Amphibole Crystallization Conditions As Record of Interaction Between
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AMPHIBOLES: Crystal Chemistry, Occurrence, and Health Issues
AMPHIBOLES: Crystal Chemistry, Occurrence, and Health Issues 67 Reviews in Mineralogy and. Geochemistry 67 TABLE OF CONTENTS 1 Amphiboles: Crystal Chemistry Frank C. Hawthorne, Roberta Oberti INTRODUCTION 1 CHEMICAL FORMULA 1 SOMi : ASPECTS OF CHEMICAL ANALYSIS 1 Chemical composition 1 Summary 6 CALCULATION OF THE CHEMICAL FORMULA 7 24 (O, OH, F, CI) 7 23 (O) 8 13 cations 8 15 cations 8 16 cations 8 Summary 8 AMPIIIBOI I S: CRYSTAL STRUCTURE 8 Space groups 9 Cell dimensions 9 Site nomenclature 9 The C2/m amphibole structure 10 The P2/m amphibole structure 12 The P2/a amphibole structure 12 The Pnma amphibole structure 12 The Pnmn amphibole structure 14 The C1 amphibole structure 17 STACKING SEQUENCES AND SPACE GROUPS 18 BOND LENGTHS AND BOND VALENCES IN [4IA1-FREE AMPHIBOLES 19 THE DOUBLE-CHAIN OF TETRAHEDRA IN [4IA1 AMPHIBOLES 19 Variation in <T-0> bondlengths in C2/m amphiboles 21 Variation in <T-0> bondlengths in Pnma amphiboles 25 THE STEREOCHEMISTRY OF THE STRIP OF OCTAHEDRA 27 The C2/m amphiboles: variation in mean bondlengths 27 The Pnma amphiboles with B(Mg,Fe,Mn): variation in mean bondlengths 30 v Amphiboles - Table of Contents The Pnma amphiboles with BLi: variation in mean bondlengths 32 THE STEREOCHEMISTRY OF THE M (4) SITE 34 The calcic, sodic-calcic and sodic amphiboles 35 Amphiboles with small B cations (magnesium-iron-manganese- lithium, magnesium-sodium and lithium-sodium) 36 The C2/m amphiboles: variation in <M(4)-0> bondlengths 36 The Pnma amphiboles: variation in <MA-0> bondlengths 36 I III! STEREOCHEMISTRY OF THE A SITE 37 The C2/m amphiboles 37 The PU a amphibole 40 The Pnma amphiboles 40 The Pnmn amphiboles 41 THE STEREOCHEMISTRY OF THE 0(3) SITE 41 The C2/m amphiboles 41 UNIT-CELL PARAMETERS AND COMPOSITION IN C2/m AMPHIBOLES 42 SUMMARY 46 ACKNOWLEDGMENTS 46 REFERENCES 47 APPENDIX 1: CRYSTAL-STRUCTURE REFINEMENTS OF AMPHIBOLE 51 Z Classification of the Amphiboles Frank C. -
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 -
Module 7 Igneous Rocks IGNEOUS ROCKS
Module 7 Igneous Rocks IGNEOUS ROCKS ▪ Igneous Rocks form by crystallization of molten rock material IGNEOUS ROCKS ▪ Igneous Rocks form by crystallization of molten rock material ▪ Molten rock material below Earth’s surface is called magma ▪ Molten rock material erupted above Earth’s surface is called lava ▪ The name changes because the composition of the molten material changes as it is erupted due to escape of volatile gases Rocks Cycle Consolidation Crystallization Rock Forming Minerals 1200ºC Olivine High Ca-rich Pyroxene Ca-Na-rich Amphibole Intermediate Na-Ca-rich Continuous branch Continuous Discontinuous branch Discontinuous Biotite Na-rich Plagioclase feldspar of liquid increases liquid of 2 Temperature decreases Temperature SiO Low K-feldspar Muscovite Quartz 700ºC BOWEN’S REACTION SERIES Rock Forming Minerals Olivine Ca-rich Pyroxene Ca-Na-rich Amphibole Na-Ca-rich Continuous branch Continuous Discontinuous branch Discontinuous Biotite Na-rich Plagioclase feldspar K-feldspar Muscovite Quartz BOWEN’S REACTION SERIES Rock Forming Minerals High Temperature Mineral Suite Olivine • Isolated Tetrahedra Structure • Iron, magnesium, silicon, oxygen • Bowen’s Discontinuous Series Augite • Single Chain Structure (Pyroxene) • Iron, magnesium, calcium, silicon, aluminium, oxygen • Bowen’s Discontinuos Series Calcium Feldspar • Framework Silicate Structure (Plagioclase) • Calcium, silicon, aluminium, oxygen • Bowen’s Continuous Series Rock Forming Minerals Intermediate Temperature Mineral Suite Hornblende • Double Chain Structure (Amphibole) -
Optical Properties of Common Rock-Forming Minerals
