Age, Origin and Emplacement of Diamonds
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South African Palaeo-Scientists the Names Listed Below Are Just Some of South Africa’S Excellent Researchers Who Are Working Towards Understanding Our African Origins
2010 African Origins Research MAP_Layout 1 2010/04/15 11:02 AM Page 1 South African Palaeo-scientists The names listed below are just some of South Africa’s excellent researchers who are working towards understanding our African origins. UNIVERSITY OF CAPE TOWN (UCT) Dr Thalassa Matthews analyses the Dr Job Kibii focuses PALAEOBIOLOGICAL RESEARCH thousands of tiny teeth and bones of fossil on how fossil hominid Professor Anusuya Chinsamy-Turan is one microfauna to reconstruct palaeoenviron- and non-hominid of only a few specialists in the world who mental and climatic changes on the west faunal communities coast over the last 5 million years. changed over time and African Origins Research studies the microscopic structure of bones of dinosaurs, pterosaurs and mammal-like uses this to reconstruct reptiles in order to interpret various aspects ALBANY MUSEUM, past palaeoenviron- of the biology of extinct animals. GRAHAMSTOWN ments and palaeo- A summary of current research into fossils of animals, plants and early hominids from the beginning of life on Earth to the Middle Stone Age PERMIAN AGE PLANTS ecology. THE HOFMEYR SKULL Dr Rose Prevec studies the “No other country in the world can boast the oldest evidence of life on Earth extending back more than 3 billion years, the oldest multi-cellular animals, the oldest land-living plants, Professor Alan Morris described the Glossopteris flora of South Africa (the PAST HUMAN BEHAVIOUR Hofmeyer skull, a prehistoric, fossilized ancient forests that formed our coal Professor Chris Henshilwood directs the most distant ancestors of dinosaurs, the most complete record of the more than 80 million year ancestry of mammals, and, together with several other African countries, a most remarkable human skull about 36 000 years old deposits) and their end-Permian excavations at Blombos Cave where that corroborates genetic evidence that extinction. -
Mantle Peridotite Xenoliths
Earth and Planetary Science Letters 260 (2007) 37–55 www.elsevier.com/locate/epsl Mantle peridotite xenoliths in andesite lava at El Peñon, central Mexican Volcanic Belt: Isotopic and trace element evidence for melting and metasomatism in the mantle wedge beneath an active arc ⁎ Samuel B. Mukasa a, , Dawnika L. Blatter b, Alexandre V. Andronikov a a Department of Geological Sciences, University of Michigan, Ann Arbor, MI 48109-1005, USA b Department of Earth and Planetary Science, University of California, Berkeley, CA 94720, USA Received 6 July 2006; received in revised form 3 May 2007; accepted 7 May 2007 Available online 13 May 2007 Editor: R.W. Carlson Abstract Peridotites in the mantle wedge and components added to them from the subducting slab are thought to be the source of most arc magmas. However, direct sampling of these materials, which provides a glimpse into the upper mantle beneath an active margin, is exceedingly rare. In the few arc localities where found, peridotite xenoliths are usually brought to the surface by basaltic magmas. Remarkably, the hornblende-bearing ultramafic xenoliths and clinopyroxene megaxenocrysts from El Peñon in the central Mexican Volcanic Belt were brought to the surface by a Quaternary high-Mg siliceous andesite, a rock type usually considered too evolved to be a direct product of mantle melting. The xenoliths and megaxenocrysts from El Peñon represent lithospheric mantle affected by significant subduction of oceanic lithosphere since as early as the Permian. Trace element and radiogenic isotope data we report here on these materials suggest a history of depletion by melt extraction, metasomatism involving a fluid phase, and finally, limited reaction between the ultramafic materials and the host andesite, probably during transport. -
