Icehouse-Greenhouse Variations in Marine Denitrification
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The Huronian Glaciation
Brasier, A.T., Martin, A.P., Melezhik, V.A., Prave, A.R., Condon, D.J., and Fallick, A.E. (2013) Earth's earliest global glaciation? Carbonate geochemistry and geochronology of the Polisarka Sedimentary Formation, Kola Peninsula, Russia. Precambrian Research, 235 . pp. 278-294. ISSN 0301-9268 Copyright © 2013 Elsevier B.V. A copy can be downloaded for personal non-commercial research or study, without prior permission or charge Content must not be changed in any way or reproduced in any format or medium without the formal permission of the copyright holder(s) When referring to this work, full bibliographic details must be given http://eprints.gla.ac.uk/84700 Deposited on: 29 August 2013 Enlighten – Research publications by members of the University of Glasgow http://eprints.gla.ac.uk 1 Earth’s earliest global glaciation? Carbonate geochemistry and geochronology of the 2 Polisarka Sedimentary Formation, Kola Peninsula, Russia 3 4 A.T. Brasier1,6*, A.P. Martin2+, V.A. Melezhik3,4, A.R. Prave5, D.J. Condon2, A.E. Fallick6 and 5 FAR-DEEP Scientists 6 7 1 Faculty of Earth and Life Sciences, Vrije Universiteit Amsterdam, De Boelelaan 1085, 1081HV 8 Amsterdam 9 2 NERC Isotope Geosciences Laboratory, British Geological Survey, Environmental Science 10 Centre, Keyworth, UK. NG12 5GG 11 3 Geological Survey of Norway, Postboks 6315 Slupen, NO-7491 Trondheim, Norway 12 4 Centre for Geobiology, University of Bergen, Postboks 7803, NO-5020 Bergen, Norway 13 5 Department of Earth and Environmental Sciences, University of St Andrews, St Andrews KY16 14 9AL, Scotland, UK 15 6 Scottish Universities Environmental Research Centre, Rankine Avenue, East Kilbride, Scotland. -
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. -
Neoproterozoic Glaciations in a Revised Global Palaeogeography from the Breakup of Rodinia to the Assembly of Gondwanaland
Sedimentary Geology 294 (2013) 219–232 Contents lists available at SciVerse ScienceDirect Sedimentary Geology journal homepage: www.elsevier.com/locate/sedgeo Invited review Neoproterozoic glaciations in a revised global palaeogeography from the breakup of Rodinia to the assembly of Gondwanaland Zheng-Xiang Li a,b,⁎, David A.D. Evans b, Galen P. Halverson c,d a ARC Centre of Excellence for Core to Crust Fluid Systems (CCFS) and The Institute for Geoscience Research (TIGeR), Department of Applied Geology, Curtin University, GPO Box U1987, Perth, WA 6845, Australia b Department of Geology and Geophysics, Yale University, New Haven, CT 06520-8109, USA c Earth & Planetary Sciences/GEOTOP, McGill University, 3450 University St., Montreal, Quebec H3A0E8, Canada d Tectonics, Resources and Exploration (TRaX), School of Earth and Environmental Sciences, University of Adelaide, SA 5005, Australia article info abstract Article history: This review paper presents a set of revised global palaeogeographic maps for the 825–540 Ma interval using Received 6 January 2013 the latest palaeomagnetic data, along with lithological information for Neoproterozoic sedimentary basins. Received in revised form 24 May 2013 These maps form the basis for an examination of the relationships between known glacial deposits, Accepted 28 May 2013 palaeolatitude, positions of continental rifting, relative sea-level changes, and major global tectonic events Available online 5 June 2013 such as supercontinent assembly, breakup and superplume events. This analysis reveals several fundamental ’ Editor: J. Knight palaeogeographic features that will help inform and constrain models for Earth s climatic and geodynamic evolution during the Neoproterozoic. First, glacial deposits at or near sea level appear to extend from high Keywords: latitudes into the deep tropics for all three Neoproterozoic ice ages (Sturtian, Marinoan and Gaskiers), al- Neoproterozoic though the Gaskiers interval remains very poorly constrained in both palaeomagnetic data and global Rodinia lithostratigraphic correlations. -
