Orogeny Through Time: an Overview
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Tectonic Imbrication and Foredeep Development in the Penokean
Tectonic Imbrication and Foredeep Development in the Penokean Orogen, East-Central Minnesota An Interpretation Based on Regional Geophysics and the Results of Test-Drilling The Penokean Orogeny in Minnesota and Upper Michigan A Comparison of Structural Geology U.S. GEOLOGICAL SURVEY BULLETIN 1904-C, D AVAILABILITY OF BOOKS AND MAPS OF THE U.S. GEOLOGICAL SURVEY Instructions on ordering publications of the U.S. Geological Survey, along with prices of the last offerings, are given in the cur rent-year issues of the monthly catalog "New Publications of the U.S. Geological Survey." Prices of available U.S. Geological Sur vey publications released prior to the current year are listed in the most recent annual "Price and Availability List." Publications that are listed in various U.S. Geological Survey catalogs (see back inside cover) but not listed in the most recent annual "Price and Availability List" are no longer available. Prices of reports released to the open files are given in the listing "U.S. Geological Survey Open-File Reports," updated month ly, which is for sale in microfiche from the U.S. Geological Survey, Books and Open-File Reports Section, Federal Center, Box 25425, Denver, CO 80225. Reports released through the NTIS may be obtained by writing to the National Technical Information Service, U.S. Department of Commerce, Springfield, VA 22161; please include NTIS report number with inquiry. Order U.S. Geological Survey publications by mail or over the counter from the offices given below. BY MAIL OVER THE COUNTER Books Books Professional Papers, Bulletins, Water-Supply Papers, Techniques of Water-Resources Investigations, Circulars, publications of general in Books of the U.S. -
Strike and Dip Refer to the Orientation Or Attitude of a Geologic Feature. The
Name__________________________________ 89.325 – Geology for Engineers Faults, Folds, Outcrop Patterns and Geologic Maps I. Properties of Earth Materials When rocks are subjected to differential stress the resulting build-up in strain can cause deformation. Depending on the material properties the result can either be elastic deformation which can ultimately lead to the breaking of the rock material (faults) or ductile deformation which can lead to the development of folds. In this exercise we will look at the various types of deformation and how geologists use geologic maps to understand this deformation. II. Strike and Dip Strike and dip refer to the orientation or attitude of a geologic feature. The strike line of a bed, fault, or other planar feature, is a line representing the intersection of that feature with a horizontal plane. On a geologic map, this is represented with a short straight line segment oriented parallel to the strike line. Strike (or strike angle) can be given as either a quadrant compass bearing of the strike line (N25°E for example) or in terms of east or west of true north or south, a single three digit number representing the azimuth, where the lower number is usually given (where the example of N25°E would simply be 025), or the azimuth number followed by the degree sign (example of N25°E would be 025°). The dip gives the steepest angle of descent of a tilted bed or feature relative to a horizontal plane, and is given by the number (0°-90°) as well as a letter (N, S, E, W) with rough direction in which the bed is dipping. -
GE OS 1234-101 Historical Geology Lecture Syllabus Instructor
G E OS 1234-101 Historical Geology Lecture Syllabus Instructor: Dr. Jesse Carlucci ([email protected]), (940) 397-4448 Class: MWF, 10am -10:50am, BO 100 Office hours: Bolin Hall 131, MWF, 11am ± 2pm, Tuesday, noon - 2pm. You can arrange to meet with me at any time, by appointment. Textbook: Earth System History by Steven M. Stanley, 3rd edition. I will occasionally post articles and other readings on blackboard. I will also upload Power Point presentations to blackboard before each class, if possible. Course Objectives: Historical Geology provides the student with a comprehensive survey of the history of life, and major events in the physical development of Earth. Most importantly, this class addresses how