AppendixA __________ Optical Properties of Common Rock-Forming Minerals 325 Optical Properties of Common Rock-Forming Minerals J. B. Lyons, S. A. Morse, and R. E. Stoiber Distinguishing Characteristics Chemical XI. System and Indices Birefringence "Characteristically parallel, but Mineral Composition Best Cleavage Sign,2V and Relief and Color see Fig. 13-3. A. High Positive Relief Zircon ZrSiO. Tet. (+) 111=1.940 High biref. Small euhedral grains show (.055) parallel" extinction; may cause pleochroic haloes if enclosed in other minerals Sphene CaTiSiOs Mon. (110) (+) 30-50 13=1.895 High biref. Wedge-shaped grains; may (Titanite) to 1.935 (0.108-.135) show (110) cleavage or (100) Often or (221) parting; ZI\c=51 0; brownish in very high relief; r>v extreme. color CtJI\) 0) Gamet AsB2(SiO.la where Iso. High Grandite often Very pale pink commonest A = R2+ and B = RS + 1.7-1.9 weakly color; inclusions common. birefracting. Indices vary widely with composition. Crystals often euhedraL Uvarovite green, very rare. Staurolite H2FeAI.Si2O'2 Orth. (010) (+) 2V = 87 13=1.750 Low biref. Pleochroic colorless to golden (approximately) (.012) yellow; one good cleavage; twins cruciform or oblique; metamorphic. Olivine Series Mg2SiO. Orth. (+) 2V=85 13=1.651 High biref. Colorless (Fo) to yellow or pale to to (.035) brown (Fa); high relief. Fe2SiO. Orth. (-) 2V=47 13=1.865 High biref. Shagreen (mottled) surface; (.051) often cracked and altered to %II - serpentine. Poor (010) and (100) cleavages. Extinction par- ~ ~ alleL" l~4~ Tourmaline Na(Mg,Fe,Mn,Li,Alk Hex. (-) 111=1.636 Mod. biref. -
(Fe-Mg Amphibole) in Plutonic Rocks of Nahuelbuta Mountains
U N I V E R S I D A D D E C O N C E P C I Ó N DEPARTAMENTO DE CIENCIAS DE LA TIERRA 10° CONGRESO GEOLÓGICO CHILENO 2003 THE OCCURRENCE AND THERMAL DISEQUILIBRIUM OF CUMMINGTONITE IN PLUTONIC ROCKS OF NAHUELBUTA MOUNTAINS CREIXELL, C.(1*); FIGUEROA, O.(1); LUCASSEN, F.(2,3), FRANZ, G.(4) & VÁSQUEZ, P.(1) (1)Universidad de Concepción, Chile, Depto. Ciencias de la Tierra, Barrio Universitario s/n, casilla 160-C (2)Freie Universität Berlin, FB Geowissenschaften, Malteserstr. 74-100, 12249 Berlin, Germany (3)GeoForschungsZentrum Potsdam, Telegrafenberg, 14473 Potsdam, Germany; [email protected] (4)TU-Berlin, Petrologie-EB15, Strasse des 17.Juni 135, 10623 Berlin, Germany; *Present Address: MECESUP-Universidad de Chile, Depto. de Geología, Plaza Ercilla 803, casilla 13518, [email protected] INTRODUCTION The “cummingtonite series” (Leake, 1978) are characterised by magnesio-cummingtonite (Mg7Si8O22(OH)2) and grunerite (Fe7Si8O22(OH)2) end-members. Cummingtonite is mainly produced under amphibolite-facies conditions, but the entire stability range cover at least a field of 400 to 800° C, at pressures between <1 to 15 kbar (Evans and Ghiorso, 1995, Ghiorso et al., 1995). Natural cummingtonite occurs in several metamorphic rock types (i.e. Kisch & Warnaars, 1969, Choudhuri, 1972) and also can coexist with incipient melt in high-grade gneisses in deep- crustal levels (Kenah and Hollister, 1983). For igneous rocks, cummingtonite had been described in some rhyolites at Taupo Zone, New Zealand (Wood & Carmichael, 1973) and as a stable phase in plutonic rocks (e.g. Bues et al., 2002). In the present study, we describe the occurrence of cummingtonite in Upper Palaeozoic plutonic rocks and their amphibolite xenoliths from the Nahuelbuta Mountains, south central Chile (37°-38°S, for location see fig. -
Wang Et Al., 2001
American Mineralogist, Volume 86, pages 790–806, 2001 Characterization and comparison of structural and compositional features of planetary quadrilateral pyroxenes by Raman spectroscopy ALIAN WANG,* BRAD L. JOLLIFF, LARRY A. HASKIN, KARLA E. KUEBLER, AND KAREN M. VISKUPIC Department of Earth and Planetary Sciences and McDonnell Center for the Space Sciences, Washington University, St. Louis, Missouri 63130, U.S.A. ABSTRACT This study reports the use of Raman spectral features to characterize the structural and composi- tional characteristics of different types of pyroxene from rocks as might be carried out using a por- table field