Two Expressions of the Transition from Mafic Cumulates To
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45. Myrmekite Formed by Na- and Ca-Metasomatism of K- Feldspar
1 ISSN 1526-5757 45. Myrmekite formed by Na- and Ca-metasomatism of K- feldspar Jiashu RONG Beijing Research Institute of Uranium Geology P.O. Box 9818, Beijing, 100029 Peoples Republic of China Email address: [email protected] September 23, 2002 Abstract Myrmekite, an intergrowth of plagioclase and quartz vermicules, often occurs in felsic-to-intermediate, calc-alkalic plutonic and gneissic rocks. Several hypotheses for myrmekite genesis are briefly reviewed and discussed. The proportional relationship between the volume of quartz vermicules and the An value of plagioclase is consistent with the hypothesis or replacement, solid state exsolution, and recrystallization of primary plagioclase. (1) Perthitic albite and K- feldspar relicts in myrmekite and (2) swapped myrmekite between two differently oriented K-feldspar crystals obviously indicate that myrmekite is formed by nibble replacement of K-feldspar by myrmekitic plagioclase because of modification by Ca-bearing sodic emanation or fluid. Myrmekite of different morphology and spatial distribution are of the same metasomatic origin. The myrmekite that was produced during deformation should be later than that formed prior to deformation. Characteristics of myrmekite Myrmekite was first described by Michel-Lévy (1874) and named by Sederholm (1897) as an intergrowth of plagioclase and quartz vermicules. Myrmekite is commonly observed in felsic-to-intermediate calc-alkalic granitic rocks (but not in alkalic-tending plutonic rocks) and in granitic gneisses of similar composition. 2 On the basis of the geologic environment, Phillips (1974) classified myrmekite in the following ways: 1. rim myrmekite, occurring at the contact of plagioclase with another differently oriented K-feldspar; 2. intergranular myrmekite, situated at the boundary between two differently oriented K-feldspars; 3. -
The Rustenburg Layered Suite Formed As a Stack of Mush with Transient Magma Chambers ✉ Zhuosen Yao1, James E
ARTICLE https://doi.org/10.1038/s41467-020-20778-w OPEN The Rustenburg Layered Suite formed as a stack of mush with transient magma chambers ✉ Zhuosen Yao1, James E. Mungall 1 & M. Christopher Jenkins 1 The Rustenburg Layered Suite of the Bushveld Complex of South Africa is a vast layered accumulation of mafic and ultramafic rocks. It has long been regarded as a textbook result of fractional crystallization from a melt-dominated magma chamber. Here, we show that most 1234567890():,; units of the Rustenburg Layered Suite can be derived with thermodynamic models of crustal assimilation by komatiitic magma to form magmatic mushes without requiring the existence of a magma chamber. Ultramafic and mafic cumulate layers below the Upper and Upper Main Zone represent multiple crystal slurries produced by assimilation-batch crystallization in the upper and middle crust, whereas the chilled marginal rocks represent complementary supernatant liquids. Only the uppermost third formed via lower-crustal assimilation–fractional crystallization and evolved by fractional crystallization within a melt-rich pocket. Layered intrusions need not form in open magma chambers. Mineral deposits hitherto attributed to magma chamber processes might form in smaller intrusions of any geometric form, from mushy systems entirely lacking melt-dominated magma chambers. 1 Department of Earth Sciences, Carleton University, 2115 Herzberg Laboratories, 1125 Colonel By Drive, Ottawa, ON K1S 5B6, Canada. ✉ email: [email protected] NATURE COMMUNICATIONS | (2021) 12:505 | https://doi.org/10.1038/s41467-020-20778-w | www.nature.com/naturecommunications 1 ARTICLE NATURE COMMUNICATIONS | https://doi.org/10.1038/s41467-020-20778-w ayered mafic intrusions represent portions of the plumbing derived by incremental crystallization must be removed. -
Guidebook for Field Trips for the Thirty-Fifth Annual Meeting of the North-Central Section of the Geological Society of America
