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Accretion of Water in Carbonaceous Chondrites: Current Evidence and Implications for the Delivery of Water to Early Earth
ACCRETION OF WATER IN CARBONACEOUS CHONDRITES: CURRENT EVIDENCE AND IMPLICATIONS FOR THE DELIVERY OF WATER TO EARLY EARTH Josep M. Trigo-Rodríguez1,2, Albert Rimola3, Safoura Tanbakouei1,3, Victoria Cabedo Soto1,3, and Martin Lee4 1 Institute of Space Sciences (CSIC), Campus UAB, Facultat de Ciències, Torre C5-parell-2ª, 08193 Bellaterra, Barcelona, Catalonia, Spain. E-mail: [email protected] 2 Institut d’Estudis Espacials de Catalunya (IEEC), Edif.. Nexus, c/Gran Capità, 2-4, 08034 Barcelona, Catalonia, Spain 3 Departament de Química, Universitat Autònoma de Barcelona, 08193 Bellaterra, Catalonia, Spain. E-mail: [email protected] 4 School of Geographical and Earth Sciences, University of Glasgow, Gregory Building, Lilybank Gardens, Glasgow G12 8QQ, UK. Manuscript Pages: 37 Tables: 2 Figures: 10 Keywords: comet; asteroid; meteoroid; meteorite; minor bodies; primitive; tensile strength Accepted in Space Science Reviews (SPAC-D-18-00036R3, Vol. Ices in the Solar System) DOI: 10.1007/s11214-019-0583-0 Abstract: Protoplanetary disks are dust-rich structures around young stars. The crystalline and amorphous materials contained within these disks are variably thermally processed and accreted to make bodies of a wide range of sizes and compositions, depending on the heliocentric distance of formation. The chondritic meteorites are fragments of relatively small and undifferentiated bodies, and the minerals that they contain carry chemical signatures providing information about the early environment available for planetesimal formation. A current hot topic of debate is the delivery of volatiles to terrestrial planets, understanding that they were built from planetesimals formed under far more reducing conditions than the primordial carbonaceous chondritic bodies. -
A New Occurrence of Terrestrial Native Iron in the Earth's Surface
geosciences Article A New Occurrence of Terrestrial Native Iron in the Earth’s Surface: The Ilia Thermogenic Travertine Case, Northwestern Euboea, Greece Christos Kanellopoulos 1,2,* ID , Eugenia Valsami-Jones 3,4, Panagiotis Voudouris 1, Christina Stouraiti 1 ID , Robert Moritz 2, Constantinos Mavrogonatos 1 ID and Panagiotis Mitropoulos 1,† 1 Department of Geology and Geoenvironment, National and Kapodistrian University of Athens, Panepistimioupolis Zografou, 15784 Athens, Greece; [email protected] (P.V.); [email protected] (C.S.); [email protected] (C.M.); [email protected] (P.M.) 2 Section of Earth and Environmental Sciences, University of Geneva, Rue des Maraichers 13, 1205 Geneva, Switzerland; [email protected] 3 School of Geography, Earth & Environmental Sciences, University of Birmingham, Edgbaston, Birmingham B15 2TT, UK; [email protected] 4 Department of Earth Sciences, Natural History Museum London, Cromwell Road, London SW7 5BD, UK * Correspondence: [email protected] † Professor Panagiotis Mitropoulos has passed away in 2017. Received: 6 April 2018; Accepted: 23 July 2018; Published: 31 July 2018 Abstract: Native iron has been identified in an active thermogenic travertine deposit, located at Ilia area (Euboea Island, Greece). The deposit is forming around a hot spring, which is part of a large active metallogenetic hydrothermal system depositing ore-bearing travertines. The native iron occurs in two shapes: nodules with diameter 0.4 and 0.45 cm, and angular grains with length up to tens of µm. The travertine laminae around the spherical/ovoid nodules grow smoothly, and the angular grains are trapped inside the pores of the travertine. -
MACKINAWITE from SOUTH AFRICA W. C J. Van RDNSBU*.O, Geological Surtey Oj Soulh Africa, Preloria, Soulh A.[Ri Co, L. Lrbnunsbyc
