Deep Sea Drilling Project Initial Reports Volume 14
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Phyllosilicate Minerals in the Hydrothermal Mafic–Ultramafic-Hosted Massive-Sulfide Deposit of Ivanovka
Contrib Mineral Petrol (2004) 147: 363–383 DOI 10.1007/s00410-004-0565-3 ORIGINAL PAPER Paolo Nimis Æ Svetlana G. Tesalina Æ Paolo Omenetto Paola Tartarotti Æ Catherine Lerouge Phyllosilicate minerals in the hydrothermal mafic–ultramafic-hosted massive-sulfide deposit of Ivanovka (southern Urals): comparison with modern ocean seafloor analogues Received: 15 August 2003 / Accepted: 9 February 2004 / Published online: 17 March 2004 Ó Springer-Verlag 2004 Abstract We have studied textural relationships and required a high contribution of Mg-rich seawater to the compositions of phyllosilicate minerals in the mafic– hydrothermal fluid, which could be achieved in a highly ultramafic-hosted massive-sulfide deposit of Ivanovka permeable, breccia-dominated seafloor. More evolved (Main Uralian Fault Zone, southern Urals). The main hydrothermal fluids produced addition of silica, car- hydrothermal phyllosilicate minerals are Mg-rich chlo- bonates and further sulfides, and led to local develop- rite, variably ferroan talc, (Mg, Si)-rich and (Ca, Na, ment of saponite after chlorite and widespread K)-poor saponite (stevensite), and serpentine. These replacement of serpentine by talc. The Ivanovka deposit minerals occur both as alteration products after mafic shows many similarities with active and fossil hydro- volcanics and ultramafic protoliths and, except serpen- thermal sites on some modern oceanic spreading centers tine, as hydrothermal vein and seafloor mound-like characterized by highly permeable upflow zones. How- precipitates associated with variable amounts of (Ca, ever, given the arc signature of the ore host rocks, the Mg, Fe)-carbonates, quartz and Fe and Cu (Co, Ni) most probable setting for the observed alteration–min- sulfides. -
Characterization of Clays and Clay Minerals for Industrial Applications: Substitution Non-Natural Additives by Clays in UV Protection
Characterization of Clays and Clay Minerals for Industrial Applications: Substitution non-Natural Additives by Clays in UV Protection Dissertation in fulfilment of the academic grade doctor rerum naturalium (Dr. rer. nat.) at the Faculty of Mathematics and Natural Sciences Ernst-Moritz-Arndt-University Greifswald HOANG-MINH Thao (Hoàng Thị Minh Thảo) born on 01.6.1979 in Quang Ninh, Vietnam Greifswald, Germany - 2006 Dekan: Prof. Dr. Klaus Fesser 1. Gutachter: PD. Dr. habil. Jörn Kasbohm 2. Gutachter: Prof. Roland Pusch Tag der Promotion: 17.11.2006 ii CONTENTS LIST OF TABLES . vi LIST OF FIGURES. vii ABBREVIATIONS . x STATEMENT OF ORIGINAL AUTHORSHIP (ERKLÄRUNG). xi ACKNOWLEDGMENTS . xii 1 INTRODUCTION . 1 2 POSSIBLE FUNCTIONS OF CLAYS, CLAY MINERALS IN UV PROTECTION . 2 2.1 Clays, clay minerals and sustainability in geosciences. 2 2.2 Ultraviolet radiation and human skin . 2 2.3 Actual substances as UV protection factor and their problems. 5 2.4 Pharmacy requirement in suncreams. 9 2.5 Clays, clay minerals and their application for human health. 11 2.6 Possible functions of clays, clay minerals in UV protection cream. 13 3 METHODOLOGY . 15 3.1 Clays and clay minerals analyses. 15 3.1.1 X-Ray diffraction. 17 3.1.2 TEM-EDX. 19 3.1.3 X-Ray fluorescence. 22 3.1.4 Mössbauer spectroscopy. 23 3.1.5 Atterberg sedimentation. 23 3.1.6 Dithionite treatment. 24 3.2 Non-clay samples analyses. 24 3.2.1 UV-measurement. 25 3.2.2 Light microscopy. 27 3.2.3 Skin model test by mouse-ear in vivo . -
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 -
Ferric Saponite and Serpentine in the Nakhlite Martian Meteorites
