Phlogopite-Forming Reactions As Indicators of Metasomatism in the Lithospheric Mantle
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A Ground Magnetic Survey of Kimberlite Intrusives in Elliott County, Kentucky
Kentucky Geological Survey James C. Cobb, State Geologist and Director University of Kentucky, Lexington A Ground Magnetic Survey of Kimberlite Intrusives in Elliott County, Kentucky John D. Calandra Thesis Series 2 Series XII, 2000 Kentucky Geological Survey James C. Cobb, State Geologist and Director University of Kentucky, Lexington A Ground Magnetic Survey of Kimberlite Intrusives in Elliott County, Kentucky John D. Calandra On the cover: Photomicrographs of olivine phenoc- rysts: (top) a stressed first-generation olivine pheno- cryst and (bottom) a late-stage olivine phenocryst. Thesis Series 2 Series XII, 2000 i UNIVERSITY OF KENTUCKY Computer and Laboratory Services Section: Charles T. Wethington Jr., President Steven Cordiviola, Head Fitzgerald Bramwell, Vice President for Research and Richard E. Sergeant, Geologist IV Graduate Studies Joseph B. Dixon, Information Technology Manager I Jack Supplee, Director, Administrative Affairs, Research James M. McElhone, Information Systems Technical and Graduate Studies Support Specialist IV Henry E. Francis, Scientist II KENTUCKY GEOLOGICAL SURVEY ADVISORY Karen Cisler, Scientist I BOARD Jason S. Backus, Research Analyst Henry M. Morgan, Chair, Utica Steven R. Mock, Research Analyst Ron D. Gilkerson, Vice Chair, Lexington Tracy Sizemore, Research Analyst William W. Bowdy, Fort Thomas Steve Cawood, Frankfort GEOLOGICAL DIVISION Hugh B. Gabbard, Winchester Coal and Minerals Section: Kenneth Gibson, Madisonville Donald R. Chesnut Jr., Head Mark E. Gormley, Versailles Garland R. Dever Jr., Geologist V Rosanne Kruzich, Louisville Cortland F. Eble, Geologist V W.A. Mossbarger, Lexington Gerald A. Weisenfluh, Geologist V Jacqueline Swigart, Louisville David A. Williams, Geologist V, Henderson office John F. Tate, Bonnyman Stephen F. Greb, Geologist IV David A. -
An Hypothesis for the Origin of Kimberlite 51
Mineral. Soc. Amer. Spec. Pap. 3,51-62 (1970). AN HYPOTHESIS FOR THE ORIGIN OF KIMBERLITE IAN D. MACGREGOR Department of Geology, University of California, Davis, California 95616 ABSTRACT Kimberlites are characteristically associated with a suite of mafic and ultramafic xenoliths whose mineralogy indicates an origin within the upper mantle. The phase chemistry of the xenoliths may be reconciled with known experimental data at high pressures, as suites of crystal cumulates, or residual phases, that have formed during the high-pressure fractional crystallization of a mafic magma. The geological association of kimberlites with specificsuites of xenoliths, and the com- parison with experimental data, give support to this cognate hypothesis previously proposed by a number of other authors. Models of the Earth's thermal history indicate that the upper mantle heated up for the first few billions of years after which time it has slowly cooled to its present state. It is postulated that the kimberlites are formed by the closed system fractional crystallization of mafic magmas which have formed by fractional fusion during the early heating of the upper mantle. During the cooling cycle in the last few billions of years, the mafic liquids have cooled through fractional crystal- lization to the ambient mantle temperatures, and changed composition towards a kimberlite. Sequential primary phase assemblages are represented by harzburgite, garnet harzburgite, garnet lherzolite, hypersthene eclogite, eclogite, kyanite eclogite to an olivine-diopside-perovskite rock. Parallel changes in the liquid composition are through picrite, tholeiite, alkali basalt, a diopside-ilmenite composition to kimberlite. INTRODUCTION logical and geophysical characteristics common to the gen- Although kimberlites occupy only a very small propor- eral description included in the following section. -