Structural and Tectonic Evolution of the Acatlán Complex, Southern Mexico
TECTONICS, VOL. 28, TC4008, doi:10.1029/2007TC002159, 2009 Click Here for Full Article Structural and tectonic evolution of the Acatla´n Complex, southern Mexico: Its role in the collisional history of Laurentia and Gondwana Ricardo Vega-Granillo,1 Thierry Calmus,2 Diana Meza-Figueroa,1 Joaquı´n Ruiz,3 Oscar Talavera-Mendoza,4 and Margarita Lo´pez-Martı´nez5 Received 24 May 2007; revised 22 January 2009; accepted 10 March 2009; published 25 July 2009. [1] Correlation of deformational phases and thermal opening. Citation: Vega-Granillo, R., T. Calmus, D. Meza- events in the Acatla´n Complex permits definition of Figueroa, J. Ruiz, O. Talavera-Mendoza, and M. Lo´pez-Martı´nez nine major tectonic events. Seven events are related to (2009), Structural and tectonic evolution of the Acatla´n Complex, the evolution of the Iapetus and Rheic oceans. By the southern Mexico: Its role in the collisional history of Laurentia Early Ordovician, the Xayacatla´n suite of Laurentian and Gondwana, Tectonics, 28, TC4008, doi:10.1029/ affinity was metamorphosed to eclogite facies and 2007TC002159. exhumed before colliding with the El Rodeo suite. From the Late Ordovician to Silurian, the Upper 1. Introduction Ordovician Ixcamilpa suite with peri-Gondwanan affinity was metamorphosed to blueschist facies, [2] The Acatla´n Complex basement of the Mixteco exhumed, and subsequently was overthrust by the terrane contains the largest exposure of eclogites, high-P Xayacatla´n–El Rodeo block. Part of the Esperanza garnet amphibolites, blueschists and eclogitized granitoids of Paleozoic age in Mexico. In a strict sense, the Mixteco suite is an Early Silurian intra-Iapetian continental arc terrane must be considered a superterrane composed of that collided with and subducted beneath continental thrust sheets containing Mesoproterozoic to Paleozoic pet- crust, generating a Silurian eclogitic event. -
The History of Ice on Earth by Michael Marshall
The history of ice on Earth By Michael Marshall Primitive humans, clad in animal skins, trekking across vast expanses of ice in a desperate search to find food. That’s the image that comes to mind when most of us think about an ice age. But in fact there have been many ice ages, most of them long before humans made their first appearance. And the familiar picture of an ice age is of a comparatively mild one: others were so severe that the entire Earth froze over, for tens or even hundreds of millions of years. In fact, the planet seems to have three main settings: “greenhouse”, when tropical temperatures extend to the polesand there are no ice sheets at all; “icehouse”, when there is some permanent ice, although its extent varies greatly; and “snowball”, in which the planet’s entire surface is frozen over. Why the ice periodically advances – and why it retreats again – is a mystery that glaciologists have only just started to unravel. Here’s our recap of all the back and forth they’re trying to explain. Snowball Earth 2.4 to 2.1 billion years ago The Huronian glaciation is the oldest ice age we know about. The Earth was just over 2 billion years old, and home only to unicellular life-forms. The early stages of the Huronian, from 2.4 to 2.3 billion years ago, seem to have been particularly severe, with the entire planet frozen over in the first “snowball Earth”. This may have been triggered by a 250-million-year lull in volcanic activity, which would have meant less carbon dioxide being pumped into the atmosphere, and a reduced greenhouse effect. -
Timing and Tempo of the Great Oxidation Event