processes like plate tectonics and climate interact with life, forming an integrated system. The first half of the class focuses on concepts, and the second on a chronologic overview of major biological and physical events in different geologic periods. L E C T UR E SC H E DU L E Aug 27-31: Overview of course; what is science? The Earth as a planet Stanley (pg. 244-247) Sep 5-7: Earth materials, rocks and minerals Stanley (pg. 13-17; 25-34) Sep 10-14: Rocks & minerals continued; plate tectonics. Stanley (pg. 3-12; 35-46; 128-141; 175-186) Sep 17-21: Geological time and dating of the rock record; chemical systems, the climate system through time. Quiz 1 (Sep 19; 5%). Stanley (pg. 187-194; 196-207; 215-223; 232-238) Sep 24-28: Sedimentary environments and life; paleoecology. Stanley (pg. 76-80; 84-96; 99-123) Oct 1-5: Biological evolution and the fossil record. -
Part 3: Normal Faults and Extensional Tectonics
12.113 Structural Geology Part 3: Normal faults and extensional tectonics Fall 2005 Contents 1 Reading assignment 1 2 Growth strata 1 3 Models of extensional faults 2 3.1 Listric faults . 2 3.2 Planar, rotating fault arrays . 2 3.3 Stratigraphic signature of normal faults and extension . 2 3.4 Core complexes . 6 4 Slides 7 1 Reading assignment Read Chapter 5. 2 Growth strata Although not particular to normal faults, relative uplift and subsidence on either side of a surface breaking fault leads to predictable patterns of erosion and sedi mentation. Sediments will fill the available space created by slip on a fault. Not only do the characteristic patterns of stratal thickening or thinning tell you about the 1 Figure 1: Model for a simple, planar fault style of faulting, but by dating the sediments, you can tell the age of the fault (since sediments were deposited during faulting) as well as the slip rates on the fault. 3 Models of extensional faults The simplest model of a normal fault is a planar fault that does not change its dip with depth. Such a fault does not accommodate much extension. (Figure 1) 3.1 Listric faults A listric fault is a fault which shallows with depth. Compared to a simple planar model, such a fault accommodates a considerably greater amount of extension for the same amount of slip. Characteristics of listric faults are that, in order to maintain geometric compatibility, beds in the hanging wall have to rotate and dip towards the fault. Commonly, listric faults involve a number of en echelon faults that sole into a lowangle master detachment. -
Copyright Notice
COPYRIGHT NOTICE The following document is subject to copyright agreements. The attached copy is provided for your personal use on the understanding that you will not distribute it and that you will not include it in other published documents. Dr Evert Hoek Evert Hoek Consulting Engineer Inc. 3034 Edgemont Boulevard P.O. Box 75516 North Vancouver, B.C. Canada V7R 4X1 Email: [email protected] Support Decision Criteria for Tunnels in Fault Zones Andreas Goricki, Nikos Rachaniotis, Evert Hoek, Paul Marinos, Stefanos Tsotsos and Wulf Schubert Proceedings of the 55th Geomechanics Colloquium, Salsberg Published in Felsbau, 24/5, 2006. Goricki et al. (2006) 22 Support decision criteria for tunnels in fault zones Support Decision Criteria for Tunnels in Fault Zones Abstract A procedure for the application of designed support measures for tunnelling in fault zones with squeezing potential is presented in this paper. Criteria for the support decision based on quantitative parameters are defined. These criteria provide an objective basis for the assignment of the designed support categories to the actual ground conditions. Besides the explanation of the criteria and the implementation into the general geomechanical design process an example from the Egnatia Odos project in Greece is given. The Metsovo tunnel is located in a geomechanical difficult area including fault zones and a major thrust zone with high overburden. Focusing on squeezing sections of this tunnel project the application of the support decision criteria is shown. Introduction Tunnelling in fault zones in general is associated with frequently changing ground and ground water conditions together with large and occasionally long lasting displacements. -
GEOLOGY What Can I Do with This Major?