Origin of Lherzolite Inclusions in the Malapai Hill Basalt, Joshua Tree National Monument, California
ROBERT J. STULL Department of Geology, California State University, Los Angeles, Los Angeles, California 90032 KENT McMILLAN Department of Geological Sciences, Stanford University, Stanford, California 94305 Origin of Lherzolite Inclusions in the Malapai Hill Basalt, Joshua Tree National Monument, California ABSTRACT dence that the nodules could be the end product of more than one partial melting. Alkali olivine basalt at Malapai Hill, Cali- fornia, occurs as a late Cenozoic stock that has INTRODUCTION intruded the Cretaceous White Tank Monzon- Basalts and ultramafic nodules from the ite. The basalt is chemically and mineralogi- Mojave Desert have been described in several cally similar to other alkaline basalts in the papers. Ross and others (1954) reported min- Mojave Desert, although it is devoid of zeolites. eral compositions of peridotite inclusions from The strontium isotopic composition of the Dish Hill and noted the world-wide similarity basalt (Sr87/Sr86 = 0.7030 ± 0.0006) suggests of nodules. Hess (1955) published one analysis that it is derived from a mantle that has of a nodule from Dish Hill (Fig. 1). Wise already experienced one period of partial (1966, 1969) described the characteristics of ba- melting. OUvine-rich lherzolite nodules in the salts in the Mojave Desert and provided a basalt are high in Mg and low in Si, Al, Ca, viable theory for the sequence of lava at Na, and K. The nodules are xenomorphic Pisgah Crater. Most petrologists agree that granular with a tectonite fabric and forsteritic basalt forms in the upper mantle (for example, olivine (F094-88). The Sr87/Sr86 ratio of the Green and Ringwood, 1967; Jackson and nodules is 0.7043 + 0.0008. -
About Our Mineral World
About Our Mineral World Compiled from series of Articles titled "TRIVIAL PURSUITS" from News Nuggets by Paul F. Hlava "The study of the natural sciences ought to expand the mind and enlarge the ability to grasp intellectual problems." Source?? "Mineral collecting can lead the interested and inquisitive person into the broader fields of geology and chemistry. This progression should be the proper outcome. Collecting for its own sake adds nothing to a person's understanding of the world about him. Learning to recognize minerals is only a beginning. The real satisfaction in mineralogy is in gaining knowledge of the ways in which minerals are formed in the earth, of the chemistry of the minerals and of the ways atoms are packed together to form crystals. Only by grouping minerals into definite categories is is possible to study, describe, and discuss them in a systematic and intelligent manner." Rock and Minerals, 1869, p. 260. Table of Contents: AGATE, JASPER, CHERT AND .............................................................................................................................2 GARNETS..................................................................................................................................................................2 GOLD.........................................................................................................................................................................3 "The Mystery of the Magnetic Dinosaur Bones" .......................................................................................................4 -
Trace Element Fractionation in Alkaline OIB
