Rates and Mechanisms of Mineral Carbonation in Peridotite: Natural Processes and Recipes for Enhanced, in Situ CO2 Capture and Storage
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Characterization of Sulfide Minerals from Gabbroic and Ultramafic Rocks by Electron Microscopy1 D.J
Blackman, D.K., Ildefonse, B., John, B.E., Ohara, Y., Miller, D.J., MacLeod, C.J., and the Expedition 304/305 Scientists Proceedings of the Integrated Ocean Drilling Program, Volume 304/305 Data report: characterization of sulfide minerals from gabbroic and ultramafic rocks by electron microscopy1 D.J. Miller,2 T. Eisenbach,2 and Z.P. Luo3 Chapter contents Abstract Abstract . 1 This objective of this research was to investigate the potential of using transmission electron microscopy (TEM) to determine sul- Introduction . 1 fide mineral speciation in gabbroic rocks from Atlantis Massif, the Geologic background . 2 site of Integrated Ocean Drilling Program Expedition 304/305. Method development . 2 The method takes advantage of TEM analysis techniques and Results . 2 proved successful in sulfide mineral identification. TEM can pro- Discussion . 3 vide imaging of the sample morphology, crystal structure through Acknowledgments. 4 the electron diffraction, and chemical compositional information References . 4 through X-ray energy dispersive spectroscopy. Electron probe mi- Figures . 5 croanalysis was also used to determine the chemical composition. Table . 11 Introduction Integrated Ocean Drilling Program (IODP) Expedition 304/305 at Atlantis Massif, 30°N on the Mid-Atlantic Ridge (MAR) (Fig. F1) comprised a coordinated, dual-expedition drilling program aimed at investigating oceanic core complex (OCC) formation and the exposure of ultramafic rocks in young oceanic lithosphere. One of the scientific objectives of this drilling program is to investigate the role of magmatism in the development of OCCs. Whereas precruise submersible and geophysical surveys suggested the po- tential of recovering substantial amounts of serpentinized perido- tite and possibly fresh residual mantle, coring on the central dome of the massif returned a 1.4 km thick section of plutonic mafic rock with only a thin (<150 m) interval of ultramafic or near-ultramafic composition rocks of indeterminate origin. -
Mantle Peridotite Xenoliths
Earth and Planetary Science Letters 260 (2007) 37–55 www.elsevier.com/locate/epsl Mantle peridotite xenoliths in andesite lava at El Peñon, central Mexican Volcanic Belt: Isotopic and trace element evidence for melting and metasomatism in the mantle wedge beneath an active arc ⁎ Samuel B. Mukasa a, , Dawnika L. Blatter b, Alexandre V. Andronikov a a Department of Geological Sciences, University of Michigan, Ann Arbor, MI 48109-1005, USA b Department of Earth and Planetary Science, University of California, Berkeley, CA 94720, USA Received 6 July 2006; received in revised form 3 May 2007; accepted 7 May 2007 Available online 13 May 2007 Editor: R.W. Carlson Abstract Peridotites in the mantle wedge and components added to them from the subducting slab are thought to be the source of most arc magmas. However, direct sampling of these materials, which provides a glimpse into the upper mantle beneath an active margin, is exceedingly rare. In the few arc localities where found, peridotite xenoliths are usually brought to the surface by basaltic magmas. Remarkably, the hornblende-bearing ultramafic xenoliths and clinopyroxene megaxenocrysts from El Peñon in the central Mexican Volcanic Belt were brought to the surface by a Quaternary high-Mg siliceous andesite, a rock type usually considered too evolved to be a direct product of mantle melting. The xenoliths and megaxenocrysts from El Peñon represent lithospheric mantle affected by significant subduction of oceanic lithosphere since as early as the Permian. Trace element and radiogenic isotope data we report here on these materials suggest a history of depletion by melt extraction, metasomatism involving a fluid phase, and finally, limited reaction between the ultramafic materials and the host andesite, probably during transport. -
Luís Pedro Esteves Internal Curing in Cement-Based Materials Universidade De Departamento De Engenharia Civil Aveiro 2009