TI.IE AMERICAN MINERALOGIST, VOL 52, JULY AUGUST, 1967 MACKINAWITE FROM SOUTH AFRICA W. C J. vAN RDNSBU*.o,Geological Surtey oJ Soulh Africa, Preloria,Soulh A.[rico, AND L. LrBnuNsByc, Deparlment of Geology,Llnit:ersity of Pretoria, Pre!oria,Soul h Africa. ABSTRAcT Mackinawite has been identified in mafic and ultramafic rocks of the Bushveld igneous complex and Insizwa and also in the carbonatite and pegmatoid of Loolekop, Phalaborrva complex in South Africa. The mineral occurs predominantly as somewhat irregular to oriented intergrowths in pentlandite in all these occurrences and less commonly as regular oriented lamellae in chalcopyrite and rarely in cubanite. The textural evidence suggests that mackinawite may represent an exsolution product of pentlandite, chalcopyrite and cubanite. INrnonucrroN The iron sulphide, mackinawite was recently named in a paper by Evans, et al, (1964). Natural occurrencesof this mineral f rom Finland were describedby- Kouvo et al (1963)and from the Muskox intrusion in Canada by Chamberlain and Delabio (1965). During the presentinvestigation mackinawite was distinguishedfrom valleriite in the carbonatite and pegmatoid of Loolekop, Phalaborwa complex, in the Bushveld igneous complex, and from Insizwa, Cape Province.The mode of occurrenceof the mackinawite in the carbonatite difiers somewhatfrom that in the mafic rocks of Insizwa and the Bush- veld complex. MrNnn.q.rocv The physicaland optical propertiesof mackinawitefrom the Bushveid complex,Insizwa and Loolekop are very similar and are in closeagree- ment with the propertiesgiven for the same mineral from the Muskox intrusion by Chamberlain and Delabio (1965). The mineral takes a fairly good polish,particularly after buffing with a chromic oxide slurry. -
Moon Minerals a Visual Guide
Moon Minerals a visual guide A.G. Tindle and M. Anand Preliminaries Section 1 Preface Virtual microscope work at the Open University began in 1993 meteorites, Martian meteorites and most recently over 500 virtual and has culminated in the on-line collection of over 1000 microscopes of Apollo samples. samples available via the virtual microscope website (here). Early days were spent using LEGO robots to automate a rotating microscope stage thanks to the efforts of our colleague Peter Whalley (now deceased). This automation speeded up image capture and allowed us to take the thousands of photographs needed to make sizeable (Earth-based) virtual microscope collections. Virtual microscope methods are ideal for bringing rare and often unique samples to a wide audience so we were not surprised when 10 years ago we were approached by the UK Science and Technology Facilities Council who asked us to prepare a virtual collection of the 12 Moon rocks they loaned out to schools and universities. This would turn out to be one of many collections built using extra-terrestrial material. The major part of our extra-terrestrial work is web-based and we The authors - Mahesh Anand (left) and Andy Tindle (middle) with colleague have build collections of Europlanet meteorites, UK and Irish Peter Whalley (right). Thank you Peter for your pioneering contribution to the Virtual Microscope project. We could not have produced this book without your earlier efforts. 2 Moon Minerals is our latest output. We see it as a companion volume to Moon Rocks. Members of staff -
Magnetite Biomineralization and Ancient Life on Mars Richard B Frankel* and Peter R Buseckt
Magnetite biomineralization and ancient life on Mars Richard B Frankel* and Peter R Buseckt Certain chemical and mineral features of the Martian meteorite with a mass distribution unlike terrestrial PAHs or those from ALH84001 were reported in 1996 to be probable evidence of other meteorites; thirdly, bacterium-shaped objects (BSOs) ancient life on Mars. In spite of new observations and up to several hundred nanometers long that resemble fos interpretations, the question of ancient life on Mars remains silized terrestrial microorganisms; and lastly, 10-100 nm unresolved. Putative biogenic, nanometer magnetite has now magnetite (Fe304), pyrrhotite (Fel_xS), and greigite (Fe3S4) become a leading focus in the debate. crystals. These minerals were cited as evidence because of their similarity to biogenic magnetic minerals in terrestrial Addresses magnetotactic bacteria. *Department of Physics, California Polytechnic State University, San Luis Obispo, California 93407, USA; e-mail: [email protected] The ancient life on Mars hypothesis has been extensively tDepartments of Geology and Chemistry/Biochemistry, Arizona State challenged, and alternative non-biological processes have University, Tempe, Arizona 85287-1404, USA; e-mail: [email protected] been proposed for each of the four features cited by McKay et al. [4]. In this paper we review the current situa tion regarding their proposed evidence, focusing on the Abbreviations putative biogenic magnetite crystals. BCM biologically controlled mineralization BIM biologically induced mineralization BSO bacterium-shaped object Evidence for and against ancient Martian life PAH polycyclic aromatic hydrocarbon PAHs and BSOs Reports of contamination by terrestrial organic materials [5°,6°] and the similarity of ALH84001 PAHs to non-bio genic PAHs in carbonaceous chondrites [7,8] make it Introduction difficult to positively identify PAHs of non-terrestrial, bio A 2 kg carbonaceous stony meteorite, designated genic origin. -
