Magnetic Properties of Sheet Silicates; 2:1:1 Layer Minerals
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Hydrothermal and Metamorphic Berthierine
n27 CanadianMineralogist Vol. 30,pp. 1127-1142 (1992) HYDROTHERMALAND METAMORPHICBERTHIERINE FROM THE KIDD CREEK VOLCANOGENICMASSTVE SULFIDE DEPOSIT. TIMMINS, ONTARIO JOHNF.SLACK U.S.Geological Survey, Nationnl Center, Mail Stop954, Reston, Virginia 22092, U.S.A. WEI-TEH JIANG ANDDONALD R. PEACOR Depamnent of Geological Sciences, University of Michigan, Ann Arbor, Michigan 48109, U.S.A. PATRICKM. OKITA* U.S.Geological Survey, National Center,Mail Stop954, Reston,Virginia 22092,U.S.A. ABSTRACT Berthierine,a 7 A pe-Al memberof the serpentinegroup, occursin the footwall stringerzone of the ArcheanKidd Creek massivesulfide deposit, Ontario, associated with quartz,muscovite, chlorite, pyrite, sphalerite,chalcopyrite, and local tourmaline' cassiterite,and halloysite. Berthierine has been identified by the lack of 14A basalreflections on X-ray powderdiffractionpattems, by its composition (electron-microprobedata), and by transmissionelectron microscopy (TEM). Peoogaphic and scanning eiectronmicroscopic (SEM) studiesreveal different types of berthierineocculrences, including interlayerswithin and rims on deformedchlorite, intergrowthswith muscoviteand halloysite,and discretecoarse grains. TEM imagesshow thick packetsof berthierineand chlorite that are parallel or relatedby low-angle boundaries,and layer terminationsof chlorite by berthierine; mixedJayer chlorite-berthierinealso is observed,intergrown with Fe-rich chlorite and berthierine.End-member (Mg-free) berthierineis presentin small domainsin two samples.The Kidd Creekberthierine is chemicallysimilar -
Devonian and Carboniferous Metamorphism in West-Central
American Mineralogist, Volume 73, pages20-47, 1988 Devonian and Carboniferousmetamorphism in west-centralMaine: The muscovite-almandinegeobarometer and the staurolite problem revisited M. J. Hololwlv Department of Geological Sciences,Southern Methodist University, Dallas, Texas 75275, U.S.A. B. L. Durnow Department of Geology, Louisiana State University, Baton Rouge, Louisiana 70803, U.S.A. R. W. HrNroN* The EnricoFermi Institute, The Universityof Chicago,Chicago, Illinois 60637,U.S.A. ABSTRAcT Important thermal metamorphic eventsin west-centralMaine occurred at 400 Ma (Mr), 394-379Ma(Mr), and325 Ma(Mr). EachiscloselyassociatedwithemplacementofS-type granites,such that the isogradpatterns produced in the surrounding pelitic schistsgenerally follow plutonic outlines. From north to south, gradeof metamorphism varies from chlorite to sillimanite-K-feldspar-muscovite. Mineral-chemistry studies on M, and M, indicate the following: (l) Much staurolite- grade chlorite is retrograde as demonstrated by the lack of a consistent relation between biotite composition and presenceor absenceofchlorite, given the restricted range ofX"ro allowed in these reduced graphitic rocks. Consequently,the first sillimanite-forming re- action for many pelitic schists in Maine does not involve chlorite. (2) Garnet zoning patterns are prograde in rocks of the staurolite zone and retrograde in rocks of higher grade. (3) Presenceof graphite and nearly pure ilmenite suggestslow Fe3* in micas and allows for end-membercalculations that include a "Ti biotite" (KTiD(Fe,Mg)AlSi3Oro(OH)r) and a "Ti muscovite" (KTi(Fe,Mg)AlSi3O,o(OH)r).(4) Staurolire contains about 3 H (48- oxygen basis) and shows subtle indications of nonideality in Fe-Mg Ko relationships. Garnet-biotite geothermometryindicates the following averagetemperatures for the first occurrenceof minerals:staurolite-510'C, sillimanite-580 "C, sillimanite-K-feldspar- 660 "C. -
Far-Infrared Spectra of Hydrous Silicates at Low Temperatures Providing Laboratory Data for Herschel and ALMA