Universidade de Departamento de Engenharia Civil Aveiro 2009 Luís Pedro Esteves Internal curing in cement-based materials Universidade de Departamento de Engenharia Civil Aveiro 2009 Luís Pedro Esteves Internal curing in cement-based materials Dissertação apresentada à Universidade de Aveiro para cumprimento dos requisitos necessários à obtenção do grau de Doutor em Engenharia Civil, realizada sob a orientação científica do Dr. Paulo Barreto Cachim, Professor Associado do Departamento de Engenharia Civil da Universidade de Aveiro e do Dr. Victor Miguel C. de Sousa Ferreira, Professor Associado do Departamento de Engenharia Civil da Universidade de Aveiro. Beside other problematic, it was often astonishing to run after thoughts. As an ancient philosophy doctor pointed out: “The greater the attempt that is made to study the nature or behaviour of a photon or a particle, the greater will be the uncertainty or error of the measurements.” Heisenberg summarised this in his uncertainty principle, the concept being demonstrated by means of idealized “thought” experiments. If it is permitted for me to say, I would add: (…), provided that it can not be seen or felt. O júri PRESIDENTE: Reitora da Universidade de Aveiro VOGAIS: Doutor Ole Mejhede Jensen, Professor Catedrático da Technical University of Denmark. Doutor Klaas van Breugel, Professor Catedrático da Delft University of Technology. Doutor Aníbal Guimarães da Costa, Professor Catedrático da Universidade de Aveiro. Doutor José Luís Barroso de Aguiar, Professor Associado com Agregação da Universidade do Minho. Doutor Paulo Barreto Cachim, Professor Associado da Universidade de Aveiro (Orientador). Doutor Victor Miguel Carneiro de Sousa Ferreira, Professor Associado da Universidade de Aveiro (Co-Orientador). -
16 /75 / 7 ~ -% in +~ In
7-'<16_ /75_ / 7 ~ R.6l3. Wolframite concentration, Scamander Mining Corporation N.L. A chip sample for the determination of the maximum recoverable amount of wolframite was supplied by the Scamander Mining Corporation and stated to be from their Scamander Tier lease. Special consideration was to be given to the production of a high grade wolframite concentrate and the rejection of the coarsest possible tailing. The chip sample was given the registered number 700174. • The chip sample was initially c rushed to -\ in and found to contain 0.82\ W03' The sample consisted mainly of quartz plus some dolerite with minor amounts of an iron oxide mineral. Large slivers of wolframite up to • 5/16 in were present. SAMPLE PREPARATION The -\ in ore was stage crushed to %" in in a laboratory Chipmunk jaw crusher, mixed, then riffled into four identical parts. One part was further riffled to supply samples for a siie analysis and a further head assay. The second part was wet, then dry screened to provide the following fractions for concentration: Size Range Concentrating Operation -% in +~ in 1 -\ in +10. 2 -10* +22. 3 • -22. +52# 4 -52. +100. 5 -100. +200# 6 • - 200. 7 The remaining two identical parts were retained for possible further work. PROCEDURE The sized fractions of the ore were gravity and magnetically concen t trated (Table 1). II Jig Concentration Jig conditions are shown in Table 2. As the jig concentration operat ions were not continuous , each fraction was fed through its respective jig ~ three times. Table Concentration Minimum amounts of water and l ow feed rates were used to obtain quartz free concentrates from each fraction. -
Hydrated Peridotite – Basaltic Melt Interaction Part I: Planetary Felsic Crust Formation at Shallow Depth Anastassia Y