Timing and tempo of the Great Oxidation Event Ashley P. Gumsleya,1, Kevin R. Chamberlainb,c, Wouter Bleekerd, Ulf Söderlunda,e, Michiel O. de Kockf, Emilie R. Larssona, and Andrey Bekkerg,f aDepartment of Geology, Lund University, Lund 223 62, Sweden; bDepartment of Geology and Geophysics, University of Wyoming, Laramie, WY 82071; cFaculty of Geology and Geography, Tomsk State University, Tomsk 634050, Russia; dGeological Survey of Canada, Ottawa, ON K1A 0E8, Canada; eDepartment of Geosciences, Swedish Museum of Natural History, Stockholm 104 05, Sweden; fDepartment of Geology, University of Johannesburg, Auckland Park 2006, South Africa; and gDepartment of Earth Sciences, University of California, Riverside, CA 92521 Edited by Mark H. Thiemens, University of California, San Diego, La Jolla, CA, and approved December 27, 2016 (received for review June 11, 2016) The first significant buildup in atmospheric oxygen, the Great situ secondary ion mass spectrometry (SIMS) on microbaddeleyite Oxidation Event (GOE), began in the early Paleoproterozoic in grains coupled with precise isotope dilution thermal ionization association with global glaciations and continued until the end of mass spectrometry (ID-TIMS) and paleomagnetic studies, we re- the Lomagundi carbon isotope excursion ca. 2,060 Ma. The exact solve these uncertainties by obtaining accurate and precise ages timing of and relationships among these events are debated for the volcanic Ongeluk Formation and related intrusions in because of poor age constraints and contradictory stratigraphic South Africa. These ages lead to a more coherent global per- correlations. Here, we show that the first Paleoproterozoic global spective on the timing and tempo of the GOE and associated glaciation and the onset of the GOE occurred between ca. -
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. -
Suprasubduction Zone Setting for the Youngest Rheic Ocean Floor
CORE Metadata, citation and similar papers at core.ac.uk Provided by EPrints Complutense Care6n ophiolite, NW Spain: Suprasubduction zone setting for the youngest Rheic Ocean floor Sonia Sanchez Martfnez "" Departamento de Petrologla y Geoqulmlca, Unlversldad Complutense, 28040 Madrid, Spain R·Icar d 0 Arenas } Florentino Dfaz Garcfa Departamento de Geologia, Unlversldad de OVledo, 33005 OVledo, Spain Jose Ram6n Martfnez Catalan Departamento de Geologia, Unlversldad de Salamanca, 37008 Salamanca, Spain Juan G6mez-Barreiro Department of Earth & Planetary SCiences, University of California at Berkeley, Berkeley, California 94720, USA Julian A. Pearce School of Earth, Ocean and Planetary SCiences, Cardiff University, CFto 3YE Cardiff, UK ABSTRACT included in the GSA Data Repository.l The The Careon ophiolite (Galicia, NW Iberian MassiO shows lithological and geochemical geochemical features of these samples (Fig. 2; features suggestive of an origin in a suprasubduction zone setting. As with other Devonian Fig. DRI [see footnote I]) show that most of the ophiolites in the European Variscan belt, it was generated within a contracting Rheic Ocean. studied metabasites have compositions equiva This setting and the general absence of large Silurian-Devonian volcanic arcs on both of the lent to tholeiitic basalts (Fig. DRIA). Average Rheic Ocean margins strongly suggest that this ocean was closed by intraoceanic subduction rare earth element (REE) contents (Rg. DRl B) directed to the north. This subduction removed the older normal (N) mid-oceanic-ridge basalt of most rock types have concentrations around (MORB) oceanic lithosphere and gave rise to a limited volume of new suprasubduction zone ten times the chondrite abundances and ahnost oceanic lithosphere. -
Subglacial Meltwater Supported Aerobic Marine Habitats During Snowball Earth
