GY343 Petrology
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Mineral Mania
The Rock Factory A Pre-Visit Information Guide for Teachers Meets Next Generation Science Standards: 5-PS1-3; MS LS4-1,2; MS ESS1-4; MS-ESS2-1 How does our Earth create so many different types of rocks? Learn about the different processes that form and reform rocks as you identify many types of rocks, minerals and fossils. Students will learn to think like geologists as they move through interactive investigation stations packed with specimens from the Museum’s collections. OBJECTIVES The Rock Cycle: Students will examine the three types of rocks - igneous, metamorphic and sedimentary – and discover the processes that create them. Tracing the connections between shale and slate, limestone and marble, students will discover how the rock cycle changes the very ground beneath our feet! Characteristics of Rocks Students will learn how to observe and identify rocks through their unique characteristics, looking for telling clues such as layering, crystal size, fossils, magnetism, and more. Students will practice their observational skills as they describe the Museum’s unique rock and mineral specimens. Investigation Stations: Students will explore Museum geology specimens up close at investigation stations to answer such questions as: “Why do fossils form only in certain rocks?” “How do rocks form from volcanic eruptions?” “How can I recognize different types of rocks?”. ACTIVITIES Teachers are encouraged to conduct pre-visit and post-visit classroom discussions and activities with their classes to make the most of their experience. Encourage your students to start a classroom rock collection, and create an exhibit with the rocks organized by type – igneous, sedimentary and metamorphic. -
Geologic Boulder Map of Campus Has Been Created As an Educational Educational an As Created Been Has Campus of Map Boulder Geologic The
Adam Larsen, Kevin Ansdell and Tim Prokopiuk Tim and Ansdell Kevin Larsen, Adam What is Geology? Igneous Geo-walk ing of marine creatures when the limestone was deposited. It also contains by edited and Written Geology is the study of the Earth, from the highest mountains to the core of The root of “igneous” is from the Latin word ignis meaning fire. Outlined in red, numerous fossils including gastropods, brachiopods, receptaculita and rugose the planet, and has traditionally been divided into physical geology and his- this path takes you across campus looking at these ancient “fire” rocks, some coral. The best example of these are in the Geology Building where the stone torical geology. Physical geology concentrates on the materials that compose of which may have been formed at great depths in the Earth’s crust. Created was hand-picked for its fossil display. Campus of the Earth and the natural processes that take place within the earth to shape by the cooling of magma or lava, they can widely vary in both grain size and Granite is another common building stone used on campus. When compa- its surface. Historical geology focuses on Earth history from its fiery begin- mineral composition. This walk stops at examples showing this variety to help nies sell granite, they do not use the same classification system as geologists. nings to the present. Geology also explores the interactions between the you understand what the change in circumstances will do to the appearance Granite is sold in many different colours and mineral compositions that a Map Boulder Geologic lithosphere (the solid Earth), the atmosphere, the biosphere (plants, animals of the rock. -
Virgin Islands National Park Geologic Resources Inventory Report
National Park Service U.S. Department of the Interior Natural Resource Program Center Virgin Islands National Park Geologic Resources Inventory Report Natural Resource Report NPS/NRPC/GRD/NRR—2010/226 THIS PAGE: Underwater ecosystems including coral reefs are a primary natural resource at Virgin Islands National Park. National Park Service photograph. ON THE COVER: This view of Trunk Bay shows the steep slopes characteristic of Virgin Islands Na- tional Park. National Park Service photo- graph courtesy Rafe Boulon (Virgin Islands National Park). Virgin Islands National Park Geologic Resources Inventory Report Natural Resource Report NPS/NRPC/GRD/NRR—2010/226 Geologic Resources