Inside: Emergence of the Aerobic Biosphere During the Archean-Proterozoic Transition: Challenges of Future Research, by Victor A

Total Page:16

File Type:pdf, Size:1020Kb

Inside: Emergence of the Aerobic Biosphere During the Archean-Proterozoic Transition: Challenges of Future Research, by Victor A VOL. 15, No. 11 A PUBLICATION OF THE GEOLOGICAL SOCIETY OF AMERICa NOVEMBER 2005 Inside: Emergence of the aerobic biosphere during the Archean-Proterozoic transition: Challenges of future research, by Victor A. Melezhik et Al., p. 4 Section Meetings: Cordilleran, p. 12 Rocky Mountain, p. 15 VoluMe 15, NuMbeR 11 NOveMbeR 2005 Cover: Paleoproterozoic (2200 Ma) lacustrine dolostone from the Pechenga Greenstone belt, northeast Fennoscandian Shield. Width of field is 15 cm. The laminated red (oxidized) dolostone is anomalously enriched in 13C (δ13C = +8‰), while the overlying material, representing the oldest known traver- GSA TODAY publishes news and information for more than tines in the world, are 13C-depleted (δ13C = −7‰). Note that 18,000 GSA members and subscribing libraries. GSA Today these rocks have experienced greenschist-facies metamor- lead science articles should present the results of exciting new phism. The 13C-rich dolostones from the Fennoscandian Shield research or summarize and synthesize important problems exemplify the evidence for an extreme global perturbation to or issues, and they must be understandable to all in the earth the carbon cycle at this time, although interpretation of these science community. Submit manuscripts to science editors 13 Keith A. Howard, [email protected], or Gerald M. Ross, lacustrine rocks in terms of a global marine δ C excursion is [email protected]. not straightforward. See “emergence of the aerobic biosphere during the Archean-Proterozoic transition: Challenges of future GSA TODAY (ISSN 1052-5173 USPS 0456-530) is published 11 research,” by Victor A. Melezhik et al., p. 4–11. times per year, monthly, with a combined April/May issue, by The Geological Society of America, Inc., with offices at 3300 Penrose Place, Boulder, Colorado. Mailing address: P.O. Box 9140, Boulder, CO 80301-9140, USA. Periodicals postage paid at Boulder, Colorado, and at additional mailing offices. Postmaster: Send address changes to GSA Today, GSA Sales and Service, SCIENCE ARTICLE P.O. Box 9140, Boulder, CO 80301-9140. Copyright © 2005, The Geological Society of America, Inc. (GSA). All rights reserved. Copyright not claimed on content prepared 4 Emergence of the aerobic biosphere during the Archean- wholly by U.S. government employees within scope of their Proterozoic transition: Challenges of future research, employment. Individual scientists are hereby granted permission, ICTOR ELEZHIK NTHONY ALLICK ERO ANSKI EE UMP without fees or further requests to GSA, to use a single figure, a V A. M , A E. F , E J. H , L R. K , single table, and/or a brief paragraph of text in other subsequent AIVO LEPLAND, ANTHONY R. PRavE, AND HARALD STRAUSS works and to make unlimited photocopies of items in this journal for noncommercial use in classrooms to further education and science. For any other use, contact Copyright Permissions, GSA, P.O. Box 9140, Boulder, CO 80301-9140, USA, Fax 303- 357-1073, [email protected]; reference GSA Today, ISSN 12 Preliminary Announcement and Call for Papers: 1052-5173. Permission is granted to authors to post the abstracts Cordilleran Section only of their articles on their own or their organization’s Web site providing the posting includes this reference: “The full paper was published in the Geological Society of America’s journal GSA 15 Preliminary Announcement and Call for Papers: Today, [include year, month, and page numbers if known, where Rocky Mountain Section the article will appear].” GSA provides this and other forums for the presentation of diverse opinions and positions by scientists worldwide, regardless of their race, citizenship, gender, religion, 17 Call for Geological Papers: 2006 GSA Section Meetings or political viewpoint. Opinions presented in this publication do not reflect official positions of the Society. 