Gravels, Conglomerates, and Breccias
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A) Conglomerate B) Dolostone C) Siltstone D) Shale 1. Which
1. Which sedimentary rock would be composed of 7. Which process could lead most directly to the particles ranging in size from 0.0004 centimeter to formation of a sedimentary rock? 0.006 centimeter? A) metamorphism of unmelted material A) conglomerate B) dolostone B) slow solidification of molten material C) siltstone D) shale C) sudden upwelling of lava at a mid-ocean ridge 2. Which sedimentary rock could form as a result of D) precipitation of minerals from evaporating evaporation? water A) conglomerate B) sandstone 8. Base your answer to the following question on the C) shale D) limestone diagram below. 3. Limestone is a sedimentary rock which may form as a result of A) melting B) recrystallization C) metamorphism D) biologic processes 4. The dot below is a true scale drawing of the smallest particle found in a sample of cemented sedimentary rock. Which sedimentary rock is shown in the diagram? What is this sedimentary rock? A) conglomerate B) sandstone C) siltstone D) shale A) conglomerate B) sandstone C) siltstone D) shale 9. Which statement about the formation of a rock is best supported by the rock cycle? 5. Which sequence of events occurs in the formation of a sedimentary rock? A) Magma must be weathered before it can change to metamorphic rock. A) B) Sediment must be compacted and cemented before it can change to sedimentary rock. B) C) Sedimentary rock must melt before it can change to metamorphic rock. C) D) Metamorphic rock must melt before it can change to sedimentary rock. D) 6. Which sedimentary rock formed from the compaction and cementation of fragments of the skeletons and shells of sea organisms? A) shale B) gypsum C) limestone D) conglomerate Base your answers to questions 10 and 11 on the diagram below, which is a geologic cross section of an area where a river has exposed a 300-meter cliff of sedimentary rock layers. -
Sequence Stratigraphy of the Neoproterozoic Infra Krol Formation and Krol Group, Lesser Himalaya, India
SEQUENCE STRATIGRAPHY OF THE NEOPROTEROZOIC INFRA KROL FORMATION AND KROL GROUP, LESSER HIMALAYA, INDIA GANQING JIANG1, NICHOLAS CHRISTIE-BLICK1, ALAN J. KAUFMAN2, DHIRAJ M. BANERJEE3, AND VIBHUTI RAI4 1 Department of Earth and Environmental Sciences and Lamont-Doherty Earth Observatory of Columbia University, Palisades, New York 10964±8000, U.S.A. 2 Department of Geology, University of Maryland, College Park, Maryland 20742±4211, U.S.A. 3 Department of Geology, University of Delhi, Delhi 110007, India 4 Department of Geology, Lucknow University, Lucknow 226007, India e-mail: [email protected] ABSTRACT: A sequence stratigraphic study of terrigenous and carbonate rocks GEOLOGICAL FRAMEWORK of the Infra Krol Formation and Krol Group in the Lesser Himalaya fold and thrust belt of northern India was undertaken as part of a broader investigation The Infra Krol Formation and Krol Group are part of a Neoproterozoic and Lower of the signi®cance of carbon isotope data in Neoproterozoic successions. Eight Cambrian succession more than 12 km thick, cropping out in the Lesser Himalaya regional stratigraphic discontinuities were traced over a distance of nearly 300 in a series of doubly plunging synclines between Solan in the northwest and Nainital, km, and interpretations were anchored in a series of local studies involving the 280 km to the southeast (Fig. 1; Bhargava 1979; Shanker et al. 1989; Shanker et mapping of key beds and the measurement of closely spaced sections. Three of al. 1993; Shanker et al. 1997; Shanker and Mathur 1992). -
A Brief History of Till Research and Developing Nomenclature
k 7 2 A Brief History of Till Research and Developing Nomenclature With relief one remembers that, after all, the facts gathered with such infinite care, over so many years, are in no ways affected: their permanency is untouched, their value as high as ever. It is the interpretation which has gone astray. Carruthers (1953, p. 36) A benchmark publication in the development of till nomenclature was contained in the final report by the INQUA Commission on Genesis and Lithology of Glacial Quaternary Deposits, entitled ‘Genetic Classification of Glacigenic Deposits’ (Goldthwait and Matsch, 1989; Figure 2.1). Most significant in this report was the paper by Aleksis Dreimanis (Figure 2.2), entitled ‘Tills: Their Genetic