Genesis of primitive Hawaiian rejuvenated-stage lavas: Evidence for carbonatite metasomatism and implications for ancient eclogite source Anastassia Y. Borisova 1,2* 1 Géosciences Environnement Toulouse, GET - UMR 5563 - OMP - CNRS, 14 Avenue E. Belin, 31400 Toulouse, France 2 Geological Department, Lomonosov Moscow State University, MGU, Vorobievu Gori, 119991, Moscow, Russia (revised version, 12/03/2020, for Geochemistry Geophysics Geosystems) *Corresponding author: E-mail: [email protected]; *Corresponding adresse: Géosciences Environnement Toulouse UMR 5563, Observatoire Midi Pyrénées, 14 Avenue E. Belin, 31400 Toulouse, France; Tel: +33(0)5 61 54 26 31; Fax: +33(0)5 61 33 25 60 Abstract – To constrain a contribution of deep carbonated mantle, to fractionation of Hf relative to rare earth elements (REE) in volcanic series, we examine available high-quality data on major, trace element and Nd-Hf isotope compositions of ~280 primitive lavas and glasses (MgO = 8.5 – 21 wt%, SiO2 = 37 - 50 wt%) erupted during preshield, postshield and mostly rejuvenated stage of the Hawaiian hot spot (Pacific Ocean). Strong variations of Hf/Sm, Zr/Sm, Ti/Eu, K/Th, Nb/Th, La/K and Ba/K in the lavas are not features of the melt equilibration with residual amphibole or phlogopite, and cannot be due to variable degrees of batch or dynamic melting of uncarbonated lherzolite source. Enrichment in REE, Th and Ba relative to K, Hf, Zr, Ti and Nb together and low Si, high Na, K and Ca contents in the Hawaiian lavas are compositional features of carbonated mantle lithospheric to asthenospheric peridotite source affected by carbonatite metasomatism at temperatures higher than 1100°C and pressures higher than 2 GPa. -
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. -
Conditions for Melting and Metasomatism in the Earth's Mantle
GEOLOGICKÝ ZBORNÍK — GEOLOGICA CARPATHICA, 36, 3, BRATISLAVA, JUNE 10(15, Pp. 323—335 PETER J. WYLLIE* CONDITIONS FOR MELTING AND METASOMATISM IN THE EARTH'S MANTLE (Figs. 6) Abstract: If we know the compositions of mantle rocks at various depths, ajnd the geotherm in different tectonic environments, then the conditions for melting are defined by experimentally determined solidus curves. The term "metasomatism" in crustal processes is defined as reac tion by solution or vapors, not by melts or magmas, and the same de finition should apply to mantle processes (reaction with magmas is "hybridization"). HiO, C02, or both are made available for metasomatic reaction at deep dissociation fronts, or by solidification of volatile-charged magmas. Regions eligible for metasomatism are limited by solidus curves above which the melts dissolve volatile components. Beneath the litho- sphere, there can be no metasomatism between about 120 and 260 km, because melting intervenes. Solidification of kimberlitic magmas at the base of continental lithosphere is a source of metasomatic fluids. Mantle metasomatism is expected in several regions above subducted oceanic lithosphere, interspersed with magmatic events. Major differentiation of the Earth is accomplished by melting, but metasomatism may cause signi ficant redistribution of some elements. Pe3K)Me: ECJIH H3BecTHM cocraBbi noKpbmaioiUHX nopofl B pa3Hbix rjiyÔHHax H reoTepMa B pa3iibix TeicroHHiecKHX cpeaax, noTOM ycjioBHH nJiaBnemw onpeflejiH- K3TCH 3KCnepHMeHTaJTbH0 Ha3HaieHHblMH KpHBblMH COJIHfla. TepMHH „MeTacoMa- TH3M" B npoueccax Kopu onpeaejiaeTCH KaK peaKuHH npoxofl^inaa npw noMomif pacTBopenHS HJIH nap, He paconaBOB HJIH Martu, H TaKyio 5Ke flettiHHHqHio MOÄHO npHMeHHTb HJIH npoueccoB MaHTHH (peaKUHeR c ManviaMH !\Bnftejcn ,,rH6pH/;H3auHH"). H„0, CO; HJIH 06a coe/THHenHsi npHroflHM una MeTacoiviaTHMeCKHX peaKunři B rxiy- ÔOKHX cjjpoHTax flHccouHauHH HJIH 3aTBepneBanHeM jieTywx Manvi. -
Nomenclature of the Garnet Supergroup