Sampling and Estimation of Diamond Content in Kimberlite Based on Microdiamonds Johannes Ferreira
Sampling and estimation of diamond content in kimberlite based on microdiamonds Johannes Ferreira To cite this version: Johannes Ferreira. Sampling and estimation of diamond content in kimberlite based on micro- diamonds. Other. Ecole Nationale Supérieure des Mines de Paris, 2013. English. NNT : 2013ENMP0078. pastel-00982337 HAL Id: pastel-00982337 https://pastel.archives-ouvertes.fr/pastel-00982337 Submitted on 23 Apr 2014 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. N°: 2009 ENAM XXXX École doctorale n° 398: Géosciences et Ressources Naturelles Doctorat ParisTech T H È S E pour obtenir le grade de docteur délivré par l’École nationale supérieure des mines de Paris Spécialité “ Géostatistique ” présentée et soutenue publiquement par Johannes FERREIRA le 12 décembre 2013 Sampling and Estimation of Diamond Content in Kimberlite based on Microdiamonds Echantillonnage des gisements kimberlitiques à partir de microdiamants. Application à l’estimation des ressources récupérables Directeur de thèse : Christian LANTUÉJOUL Jury T M. Xavier EMERY, Professeur, Université du Chili, Santiago (Chili) Président Mme Christina DOHM, Professeur, Université du Witwatersrand, Johannesburg (Afrique du Sud) Rapporteur H M. Jean-Jacques ROYER, Ingénieur, HDR, E.N.S. Géologie de Nancy Rapporteur M. -
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. -
Hydrated Peridotite – Basaltic Melt Interaction Part I: Planetary Felsic Crust Formation at Shallow Depth Anastassia Y
Hydrated Peridotite – Basaltic Melt Interaction Part I: Planetary Felsic Crust Formation at Shallow Depth Anastassia Y. BORISOVA1,2*, Nail R. ZAGRTDENOV1, Michael J. TOPLIS3, Wendy A. BOHRSON4, Anne NEDELEC1, Oleg G. SAFONOV2,5,6, Gleb S. POKROVSKI1, Georges CEULENEER1, Ilya N. BINDEMAN7, Oleg E. MELNIK8, Klaus Peter JOCHUM9, Brigitte STOLL9, Ulrike WEIS9, Andrew Y. BYCHKOV2, Andrey A. GURENKO10, Svyatoslav SHCHEKA11, Artem TEREHIN5, Vladimir M. POLUKEEV5, Dmitry A. VARLAMOV5, Kouassi E.A. CHARITEIRO1, Sophie GOUY1, Philippe de PARSEVAL1 1 Géosciences Environnement Toulouse, Université de Toulouse; UPS, CNRS, IRD, Toulouse, France 2 Geological Department, Lomonosov Moscow State University, Vorobievy Gory, 119899, Moscow, Russia 3 Institut de Recherche en Astrophysique et Planétologie (IRAP) UPS, CNRS, Toulouse, France 4 Central Washington University, Department of Geological Sciences, Ellensburg, WA 98926, USA 5 Korzhinskii Institute of Experimental Mineralogy, 142432, Chernogolovka, Moscow region, Russia 6 Department of Geology, University of Johannesburg PO Box 524, Auckland Park, 2006, Johannesburg, South Africa 7 Geological Sciences, University of Oregon, 1275 E 13th street, Eugene, OR, USA 8 Institute of Mechanics, Moscow State University, 1- Michurinskii prosp, 119192, Moscow, Russia 9 Climate Geochemistry Department, Max Planck Institute for Chemistry, P.O. Box 3060, D-55020 Mainz, Germany 10 Centre de Recherches Pétrographiques et Géochimiques, UMR 7358, Université de Lorraine, 54501 Vandœuvre-lès-Nancy, France 11 Bavarian Research -
Origin of Lherzolite Inclusions in the Malapai Hill Basalt, Joshua Tree National Monument, California
