The Role of Fossils in Interpreting the Development of the Karoo Basin
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
On the Stratigraphic Range of the Dicynodont Taxon Emydops (Therapsida: Anomodontia) in the Karoo Basin, South Africa
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Wits Institutional Repository on DSPACE On the stratigraphic range of the dicynodont taxon Emydops (Therapsida: Anomodontia) in the Karoo Basin, South Africa Kenneth D. Angielczyk1*, Jörg Fröbisch2 & Roger M.H. Smith3 1Department of Earth Sciences, University of Bristol, Wills Memorial Building, Queens Road, BS8 1RJ, United Kingdom 2Department of Biology, University of Toronto at Mississauga, 3359 Mississauga Rd., Mississauga, ON, L5L 1C6, Canada 3Divison of Earth Sciences, South African Museum, P.O. Box 61, Cape Town, 8000 South Africa Received 19 May 2005. Accepted 8 June 2006 The dicynodont specimen SAM-PK-708 has been referred to the genera Pristerodon and Emydops by various authors, and was used to argue that the first appearance of Emydops was in the Tapinocephalus Assemblage Zone in the Karoo Basin of South Africa. However, the specimen never has been described in detail, and most discussions of its taxonomic affinities were based on limited data. Here we redescribe the specimen and compare it to several small dicynodont taxa from the Tapinocephalus and Pristerognathus assemblage zones. Although the specimen is poorly preserved, it possesses a unique combination of features that allows it to be assigned confidently to Emydops. The locality data associated with SAM-PK-708 are vague, but they allow the provenance of the specimen to be narrowed down to a relatively limited area southwest of the town of Beaufort West. Strata from the upper Tapinocephalus Assemblage Zone and the Pristerognathus Assemblage Zone crop out in this area, but we cannot state with certainty from which of these biostratigraphic divisions the specimen was collected. -
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. -
South Africa's Coalfields — a 2014 Perspective
International Journal of Coal Geology 132 (2014) 170–254 Contents lists available at ScienceDirect International Journal of Coal Geology journal homepage: www.elsevier.com/locate/ijcoalgeo South Africa's coalfields — A 2014 perspective P. John Hancox a,⁎,AnnetteE.Götzb,c a University of the Witwatersrand, School of Geosciences and Evolutionary Studies Institute, Private Bag 3, 2050 Wits, South Africa b University of Pretoria, Department of Geology, Private Bag X20, Hatfield, 0028 Pretoria, South Africa c Kazan Federal University, 18 Kremlyovskaya St., Kazan 420008, Republic of Tatarstan, Russian Federation article info abstract Article history: For well over a century and a half coal has played a vital role in South Africa's economy and currently bituminous Received 7 April 2014 coal is the primary energy source for domestic electricity generation, as well as being the feedstock for the Received in revised form 22 June 2014 production of a substantial percentage of the country's liquid fuels. It furthermore provides a considerable source Accepted 22 June 2014 of foreign revenue from exports. Available online 28 June 2014 Based on geographic considerations, and variations in the sedimentation, origin, formation, distribution and quality of the coals, 19 coalfields are generally recognised in South Africa. This paper provides an updated review Keywords: Gondwana coal of their exploration and exploitation histories, general geology, coal seam nomenclature and coal qualities. With- Permian in the various coalfields autocyclic variability is the norm rather than the exception, whereas allocyclic variability Triassic is much less so, and allows for the correlation of genetically related sequences. During the mid-Jurassic break up Coalfield of Gondwana most of the coal-bearing successions were intruded by dolerite. -
Topic 10 - Earth's History
Topic 10 - Earth's History 1. Base your answer to the following question on the data table below. The table shows the percentage of original carbon-14 remaining in three different fossils. The approximate ages of the gastropod shell and the tree wood are shown in years. The age of the human bone has been left blank. What is the approximate age of the human bone fossil? A) 5,700 y B) 17,100 y C) 22,800 y D) 39,900 y 2. Carbon-14, an isotope used to date recent organic 6. The photograph below shows the bedrock structure of remains, would most likely be useful in determining a limestone outcrop. the age of a fossil A) trilobite B) Coelophysis C) armored fish D) Beluga whale 3. Approximately how many years ago did the solar system originate? A) 570,000,000 B) 1,000,000,000 C) 4,500,000,000 D) 10,000,000,000 4. Much of the evidence for the evolution of lifeforms on Earth has been obtained by A) studying the life spans of present-day animals B) radioactive dating of metamorphic rock C) correlating widespread igneous ash deposits Which process is responsible for the deformation of D) examining fossils preserved in the rock record this bedrock? 5. Fossil pollen has been recovered from sediments A) folding B) weathering deposited in late-Pleistocene lakes. The pollen’s C) mass movement D) volcanic activity geologic age can most accurately be measured by 7. Which group of organisms survived mass extinctions using that marked the ends of both the Paleozoic Era and A) rubidium-87 B) potassium-40 the Mesozoic Era? C) oxygen-18 D) carbon-14 A) ammonoids B) graptolites C) eurypterids D) gastropods Page 1 Page 1 Topic 10 - Earth's History Base your answers to questions 8 through 10 on the reading passage and the drawing below and on your knowledge of Earth science. -
