Crustal Structure of the Southern Margin of the African Plate: Results
Total Page:16
File Type:pdf, Size:1020Kb

Load more
Recommended publications
-
The Western Branch of the East African Rift: a Review of Tectonics, Volcanology and Geothermal Activity
Presented at SDG Short Course IV on Exploration and Development of Geothermal Resources, organized by UNU-GTP and KenGen, at Lake Bogoria and Lake Naivasha, Kenya, Nov. 13 – Dec. 3, 2019. THE WESTERN BRANCH OF THE EAST AFRICAN RIFT: A REVIEW OF TECTONICS, VOLCANOLOGY AND GEOTHERMAL ACTIVITY Björn S. Hardarson Iceland GeoSurvey (ÍSOR) Grensásvegur 9, 108 Reykjavik ICELAND [email protected] ABSTRACT The East African Rift System (EARS) is a classic example of continental rifting and provides an excellent framework to study extensional magmatism and the evolution of several central volcanic systems that have formed along the rift from the Tertiary to Recent. Many of the volcanic structures have developed substantial high-temperature geothermal systems where the heat source is magmatic and related to central volcanoes. Detailed studies indicate that the geothermal potential in Eastern Africa is in the excess of 15,000 MWe. However, despite the high geothermal potential of EARS only Kenya has installed significant capacity of about 570 MW. Magmatism along the EARS is generally believed to be associated with mantle plume activities but the number and nature of mantle plumes is still, however, controversial. EARS is divided into two main branches, the Eastern- and Western rifts, and it is well documented that significantly greater volcanism is observed in the older Eastern rift (i.e. Ethiopia and Kenya) compared to that in the younger Western rift, where eruptive activity is, in general, restricted to four spatially distinct provinces along the rift axis. These are the Toro-Ankole in western Uganda, the Virunga and Kivu provinces along the border of the DRC with Uganda, Rwanda and Burundi, and the Rungwe volcanic field in SW Tanzania. -
Exkursionen Excursions
EXKURSIONEN EXCURSIONS 174 MITT.ÖSTERR.MINER.GES. 161 (2015) A GEOLOGICAL EXCURSION TO THE MINING AREAS OF SOUTH AFRICA by Aberra Mogessie, Christoph Hauzenberger, Sara Raic, Philip Schantl, Lukas Belohlavek, Antonio Ciriello, Donia Daghighi, Bernhard Fercher, Katja Goetschl, Hugo Graber, Magdalena Mandl, Veronika Preissegger, Gerald Raab, Felix Rauschenbusch, Theresa Sattler, Simon Schorn, Katica Simic, Michael Wedenig & Sebastian Wiesmair Institute of Earth Sciences, University of Graz, Universitaetsplatz 2, A-8010 Graz Frank Melcher, Walter Prochaska, Heinrich Mali, Heinz Binder, Marco Dietmayer-Kräutler, Franz Christian Friedman, Maximilian Mathias Haas, Ferdinand Jakob Hampl, Gustav Erwin Hanke, Wolfgang Hasenburger, Heidi Maria Kaltenböck, Peter Onuk, Andrea Roswitha Pamsl, Karin Pongratz, Thomas Schifko, Sebastian Emanuel Schilli, Sonja Schwabl, Cornelia Tauchner, Daniela Wallner & Juliane Hentschke Chair of Geology and Economic Geology, Mining University of Leoben, Peter-Tunner-Strasse 5, A-8700 Leoben Christoph Gauert Department of Geology, University of the Free State, South Africa 1. Preface Almost a year ago Aberra Mogessie planned to organize a field excursion for the students of the Institute of Earth Sciences, University of Graz. The choices were Argentina, Ethiopia (where we had organized past excursions) and South Africa. Having discussed the matter with Christoph Hauzenberger concerning geology, logistics etc. we decided to organize a field excursion to the geologically interesting mining areas of South Africa. We contacted Christoph Gauert from the University of Free State, South Africa to help us with the local organization especially to get permission from the different mining companies to visit their mining sites. We had a chance to discuss with him personally during his visit to our institute at the University of Graz in May 2014 and make the first plan. -
Footprint of a Late Carboniferous Ice Sheet D.P