GEOLOGY What can I do with this major? AREAS EMPLOYERS STRATEGIES Some employment areas follow. Many geolo- gists specialize at the graduate level. ENERGY (Oil, Coal, Gas, Other Energy Sources) Stratigraphy Petroleum industry including oil and gas explora- Geologists working in the area of energy use vari- Sedimentology tion, production, storage and waste disposal ous methods to determine where energy sources are Structural Geology facilities accumulated. They may pursue work tasks including Geophysics Coal industry including mining exploration, grade exploration, well site operations and mudlogging. Geochemistry assessment and waste disposal Seek knowledge in engineering to aid communication, Economic Geology Federal government agencies: as geologists often work closely with engineers. Geomorphology National Labs Coursework in geophysics is also advantageous Paleontology Department of Energy for this field. Fossil Energy Bureau of Land Management Gain experience with computer modeling and Global Hydrogeology Geologic Survey Positioning System (GPS). Both are used to State government locate deposits. Consulting firms Many geologists in this area of expertise work with oil Well services and drilling companies and gas and may work in the geographic areas Oil field machinery and supply companies where deposits are found including offshore sites and in overseas oil-producing countries. This industry is subject to fluctuations, so be prepared to work on a contract basis. Develop excellent writing skills to publish reports and to solicit grants from government, industry and private foundations. Obtain leadership experience through campus organi- zations and work experiences for project man- agement positions. (Geology, Page 2) AREAS EMPLOYERS STRATEGIES ENVIRONMENTAL GEOLOGY Sedimentology Federal government agencies: Geologists in this category may focus on studying, Hydrogeology National Labs protecting and reclaiming the environment. -
Tectonics of the Musandam Peninsula and Northern Oman Mountains: from Ophiolite Obduction to Continental Collision
GeoArabia, 2014, v. 19, no. 2, p. 135-174 Gulf PetroLink, Bahrain Tectonics of the Musandam Peninsula and northern Oman Mountains: From ophiolite obduction to continental collision Michael P. Searle, Alan G. Cherry, Mohammed Y. Ali and David J.W. Cooper ABSTRACT The tectonics of the Musandam Peninsula in northern Oman shows a transition between the Late Cretaceous ophiolite emplacement related tectonics recorded along the Oman Mountains and Dibba Zone to the SE and the Late Cenozoic continent-continent collision tectonics along the Zagros Mountains in Iran to the northwest. Three stages in the continental collision process have been recognized. Stage one involves the emplacement of the Semail Ophiolite from NE to SW onto the Mid-Permian–Mesozoic passive continental margin of Arabia. The Semail Ophiolite shows a lower ocean ridge axis suite of gabbros, tonalites, trondhjemites and lavas (Geotimes V1 unit) dated by U-Pb zircon between 96.4–95.4 Ma overlain by a post-ridge suite including island-arc related volcanics including boninites formed between 95.4–94.7 Ma (Lasail, V2 unit). The ophiolite obduction process began at 96 Ma with subduction of Triassic–Jurassic oceanic crust to depths of > 40 km to form the amphibolite/granulite facies metamorphic sole along an ENE- dipping subduction zone. U-Pb ages of partial melts in the sole amphibolites (95.6– 94.5 Ma) overlap precisely in age with the ophiolite crustal sequence, implying that subduction was occurring at the same time as the ophiolite was forming. The ophiolite, together with the underlying Haybi and Hawasina thrust sheets, were thrust southwest on top of the Permian–Mesozoic shelf carbonate sequence during the Late Cenomanian–Campanian. -
Plate Tectonics
