Termination of Cryogenian Ironstone Deposition by Deep Ocean Euxinia
Total Page:16
File Type:pdf, Size:1020Kb
Load more
Recommended publications
-
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. -
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. -
Geochemical Characteristics of Late Ordovician Shales in the Upper Yangtze Platform, South China: Implications for Redox Environmental Evolution
minerals Article Geochemical Characteristics of Late Ordovician Shales in the Upper Yangtze Platform, South China: Implications for Redox Environmental Evolution Donglin Lin 1,2,3, Shuheng Tang 1,2,3,*, Zhaodong Xi 1,2,3, Bing Zhang 1,2,3 and Yapei Ye 1,2,3 1 School of Energy Resource, China University of Geosciences, Beijing 100083, China; [email protected] (D.L.); [email protected] (Z.X.); [email protected] (B.Z.); [email protected] (Y.Y.) 2 Key Laboratory of Marine Reservoir Evolution and Hydrocarbon Enrichment Mechanism, Ministry of Education, Beijing 100083, China 3 Key Laboratory of Strategy Evaluation for Shale Gas, Ministry of Land and Resources, Beijing 100083, China * Correspondence: [email protected]; Tel.: +86-134-8882-1576 Abstract: Changes to the redox environment of seawater in the Late Ordovician affect the process of organic matter enrichment and biological evolution. However, the evolution of redox and its underlying causes remain unclear. This paper analyzed the vertical variability of main, trace elements and δ34Spy from a drill core section (well ZY5) in the Upper Yangtze Platform, and described the redox conditions, paleoproductivity and paleoclimate variability recorded in shale deposits of the P. pacificus zone and M. extraordinarius zone that accumulated during Wufeng Formation. The results showed that shale from well ZY5 in Late Ordovician was deposited under oxidized water environment, and Citation: Lin, D.; Tang, S.; Xi, Z.; Zhang, B.; Ye, Y. Geochemical there are more strongly reducing bottom water conditions of the M. extraordinarius zone compared Characteristics of Late Ordovician with the P. -
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. -
Jocelyn A. Sessa
Jocelyn A. Sessa Current: Assistant Curator of Invertebrate Paleontology, Academy of Natural Sciences, & Assistant Professor, Department of Biodiversity, Earth & Environmental Science of Drexel University. Past Positions: 2016 to 2017 Senior Scientist in Paleontology & Education, American Museum of Natural History. Postdoctoral Fellowships: 2012 to 2016 Departments of Paleontology & Education, American Museum of Natural History. 2010 to 2012 Department of Paleobiology, Smithsonian National Museum of Natural History. 2009 to 2010 Department of Earth Sciences, Syracuse University. Education: Ph.D., 2009 Department of Geosciences, Pennsylvania State University, University Park, PA. M.S., 2003 Department of Geology, University of Cincinnati, Cincinnati, Ohio. B.A., 2000 Department of Geological Sciences, State University of New York at Geneseo, Geneseo, NY. Cum laude, minor in Environmental Studies. Publications (* indicates student author; for student work, ‡ indicates corresponding author): Buczek, A.J.*, Hendy, A., Hopkins, M. Sessa, J.A.‡ 2020. On the reconciliation of biostratigraphy and strontium isotope stratigraphy of three southern Californian Plio-Pleistocene formations. Geological Society of America Bulletin 132 ; doi.org/10.1130/B35488.1. Oakes, R.L., Sessa, J.A. 2020. Determining how biotic and abiotic variables affect the shell condition and parameters of Heliconoides inflatus pteropods from a sediment trap in the Cariaco Basin. Biogeosciences 17:1975–1990; doi.org/10.5194/bg-17-1975-2020. Oakes, R.L., Hill Chase, M., Siddall, M.E., Sessa, J.A. 2020. Testing the impact of two key scan parameters on the quality and repeatability of measurements from CT scan data. Palaeontologia Electronica 23(1):a07; doi.org/10.26879/942. Ferguson, K.*, MacLeod, K.G.‡, Landman, N.H., Sessa, J.A.‡ 2019. -
