The Geology of England – Critical Examples of Earth History – an Overview
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Proceedings of the Open University Geological Society
0 OUGS Proceedings 5 2019_OUGSJ 26/02/2019 11:45 Page i Proceedings of the Open University Geological Society Volume 5 2019 Including articles from the AGM 2018 Geoff Brown Memorial Lecture, the ‘Music of the Earth’ Symposium 2018 lectures (Worcester University), OUGS Members’ field trip reports, the Annual Report for 2018, and the 2018 Moyra Eldridge Photographic Competition Winning and Highly Commended photographs Edited and designed by: Dr David M. Jones 41 Blackburn Way, Godalming, Surrey GU7 1JY e-mail: [email protected] The Open University Geological Society (OUGS) and its Proceedings Editor accept no responsibility for breach of copyright. Copyright for the work remains with the authors, but copyright for the published articles is that of the OUGS. ISSN 2058-5209 © Copyright reserved Proceedings of the OUGS 5 2019; published 2019; printed by Hobbs the Printers Ltd, Totton, Hampshire 0 OUGS Proceedings 5 2019_OUGSJ 26/02/2019 11:46 Page 35 The complex tectonic evolution of the Malvern region: crustal accretion followed by multiple extensional and compressional reactivation Tim Pharaoh British Geological Survey, Keyworth, Nottingham, NG12 5GG ([email protected]) Abstract The Malvern Hills include some of the oldest rocks in southern Britain, dated by U-Pb zircon analysis to c. 680Ma. They reflect calc- alkaline arc magmatic activity along a margin of the Rodinia palaeocontinent, hints of which are provided by inherited zircon grains as old as 1600Ma. Metamorphic recrystallisation under upper greenschist/amphibolite facies conditions occurred from c. 650–600Ma. Subsequently, rifting of the magmatic arc (c.f. the modern western Pacific) at c. 565Ma led to the formation of a small oceanic mar- ginal basin, evidenced by basaltic pillow lavas and tuffs of the Warren House Formation, and Kempsey Formation equivalents beneath the Worcester Graben. -
The North-Subducting Rheic Ocean During the Devonian: Consequences for the Rhenohercynian Ore Sites
Published in "International Journal of Earth Sciences 106(7): 2279–2296, 2017" which should be cited to refer to this work. The north-subducting Rheic Ocean during the Devonian: consequences for the Rhenohercynian ore sites Jürgen F. von Raumer1 · Heinz-Dieter Nesbor2 · Gérard M. Stampfli3 Abstract Base metal mining in the Rhenohercynian Zone activated Early Devonian growth faults. Hydrothermal brines has a long history. Middle-Upper Devonian to Lower Car- equilibrated with the basement and overlying Middle-Upper boniferous sediment-hosted massive sulfide deposits Devonian detrital deposits forming the SHMS deposits in the (SHMS), volcanic-hosted massive sulfide deposits (VHMS) southern part of the Pyrite Belt, in the Rhenish Massif and and Lahn-Dill-type iron, and base metal ores occur at sev- in the Harz areas. Volcanic-hosted massive sulfide deposits eral sites in the Rhenohercynian Zone that stretches from the (VHMS) formed in the more eastern localities of the Rheno- South Portuguese Zone, through the Lizard area, the Rhen- hercynian domain. In contrast, since the Tournaisian period ish Massif and the Harz Mountain to the Moravo-Silesian of ore formation, dominant pull-apart triggered magmatic Zone of SW Bohemia. During Devonian to Early Carbonif- emplacement of acidic rocks, and their metasomatic replace- erous times, the Rhenohercynian Zone is seen as an evolv- ment in the apical zones of felsic domes and sediments in ing rift system developed on subsiding shelf areas of the the northern part of the Iberian Pyrite belt, thus changing the Old Red continent. A reappraisal of the geotectonic setting general conditions of ore precipitation. -