Guidebook for Field Trips for the Thirty-Fifth Annual Meeting of the North-Central Section of the Geological Society of America April 23-24, 2001 David Malone, Editor ISGS Guidebook 33 2001 George H. Ryan, Governor Department of Natural Resources ILLINOIS STATE GEOLOGICAL SURVEY William W. Shilts, Chief EDITOR'S MESSAGE Greetings from the Executive Committee of the North Central Section of the Geological Society of America! As geologists, we all recognize the great importance of field experiences. This year's meeting includes a diverse and excellent set of field trips. Collectively, this year's field trips visit a broad spectrum of the geologic features of Illinois and Missouri that range in age from Precambrian to Quaternary. These trips present a number of new ideas and interpretations that will broaden the perspectives of all field trip participants. Your participation, interaction, and exchange of ideas with the field trip leaders are encouraged at all times These trips are the culmination of the time and energy freely given by a number of individuals. I would like to thank and recognize the field trip leaders for their hard work in planning the field trips and preparing the individual field guides. I would also like to thank the technical reviewers at Illinois State University and the Illinois State Geological Survey for their efforts. I appreciate the efforts of Jon Goodwin and the publication staff at the Illinois State Geological Survey for their substantial work in preparing this field guide. A special thanks goes out to the property owners who have been most helpful in planning these trips. -
The Nakhlite Meteorites: Augite-Rich Igneous Rocks from Mars ARTICLE
ARTICLE IN PRESS Chemie der Erde 65 (2005) 203–270 www.elsevier.de/chemer INVITED REVIEW The nakhlite meteorites: Augite-rich igneous rocks from Mars Allan H. Treiman Lunar and Planetary Institute, 3600 Bay Area Boulevard, Houston, TX 77058-1113, USA Received 22 October 2004; accepted 18 January 2005 Abstract The seven nakhlite meteorites are augite-rich igneous rocks that formed in flows or shallow intrusions of basaltic magma on Mars. They consist of euhedral to subhedral crystals of augite and olivine (to 1 cm long) in fine-grained mesostases. The augite crystals have homogeneous cores of Mg0 ¼ 63% and rims that are normally zoned to iron enrichment. The core–rim zoning is cut by iron-enriched zones along fractures and is replaced locally by ferroan low-Ca pyroxene. The core compositions of the olivines vary inversely with the steepness of their rim zoning – sharp rim zoning goes with the most magnesian cores (Mg0 ¼ 42%), homogeneous olivines are the most ferroan. The olivine and augite crystals contain multiphase inclusions representing trapped magma. Among the olivine and augite crystals is mesostasis, composed principally of plagioclase and/or glass, with euhedra of titanomagnetite and many minor minerals. Olivine and mesostasis glass are partially replaced by veinlets and patches of iddingsite, a mixture of smectite clays, iron oxy-hydroxides and carbonate minerals. In the mesostasis are rare patches of a salt alteration assemblage: halite, siderite, and anhydrite/ gypsum. The nakhlites are little shocked, but have been affected chemically and biologically by their residence on Earth. Differences among the chemical compositions of the nakhlites can be ascribed mostly to different proportions of augite, olivine, and mesostasis. -
A Petrologic and Geochemical Study of Granophyric Granite in the Roof of the Keweenawan Duluth Complex, Eagle Mountain, Cook County, Minnesota
A PETROLOGIC AND GEOCHEMICAL STUDY OF GRANOPHYRIC GRANITE IN THE ROOF OF THE KEWEENAWAN DULUTH COMPLEX, EAGLE MOUNTAIN, COOK COUNTY, MINNESOTA A Thesis Submitted to the Faculty of the Graduate School of the University of Minnesota By Nancy Nelson In Partial Fulfillment of the Requirements for the Degree of Master of Science April, 1991 ABSTRACT Field work in the roof zone of the Keweenawan (1.1 b.y.) Duluth Complex in the area of Eagle Mountain, Cook County, Minnesota, resulted in the identification of eight major rock units. These are metabasalt, metagabbro, ophitic diabase, syenogabbro, ferrodiorite, rhyolite, and two distinct granophyre units. On the basis of field relations and petrography, the rhyolite appears to be the oldest unit in the area and to have formed the roof rocks below which the intrusive units were emplaced. The metabasalt unit is composed of xenoliths of basalt that were carried and slightly metamorphosed by the magma now represented by the metagabbro unit. This metagabbro was emplaced beneath the rhyolite and later slightly metamorphosed by the intrusion of the magma that formed the Eagle Mountain granophyre. The Eagle Mountain granophyre shares a gradational contact with the ferrodiorite, and these two units appear to be genetically related. The relationship of the syenogabbro to other units is unknown. The miarolitic granophyre was intruded beneath the rhyolite, but its age relation to other units is ambiguous. The ophitic diabase crosscuts other units and appears to be the youngest unit in the field area. The Eagle Mountain granophyre (EMG) is red-brown, fine-grained, porphyritic, and locally granophyric and spherulitic. -