17 Invitation from GSA’s History of Geology Division SUBSCRIPTIONS for 2005 calendar year: Society Members: GSA Today is provided as part of membership dues. Contact 18 Upcoming Deadlines GSA Sales and Service at 1-888-443-4472, (303) 357-1000, option 3, or [email protected] for membership 20 2006 Birdsall-Dreiss Lecturer information. Nonmembers & Institutions: Free with paid subscription to both GSA Bulletin and Geology, otherwise 21 2006 Jahns Distinguished Lecturer $75. Contact Subscription Services at (800) 627-0629 or [email protected]. Also available on an annual CD-ROM (together with GSA Bulletin, Geology, GSA Data Repository, and 21 GSA Offers Awards in Geomorphology and Micropaleontology an Electronic Retrospective Index to journal articles from 1972); $99 to GSA Members, others call GSA Subscription Services 22 2005 Biggs Awardee Named for prices and details. Claims: For nonreceipt or for damaged copies, members contact GSA Sales and Service; all others 22 Call for Applications: 2006–2007 GSA–USGS Congressional contact Subscription Services. Claims are honored for one year; please allow sufficient delivery time for overseas copies, up to Science Fellowship six months. GSA Today STAFF: 23 A New Use for Old Geology Books and Journals Executive Director: John W. Hess TM Science Editors: Keith A. Howard, U.S. Geological Survey, 24 GeoVentures Memories MS 919, Menlo Park, CA 94025, USA, [email protected]; and Gerald M. Ross, Kupa’a Farm, Box 458, Kula, HI 96790, 25 GeoHostelTM: The Tectonic Development of Southern California [email protected]. Director of Publications: Jon Olsen TM Managing Editor: Kristen E. Asmus, [email protected] 26 GeoCorps America: 2005 Participants Editorial Staff: Matt Hudson, Beth Clemens Production Coordinator: Margo Y. Sajban 27 Call for Proposals: Short Courses and K–16 Workshops Graphics Production: Margo Y. Sajban ADVERTISING: 28 GSA Foundation Update Classifieds & Display: Ann Crawford, 1-800-472-1988, ext. 1053, (303) 357-1053, Fax 303-357-1070; [email protected] 29 Changes to GSA Graduate Student Research Grant Eligibility GSA ONLINE: www.geosociety.org 30 GSA Awards First Science Fair Prizes Printed in the USA using pure soy inks. 32 Classified Advertising 38 GeoMart Geoscience Directory 50% Total Recovered Fiber 10% Postconsumer 39 Journal Highlights of the Proterozoic, Earth’s lithosphere underwent the assem- bly of two supercontinents: one, Kenorland, comprising the Laurentian, Fennoscandian, and Siberian shields; the other, the amalgamated Zimbabwe, Kaapvaal, Pilbara, Sao Francisco, and Indian cratons (Aspler and Chiarenzelli, 1998; Williams et al., 1991). Subsequent breakup involved the emplacement of voluminous continental flood basalts, giant radiating dike swarms and layered gabbro-norite intrusions (e.g., Heaman, 1997; Vogel et al., 1998), and deposition of banded iron for- mations (Pickard, 2003). Profound climatic and biogeochemi- cal events also were occurring, such as icehouse conditions (Young et al., 2001; Evans, 2003), the rise in atmospheric oxy- gen levels (Bekker et al., 2004), and the largest and longest Victor A. Melezhik, Geological Survey of Norway, Leiv duration positive excursion of carbon isotopic composition Eirikssons vei 39, 7491 Trondheim, Norway; Anthony E. of sedimentary carbonates (Lomagundi-Jatuli Event), which Fallick, Scottish Universities Environmental Research Centre, predated deposition of anomalously organic carbon–rich sedi- Rankine Avenue, East Kilbride, Glasgow G75 0QF, Scotland; ments forming giant petroleum fields (Shunga Event; both Eero J. Hanski, University of Oulu, Linnanmaa, 90014 Oulu, events are reviewed in Melezhik et al., 1999a, 1999b). It was Finland; Lee R. Kump*, Dept. of Geosciences, Pennsylvania out of this