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. -
Microbial Diversity Under Extreme Euxinia: Mahoney Lake, Canada V
Geobiology (2012), 10, 223–235 DOI: 10.1111/j.1472-4669.2012.00317.x Microbial diversity under extreme euxinia: Mahoney Lake, Canada V. KLEPAC-CERAJ,1,2 C. A. HAYES,3 W. P. GILHOOLY,4 T. W. LYONS,5 R. KOLTER2 AND A. PEARSON3 1Department of Molecular Genetics, Forsyth Institute, Cambridge, MA, USA 2Department of Microbiology and Molecular Genetics, Harvard Medical School, Boston, MA, USA 3Department of Earth and Planetary Sciences, Harvard University, Cambridge, MA, USA 4Department of Earth and Planetary Sciences, Washington University, Saint Louis, MO, USA 5Department of Earth Sciences, University of California, Riverside, CA, USA ABSTRACT Mahoney Lake, British Columbia, Canada, is a stratified, 15-m deep saline lake with a euxinic (anoxic, sulfidic) hypolimnion. A dense plate of phototrophic purple sulfur bacteria is found at the chemocline, but to date the rest of the Mahoney Lake microbial ecosystem has been underexamined. In particular, the microbial community that resides in the aphotic hypolimnion and ⁄ or in the lake sediments is unknown, and it is unclear whether the sulfate reducers that supply sulfide for phototrophy live only within, or also below, the plate. Here we profiled distribu- tions of 16S rRNA genes using gene clone libraries and PhyloChip microarrays. Both approaches suggest that microbial diversity is greatest in the hypolimnion (8 m) and sediments. Diversity is lowest in the photosynthetic plate (7 m). Shallower depths (5 m, 7 m) are rich in Actinobacteria, Alphaproteobacteria, and Gammaproteo- bacteria, while deeper depths (8 m, sediments) are rich in Crenarchaeota, Natronoanaerobium, and Verrucomi- crobia. The heterogeneous distribution of Deltaproteobacteria and Epsilonproteobacteria between 7 and 8 m is consistent with metabolisms involving sulfur intermediates in the chemocline, but complete sulfate reduction in the hypolimnion. -
Persistent Global Marine Euxinia in the Early Silurian ✉ Richard G
ARTICLE https://doi.org/10.1038/s41467-020-15400-y OPEN Persistent global marine euxinia in the early Silurian ✉ Richard G. Stockey 1 , Devon B. Cole 2, Noah J. Planavsky3, David K. Loydell 4,Jiří Frýda5 & Erik A. Sperling1 The second pulse of the Late Ordovician mass extinction occurred around the Hirnantian- Rhuddanian boundary (~444 Ma) and has been correlated with expanded marine anoxia lasting into the earliest Silurian. Characterization of the Hirnantian ocean anoxic event has focused on the onset of anoxia, with global reconstructions based on carbonate δ238U 1234567890():,; modeling. However, there have been limited attempts to quantify uncertainty in metal isotope mass balance approaches. Here, we probabilistically evaluate coupled metal isotopes and sedimentary archives to increase constraint. We present iron speciation, metal concentration, δ98Mo and δ238U measurements of Rhuddanian black shales from the Murzuq Basin, Libya. We evaluate these data (and published carbonate δ238U data) with a coupled stochastic mass balance model. Combined statistical analysis of metal isotopes and sedimentary sinks provides uncertainty-bounded constraints on the intensity of Hirnantian-Rhuddanian euxinia. This work extends the duration of anoxia to >3 Myrs – notably longer than well-studied Mesozoic ocean anoxic events. 1 Stanford University, Department of Geological Sciences, Stanford, CA 94305, USA. 2 School of Earth & Atmospheric Sciences, Georgia Institute of Technology, Atlanta, GA 30332, USA. 3 Department of Geology and Geophysics, Yale University, New Haven, CT 06511, USA. 4 School of the Environment, Geography and Geosciences, University of Portsmouth, Portsmouth PO1 3QL, UK. 5 Faculty of Environmental Sciences, Czech University of Life Sciences ✉ Prague, Prague, Czech Republic. -