https://doi.org/10.1130/G46590.1 Manuscript received 3 June 2019 Revised manuscript received 31 July 2019 Manuscript accepted 7 August 2019 © 2019 The Authors. Gold Open Access: This paper is published under the terms of the CC-BY license. Published online 23 September 2019 Scratching the surface: Footprint of a late Carboniferous ice sheet D.P. Le Heron1, P. Dietrich2,3, M.E. Busfield4, C. Kettler1, S. Bermanschläger1 and B. Grasemann1 1 Department für Geodynamik und Sedimentologie, Althanstraße 14, Universität Wien, 1190 Vienna, Austria 2 Department of Geology, University of Johannesburg, Auckland Park Kingsway Campus, Johannesburg 2092, South Africa 3 Géosciences Rennes, UMR6118, Université de Rennes 1, 263 Avenue du Général Leclerc, Bâtiment 15, Campus de Beaulieu, 35042 Rennes Cedex, France 4 Department of Geography and Earth Sciences, Aberystwyth University, Llandinam Building, Aberystwyth SY23 3DB, UK ABSTRACT records deglaciation punctuated by short-term Field observations in conjunction with aerial images from an unmanned aerial vehicle stillstands and minor readvances (Dietrich and were used to create the first map of a glacial unconformity underlying the late Carboniferous Hofmann, 2019). Such basin-margin locali- Dwyka Group of South Africa. Crosscutting relationships reveal that the glacial unconformity ties record glacially striated pavements of two at Oorlogskloof, in which flutes, grooves, and striae were ploughed into unconsolidated sand, types: (1) hard-bedrock pavements, recording formed in a three-phased process charting a periodic shift in the locus of subglacial erosion. the direct abrasion of LPIA ice sheets onto The unconformity formed by a periodically decoupled ice sheet in a probable tidewater set- hard bedrock material (Du Toit, 1954; Visser ting. -
Africa-Arabia-Eurasia Plate Interactions and Implications for the Dynamics of Mediterranean Subduction and Red Sea Rifting
This page added by the GeoPRISMS office. Africa-Arabia-Eurasia plate interactions and implications for the dynamics of Mediterranean subduction and Red Sea rifting Authors: R. Reilinger, B. Hager, L. Royden, C. Burchfiel, R. Van der Hilst Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA USA, [email protected], Tel: (617)253 -7860 This page added by the GeoPRISMS office. Our proposed GeoPRISMS Initiative is based on the premise that understanding the mechanics of plate motions (i.e., the force balance on the plates) is necessary to develop realistic models for plate interactions, including processes at subduction and extensional (rifting) plate boundaries. Important advances are being made with new geologic and geophysical techniques and observations that are providing fundamental insights into the dynamics of these plate tectonic processes. Our proposed research addresses directly the following questions identified in the GeoPRISMS SCD Draft Science Plan: 4.2 (How does deformation across the subduction plate boundary evolve in space and time, through the seismic cycle and beyond?), 4.6 (What are the physical and chemical conditions that control subduction zone initiation and the development of mature arc systems?), and 4.7 (What are the critical feedbacks between surface processes and subduction zone mechanics and dynamics?). It has long been recognized that the Greater Mediterranean region provides a natural laboratory to study a wide range of geodynamic processes (Figure 1) including ocean subduction and continent- continent collision (Hellenic arc, Arabia-Eurasia collision), lithospheric delamination (E Turkey High Plateau, Alboran Sea/High Atlas), back-arc extension (Mediterranean basins, including Alboran, Central Mediterranean, Aegean), “escape” tectonics and associated continental transform faulting (Anatolia, North and East Anatolian faults), and active continental and ocean rifting (East African and northern Red Sea rifting, central Red Sea and Gulf of Aden young ocean rifting). -
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. -
The Sauropodomorph Biostratigraphy of the Elliot Formation of Southern Africa: Tracking the Evolution of Sauropodomorpha Across the Triassic–Jurassic Boundary
