Chapter 3: Igneous Textures
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45. Myrmekite Formed by Na- and Ca-Metasomatism of K- Feldspar
1 ISSN 1526-5757 45. Myrmekite formed by Na- and Ca-metasomatism of K- feldspar Jiashu RONG Beijing Research Institute of Uranium Geology P.O. Box 9818, Beijing, 100029 Peoples Republic of China Email address: [email protected] September 23, 2002 Abstract Myrmekite, an intergrowth of plagioclase and quartz vermicules, often occurs in felsic-to-intermediate, calc-alkalic plutonic and gneissic rocks. Several hypotheses for myrmekite genesis are briefly reviewed and discussed. The proportional relationship between the volume of quartz vermicules and the An value of plagioclase is consistent with the hypothesis or replacement, solid state exsolution, and recrystallization of primary plagioclase. (1) Perthitic albite and K- feldspar relicts in myrmekite and (2) swapped myrmekite between two differently oriented K-feldspar crystals obviously indicate that myrmekite is formed by nibble replacement of K-feldspar by myrmekitic plagioclase because of modification by Ca-bearing sodic emanation or fluid. Myrmekite of different morphology and spatial distribution are of the same metasomatic origin. The myrmekite that was produced during deformation should be later than that formed prior to deformation. Characteristics of myrmekite Myrmekite was first described by Michel-Lévy (1874) and named by Sederholm (1897) as an intergrowth of plagioclase and quartz vermicules. Myrmekite is commonly observed in felsic-to-intermediate calc-alkalic granitic rocks (but not in alkalic-tending plutonic rocks) and in granitic gneisses of similar composition. 2 On the basis of the geologic environment, Phillips (1974) classified myrmekite in the following ways: 1. rim myrmekite, occurring at the contact of plagioclase with another differently oriented K-feldspar; 2. intergranular myrmekite, situated at the boundary between two differently oriented K-feldspars; 3. -
Hydrogeologic Applications for Historical Records and Images from Rock Samples Collected at the Nevada National Security Site An
A. 1,461 ft 1,600 ft 2,004.5 ft Lithology interpreted by Richard G. Warren, Comprehensive Volcanic Petrographics, LLC 2,204 ft Figure 3. Representation of rock column derived from lithologic records (A) compared with core samples and thin sections thin-section images (B–E) from the UE-19p borehole. B. Adularia (AA) – Orthoclase (a K-spar polymorph typical of granite), that has formed under hydrothermal rather than magmatic conditions. Image from 2,204 ft at 30 degrees polarization. Acmite (AC) – A Na- and Fe3-rich pyroxene typically found as a Allanite (AL) – An epidote-group mineral containing high contents groundmass phase within devitrified peralkaline rock. Image from of rare-earth elements, found in alkali-calcic volcanic rocks. Image 2,004.5 ft at 90 degrees polarization. from 1,600 ft at 30 degrees polarization. C. Biotite (BT) – A hydrated mafic mineral typical of evolved volcanic rocks. Generally lacking in peralkaline units. Image from 1,461 ft at 90 degrees polarization. Glass (GL) – Typically Ca- and Fe-poor, compositionally at the “granite eutectic” within rhyolitic rocks such as those dominant within the Southwestern Nevada Volcanic Field (SWNVF). Unpolarized image from 1,461 ft. Clinopyroxene (CX) – A Ca-rich pyroxene and anhydrous mafic mineral found in a wide variety of volcanic rocks. Image from 1,461 ft at 30 degrees polarization. D. K-feldspar (KF) – A felsic phenocryst ubiquitous as sanidine within the SWNVF, except absent within the wahmonie Formation. Image from 2,004.5 ft at 30 degrees polarization. Lithic (LI) – A rock fragment incorporated into tuff during eruption, Perrierite/Chevkinite (PE) – A pseudobrookite-group mineral usually from the vent. -
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. -
Pamphlet to Accompany Scientific Investigations Map 3131