spectrometer or by planetary on-surface exploration. Samples studied include lunar rocks, martian meteorites, and terrestrial rocks. The major structural types of quadrilateral pyroxene can be identified using their Raman spectral pattern and peak positions. Values of Mg/(Mg + Fe + Ca) of pyroxene in the (Mg, Fe, Ca) quadrilateral can be determined within an accuracy of ±0.1. The preci- sion for Ca/(Mg + Fe + Ca) values derived from Raman data is about the same, except that correc- tions must be made for very low-Ca and very high-Ca samples. Pyroxenes from basalts can be distinguished from those in plutonic equivalents from the distribution of their Mg′ [Mg/(Mg + Fe)] and Wo values, and this can be readily done using point-counting Raman measurements on unpre- pared rock samples. The correlation of Raman peak positions and spectral pattern provides criteria to distinguish pyroxenes with high proportions of non-quadrilateral components from (Mg, Fe, Ca) quadrilateral pyroxenes. INTRODUCTION pyroxene group of minerals is amenable to such identification Laser Raman spectroscopy is well suited for characteriza- and characterization. -
Pyroxenes, Amphibole, and Mica from the Tiree Marble. 1 (With Plate XIV.)
230 Pyroxenes, amphibole, and mica from the Tiree marble. 1 (With Plate XIV.) By A. F. HALLIMOND,M.A., Sc.D. With chemical analyses by C. O. HARVEY, B.Sc., A.R.C.S. [Read March 27, 1947.] I. INTRODUCTION. HE Tiree pink marble, a fine-grained, severely crushed limestone T with evidence of earlier coarse crystallization, is exposed in several small areas up to 100 feet across on the farm of Balephetrish near the north coast of the island of Tiree in the Hebrides. It contains a r~mark- able quantity of dark silicate minerals and has discordant contacts with the adjacent Lewisian gneiss. The precise nature of its relation to the gneiss, and mode of emplacement, have been much discussed. ~ The writer has been permitted to consult accounts of the literature, by Mr. V. A. Eyles, and of the petrography, by Sir Edward B. Bailey, and is also indebted to those authors for discussion of the problems. At the suggestion of Sir Edward Bailey the present work was undertaken as a contribution to the study of this problem from the mineralogical point of view. Most of the determinations were made in 1938, but it was not possible to complete publication at that time. Scattered somewhat evenly throughout the carbonate groundmass of the marble are numerous dark green crystalline patches which usually do not exceed half an inch across and are often much smaller; locally, however, there are pieces of dark gneiss-like rock of much larger size. The majority consist of pyroxene, sometimes accompanied by amphi- bole, &c., and the latter were regarded by Coom~rasw~my and others as modified gneiss inclusions. -
Crystallization and Metasomatism of Nepheline Syenite Xenoliths in Quartz-Bearing Intrusive Rocks in the Permian Oslo Rift, SE Norway
Crystallization and metasomatism of nepheline syenite xenoliths in quartz-bearing intrusive rocks in the Permian Oslo rift, SE Norway TOM ANDERSEN & HENNING SØRENSEN Andersen, T. & Sørensen, H.: Crystallization and metasomatism of nepheline syenite xenoliths in quartz-bearing intrusive rocks in the Permian Oslo rift, SE Norway. Norsk Geologisk Tidsskrift, Vol. 73, pp. 250-266. Oslo 1993. ISSN 0029-196X. Small bodies of metasomatized nepheline syenite occur as xenoliths in syenitic and granitic intrusions in the Mykle area, ca. 30 km N of the Larvik pluton in the Vestfold Graben of the late Paleozoic Qslo rift of SE Norway. The nepheline syenite has a metaluminous major element composition, and its primary igneous mineralogy is: alkali feldspar + nepheline + clinopyroxene + titanite + magnetite + apatite ± amphibole. The mafic silicate minerals have lower (Na + K)/AI than comparable minerals in other fe lsic intrusions in the Oslo Rift. Gamet (grossular-andradite), analcime, sodalite, thomsonite and