Plate Tectonics Plate Tectonics is a unifying theory that states that the Earth is composed of lithospheric crustal plates that move slowly, change size, and interact with one another. This theory was amalgamated from a variety of studies that began in the early 20th century and culminated in the 1960s. Early Players: Richard Oldham (1858-1936): discovered P Wave Shadow Zones Inge Lehmann (1888-1993): discovered the S Wave Shadow Zone, including the fact that the outer core is liquid Eduard Suess (1831-1914): published internal structure of the Earth, utilizing some of Oldham’s data Andrija Mohorovicic (1857-1936): discovered the seismic discontinuity between the crust and the mantle Beno Gutenberg (1889-1960): found the CMB to be at 2900 km The Great Synthesizer: Alfred Wagener (1880-1930) Book: The Origin of Continents and Oceans (1915) Found six major pieces of evidence the continents move, hence his theory is known as Continental Drift. (Figures 19.2-1911) 1) The shape of the continents: they fit together 2) Paleontological Evidence: found matching fossils on several continents a) Glossopteris: found in rocks of the same age on South America, South Africa, Australia, India and Antarctica b) Lystrosaurus: found in rocks of the same age on Africa, India, also some in Asia and Antarctica c) Mesosaurus: found in rocks of the same age on South America, South Africa d) Cynognathus: found in rocks of the same age on South America, South Africa 3) Glacial Evidence: the glaciers appear to originate from the modern-day oceans (which is impossible) 4) Structure and Rock Type: geologic features end on one continent and reappear on the other (South America and Africa) 5) Paleoclimate Zones: like today, the old Earth had climate zones. -
Geotectonic Model of the Alpine Development of Lakavica Graben in the Eastern Part of the Vardar Zone in the Republic of Macedonia
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by UGD Academic Repository Geologica Macedonica, Vol. 27, No. 1, pp. 87–93 (2013) GEOME 2 ISSN 0352 – 1206 Manuscript received: May 17, 2013 UDC: 551.245.03(497.71/.73) Accepted: October 25, 2013 Original scientific paper GEOTECTONIC MODEL OF THE ALPINE DEVELOPMENT OF LAKAVICA GRABEN IN THE EASTERN PART OF THE VARDAR ZONE IN THE REPUBLIC OF MACEDONIA Goše Petrov, Violeta Stojanova, Gorgi Dimov Faculty of Natural and Technical Sciences, “Goce Delčev” University, P.O.Box 201, MK 2000 Štip, Republic of Macedonia [email protected]//[email protected] A b s t r a c t: Lakavica graben is located in the eastern subzone of the Vardar zone, which during the Alpine orogenesis was covered with very complex processes of tectogenesis. On the area of about 200 km2, in the Lakavica graben, are present geological units from the oldest geological periods (Precam- brian) to the youngest (Neogene and Quaternary). Tectonic structure, or rupture tectonic, is very intense developed and gives possibility for analysis of the geotectonic processes in the Alpine orogen phase. This paper presents the possible model for geotectonic processes in the Lakavica graben, according to which can be generalized geotectonic processes in the Vardar zone during the Alpine orogeny. Key words: Lakavica graben; geotectonic model; Alpine orogeny; Vardar zone INTRODUCTION Vardar zone as a tectonic unit, for the first niki Gulf (Greece), than bent eastward and crosses time, is separated and showed on the "Geological- the ophiolite zone Izmir–Ankara (Turkey). -
Weathering, Erosion, and Susceptibility to Weathering Henri Robert George Kenneth Hack
Weathering, erosion, and susceptibility to weathering Henri Robert George Kenneth Hack To cite this version: Henri Robert George Kenneth Hack. Weathering, erosion, and susceptibility to weathering. Kanji, Milton; He, Manchao; Ribeira e Sousa, Luis. Soft Rock Mechanics and Engineering, Springer Inter- national Publishing, pp.291-333, 2020, 9783030294779. 10.1007/978-3-030-29477-9. hal-03096505 HAL Id: hal-03096505 https://hal.archives-ouvertes.fr/hal-03096505 Submitted on 5 Jan 2021 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Published in: Hack, H.R.G.K., 2020. Weathering, erosion and susceptibility to weathering. 1 In: Kanji, M., He, M., Ribeira E Sousa, L. (Eds), Soft Rock Mechanics and Engineering, 1 ed, Ch. 11. Springer Nature Switzerland AG, Cham, Switzerland. ISBN: 9783030294779. DOI: 10.1007/978303029477-9_11. pp. 291-333. Weathering, erosion, and susceptibility to weathering H. Robert G.K. Hack Engineering Geology, ESA, Faculty of Geo-Information Science and Earth Observation (ITC), University of Twente Enschede, The Netherlands e-mail: [email protected] phone: +31624505442 Abstract: Soft grounds are often the result of weathering. Weathering is the chemical and physical change in time of ground under influence of atmosphere, hydrosphere, cryosphere, biosphere, and nuclear radiation (temperature, rain, circulating groundwater, vegetation, etc.). -