Arsenian Sphalerite from Mina Ai,Caran, Pampa Larga
MINERALOGICAL NOTES AMERICAN MINERALOGIST, \IOL. 55, SEPTEMBER.OCTOBER, 1970 ARSENIANSPHALERITE FROM MINA AI,CARAN, PAMPALARGA, COPIAPO, CHILE Arew H. Cr-anr, Department oJ GeologicalSciences, Queen's Uniaersity, Kingston, Ontario, Canado. ABSTRACT Bright pink sphalerite from the arsenic-rich Alacr6n deposit, with a:5.4110 +0.0003 A, is shown by electron-probe microanalysis to contain only traces of iron but 17 +0.3 weight percent As INrnooucrroN The literature containsnumerous reports of appreciablesolid solution of arsenicin sphalerite(e.g. Schroll, 1953; Fleischer,1955), but the an- alytical evidenceremains largeiy unconvincing.Moss (1955;and in Hey, 1955,Frondel, 1967)proposed that the mineral voltzite has the general composition (Zn,As)S or Zn(As,S), but Frondel (1967) subsequently found no evidenceto support this suggestion.Most recent electron- probe microanalysesof sphaleritedo not record even traces of arsentc. Ilowever, Herzenberg(1932,1933) found 0.64 weight percentarsenic by chemical analysisof a raspberry-redsphalerite-like mineral from Llall- agua, Bolivia, which he named gumuc'ionite.Later workers (e.g.Hey, 1955)have assumedthat this material representsa mixture of sphalerite and realgarbut no further work appearsto have been carried out on the original or similar specimens.The presentnote describesthe occurrence of an apparently similar, and demonstrably arsenic-bearingsphalerite. Spner-Bnrrr rN rHE Ar,acnAN DBposrr Sphalerite is a minor constituent of the mineralogically complex, polymetallic Alacr6n vein deposit (Parker, Salas and P6rez, 1963),in the Pampa Larga mining district of northern Chile (Lat. 27"36'5.;Long. 70'11'W.). It occurs, however, in at least three parageneticcontexts: (1) in associationwith early arsenopyrite, pyrite, stibnite, smithite, aAsS (Clark, 1970a)and arsenolamprite(Clark, 1970b), among other minerals; (2) with late-stagegreigite, pyrite, native arsenic,realgar, and orpiment;and (3) rarely, as free-standingcrystals in vugs, in association with realgar and orpiment. -
Using the High-Temperature Phase Transition of Iron Sulfide Minerals As
www.nature.com/scientificreports OPEN Using the high-temperature phase transition of iron sulfde minerals as an indicator of fault Received: 9 November 2018 Accepted: 15 May 2019 slip temperature Published: xx xx xxxx Yan-Hong Chen1, Yen-Hua Chen1, Wen-Dung Hsu2, Yin-Chia Chang2, Hwo-Shuenn Sheu3, Jey-Jau Lee3 & Shih-Kang Lin2 The transformation of pyrite into pyrrhotite above 500 °C was observed in the Chelungpu fault zone, which formed as a result of the 1999 Chi-Chi earthquake in Taiwan. Similarly, pyrite transformation to pyrrhotite at approximately 640 °C was observed during the Tohoku earthquake in Japan. In this study, we investigated the high-temperature phase-transition of iron sulfde minerals (greigite) under anaerobic conditions. We simulated mineral phase transformations during fault movement with the aim of determining the temperature of fault slip. The techniques used in this study included thermogravimetry and diferential thermal analysis (TG/DTA) and in situ X-ray difraction (XRD). We found diversifcation between 520 °C and 630 °C in the TG/DTA curves that signifes the transformation of pyrite into pyrrhotite. Furthermore, the in situ XRD results confrmed the sequence in which greigite underwent phase transitions to gradually transform into pyrite and pyrrhotite at approximately 320 °C. Greigite completely changed into pyrite and pyrrhotite at 450 °C. Finally, pyrite was completely transformed into pyrrhotite at 580 °C. Our results reveal the temperature and sequence in which the phase transitions of greigite occur, and indicate that this may be used to constrain the temperature of fault-slip. This conclusion is supported by feld observations made following the Tohoku and Chi-Chi earthquakes. -
Bulk Mineralogical Changes of Hydrous Micrometeorites During Heating in the Upper Atmosphere at Temperatures Below 1000 °C
