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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. -
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. -
Geomorphology of the Bushveld Complex
Cademo Lab. Xeo16xico de Laxe Coruña. 1997. Vol. 22, pp. 209-227 Geomorphology of the Bushveld Complex Geomorfología del Complejo de Bushveld LAGEAT,Y. This paper deals wich che differenc relacion becween scruccure and lichology in che geomorphology of che Bushveld Complexo The final resules demonscrace chac, even so differenc scale ofsize, widerfor che epirogenic-cecconic movements and smaller for che lichology, che cwo faccors need co be considered for a beccer underscanding ofche landscape evolucion ofche area. Key words: ulerabasic and basic rocks, Bushveld Complex, scruccural geomorphology, lichological differences. LAGEAT, Y. (Universicé Blaise Pascaland UPRES-A 6042 (CNRS). Clermont-Ferrand (France) 210 Lageat, Y. CAD. LAB. XEOL. LAXE 22 (997) INTRODUCTION subdued topography. So, being concerned with the relationships between scenery and In spiteofthestrong emphasisonclimatic structure, the study wil1 consider two topics in French geomorphology since the different but complementary topics: fifties, research dealing with structural differential erosion and regional evolution landforms developed in crystalline shields ofa shield area (Y. LAGEAT, 1989). pioneered by the late Professor P. Birot has been upheld. In numerous regional monographs, widely distributed between GEOLOGICAL POTENTIAL theArcticCircleand theTropicofCapricorn, special attention has been devoted to the A presentation of the geology of the relationships between landforms and Bushveld Complex is essential to any geological structure, with the purpose to understanding of its surface morphology. distinguish between the direct control of Ranging in composition from ultrabasic ro recent faulting and the response of acid, it outcrops largely within a region contrasting rock units todifferential erosiono covered bya characteristicvegetation termed This ambiguity may be easily overcome in «Bushveld». -
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. -
The Nain Anorthosite Project, Labrador: Field
THE NAIN ANORTHOSITE PROJECT, LABRADOR: FIELD REPORT 1971 S. A. MORSE I EDITOR R. V. PITS I ULAK CONTRIBUTION NO. 9 GEOLOGY DEPARTMENT UNIVERSITY OF MASSACHUSETTS AMHERST, MASSACHUSETTS L THE NAIN ANORTHOSITE PROJECT, LABRADOR: FIElD REPORT 1971 S. A. Morse, Editor Final Report under NSF Grants GA-21386 and GA-27134 to Franklin and Marshall College: "Evolution of Anorthosite and Related Crustal Rocks in Coastal Labrador", and "Facility for Crustal Studies in Coastal Labrador." S. A. Morse, Principal Investigator (now at U.Mass/Amherst) Dirk de Waard, Syracuse Associate Investigators E. P. Wheeler 2nd, Cornell Other contributors: Research Assistants: J. H. Berg, U. Mass/Amherst C. D. Brauer, Vassar G. A. Plananaky, Harvard F. Finley, Syracuse C. C. Rubins, Syracuse T. H. Folkomer, Franklin & Marshall B.G.J. Upton, Edinburgh D. Russell, Syracuse Charles Woodward, Syracuse J. A. Speer, Virginia Polytechnic Contribution No. 9 Amherst, Massachusetts Geology Department December, 1971 Uni~ersity of Massachusetts L I - CONTENTS INTRODUCTION •••••••••.•••••.•••••••••• ......................... 1 GEOLOGIC~ REPORT. • • • • • • • . • • . • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • • 9 General Statement ••••••• 9 Collateral Studies •• 12 Eastern Con tact Zone . .....................................•.... 15 Country rocks of the anorthosite massif and anorthosite contacts in the Ford Harbour Region (de Waard) ••••••••••••••••••••• 15 Intrusive contact relations in the outer is lands (Wlleele r) .................................... -
62237 Troctolitic Anorthosite 62.4 Grams
62237 Troctolitic Anorthosite 62.4 grams Figure 1: Photo of 62237. NASA S72-41797 (B&W), NASA S72-38959 (color). Cube is 1 cm. Introduction 62237 and 62236 are chalky white rocks that were Warren and Wasson (1977) concluded that 62237 is collected together along with 62235 and incidental soil, “chemically pristine”, because it was lacking in from the rim of Buster Crater, station 2, Apollo 16 meteoritic siderophiles. (figure 2), where they were found half buried in the regolith (Sutton 1981). The mineral chemistry of these 62237 has been crushed to form a cataclastic texture, rocks is similar and indicates that they belong to the but, in places, the original coarse-grained igneous suite of lunar plutonic