Division Natural Resource Program Center P.O. Box 25287 Denver, Colorado 80225 July 2010 U.S. Department of the Interior National Park Service Natural Resource Program Center Fort Collins, Colorado The National Park Service, Natural Resource Program Center publishes a range of reports that address natural resource topics of interest and applicability to a broad audience in the National Park Service and others in natural resource management, including scientists, conservation and environmental constituencies, and the public. The Natural Resource Report Series is used to disseminate high-priority, current natural resource management information with managerial application. The series targets a general, diverse audience, and may contain NPS policy considerations or address sensitive issues of management applicability. All manuscripts in the series receive the appropriate level of peer review to ensure that the information is scientifically credible, technically accurate, appropriately written for the intended audience, and designed and published in a professional manner. This report received informal peer review by subject-matter experts who were not directly involved in the collection, analysis, or reporting of the data. -
Exploring Origins of Pitted/Vesicular Rocks in Perseverance Valley, Endeavour Crater
50th Lunar and Planetary Science Conference 2019 (LPI Contrib. No. 2132) 2327.pdf EXPLORING ORIGINS OF PITTED/VESICULAR ROCKS IN PERSEVERANCE VALLEY, ENDEAVOUR CRATER. A. W. Tait1*, C. Schröder1, W. H Farrand2, J. W. Ashley3, B. A. Cohen4, R. Gellert5, J. Rice6, L. C. Crumpler7, B. Jolliff8, 1Biological and Environmental Sciences, University of Stirling, Stirling, FK9 4LA, UK ([email protected]), 2Space Science Institute, Boulder, CO, USA, 3Jet Propulsion Laboratory, California In- stitute of Technology, Pasadena, CA, USA, 4NASA Goddard Space Flight Centre, Greenbelt, MD, USA, 5Department of Physics, University of Guelph, Ontario, Canada, 6Planetary Science Institute, Tucson, AZ, USA, 7NM Museum of Natural History & Science, Albuquerque, NM, USA, 8Washington University in St. Louis, MO, USA. Introduction: Since sol 4780, the NASA Mars Ex- ploration Rover (MER) Opportunity has been traversing down Perseverance Valley (PV), a linear, negative-re- lief feature trending perpendicular to the western flank of Endeavour crater. The goal of the current investiga- tion is to understand PVs geomorphology and chemical composition to determine its mode of formation and ap- proximate age. Formation hypotheses include debris or fluid flow, and wind sculpting, all while intersecting possible Noachian lithologies [1]. Rover observations confirms orbital data that there exists a dextral off-set, indicating a structural origin to the valleys formation [2]. This faulting may have allowed for fluids to interact with the rocks [3]. On sol ~5000 Opportunity started to investigate a train of dark pitted/vesicular rocks with an unusual morphology, texture, and composition enriched in Al and Si. Here we describe the rock facies, and ex- plore preliminary formation/alteration hypotheses. -
Geology and Mineral Resources
UNITED STATES DEPARTMENT OF THE INTERIOR Harold L. Ickes, Secretary GEOLOGICAL SURVEY W. C. Mendenhall, Director Bulletin 879 GEOLOGY AND MINERAL RESOURCES OF THE BAKER QUADRANGLE, OREGON BY JAMES GILLULY Prepared in cooperation with the OREGON STATE MINING BOARD UNITED STATES GOVERNMENT PRINTING OFFICE WASHINGTON : 1937 For sale by the Superintendent of Documents, Washington, D. C. ------ Price -65 cents CONTENTS Page Abstract. ______________.________--_-_---_-_--.--_-.---------.---_ 1 Introduction._ _ _ ________________________________________________ 2 Field work and acknowledgments.______________________________ 2 Bibliography_.____._____..._.._.-_..---.._--_-...--......-._. 3 Geography.________ ...........^..-..-....... __-_____--__--.__--_. 4 Location and general features of the region.._____-_-.-___---._.._ 4 Topography.____..__.______._._._.___..-___ __-_.__.___.__. 5 Climate_._______-___--__.---__--__---_---_----__.-----.---_ 6 Drainage_ _ -__-_----_----.---------------------------------- 6 Geology .__.____-___.-____-.-__._.---.--_-_.._-.-.--....-_-. 7 General features.______-____----_--------_-____---_-_---__--__ 7 Pre-Tertiary rocks.___.-_-----------------------.--------.--.. 