Geological Mapping and Characterization of Possible Primary Input Materials for the Mineral Sequestration of Carbon Dioxide in Europe
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Metamorphism of Sedimentary Manganese Deposits
Acta Mineralogica-Petrographica, Szeged, XX/2, 325—336, 1972. METAMORPHISM OF SEDIMENTARY MANGANESE DEPOSITS SUPRIYA ROY ABSTRACT: Metamorphosed sedimentary deposits of manganese occur extensively in India, Brazil, U. S. A., Australia, New Zealand, U. S. S. R., West and South West Africa, Madagascar and Japan. Different mineral-assemblages have been recorded from these deposits which may be classi- fied into oxide, carbonate, silicate and silicate-carbonate formations. The oxide formations are represented by lower oxides (braunite, bixbyite, hollandite, hausmannite, jacobsite, vredenburgite •etc.), the carbonate formations by rhodochrosite, kutnahorite, manganoan calcite etc., the silicate formations by spessartite, rhodonite, manganiferous amphiboles and pyroxenes, manganophyllite, piedmontite etc. and the silicate-carbonate formations by rhodochrosite, rhodonite, tephroite, spessartite etc. Pétrographie and phase-equilibia data indicate that the original bulk composition in the sediments, the reactions during metamorphism (contact and regional and the variations and effect of 02, C02, etc. with rise of temperature, control the mineralogy of the metamorphosed manga- nese formations. The general trend of formation and transformation of mineral phases in oxide, carbonate, silicate and silicate-carbonate formations during regional and contact metamorphism has, thus, been established. Sedimentary manganese formations, later modified by regional or contact metamorphism, have been reported from different parts of the world. The most important among such deposits occur in India, Brazil, U.S.A., U.S.S.R., Ghana, South and South West Africa, Madagascar, Australia, New Zealand, Great Britain, Japan etc. An attempt will be made to summarize the pertinent data on these metamorphosed sedimentary formations so as to establish the role of original bulk composition of the sediments, transformation and reaction of phases at ele- vated temperature and varying oxygen and carbon dioxide fugacities in determin- ing the mineral assemblages in these deposits. -
The Forsterite-Anorthite-Albite System at 5 Kb Pressure Kristen Rahilly
The Forsterite-Anorthite-Albite System at 5 kb Pressure Kristen Rahilly Submitted to the Department of Geosciences of Smith College in partial fulfillment of the requirements for the degree of Bachelor of Arts John B. Brady, Honors Project Advisor Acknowledgements First I would like to thank my advisor John Brady, who patiently taught me all of the experimental techniques for this project. His dedication to advising me through this thesis and throughout my years at Smith has made me strive to be a better geologist. I would like to thank Tony Morse at the University of Massachusetts at Amherst for providing all of the feldspar samples and for his advice on this project. Thank you also to Michael Jercinovic over at UMass for his help with last-minute carbon coating. This project had a number of facets and I got assistance from many different departments at Smith. A big thank you to Greg Young and Dale Renfrow in the Center for Design and Fabrication for patiently helping me prepare and repair the materials needed for experiments. I’m also grateful to Dick Briggs and Judith Wopereis in the Biology Department for all of their help with the SEM and carbon coater. Also, the Engineering Department kindly lent their copy of LabView software for this project. I appreciated the advice from Mike Vollinger within the Geosciences Department as well as his dedication to driving my last three samples over to UMass to be carbon coated. The Smith Tomlinson Fund provided financial support. Finally, I need to thank my family for their support and encouragement as well as my friends here at Smith for keeping this year fun and for keeping me balanced. -
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. -
Washington State Minerals Checklist