Resolving the Variscan Evolution of the Moldanubian Sector of The
Journal of Geosciences, 52 (2007), 9–28 DOI: 10.3190/jgeosci.005 Original paper Resolving the Variscan evolution of the Moldanubian sector of the Bohemian Massif: the significance of the Bavarian and the Moravo–Moldanubian tectonometamorphic phases Fritz FINGER1*, Axel GERDEs2, Vojtěch JANOušEk3, Miloš RENé4, Gudrun RIEGlER1 1University of Salzburg, Division of Mineralogy, Hellbrunnerstraße 34, A-5020 Salzburg, Austria; [email protected] 2University of Frankfurt, Institute of Geoscience, Senckenberganlage 28, D-60054 Frankfurt, Germany 3Czech Geological Survey, Klárov 3, 118 21 Prague 1, Czech Republic 4Academy of Sciences, Institute of Rock Structure and Mechanics, V Holešovičkách 41, 182 09 Prague 8, Czech Republic *Corresponding author The Variscan evolution of the Moldanubian sector in the Bohemian Massif consists of at least two distinct tectonome- tamorphic phases: the Moravo–Moldanubian Phase (345–330 Ma) and the Bavarian Phase (330–315 Ma). The Mora- vo–Moldanubian Phase involved the overthrusting of the Moldanubian over the Moravian Zone, a process which may have followed the subduction of an intervening oceanic domain (a part of the Rheiic Ocean) beneath a Moldanubian (Armorican) active continental margin. The Moravo–Moldanubian Phase also involved the exhumation of the HP–HT rocks of the Gföhl Unit into the Moldanubian middle crust, represented by the Monotonous and Variegated series. The tectonic emplacement of the HP–HT rocks was accompanied by intrusions of distinct magnesio-potassic granitoid melts (the 335–338 Ma old Durbachite plutons), which contain components from a strongly enriched lithospheric mantle source. Two parallel belts of HP–HT rocks associated with Durbachite intrusions can be distinguished, a western one at the Teplá–Barrandian and an eastern one close to the Moravian boundary. -
Geological Survey of Finland
Geological Survey of Finland Bulletin 357 Paleoproterozoic volcanism in the Kühtelysvaara - Tohmajärvi district, eastern Finland by Lauri J. Pekkarinen and Heikki Lukkarinen Geologian tutkimuskeskus Espoo 1991 - - ----- --- - - Geological Survey of Finland, Bulletin 357 P ALEOPROTEROZOIC VOLCANISM IN THE KIIHTELYSVAARA - TOHMAJÄRVI DISTRICT, EASTERN FINLAND by LAURI J. PEKKARINEN AND HEIKKI LUKKARINEN with 17 figures, 1 table and 3 appendices GEOLOGIAN TUTKIMUSKESKUS ESPOO 1991 Pekkarinen, L.J. & Lukkarinen, H., 1991. Paleoproterozoie volcanism in the Kiih telysvaara - Tohmajärvi distriet, eastern Finland. Geological Survey 0/ Finland, Bulletin 357,30 pages, 17 figures, I table and 3 appendiees. The numerous episodes of Paleoproterozoie volcanism and assoeiated sedimen tation preserved in the Kiihtelysvaara - Tohmajärvi distriet represent both prolonged and episodie rifting of eratonie erust. V-Pb zireon age determinations from two mafie dykes intruded in eonjunetion with the basalmost lava flows indieate an age of ca. 2120 - 2100 Ma for this earliest mafie magmatism. However, no informa tion is yet available eoneerning the age of the younger flows, dykes or sills. Pyroclastie units are also present and have, along with the mafie lava flows and intrusions, been metamorphosed under greenschist facies eonditions. Volcan ism took plaee in an intraeratonie, within-plate setting, with predominantly basal tie eompositions. Hydrothermal alteration oeeurred both during and after erup tion. This affeeted the chemical composition of the earlier lava in particular, the younger lava flows as weil as the dykes and sills generally showing less evidence of ehemical alteration. The volcanogenic and sedimentary formations of the Kiihtelysvaara area have been renamed according to local geographical place names and regional correla tions and comparisons have been made between the study area and similar sequences elsewhere in Finland, particularly with respect to the mafie units. -