Terminology k k and Classification’, a summary of the findings of the Till Work Group, which operated over the period 1974–1986. It was a synthesis of knowledge and a rationale for a unified process-based nomenclature but at the same time afforded the presentation of alternative standpoints on till classification, and hence delivered a selection of frameworks containing complex and overlapping genetic terms. More broadly, ‘till’ at this juncture was defined as: a sediment that has been transported and is subsequently deposited by or from glacier ice, with little or no sorting by water. (Dreimanis and Lundqvist, 1984, p. 9) As a way forward, the Till Work Group, through Dreimanis (1989), arrived at a series of nomencla- ture diagrams (Figure 2.3), which aimed at an inclusive but at the same time simplified and unambigu- ous, process-based till classification scheme. More specifically, Dreimanis (1989), within the same volume, compiled a table of diagnostic characteristics for differentiating what he termed ‘lodgement till’, ‘melt-out till’ and ‘gravity flowtill’. -
Sedimentary Rocks
Illinois State Museum Geology Online – http://geologyonline.museum.state.il.us Sedimentary Rocks Grade Level: 9 – 12 Purpose: The purpose of this lesson is to introduce sedimentary rocks. Students will learn what sedimentary rocks are and how they form. It will teach them how to identify some common examples. Suggested Goals: Students will shake a flask of sand and water to see how particles settle. They will draw a picture showing where the various rocks form and they will identify some common examples. Targeted Objectives: All of Illinois is covered by sedimentary rocks. In most places, they reach a thickness that could be expressed in miles rather than feet. Ancient seas dropped untold numbers of particles for hundreds of millions of years creating the layers that bury the original igneous rocks in 2,000 to 17,000 feet of sedimentary layers. These valuable layers are used to construct our homes, build our highways, and some were even used to heat our homes. The Illinois Basin dominates the geology of southern Illinois. There the layers dip down until they are over three miles thick. The geology of Illinois cannot be told without discussing sedimentary rocks because they are what Illinois is made of. Students will learn to tell the difference between the major sedimentary rock varieties. Students will learn in what environments different sedimentary rocks form. Students will learn what sedimentary rocks are. Background: Most sedimentary rocks are formed when weathering crumbles the parent rock to such a small size that they can be carried by wind or water. Those particles suspended in water collide with one another countless times gradually becoming smaller and more rounded. -
Part 629 – Glossary of Landform and Geologic Terms
Title 430 – National Soil Survey Handbook Part 629 – Glossary of Landform and Geologic Terms Subpart A – General Information 629.0 Definition and Purpose This glossary provides the NCSS soil survey program, soil scientists, and natural resource specialists with landform, geologic, and related terms and their definitions to— (1) Improve soil landscape description with a standard, single source landform and geologic glossary. (2) Enhance geomorphic content and clarity of soil map unit descriptions by use of accurate, defined terms. (3) Establish consistent geomorphic term usage in soil science and the National Cooperative Soil Survey (NCSS). (4) Provide standard geomorphic definitions for databases and soil survey technical publications. (5) Train soil scientists and related professionals in soils as landscape and geomorphic entities. 629.1 Responsibilities This glossary serves as the official NCSS reference for landform, geologic, and related terms. The staff of the National Soil Survey Center, located in Lincoln, NE, is responsible for maintaining and updating this glossary. Soil Science Division staff and NCSS participants are encouraged to propose additions and changes to the glossary for use in pedon descriptions, soil map unit descriptions, and soil survey publications. The Glossary of Geology (GG, 2005) serves as a major source for many glossary terms. The American Geologic Institute (AGI) granted the USDA Natural Resources Conservation Service (formerly the Soil Conservation Service) permission (in letters dated September 11, 1985, and September 22, 1993) to use existing definitions. Sources of, and modifications to, original definitions are explained immediately below. 629.2 Definitions A. Reference Codes Sources from which definitions were taken, whole or in part, are identified by a code (e.g., GG) following each definition. -