Available online at www.sciencedirect.com ScienceDirect Geochimica et Cosmochimica Acta 136 (2014) 194–210 www.elsevier.com/locate/gca Ferric saponite and serpentine in the nakhlite martian meteorites L.J. Hicks a, J.C. Bridges a,⇑, S.J. Gurman b a Space Research Centre, Dept. of Physics & Astronomy, University of Leicester, Leicester LE1 7RH, UK b Dept. of Physics & Astronomy, University of Leicester, Leicester LE1 7RH, UK Received 29 October 2013; accepted in revised form 7 April 2014; available online 18 April 2014 Abstract Transmission electron microscopy and Fe-K X-ray absorption spectroscopy have been used to determine structure and ferric content of the secondary phase mineral assemblages in the nakhlite martian meteorites, NWA 998, Lafayette, Nakhla, GV, Y 000593, Y 000749, MIL 03346, NWA 817, and NWA 5790. The secondary phases are a rapidly cooled, metastable assemblage that has preserved Mg# and Ca fractionation related to distance from the fluid source, for most of the nakhlites, though one, NWA 5790, appears not to have experienced a fluid pathway. All nine nakhlite samples have also been analysed with scanning electron microscopy, electron probe micro analysis, Bright Field high-resolution transmission electron microscopy (HRTEM) and selected area electron diffraction. By measuring the energy position of the Fe-K XANES 1s ! 3d pre-edge transition centroid we calculate the ferric content of the minerals within the nakhlite meteorites. The crystalline phyllosilicates and amorphous silicate of the hydrothermal deposits filling the olivine fractures are found to have variable Fe3+/RFe values ranging from 0.4 to 0.9. In Lafayette, the central silicate gel parts of the veins are more ferric than the phyllosilicates around it, showing that the fluid became increasingly oxidised. -
HIGH TEMPERATURE PHASES in SEPIOLITB, ATTAPULGITE and SAPONITE Gnoncrs Kulnrcrr,* Departmentof Geology, Uniters'ityof Lllinois, Urbana,Illinois
THE AMERICAN MINERALOGIST, VOL 44, JULY_AUGUST, 1959 HIGH TEMPERATURE PHASES IN SEPIOLITB, ATTAPULGITE AND SAPONITE Gnoncrs Kulnrcrr,* Departmentof Geology, Uniters'ityof lllinois, Urbana,Illinois. AssrnA.cr The high temperature reactions of sepiolite, attapulgite and saponite were studied by continuous high temperatute rc-ray diffraction techniques. The easy formation of enstatite from the fibrous minerals is explained by structural analogy. The reactions of the well crystallized specimens of sepiolite and attapulgite difier somewhat from those of their massive sedimentary varieties. The difierences cannot be ex- plained with the chemical and structural data, suggesting possible variations in some inti- mate details of the framework of these two varieties. INrnooucuox The nature of the crystalline phases formed by firing the magnesian clay mineralshas beendescribed (2,3,7, I0, 12,15, 16),but only for the well crystallized chlorites (3) have the precise conditions of formation of these phases as well as their structural relationships with the starting material been clearly determined. The three minerals chosenfor this investigation provide difierent struc- tural arrangementsof the same type of lattice in a series of Al-Mg hydrous silicates.Saponite and sepiolite have the same bulk composi- tion but they difier in the mode of assemblage,i.e. layers or ribbons, of their structural units. Attapulgite has the same kind of framework as sepiolite, but a large proportion of magnesium has been replaced by aluminum or iron. It was thought that, by taking advantage of these features and by using a method of continuous high-tempetature x-ray diffraction analysis,a new contribution to the problem would be possible. -
Hectorite: Synthesis, Modification, Assembly and Applications Jing Zhang, Chun Hui Zhou, Sabine Petit, Hao Zhang