Bedrock Geologic Map of the Seward Peninsula, Alaska, and Accompanying Conodont Data By Alison B. Till, Julie A. Dumoulin, Melanie B. Werdon, and Heather A. Bleick Pamphlet to accompany Scientific Investigations Map 3131 View of Salmon Lake and the eastern Kigluaik Mountains, central Seward Peninsula 2011 U.S. Department of the Interior U.S. Geological Survey Contents Introduction ....................................................................................................................................................1 Sources of data ....................................................................................................................................1 Components of the map and accompanying materials .................................................................1 Geologic Summary ........................................................................................................................................1 Major geologic components ..............................................................................................................1 York terrane ..................................................................................................................................2 Grantley Harbor Fault Zone and contact between the York terrane and the Nome Complex ..........................................................................................................................3 Nome Complex ............................................................................................................................3 -
Introduction to Igneous Petrology
Cambridge University Press 978-1-107-02754-1 - Essentials of Igneous and Metamorphic Petrology B. Ronald Frost and Carol D. Frost Excerpt More information Chapter 1 Introduction to Igneous Petrology 1.1 Introduction Igneous petrology is the study of magma and the rocks that solidify from magma. Th us igneous petrologists are concerned with the entire spectrum of processes that describe how magmas are produced and how they ascend through the mantle and crust, their mineralogical and geochemical evolution, and their eruption or emplacement to form igneous rocks. Igneous petrology requires a working knowledge of mineralogy. Readers who wish to review the characteristics of the major rock-forming igneous minerals will fi nd a concise sum- mary in Appendix 1. Th e appendix emphasizes the identifi cation of rock-forming minerals in hand sample and in thin section. In addition, the appendix includes descriptions of minerals found in minor abundance but commonly occurring in igneous rocks, including accessory minerals that contain trace amounts of uranium and are important geochronometers. Before geologists can understand the origin of igneous rocks, they must classify and describe them. Th is chapter introduces the classifi cation of igneous rocks using the mineralogical classifi cation system recom- mended by the International Union of Geological Sciences (IUGS) Subcommission on the Systematics of Igneous Rocks, which has the advantage that it is relatively simple and can be applied in the fi eld. For rocks that are too fi ne-grained to name using this classifi cation, a geochemical classifi cation can be employed instead. Th e simplest of these, the total alkali versus silica classifi cation, is introduced in this text. -
A POST IMPACT VOLCANISM SCENARIO for the FORMATION of the OLIVINE-RICH UNIT in the REGION of NILI FOSSAE, MARS. L. Mandon1, C. Q