Igneous Intrusive Rocks of the Peake and Denison Ranges Within the Adelaide Geosyncline
tl-io' -GIÜEOIJS IìÜTFÈIJSIVE R.OCKS OF TI;IE PE.ã,KE .ã.¡ÜED DEDÜTSO¡Ü FI.ãNGES T'i'ITIT-¡Ü 1FI:[E .â'EDEI,.â'IDE GEOSYIÜCI,IìÜE \/OLL[&fE I f = Figrures, Plates, Captions, Irfaps, Tabl.es and Appendicies. By: Robert Sinclair Irlorrison B.Sc. (Acadia, L98L) B.Sc. Hons. (Adelaide, 1982) The Department of Geology and Geophysics The University of Adelaide South Australia. This thesis is submitted as fulfilment of the requirements for the degree of Doctor of Philosophy in GeologY at The University of Adelaide South Australia. February 298à, l-988. Resubmitted March 3L-t, 1989. n¡ q: t c! Jr '"f.' .''ì r ll,r.-¡. lci- I\ \, \ , .' ì T.ã.BI,E OF COIÜTEIÜTS Chapter One: Symopsis of tlre Adelaide Geoslmcline. Figure 1.1: General Geology of Èhe Adelaide Geosynclj-ne. Figure L.2= Structural Geology of the Adelaide Geosybcline. Figure l-.3: Stratigraphic Nomenclature for the Adelaide Geosyncline. Figure L.5.4: Cross-Section of Adelaidean Evaporite Deformation. Plate 1.1-: Diapiric Breccia. Plate L.2z Diapiric Breccia and Contacts. Table L.3.1: RepresentaÈive Geochemistry of Callanna Group Volcanics in the Adelaide Geosyncline. Table 1.3.2: Representative Geochemistry of Burra Group Volcanics in the Adelaide Geosyncline. Table 1.3.3: Representative Geochernistry of the Umberatana Group Volcanic Equivalents. Table l-. 3.5: Representative Geochemistry of Moralana Supergroup Volcanics in the Adelaide Geosyncline. Chapter thtos Igmeous Intn¡sions of the Adelaide Geoslmcline: A Revies. Figure 2.Lz lgneous Rocks of the Adelaide Geosyncline and Kanmantoo Trough. Figure 2.7.1-'. Geology of a Northern Section in the willouran Ranges. -
Komatiites of the Weltevreden Formation, Barberton Greenstone
Louisiana State University LSU Digital Commons LSU Doctoral Dissertations Graduate School 2005 Komatiites of the Weltevreden Formation, Barberton Greenstone Belt, South Africa: implications for the chemistry and temperature of the Archean mantle Keena Kareem Louisiana State University and Agricultural and Mechanical College, [email protected] Follow this and additional works at: https://digitalcommons.lsu.edu/gradschool_dissertations Part of the Earth Sciences Commons Recommended Citation Kareem, Keena, "Komatiites of the Weltevreden Formation, Barberton Greenstone Belt, South Africa: implications for the chemistry and temperature of the Archean mantle" (2005). LSU Doctoral Dissertations. 3249. https://digitalcommons.lsu.edu/gradschool_dissertations/3249 This Dissertation is brought to you for free and open access by the Graduate School at LSU Digital Commons. It has been accepted for inclusion in LSU Doctoral Dissertations by an authorized graduate school editor of LSU Digital Commons. For more information, please [email protected]. KOMATIITES OF THE WELTEVREDEN FORMATION, BARBERTON GREENSTONE BELT, SOUTH AFRICA: IMPLICATIONS FOR THE CHEMISTRY AND TEMPERATURE OF THE ARCHEAN MANTLE A Dissertation Submitted to the Graduate Faculty of the Louisiana State University and Agricultural and Mechanical College in partial fulfillment of the requirements for the degree of Doctor of Philosophy in The Department of Geology and Geophysics by Keena Kareem B.S., Tulane University, 1999 May 2005 ACKNOWLEDGMENTS The author wishes to thank, Dr. Gary Byerly, the author’s major advisor for guidance and support in defining the project, technical assistance with instrumentation, and practical advice concerning non-dissertation related issues. Appreciation goes out to the other members of the advisory committee: Drs. Huiming Bao, Lui-Heung Chan, Ray Ferrell, Darrell Henry, of the Department of Geology and Geophysics, and Dr. -
General Geological Setting and the Structural Features of the Guleman Peridotite Unit and the Chromite Deposits (Elaziğ, Eastern Turkey)