Hydrated Peridotite – Basaltic Melt Interaction Part I: Planetary Felsic Crust Formation at Shallow Depth Anastassia Y. BORISOVA1,2*, Nail R. ZAGRTDENOV1, Michael J. TOPLIS3, Wendy A. BOHRSON4, Anne NEDELEC1, Oleg G. SAFONOV2,5,6, Gleb S. POKROVSKI1, Georges CEULENEER1, Ilya N. BINDEMAN7, Oleg E. MELNIK8, Klaus Peter JOCHUM9, Brigitte STOLL9, Ulrike WEIS9, Andrew Y. BYCHKOV2, Andrey A. GURENKO10, Svyatoslav SHCHEKA11, Artem TEREHIN5, Vladimir M. POLUKEEV5, Dmitry A. VARLAMOV5, Kouassi E.A. CHARITEIRO1, Sophie GOUY1, Philippe de PARSEVAL1 1 Géosciences Environnement Toulouse, Université de Toulouse; UPS, CNRS, IRD, Toulouse, France 2 Geological Department, Lomonosov Moscow State University, Vorobievy Gory, 119899, Moscow, Russia 3 Institut de Recherche en Astrophysique et Planétologie (IRAP) UPS, CNRS, Toulouse, France 4 Central Washington University, Department of Geological Sciences, Ellensburg, WA 98926, USA 5 Korzhinskii Institute of Experimental Mineralogy, 142432, Chernogolovka, Moscow region, Russia 6 Department of Geology, University of Johannesburg PO Box 524, Auckland Park, 2006, Johannesburg, South Africa 7 Geological Sciences, University of Oregon, 1275 E 13th street, Eugene, OR, USA 8 Institute of Mechanics, Moscow State University, 1- Michurinskii prosp, 119192, Moscow, Russia 9 Climate Geochemistry Department, Max Planck Institute for Chemistry, P.O. Box 3060, D-55020 Mainz, Germany 10 Centre de Recherches Pétrographiques et Géochimiques, UMR 7358, Université de Lorraine, 54501 Vandœuvre-lès-Nancy, France 11 Bavarian Research -
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 -
Geochemistry and Petrology of Listvenite in the Samail Ophiolite, Sultanate of Oman: Complete Carbonation of Peridotite During Ophiolite Emplacement
Available online at www.sciencedirect.com ScienceDirect Geochimica et Cosmochimica Acta 160 (2015) 70–90 www.elsevier.com/locate/gca Geochemistry and petrology of listvenite in the Samail ophiolite, Sultanate of Oman: Complete carbonation of peridotite during ophiolite emplacement Elisabeth S. Falk ⇑, Peter B. Kelemen Lamont-Doherty Earth Observatory, Columbia University, Palisades, NY 10964, USA Received 16 May 2014; accepted in revised form 14 March 2015; available online 20 March 2015 Abstract Extensive outcrops of listvenite—fully carbonated peridotite, with all Mg in carbonate minerals and all Si in quartz—occur along the basal thrust of the Samail ophiolite in Oman. These rocks can provide insight into processes including (a) carbon fluxes at the “leading edge of the mantle wedge” in subduction zones and (b) enhanced mineral carbonation of peridotite as a means of carbon storage. Here we examine mineralogical, chemical and isotopic evidence on the temperatures, timing, and fluid compositions involved in the formation of this listvenite. The listvenites are composed primarily of magnesite and/or dolomite + quartz + relict Cr-spinel. In some instances the conversion of peridotite to listvenite is nearly isochemical except for the addition of CO2, while other samples have also seen significant calcium addition and/or variable, minor addition of K and Mn. Along margins where listvenite bodies are in contact with serpentinized peridotite, talc and antigorite are present in addition to carbonate and quartz. The presence of antigorite + quartz + talc in these samples implies temperatures of 80– 130 °C. This range of temperature is consistent with dolomite and magnesite clumped isotope thermometry in listvenite (aver- age T = 90 ± 15 °C) and with conventional mineral-water oxygen isotope exchange thermometry (assuming fluid d18O near zero). -
Experimental Investigation of the Pressure of Crystallization of Ca(OH)2: Implications for the Reactive Cracking Process
Geochemistry, Geophysics, Geosystems RESEARCH ARTICLE Experimental Investigation of the Pressure of Crystallization 10.1029/2018GC007609 of Ca(OH)2: Implications for the Reactive Cracking Process Key Points: S. Lambart1,2 , H. M. Savage1, B. G. Robinson1, and P. B. Kelemen1 • Crystallization pressure of CaO hydration exceeds 27 MPa at 1-km 1Lamont-Doherty Earth Observatory, Columbia University, Palisades, NY, USA, 2Geology and Geophysics, University of Utah, crustal depth • Fluid transport via capillary flow is Salt Lake City, UT, USA rate limiting • Strain rate exhibits negative, power law dependence on uniaxial load Abstract Mineral hydration and carbonation can produce large solid volume increases, deviatoric stress, and fracture, which in turn can maintain or enhance permeability and reactive surface area. Supporting Information: Despite the potential importance of this process, our basic physical understanding of the conditions • Supporting Information S1 under which a given reaction will drive fracture (if