American Mineralogist, Volume 98, pages 785–811, 2013 IMA REPORT Nomenclature of the garnet supergroup EDWARD S. GREW,1,* ANDREW J. LOCOCK,2 STUART J. MILLS,3,† IRINA O. GALUSKINA,4 EVGENY V. GALUSKIN,4 AND ULF HÅLENIUS5 1School of Earth and Climate Sciences, University of Maine, Orono, Maine 04469, U.S.A. 2Department of Earth and Atmospheric Sciences, University of Alberta, Edmonton, Alberta T6G 2E3, Canada 3Geosciences, Museum Victoria, GPO Box 666, Melbourne 3001, Victoria, Australia 4Faculty of Earth Sciences, Department of Geochemistry, Mineralogy and Petrography, University of Silesia, Będzińska 60, 41-200 Sosnowiec, Poland 5Swedish Museum of Natural History, Department of Mineralogy, P.O. Box 50 007, 104 05 Stockholm, Sweden ABSTRACT The garnet supergroup includes all minerals isostructural with garnet regardless of what elements occupy the four atomic sites, i.e., the supergroup includes several chemical classes. There are pres- ently 32 approved species, with an additional 5 possible species needing further study to be approved. The general formula for the garnet supergroup minerals is {X3}[Y2](Z3)ϕ12, where X, Y, and Z refer to dodecahedral, octahedral, and tetrahedral sites, respectively, and ϕ is O, OH, or F. Most garnets are cubic, space group Ia3d (no. 230), but two OH-bearing species (henritermierite and holtstamite) have tetragonal symmetry, space group, I41/acd (no. 142), and their X, Z, and ϕ sites are split into more symmetrically unique atomic positions. Total charge at the Z site and symmetry are criteria for distinguishing groups, whereas the dominant-constituent and dominant-valency rules are critical in identifying species. Twenty-nine species belong to one of five groups: the tetragonal henritermierite group and the isometric bitikleite, schorlomite, garnet, and berzeliite groups with a total charge at Z of 8 (silicate), 9 (oxide), 10 (silicate), 12 (silicate), and 15 (vanadate, arsenate), respectively. -
Garnets from the Camafuca-Camazambo Kimberlite (Angola)
Anais da Academia Brasileira de Ciências (2006) 78(2): 309-315 (Annals of the Brazilian Academy of Sciences) ISSN 0001-3765 www.scielo.br/aabc Garnets from the Camafuca-Camazambo kimberlite (Angola) EUGÉNIO A. CORREIA and FERNANDO A.T.P. LAIGINHAS Departamento de Geologia, Faculdade de Ciências da Universidade do Porto Praça de Gomes Teixeira, 4050 Porto, Portugal Manuscript received on November 17, 2004; accepted for publication on June 13, 2005; presented by ALCIDES N. SIAL ABSTRACT This work presents a geochemical study of a set of garnets, selected by their colors, from the Camafuca- Camazambo kimberlite, located on northeast Angola. Mantle-derived garnets were classified according to the scheme proposed by Grütter et al. (2004) and belong to the G1, G4, G9 and G10 groups. Both sub-calcic (G10) and Ca-saturated (G9) garnets, typical, respectively, of harzburgites and lherzolites, were identified. The solubility limit of knorringite molecule in G10D garnets suggests they have crystallized at a minimum pressure of about 40 to 45 kbar (4– 4.5 GPa). The occurrence of diamond stability field garnets (G10D) is a clear indicator of the potential of this kimberlite for diamond. The chemistry of the garnets suggests that the source for the kimberlite was a lherzolite that has suffered a partial melting that formed basaltic magma, leaving a harzburgite as a residue. Key words: kimberlite, diamond, garnet, lherzolite, harzburgite. INTRODUCTION GEOCHEMICAL STUDY OF GARNETS The Camafuca-Camazambo kimberlite belongs to The geochemical study of mantle-derived garnets a kimberlite province comprising over a dozen of occurring in kimberlites progressed remarkably in primary occurrences of diamond, located along- recent years, as their chemistry is not only a possible side the homonymous brook which is a tributary of indicator of the presence of diamonds in their host the Chicapa river, in the proximity of the Calonda rock but also their abundance is a likely indicator of village, northeast Angola (Fig. -