W.J. B , B.E. L and C.N. Waters
DRAFT – FOR BGS APPROVAL THE GLOBAL DEVONIAN, CARBONIFEROUS AND PERMIAN CORRELATION PROJECT: A REVIEW OF THE CONTRIBUTION FROM GREAT BRITAIN 1 2 2 3 G. WARRINGTON , W.J. BARCLAY , B.E. LEVERIDGE AND C.N. WATERS Warrington, G., Barclay, W.J., Leveridge, B.E. and Waters, C.N. 201x. The Global Devonian, Carboniferous and Permian Correlation Project: a review of the contribution from Great Britain. Geoscience in South-West England, 13, xx-xx. A contribution on the lithostratigraphy and palaeoenvironments of Devonian, Carboniferous and Permian successions onshore in Great Britain, prepared for an international project, is summarised with particular reference to south-west England. Devonian and Carboniferous successions present in that region occur in the Rhenohercynian Tectonic Zone, to the south of the Variscan Front (VF), and their complexity reflects formation in six composite basins. They differ substantially from contemporaneous successions north of the VF. Whereas Devonian successions south of the VF are largely marine, those to the north are continental. Carboniferous successions south of the VF are predominantly marine, but shallow-water and deltaic facies occur in the highest formations. North of the VF, marine conditions were superseded by paralic and continental sedimentation. Erosion, following Variscan tectonism, resulted in the Permian successions generally resting unconformably upon older Palaeozoic rocks. In south-west England a continental succession may extend, with depositional hiatuses, from the latest Carboniferous to the Late Permian and is the most complete Permian succession in Great Britain. However, the position of the Permian–Triassic boundary in the south- west, and elsewhere in the country, is not yet resolved. -
Hydrographic Development of the Aral Sea During the Last 2000 Years Based on a Quantitative Analysis of Dinoflagellate Cysts
Palaeogeography, Palaeoclimatology, Palaeoecology 234 (2006) 304–327 www.elsevier.com/locate/palaeo Hydrographic development of the Aral Sea during the last 2000 years based on a quantitative analysis of dinoflagellate cysts P. Sorrel a,b,*, S.-M. Popescu b, M.J. Head c,1, J.P. Suc b, S. Klotz b,d, H. Oberha¨nsli a a GeoForschungsZentrum, Telegraphenberg, D-14473 Potsdam, Germany b Laboratoire Pale´oEnvironnements et Pale´obioSphe`re (UMR CNRS 5125), Universite´ Claude Bernard—Lyon 1, 27-43, boulevard du 11 Novembre, 69622 Villeurbanne Cedex, France c Department of Geography, University of Cambridge, Downing Place, Cambridge CB2 3EN, UK d Institut fu¨r Geowissenschaften, Universita¨t Tu¨bingen, Sigwartstrasse 10, 72070 Tu¨bingen, Germany Received 30 June 2005; received in revised form 4 October 2005; accepted 13 October 2005 Abstract The Aral Sea Basin is a critical area for studying the influence of climate and anthropogenic impact on the development of hydrographic conditions in an endorheic basin. We present organic-walled dinoflagellate cyst analyses with a sampling resolution of 15 to 20 years from a core retrieved at Chernyshov Bay in the NW Large Aral Sea (Kazakhstan). Cysts are present throughout, but species richness is low (seven taxa). The dominant morphotypes are Lingulodinium machaerophorum with varied process length and Impagidinium caspienense, a species recently described from the Caspian Sea. Subordinate species are Caspidinium rugosum, Romanodinium areolatum, Spiniferites cruciformis, cysts of Pentapharsodinium dalei, and round brownish protoper- idiniacean cysts. The chlorococcalean algae Botryococcus and Pediastrum are taken to represent freshwater inflow into the Aral Sea. The data are used to reconstruct salinity as expressed in lake level changes during the past 2000 years. -