A&A 492, 117–125 (2008) Astronomy DOI: 10.1051/0004-6361:200810312 & c ESO 2008 Astrophysics Far-infrared spectra of hydrous silicates at low temperatures Providing laboratory data for Herschel and ALMA H. Mutschke1,S.Zeidler1, Th. Posch2, F. Kerschbaum2, A. Baier2, and Th. Henning3 1 Astrophysikalisches Institut, Schillergässchen 2-3, 07745 Jena, Germany e-mail: [mutschke;sz]@astro.uni-jena.de 2 Institut für Astronomie, Türkenschanzstraße 17, 1180 Wien, Austria e-mail: [email protected] 3 Max-Planck-Institut für Astronomie (MPIA), Königstuhl 17, 69117 Heidelberg, Germany e-mail: [email protected] Received 2 June 2008 / Accepted 4 September 2008 ABSTRACT Context. Hydrous silicates occur in various cosmic environments, and are among the minerals with the most pronounced bands in the far infrared (FIR) spectral region. Given that Herschel and ALMA will open up new possibilities for astronomical FIR and sub-mm spectroscopy, data characterizing the dielectric properties of these materials at long wavelengths are desirable. Aims. We aimed at examining the FIR spectra of talc, picrolite, montmorillonite, and chamosite, which belong to four different groups of phyllosilicates. We tabulated positions and band widths of the FIR bands of these minerals depending on the dust temperature. Methods. By means of powder transmission spectroscopy, spectra of the examined materials were measured in the wavelength range 25−500 μm at temperatures of 300, 200, 100, and 10 K. Results. Room-temperature measurements yield the following results. For talc, a previously unknown band, centered at 98.5 μm, was found, in addition to bands at 56.5 and 59.5 μm. -
On the Relation of Chamosite and Daphnite to the Chlorite Group. 1 (With Plates XVIII and XIX.) by A
441 On the relation of chamosite and daphnite to the chlorite group. 1 (With Plates XVIII and XIX.) By A. F. HXLLIMOSD, M.A., Sc.D. Assistant Curator, Museum of Practical Geology, London. With chemical analyses by C. O. HARVEY, B.Sc., A.R.C.S. and X-ray measurements by F. A. BANNISTER, M.A. [Read June 9, 1938.] I. INTRODUCTION. HERE is a close optical and chemical resemblance between chamo- T site, the chloritic mineral of the bedded ironstones, and daphnite, a low-temperature vein-chlorite common in some of the Cornish tin mines. New material has made it possible to undertake a fresh com- parison of the two minerals: chemical analyses have been made by Mr. C. O. Harvey, chemist to H.M. Geological Survey, and a report on the X-ray measurements is contributed by Mr. F. A. Bannister, of the Mineral Department of the British Museum. The new analysis of chamosite agrees with the simple formula pre- viously assigned: X-ray examination of material from several localities has now established the distinctive crystalline nature of this fine-grained mineral, which differs structurally from ordinary chlorites such as clinochlore. Daphnite, on the other hand, has the ordinary chlorite structure, but the new analysis hilly confirms Tschermak's original opinion that it cannot be represented chemically as a mixture of serpen- tine and amesite. In attempting a comparison with chlorite analyses already published, great difficulty arises from the confused nomenclature. In order to ascertain the nearest chemically allied chlorites to those under dis- cussion, a representative number of selected chlorite analyses have been plotted on a diagram with co-ordinates proportional to R2Oa/SiO2 and RO/Si02. -
The Ore and Gangue Mineralogy of the Newly Discovered Federation Massive Sulfide Deposit, Central New South Wales, Australia †