ROBERT J. STULL Department of Geology, California State University, Los Angeles, Los Angeles, California 90032 KENT McMILLAN Department of Geological Sciences, Stanford University, Stanford, California 94305 Origin of Lherzolite Inclusions in the Malapai Hill Basalt, Joshua Tree National Monument, California ABSTRACT dence that the nodules could be the end product of more than one partial melting. Alkali olivine basalt at Malapai Hill, Cali- fornia, occurs as a late Cenozoic stock that has INTRODUCTION intruded the Cretaceous White Tank Monzon- Basalts and ultramafic nodules from the ite. The basalt is chemically and mineralogi- Mojave Desert have been described in several cally similar to other alkaline basalts in the papers. Ross and others (1954) reported min- Mojave Desert, although it is devoid of zeolites. eral compositions of peridotite inclusions from The strontium isotopic composition of the Dish Hill and noted the world-wide similarity basalt (Sr87/Sr86 = 0.7030 ± 0.0006) suggests of nodules. Hess (1955) published one analysis that it is derived from a mantle that has of a nodule from Dish Hill (Fig. 1). Wise already experienced one period of partial (1966, 1969) described the characteristics of ba- melting. OUvine-rich lherzolite nodules in the salts in the Mojave Desert and provided a basalt are high in Mg and low in Si, Al, Ca, viable theory for the sequence of lava at Na, and K. The nodules are xenomorphic Pisgah Crater. Most petrologists agree that granular with a tectonite fabric and forsteritic basalt forms in the upper mantle (for example, olivine (F094-88). The Sr87/Sr86 ratio of the Green and Ringwood, 1967; Jackson and nodules is 0.7043 + 0.0008. -
Constraints on the Timescale of Animal Evolutionary History
Palaeontologia Electronica palaeo-electronica.org Constraints on the timescale of animal evolutionary history Michael J. Benton, Philip C.J. Donoghue, Robert J. Asher, Matt Friedman, Thomas J. Near, and Jakob Vinther ABSTRACT Dating the tree of life is a core endeavor in evolutionary biology. Rates of evolution are fundamental to nearly every evolutionary model and process. Rates need dates. There is much debate on the most appropriate and reasonable ways in which to date the tree of life, and recent work has highlighted some confusions and complexities that can be avoided. Whether phylogenetic trees are dated after they have been estab- lished, or as part of the process of tree finding, practitioners need to know which cali- brations to use. We emphasize the importance of identifying crown (not stem) fossils, levels of confidence in their attribution to the crown, current chronostratigraphic preci- sion, the primacy of the host geological formation and asymmetric confidence intervals. Here we present calibrations for 88 key nodes across the phylogeny of animals, rang- ing from the root of Metazoa to the last common ancestor of Homo sapiens. Close attention to detail is constantly required: for example, the classic bird-mammal date (base of crown Amniota) has often been given as 310-315 Ma; the 2014 international time scale indicates a minimum age of 318 Ma. Michael J. Benton. School of Earth Sciences, University of Bristol, Bristol, BS8 1RJ, U.K. [email protected] Philip C.J. Donoghue. School of Earth Sciences, University of Bristol, Bristol, BS8 1RJ, U.K. [email protected] Robert J. -
Evolution of K-Rich Magmas Derived from a Net Veined
Evolution of K-rich magmas derived from a net veined lithospheric mantle in an ongoing extensional setting: Geochronology and geochemistry of Eocene and Miocene volcanic rocks from Eastern Pontides (Turkey) Cem Yücel, Mehmet Arslan, Irfan Temizel, Emel Abdioğlu, Gilles Ruffet To cite this version: Cem Yücel, Mehmet Arslan, Irfan Temizel, Emel Abdioğlu, Gilles Ruffet. Evolution of K-rich magmas derived from a net veined lithospheric mantle in an ongoing extensional setting: Geochronology and geochemistry of Eocene and Miocene volcanic rocks from Eastern Pontides (Turkey). Gondwana Research, Elsevier, 2017, 45, pp.65-86. 10.1016/j.gr.2016.12.016. insu-01462865 HAL Id: insu-01462865 https://hal-insu.archives-ouvertes.fr/insu-01462865 Submitted on 9 Feb 2017 HAL is a multi-disciplinary open access L’archive ouverte pluridisciplinaire HAL, est archive for the deposit and dissemination of sci- destinée au dépôt et à la diffusion de documents entific research documents, whether they are pub- scientifiques de niveau recherche, publiés ou non, lished or not. The documents may come from émanant des établissements d’enseignement et de teaching and research institutions in France or recherche français ou étrangers, des laboratoires abroad, or from public or private research centers. publics ou privés. Accepted Manuscript Evolution of K-rich magmas derived from a net veined lithospheric mantle in an ongoing extensional setting: Geochronology and geochemistry of Eocene and Miocene volcanic rocks from Eastern Pontides (Turkey) Cem Yücel, Mehmet Arslan, -