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. -
Coincidence of Photic Zone Euxinia and Impoverishment of Arthropods
www.nature.com/scientificreports OPEN Coincidence of photic zone euxinia and impoverishment of arthropods in the aftermath of the Frasnian- Famennian biotic crisis Krzysztof Broda1*, Leszek Marynowski2, Michał Rakociński1 & Michał Zatoń1 The lowermost Famennian deposits of the Kowala quarry (Holy Cross Mountains, Poland) are becoming famous for their rich fossil content such as their abundant phosphatized arthropod remains (mostly thylacocephalans). Here, for the frst time, palaeontological and geochemical data were integrated to document abundance and diversity patterns in the context of palaeoenvironmental changes. During deposition, the generally oxic to suboxic conditions were interrupted at least twice by the onset of photic zone euxinia (PZE). Previously, PZE was considered as essential in preserving phosphatised fossils from, e.g., the famous Gogo Formation, Australia. Here, we show, however, that during PZE, the abundance of arthropods drastically dropped. The phosphorous content during PZE was also very low in comparison to that from oxic-suboxic intervals where arthropods are the most abundant. As phosphorous is essential for phosphatisation but also tends to fux of the sediment during bottom water anoxia, we propose that the PZE in such a case does not promote the fossilisation of the arthropods but instead leads to their impoverishment and non-preservation. Thus, the PZE conditions with anoxic bottom waters cannot be presumed as universal for exceptional fossil preservation by phosphatisation, and caution must be paid when interpreting the fossil abundance on the background of redox conditions. 1 Euxinic conditions in aquatic environments are defned as the presence of H2S and absence of oxygen . If such conditions occur at the chemocline in the water column, where light is available, they are defned as photic zone euxinia (PZE). -
This Article Was Published in an Elsevier Journal. the Attached Copy
This article was published in an Elsevier journal. The attached copy is furnished to the author for non-commercial research and education use, including for instruction at the author’s institution, sharing with colleagues and providing to institution administration. Other uses, including reproduction and distribution, or selling or licensing copies, or posting to personal, institutional or third party websites are prohibited. In most cases authors are permitted to post their version of the article (e.g. in Word or Tex form) to their personal website or institutional repository. Authors requiring further information regarding Elsevier’s archiving and manuscript policies are encouraged to visit: http://www.elsevier.com/copyright Author's personal copy Available online at www.sciencedirect.com Geochimica et Cosmochimica Acta 72 (2008) 1396–1414 www.elsevier.com/locate/gca Okenane, a biomarker for purple sulfur bacteria (Chromatiaceae), and other new carotenoid derivatives from the 1640 Ma Barney Creek Formation Jochen J. Brocks a,*, Philippe Schaeffer b a Research School of Earth Sciences and Centre for Macroevolution and Macroecology, The Australian National University, Canberra, ACT 0200, Australia b Laboratoire de Ge´ochimie Bio-organique, CNRS UMR 7177, Ecole Europe´enne de Chimie, Polyme`res et Mate´riaux, 25 rue Becquerel, 67200 Strasbourg, France Received 20 June 2007; accepted in revised form 12 December 2007; available online 23 December 2007 Abstract Carbonates of the 1640 million years (Ma) old Barney Creek Formation (BCF), McArthur Basin, Australia, contain more than 22 different C40 carotenoid derivatives including lycopane, c-carotane, b-carotane, chlorobactane, isorenieratane, b-iso- renieratane, renieratane, b-renierapurpurane, renierapurpurane and the monoaromatic carotenoid okenane. -
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).