Style, Scale and Significance of Sand Bodies in the Northern and Central Belts, Southwest Southern Uplands
Journal ofthe Geological Society, London, Vol. 144, 1987, pp. 787-805, 13 figs, 3 tables, Printed in Northern Ireland Style, scale and significance of sand bodies in the Northern and Central Belts, southwest Southern Uplands G.KELLINGl, P. DAVIES' & J. HOLROYD2 1 Geology Department, University of Keele, Staffs. ST5 5BG, UK 21 Blythe Road, Forsbrook, Blythe Bridge, Staffs., UK Abstract: Sedimentological and biostratigraphical data fromthe Rhinns of Galloway andadjacent areas in SW Scotland confirm that deep-water depositional systems consistently operated along, and were sourced from, the northwestern margin of an asymmetrical basin during the late Ordovician and earlySilurian, while pelagic facies accumulated simultaneously tothe SE, providing ascenario analogous to many modern trench systems. Most of the observedsedimentological anomalies, with regard to thisgeneral model, can be explained within the context of the varied styles of trench-filling depositional systems, briefly reviewed here, and the major stratigraphic and sedimentologic features can be best explained in terms of a geotectonically evolving fore-arcregion. Two main phases of development are recognized: (a) Llandeilo-late Ashgill: during this time interval the fore-arc trench region was tectonically juxtaposed against an active continental margin arc. Small- to medium-scale, SE-prograding sand-rich fans were formed within a relatively narrow trench, leading to axial diversion of the fans, initially to NE but later mainly to SW. Simultaneously a coarse volcanilithic sediment apron, flanking the arc, migrated gradually northeastwards, probably in response to relative fault displacement of the arc and trench; (b) Llandovery: during this time interval the fore-arc trench region was dominated by a variety of mainly fan-typedepositional systems which were exclusively sourced(at least until theuppermost Llandovery) from the northwestern margin. -
Activity #4 Evidence for an Atmosphere on Mars Over Time: Water Surface Features [Adult]
Activity #4 Evidence for an Atmosphere on Mars Over Time: Water Surface Features [Adult] Adapted from: “Did Water Create Features On Mars?” from NASA’s Mars and Earth: Science and Learning Activities for Afterschool: http://tinyurl.com/pcfbln3 and Rivers on Mars?: http://tinyurl.com/qfeqv4q with permission from the Lunar and Planetary Institute, LPI Contribution Number 1490. Unless otherwise noted, all images are courtesy of SETI Institute. 1. Introduction In this activity, you will compare images of Mars and Earth surface features that have been eroded by water. Then you will construct, observe, and test a model of flowing water and look for similar erosion patterns. You will also “Think like a scientist. Be a Scientist!” 2. Science Objectives You will: • construct models to test ideas about processes that cannot be directly studied on Mars; • ask experimental questions, collect data, and use evidence to answer those questions about flowing water erosion; • relate evidence of sustained flowing water on Mars as support for a thicker early Martian atmosphere and a warmer climate more like Earth’s; and • appreciate evidence of ancient water erosion that points to changes in Mars’ atmosphere over a very long period of time. 3. Materials For each group of Cadettes: recommend teams of 4 Cadettes. Direct the Cadettes to find materials. • [1] solid plastic growing tray (no holes), 28 x 53 x 6 cm (11 x 21 x 2.5 in) lined with a lightweight plastic sheet such as a paint drop cloth. Trays can be ordered from Amazon.com or found in local hardware stores. -
Activity #4 Evidence for an Atmosphere on Mars Over Time: Water Surface Features [Cadette]
