Sedimentary Rocks
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Bedrock Geology Glossary from the Roadside Geology of Minnesota, Richard W
Minnesota Bedrock Geology Glossary From the Roadside Geology of Minnesota, Richard W. Ojakangas Sedimentary Rock Types in Minnesota Rocks that formed from the consolidation of loose sediment Conglomerate: A coarse-grained sedimentary rock composed of pebbles, cobbles, or boul- ders set in a fine-grained matrix of silt and sand. Dolostone: A sedimentary rock composed of the mineral dolomite, a calcium magnesium car- bonate. Graywacke: A sedimentary rock made primarily of mud and sand, often deposited by turbidi- ty currents. Iron-formation: A thinly bedded sedimentary rock containing more than 15 percent iron. Limestone: A sedimentary rock composed of calcium carbonate. Mudstone: A sedimentary rock composed of mud. Sandstone: A sedimentary rock made primarily of sand. Shale: A deposit of clay, silt, or mud solidified into more or less a solid rock. Siltstone: A sedimentary rock made primarily of sand. Igneous and Volcanic Rock Types in Minnesota Rocks that solidified from cooling of molten magma Basalt: A black or dark grey volcanic rock that consists mainly of microscopic crystals of pla- gioclase feldspar, pyroxene, and perhaps olivine. Diorite: A plutonic igneous rock intermediate in composition between granite and gabbro. Gabbro: A dark igneous rock consisting mainly of plagioclase and pyroxene in crystals large enough to see with a simple magnifier. Gabbro has the same composition as basalt but contains much larger mineral grains because it cooled at depth over a longer period of time. Granite: An igneous rock composed mostly of orthoclase feldspar and quartz in grains large enough to see without using a magnifier. Most granites also contain mica and amphibole Rhyolite: A felsic (light-colored) volcanic rock, the extrusive equivalent of granite. -
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. -
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. -
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. -
06Metamorphs.Pdf
Clicker • The transformation of one rock into another by solid-state Metamorphism and recrystallization is known as Metamorphic Rocks – a) Sedimentation – b) Metamorphism – c) Melting – d) Metasomatism – e) Hydrothermal alteration Metamorphism • Metamorphism is the solid- state transformation of pre- existing rock into texturally or mineralogically distinct new rock as the result of high temperature, high pressure, or both. Diamond is Metamorphic Metamorphism • The mineralogy of a metamorphic rock changes with temperature and pressure. • In general, the highest temperature mineral assemblage is preserved. • It is possible to infer the highest P- T conditions from the mineralogy. 1 Metamorphic Environments Metamorphic Environments • Regional metamorphism • Where do you find metamorphic involves the burial and rocks? metamorphism of entire regions • In the mountains and in continental (hundreds of km2) shield areas. • Contact metamorphism results from local heating adjacent to • Why? igneous intrusions. (several meters) • Because elsewhere they are covered by sediments. Metamorphic Environments Regional Metamorphism • Because the tectonic forces required to bury, metamorphose, and re- exhume entire regions are slow, • most regionally metamorphosed terranes are old (> 500 MY), and • most Precambrian (> 500 MY) terranes are metamorphosed. Regional Metamorphism Regional Metamorphism • Regional metamorphism is typically • Regional metamorphism is typically isochemical (composition of rock isochemical (composition of rock does not change), although water does not change), although water may be lost. may be lost. • Metasomatism is a term for non- • Metasomatism is a term for non- isochemical metamorphism. isochemical metamorphism. • Contact metamorphism is typically • Contact metamorphism is typically metasomatic. metasomatic. 2 Effect of Increasing Conditions of Metamorphism Temperature • Changing the mineralogy of a sediment requires temperature > • Increases the atomic vibrations 300ºC and pressures > 2000 • Decreases the density (thermal atmospheres (~6 km deep). -
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. -
Antrim Shale in the Michigan Basin Resources Estimated in Play 6319 and Play 6320