9 Supracrustal rocks_______________--_--__-___-_-_-------__ 9 Burnt River schist.__-____-__---__--__-_---_---__---__ 9 Distribution and topographic expression.._.._....._. 9 Thickness.__-__---_----------_-----------------_- 9 Lithology __-_-_______-_---_-..------.-__--_-_--_- 10 Conditions of sedimentation._..______--___-_.__-.._ 12 Stratigraphic relations and age_________._____.-.__ 12 Elkhorn Ridge argillite.-..__._-.----_-__-..-_-____-_-. 14 General features-___---___-------_----------_--___ 14 Thickness-__--__--_--_---_----------_-_-----_--__ 14 Lithology _____._---_-__-__--__--_-_--__-_-.-_-___ 14 Nonfissility of the argillite____-.______._-__-_---_ 18 Conditions of deposition.______.-___.-__._-___.____ 20 Age and relations to other formations.-.--._------_-. -
Petrology of Volcanic Rocks from Kaula Island, Hawaii Implications for the Origin of Hawaiian Phonolites
Contributions to Contrib Mineral Petrol (1986) 94:461-471 Mineralogy and Petrology Springer-Verlag 1986 Petrology of volcanic rocks from Kaula Island, Hawaii Implications for the origin of Hawaiian phonolites Michael O. Garcia 1, Frederick A. Frey 2, and David G. Grooms 1 * 1 Hawaii Institute of Geophysics, University of Hawaii, Honolulu, HI 96822, USA 2 Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA Abstract. A compositionally diverse suite of volcanic rocks, visited the island by helicopter courtesy of the U.S. Navy. including tholeiites, phonolites, basanites and nephelinites, Abundant unexploded ordnance, bird nests (total bird pop- occurs as accidental blocks in the palagonitic tuff of Kaula ulation >45,000) and steep cliffs surrounding the island Island. The Kaula phonolites are the only documented made sample collection hazardous. phonolites from the Hawaiian Ridge. Among the accidental Kaula Island consists of approximately 160 m of well- blocks, only the phonolites and a plagioclase basanite were bedded, palagonitic tuff (Fig. 2). The tuff contains acciden- amenable to K-Ar age dating. They yielded ages of tal fragments of light gray (phonolite) and dark gray (ba- 4.0-4.2 Ma and 1.8 ___0.2 Ma, respectively. Crystal fraction- salt) volcanic rocks, coralline material, coarse-grained ultra- ation modeling of major and trace element data indicates mafic and marie xenoliths (including spinel pyroxenites, that the phonolites could be derived from a plagioclase garnet pyroxenites, spinel peridotites and dunites) and me- basanite by subtraction of 27% clinopyroxene, 21% plagio- gacrysts (augite, anorthoclase, olivine, Al-spinel and titano- clase, 16% anorthoclase, 14% olivine, 4% titanomagnetite magnetite). -
Petrology on Mars†K
American Mineralogist, Volume 100, pages 2380–2395, 2015 INVITED CENTENNIAL ARTICLE REVIEW Petrology on Mars†k HARRY Y. MCSWEEN JR.1,* 1Department of Earth and Planetary Sciences and Planetary Geoscience Institute, University of Tennessee, Knoxville, Tennessee 37996-1410, U.S.A. ABSTRACT Petrologic investigations of martian rocks have been accomplished by mineralogical, geochemical, and textural analyses from Mars rov- ers (with geologic context provided by orbiters), and by laboratory analyses of martian meteorites. Igneous rocks are primarily lavas and volcaniclastic rocks of basaltic composition, and ultramafic cumulates; alkaline rocks are common in ancient terranes and tholeiitic rocks occur in younger terranes, suggesting global magmatic evolution. Relatively uncommon feldspathic rocks represent the ultimate fractionation prod- ucts, and granitic rocks are unknown. Sedimentary rocks are of both clastic (mudstone, sandstone, conglomerate, all containing significant igneous detritus) and chemical (evaporitic sulfate and less common carbonate) origin. High-silica sediments formed by hydrothermal activity. Sediments on Mars formed from different protoliths and were weathered under different environmental conditions from terrestrial sediments. Metamorphic rocks have only been inferred from orbital remote-sensing measurements. Metabasalt and serpentinite have mineral assemblages consistent with those predicted from low-pressure phase equilibria and likely formed in geothermal systems. Shock effects are com- mon in martian meteorites, and impact breccias are probably widespread in the planet’s crustal rocks. The martian rock cycle during early periods was similar in many respects to that of Earth. However, without plate tectonics Mars did not experience the thermal metamorphism and flux melting associated with subduction, nor deposition in subsided basins and rapid erosion resulting from tectonic uplift. -