Proceedings The Ore and Gangue Mineralogy of the Newly Discovered Federation Massive Sulfide Deposit, Central New South Wales, Australia † Khalid Schellen 1, Ian T. Graham 1,*, Adam McKinnon 2, Karen Privat 1,3 and Christian Dietz 4 1 School of Biological, Earth, and Environmental Sciences, UNSW Sydney, Sydney, NSW 2052, Australia; [email protected] (K.S); [email protected] (K.P.) 2 Aurelia Metals Limited, Level 17, 144 Edward Street, Brisbane, QLD 4000, Australia; [email protected] 3 Electron Microscope Unit, Mark Wainwright Analytical Centre, UNSW Sydney, Sydney, NSW 2052, Australia 4 Central Science Laboratory, University of Tasmania, Hobart, TAS 7001, Australia; [email protected] * Correspondence: [email protected]; Tel.: +61-435-296-555 † Presented at the 2nd International Electronic Conference on Mineral Science, 1–15 March 2021; Available online: https://iecms2021.sciforum.net/. Abstract: The newly discovered Federation deposit, with a resource estimate of 2.6 Mt @ 7.7% Pb, 13.5% Zn, 0.8 g/t Au, and 9 g/t Ag, lies 10 km south of the Hera deposit within the Cobar Basin of the Lachlan Orogen. Located just north of the Erimeran Granite contact and between the Lower Amphitheatre Group and underlying shallow marine Mouramba Group Roset Sandstone, the host siltstones and sandstones have been brecciated, intensely silicified, and chloritized close to miner- alization. Oriented in an overall east-northeast strike and with a steep south-southeast dip, the silt- stones mainly comprise quartz, clinochlore, biotite, and muscovite. Federation also has highly frag- mented zones with breccia and vein-fill of calcite. -
Miissbauer Spectra of Minnesotaite and Ferroan Talc J.M.D. Corv, T
American Mineralogist, Volume 76, pages 1905-1909, 1991 Miissbauer spectra of minnesotaite and ferroan talc J.M.D. Corv, T. Blxls* Department of Pure and Applied Physics,Trinity College,Dublin 2, Ireland S. GuccnNnprnr Department of Geological Sciences,University of Illinois at Chicago, Chicago,Illinois 60680, U.S.A, Arsrru.cr Mdssbauer spectra of five samples of minnesotaite and one of ferroan talc have been recordedat 296 K and 4.2 K. A singleferrous doublet with isomer shift 6 : 1.13 mm/s relative to aFe and quadrupolesplitting L:2J4 mm/s is observedin all minnesotaite samples at room temperature. The ferroan talc has a smaller quadrupole splitting, A : 2.55 mm/s. All minnesotaite samplesorder antiferromagnetically,with N6el points in the tange 25-37 K, but ferroan talc does not order magnetically down to 4.2 K. Two distinct ferrous populations in minnesotaite are inferred from the resolved magneticallysplit spec- tra at 4.2 K. The minority sites may be those coordinated by the excessOH in the min- nesotaitestructure. The P-cell and C-cell variants have distinctly different hyperfine fields (10.4 and 14.9T for the two sitesin the P cell but 8.9 and 14.4T in the C cell),although their N6el points are similar. INrnooucrroN taite, ferroan talc, and talc and found a lack of compo- Minnesotaite was originally considered by Gruner sitions having the octahedralFe fraction in the range0.45- (1944) to be an Fe analogueof talc having ideal formula 0.60, perhapsindicating the chemical limits of the struc- tures. {Fel*}[Sio]O,o(OH),,where { } and [ ] denotethe oc- tahedral and tetrahedral sites, respectively.More recent- Both minnesotaite and talc have a continuous octahe- ly, X-ray and electron diffraction studies (Guggenheim dral sheet(Fe in minnesotaite, Fe,Mg in ferroan talc) but and Bailey, 1982; Guggenheim and Eggleton, 1986) differ in the nature ofthe tetrahedral sheets.It is therefore showed that the structure is considerablymore complex. -
The Role of Ferrous Clays in the Interpretation of Wettability – a Case Study