Hectorite: Synthesis, modification, assembly and applications Jing Zhang, Chun Hui Zhou, Sabine Petit, Hao Zhang To cite this version: Jing Zhang, Chun Hui Zhou, Sabine Petit, Hao Zhang. Hectorite: Synthesis, modification, assembly and applications. Applied Clay Science, Elsevier, 2019, 177, pp.114-138. 10.1016/j.clay.2019.05.001. hal-02363196 HAL Id: hal-02363196 https://hal-cnrs.archives-ouvertes.fr/hal-02363196 Submitted on 2 Dec 2020 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. 1 Hectorite:Synthesis, Modification, Assembly and Applications 2 3 Jing Zhanga, Chun Hui Zhoua,b,c*, Sabine Petitd, Hao Zhanga 4 5 a Research Group for Advanced Materials & Sustainable Catalysis (AMSC), State Key Laboratory 6 Breeding Base of Green Chemistry-Synthesis Technology, College of Chemical Engineering, Zhejiang 7 University of Technology, Hangzhou 310032, China 8 b Key Laboratory of Clay Minerals of Ministry of Land and Resources of the People's Republic of 9 China, Engineering Research Center of Non-metallic Minerals of Zhejiang Province, Zhejiang Institute 10 of Geology and Mineral Resource, Hangzhou 310007, China 11 c Qing Yang Institute for Industrial Minerals, You Hua, Qing Yang, Chi Zhou 242804, China 12 d Institut de Chimie des Milieux et Matériaux de Poitiers (IC2MP), UMR 7285 CNRS, Université de 13 Poitiers, Poitiers Cedex 9, France 14 15 Correspondence to: Prof. -
The Nature of Laponite: Pure Hectorite Or a Mixture of Different Trioctahedral Phases?
minerals Article The Nature of Laponite: Pure Hectorite or a Mixture of Different Trioctahedral Phases? George E. Christidis 1,*, Carlos Aldana 2, Georgios D. Chryssikos 3, Vassilis Gionis 3, Hussein Kalo 4 ID , Matthias Stöter 5, Josef Breu 5 and Jean-Louis Robert 6,† 1 School of Mineral Resources Engineering, Technical University of Crete, 73100 Chania, Greece 2 Institut des Sciences de la Terre d’Orléans, CNRS, 1A Rue de la Ferollerie, 45100 Orléans, France; [email protected] 3 Theoretical and Physical Chemistry Institute, National Hellenic Research Foundation, 48 Vass. Constantinou Ave., 11635 Athens, Greece; [email protected] (G.D.C.); [email protected] (V.G.) 4 BYK-Chemie GmbH, Stadtwaldstrasse 44, 85368 Moosburg, Germany; [email protected] 5 Lehrstuhl für Anorganische Chimie I, Universität Bayreuth, 95440 Bayreuth, Germany; [email protected] (M.S.); [email protected] (J.B.) 6 IMPMC, Sorbonne Universités, UMR 7590, UPMC, CNRS, MNHN, IRD, 4 Place Jussieu, CEDEX 05, 75231 Paris, France; [email protected] * Correspondence: [email protected] † Deceased. Received: 30 June 2018; Accepted: 24 July 2018; Published: 26 July 2018 Abstract: A series of laponites and synthetic OH- and fluorinated hectorites prepared from hydrothermal and melting experiments at both industrial and laboratory scale were examined with XRD and FTIR (MIR and NIR) to determine their mineralogical composition and possible compositional heterogeneity. The end materials contained both Li- and Na-bearing phases. The industrial hydrothermal OH-smectites prepared at low temperatures consist of random mixed layer hectorite-stevensite-kerolite with about 40–50% hectorite layers, the remaining being stevensite and kerolite at roughly equal proportions. -
AP42 Section: Reference: Title: 11.25 Clays, S. H. Patterson and H. H
AP42 Section: 11.25 Reference: ~ Title: Clays, S. H. Patterson and H. H. Murray, Industrial Minerals And Rocks, Volume 1, Society Of Mining Engineers, New York, 1983. The term clay is somewhat ambiguous un- less specifically defined, because it is used in three ways: (I) as a diverse group of fine- grained minerals, (2) a5 a rock term, and (3) as a particle-size term. Actually, most persons using the term clay realize that it has several meanings, and in most instances they define it. As a rock term, clay is difficult to define be- cause of the wide variety of materials that com- ,me it; therefore, the definition must be gen- 'eral. Clay is a natural earthy, fine-grained ma- Iterial composed largely of a group of crystalline ;minerals known as the clay minerals. These minerals are hydrous silicates composed mainly of silica, alumina, and water. Several of these minerals also contain appreciable quantities of iron, alkalies, and alkaline earths. Many defini- tions state that a clay is plastic when wet. Most clay materials do have this property, but some clays are not plastic; for exaniple, halloysite and flint clay. As a particle-size term, clay is used for the category that includes the smallest particles. The maximum-size particles in the clay-size grade are defined differently on various grade scales. Soil imestigators and mineralogists gen- erally use 2 micrometers as the maximum size, whereas the widely used scale by Wentworth (1922) defines clay as material finer than ap proximately 4 micrometers. Some authorities find it convenient to'use the term clay'for any fine-grained, natural, earthy, argillaceous material (Grim. -