Structure of the Earth
And the ROCK CYCLE Structure of the Earth Compositional (Chemical) Layers Crust: Low density High in silicon (Si) and oxygen (O) Moho: Density boundary between crust and mantle Mantle: Higher density High in Magnesium (Mg) and Iron (Fe) Core: High in Nickel (Ni) and Iron (Fe) Heat Flow in the Earth Heat sources: latent heat from the formation of the Earth Radioactive decay in the core and mantle Temperature in the core: 3000- 5000° C Cooling processes: Convection currents: in outer core and asthenosphere transport heat to the surface Plate tectonics releases heat through the crust (volcanoes) Convection cells in the mantle and core transport heat from the interior of earth to the surface and also return cooler material back into the earth. Mechanical (Physical) Layers of the Earth Lithosphere: Crust and upper, solid part of the mantle; “plates” in plate tectonics Asthenosphere: Partially molten part of mantle; location of convection current that drive plates Outer core: Liquid Inner core: Solid Greatest temperatures, solid due to intense pressure Comparing Compositional Layers to Mechanical Layers Moho What is a Rock? A group of minerals bound together Three major groups: 1) Igneous: Solidified Molten Magma 2) Sedimentary: formed by cementing of sediments. Sediments come from the erosion of other rocks. 3) Metamorphic: Heat and pressure change a rock into something new, without melting. Rock Types Igneous: Solidified molten magma 2 types of Igneous: 1) Extrusive (volcanic) = erupted lava Cools more quickly, so only small crystals form. 2) Intrusive (plutonic) = never erupted magma Cools more slowly within the earth, so larger crystals can form. -
Package 'NORRRM'
Package ‘NORRRM’ March 11, 2015 Type Package Title Geochemical Toolkit for R Version 1.0.0 Date 2015-01-29 Author Renee Gonzalez Guzman Maintainer Renee Gonzalez Guzman <[email protected]> Imports ggplot2,SDMTools Description CIPW Norm (acronym from the surnames of the authors: Cross, Iddings, Pirrson and Washington) is the most commonly used calculation algorithm to estimate the standard mineral assemblages for igneous rocks from its geochemical composition. NORRRM (acronym from noRm, R lan- guage and Renee) is the highly consistent program to calculate the CIPW Norm. Depends R (>= 3.1.1) License GPL (>= 3) NeedsCompilation no Repository CRAN Date/Publication 2015-03-11 21:49:49 R topics documented: NORRRM-package . .2 AdjRock . .3 Andes . .4 AtomWeight . .5 CIPW............................................6 CIPW.trace . .7 MinWeight . .9 OxiWeight . 10 TASplot . 11 TestTAS . 12 Index 13 1 2 NORRRM-package NORRRM-package Geochemical Toolkit for R Description According to the IUGS (International Union of Geological Science), Subcommission on the Sys- tematics of Igneous Rocks, the primary classification of igneous rocks must be based according to their modal mineral composition, expressed in volume percent. Nevertheless, where these data are not available or can not be determined owing to fine-grained mineral assemblage, glassy content or changes in the original mineralogy, then other criteria based on chemical bulk composition may be used. Computed from the chemical composition, the normative mineralogy is an alternative approach for mineralogical classification and useful for set up the naming of igneous rocks (as parts of the TAS classification, TASplot). The CIPW Norm is the most commonly used calculation algorithm to estimate the standard mineral assemblages for igneous rocks CIPW, generated over more than a hundred years ago and thereafter modified by some authors to the passage of the years (e.g., Verma et al., 2002). -
Geologica Macedonica