Geology: Ordovician Paleogeography and the Evolution of the Iapetus Ocean
Ordovician paleogeography and the evolution of the Iapetus ocean Conall Mac Niocaill* Department of Geological Sciences, University of Michigan, 2534 C. C. Little Building, Ben A. van der Pluijm Ann Arbor, Michigan 48109-1063. Rob Van der Voo ABSTRACT thermore, we contend that the combined paleomagnetic and faunal data ar- Paleomagnetic data from northern Appalachian terranes identify gue against a shared Taconic history between North and South America. several arcs within the Iapetus ocean in the Early to Middle Ordovi- cian, including a peri-Laurentian arc at ~10°–20°S, a peri-Avalonian PALEOMAGNETIC DATA FROM IAPETAN TERRANES arc at ~50°–60°S, and an intra-oceanic arc (called the Exploits arc) at Displaced terranes occur along the extent of the Appalachian-Cale- ~30°S. The peri-Avalonian and Exploits arcs are characterized by Are- donian orogen, although reliable Ordovician paleomagnetic data from Ia- nigian to Llanvirnian Celtic fauna that are distinct from similarly aged petan terranes have only been obtained from the Central Mobile belt of the Toquima–Table Head fauna of the Laurentian margin, and peri- northern Appalachians (Table 1). The Central Mobile belt separates the Lau- Laurentian arc. The Precordillera terrane of Argentina is also charac- rentian and Avalonian margins of Iapetus and preserves remnants of the terized by an increasing proportion of Celtic fauna from Arenig to ocean, including arcs, ocean islands, and ophiolite slivers (e.g., Keppie, Llanvirn time, which implies (1) that it was in reproductive communi- 1989). Paleomagnetic results from Arenigian and Llanvirnian volcanic units cation with the peri-Avalonian and Exploits arcs, and (2) that it must of the Moreton’s Harbour Group and the Lawrence Head Formation in cen- have been separate from Laurentia and the peri-Laurentian arc well tral Newfoundland indicate paleolatitudes of 11°S (Table 1), placing them before it collided with Gondwana. -
Geology and Petroleum Systems of the Eastern Meseta and Atlas Domains of Morocco
258 Paper 22 Geology and petroleum systems of the Eastern Meseta and Atlas Domains of Morocco FATIMA CHARRAT\ MOHAMAD ELALTI\ MoHO HAMIDI M. NOR2, NG TONG SAN2, SUPIAN SUNTEK2 AND TJIA, H.D.2 10ttice National de Recherches et d'Exploitations Petrolieres Rabat, Maghreb 2PETRONAS Carigali, Tower 1, Petronas Twin Towers 50088 Kuala Lumpur, Malaysia Morocco (Maghreb), located in Northwest Africa, has three main structural domains: The (a) RifDomain, the (b) Atlas Domain comprising two different structural regions, the relatively stable eastern and western Meseta, (characterized by mildly deformed Mesozoic strata) and the active Middle-High Atlas Belts, where the Meso Cenozoic section was highly folded during the Alpine orogeny; and finally, the (c) Sahara-Anti Atlas Domain at the south, marks the stable margin of the West African Craton. The eastern Meseta, with the Middle and the High Atlas chains (Atlas Domain ss.) is the objective of our study; it extends eastward through Algeria. The Middle Atlas and the High Atlas tectonic belts frame the Meseta. The Cambrian marine transgression over the northwestern African continental platform allowed deposition of shales, silts and sands over a faulted land surface. Folding at the Late Cambrian generated an irregular angular unconformity with the Ordovician sequence. This sequence, dominantly argillaceous at the beginning, ended with a regressive phase of glacio-marine sedimentation that developed coarse sandstones and micro-conglomerate. Volcanic eruptions caused localised metamorphism. The Ordovician ended with regression due to the emergence of the area (Taconic phase). Glacio-eustatism followed, leading to the widespread Silurian deposits of graptolite bearing black clays in shallow marine, confined (euxinic) troughs. -