UNITED STATES DEPARTMENT OF THE INTERIOR Figure 7. Assessment form showing input for Play 6319. .......6 U.S. GEOLOGICAL SURVEY Figure 8. Assessment form showing input for Play 6320. .......7 An Initial Resource Assessment of the Upper Figure 9. Potential additions of technically recoverable resources. Cumulative probability distribution of gas Devonian Antrim Shale in the Michigan basin resources estimated in Play 6319 and Play 6320. ...........7 by Gordon L. Dolton and John C Quinn TABLES U.S. Geological Survey Table 1. Producing units analysed, showing drainage areas Open-File Report 95-75K and estimated ultimate recovery (EUR) calcuated per well, in billions of cubic feet gas (BCFG)..........................4 This report is preliminary and has not been reviewed for conformity with U.S. Geological Survey editorial Table 2. Undiscovered gas resources of the Antrim Shale. standards and stratigraphic nomenclature. Potential reserve additions of gas are shown for Plays 6319 and 6320. Gas in billions of cubic feet; natural gas U.S. Geological Survey, MS 934, Box 25046, Denver liquids are not considered to be present.. ........................7 Federal Center, Denver CO, 80225 1996 Introduction: An assessment of oil and gas resources of the United CONTENTS States was completed by the United States Geological Survey (USGS) in 1994 and published in 1995 (U.S. Introduction........................................................................ 1 Geological Survey National Oil and Gas Resource Antrim Shale gas plays ..................................................... 1 Assessment Team, 1995; Gautier and others, 1995; Dolton, 1995). As part of this assessment and for the Reservoirs ......................................................................... 2 first time, the USGS assessed recoverable resources Source Rocks.................................................................... 2 from unconventional or continuous-type deposits nationally. -
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. -
Origin and Resources of World Oil Shale Deposits - John R
COAL, OIL SHALE, NATURAL BITUMEN, HEAVY OIL AND PEAT – Vol. II - Origin and Resources of World Oil Shale Deposits - John R. Dyni ORIGIN AND RESOURCES OF WORLD OIL SHALE DEPOSITS John R. Dyni US Geological Survey, Denver, USA Keywords: Algae, Alum Shale, Australia, bacteria, bitumen, bituminite, Botryococcus, Brazil, Canada, cannel coal, China, depositional environments, destructive distillation, Devonian oil shale, Estonia, Fischer assay, Fushun deposit, Green River Formation, hydroretorting, Iratí Formation, Israel, Jordan, kukersite, lamosite, Maoming deposit, marinite, metals, mineralogy, oil shale, origin of oil shale, types of oil shale, organic matter, retort, Russia, solid hydrocarbons, sulfate reduction, Sweden, tasmanite, Tasmanites, thermal maturity, torbanite, uranium, world resources. Contents 1. Introduction 2. Definition of Oil Shale 3. Origin of Organic Matter 4. Oil Shale Types 5. Thermal Maturity 6. Recoverable Resources 7. Determining the Grade of Oil Shale 8. Resource Evaluation 9. Descriptions of Selected Deposits 9.1 Australia 9.2 Brazil 9.2.1 Paraiba Valley 9.2.2 Irati Formation 9.3 Canada 9.4 China 9.4.1 Fushun 9.4.2 Maoming 9.5 Estonia 9.6 Israel 9.7 Jordan 9.8 Russia 9.9 SwedenUNESCO – EOLSS 9.10 United States 9.10.1 Green RiverSAMPLE Formation CHAPTERS 9.10.2 Eastern Devonian Oil Shale 10. World Resources 11. Future of Oil Shale Acknowledgments Glossary Bibliography Biographical Sketch Summary ©Encyclopedia of Life Support Systems (EOLSS) COAL, OIL SHALE, NATURAL BITUMEN, HEAVY OIL AND PEAT – Vol. II - Origin and Resources of World Oil Shale Deposits - John R. Dyni Oil shale is a fine-grained organic-rich sedimentary rock that can produce substantial amounts of oil and combustible gas upon destructive distillation. -
Data of Geochemistry
Data of Geochemistry ' * Chapter W. Chemistry of the Iron-rich Sedimentary Rocks GEOLOGICAL SURVEY PROFESSIONAL PAPER 440-W Data of Geochemistry MICHAEL FLEISCHER, Technical Editor Chapter W. Chemistry of the Iron-rich Sedimentary Rocks By HAROLD L. JAMES GEOLOGICAL SURVEY PROFESSIONAL PAPER 440-W Chemical composition and occurrence of iron-bearing minerals of sedimentary rocks, and composition, distribution, and geochemistry of ironstones and iron-formations UNITED STATES GOVERNMENT PRINTING OFFICE, WASHINGTON : 1966 UNITED STATES DEPARTMENT OF THE INTERIOR STEWART L. UDALL, Secretary GEOLOGICAL SURVEY William T. Pecora, Director For sale by the Superintendent of Documents, U.S. Government Printing Office Washington, D.C. 20402 - Price 45 cents (paper cover) CONTENTS Page Face Abstract. _ _______________________________ Wl Chemistry of iron-rich