period of geological upheaval that the aerobic State University, 535 Deike Bldg, University Park, Pennsylvania earth system began to emerge, with biogeochemical cycles 16802, USA; Aivo Lepland, Geological Survey of Norway, Leiv in the oceans and on land using the highly energetic aerobic Eirikssons vei 39, 7491 Trondheim, Norway; Anthony R. Prave, pathway. Note though that some workers suggest that deep University of St. Andrews, St. Andrews, Fife KY16 9AL, Scotland; marine basins and perhaps the global deep ocean itself were euxinic (rich in H S) for much of the ensuing Proterozoic Harald Strauss, Westfälische Wilhelms–Universität Münster, 2 Corrensstraße 24, 48149 Münster, Germany (Canfield, 1998; Anbar and Knoll, 2002; Poulton et al., 2004). Here we present a synthesis of the hallmark features of the Archean-Paleoproterozoic transition in the Fennoscandian ABSTRACT Shield (Fig. 1). It is representative of other shield areas and The earth system experienced a series of fundamental provides important insights into the biogeochemical evolution upheavals throughout the Archean-Paleoproterozoic transition of the earth system. (ca. 2500–2000 Ma). Most important were the establishment of Early Paleoproterozoic Environmental Upheavals: an oxygen-rich atmosphere and the emergence of an aerobic Insight from the Fennoscandian Shield biosphere. Fennoscandia provides a fairly complete record The Fennoscandian Shield comprises Archean, of the hallmark events of that transition: widespread igneous Paleoproterozoic, and Mesoproterozoic domains (Fig. 1). activity, its association with a possible upper-mantle oxidizing In particular, its eastern part is a composite of Late Archean event, the global Huronian glaciation, a rise in atmospheric granite-greenstone belts, Paleoproterozoic rifts, the ca. 1900 oxygen, the protracted and large-magnitude Lomagundi-Jatuli Ma Kola Orogen, and multiphase Svecofennian orogens. carbon isotope excursion, a
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.
    [Show full text]
  • Timeline of Natural History
    Timeline of natural history This timeline of natural history summarizes significant geological and Life timeline Ice Ages biological events from the formation of the 0 — Primates Quater nary Flowers ←Earliest apes Earth to the arrival of modern humans. P Birds h Mammals – Plants Dinosaurs Times are listed in millions of years, or Karo o a n ← Andean Tetrapoda megaanni (Ma). -50 0 — e Arthropods Molluscs r ←Cambrian explosion o ← Cryoge nian Ediacara biota – z ←Earliest animals o ←Earliest plants i Multicellular -1000 — c Contents life ←Sexual reproduction Dating of the Geologic record – P r The earliest Solar System -1500 — o t Precambrian Supereon – e r Eukaryotes Hadean Eon o -2000 — z o Archean Eon i Huron ian – c Eoarchean Era ←Oxygen crisis Paleoarchean Era -2500 — ←Atmospheric oxygen Mesoarchean Era – Photosynthesis Neoarchean Era Pong ola Proterozoic Eon -3000 — A r Paleoproterozoic Era c – h Siderian Period e a Rhyacian Period -3500 — n ←Earliest oxygen Orosirian Period Single-celled – life Statherian Period -4000 — ←Earliest life Mesoproterozoic Era H Calymmian Period a water – d e Ectasian Period a ←Earliest water Stenian Period -4500 — n ←Earth (−4540) (million years ago) Clickable Neoproterozoic Era ( Tonian Period Cryogenian Period Ediacaran Period Phanerozoic Eon Paleozoic Era Cambrian Period Ordovician Period Silurian Period Devonian Period Carboniferous Period Permian Period Mesozoic Era Triassic Period Jurassic Period Cretaceous Period Cenozoic Era Paleogene Period Neogene Period Quaternary Period Etymology of period names References See also External links Dating of the Geologic record The Geologic record is the strata (layers) of rock in the planet's crust and the science of geology is much concerned with the age and origin of all rocks to determine the history and formation of Earth and to understand the forces that have acted upon it.