Alpine Orogeny the Geologic Development of the Mediterranean
Alpine Orogeny The geologic development of the Mediterranean region is driven by the Alpine-Himalayan orogeny, a suturing of Gondwana-derived terranes with the Eurasion craton. In broad terms, this is a Mesozoic and Cenozoic convergent zone that extends from the Spain to Southeastern Asia and may extend along the southwest Pacific as far as New Zealand (Rosenbaum and Lister, 2002). The Alpine orogeny was caused by the convergence of the African and European plates (Frisch, 1979; Tricart, 1984; Haas et al., 1995) with peak collisional phases occurring at different times: Cretaceous in the Eastern Alps and Tertiary in the Western Alps (Schmid et al., 2004). Note: prior to the opening of the Paleotethys sea, the Variscan orogenic belt developed in central Europe then the Laurussian and Gondwana converged in the Devonian and Late Carboniferous. Although the location of the suture Extent of the Alpine-Himalayan orogenic belt is not clear, the orogenic belt was extensive, (Rosenbaum and Lister, 2002). running from the Bohemian Massif to the Alpine-Carpathian-Dinarides belt (). The Paleotethys sea existed in the Triassic but closed in the early Mesozoic due to convergence along the Cimmerian (and Indosinian) suture zone. The Paleotethys (or Tethys I) has been described as a wedge- shaped ocean that opened to the east, separating Eurasia from Africa, India, and Australia (Laurasia and Gondwana). Very little evidence of the Paleotethys exists today which has caused some to question its existence (Meyerhoff and Eremenko, 1976) The Tethys opened as Pangea broke up in the Early Jurassic and Africa moved east relative to Europe. -
2012-Ruiz-Martinez-Etal-EPSL.Pdf
Earth and Planetary Science Letters 331-332 (2012) 67–79 Contents lists available at SciVerse ScienceDirect Earth and Planetary Science Letters journal homepage: www.elsevier.com/locate/epsl Earth at 200 Ma: Global palaeogeography refined from CAMP palaeomagnetic data Vicente Carlos Ruiz-Martínez a,b,⁎, Trond H. Torsvik b,c,d,e, Douwe J.J. van Hinsbergen b,c, Carmen Gaina b,c a Departamento de Geofísica y Meteorología, Facultad de Física, Universidad Complutense de Madrid, Avda. Complutense s/n, 28040 Madrid, Spain b Center for Physics of Geological Processes, University of Oslo, 0316 Oslo, Norway c Center of Advanced Study, Norwegian Academy of Science and Letters, 0271 Oslo, Norway d Geodynamics, NGU, N-7491 Trondheim, Norway e School of Geosciences, University of the Witwatersrand, WITS, 2050, South Africa article info abstract Article history: The Central Atlantic Magmatic Province was formed approximately 200 Ma ago as a prelude to the breakup of Received 21 November 2011 Pangea, and may have been a cause of the Triassic–Jurassic mass extinction. Based on a combination of (i) a Received in revised form 26 January 2012 new palaeomagnetic pole from the CAMP related Argana lavas (Moroccan Meseta Block), (ii) a global compila- Accepted 2 March 2012 tion of 190–210 Ma poles, and (iii) a re-evaluation of relative fits between NW Africa, the Moroccan Meseta Available online xxxx Block and Iberia, we calculate a new global 200 Ma pole (latitude=70.1° S, longitude=56.7° E and A95 =2.7°; Editor: P. DeMenocal N=40 poles; NW Africa co-ordinates). We consider the palaeomagnetic database to be robust at 200±10 Ma, which allows us to craft precise reconstructions near the Triassic–Jurassic boundary: at this very important Keywords: time in Earth history, Pangea was near-equatorially centered, the western sector was dominated by plate conver- palaeomagnetism gence and subduction, while in the eastern sector, the Palaeotethys oceanic domain was almost consumed palaeogeography because of a widening Neothethys. -