SCA2018-019 1/12 THE ROLE OF FERROUS CLAYS IN THE INTERPRETATION OF WETTABILITY – A CASE STUDY Velazco M.A, Bruce A., Ferris M, Reed J., Kandasamy R. Lloyd’s Register Energy Consultancy, Rock Properties Group, Aberdeen, UK This paper was prepared for presentation at the International Symposium of the Society of Core Analysts held in Trondheim, Norway, 27-30 August 2018 ABSTRACT Clean sandstone, with minimal clay content, is expected to be strongly water wet once the rock has been through an effective cleaning process. Even samples containing significant clay minerals are usually expected to be water wet after appropriate cleaning. However, tests carried out on core samples from Fields in three different global locations show mixed indices, even for clean state samples where no aging with crude oil has taken place. A few hypotheses for this behaviour considered herein are: whether the cleaning method was adequate, whether wettability was altered by an external factor, or if wettability was due to mineral composition. This paper presents the results obtained from wettability studies on fresh, clean and restored state core plug samples from three different Fields. Wettability indices were obtained by using the combined Amott-USBM method. Petrography was performed on sample end-trims to investigate the possible presence of halite or barite in the clean state samples, thought to be from drilling fluid infiltration, which should have been removed by the methanol cleaning cycle. This showed no organic material or salt (halite), negating wetting change from inefficient cleaning. From a reactive clays [1] model perspective, these rock samples are considered clean-sand (i.e. -
Phyllosilicates in the Sediment-Forming Processes: Weathering, Erosion, Transportation, and Deposition
Acta Geodyn. Geomater., Vol. 6, No. 1 (153), 13–43, 2009 PHYLLOSILICATES IN THE SEDIMENT-FORMING PROCESSES: WEATHERING, EROSION, TRANSPORTATION, AND DEPOSITION Jiří KONTA Faculty of Sciences, Charles University, Albertov 6, 128 43 Prague 2 Home address: Korunní 127, 130 00 Prague 3, Czech Republic *Corresponding author‘s e-mail: [email protected] (Received October 2008, accepted January 2009) ABSTRACT Phyllosilicates are classified into the following groups: 1 - Neutral 1:1 structures: the kaolinite and serpentine group. 2 - Neutral 2:1 structures: the pyrophyllite and talc group. 3 - High-charge 2:1 structures, non-expansible in polar liquids: illite and the dioctahedral and trioctahedral micas, also brittle micas. 4 - Low- to medium-charge 2:1 structures, expansible phyllosilicates in polar liquids: smectites and vermiculites. 5 - Neutral 2:1:1 structures: chlorites. 6 - Neutral to weak-charge ribbon structures, so-called pseudophyllosilicates or hormites: palygorskite and sepiolite (fibrous crystalline clay minerals). 7 - Amorphous clay minerals. Order-disorder states, polymorphism, polytypism, and interstratifications of phyllosilicates are influenced by several factors: 1) a chemical micromilieu acting during the crystallization in any environment, including the space of clay pseudomorphs after original rock-forming silicates or volcanic glasses; 2) the accepted thermal energy; 3) the permeability. The composition and properties of parent rocks and minerals in the weathering crusts, the elevation, and topography of source areas and climatic conditions control the intensity of weathering, erosion, and the resulting assemblage of phyllosilicates to be transported after erosion. The enormously high accumulation of phyllosilicates in the sedimentary lithosphere is primarily conditioned by their high up to extremely high chemical stability in water-rich environments (expressed by index of corrosion, IKO). -
Greenalite, Mg-Rich Minnesotaite and Stilpnomelane from the Osj6berg and Sirsj6berg Iron-Ore Mines, Hjulsj6, W