    [Show full text]
  • 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.
    [Show full text]
  • The Ice Age in North Hertfordshire
    The Ice Age in North Hertfordshire What do we mean by ‘the Ice Age’? Thinking about ‘the Ice Age’ brings up images of tundra, mammoths, Neanderthals and great sheets of ice across the landscape. This simple picture is wrong in many ways. Firstly, there have been many different ‘Ice Ages’ in the history of the earth. The most dramatic happened between 2.4 and 2.1 billion years ago, known as the Huronian Glaciation. About the same time, earth’s atmosphere suddenly became rich in oxygen, and some scientists believe that the atmospheric changes reduced the temperature so much that the whole planet became covered in ice. 1: an Arctic ice sheet (© Youino Joe, USFWS, used under a Creative Commons licence) Another global cover of ice happened 650 million years ago when the first multi-celled animals were evolving. Geologists sometimes refer to this period as the ‘Snowball Earth’ and biologists know it as the Proterozoic. Temperatures were so low that the equator was as cold as present-day Antarctica. They began to rise again as concentrations of carbon dioxide in the atmosphere rose to about 13%, 350 times greater than today. Some carbon dioxide came from volcanic eruptions, but some was excreted by microbial life, which was beginning to diversify and increase in numbers. Neither of these Ice Ages is the one that dominates the popular imagination. Both happened many millions of years before life moved on to land. There were no humans, no mammals, no dinosaurs: none of the creatures familiar from The Flintstones. The period most people think about as the ‘real’ Ice Age is the geologists’ Pleistocene era, from more than two-and-a-half million years ago to the beginning of the Holocene, almost 12,000 years ago.
    [Show full text]
  • 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.
    [Show full text]
  • Manganese Enrichment in the Gowganda Formation of the Huronian Supergroup: a Highly Oxidizing Shallow-Marine Environment After the Last Huronian Glaciation
    Earth and Planetary Science Letters 307 (2011) 201–210 Contents lists available at ScienceDirect Earth and Planetary Science Letters journal homepage: www.elsevier.com/locate/epsl Manganese enrichment in the Gowganda Formation of the Huronian Supergroup: A highly oxidizing shallow-marine environment after the last Huronian glaciation Yasuhito Sekine a,⁎, Eiichi Tajika a, Ryuji Tada b, Takemaru Hirai b,1, Kosuke T. Goto b, Tatsu Kuwatani a, Kazuhisa Goto c, Shinji Yamamoto b, Shogo Tachibana b, Yukio Isozaki d, Joseph L. Kirschvink e a Dept. of Complexity Sci. & Engr., Univ. of Tokyo, Kashiwa, Chiba 277–8561, Japan b Dept. of Earth & Planetary Sci., Univ. of Tokyo, Bunkyo, Tokyo 113-0033, Japan c Planetary Exploration Res. Center, Chiba Inst. of Tech., Tsudanuma, Chiba 275–0016, Japan d Dept. of Earth Science & Astronomy, Univ. of Tokyo, Meguro, Tokyo 153–8902, Japan e Division of Geological & Planetary Sci., California Inst. of Tech., Pasadena, California 91125, USA article info abstract Article history: Oxidative precipitation and authigenic enrichment of the redox sensitive element Mn in sedimentary rocks Received 14 February 2011 can serve as a proxy for the release of high levels of O2 during the Great Oxidization Event (GOE). Here we Received in revised form 27 April 2011 investigate Mn abundance in sedimentary rocks of the 2.45–2.22 Ga Huronian Supergroup, Canada. We found Accepted 1 May 2011 authigenic Mn enrichments with high Mn/Fe ratios following the appearance of Fe oxides in the Firstbrook Available online 23 May 2011 Member of the Gowganda Formation of the Huronian Supergroup, which was deposited immediately after the Editor: P.