49th Lunar and Planetary Science Conference 2018 (LPI Contrib. No. 2083) 1473.pdf A POST IMPACT VOLCANISM SCENARIO FOR THE FORMATION OF THE OLIVINE - RICH UNIT IN THE REGION OF NILI FOSSAE, MARS. L. Mandon 1 , C. Quantin 1 , P. Thollot 1 , L. Lozac’h 1 , N. Mangold 2 , G. Dromart 1 , P. Beck 3 , E. Dehouck 1 , S. Breton 1 , C. Millot 1 . 1 Laboratoire de Géologie de Lyon Terre, Planètes, Environnement , Université de Lyon, France. 2 Laboratoire de Planétologie et Géodynamique , Université de Nantes, France. 3 Institut de Planétologie et d'Astrophysique de Gre- noble , Université Grenoble Alpes, France. lucia.ma ndon@univ - lyon1.fr. Introduction: The Nili Fossae region exhibits the gets using MarsSI. We used HRSC DTMs computed largest Martian exposures of olivine - rich materials, as by the Fr eie Universitaet Berlin and DLR Berlin . deduced from orbital near - infrared and thermal spec- Strikes and dips measurements were performed using troscopy [1, 2] . Several hypotheses have been pro- the ArcGIS extension LayerTools [7]. Finally, we posed to explain the origin of a widespread olivine - rich performed crater size analyses on both small (~1 km²) formati on in the region: (1) these materials might be and wide (~900 km²) olivine - rich areas. Using the crustal rocks excavated by the giant impact leading to Craterstats software [8], we compared size distribu- the formation of Isidis Planitia [2], a 1200 km wide tions to isochrons generated by the Ivanov production impact basin east of Nili Fossae. (2) They could result function to estimate a surface age [9]. from mafic effusive lava flows occurring befo re [3] or Results: At HiRISE resolution, the unit appears after [4] the giant impact. -
Mineralogy and Petrology of the Santo Tomas-Black Mountain Basalt Field, Potrillo Volcanics, South-Central New Mexico
JERRY M. HOFFER Department of Geological Sciences, The University of Texas at El Paso, El Paso, Texas 79900 Mineralogy and Petrology of the Santo Tomas-Black Mountain Basalt Field, Potrillo Volcanics, South-Central New Mexico ABSTRACT called the Santo Tomas-Black Mountain basalt field (Hoffer, 1969c). The Santo Tomas-Black Mountain basalts The Santo Tomas-Black Mountain basalt were erupted during the Quaternary from field includes four major centers, each with four centers. Six lava flows are present at one or more cones and associated flows Black Mountain, three at Santo Tomas, and (Hoffer, 1969a). From north to south, the one each at Little Black Mountain and San four volcanic centers are Santo Tomas, San Miguel. The basalts are grouped into three Miguel, Little Black Mountain, and Black major types of phenocryst mineralogy: (l) Mountain. The largest volume of lava has plagioclase abundant, (2) olivine abundant, been extruded from the Black Mountain and and (3) both olivine and plagioclase abundant. Santo Tomas centers where six and three All three types are alkali-olivine basalts, individual flows, respectively, have been showing high alkali-silica ratios and total mapped (Hoffer, 1969a). Each of the two alkali content increasing with silica. intervening centers, Little Black Mountain Seven periods of basaltic extrusion among and San Miguel, shows only a single flow. the centers have been established on the No flow from a given center coalesces with basis of field evidence, phenocryst mineralogy, those from neighboring centers, but all ap- and pyroxene-olivine ratios. K-Ar dates show pear to be closely related in time (Kottlowski, the basalts to be less than 0.3 X 106 m.y. -
Structural Geology of the Upper Rock Creek Area, Inyo County, California, and Its Relation to the Regional Structure of the Sierra Nevada
Structural geology of the upper Rock Creek area, Inyo County, California, and its relation to the regional structure of the Sierra Nevada Item Type text; Dissertation-Reproduction (electronic); maps Authors Trent, D. D. Publisher The University of Arizona. Rights Copyright © is held by the author. Digital access to this material is made possible by the University Libraries, University of Arizona. Further transmission, reproduction or presentation (such as public display or performance) of protected items is prohibited except with permission of the author. Download date 27/09/2021 06:38:23 Link to Item http://hdl.handle.net/10150/565293 STRUCTURAL GEOLOGY OF THE UPPER ROCK CREEK AREA, INYO COUNTY, CALIFORNIA, AND ITS RELATION TO THE REGIONAL STRUCTURE OF THE SIERRA NEVADA by Dee Dexter Trent A Dissertation Submitted to the Faculty of the DEPARTMENT OF GEOSCIENCES In Partial Fulfillment of the Requirements For the Degree of DOCTOR OF PHILOSOPHY In the Graduate College THE UNIVERSITY OF ARIZONA 1 9 7 3 THE UNIVERSITY OF ARIZONA GRADUATE COLLEGE I hereby recommend that this dissertation prepared under my direction by __________ Dee Dexter Trent______________________ entitled Structural Geology of the Upper Rock Creek Area . Tnvo County, California, and Its Relation to the Regional Structure of the Sierra Nevada ________________ be accepted as fulfilling the dissertation requirement of the degree of ____________Doctor of Philosophy_________ ___________ P). /in /'-/7. 