Activity #4 Evidence for an Atmosphere on Mars Over Time: Water Surface Features [Cadette] Adapted from: “Did Water Create Features On Mars?” from NASA’s Mars and Earth: Science and Learning Activities for Afterschool: http://tinyurl.com/pcfbln3 and Rivers on Mars?: http://tinyurl.com/qfeqv4q with permission from the Lunar and Planetary Institute, LPI Contribution Number 1490. Unless otherwise noted, all images are courtesy of SETI Institute. 1. Introduction In this activity, you will compare images of Mars and Earth surface features that have been eroded by water. Then you will construct, observe, and test a model of flowing water and look for similar erosion patterns. You will also “Think like a scientist. Be a Scientist!” 2. Science Objectives You will: • construct models to test ideas about processes that cannot be directly studied on Mars; • ask experimental questions, collect data, and use evidence to answer those questions about flowing water erosion; • relate evidence of sustained flowing water on Mars as support for a thicker early Martian atmosphere and a warmer climate more like Earth’s; and • appreciate evidence of ancient water erosion that points to changes in Mars’ atmosphere over a very long period of time. 3. Materials For each group of Cadettes: recommend teams of 4 Cadettes. Pick up your materials as directed by your adult leader. • [1] model Stream Table • [1] conglomerate rock • [1] 1.0 liter (34 oz) disposable water bottle filled with tap water • [1] plastic catch-bucket, about 4 liters (about 1 gal) or even larger for drainage water • [3–4] thinly-sliced foam florist blocks to raise one end of the tray; view on Amazon.com: http://tinyurl.com/knv57cc • [1] protractor • [4–5] assorted rocks from thumb- to palm-sized • [2] colored pencils (2 per Cadette; any color) • newspapers to place under tray and bucket (for cleanup) • (optional) latex gloves (caution: check for allergies), sponges, rags, and brooms ©SETI Institute 2015 Activity 4: Evidence for an Atmosphere on Mars Over Time [Cadette] • 1 4. -
Cat Herding on a Global Scale
OneGeology-Europe – an INSPIRE testbed for semantic harmonisation of „geology“ data across Europe (WP 3) Kristine Asch and John Laxton Project deliverables • Interoperable on- shore geology spatial dataset • with ”progress • Mutilingual metadata for towards discovery harmonisation” • View services • Forerunner and “guinea • Geological pig” for the vocabulary and data implementation of specifications for INSPIRE Directive Europe • Use case studies Fact Vast amount of data hidden in the archives and hard disks in governmental organisations across Europe … Kristine Asch ©BGR.de And they are all different.. Edge matching at national boundaries? Î National boundary Î geological terms and classifications (age, lithology, tectonics ..) Î age of data (mapping campaign) Î choice of units to be mapped Î level of detail / scale Î topographical base (projection, spheroid, drainage system, ...) Î Portrayal (colours and symbols) Î Mapped border of the units Interoperability and harmonisation • Interoperability – when the data model/structure and properties to describe its parts (what GeoSciML does) is agreed – E.g. agreeing a data model will have the feature of “GeologicUnit” with properties of “age” and “lithology” • Semantic harmonisation – when the use of the same definitions and classifications to describe a concept/term is agreed – E.g. ‘clay’. The same concept can be labelled with several terms (“argilla” in Italian, “Ton” in German), but needs to have the same definition, in this case of “clay/Ton/argilla, …”): > 50% particles < 0,004 mm (Wentworth -
A Systematic Nomenclature for Metamorphic Rocks
A systematic nomenclature for metamorphic rocks: 1. HOW TO NAME A METAMORPHIC ROCK Recommendations by the IUGS Subcommission on the Systematics of Metamorphic Rocks: Web version 1/4/04. Rolf Schmid1, Douglas Fettes2, Ben Harte3, Eleutheria Davis4, Jacqueline Desmons5, Hans- Joachim Meyer-Marsilius† and Jaakko Siivola6 1 Institut für Mineralogie und Petrographie, ETH-Centre, CH-8092, Zürich, Switzerland, [email protected] 2 British Geological Survey, Murchison House, West Mains Road, Edinburgh, United Kingdom, [email protected] 3 Grant Institute of Geology, Edinburgh, United Kingdom, [email protected] 4 Patission 339A, 11144 Athens, Greece 5 3, rue de Houdemont 54500, Vandoeuvre-lès-Nancy, France, [email protected] 6 Tasakalliontie 12c, 02760 Espoo, Finland ABSTRACT The usage of some common terms in metamorphic petrology has developed differently in different countries and a range of specialised rock names have been applied locally. The Subcommission on the Systematics of Metamorphic Rocks (SCMR) aims to provide systematic schemes for terminology and rock definitions that are widely acceptable and suitable for international use. This first paper explains the basic classification scheme for common metamorphic rocks proposed by the SCMR, and lays out the general principles which were used by the SCMR when defining terms for metamorphic rocks, their features, conditions of formation and processes. Subsequent papers discuss and present more detailed terminology for particular metamorphic rock groups and processes. The SCMR recognises the very wide usage of some rock names (for example, amphibolite, marble, hornfels) and the existence of many name sets related to specific types of metamorphism (for example, high P/T rocks, migmatites, impactites). -