Division of Geology and Earth Resources MS 47007; Olympia, WA 98504-7007 Washington State 360-902-1450; 360-902-1785 fax E-mail: [email protected] Website: http://www.dnr.wa.gov/geology Minerals Checklist Note: Mineral names in parentheses are the preferred species names. Compiled by Raymond Lasmanis o Acanthite o Arsenopalladinite o Bustamite o Clinohumite o Enstatite o Harmotome o Actinolite o Arsenopyrite o Bytownite o Clinoptilolite o Epidesmine (Stilbite) o Hastingsite o Adularia o Arsenosulvanite (Plagioclase) o Clinozoisite o Epidote o Hausmannite (Orthoclase) o Arsenpolybasite o Cairngorm (Quartz) o Cobaltite o Epistilbite o Hedenbergite o Aegirine o Astrophyllite o Calamine o Cochromite o Epsomite o Hedleyite o Aenigmatite o Atacamite (Hemimorphite) o Coffinite o Erionite o Hematite o Aeschynite o Atokite o Calaverite o Columbite o Erythrite o Hemimorphite o Agardite-Y o Augite o Calciohilairite (Ferrocolumbite) o Euchroite o Hercynite o Agate (Quartz) o Aurostibite o Calcite, see also o Conichalcite o Euxenite o Hessite o Aguilarite o Austinite Manganocalcite o Connellite o Euxenite-Y o Heulandite o Aktashite o Onyx o Copiapite o o Autunite o Fairchildite Hexahydrite o Alabandite o Caledonite o Copper o o Awaruite o Famatinite Hibschite o Albite o Cancrinite o Copper-zinc o o Axinite group o Fayalite Hillebrandite o Algodonite o Carnelian (Quartz) o Coquandite o o Azurite o Feldspar group Hisingerite o Allanite o Cassiterite o Cordierite o o Barite o Ferberite Hongshiite o Allanite-Ce o Catapleiite o Corrensite o o Bastnäsite -
Mineral Processing
Mineral Processing Foundations of theory and practice of minerallurgy 1st English edition JAN DRZYMALA, C. Eng., Ph.D., D.Sc. Member of the Polish Mineral Processing Society Wroclaw University of Technology 2007 Translation: J. Drzymala, A. Swatek Reviewer: A. Luszczkiewicz Published as supplied by the author ©Copyright by Jan Drzymala, Wroclaw 2007 Computer typesetting: Danuta Szyszka Cover design: Danuta Szyszka Cover photo: Sebastian Bożek Oficyna Wydawnicza Politechniki Wrocławskiej Wybrzeze Wyspianskiego 27 50-370 Wroclaw Any part of this publication can be used in any form by any means provided that the usage is acknowledged by the citation: Drzymala, J., Mineral Processing, Foundations of theory and practice of minerallurgy, Oficyna Wydawnicza PWr., 2007, www.ig.pwr.wroc.pl/minproc ISBN 978-83-7493-362-9 Contents Introduction ....................................................................................................................9 Part I Introduction to mineral processing .....................................................................13 1. From the Big Bang to mineral processing................................................................14 1.1. The formation of matter ...................................................................................14 1.2. Elementary particles.........................................................................................16 1.3. Molecules .........................................................................................................18 1.4. Solids................................................................................................................19 -
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. -
The Forsterite-Tephroite Series:I
American Mineralogist, Volume 65, pages 1263-1269, 1980 The forsterite-tephroite series:I. Crystal structure refinements Cenr A. FReNcIs Mineralogical Museum,Hamard University Cambridge,M assachusetts02 I 38 AND PAUL H. RIBBE Department of Geological Sciences Virginia Polytechnic Institute and State University B lac ksbur g, Virginia 2 4 06 I Abstract The crystal structures of the following metamorphic olivines, M;*[SiO4], in the forsterite- tephroite (Fo-Te) serieswere refned in space group Pbnm: Cation compositionM Cell parameters(A) Mg Mn Ca Fe a b c Rfactor Fol 1.028 0964 0.006 0.002 4.794 10.491 6.t23 0.029 Ten, 0.181 1.780 0.013 0.026 4.879 10.589 6.234 0.039 Treating minql ps and Ca as though they were Mn, the refined cation distributions (esds < 0.01) and mean bond lengths are: M(1) site M(2) site Mg Mn (M(lFo) Mg Mn (M(2)-o) (si-o) For, 0.92 0.08 2.116I^ 0.1I 0.89 2.185A r.6374 Te", O.l7 0.83 