3 Dissertation Director fJ Date After inspection of the final copy of the dissertation, the following members of the Final Examination Committee concur in its approval and recommend its acceptance:* f t M m /q 2 g ££2 3 This approval and acceptance is contingent on the candidate's adequate performance and defense of this dissertation at the final oral examination. -
Economic Geology Report ER79-4: Porphyritic Intrusions and Related
MANITOBA CANADA DEPARTMENT OF ENERGY AND MINES MANITOBA MINERAL RESOURCES DIVISION ECONOMIC GEOLOGY REPORT ER79-4 PORPHYRITIC INTRUSIONS AND RELATED MINERALIZATION IN THE FLIN FLON VOLCANIC BELT by D.A. BALDWIN 1980 Funding for this project was provided under the cost-shared Canada-Manitoba Non-renewable Resources Evaluation Program by the Canada Department of Energy, Mines and Resources and the Manitoba Department of Mines, Resources and Environmental Management. MANITOBA DEPARTMENT OF ENERGY AND MINES HON. DONALD W. CRAIK PAUL E. JARVIS Minister Deputy Minister MINERAL RESOURCES DIVISION IAN HAUGH Executive Director ECONOMIC GEOLOGY REPORT ER79-4 PORPHYRITIC INTRUSIONS AND RELATED MINERALIZATION IN THE FLIN FLON VOLCANIC BELT by D.A. BALDWIN 1980 LEGEND I Cliff Lake Stock 5 Elbow Lake Stock 2 Whitefish Lake Porphyry 6 Fourmile Island Intrusion 3 Alberts Lake Intrusion 7 Chisel Lake Intrusion 4 Nisto Lake Intrusion 8 Wekusko Lake Intrusion ,~ -./ - -, I \." ~herridon '" , ;. <,.... ,1 if 55°00' 55°00' c, t,:) ,J -3 , I"" . c;? '" 1[' . ::t} \'''If!? ~,/J~ /j' ., ~), F lin.~ i;\))F ' I,".!0l~' ,d ' ;)/", ' ~.;'. l ;' ~" ,r~n ;t j; (I:/,1 ,r Lake ' \\ ;\~ ' ~i'/ 'lUi':;- -'i' //{ ,'/ , ,\" ,,/,1,1 pI , .h .(,1;' '\:. (IiI' ' .. '~'4_hl i / 'Y{j,'{:" 5 2.5 a 10 15 KILOMETRES J!) "'.t3 f3,F-"\ ---- :i~ f)J~c~. V 99°30' ">/)AfhapaplJskoj¥ !ZJ Porphyritic Intrusive Rocks 54°30' ! ,1 Lake .; ... 100°30' D Felsic Volcanic Rocks FIGURE 1: Distribution of porphyritic intrusive and felsic volcanic rocks in the Flin Flon volcanic belt, TABLE OF -
Nanomaterials How to Analyze Nanomaterials Using Powder Diffraction and the Powder Diffraction File™
Nanomaterials How to analyze nanomaterials using powder diffraction and the Powder Diffraction File™ Cerium Oxide CeO2 PDF 00-064-0737 7,000 6,000 5,000 4,000 Intensity 3,000 2,000 1,000 20 30 40 50 60 70 80 90 100 110 120 Nanomaterials Table of Contents Materials with new and incredible properties are being produced around the world by controlled design at the atomic and molecular level. These nanomaterials are typically About the Powder Diffraction File ......... 1 produced in the 1-100 nm size scale, and with this small size they have tremendous About Powder Diffraction ...................... 1 surface area and corresponding relative percent levels of surface atoms. Both the size and available (reactive) surface area can contribute to unique physical properties, Analysis Tools for Nanomaterials .......... 1 such as optical transparency, high dissolution rate, and enormous strength. Crystallite Size and Particle Size ������������ 2 In this Technical Bulletin, we are primarily focused on the use of structural simulations XRPD Pattern for NaCI – An Example .... 2 in order to examine the approximate crystallite size and molecular orientation in nanomaterials. The emphasis will be on X-ray analysis of nanomaterials. However, Total Pattern Analysis and the �������������� 3 Powder Diffraction File electrons and neutrons can have similar wavelengths as X-rays, and all of the X-ray methods described have analogs with neutron and electron diffraction. The use of Pair Distribution Function Analysis ........ 3 simulations allows one to study any nanomaterials that have a known atomic and Amorphous Materials ............................ 4 molecular structure or one can use a characteristic and reproducible experimental diffraction pattern. -