Nontronite Is a Smectire Group Clay Mineral Which. Ff,T'lffi'"Fff"#:J""
The American Mineralogist, Yolume60, pages 840448, 1975 Primary NontroniteFrom the VenezuelanGuayana W. C. ISpHoRpllrC Department of Geology and Geography, Uniuersity of South Alabama Mobile, Alabama 36688 Abstract Nontronite, the iron-rich end member of SmectiteGroup clays, has previouslybeen reported as a hydrothermalalteration product, as a constituentof soil clays formed by weatheringof a variety of rock types,and as an alterationproduct of volcanicrocks. This paper describesthe chemical,optical, and X-ray propertiesof a new occurrenceof the mineralwhere its origin is apparentlyrelated to directcrystallization from high temperature waters.The mineral is further unique in that it containsonly a very small percentageof aluminaand therebyclosely approaches the previouslyunreported wholly iron end-member. Significantdifferences were found in the optical propertiesof the Venezuelannontronit€ when comparedwith those of an earlier study, especiallywith regard to the variation in refractiveindex with Fe2Oscontent. It now appearsthat this variationhas been over-simpli- fied and may not be as orderlyas was previouslybelieved. The variouslines of evidencethat argue againstan origin by either hydrothermalalteration or chemicalweathering are dis- cussed,as well as thosesupporting an origin by direct crystallizationfrom high temperature watersof probablemagmatic or metamorphicorigin. lntroduction product in gneissesand slates.At the other sites,non- Nontroniteisa Smectire Group clay mineral which. ff,T'Lffi'"fff"#:j""1|# ,XXT::""."t1:j'# occurs as the iron-rich end-memberin the d.ioc- rr-;i",;-be an arterationproduct. At the type tahedral sub-group montmorillonite-beidellite- io.uri,v,Nontron, France, Berthier (1g27) descri6ed nontroniteseries' It haspreviously been *p":l:9^:t^1 ,tr" ri".r"r-: as occurringas "onion-like" massesas- constituentof sedimentaryrocks, as the productof -:-,--; -,,, alterationorvolcanic grasses andas a hydrother.mal alterationproduct. -
Bio-Preservation Potential of Sediment in Eberswalde Crater, Mars
Western Washington University Western CEDAR WWU Graduate School Collection WWU Graduate and Undergraduate Scholarship Fall 2020 Bio-preservation Potential of Sediment in Eberswalde crater, Mars Cory Hughes Western Washington University, [email protected] Follow this and additional works at: https://cedar.wwu.edu/wwuet Part of the Geology Commons Recommended Citation Hughes, Cory, "Bio-preservation Potential of Sediment in Eberswalde crater, Mars" (2020). WWU Graduate School Collection. 992. https://cedar.wwu.edu/wwuet/992 This Masters Thesis is brought to you for free and open access by the WWU Graduate and Undergraduate Scholarship at Western CEDAR. It has been accepted for inclusion in WWU Graduate School Collection by an authorized administrator of Western CEDAR. For more information, please contact [email protected]. Bio-preservation Potential of Sediment in Eberswalde crater, Mars By Cory M. Hughes Accepted in Partial Completion of the Requirements for the Degree Master of Science ADVISORY COMMITTEE Dr. Melissa Rice, Chair Dr. Charles Barnhart Dr. Brady Foreman Dr. Allison Pfeiffer GRADUATE SCHOOL David L. Patrick, Dean Master’s Thesis In presenting this thesis in partial fulfillment of the requirements for a master’s degree at Western Washington University, I grant to Western Washington University the non-exclusive royalty-free right to archive, reproduce, distribute, and display the thesis in any and all forms, including electronic format, via any digital library mechanisms maintained by WWU. I represent and warrant this is my original work, and does not infringe or violate any rights of others. I warrant that I have obtained written permissions from the owner of any third party copyrighted material included in these files. -