2.0294 0.00 1.00 2.2274 l.6,t0A By comparison, a previously refned synthetic ForrT€o, specimen "heat-treated at l(X)0oC" is significantlymore disordered(KD : 0.196)than the naturally occurring For' (Ko: 0.011). As expected,mean M(l)-O and M(2)-O distancescorrelate linearly with Mgl(Mg+Mn) oc- cupancy. Introduction However, the crystal structures of only two Mg- With the widespread availability of automated X- Mn olivines have previously been refined. One of ray di-ffractometeruand least-squaresrefinement pro- them contains I I mole percent of Zn SiOo, thereby grams, order-disorder has become a principal theme complicating the octahedral site refinement (Brown, of contemporary crystal chemical investigations 1970). -
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) -
Volcanism on Mars
Author's personal copy Chapter 41 Volcanism on Mars James R. Zimbelman Center for Earth and Planetary Studies, National Air and Space Museum, Smithsonian Institution, Washington, DC, USA William Brent Garry and Jacob Elvin Bleacher Sciences and Exploration Directorate, Code 600, NASA Goddard Space Flight Center, Greenbelt, MD, USA David A. Crown Planetary Science Institute, Tucson, AZ, USA Chapter Outline 1. Introduction 717 7. Volcanic Plains 724 2. Background 718 8. Medusae Fossae Formation 725 3. Large Central Volcanoes 720 9. Compositional Constraints 726 4. Paterae and Tholi 721 10. Volcanic History of Mars 727 5. Hellas Highland Volcanoes 722 11. Future Studies 728 6. Small Constructs 723 Further Reading 728 GLOSSARY shield volcano A broad volcanic construct consisting of a multitude of individual lava flows. Flank slopes are typically w5, or less AMAZONIAN The youngest geologic time period on Mars identi- than half as steep as the flanks on a typical composite volcano. fied through geologic mapping of superposition relations and the SNC meteorites A group of igneous meteorites that originated on areal density of impact craters. Mars, as indicated by a relatively young age for most of these caldera An irregular collapse feature formed over the evacuated meteorites, but most importantly because gases trapped within magma chamber within a volcano, which includes the potential glassy parts of the meteorite are identical to the atmosphere of for a significant role for explosive volcanism. Mars. The abbreviation is derived from the names of the three central volcano Edifice created by the emplacement of volcanic meteorites that define major subdivisions identified within the materials from a centralized source vent rather than from along a group: S, Shergotty; N, Nakhla; C, Chassigny. -
Tourmaline Reference Materials for the in Situ Analysis of Oxygen and Lithium Isotope Ratio Compositions
Vol. 45 — N° 1 03 P.97 – 119 21 Tourmaline Reference Materials for the In Situ Analysis of Oxygen and Lithium Isotope Ratio Compositions Michael Wiedenbeck (1)*, Robert B. Trumbull (1), Martin Rosner (2),AdrianBoyce (3), John H. Fournelle (4),IanA.Franchi (5),RalfHalama (6),ChrisHarris (7),JackH.Lacey (8), Horst Marschall (9) , Anette Meixner (10),AndreasPack (11), Philip A.E. Pogge von Strandmann (9), Michael J. Spicuzza (4),JohnW.Valley (4) and Franziska D.H. Wilke (1) (1) GFZ German Research Centre for Geosciences, Potsdam 14473, Germany (2) Department of Marine Chemistry and Geochemistry, Woods Hole Oceanographic Institution, Woods Hole, MA, 02543, USA (3) Scottish Universities Environmental Research Centre, East Kilbride G75 0QF, UK (4) Department of Geoscience, University of Wisconsin, Madison, WI, 53706, USA (5) School of Physical Sciences, Open University, Milton Keynes MK7 6AA, UK (6) Department of Geology, University of Maryland, College Park, MD, 20742, USA (7) Department of Geological Sciences, University of Cape Town, Rondebosch 7701, South Africa (8) National Environmental Isotope Facility, British Geological Survey, Keyworth NG12 5GG, UK (9) Bristol Isotope Group, School of Earth Sciences, University of Bristol, Bristol BS8 1RJ, UK (10) Faculty of Geosciences & MARUM – Center for Marine Environmental Sciences, University of Bremen, Bremen 28359, Germany (11) Geowissenschaftliches Zentrum, Universitat¨ Gottingen,¨ Gottingen¨ 37077, Germany (12) Present address: IsoAnalysis UG, Berlin 12489, Germany (13) Present address: School of Geography, Geology and Environment, Keele University, Keele ST5 5BG, UK (14) Present address: Institut fur¨ Geowissenschaften, Goethe-Universitat,¨ Frankfurt am Main 60438, Germany (15) Present address: Institute of Earth and Planetary Sciences, University College London and Birkbeck, University of London, London WC1E 6BS, UK * Corresponding author. -