Module 7 Igneous Rocks IGNEOUS ROCKS
Module 7 Igneous Rocks IGNEOUS ROCKS ▪ Igneous Rocks form by crystallization of molten rock material IGNEOUS ROCKS ▪ Igneous Rocks form by crystallization of molten rock material ▪ Molten rock material below Earth’s surface is called magma ▪ Molten rock material erupted above Earth’s surface is called lava ▪ The name changes because the composition of the molten material changes as it is erupted due to escape of volatile gases Rocks Cycle Consolidation Crystallization Rock Forming Minerals 1200ºC Olivine High Ca-rich Pyroxene Ca-Na-rich Amphibole Intermediate Na-Ca-rich Continuous branch Continuous Discontinuous branch Discontinuous Biotite Na-rich Plagioclase feldspar of liquid increases liquid of 2 Temperature decreases Temperature SiO Low K-feldspar Muscovite Quartz 700ºC BOWEN’S REACTION SERIES Rock Forming Minerals Olivine Ca-rich Pyroxene Ca-Na-rich Amphibole Na-Ca-rich Continuous branch Continuous Discontinuous branch Discontinuous Biotite Na-rich Plagioclase feldspar K-feldspar Muscovite Quartz BOWEN’S REACTION SERIES Rock Forming Minerals High Temperature Mineral Suite Olivine • Isolated Tetrahedra Structure • Iron, magnesium, silicon, oxygen • Bowen’s Discontinuous Series Augite • Single Chain Structure (Pyroxene) • Iron, magnesium, calcium, silicon, aluminium, oxygen • Bowen’s Discontinuos Series Calcium Feldspar • Framework Silicate Structure (Plagioclase) • Calcium, silicon, aluminium, oxygen • Bowen’s Continuous Series Rock Forming Minerals Intermediate Temperature Mineral Suite Hornblende • Double Chain Structure (Amphibole) -
Mid-Infrared Optical Constants of Clinopyroxene and Orthoclase Derived from Oriented Single-Crystal Reflectance Spectra
American Mineralogist, Volume 99, pages 1942–1955, 2014 Mid-infrared optical constants of clinopyroxene and orthoclase derived from oriented single-crystal reflectance spectra JESSICA A. ARNOLD1,*, TIMOTHY D. GLOTCH1 AND ANNA M. PLONKA1 1Department of Geosciences, Stony Brook University, Stony Brook, New York 11794, U.S.A. ABSTRACT We have determined the mid-IR optical constants of one alkali feldspar and four pyroxene compo- sitions in the range of 250–4000 cm–1. Measured reflectance spectra of oriented single crystals were iteratively fit to modeled spectra derived from classical dispersion analysis. We present the real and imaginary indices of refraction (n and k) along with the oscillator parameters with which they were modeled. While materials of orthorhombic symmetry and higher are well covered by the current literature, optical constants have been derived for only a handful of geologically relevant monoclinic materials, including gypsum and orthoclase. Two input parameters that go into radiative transfer models, the scattering phase function and the single scattering albedo, are functions of a material’s optical constants. Pyroxene is a common rock-forming mineral group in terrestrial bodies as well as meteorites and is also detected in cosmic dust. Hence, having a set of pyroxene optical constants will provide additional details about the composition of Solar System bodies and circumstellar materials. We follow the method of Mayerhöfer et al. (2010), which is based on the Berreman 4 × 4 matrix formulation. This approach provides a consistent way to calculate the reflectance coefficients in low- symmetry cases. Additionally, while many models assume normal incidence to simplify the dispersion relations, this more general model applies to reflectance spectra collected at non-normal incidence.