45. Sedimentary Facies and Depositional History of the Iberia Abyssal Plain1
Whitmarsh, R.B., Sawyer, D.S., Klaus, A., and Masson, D.G. (Eds.), 1996 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 149 45. SEDIMENTARY FACIES AND DEPOSITIONAL HISTORY OF THE IBERIA ABYSSAL PLAIN1 D. Milkert,2 B. Alonso,3 L. Liu,4 X. Zhao,5 M. Comas,6 and E. de Kaenel4 ABSTRACT During Leg 149, a transect of five sites (Sites 897 to 901) was cored across the rifted continental margin off the west coast of Portugal. Lithologic and seismostratigraphical studies, as well as paleomagnetic, calcareous nannofossil, foraminiferal, and dinocyst stratigraphic research, were completed. The depositional history of the Iberia Abyssal Plain is generally characterized by downslope transport of terrigenous sedi- ments, pelagic sedimentation, and contourite sediments. Sea-level changes and catastrophic events such as slope failure, trig- gered by earthquakes or oversteepening, are the main factors that have controlled the different sedimentary facies. We propose five stages for the evolution of the Iberia Abyssal Plain: (1) Upper Cretaceous and lower Tertiary gravitational flows, (2) Eocene pelagic sedimentation, (3) Oligocene and Miocene contourites, (4) a Miocene compressional phase, and (5) Pliocene and Pleistocene turbidite sedimentation. Major input of terrigenous turbidites on the Iberia Abyssal Plain began in the late Pliocene at 2.6 Ma. INTRODUCTION tured by both Mesozoic extension and Eocene compression (Pyrenean orogeny) (Boillot et al., 1979), and to a lesser extent by Miocene com- Leg 149 drilled a transect of sites (897 to 901) across the rifted mar- pression (Betic-Rif phase) (Mougenot et al., 1984). gin off Portugal over the ocean/continent transition in the Iberia Abys- Previous studies of the Cenozoic geology of the Iberian Margin sal Plain. -
Stratigraphic Signature of the Late Palaeozoic Ice Age in the Parmeener Supergroup of Tasmania, SE Australia, and Inter- Regional Comparisons
University of Nebraska - Lincoln DigitalCommons@University of Nebraska - Lincoln Earth and Atmospheric Sciences, Department Papers in the Earth and Atmospheric Sciences of 2010 Stratigraphic signature of the late Palaeozoic Ice Age in the Parmeener Supergroup of Tasmania, SE Australia, and inter- regional comparisons Christopher R. Fielding University of Nebraska-Lincoln, [email protected] Tracy D. Frank University of Nebraska-Lincoln, [email protected] John L. Isbell University of Wisconsin-Milwaukee, [email protected] Lindsey C. Henry University of Wisconsin-Milwaukee Eugene W. Domack Hamilton College, Clinton, NY, [email protected] Follow this and additional works at: https://digitalcommons.unl.edu/geosciencefacpub Part of the Earth Sciences Commons Fielding, Christopher R.; Frank, Tracy D.; Isbell, John L.; Henry, Lindsey C.; and Domack, Eugene W., "Stratigraphic signature of the late Palaeozoic Ice Age in the Parmeener Supergroup of Tasmania, SE Australia, and inter-regional comparisons" (2010). Papers in the Earth and Atmospheric Sciences. 263. https://digitalcommons.unl.edu/geosciencefacpub/263 This Article is brought to you for free and open access by the Earth and Atmospheric Sciences, Department of at DigitalCommons@University of Nebraska - Lincoln. It has been accepted for inclusion in Papers in the Earth and Atmospheric Sciences by an authorized administrator of DigitalCommons@University of Nebraska - Lincoln. Published in Palaeogeography, Palaeoclimatology, Palaeoecology 298 (2010), pp. 70–90; doi:10.1016/j.palaeo.2010.05.023 Copyright © 2010 Elsevier B.V. Used by permission Submitted September 25, 2009; revised April 20, 2010; accepted May 20, 2010; published online June 1, 2010. Stratigraphic signature of the late Palaeozoic Ice Age in the Parmeener Supergroup of Tasmania, SE Australia, and inter-regional comparisons Christopher R.