rocks termed ferroan anorthosite texture can be discerned by relic clasts (figure 3). (James 1980). Mineralogy Olivine: Olivine (Fo ) crystals up to 3 mm in size Petrography 59-61 Dymek et al. (1975) concluded that 62237 was a slowly are reported in 62237 by Dymek et al. (1975). Warren cooled plutonic lunar rock (figure 1). The mineralogy and Wasson (1977) and Bersch et al. (1991) also of 62237 is that of a ferroan anorthosite with fairly provided analyses of olivine in 62237. Dymek et al. abundant (~20%) mafic minerals (figure 5). noted that olivine in 62237 was extremely depleted in Ca. Lunar Sample Compendium C Meyer 2011 Figure 2: Location of 62237. Pyroxene: Dymek et al. (1975) and Bersch et al. (1991) determined the composition of pyroxene in 62237 (figure 4). Plagioclase: Plagioclase in 62237 is An95-99 and contains only small amount of minor elements (Dymek et al. -
Nickel Content of an Alaskan Basic Rock
If yon do not need this publication after it has served your purpose, please return it to the Geological Survey, using the official mailing label at the end UNITED STATES DEPARTMENT OF THE INTERIOR Harold L. Ickes, Secretary GEOLOGICAL SURVEY W. C. Mendenhall, Director Bulletin 897 D NICKEL CONTENT OF AN ALASKAN BASIC ROCK BY JOHN C. REED Mineral resources of Alaska, 1936 (Pages 263-268) UNITED STATES GOVERNMENT PRINTING OFFICE WASHINGTON : 1939 ?For sale by the Superintendent of Documents, Washington, D. C. ....... Price 5 cent! CONTENTS Page- Abstract__----------__...__-_--_--__--___-._--_._..__.____ 265 Location and general features.__--_--_------__-_-__---_-_--___-_-___ 263 Petrographic studies-______-_-__---_--_-----___---_--_-__-____-____ 265- Chemical analyses----___-_-__-_-_--__-_---_-____-_____-___________ 267 Conclusions_ _ ___-_________________-_____-_--_-____-___--___----__ 268- ILLUSTRATION Page FIGURE 11. Index map showing location of nickel-bearing sill on Admiralty Island.. ....... ______________--..________ 264 NICKEL CONTENT OF AN ALASKAN BASIC ROCK By JOHN C. REED ABSTRACT A nickel-bearing sill, about 126 feet thick, lies in a thick sequence of greenstone schists, graphitic phyllites, and quartzites near the north end of Admiralty Island not far from Juneau, Alaska. Petrographic measurements show that volumetrically the rock is made up of about 62.07 percent labradprite, 34.22 percent olivine, 2.42 percent pyroxene, 0.79 percent pyrrhotite, 0.21 percent magnetite, 0.14 percent chalcopyrite, and 0.06 percent pentlandite. -
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. -
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. -
Anorthosite-Gabbro-Granophyte Relationships, Mount Sheridan Area
RICE UNIVERSITY ANORTHOSITE-GABBRO-GRANOPHYRE RELATIONSHIPS, MOUNT SHERIDAN AREA, OKLAHOMA by EDWARD C. THORNTON A THESIS SUBMITTED IN PARTIAL FULFILLMENT OF THE REQUIREMENTS FOR THE DEGREE OF MASTER OF ARTS Thesis Director's Signature: Houston, Texas May, 1975 ABSTRACT ANORTHOSITE-GABBRO-GRANOPHYRE RELATIONSHIPS MOUNT SHERIDAN AREA, OKLAHOMA Edward C. Thornton Field work, phase analysis by microprobe, petrography, and oxygen isotope analysis have been undertaken in an ef¬ fort to establish the relationships among the anorthositic, gabbroic, and granophyric rocks of the Mount Sheridan area in southwestern Oklahoma. The gabbro has been found to be somewhat finer-grained when in contact with the anorthosite. Petrographically, the gabbro is quite different from the anorthosite. The anorthosite is essentially a one-pyroxene rock (clinopy- roxene) while the gabbro contains both augite and hyper- sthene. Quartz, micropegmatite, and biotite are present in the gabbro but essentially absent in the anorthosite. The anorthosite is a cumulate rock with well-developed igneous lamination whereas the gabbro is generally not laminated. The above information established that the anorthosite is the older unit and that the gabbro was sub¬ sequently intruded into it. The gabbro is transitional into the overlying grano- phyre through a zone of intermediate rock. The zone of transition has been found to extend into the gabbro itself as has been determined by phase analysis, in addition, diabasic inclusions are present in the granophyre - evi¬ dence of possible mixing of basaltic and granophyric magma. These observations suggest that gabbroic and granophyric magmas were emplaced simultaneously at Mount Sheridan and that the intermediate rock between the gabbro and grano¬ phyre may have been generated by mixing of the two magma types.