Subglacial meltwater supported aerobic marine habitats during Snowball Earth Maxwell A. Lechtea,b,1, Malcolm W. Wallacea, Ashleigh van Smeerdijk Hooda, Weiqiang Lic, Ganqing Jiangd, Galen P. Halversonb, Dan Asaele, Stephanie L. McColla, and Noah J. Planavskye aSchool of Earth Sciences, University of Melbourne, Parkville, VIC 3010, Australia; bDepartment of Earth and Planetary Science, McGill University, Montréal, QC, Canada H3A 0E8; cState Key Laboratory for Mineral Deposits Research, School of Earth Sciences and Engineering, Nanjing University, 210093 Nanjing, China; dDepartment of Geoscience, University of Nevada, Las Vegas, NV 89154; and eDepartment of Geology and Geophysics, Yale University, New Haven, CT 06511 Edited by Paul F. Hoffman, University of Victoria, Victoria, BC, Canada, and approved November 3, 2019 (received for review May 28, 2019) The Earth’s most severe ice ages interrupted a crucial interval in Cryogenian ice age. These marine chemical sediments are unique eukaryotic evolution with widespread ice coverage during the geochemical archives of synglacial ocean chemistry. To develop Cryogenian Period (720 to 635 Ma). Aerobic eukaryotes must have sur- a global picture of seawater redox state during extreme glaci- vived the “Snowball Earth” glaciations, requiring the persistence of ation, we studied 9 IF-bearing Sturtian glacial successions across 3 oxygenated marine habitats, yet evidence for these environments paleocontinents (Fig. 1): Congo (Chuos Formation, Namibia), is lacking. We examine iron formations within globally distributed Australia (Yudnamutana Subgroup), and Laurentia (Kingston Cryogenian glacial successions to reconstruct the redox state of the Peak Formation, United States). These IFs were selected for synglacial oceans. Iron isotope ratios and cerium anomalies from a analysis because they are well-preserved, and their depositional range of glaciomarine environments reveal pervasive anoxia in the environment can be reliably constrained. -
Duration and Nature of the End-Cryogenian (Marinoan) Glaciation
1 Duration and nature of the end-Cryogenian (Marinoan) glaciation 2 1Anthony R. Prave, 2Daniel J. Condon, 3Karl Heinz Hoffmann, 2Simon Tapster, and 4Anthony 3 E. Fallick 4 1Department of Earth and Environmental Sciences, University of St Andrews, St Andrews, KY16 5 9AL, UK 6 2NERC Isotope Geosciences Laboratory, British Geological Survey, Nottingham, NG12 5GG, UK 7 3Geological Survey of Namibia, 1 Aviation Road, Windhoek, Namibia 8 4Scottish Universities Environmental Research Centre, East Kilbride, G75 0QF, UK 9 10 ABSTRACT 11 The end-Cryogenian glaciation (Marinoan) was Earth’s last global glaciation yet its duration 12 and character remain uncertain. Here we report U-Pb zircon ages for two discrete ash beds within 13 glacimarine deposits from widely separated localities of the Marinoan-equivalent Ghaub Formation 14 in Namibia: 639.29 ± 0.26/0.31/0.75 Ma and 635.21 ± 0.59/0.61/0.92 Ma. These findings, for the 15 first time, verify the key prediction of the Snowball Earth hypothesis for the Marinoan glaciation: 16 longevity, with a duration of ≥4.08 ± 0.64 Myr. They also show that glacigenic sedimentation, 17 erosion, and at least intermittent open-water conditions occurred 4 million years prior to termination 18 of the Marinoan glaciation and that the interval of non-glacial conditions between the two 19 Cryogenian glaciations was 20 Myr or less. 20 INTRODUCTION 21 The Cryogenian Period (c. 720 – 635 Ma) was marked by the two most severe glaciations in 22 Earth history (Hoffman et al., 1998; Fairchild and Kennedy, 2007), the older Sturtian and younger 23 Marinoan, and their association with unique lithofacies of cap carbonates (Kennedy et al., 2001; 24 Hoffman and Schrag, 2002; Hoffman et al., 2011), stable isotope fluctuations (carbon, oxygen, 25 boron, calcium; Halverson et al., 2005; Kasemann et al., 2005; Bao et al., 2008) and banded iron 26 formation are evidence for global-scale environmental changes with postulated links to ocean- 27 atmosphere oxygenation and biosphere evolution (Butterfield, 2009; Och and Sjields-Zhou, 2012; 28 Sperling et al., 2013). -