Bulk mineralogical changes of hydrous micrometeorites during heating in the upper atmosphere at temperatures below 1000 °C Item Type Article; text Authors Nozaki, Wataru; Nakamura, Tomoki; Noguchi, Takaaki Citation Nozaki, W., Nakamura, T., & Noguchi, T. (2006). Bulk mineralogical changes of hydrous micrometeorites during heating in the upper atmosphere at temperatures below 1000 °C. Meteoritics & Planetary Science, 41(7), 1095-1114. DOI 10.1111/j.1945-5100.2006.tb00507.x Publisher The Meteoritical Society Journal Meteoritics & Planetary Science Rights Copyright © The Meteoritical Society Download date 06/10/2021 08:34:17 Item License http://rightsstatements.org/vocab/InC/1.0/ Version Final published version Link to Item http://hdl.handle.net/10150/656158 Meteoritics & Planetary Science 41, Nr 7, 1095–1114 (2006) Abstract available online at http://meteoritics.org Bulk mineralogical changes of hydrous micrometeorites during heating in the upper atmosphere at temperatures below 1000 °C Wataru NOZAKI1, Tomoki NAKAMURA1*, and Takaaki NOGUCHI2 1Department of Earth and Planetary Sciences, Faculty of Science, Kyushu University 33, Hakozaki, Fukuoka 812-8581, Japan 2Materials and Biological Science, Faculty of Science, Ibaraki University, Bunkyo, Mito 310-8512, Japan *Corresponding author. E-mail: [email protected] (Received 04 August 2005; revision accepted 25 April 2006) Abstract–Small particles 200 μm in diameter from the hydrous carbonaceous chondrites Orgueil CI, Murchison CM2, and Tagish Lake were experimentally heated for short durations at subsolidus temperatures under controlled ambient pressures in order to examine the bulk mineralogical changes of hydrous micrometeorites during atmospheric entry. The three primitive meteorites consist mainly of various phyllosilicates and carbonates that are subject to decomposition at low temperatures, and thus the brief heating up to 1000 °C drastically changed the mineralogy. -
ANHYDROUS SYNTHESIS of GREIGITE. Fe3s4
MINERALOGICAL JOURNAL, VOL. 6, No. 6, pp. 458-463, APRIL 1972 ANHYDROUS SYNTHESIS OF GREIGITE. Fe3S4 HIROMOTO NAKAZAWA and KouSUKE SAKAGUCHI National Institute for Researches in Inorganic Materials, Kurakake, Sakura-mura, Niihari-gun, Ibaragi, Japan ABSTRACT The vacuum evaporation method has been applied for preparation of low-temperature phases of iron sulfides. Thin films were synthesized from natural pyrrhotite crystals on cleaved halite crystals heated at different temperatures. The films have been identified by the electron diffraction method to be greigite, Fe3S4. Presence of a small amount of marcasite has been also confirmed in the films prepared on halite crystals at room tem perature. Introduction The phase relations of the iron-sulfur system were recently studied below 320•Ž in detail (Morimoto et al., 1970; Nakazawa & Morimoto, 1971). However, the relations have not been completely settled at relatively low temperatures, because the reaction rate was very slow in the usual dry synthesis of the iron sulfides stable in nature. In order to study the phase relations in more details, it is indispensable to produce low temperature phases under known conditions and to examine their properties. For the preparation of the low-temperature phases in dry condition, the vacuum evapora tion method was considered to be useful, because the evaporated atoms or molecules were considered to deposit on the substrate of low temperatures and crystallize into low-temperature phases. In this investigation, greigite and marcasite have been success- fully synthesized by vacuum evaporation technique as examples of H. NAKAZAWA and K . SAKAGUCHI 459 dry synthesis of low-temperature phases of the iron -sulfur system . -
Characterisation of Iron (II) Sulfides in Wet Archaeological Woods: The