Editors' choice The sauropodomorph biostratigraphy of the Elliot Formation of southern Africa: Tracking the evolution of Sauropodomorpha across the Triassic–Jurassic boundary BLAIR W. MCPHEE, EMESE M. BORDY, LARA SCISCIO, and JONAH N. CHOINIERE McPhee, B.W., Bordy, E.M., Sciscio, L., and Choiniere, J.N. 2017. The sauropodomorph biostratigraphy of the Elliot Formation of southern Africa: Tracking the evolution of Sauropodomorpha across the Triassic–Jurassic boundary. Acta Palaeontologica Polonica 62 (3): 441–465. The latest Triassic is notable for coinciding with the dramatic decline of many previously dominant groups, followed by the rapid radiation of Dinosauria in the Early Jurassic. Among the most common terrestrial vertebrates from this time, sauropodomorph dinosaurs provide an important insight into the changing dynamics of the biota across the Triassic–Jurassic boundary. The Elliot Formation of South Africa and Lesotho preserves the richest assemblage of sauropodomorphs known from this age, and is a key index assemblage for biostratigraphic correlations with other simi- larly-aged global terrestrial deposits. Past assessments of Elliot Formation biostratigraphy were hampered by an overly simplistic biozonation scheme which divided it into a lower “Euskelosaurus” Range Zone and an upper Massospondylus Range Zone. Here we revise the zonation of the Elliot Formation by: (i) synthesizing the last three decades’ worth of fossil discoveries, taxonomic revision, and lithostratigraphic investigation; and (ii) systematically reappraising the strati- graphic provenance of important fossil locations. We then use our revised stratigraphic information in conjunction with phylogenetic character data to assess morphological disparity between Late Triassic and Early Jurassic sauropodomorph taxa. Our results demonstrate that the Early Jurassic upper Elliot Formation is considerably more taxonomically and morphologically diverse than previously thought. -
Geological Evolution of the Red Sea: Historical Background, Review and Synthesis
See discussions, stats, and author profiles for this publication at: https://www.researchgate.net/publication/277310102 Geological Evolution of the Red Sea: Historical Background, Review and Synthesis Chapter · January 2015 DOI: 10.1007/978-3-662-45201-1_3 CITATIONS READS 6 911 1 author: William Bosworth Apache Egypt Companies 70 PUBLICATIONS 2,954 CITATIONS SEE PROFILE Some of the authors of this publication are also working on these related projects: Near and Middle East and Eastern Africa: Tectonics, geodynamics, satellite gravimetry, magnetic (airborne and satellite), paleomagnetic reconstructions, thermics, seismics, seismology, 3D gravity- magnetic field modeling, GPS, different transformations and filtering, advanced integrated examination. View project Neotectonics of the Red Sea rift system View project All content following this page was uploaded by William Bosworth on 28 May 2015. The user has requested enhancement of the downloaded file. All in-text references underlined in blue are added to the original document and are linked to publications on ResearchGate, letting you access and read them immediately. Geological Evolution of the Red Sea: Historical Background, Review, and Synthesis William Bosworth Abstract The Red Sea is part of an extensive rift system that includes from south to north the oceanic Sheba Ridge, the Gulf of Aden, the Afar region, the Red Sea, the Gulf of Aqaba, the Gulf of Suez, and the Cairo basalt province. Historical interest in this area has stemmed from many causes with diverse objectives, but it is best known as a potential model for how continental lithosphere first ruptures and then evolves to oceanic spreading, a key segment of the Wilson cycle and plate tectonics. -
The Structure and Transport of the Agulhas Return Current