(Acadian) Orogenic Events in Scotland John R Mendum British Geological Survey, Edinburgh
Late Caledonian (Scandian) and Proto-Variscan (Acadian) orogenic events in Scotland John R Mendum British Geological Survey, Edinburgh Abstract The later tectonic phases of the Caledonian Orogeny reflect the collision of Baltica and Laurentia. The result was the Scandian event in Silurian times, and the oblique docking of Eastern Avalonia with Scotland, generating deformation and metamorphism in the Southern Uplands. The exhumation of the Caledonide Orogen was then accompanied by sinistral transtensional faulting and emplacement of granitoid plutons. The Iapetus Ocean was finally closed, and subduction activity had migrated south to the Rheic Ocean by early Devonian times. Continental rifting and deposition of the Lower Old Red Sandstone fluvial-lacustrine succession, accompanied by basaltic-andesitic volcanism, occurred across Scotland. Deposition commenced in the late Silurian and continued through to Emsian times, when it was interrupted by the short-lived, northward-directed Acadian event. The resultant deformation and folding, a product of sinistral transpression, were focussed along the major pre-existing faults and shear zones. Evidence for Acadian transpressional movements along the Great Glen Fault (GGF) is found near Rosemarkie, where Moine psammites and semipelites are interleaved with Lewisianoid gneisses in a structural inlier. These lithologies are intruded by pink leucogranite veins that themselves show evidence of two phases of ductile deformation and folding. U-Pb monazite and zircon ages show that the leucogranites were emplaced at c. 399 Ma. Leucogranite intrusion and subsequent deformation are interpreted to have occurred during oblique extrusion of the inlier as an elongate ‘pip’, generated at a northwestward step-over that developed on the GGF during the Acadian Event. -
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Contents lists available at ScienceDirect Palaeogeography, Palaeoclimatology, Palaeoecology journal homepage: www.elsevier.com/locate/palaeo Pangea B and the Late Paleozoic Ice Age ⁎ D.V. Kenta,b, ,G.Muttonic a Earth and Planetary Sciences, Rutgers University, Piscataway, NJ 08854, USA b Lamont-Doherty Earth Observatory of Columbia University, Palisades, NY 10964, USA c Dipartimento di Scienze della Terra 'Ardito Desio', Università degli Studi di Milano, via Mangiagalli 34, I-20133 Milan, Italy ARTICLE INFO ABSTRACT Editor: Thomas Algeo The Late Paleozoic Ice Age (LPIA) was the penultimate major glaciation of the Phanerozoic. Published compi- Keywords: lations indicate it occurred in two main phases, one centered in the Late Carboniferous (~315 Ma) and the other Late Paleozoic Ice Age in the Early Permian (~295 Ma), before waning over the rest of the Early Permian and into the Middle Permian Pangea A (~290 Ma to 275 Ma), and culminating with the final demise of Alpine-style ice sheets in eastern Australia in the Pangea B Late Permian (~260 to 255 Ma). Recent global climate modeling has drawn attention to silicate weathering CO2 Greater Variscan orogen consumption of an initially high Greater Variscan edifice residing within a static Pangea A configuration as the Equatorial humid belt leading cause of reduction of atmospheric CO2 concentrations below glaciation thresholds. Here we show that Silicate weathering CO2 consumption the best available and least-biased paleomagnetic reference poles place the collision between Laurasia and Organic carbon burial Gondwana that produced the Greater Variscan orogen in a more dynamic position within a Pangea B config- uration that had about 30% more continental area in the prime equatorial humid belt for weathering and which drifted northward into the tropical arid belt as it transformed to Pangea A by the Late Permian.