GENERAL GEOLOGICAL SETTING AND THE STRUCTURAL FEATURES OF THE GULEMAN PERIDOTITE UNIT AND THE CHROMITE DEPOSITS (ELAZIĞ, EASTERN TURKEY) Tandoğan ENGİN*; Mehmet BALCI*; Yücel SÜMER* and Yusuf Z. ÖZKAN* ABSTRACT. — The Guleman peridotite unit covering an area of about 200 km2 is made up of tectonite and cumulate rock groups. Tectonite forms 65 %, the remainder being cumulates. Cumulates broadly encircle and rest on tectonites. Both groups of rocks include chromite deposits but those found in tectonites are far more important than the others. The mineralogy and petrology of the peridotites is briefly described. A thick dunite unit in the Kef area is defined as a transition zone between cumulate and tectonite on the basis of field relations and textural features they ex- hibit. Batı Kef which is one of the major chromite deposit in the area is situated at the base of this thick dunite unit. Numbers of major chromite deposits are located in harzburgite with a thin dunite envelope around them. Chromite de- posits in Guleman are classified as alpine or podiform type but they demonstrate extensive continuation along their strike as well as dip directions. The peridotile unit dealt with here presents rather orderly internal structural patterns. Layering and foliation in the peridotite are invariably found parallel to each other. Chromite bodies which have primary contact relations with the host peridotite are also parallel to the layering and foliation, thus the chromite bodies themselves form an important element in the internal structure of the peridotite. Chromite deposits have been divided into groups on the basis of the local lithological and structural characters of the host peridotite and the characteristic features of the chromite deposits themselves. -
Resources in the Upper Zone of the Bushveld Complex, South Africa
Papers and Proceedings of the Royal Society of Tasmania, Volume 150(1), 2016 15 Fe-Ti-V-(P) RESOURCES IN THE UPPER ZONE OF THE BUSHVELD COMPLEX, SOUTH AFRICA by L.A. Fischer and Q. Yuan (with four text-figures and two plates) Fischer, L.A. & Yuan, Q. 2016 (31:viii): Fe-Ti-V-(P) resources in the Upper Zone of the Bushveld Complex, South Africa. Papers and Proceedings of the Royal Society of Tasmania 150(1): 15–22. https://doi.org/10.26749/rstpp.150.1.15 ISSN 0080-4703. Institut für Mineralogie, Leibniz Universität Hannover, 30167 Hannover, Germany, and School of Physical Sciences, University of Tasmania, Hobart, Tasmania 7001, Australia (LAF*); Faculty of Earth Resources, China University of Geosciences, Wuhan 430074, China, and Department of Geology, University of Liege, 4000 Sart Tilman, Belgium (QY). *Author for correspondence. Email: [email protected] The Bushveld Complex in South Africa is the largest layered intrusion on Earth. Its upper part is known for huge resources of iron, tita- nium, vanadium and phosphorus. Associated with the layered character of the rocks, these resources are enriched at certain levels of the intrusion, which makes it important to understand the formation processes of those layers. In this paper we give an introduction and overview of recent debates and challenges. Key Words: layered intrusion, Bushveld, resources. INTRODUCTION Fe, Ti, V and P never or only rarely occur as native elements in nature. Minerals, rich in one or more of these Iron (Fe), titanium (Ti) and vanadium (V) are important elements are mined and their components are extracted. -
Bedrock Geology of the Cape St. Mary's Peninsula
BEDROCK GEOLOGY OF THE CAPE ST. MARY’S PENINSULA, SOUTHWEST AVALON PENINSULA, NEWFOUNDLAND (INCLUDES PARTS OF NTS MAP SHEETS 1M/1, 1N/4, 1L/16 and 1K/13) Terence Patrick Fletcher Report 06-02 St. John’s, Newfoundland 2006 Department of Natural Resources Geological Survey COVER The Placentia Bay cliff section on the northern side of Hurricane Brook, south of St. Bride’s, shows the prominent pale limestones of the Smith Point Formation intervening between the mudstones of the Cuslett Member of the lower Bonavista Formation and those of the overlying Redland Cove Member of the Brigus Formation. The top layers of this marker limestone on the southwestern limb of the St. Bride’s Syncline contain the earliest trilobites found in this map area. Department of Natural Resources Geological Survey BEDROCK GEOLOGY OF THE CAPE ST. MARY’S PENINSULA, SOUTHWEST AVALON PENINSULA, NEWFOUNDLAND (INCLUDES PARTS OF NTS MAP SHEETS 1M/1, 1N/4, 1L/16 and 1K/13) Terence P. Fletcher Report 06-02 