynamic, mantle-driven processes. Using recent structural constraints for Accepted 14 September 2014 the crust and mantle we find that the expected crustal isostatic component explains only a fraction of Available online xxxx the topography of the belt, indicating positive residual topography in the central Apennines and negative Editor: Y. Ricard residual topography in the northern Apennines and Calabria. The trend of the residual topography Keywords: matches the mantle flow induced dynamic topography estimated from regional tomography models. Apennines We infer that a large fraction of the Apennines topography is related to mantle dynamics, producing elevation relative upwellings in the central Apennines and downwellings in the northern Apennines and Calabria subduction where subduction is still ongoing. -
RESEARCH Topographic Expressions of Lunar Graben
RESEARCH Topographic expressions of lunar graben Melanie B. Callihan* and Christian Klimczak STRUCTURAL GEOLOGY AND GEOMECHANICS GROUP, DEPARTMENT OF GEOLOGY, UNIVERSITY OF GEORGIA, ATHENS, GEORGIA 30602, USA ABSTRACT Graben, defined as landforms produced by normal faulting, have long been recognized on the Moon, but their map patterns, as well as topographic expressions, have not been studied systematically. The topography across graben and its along-strike variations reveal details about the growth of the normal faults forming the graben. Individual normal faults grow in length by the propagation of fault tips during slip events, which can also enlarge the displacement along the fault plane. Displacement and length accumulate and grow larger over time with more slip events, fault interaction, and linkage. We measured fault lengths and vertical offsets and then calculated the displacement for lunar graben using data from the camera and laser altimeter onboard the Lunar Reconnaissance Orbiter. Our study systematically investigated 14 graben systems across the lunar surface. Graben lengths were found to range from ~43 to 453 km, and displacements ranged from ~127 to 1115 m. These displacements were plotted against graben fault length to produce slip distributions, which revealed growth patterns involving mechanical interaction and fault linkage. Displacement-to-length scaling was used to further study the evolu- tion of graben-bounding normal faults. We observed a sublinear growth pattern for lunar graben-bounding normal faults, consistent with growth of faults via segment linkage, where different stages of linkage are present on the lunar surface. Lunar graben-bounding faults show higher scaling ratios than previously estimated, likely due to variations in host-rock properties and mechanical stratigraphy.