at all) is relatively limited. Our hydration experiments • Table S2 on CaO under uniaxial loads of 0.1 to 27 MPa show that strain and strain rate are proportional to the • Table S3 square root of time and exhibit negative, power law dependence on uniaxial load, suggesting that (1) fl fl fi Correspondence to: uid transport via capillary ow is rate limiting and (2) decreasing strain rate with increasing con ning S. Lambart, pressure might be a limiting factor in reaction driven cracking at depth. However, our experiments also [email protected] demonstrate that crystallization pressure due to hydration exceeds 27 MPa (consistent with a maximum crystallization pressure of 153 MPa for the same reaction, Wolterbeek et al., https://doi.org/10.1007/ Citation: s11440-017-0533-5). -
Technologic Tests of Turkey-Gordes Zeolite Minerals
Journal of Minerals and Materials Characterization and Engineering, 2017, 5, 252-265 http://www.scirp.org/journal/jmmce ISSN Online: 2327-4085 ISSN Print: 2327-4077 Technologic Tests of Turkey-Gordes Zeolite Minerals Oyku Bilgin Department of Mining Engineering, Sirnak University, Sirnak, Turkey How to cite this paper: Bilgin, O. (2017) Abstract Technologic Tests of Turkey-Gordes Zeo- lite Minerals. Journal of Minerals and Ma- Natural zeolites are found at many points of the world in the form of miner- terials Characterization and Engineering, 5, als. As for Turkey, quite large volumes of zeolites reserves are available in the 252-265. following regions: Ankara (Nallihan, Beypazari, Polatli etc.), Kütahya-Sa- https://doi.org/10.4236/jmmce.2017.55021 phane, Manisa-Gördes, Manisa-Demirci, Izmir-Urla, Balıkesir-Bigadiç and Received: February 23, 2017 Cappadocia. By means of the works carried out only at the field in Balikesir- Accepted: August 11, 2017 Bigadiç region, one of the detected reserves in Turkey, it was understood that Published: August 14, 2017 an easily workable potential around 500 million ton is available. According to Copyright © 2017 by author and the very limited observations made until today, it is stated that the total re- Scientific Research Publishing Inc. serve in our country may be around 500 billion ton. In these regions, the types This work is licensed under the Creative of clinoptilolite, hoylandit, chabazite, analcime and erionite from the zeolite Commons Attribution International minerals exist. Zeolites are widely used in many sectors such as energy, envi- License (CC BY 4.0). http://creativecommons.org/licenses/by/4.0/ ronment, construction, detergent, chemistry, medicine, mining, agriculture Open Access and livestock. -
The Ronda Peridotite: Garnet-, Spinel-, and Plagioclase-Lherzolite Facies and the P—T Trajectories of a High-Temperature Mantle Intrusion
The Ronda Peridotite: Garnet-, Spinel-, and Plagioclase-Lherzolite Facies and the P—T Trajectories of a High-Temperature Mantle Intrusion by MASAAKI OBATA* Institutfiir Kristallographie und Petrographie, Eidgenossische Technische Hochschule, Zurich, CH-8092, Zurich, Switzerland (Received 18 October 1978; in revised form 28 June 1979) ABSTRACT The Ronda peridotite is a high-temperature, alpine-type peridotite emplaced in the internal Zone of the Betic Cordilleras, southern Spain. Using the mineral assemblages of the peridotite and mafic layers, the peridotite mass has been subdivided into 4 zones of mineral facies: (l)garnet-lherzolite facies, (2) ariegite subfacies of spinel-lherzolite facies, (3) seiland subfacies of spinel-lherzolite facies, and (4) plagioclase-lherzolite facies. It is proposed that this mineralogical zonation developed through a syntectic recrystallization of a hot (1100 to 1200 °C), solid mantle peridotite during its ascent into the Earth's crust. Coexisting minerals from 12 peridotites covering all the mineral facies above were analysed with an electron microprobe. Core compositions of pyroxene porphyroclasts are constant in all mineral facies and indicate that the peridotite was initially equilibrated at temperatures of 1100 to 1200 °C and pressures of 20 to 25 kb. In contrast, the compositions of pyroxene neoblasts and spinel grains (which appear to have grown during later recrystallization) are well correlated with mineral facies. They indicate that the recrystallization temperature throughout the mass is more or less constant, 800 to 900 °C, but that the pressure ranges from 5-7 kb in the plagioclase-lherzolite facies to 12-15 kb in the garnet-lherzolite facies. Therefore, variation in pressure appears to be primarily responsible for the four mineral facies types. -