Geochemistry of an Ultramafic-Rodingite Rock Association in the Paleoproterozoic Dixcove Greenstone Belt, Southwestern Ghana
Journal of African Earth Sciences 45 (2006) 333–346 www.elsevier.com/locate/jafrearsci Geochemistry of an ultramafic-rodingite rock association in the Paleoproterozoic Dixcove greenstone belt, southwestern Ghana Kodjopa Attoh a,*, Matthew J. Evans a,1, M.E. Bickford b a Department of Earth and Atmospheric Sciences, Cornell University, Snee Hall, Ithaca, NY 14853, USA b Department of Earth Sciences, Syracuse University, Syracuse, NY 13244, USA Received 11 January 2005; received in revised form 20 February 2006; accepted 2 March 2006 Available online 18 May 2006 Abstract Rodingite occurs in ultramafic rocks within the Paleoproterozoic (Birimian) Dixcove greenstone belt in southwestern Ghana. U–Pb analyses of zircons from granitoids intrusive into the greenstone belt constrain the age of the rodingite-ultramafic association to be older than 2159 Ma. The ultramafic complex consists of variably serpentinized dunite and harzburgite overlain by gabbroic rocks, which together show petrographic and geochemical characteristics consistent with their formation by fractional crystallization involving olivine and plagioclase cumulates. Major and trace element concentrations and patterns in the ultramafic–mafic cumulate rocks and associated plagiogranite are similar to rocks in ophiolitic suites. The rodingites, which occur as irregular pods and lenses, and as veins and blocks in the serpentinized zones, are characterized by high Al2O3 and CaO contents, which together with petrographic evidence indicate their formation from plagioclase-rich protoliths. The peridotites are highly depleted in REE and display flat, chondrite-normalized REE pat- terns with variable, but mostly small, positive Eu anomalies whereas the rodingites, which are also highly depleted, with overall REE contents from 0.04 to 1.2 times chondrite values, display distinct large positive Eu anomalies. -
GSA TODAY Conference, P
Vol. 10, No. 2 February 2000 INSIDE • GSA and Subaru, p. 10 • Terrane Accretion Penrose GSA TODAY Conference, p. 11 A Publication of the Geological Society of America • 1999 Presidential Address, p. 24 Continental Growth, Preservation, and Modification in Southern Africa R. W. Carlson, F. R. Boyd, S. B. Shirey, P. E. Janney, Carnegie Institution of Washington, 5241 Broad Branch Road, N.W., Washington, D.C. 20015, USA, [email protected] T. L. Grove, S. A. Bowring, M. D. Schmitz, J. C. Dann, Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, USA D. R. Bell, J. J. Gurney, S. H. Richardson, M. Tredoux, A. H. Menzies, Department of Geological Sciences, University of Cape Town, Rondebosch 7700, South Africa D. G. Pearson, Department of Geological Sciences, Durham University, South Road, Durham, DH1 3LE, UK R. J. Hart, Schonland Research Center, University of Witwater- srand, P.O. Box 3, Wits 2050, South Africa A. H. Wilson, Department of Geology, University of Natal, Durban, South Africa D. Moser, Geology and Geophysics Department, University of Utah, Salt Lake City, UT 84112-0111, USA ABSTRACT To understand the origin, modification, and preserva- tion of continents on Earth, a multidisciplinary study is examining the crust and upper mantle of southern Africa. Xenoliths of the mantle brought to the surface by kimber- lites show that the mantle beneath the Archean Kaapvaal Figure 2. Bouguer gravity image (courtesy of South African Council for Geosciences) craton is mostly melt-depleted peridotite with melt extrac- across Vredefort impact structure, South Africa. Color scale is in relative units repre- senting total gravity variation of 90 mgal across area of figure. -