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. -
A. the Cape Province Fold Belt
SECTION II-A BRIEF SURVEY OF THE GEOLOGY OF THE CAPE SYSTEM A. THE CAPE PROVINCE FOLD BELT 1. Distribution and Folding The main occurrence of the Cape System in South Africa is confined to the Cape Province where a threefold division is recognised, namely the Table Mountain Series, or T.M.S., the Bokkeveld Series and, at the top, the Witte berg Series. The rocks occur along the western and southern margins of the sub-continent (see map on p. 10) where they lie with marked unconformity on older formations with granite intrusives. In the south and southwest, the Cape System dips beneath and is overlain conformably by the tillite of the Dwyka Series which forms the base of the Karroo System, but along the 'western margin the tillite when followed northwards, gradually overlaps the variolls series of the Cape System and finally lies directly on pre-Cape rocks. The whole system has been folded with a general N-S strik on the West and more intensely with a general E-W strike in the south with especially complex crumpling in the SW in the vicinity of Ceres and the Hex River Mountains, where the two fold axes Ineet. The folds in the south are frequently overturned, and are sometimes isoclinal. Usually lateral folds display a fairly teep pitch with the result that they ar hortened, outcrops occur en echelon and a particular horizon may reappear a nwnber of times in a traverse acros the ),stem. Pressure .has resulted in the alteration of organic matter to graphite in many cases and the cOlnplete de truction of micro flora. -
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 Origin and Early Evolution of Dinosaurs
Biol. Rev. (2010), 85, pp. 55–110. 55 doi:10.1111/j.1469-185X.2009.00094.x The origin and early evolution of dinosaurs Max C. Langer1∗,MartinD.Ezcurra2, Jonathas S. Bittencourt1 and Fernando E. Novas2,3 1Departamento de Biologia, FFCLRP, Universidade de S˜ao Paulo; Av. Bandeirantes 3900, Ribeir˜ao Preto-SP, Brazil 2Laboratorio de Anatomia Comparada y Evoluci´on de los Vertebrados, Museo Argentino de Ciencias Naturales ‘‘Bernardino Rivadavia’’, Avda. Angel Gallardo 470, Cdad. de Buenos Aires, Argentina 3CONICET (Consejo Nacional de Investigaciones Cient´ıficas y T´ecnicas); Avda. Rivadavia 1917 - Cdad. de Buenos Aires, Argentina (Received 28 November 2008; revised 09 July 2009; accepted 14 July 2009) ABSTRACT The oldest unequivocal records of Dinosauria were unearthed from Late Triassic rocks (approximately 230 Ma) accumulated over extensional rift basins in southwestern Pangea. The better known of these are Herrerasaurus ischigualastensis, Pisanosaurus mertii, Eoraptor lunensis,andPanphagia protos from the Ischigualasto Formation, Argentina, and Staurikosaurus pricei and Saturnalia tupiniquim from the Santa Maria Formation, Brazil. No uncontroversial dinosaur body fossils are known from older strata, but the Middle Triassic origin of the lineage may be inferred from both the footprint record and its sister-group relation to Ladinian basal dinosauromorphs. These include the typical Marasuchus lilloensis, more basal forms such as Lagerpeton and Dromomeron, as well as silesaurids: a possibly monophyletic group composed of Mid-Late Triassic forms that may represent immediate sister taxa to dinosaurs. The first phylogenetic definition to fit the current understanding of Dinosauria as a node-based taxon solely composed of mutually exclusive Saurischia and Ornithischia was given as ‘‘all descendants of the most recent common ancestor of birds and Triceratops’’. -
A Phylogenetic Analysis of the Basal Ornithischia (Reptilia, Dinosauria)
A PHYLOGENETIC ANALYSIS OF THE BASAL ORNITHISCHIA (REPTILIA, DINOSAURIA) Marc Richard Spencer A Thesis Submitted to the Graduate College of Bowling Green State University in partial fulfillment of the requirements of the degree of MASTER OF SCIENCE December 2007 Committee: Margaret M. Yacobucci, Advisor Don C. Steinker Daniel M. Pavuk © 2007 Marc Richard Spencer All Rights Reserved iii ABSTRACT Margaret M. Yacobucci, Advisor The placement of Lesothosaurus diagnosticus and the Heterodontosauridae within the Ornithischia has been problematic. Historically, Lesothosaurus has been regarded as a basal ornithischian dinosaur, the sister taxon to the Genasauria. Recent phylogenetic analyses, however, have placed Lesothosaurus as a more derived ornithischian within the Genasauria. The Fabrosauridae, of