The Structure and Transport of the Agulhas Return Current Isabelle Jane Ansorge Submitted in fulfillment of the requirements of the Master of Science degree Department of Oceanography University of Cape Town 1996 University of Cape Town The copyright of this thesis vests in the author. No quotation from it or information derived from it is to be published without full acknowledgement of the source. The thesis is to be used for private study or non- commercial research purposes only. Published by the University of Cape Town (UCT) in terms of the non-exclusive license granted to UCT by the author. University of Cape Town I ABSTRACT The Agulhas Current flows along the eastern coast of southern Africa as one of the largest western boundary currents in the world's ocean. On overshooting the southern tip of Africa at approximately 20°E, a retroflection loop is formed that causes the current to double back on itself and to fonn the easterly flowing Agulhas Return Current. No focussed investigation to establish the hydrography of this imponant component of global ocean circulation has to date been carried out. To trace the Agulhas Return Current's passage eastwards into the South Indian Ocean, data collected from six CTD hydrographic cruises; AJAX, ARC, SCARC, Marathon, Discovery 164 and SUZIL, as well as from three XBT temperature cruises,· Marion 83, Gallieni 72 and FIBEX, have been analysed. It is shown that the Agulhas Return Current initially flows zonally from 20°-25°E at a latitude approximately 39°30'-40°30'S before forming a planetary wave over the Agulhas Plateau between 25°-28°E. -
Mafic Dyke Swarm, Brazil: Implications for Archean Supercratons
Michigan Technological University Digital Commons @ Michigan Tech Michigan Tech Publications 12-3-2018 Revisiting the paleomagnetism of the Neoarchean Uauá mafic dyke swarm, Brazil: Implications for Archean supercratons J. Salminen University of Helsinki E. P. Oliveira State University of Campinas, Brazil Elisa J. Piispa Michigan Technological University Aleksey Smirnov Michigan Technological University, [email protected] R. I. F. Trindade Universidade de Sao Paulo Follow this and additional works at: https://digitalcommons.mtu.edu/michigantech-p Part of the Geological Engineering Commons, and the Physics Commons Recommended Citation Salminen, J., Oliveira, E. P., Piispa, E. J., Smirnov, A., & Trindade, R. I. (2018). Revisiting the paleomagnetism of the Neoarchean Uauá mafic dyke swarm, Brazil: Implications for Archean supercratons. Precambrian Research, 329, 108-123. http://dx.doi.org/10.1016/j.precamres.2018.12.001 Retrieved from: https://digitalcommons.mtu.edu/michigantech-p/443 Follow this and additional works at: https://digitalcommons.mtu.edu/michigantech-p Part of the Geological Engineering Commons, and the Physics Commons Precambrian Research 329 (2019) 108–123 Contents lists available at ScienceDirect Precambrian Research journal homepage: www.elsevier.com/locate/precamres Revisiting the paleomagnetism of the Neoarchean Uauá mafic dyke swarm, T Brazil: Implications for Archean supercratons ⁎ J. Salminena,b, , E.P. Oliveirac, E.J. Piispad,e, A.V. Smirnovd,f, R.I.F. Trindadeg a Physics Department, University of Helsinki, P.O. Box -
Variations in the Thickness of the Crust of the Kaapvaal Craton, and Mantle Structure Below Southern Africa
Earth Planets Space, 56, 125–137, 2004 Variations in the thickness of the crust of the Kaapvaal craton, and mantle structure below southern Africa C. Wright, M. T. O. Kwadiba∗,R.E.Simon†,E.M.Kgaswane‡, and T. K. Nguuri∗∗ Bernard Price Institute of Geophysical Research, School of Geosciences, University of the Witwatersrand, Private Bag 3, Wits 2050, South Africa (Received September 17, 2003; Revised March 3, 2004; Accepted March 3, 2004) Estimates of crustal thicknesses using Pn times and receiver functions agree well for the southern part of the Kaapvaal craton, but not for the northern region. The average crustal thicknesses determined from Pn times for the northern and southern regions of the craton were 50.52 ± 0.88 km and 38.07 ± 0.85 km respectively, with corresponding estimates from receiver functions of 43.58 ± 0.57 km and 37.58 ± 0.70 km. The lower values of crustal thicknesses for receiver functions in the north are attributed to variations in composition and metamorphic grade in an underplated, mafic lower crust, resulting in a crust-mantle boundary that yields weak P-to-SV conversions. P and S wavespeeds in the uppermost mantle of the central regions of the Kaapvaal craton are high and uniform with average values of 8.35 and 4.81 km/s respectively, indicating the presence of depleted magnesium-rich peridotite. The presence of a low wavespeed zone for S waves in the upper mantle between depths of 210 and about 345 km that is not observed for P waves was inferred outside the Kaapvaal craton. -