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INFORMATION TO USERS This manuscript has been reproduced from the microfilm master. UMI films the tact directly from the original or copy submitted. Thus, some thesis and dissertation copies are in typewriter free, while others may be from any type o f computer printer. The quality of this reproduction is dependent upon the quality of the copy submitted. Broken or indistinct print, colored or poor quality illustrations and photographs, print bleedthrough, substandard margins, and improper alignment can adversely affect reproduction. In the unlikely event that the author did not send UMI a complete manuscript and there are missing pages, these will be noted. Also, if unauthorized copyright material had to be removed, a note will indicate the deletion. Oversize materials (e.g., maps, drawings, charts) are reproduced by sectioning the original, beginning at the upper left-hand comer and continuing from left to right in equal sections with small overlaps. Each original is also photographed in one ocposure and is included in reduced form at the back of the book. Photographs included in the original manuscript have been reproduced xerographically in this copy. Higher quality 6” x 9” black and white photographic prints are available for any photographs or illustrations appearing in this copy for an additional charge. Contact UMI directly to order. UMI A Bell & Howell Information Company 300 North Zeeb Road, Arm Arbor MI 48106-1346 USA 313/761-4700 800/521-0600 A MECHANISTIC STUDY OF SORPTION OF IONIC ORGANIC COMPOUNDS ON PHYLLOSILICATES DISSERTATION Presented in Partial Fulfillment of the Requirements for the Degree Doctor of Philosophy in the Graduate School of The Ohio State University By Sandip Chattopadhyay ***** The Ohio State University 1997 Dissertation Committee: Approved by Dr. -
The History of Water on Mars: Hydrated Minerals As a Water Sink in the Martian Crust
Ninth International Conference on Mars 2019 (LPI Contrib. No. 2089) 6065.pdf THE HISTORY OF WATER ON MARS: HYDRATED MINERALS AS A WATER SINK IN THE MARTIAN CRUST. L. J. Wernicke1,2 and B. M. Jakosky1,3, 1Laboratory for Atmospheric and Space Physics, University of Colorado Boulder. [email protected]. [email protected]. Introduction: The ancient landscape of Mars pro- example calculation. Nontronite’s empirical formula vides morphological and mineralogical evidence that and all other values used in the example calculation can significant amounts of liquid water once flowed on its be found in Table 1. Nontronite has 6 oxygen atoms surface. Previous research has identified the amount of from water and hydroxyl, which comprises 19.36% of water stored in the polar caps and in high latitude sub- its molecular mass. The oxygen mass/thickness of surface ice [1]. The amount of water lost to space has nontronite is: also been constrained [2]. But how much water is stored (0.1936)*(2300 kg/m3)*(1.449×1014 m2) in Martian rocks? 16 =6.45×10 kg/m Chemical alteration hydrates Martian minerals, stor- 3+ ing water within Martian rocks. A large variety of hy- Nontronite - Na0.3Fe 2Si3AlO10(OH)2•4(H2O) drated minerals have been detected on the surface of Molecular mass (kg) 0.4959 Mars [3,4], and a significant abundance of hydrated minerals has been detected inside Martian craters [5,6]. Oxygen from water 19.36% We use published surveys of the global distribution and Density (kg/m3) 2300 abundance of hydrated minerals to calculate the total Surface area of Mars (m2) 1.449×1014 volume of water stored in hydrated minerals within the Oxygen Mass/thick (kg/m) 6.45×1016 Martian crust.