which Lesothosaurus was considered a member, has never been phylogenetically corroborated and has been considered a paraphyletic assemblage. Prior to recent phylogenetic analyses, the problematic Heterodontosauridae was placed within the Ornithopoda as the sister taxon to the Euornithopoda. The heterodontosaurids have also been considered as the basal member of the Cerapoda (Ornithopoda + Marginocephalia), the sister taxon to the Marginocephalia, and as the sister taxon to the Genasauria. To reevaluate the placement of these taxa, along with other basal ornithischians and more derived subclades, a phylogenetic analysis of 19 taxonomic units, including two outgroup taxa, was performed. Analysis of 97 characters and their associated character states culled, modified, and/or rescored from published literature based on published descriptions, produced four most parsimonious trees. Consistency and retention indices were calculated and a bootstrap analysis was performed to determine the relative support for the resultant phylogeny. The Ornithischia was recovered with Pisanosaurus as its basalmost member. -
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. -
Massospondylus Carinatus Owen 1854 (Dinosauria: Sauropodomorpha) from the Lower Jurassic of South Africa: Proposed Conservation of Usage by Designation of a Neotype
Massospondylus carinatus Owen 1854 (Dinosauria: Sauropodomorpha) from the Lower Jurassic of South Africa: Proposed conservation of usage by designation of a neotype Adam M. Yates1* & Paul M. Barrett2 1Bernard Price Institute for Palaeontological Research, University of the Witwatersrand, Private Bag 3, WITS, 2050 Johannesburg, South Africa 2Department of Palaeontology, The Natural History Museum, Cromwell Road, London, SW7 5BD, U.K. Received 17 February 2010. Accepted 12 November 2010 The purpose of this article is to preserve the usage of the binomen Massospondylus carinatus by designating a neotype specimen. Massospondylus is the most abundant basal sauropodomorph dinosaur from the Early Jurassic strata of southern Africa. This taxon forms the basis for an extensive palaeobiological literature and is the eponym of Massospondylidae and the nominal taxon of a biostratigraphical unit in current usage, the ‘Massospondylus Range Zone’. The syntype series of M. carinatus (five disarticulated and broken vertebrae) was destroyed during World War II, but plaster casts and illustrations of the material survive. Nonetheless, these materials cannot act as type material for this taxon under the rules of the ICZN Code. In order to avoid nomenclatural instability, we hereby designate BP/1/4934 (a skull and largely complete postcranial skeleton) as the neotype of Massospondylus carinatus. Keywords: Dinosauria, Sauropodomorpha, Massospondylidae, Massospondylus, Massospondylus carinatus, neotype, South Africa, upper Elliot Formation, Early Jurassic. INTRODUCTION same taxon, possibly even the same individual, as at least Richard Owen described and named Massospondylus some of the syntype series of Massospondylus carinatus. carinatus (1854, p. 97) with carinatus as the type species of Their initial separation from Massospondylus carinatus the genus by monotypy. -
Revealing the Beattie Magnetic Anomaly and the Anatomy Of
11th SAGA Biennial Technical Meeting and Exhibition Swaziland, 16 - 18 September 2009, pages 490 - 499 Revealing the Beattie Magnetic Anomaly and the anatomy of the crust of southernmost Africa: Geophysics and deep sub- surface geology where the Cape Fold Belt and Karroo Basin meet A. S. Lindeque1,2,3, M.J. de Wit4 1. Now at Alfred Wegener Institute for Polar and Marine Research, Geophysics, Building D3280, Am Alten Hafen 26, 27568 Bremerhaven, Germany, [email protected] 2. Council for Geoscience, Western Cape, P.O. Box 572, Bellville 7535, Cape Town, South Africa 3. GeoForschungsZentrum Potsdam, Section 2.2, Telegrafenberg, 14473 Potsdam, Germany 4. AEON - Africa Earth Observatory Network and Department of Geological Sciences, University of Cape Town, Rondebosch 7701, South Africa, [email protected] ABSTRACT The deep crust of the southernmost margin of Africa contains unresolved tectonic features such as the Paleozoic Cape Fold Belt (CFB), the Paleozoic-Mesozoic Karroo Basin and the largest terrestrial magnetic anomaly, the Beattie Magnetic Anomaly (BMA). Without resolving these structures, our understanding of the evolution of the southern margin will be incomplete and limited. Under the auspices of the Inkaba yeAfrica framework, several geophysical datasets were acquired from 2004 to 2007, along two transects across the margin and its unique tectonic features. This research presents a tectonic model and crustal geometry, at the centre 100 km of the western transect. The model is derived from the joint interpretation of: surface geology, aeromagnetic data, nearby deep boreholes, teleseismic receiver functions, impedance spectroscopy measurements on borehole samples, near vertical reflection seismic data (NVR), shallow P- and S-wave velocity data, wide angle refraction data and magnetotelluric data.