Characterisation of iron (II) sulfides in wet archaeological woods: the wreck of Mandirac (IV th century, antique ports of Narbonne, France) Céline Remazeilles, Francois Leveque, Maylis Minjacq, Philippe Refait, Corinne Sanchez, Marie-Pierre Jézégou To cite this version: Céline Remazeilles, Francois Leveque, Maylis Minjacq, Philippe Refait, Corinne Sanchez, et al.. Char- acterisation of iron (II) sulfides in wet archaeological woods: the wreck of Mandirac (IV th century, antique ports of Narbonne, France). WOAM 2016, May 2016, Florence, Italy. hal-02345869 HAL Id: hal-02345869 https://hal-univ-rochelle.archives-ouvertes.fr/hal-02345869 Submitted on 4 Nov 2019 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. Characterisation of iron (II) sulfides in wet archaeological woods: the wreck of Mandirac (IVth century, antique ports of Narbonne, France) Céline Rémazeillesa*, François Lévêqueb, Maylis Minjacqab, Philippe Refaita, Corinne Sanchezc, Marie-Pierre Jézégoud aLaSIE, Laboratory of Engineering Sciences for the Environment UMR 7356 CNRS/University of La Rochelle [email protected] bLIENSs, Littoral, Environment and Societies UMR 7266 CNRS/University of La Rochelle cASM, Archaeology of Mediterranean Societies UMR-5140 CNRS/University of Montpellier Ministry of Culture and Communication/INRAP, French National Institute for Preventive Archaeological Research dDRASSM, Department for Underwater and Undersea Archaeological Research Abstract The wreck of Mandirac (Narbonne, France, IV century) was excavated in 2013 and 2014 from waterlogged soil. -
Iron Sulfides from Magnetotactic Bacteria: Structure, Composition
American Mineralogist, Volume 83, pages 1469-1481, 1998 Iron sulfidesfrom magnetotacticbacteria: Structure, composition, and phasetransitions Mrnfu,v PosrlIr''x Pprnn R. Busrcrrl DENNTsA. BlzyLrNSKrr2aNo RrcnlRD B. FnaNrrl3 lDepaftmentsof Geology and Chemistry/Biochemistry,Arizona State University, Tempe,Arizona 85287, U.S.A. '?Departmentof Microbiology, Immunology and PreventiveMedicine, Iowa State University, Ames, Iowa 50011, U.S.A. rDepartmentof Physics,Californa Polytechnic State University, San Luis Obispo, California 93407, U.S A. AesrRAcr Using transmissionelectron microscopy, we studied the structuresand compositionsof Fe sulfides within cells of magnetotacticbacteria that were collected from natural habitats. Ferrimagnetic greigite (Fe.S.) occurred in all types of sulfide-producing magnetotactic bacteriaexamined. Mackinawite (tetragonalFeS) and, tentatively, sphalerite-typecubic FeS were also identified. In contrastto earlier reports,we did not find pyrite (FeSr)or pyrrhotite (Fe, ,S). Mackinawite converted to greigite over time within the bacteria that were de- posited on electron microscope grids and stored in air. Orientation relationshipsbetween the two minerals indicate that the cubic-close-packedS substructureremains unchanged during the transformation; only the Fe atoms rearrange. Neither mackinawite nor cubic FeS are magnetic, and yet they are aligned in chains such that when convertedto magnetic greigite, the probable easy axis of magnetization, [100], is parallel to the chain direction. The resulting chains of greigite -
Synthesis and Rietveld Crystal Structure Refinement of Mackinawite, Tetragonal Fes
Synthesis and Rietveld crystal structure refinement of mackinawite, tetragonal FeS A. R. LENN1E*, S. A. T. REDFERN1", P. F. SCHOF1ELD :~ AND D. J. VAUGHAN* * Department of Earth Sciences, The University of Manchester, Oxford Road, Manchester, M13 9PL, UK 1Department of Earth Sciences, University of Cambridge, Downing Street, Cambridge, CB2 3EQ, UK ~tDepartment of Mineralogy, The Natural History Museum, Cromwell Road, London, SW7 5BD, UK Abstract Mackinawite, tetragonal FeS, has been synthesised by reacting iron with Na2S solutions. A Rietveld structure refinement of X-ray powder diffraction data, recorded using X-rays monochromated from synchrotron radiation with a wavelength of 0.6023 A, has been performed. The structure has been refined in the tetragonal s~ace group, P4/nmm, and has the following cell parameters: a = 3.6735(4), c = 5.0328(7) A, V = 67.914(24) A 3. Our refinement shows that the FeS4 tetrahedron in mackinawite is almost perfectly regular, with a much smaller distortion than has been previously reported. An improved X-ray diffraction data set is provided. I~Ywo~s: mackinawite, Rietveld structure refinement, synthesis. Introduction tetrahedra which are stacked normal to the c-axis, with only weak van der Waals forces holding these THE mineral mackinawite, first described by Evans et sheets together. Mackinawite has been reported as al. (1962, 1964), is identical to synthetic tetragonal both a metal-excess (Clark, 1966) and a sulphur iron monosulphide (Berner, 1962, 1964), an unnamed deficient (Taylor and Finger, 1970) phase. tetragonal iron sulphide mineral (Kuovo et al., 1963) Tetragonal Fel+xSe and Fel+xTe, which share the and the synthetic iron sulphide 'kansite' (Meyer et anti-litharge structure found in mackinawite, are al., 1958).