gonnardite occur as interstitial minerals in the )east altered parts of the nepheline syenite. The xenoliths were metasomatized as a result of interaction between nepheline syenite and younger silica-saturated to oversaturated magrnas and their associated fluids. Early, pervasive metasomatism led to breakdown of nepheline, replacement of pyroxene by biotite ± garnet and crystallization of quartz. Recrystallization took place at solidus-near temperatures (700-725°C), and was controlled by an increase in silica activity and oxygen fugacity. Titanite + magnetite were replaced by rutile + quartz + hematite + calcite at a late stage of the metasomatic history, at oxygen fugacities above the HM buffer, and T < 450°C. The xenoliths indicate the former presence of larger bodies of nepheline syenite in an area where no such rocks were known previously. -
A Systematic Nomenclature for Metamorphic Rocks
A systematic nomenclature for metamorphic rocks: 1. HOW TO NAME A METAMORPHIC ROCK Recommendations by the IUGS Subcommission on the Systematics of Metamorphic Rocks: Web version 1/4/04. Rolf Schmid1, Douglas Fettes2, Ben Harte3, Eleutheria Davis4, Jacqueline Desmons5, Hans- Joachim Meyer-Marsilius† and Jaakko Siivola6 1 Institut für Mineralogie und Petrographie, ETH-Centre, CH-8092, Zürich, Switzerland, [email protected] 2 British Geological Survey, Murchison House, West Mains Road, Edinburgh, United Kingdom, [email protected] 3 Grant Institute of Geology, Edinburgh, United Kingdom, [email protected] 4 Patission 339A, 11144 Athens, Greece 5 3, rue de Houdemont 54500, Vandoeuvre-lès-Nancy, France, [email protected] 6 Tasakalliontie 12c, 02760 Espoo, Finland ABSTRACT The usage of some common terms in metamorphic petrology has developed differently in different countries and a range of specialised rock names have been applied locally. The Subcommission on the Systematics of Metamorphic Rocks (SCMR) aims to provide systematic schemes for terminology and rock definitions that are widely acceptable and suitable for international use. This first paper explains the basic classification scheme for common metamorphic rocks proposed by the SCMR, and lays out the general principles which were used by the SCMR when defining terms for metamorphic rocks, their features, conditions of formation and processes. Subsequent papers discuss and present more detailed terminology for particular metamorphic rock groups and processes. The SCMR recognises the very wide usage of some rock names (for example, amphibolite, marble, hornfels) and the existence of many name sets related to specific types of metamorphism (for example, high P/T rocks, migmatites, impactites). -
The Stability of Amphibole in Andesite and Basalt at High Pressuresr
American Mineralogist, Volume 68, pages 307-314, 1983 The stability of amphibole in andesiteand basalt at high pressuresr J. C. Alt-BN Department of Geology and Geography Bucknell University Lewisburg, Pennsylvania 17837 exo A. L. Bonrrcsen Institute of Geophysics and Planetary Physics and Department of Earth and Space Sciences University of Califurnia, Los Angeles Los Angeles, California 90024 Abstract Some of our earlier work (Allen et al., 1975)on the stability of amphibolesin andesite and basalt at high pressuresis subject to criticism becauseofloss ofiron from the starting material to the walls of the capsules(AgsoPdso) during the runs of/6, bufered over the range of stability of magnetite.Analyses of fused run products show substantialloss of iron from runs at magnetite-wiistite and nickel-nickel oxide conditions, but none from those at magnetite-hematiteconditions. We have now redone our earlier work on the Mt. Hood andesiteand l92l Kilauea olivine tholeiite under N-NO conditions and with silver capsules.Analyses of fused run products show no iron loss, and the reversed curve representing the maximum stability of the amphibolesin the Mt. Hood andesiteshows no changein location, although we now have better control on the high-pressurepart of this curve. The revised curve for the appetrance of garnet is significantly lower in pressure, passing through 15.5 kbar/940'C and 14.5 kbar/9fi)'C. No orthopyroxene appearedin the run products, in contrast to the results of our earlier work. The high-temperature segment of the amphibole-out curve for the tholeiite is at least as high as 1040'Cat 13kbar and 1050"Cat 16kbar, and the high-pressure part of this curve is at about 27 kbars, about 6 kbar higher than in our earlier work. -