Fingerprints of Kamafugite-Like Magmas in Mesozoic Lamproites of the Aldan Shield: Evidence from Olivine and Olivine-Hosted Inclusions
minerals Article Fingerprints of Kamafugite-Like Magmas in Mesozoic Lamproites of the Aldan Shield: Evidence from Olivine and Olivine-Hosted Inclusions Ivan F. Chayka 1,2,*, Alexander V. Sobolev 3,4, Andrey E. Izokh 1,5, Valentina G. Batanova 3, Stepan P. Krasheninnikov 4 , Maria V. Chervyakovskaya 6, Alkiviadis Kontonikas-Charos 7, Anton V. Kutyrev 8 , Boris M. Lobastov 9 and Vasiliy S. Chervyakovskiy 6 1 V. S. Sobolev Institute of Geology and Mineralogy Siberian Branch of the Russian Academy of Sciences, 630090 Novosibirsk, Russia; [email protected] 2 Institute of Experimental Mineralogy, Russian Academy of Sciences, 142432 Chernogolovka, Russia 3 Institut des Sciences de la Terre (ISTerre), Université de Grenoble Alpes, 38041 Grenoble, France; [email protected] (A.V.S.); [email protected] (V.G.B.) 4 Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian Academy of Sciences, Moscow, Russia; [email protected] 5 Department of Geology and Geophysics, Novosibirsk State University, 630090 Novosibirsk, Russia 6 Institute of Geology and Geochemistry, Ural Branch of the Russian Academy of Sciences, 620016 Yekaterinburg, Russia; [email protected] (M.V.C.); [email protected] (V.S.C.) 7 School of Chemical Engineering and Advanced Materials, The University of Adelaide, Adelaide, SA 5005, Australia; [email protected] 8 Institute of Volcanology and Seismology, Far Eastern Branch of the Russian Academy of Sciences, 683000 Petropavlovsk-Kamchatsky, Russia; [email protected] 9 Institute of Mining, Geology and Geotechnology, Siberian Federal University, 660041 Krasnoyarsk, Russia; [email protected] * Correspondence: [email protected]; Tel.: +7-985-799-4936 Received: 17 February 2020; Accepted: 6 April 2020; Published: 9 April 2020 Abstract: Mesozoic (125–135 Ma) cratonic low-Ti lamproites from the northern part of the Aldan Shield do not conform to typical classification schemes of ultrapotassic anorogenic rocks. -
Influence of Mineral Composition of Melaphyre Grits on Durability of Motorway Surface
Physicochemical Problems of Mineral Processing, 38 (2004) 341-350 Fizykochemiczne Problemy Mineralurgii, 38 (2004) 341-350 Tadeusz CHRZAN4 INFLUENCE OF MINERAL COMPOSITION OF MELAPHYRE GRITS ON DURABILITY OF MOTORWAY SURFACE Received April 4, 2004; reviewed; accepted June 5; 2004 The surface layer of the Konin-Września motorway section was made between July and November of 2001. Although the tests of melaphyre aggregates against grade and class requirements had confirmed that grits were the first class and grade according to the Polish standards, the motorway has been wearing rapidly with the first repairs being carried out as early as 2003. The motorway surface has been excessively worn and looks as if it were used for at least 5 years. The paper explains why the motorway surface has been worn so rapidly. Key words: motorway, ,melaphyre grit, weathering INTRODUCTION The surface layer of the Konin-Września motorway section was made during the period from July to November 2001. The layer was made with granulated aggregate 0- 20 mm in diameter from Borówko and Grzędy melaphyre quarry, bounded with modified bituminous mass. The tests of melaphyre aggregates against grade and class requirements had confirmed that the grits were the first class and grade (Chrzan, 1997; Wysokowski, 2000/2001) according to the Polish Standards (PN-11112:96, PN- 11110:96, PN-EN 1097-2). The binding layer of asphaltic concrete made and tested on samples that were taken from the completed motorway also conformed to the standard requirements according to Polish Standards (PN-S/96025, PN-74/S-96022). Also, the adhesion of asphalt to the melaphyre grit conformed to the standard (PN-84/B-6714/22).