Trace Element Fractionation in Alkaline OIB
Genesis of primitive Hawaiian rejuvenated-stage lavas: Evidence for carbonatite metasomatism and implications for ancient eclogite source Anastassia Y. Borisova 1,2* 1 Géosciences Environnement Toulouse, GET - UMR 5563 - OMP - CNRS, 14 Avenue E. Belin, 31400 Toulouse, France 2 Geological Department, Lomonosov Moscow State University, MGU, Vorobievu Gori, 119991, Moscow, Russia (revised version, 12/03/2020, for Geochemistry Geophysics Geosystems) *Corresponding author: E-mail: [email protected]; *Corresponding adresse: Géosciences Environnement Toulouse UMR 5563, Observatoire Midi Pyrénées, 14 Avenue E. Belin, 31400 Toulouse, France; Tel: +33(0)5 61 54 26 31; Fax: +33(0)5 61 33 25 60 Abstract – To constrain a contribution of deep carbonated mantle, to fractionation of Hf relative to rare earth elements (REE) in volcanic series, we examine available high-quality data on major, trace element and Nd-Hf isotope compositions of ~280 primitive lavas and glasses (MgO = 8.5 – 21 wt%, SiO2 = 37 - 50 wt%) erupted during preshield, postshield and mostly rejuvenated stage of the Hawaiian hot spot (Pacific Ocean). Strong variations of Hf/Sm, Zr/Sm, Ti/Eu, K/Th, Nb/Th, La/K and Ba/K in the lavas are not features of the melt equilibration with residual amphibole or phlogopite, and cannot be due to variable degrees of batch or dynamic melting of uncarbonated lherzolite source. Enrichment in REE, Th and Ba relative to K, Hf, Zr, Ti and Nb together and low Si, high Na, K and Ca contents in the Hawaiian lavas are compositional features of carbonated mantle lithospheric to asthenospheric peridotite source affected by carbonatite metasomatism at temperatures higher than 1100°C and pressures higher than 2 GPa. -
PRELIMINARY EVALUATION of BEDROCK POTENTIAL for NATURALLY OCCURRING ASBESTOS in ALASKA by Diana N
Alaska Division of Geological & Geophysical Surveys MISCELLANEOUS PUBLICATION 157 PRELIMINARY EVALUATION OF BEDROCK POTENTIAL FOR NATURALLY OCCURRING ASBESTOS IN ALASKA by Diana N. Solie and Jennifer E. Athey Tremolite (UAMES 34960) displaying the soft, friable fibers of asbestiform minerals. Sample collected from the Cosmos Hills area, Kobuk District, Alaska, by Eskil Anderson. Image courtesy of the University of Alaska Museum Earth Sciences Department. June 2015 Released by STATE OF ALASKA DEPARTMENT OF NATURAL RESOURCES Division of Geological & Geophysical Surveys 3354 College Road, Fairbanks, Alaska 99709-3707 907-451-5020 dggs.alaska.gov [email protected] $2.00 (text only) $13.00 (per map sheet) TABLE OF CONTENTS Abstract ................................................................................................................................................................................................................................. 1 Introduction ........................................................................................................................................................................................................................ 1 General geology of asbestos ......................................................................................................................................................................................... 2 Naturally occurring asbestos potential in Alaska ..............................................................................................................................................