UDC 55 In print: ISSN 0352–1206 CODEN – GEOME 2 On line: ISSN 1857–8586 GEOLOGICA MACEDONICA Geologica Macedonica Vol. No pp. Štip 31 1 1–102 2017 Geologica Macedonica . . Geologica Macedonica Vol. No pp. Štip Geologica Macedonica . 31 1 . 1–102 2017 GEOLOGICA MACEDONICA Published by: – : "Goce Delev" University in Štip, Faculty of Natural and Technical Sciences, Štip, Republic of Macedonia „ “ , , , EDITORIAL BOARD Todor Serafimovski (R. Macedonia, Editor in Chief), Blažo Boev (R. Macedonia, Editor), David Alderton (UK), Tadej Dolenec (R. Slovenia), Ivan Zagorchev (R. Bulgaria), Wolfgang Todt (Germany), acad. Nikolay S. Bortnikov (Russia), Clark Burchfiel (USA), Thierry Augé (France), Todor Delipetrov (R. Macedonia), Vlado Bermanec (Croatia), Milorad Jovanovski (R. Macedonia), Spomenko Mihajlovi (Serbia), Dragan Milovanovi (Serbia), Dejan Prelevi (Germany), Albrecht von Quadt (Switzerland) ! " #" $ %&' ( (. , ), #) # (. , ), (. ), (. ), (. ), ! (" ), . # . ( ), $ ! (%), & (' ), (. ), " ((), ) (. ), " * + (, ), + (, ), - + (" ), %,* ! $ ( ) Language editor . Marijana Kroteva (English) ( ) Georgi Georgievski * *( (Macedonian) (" ) Technical editor * Blagoja Bogatinoski #* # * ( Proof-reader $ Alena Georgievska *( Address % GEOLOGICA MACEDONICA GEOLOGICA MACEDONICA EDITORIAL BOARD +!, Faculty of Natural and Technical Sciences ' * P. O. Box 96 /. !* 96 MK-2000 Štip, Republic of Macedonia $-2000 , , Tel. ++ 389 032 550 575 . 032 550 575 E-mail: [email protected] -
Extrusive Igneous Rocks- a Rock Formed on the Earth’S Surface
Rocks What is a rock? • Rock- naturally formed, consolidated materials composed of one or more minerals. • There are 3 types of rocks: • Igneous • Sedimentary • Metamorphic Igneous Rocks What are Igneous Rocks? • Magma vs. Lava • Magma- molten rock below the Earth’s surface. • Lava- magma on the Earth’s surface. • Igneous Rock- rocks made from cooling magma or lava. • They can be intrusive or extrusive. Intrusive vs. Extrusive • Intrusive Igneous Rocks- a rock that forms below the Earth’s surface. • Normally made from magma • Extrusive Igneous Rocks- a rock formed on the Earth’s surface. • Normally made from lava. Extrusive rock The white rock is intrusive. Intrusive Igneous Rocks • We cannot see these rocks be formed. • They typically have large crystal minerals. • The rock itself can give you a lot of information about how it was formed. Extrusive Igneous Rocks • You can see them form: • Lava flow • Ash Flow • Lava that cools down very quickly so all you see is ask coming out • Pyroclastic Flow • Clouds flowing downhill like a huge avalanche. • Data from these rocks can be used to interpret ancient volcanic activity. Igneous Rock Textures • The crystal size of the rock is related to the speed of the rock cooling. • Fast gives you small crystals and slow cooling gives you large crystals. • Also the rocks can appear: • Glassy- look like a piece of glass. • From the magma/lava cooling too quickly. • Vesicular- has air bubbles in it. This is vesicular. • From air bubbles getting trapped in the magma/lava. • Fragmental- they look jagged and angular. This is glassy and fragmental. -
Lavas. Understanding Volcanism Provides a Background for Theories
lavas. Understanding volcanism provides a background for theories relating to mountain building, the development and evolution of continental and oceanic crt~st,and how the crust is deformed. Our observations of volcanic activity fit nicely into plate-tectonic theory as described in chapter 11. The May 18, 1980 eruption of Mount St. Helens (box 10.1) was a spectacular release of energy from the earth's interior. The plate-tectonic explanation is that North America, moving weritwa~d,is overriding a portion of the Pacific Ocean Aoor. Melting of previously solid rock takes place at depth, just above the subduction zone. (Thii was described briefly in chapter 1 and more thoroughly in chapter 11.) At least some of the magma (molten rock or liquid that is mostly silica) works its way upward to the earth's surface to erupt. Magma does not always reach the earth's surface before solidifying, but when it does it is called lava. At Mount St. Helens the lava solidified quickly as it was blasted explosively by gases into the air, producing rock frag- ments known as pyrodasw (from the Greekpyro, "fire," and clart, "broken"). Pyroclastic debris is also known as tcphra. Elsewhere in the world (notably Hawaii) lava extrudes out of Flgulr 10.1 fissures in the ground as lava flows. Pyrodastic debris and Volcanic eruptions in Hawaii, 1969. A lava fountain is supply11 rock formed by solidification of lava are collectively regarded the lava cascading over the cliff. as emwive rock, surface rock resulting from volcanic Photo by D A Swanson, US Geolog~calSurvey acrivity.