IDENTIFYING TWO DISTINCT OLIVINE COMPOSITIONS in TYRRHENA TERRA and LIBYA MONTES, MARS. M. D. Lane1, J. L. Bishop2, D. Loizeau3, D
52nd Lunar and Planetary Science Conference 2021 (LPI Contrib. No. 2548) 2550.pdf IDENTIFYING TWO DISTINCT OLIVINE COMPOSITIONS IN TYRRHENA TERRA AND LIBYA MONTES, MARS. M. D. Lane1, J. L. Bishop2, D. Loizeau3, D. Tirsch4, L. L. Tornabene5, L. Sacks5, C. Viviano6, J. R. C. Voigt7 1Fibernetics LLC, Lititz, PA ([email protected]), 2Carl Sagan Center, SETI Institute, Mountain View, CA, 3IAS, Université-Sud, Orsay, France, 4Institute of Planetary Research, German Aerospace Center (DLR), Ber- lin, Germany, 5Dept. of Earth Sciences, Institute for Earth and Space Exploration, University of Western Ontario, London, Canada, 6Johns Hopkins University Applied Physics Lab (JHUAPL), Laurel, MD, 7Lunar and Planetary Labora- tory, University of Arizona, Tucson, AZ. Introduction: Olivine is present across Terra Tyr- rhena (TT) and in the southern rim of the Isidis basin Figure 2. Ther- in the Libya Montes (LM) region. Using both near-IR mal emissivity Compact Reconnaissance Imaging Spectrometer for Mars spectra of syn- (CRISM) and mid-IR Thermal Emission Spectrometer thetic Mg-Fe oli- (TES) data to characterize our study site (Fig. 1), the vines. The dots strongest olivine signatures across TT are identified in represent the flec- isolated crater floor deposits, while the olivine in the tion points for LM area is associated with a stratigraphic unit con- each composi- sistent with an airfall ash deposit [2]. Using mid-IR tion. These points spectral indices developed from synthetic olivine data and the bands to [3] for 13 different olivine compositions in the forster- each side migrate ite (Fo100) to fayalite (Fo0) solid solution series (Fig. with changes in 2), specific Mg-Fe olivine compositions were deter- chemistry. -
Mineral Collecting Sites in North Carolina by W
.'.' .., Mineral Collecting Sites in North Carolina By W. F. Wilson and B. J. McKenzie RUTILE GUMMITE IN GARNET RUBY CORUNDUM GOLD TORBERNITE GARNET IN MICA ANATASE RUTILE AJTUNITE AND TORBERNITE THULITE AND PYRITE MONAZITE EMERALD CUPRITE SMOKY QUARTZ ZIRCON TORBERNITE ~/ UBRAR'l USE ONLV ,~O NOT REMOVE. fROM LIBRARY N. C. GEOLOGICAL SUHVEY Information Circular 24 Mineral Collecting Sites in North Carolina By W. F. Wilson and B. J. McKenzie Raleigh 1978 Second Printing 1980. Additional copies of this publication may be obtained from: North CarOlina Department of Natural Resources and Community Development Geological Survey Section P. O. Box 27687 ~ Raleigh. N. C. 27611 1823 --~- GEOLOGICAL SURVEY SECTION The Geological Survey Section shall, by law"...make such exami nation, survey, and mapping of the geology, mineralogy, and topo graphy of the state, including their industrial and economic utilization as it may consider necessary." In carrying out its duties under this law, the section promotes the wise conservation and use of mineral resources by industry, commerce, agriculture, and other governmental agencies for the general welfare of the citizens of North Carolina. The Section conducts a number of basic and applied research projects in environmental resource planning, mineral resource explora tion, mineral statistics, and systematic geologic mapping. Services constitute a major portion ofthe Sections's activities and include identi fying rock and mineral samples submitted by the citizens of the state and providing consulting services and specially prepared reports to other agencies that require geological information. The Geological Survey Section publishes results of research in a series of Bulletins, Economic Papers, Information Circulars, Educa tional Series, Geologic Maps, and Special Publications.