St. John’s, Newfoundland 2006 EDITING, LAYOUT AND CARTOGRAPHY Senior Geologist S.J. O’BRIEN Editor C.P.G. PEREIRA Graphic design, D. DOWNEY layout and J. ROONEY typesetting B. STRICKLAND Cartography D. LEONARD T. PALTANAVAGE T. SEARS Publications of the Geological Survey are available through the Geoscience Publications and Information Section, Geological Survey, Department of Natural Resources, P.O. Box 8700, St. John’s, NL, Canada, A1B 4J6. This publication is also available through the departmental website. Telephone: (709) 729-3159 Fax: (709) 729-4491 Geoscience Publications and Information Section (709) 729-3493 Geological Survey - Administration (709) 729-4270 Geological Survey E-mail: [email protected] Website: http://www.gov.nl.ca/mines&en/geosurv/ Author’s Address: Dr. -
The Geology of the Eastern Mellen Intrusive Complex, Wisconsin
THE GEOLOGY OF THE EASTERN MELLEN INTRUSIVE COMPLEX, WISCONSIN by 1 2 David E. Tabet and Joel R. Mangham ABSTRACT The eastern Mellen intrusive complex is a slightly discordant, sill like layered intrusive located on the southern limb of the Lake Superior syncline. It is approximately 37 km long and as much as 6 km thick. The Mellen granite stock separates the eastern part of the complex from the Mineral Lake Intrusion, the western half of the complex. Primary planar strucutres in the complex indicate that it has a northeasterly strike and dips steeply to the northwest. At least three separate intrusive sequences of basaltic magma were emplaced one on top of another to form the Mellen complex. Each sequence developed an olivine-rich lower part and a plagioclase-rich upper part as a result of crystal settling. Density currents produced rhythmic layering in the olivine gabbros and troctolites. The first two, or lowest sequences, contain mostly gabbroic rocks while the third also contains more highly indifferentiated rocks including monzogabbro and granophyre. Emplacement of each sequence took place after the preceding one had solidified, but the lack of chilled margins between them suggests that the earlier bodies were still hot at the time of subsequent intrusions. Intrusion of the eastern complex occurred near the close of Middle Keweeawan extrusive activity. The complex was emplaced in the slowly sub siding southern limb of the Lake Superior syncline when the tilt of that limb was probably less than 10° to 15° to the northwest. No evidence for thrust faulting was found in Or at the base of the complex. -
Some Geochemical Data of the Mafic-Ultramafic Complex at Tulu Dimitri, Ethiopia, and Their Genetic Significance
ZOBODAT - www.zobodat.at Zoologisch-Botanische Datenbank/Zoological-Botanical Database Digitale Literatur/Digital Literature Zeitschrift/Journal: Sitzungsberichte der Akademie der Wissenschaften mathematisch-naturwissenschaftliche Klasse Jahr/Year: 1982 Band/Volume: 191 Autor(en)/Author(s): Warden Arthur J., Kazmin V., Kiesl W., Pohl Walter Artikel/Article: Some Geochemical Data of the Mafic-Ultramafic Complex at Tulu Dimitri, Ethiopia, and their Genetic Significance. 111-131 Some Geochemical©Akademie d. Wissenschaften Wien; Data download ofunter thewww.biologiezentrum.at Mafic-Ultramafic Complex at Tulu Dimitri, Ethiopia, and their Genetic Significance By A. J. W a r d e n * ), V. K a z m i n * ), W . K i e s l *) and W . P o h l *) With 13 Figures (Vorgelegt in der Sitzung der mathem.-naturw. Klasse am 11. März 1982 durch das w. M. W . Pe t r a s c h e k ) Abstract The Upper Proterozoic Western Volcanic Belt of Ethiopia contains at Tulu Dimitri an elongate mafic-ultramafic complex, which was interpreted earlier on field evidence as an ophiolite. In view of the important regional tectonic implications a confirmation was sought by carrying out geochemical analyses on a small suite of representative rocks of the complex. The chemical data confirm the ophiolitic identity of the Tulu Dimitri complex. REE-contents differ, however, from published standards. Zusammenfassung Der jung-proterozoische westliche Vulkanitgürtel in Äthiopien enthält bei Tulu Dimitri einen länglichen mafisch-ultramafischen Komplex, der vor kurzem auf Grund geologischer Feldarbeit als Ophiolit interpretiert wurde. Da dies wichtige Konsequenzen für die Deutung der regionalen geologischen Zusammenhänge hat, wurde eine Überprüfung dieser Interpretation durch gesteinsgeochemische Analysen einer Anzahl repräsentativer Proben aus dem Komplex durchgeführt.