MINERALOGICAL MAGAZINE, SEPTEMBER 1985, VOL. 49, PP. 611 613 Greenalite, Mg-rich minnesotaite and stilpnomelane from the Osj6berg and Sirsj6berg iron-ore mines, Hjulsj6, W. Bergslagen, Sweden GREENALITE, Mg-rich minnesotaite, and stilpno- subvertical body which strikes approximately E-W melane have been identified by electron micro- and is considered by Baker and de Groot (1983b) to probe analysis in samples taken from dumps of the be continuation of the Osj6berg ore horizon. The abandoned Qsj6berg and Sirsj6berg mines 5 km ore is separated from an underlying limestone NW of Hjulsj6, Bergslagen. This is the first horizon by a garnet-pyroxene-amphibole skarn. report of the occurrence of these minerals in the Magnetite is present in the skarn and the limestone. Proterozoic iron ores of Central Sweden. The two Epidote and calcite are later minerals filling tectonic mines, some 700 m apart, worked a large, 7 km long, fissures and cracks. meta-rhyotite-hosted, magnetite ore horizon--one Greenalite occurs in a sample from ()sj6berg of the many concordant skarn iron ores in the mine which comprises a fine grained aggregate of 1.8-1.9 Ga Proterozoic Bergslagen Supracrustal magnetite grains (+0.05 mm) with some larger Series (Oen et al., 1982). They were amongst the grains up to 0.5 mm in a matrix composed pre- largest iron producers of this area. dominantly of talc with minor green chlorite. Talc The subsurface geology of the mines has been also fills fractures in the larger magnetite grains. described by Geijer and Magnusson (1944); earlier Very minor pyrite and rare chalcopyrite are seen descriptions are given by Blomberg (1879) and enclosing magnetite. -
Microbial Interaction with Clay Minerals and Its Environmental and Biotechnological Implications
minerals Review Microbial Interaction with Clay Minerals and Its Environmental and Biotechnological Implications Marina Fomina * and Iryna Skorochod Zabolotny Institute of Microbiology and Virology of National Academy of Sciences of Ukraine, Zabolotny str., 154, 03143 Kyiv, Ukraine; [email protected] * Correspondence: [email protected] Received: 13 August 2020; Accepted: 24 September 2020; Published: 29 September 2020 Abstract: Clay minerals are very common in nature and highly reactive minerals which are typical products of the weathering of the most abundant silicate minerals on the planet. Over recent decades there has been growing appreciation that the prime involvement of clay minerals in the geochemical cycling of elements and pedosphere genesis should take into account the biogeochemical activity of microorganisms. Microbial intimate interaction with clay minerals, that has taken place on Earth’s surface in a geological time-scale, represents a complex co-evolving system which is challenging to comprehend because of fragmented information and requires coordinated efforts from both clay scientists and microbiologists. This review covers some important aspects of the interactions of clay minerals with microorganisms at the different levels of complexity, starting from organic molecules, individual and aggregated microbial cells, fungal and bacterial symbioses with photosynthetic organisms, pedosphere, up to environmental and biotechnological implications. The review attempts to systematize our current general understanding of the processes of biogeochemical transformation of clay minerals by microorganisms. This paper also highlights some microbiological and biotechnological perspectives of the practical application of clay minerals–microbes interactions not only in microbial bioremediation and biodegradation of pollutants but also in areas related to agronomy and human and animal health. -
Comparison of Phyllosilicates Observed on the Surface of Mars with Those Found in Martian Meteorites