rocks, etc. Continued Introduction. _________ ___________________ 1 Oxide facies Continued Iron minerals of sedimentary rocks __ ______ 2 Hematitic iron-formation of Precambrian age__ W18 Iron oxides __ _______________________ 2 Magnetite-rich rocks of Mesozoic and Paleozoic Goethite (a-FeO (OH) ) and limonite _ 2 age___________-__-._____________ 19 Lepidocrocite (y-FeO(OH) )________ 3 Magnetite-rich iron-formation of Precambrian Hematite (a-Fe2O3) _ _ _ __ ___. _ _ 3 age._____-__---____--_---_-------------_ 21 Maghemite (7-Fe203) __ __________ 3 Silicate facies_________________________________ 21 Magnetite (Fe3O4) ________ _ ___ 3 Chamositic ironstone____--_-_-__----_-_---_- 21 3 Silicate iron-formation of Precambrian age_____ 22 Iron silicates 4 Glauconitic rocks__-_-____--------__-------- 23 4 Carbonate facies______-_-_-___-------_---------- 23 Greenalite. ________________________________ 6 Sideritic rocks of post-Precambrian age._______ 24 Glauconite____ _____________________________ 6 Sideritic iron-formation of Precambrian age____ 24 Chlorite (excluding chamosite) _______________ 7 Sulfide facies___________________________ 25 Minnesotaite. -
Chapter 4 SILICICLASTIC ROCKS
Chapter 4 SILICICLASTIC ROCKS 1. SANDSTONES 1.1 Introduction 1.1.1 Sandstones are an important group of sedimentary rocks. I suppose a good estimate of the percentage of sedimentary rocks that would be classified as sandstones is about 25%. 1.1.2 Defining what's meant by the term sandstone turns out not to be easy. Recall from Chapter 1 that all sedimentary particles between 1/16 mm and 2 mm should be called sand, regardless of composition. But terminology for a sand deposit, as distinct from sand grain size, is more difficult. For a deposit to be called a sand, "most" of the particles must be in the sand size range. But how much is "most"? How much finer and/or coarser material can there be in a sand deposit? Various attempts have been made to erect terminology for mixtures of sand and finer/coarser sediment, with quantitative boundaries. There's no standard classification, but nobody seems to worry much about that. Figure 4-1 shows two ways of dealing with mixtures of sand and mud, one "rational", seemingly composed with logicality and symmetry in mind, and the other reflecting marine- geological practice. And 4-2 shows two ways of dealing with mixtures of sand and gravel, the first idealized and symmetrical, and the other reflecting field usage. The same difficulties in distinguishing between a sandstone and a conglomerate, at the one end, and between a sandstone and a siltstone, on the other end, are similar. If the rock has a lot of silt in it as well as sand, you can call it a silty sandstone, and if it has a lot of gravel in it was well as sand, you can call it a gravelly (or pebbly) sandstone or a conglomeratic sandstone. -
Weathering Effects on the Mineralogy, Chemistry and Micromorphology of Pierre Shale Matthew Alan Birchmier Iowa State University
Masthead Logo Iowa State University Capstones, Theses and Retrospective Theses and Dissertations Dissertations 1-1-2005 Weathering effects on the mineralogy, chemistry and micromorphology of Pierre Shale Matthew Alan Birchmier Iowa State University Follow this and additional works at: https://lib.dr.iastate.edu/rtd Recommended Citation Birchmier, Matthew Alan, "Weathering effects on the mineralogy, chemistry and micromorphology of Pierre Shale" (2005). Retrospective Theses and Dissertations. 18911. https://lib.dr.iastate.edu/rtd/18911 This Thesis is brought to you for free and open access by the Iowa State University Capstones, Theses and Dissertations at Iowa State University Digital Repository. It has been accepted for inclusion in Retrospective Theses and Dissertations by an authorized administrator of Iowa State University Digital Repository. For more information, please contact [email protected]. Weathering effects on the mineralogy, chemistry and micromorphology of Pierre Shale by Matthew Alan Birchmier A thesis submitted to the graduate faculty in partial fulfillment of the requirements for the degree of MASTER OF SCIENCE Major: Civil Engineering (Geotechnical Engineering) Program of Study Committee: Vernon Schaefer, Major Professor David White Michael Thompson Iowa State University Ames, Iowa 2005 Copyright© Matthew Alan Birchmier, 2005. All rights reserved. 11 Graduate College Iowa State University This is to certify that the master's thesis of Matthew Alan Birchmier has met the thesis requirements of Iowa State University Signatures