GLY5455 Introduction to Geophysics/Geodynamics Syllabus Fall 2015 Instructor: Mark Panning Location: Williamson 218 Time: Tuesday and Thursday, 1:55-3:10Pm
GLY5455 Introduction to Geophysics/Geodynamics Syllabus Fall 2015 Instructor: Mark Panning Location: Williamson 218 Time: Tuesday and Thursday, 1:55-3:10pm Contact Info Office: 229 Williamson Hall Phone: 392-2634 Email: [email protected] Office hours: Can be arranged at any time via email Textbook Turcotte & Schubert, Geodynamics, 3rd Edition (required) We will also be pulling material from the following books (not required) Physics of the Earth, Stacey and Davis (2008) The Magnetic Field of the Earth, Merrill, McElhinny, and McFadden (1996) Introduction to Seismology, Shearer (2006) Pre-reqs You will ideally have completed 1 year of calculus and a semester of physics. This class will deal with vector calculus… if this worries you, check out div grad curl and all that, by H.M. Schey (available for around $30 online). Grading 60% Homework 20% Midterm 20% Final Course topics (roughly 2-3 weeks per topic… but very flexible!) Topic Text Gravity Ch. 5 + other notes Heat Ch. 4 Magnetism Material from The Magnetic Field of the Earth Seismology Ch. 2, 3, and material from Introduction to Seismology Plate Tectonics & Mantle Geodynamics Ch. 1,6,7 Geophysical inverse theory (if time allows) Outside readings TBA Class notes Lecture notes will be distributed, sometimes before the material is covered in lecture, and sometimes after. Regardless, as always, such notes are meant to be supplementary to your own notes. I may cover things not in the distributed notes, and likewise may not cover everything in lecture that is included in the notes. Homework The first homework assignment will be assigned in week 2. -
Geodynamics and Rate of Volcanism on Massive Earth-Like Planets
The Astrophysical Journal, 700:1732–1749, 2009 August 1 doi:10.1088/0004-637X/700/2/1732 C 2009. The American Astronomical Society. All rights reserved. Printed in the U.S.A. GEODYNAMICS AND RATE OF VOLCANISM ON MASSIVE EARTH-LIKE PLANETS E. S. Kite1,3, M. Manga1,3, and E. Gaidos2 1 Department of Earth and Planetary Science, University of California at Berkeley, Berkeley, CA 94720, USA; [email protected] 2 Department of Geology and Geophysics, University of Hawaii at Manoa, Honolulu, HI 96822, USA Received 2008 September 12; accepted 2009 May 29; published 2009 July 16 ABSTRACT We provide estimates of volcanism versus time for planets with Earth-like composition and masses 0.25–25 M⊕, as a step toward predicting atmospheric mass on extrasolar rocky planets. Volcanism requires melting of the silicate mantle. We use a thermal evolution model, calibrated against Earth, in combination with standard melting models, to explore the dependence of convection-driven decompression mantle melting on planet mass. We show that (1) volcanism is likely to proceed on massive planets with plate tectonics over the main-sequence lifetime of the parent star; (2) crustal thickness (and melting rate normalized to planet mass) is weakly dependent on planet mass; (3) stagnant lid planets live fast (they have higher rates of melting than their plate tectonic counterparts early in their thermal evolution), but die young (melting shuts down after a few Gyr); (4) plate tectonics may not operate on high-mass planets because of the production of buoyant crust which is difficult to subduct; and (5) melting is necessary but insufficient for efficient volcanic degassing—volatiles partition into the earliest, deepest melts, which may be denser than the residue and sink to the base of the mantle on young, massive planets.