The Role of Fossils in Interpreting the Development of the Karoo Basin
Palaeon!. afr., 33,41-54 (1997) THE ROLE OF FOSSILS IN INTERPRETING THE DEVELOPMENT OF THE KAROO BASIN by P. J. Hancox· & B. S. Rubidge2 IGeology Department, University of the Witwatersrand, Private Bag 3, Wits 2050, South Africa 2Bernard Price Institute for Palaeontological Research, University of the Witwatersrand, Private Bag 3, Wits 2050, South Africa ABSTRACT The Permo-Carboniferous to Jurassic aged rocks oft1:J.e main Karoo Basin ofSouth Africa are world renowned for the wealth of synapsid reptile and early dinosaur fossils, which have allowed a ten-fold biostratigraphic subdivision ofthe Karoo Supergroup to be erected. The role offossils in interpreting the development of the Karoo Basin is not, however, restricted to biostratigraphic studies. Recent integrated sedimentological and palaeontological studies have helped in more precisely defming a number of problematical formational contacts within the Karoo Supergroup, as well as enhancing palaeoenvironmental reconstructions, and basin development models. KEYWORDS: Karoo Basin, Biostratigraphy, Palaeoenvironment, Basin Development. INTRODUCTION Invertebrate remains are important as indicators of The main Karoo Basin of South Africa preserves a facies genesis, including water temperature and salinity, retro-arc foreland basin fill (Cole 1992) deposited in as age indicators, and for their biostratigraphic potential. front of the actively rising Cape Fold Belt (CFB) in Fossil fish are relatively rare in the Karoo Supergroup, southwestern Gondwana. It is the deepest and but where present are useful indicators of gross stratigraphically most complete of several depositories palaeoenvironments (e.g. Keyser 1966) and also have of Permo-Carboniferous to Jurassic age in southern biostratigraphic potential (Jubb 1973; Bender et al. Africa and reflects changing depositional environments 1991). -
Black, R. & J.-P. Liegeois, Cratons, Mobile Belts, Alkaline Rocks And
Journal of the Geological Society, London, Vol. 150, 1993, pp. 89-98, 8 figs. Printed in Northern Ireland Cratons, mobile belts, alkaline rocks and continental lithospheric mantle: the Pan-African testimony R. BLACK l& J.-P. LIEGEOIS 2 1CNRS, URA 736, Laboratoire de Minkralogie, Muskum National d'Histoire Naturelle, 61 rue Buffon, 75005 Paris, France 2Dkpartement de Gkologie (Section de Gkochronologie) Muske Royal de l'Afrique Centrale, 3080 Tervuren, Belgique Abstract: Several late-collision and intraplate features are not entirely integrated in the classical plate tectonic model. The Pan-African orogeny (730-550 Ma) in Saharan Africa provides some insight into the contrasting behaviour of cratons and mobile belts. Simple geophysical considerations and geological observations indicate that rigidity and persistence of cratons are linked to the presence of a thick mechan- ical boundary layer, the upper brittle part of the continental lithospheric mantle, well attached to an ancient weakly radioactive crust. The surrounding Pan-African mobile belts, characterized by a much thinner mechanical boundary layer and more radioactive crust, were the locus of A-type granitoids, volcanism, tectonic reactivation and basin development during the Phanerozoic. During oceanic closures leading to the assembly of Gondwana, lithosphere behaviour was controlled by its mechanical boundary layer, the crust being much less rigid. We suggest that the 5000 km wide Pan-African domain of Saharan Africa, a collage of juvenile and old reactivated basement terranes,