Structure and Metamorphic Petrology of the Forth Metamorphic Complex
STRUCTURE AND METAMORPHIC PETROLOGY OF THE FORTH METAMORPHIC COMPLEX ROB LEWIS A research thesis submitted in partial fulfilment of ~e degree Bachelor of Science with Honours. Geology department. University of Tasmania 1991 ii ABSTRACT The Forth Metamorphics outcrop in the lower reaches of the Forth River, Northern Tasmania and comprise a banded garnetiferous schist and quartzite, interlayered with sub-ordinate orthoamphibolites of tholeiitic MORB-type affinity. Geochemical and sedimentological constraints are consistent with a passive continental depositional environment and the sequence has been regionally metamorphosed during a two-phase tectono-metamorphic event. An early isoclinal fold phase (D1) produced a penetrative muscovite foliation but is largely overprinted by the dominant S2 schistosity. High temperature, relatively low strain quartz mylonites developed in narrow zones during west-directed D2 transport and are separated by domains of west vergent isoclinal F2 folds. Microprobe analyses of stable pelitic and metabasite assemblages have been used in conjunction with ( traditional/dataset thermobarometric methods and phase equilibrium constraints to estimate P-T conditions during D2. Peak conditions of 700°C +/- 50° C and 13 kb +/- 2 kb for kyanite-garnet-biotite schists in the Forth Valley are matched by independant estimates for garnet amphibole plagioclase assemblages and the latter preserve an early garnet-clinopyroxene-albite assemblage indicating conditions of 660° C and 11 kb during core growth. These results are supported by semi-quantitative P-T modelling of local calcite-altered garnet clinopyroxene zoisite intetbands, which formed in a locally H20-poor environment during compression/heating from 675° C 9-11 kb to peak conditions of 740° C and 13- 15kb. -
SILICATES MINERALS Sarah Lambart
quartz CHAPTER 8: muscovite SILICATES MINERALS Sarah Lambart olivine epidote beryl amphibole CONTENT CHAPT. 8 (6 LECTURES) Part 1: Orthosilicates (= nesosilicates) Part 2: Sorosilicates & Cyclosilicates Part 3: Chain silicates (= inosilicates) Part 4: Sheet silicates (= Phyllosilicates) Part 5: Framework silicates (= tectosilicates) CLASSIFICATION: STRUCTURAL Why? 1) Silicates have various forms (needles, flakes, cube,…) 4- due to the arrangement of the SiO4 tetrahedra 2) Tetrahedra link via cations: nature of the cation depends on the arrangement of the tetrahedra Nature of the cation: controls some of the physical properties (Ex.: color, density) MAFIC VERSUS FELSIC Mafic silicate: major cation: Mg and Fe (mafic: magnesia; “ferrum”) Ex.: biotite, amphiboles, pyroxenes, olivine Felsic silicates: lack of Fe or Mg as major constituents Ex.: feldspars (from which the name is derived), quartz, muscovite, feldspathoïds. IGNEOUS ROCKS Mostly silicate (O and Si: most abundant element in Earth’s crust) Silicate in igneous rocks: quartz, K-feldspar, plagioclase, muscovite, biotite, Ca-clinoamphibole (e.g.: hornblende), Ca- clinopyroxene (e.g., augite), orthopyroxene and olivine, feldspathoids (e.g., leucite, nepheline) Classification: based on modal mineralogy ↳volume of rock occupied by each mineral: obtained by “point counting” Streckheisen classification: based on modal mineralogy ↳volume of rock occupied by each mineral: obtained by “point counting” Mostly for felsic plutonic rocks because - grains in volcanic rocks are often