80th Annual Meeting of the Meteoritical Society 2017 (LPI Contrib. No. 1987) 6115.pdf COMPARISON OF PHYLLOSILICATES OBSERVED ON THE SURFACE OF MARS WITH THOSE FOUND IN MARTIAN METEORITES. J. L. Bishop1, and M. A. Velbel2,3, 1SETI Institute & NASA-Ames (Mountain View, CA, USA; [email protected]), 2Michigan State University (East Lansing, MI); 3Smithsonian Institution (Washington, DC). Introduction: Phyllosilicates are an important indicator of aqueous processes on Mars and have been observed on the martian surface as well as inside martian meteorites. Here we survey the types of phyllosilicates detected at the surface of Mars and inside martian rocks in order to gain a better understanding of aqueous alteration processes taking place at Mars. Comparing the phyllosilicates observed on the surface today with those found in meteorites [1] may provide clues toward understanding which phyllosilicates formed in surface environments and which formed through subsurface processes. Martian Surface: Fe/Mg-phyllosilicates are present in numerous sites where the Noachian rocks are exposed [2]. These have been detected and characterized with the OMEGA [3] and CRISM [4] imaging spectrometers. Fe- rich smectite is the most abundant phyllosilicate on the surface of Mars [5], but a large variety of phyllosilicates and short-range-ordered (SRO) materials [6] have been observed. These include: nontronite, saponite, clinochlore, chamosite, serpentine, prehnite, talc, illite, beidelite, montmorillonite, kaolinite, halloysite, opal, hydrated silica, allophane, and imogolite. These are often observed together with iron oxides/hydroxides (FeOx), sulfates or car- bonates. Phyllosilicates and SROs have also been detected on Mars by CheMin on MSL [7]. Analyses of these data from several locations indicate the presence of trioctahedral and dioctahedral smectites and SRO phases [8, 9]. -
Data of Geochemistry
Data of Geochemistry ' * Chapter W. Chemistry of the Iron-rich Sedimentary Rocks GEOLOGICAL SURVEY PROFESSIONAL PAPER 440-W Data of Geochemistry MICHAEL FLEISCHER, Technical Editor Chapter W. Chemistry of the Iron-rich Sedimentary Rocks By HAROLD L. JAMES GEOLOGICAL SURVEY PROFESSIONAL PAPER 440-W Chemical composition and occurrence of iron-bearing minerals of sedimentary rocks, and composition, distribution, and geochemistry of ironstones and iron-formations UNITED STATES GOVERNMENT PRINTING OFFICE, WASHINGTON : 1966 UNITED STATES DEPARTMENT OF THE INTERIOR STEWART L. UDALL, Secretary GEOLOGICAL SURVEY William T. Pecora, Director For sale by the Superintendent of Documents, U.S. Government Printing Office Washington, D.C. 20402 - Price 45 cents (paper cover) CONTENTS Page Face Abstract. _ _______________________________ Wl Chemistry of iron-rich rocks, etc. Continued Introduction. _________ ___________________ 1 Oxide facies Continued Iron minerals of sedimentary rocks __ ______ 2 Hematitic iron-formation of Precambrian age__ W18 Iron oxides __ _______________________ 2 Magnetite-rich rocks of Mesozoic and Paleozoic Goethite (a-FeO (OH) ) and limonite _ 2 age___________-__-._____________ 19 Lepidocrocite (y-FeO(OH) )________ 3 Magnetite-rich iron-formation of Precambrian Hematite (a-Fe2O3) _ _ _ __ ___. _ _ 3 age._____-__---____--_---_-------------_ 21 Maghemite (7-Fe203) __ __________ 3 Silicate facies_________________________________ 21 Magnetite (Fe3O4) ________ _ ___ 3 Chamositic ironstone____--_-_-__----_-_---_- 21 3 Silicate iron-formation of Precambrian age_____ 22 Iron silicates 4 Glauconitic rocks__-_-____--------__-------- 23 4 Carbonate facies______-_-_-___-------_---------- 23 Greenalite. ________________________________ 6 Sideritic rocks of post-Precambrian age._______ 24 Glauconite____ _____________________________ 6 Sideritic iron-formation of Precambrian age____ 24 Chlorite (excluding chamosite) _______________ 7 Sulfide facies___________________________ 25 Minnesotaite.