Mapping a Hidden Terrane Boundary in the Mantle Lithosphere with Lamprophyres
ARTICLE DOI: 10.1038/s41467-018-06253-7 OPEN Mapping a hidden terrane boundary in the mantle lithosphere with lamprophyres Arjan H. Dijkstra 1 & Callum Hatch1,2 Lamprophyres represent hydrous alkaline mantle melts that are a unique source of information about the composition of continental lithosphere. Throughout southwest Britain, post-Variscan lamprophyres are (ultra)potassic with strong incompatible element enrich- 1234567890():,; ments. Here we show that they form two distinct groups in terms of their Sr and Nd isotopic compositions, occurring on either side of a postulated, hitherto unrecognized terrane boundary. Lamprophyres emplaced north of the boundary fall on the mantle array with εNd −1 to +1.6. Those south of the boundary are enriched in radiogenic Sr, have initial εNd values of −0.3 to −3.5, and are isotopically indistinguishable from similar-aged lamprophyres in Armorican massifs in Europe. We conclude that an Armorican terrane was juxtaposed against Avalonia well before the closure of the Variscan oceans and the formation of Pangea. The giant Cornubian Tin-Tungsten Ore Province and associated batholith can be accounted for by the fertility of Armorican lower crust and mantle lithosphere. 1 School of Geography, Earth and Environmental Sciences, Plymouth University, Plymouth PL4 8AA, UK. 2 Department of Core Research Laboratories, Natural History Museum, Cromwell Road, London, SW7 5BD UK. Correspondence and requests for materials should be addressed to A.H.D. (email: [email protected]) NATURE COMMUNICATIONS | (2018) 9:3770 | DOI: 10.1038/s41467-018-06253-7 | www.nature.com/naturecommunications 1 ARTICLE NATURE COMMUNICATIONS | DOI: 10.1038/s41467-018-06253-7 ilson’s cycle1 of the opening and closing of ocean typically form 10 cm to m-wide dykes and other types of minor Wbasins throughout Earth history was based on the intrusions cutting across Variscan foliations in Carboniferous and similarity of Early Palaeozoic faunal assemblages in Devonian rocks. -
A Template for an Improved Rock-Based Subdivision of the Pre-Cryogenian Timescale
Downloaded from http://jgs.lyellcollection.org/ by guest on September 28, 2021 Perspective Journal of the Geological Society Published Online First https://doi.org/10.1144/jgs2020-222 A template for an improved rock-based subdivision of the pre-Cryogenian timescale Graham A. Shields1*, Robin A. Strachan2, Susannah M. Porter3, Galen P. Halverson4, Francis A. Macdonald3, Kenneth A. Plumb5, Carlos J. de Alvarenga6, Dhiraj M. Banerjee7, Andrey Bekker8, Wouter Bleeker9, Alexander Brasier10, Partha P. Chakraborty7, Alan S. Collins11, Kent Condie12, Kaushik Das13, David A. D. Evans14, Richard Ernst15,16, Anthony E. Fallick17, Hartwig Frimmel18, Reinhardt Fuck6, Paul F. Hoffman19,20, Balz S. Kamber21, Anton B. Kuznetsov22, Ross N. Mitchell23, Daniel G. Poiré24, Simon W. Poulton25, Robert Riding26, Mukund Sharma27, Craig Storey2, Eva Stueeken28, Rosalie Tostevin29, Elizabeth Turner30, Shuhai Xiao31, Shuanhong Zhang32, Ying Zhou1 and Maoyan Zhu33 1 Department of Earth Sciences, University College London, London, UK 2 School of the Environment, Geography and Geosciences, University of Portsmouth, Portsmouth, UK 3 Department of Earth Science, University of California at Santa Barbara, Santa Barbara, CA, USA 4 Department of Earth and Planetary Sciences, McGill University, Montreal, Canada 5 Geoscience Australia (retired), Canberra, Australia 6 Instituto de Geociências, Universidade de Brasília, Brasilia, Brazil 7 Department of Geology, University of Delhi, Delhi, India 8 Department of Earth and Planetary Sciences, University of California, Riverside,