Cr3+ in Phyllosilicates
Mineral Spectroscopy: A Tribute to Roger G. Bums © The Geochemical Society, Special Publication No.5, ]996 Editors: M. D. Dyar, C. McCammon and M. W. Schaefer 3 Cr + in phyllosilicates: Influence of the nature of coordinating ligands and their next cationic neighbors on the crystal field parameters I 2 2 A. N. PLATONOV , K. LANGER , M. ANDRUT .3, G. CALAS4 'Institute of Geochemistry, Mineralogy and Ore Formation, Academy of Science of Ukraine, 252680 Kiev, Ukraine 2Institute of Mineralogy and Crystallography, Technical University, D-10623 Berlin, Germany 3GeoForschungszentrum Potsdam, D-14473 Potsdam, Deutschland "Laboratoire de Mineralogie et de Cristallographie, Universite de Paris 6 et 7, F-7525l Paris, France 3 Abstract- The electronic absorption spectra of Cr + -bearing clinochlore (I, kammererite), amesite (II), muscovite (III, fuchsite), dickite (IV), and montmorillonite (V, volkonskite) analysed by electron microprobe were obtained on single crystals. Microscope-spectrometric techniques and polarized radiation in the spectral range 10000-38000 cm " (I, II, III) or (on fine grained material) diffuse reflectance spectrometry in the spectral range 8000-50000 cm-I (IV, V) were used. The ligand field theoretical evaluation of the spectra showed the following: (i) The fl.o = 10Dq = f(1/R5) relation, wherein fl.o is the octahedral crystal field parameter and R the mean cation ligand distance, is valid within each series of layer silicates containing octahedral Cr3+ either in a trioctahedral layer (I, II and phlogopite) or in a dioctahedral layer (III, IV, V). Between the two functions, fl.o.trioct = f(1lR~ioct) and fl.o.di=t = f(1/R~ioct), there exists an energy difference of about 2200 em -I. -
Partitioning of Chromium Between Garnet and Clinopyroxene: first-Principle Modelling Versus Metamorphic Assemblages
Eur. J. Mineral., 32, 387–403, 2020 https://doi.org/10.5194/ejm-32-387-2020 © Author(s) 2020. This work is distributed under the Creative Commons Attribution 4.0 License. Partitioning of chromium between garnet and clinopyroxene: first-principle modelling versus metamorphic assemblages Sarah Figowy, Benoît Dubacq, Yves Noël, and Philippe d’Arco Sorbonne Université, CNRS-INSU, Institut des Sciences de la Terre de Paris, ISTeP UMR 7193, 75005 Paris, France Correspondence: Sarah Figowy (sarah.fi[email protected]) Received: 30 December 2019 – Revised: 28 May 2020 – Accepted: 15 June 2020 – Published: 3 July 2020 Abstract. Understanding the geochemical behaviour of trace and minor elements in mineral assemblages is of primary importance to study small- and large-scale geological processes. Partition coefficients are frequently used to model the chemical evolution of minerals and fluids during melting and in metamorphic rocks of all grades. However, kinetic effects hampering equilibrium partitioning may invalidate the modelling. This study aims at calculating partition coefficients and testing their applicability in natural mineral assemblages, choosing Cr in garnet and clinopyroxene via exchange with Al as a case study. First-principle modelling has been com- bined with measurements and element mapping to estimate partition coefficients for Cr and the deviation from equilibrium. Results highlight the role of crystal chemistry over the strain field around point defects, controlling the dynamics of the Cr3C D Al3C exchange between clinopyroxene and garnet. Ab initio calculations allowed estimation of Cr partition coefficients between garnet and clinopyroxene, using a thermodynamic approach based on endmembers and mixing models simplified for trace element behaviour.