    [Show full text]
  • 5.18 Soils and Global Change in the Carbon Cycle Over Geological Time G
    5.18 Soils and Global Change in the Carbon Cycle over Geological Time G. J. Retallack University of Oregon, Eugene, OR, USA 5.18.1 INTRODUCTION 1 5.18.2 APPROACHES TO THE STUDY OF PALEOSOLS 3 5.18.2.1 Molecular Weathering Ratios 4 5.18.2.2 Strain and Mass-Transfer Analysis 5 5.18.2.3 Analyses of Stable Isotopes of Carbon and Oxygen 7 5.18.3 RECORD OF PAST SOIL AND GLOBAL CHANGE 7 5.18.3.1 Origins of Soil 8 5.18.3.2 Archean–Paleoproterozoic Greenhouse Paleosols 9 5.18.3.3 Proterozoic Icehouse Paleosols 10 5.18.3.4 Cambro-Ordovician Greenhouse Paleosols 11 5.18.3.5 Terminal Ordovician Icehouse Paleosols 13 5.18.3.6 Siluro-Devonian Greenhouse Paleosols 13 5.18.3.7 Late Devonian to Permian Icehouse Paleosols 13 5.18.3.8 Triassic–Jurassic Greenhouse Paleosols 15 5.18.3.9 Early Cretaceous Icehouse Paleosols 17 5.18.3.10 Cretaceous–Paleogene Greenhouse Paleosols 17 5.18.3.11 Neogene Icehouse Paleosols 17 5.18.3.12 Pleistocene Glacial and Interglacial Paleosols 19 5.18.4 SOILS AND GLOBAL CARBON CYCLE CHANGES 21 ACKNOWLEDGMENTS 23 REFERENCES 23 5.18.1 INTRODUCTION amplified by biological acidification (Schwartz- mann and Volk, 1991; see Chapter 5.06). These Soils play an important role in the carbon mineral nutrients fuel photosynthetic fixation cycle as the nutrition of photosynthesized bio- and chemical reduction of atmospheric CO2 mass. Nitrogen fixed by microbes from air is a into plants and plantlike microbes, which are at limiting nutrient for ecosystems within the first the base of the food chain.
    [Show full text]
  • CLIMATIC CHANGES: Anthropogenic Influence Or Naturally Induced Phenomenon
    CLIMATIC CHANGES: Anthropogenic Influence Or Naturally Induced Phenomenon By Anthony Foscolos 1 CLIMATIC CHANGES: Anthropogenic Influence or Naturally Induced Phenomenon By A.E. Foscolos Department of Mineral Resources Engineering Technical University of Crete By the end of the 18th century eminent scientists (Franklin, 1784; Fourier, 1824; 1827; Agassiz, 1840; Tyndal, 1859; Croll, 1864; Koppen, 1873; Czerney, 1881; Arrhenius, 1896) explained the climatic changes on the basis of tempera- ture and the ensuing glacial retreat. This disturbing observation led many prominent scientists (de Saussure, Bunsen, Pettenkoffer, Kroch1 and Warburg1) to send air balloons equipped with special devices to trap air from the lower atmosphere in order to measure CO2 concentrations. Ninety thousand (90,000) measurements were carried out at 138 locations in 4 continents between 1810 and 1961. th The data indicated that atmospheric CO2 concentrations, during the 19 century varied between 290 ppm and 430 ppm (with an average of 322 ppm for the pre-industrial period). For the 20th century, the average concentration is 338 ppm when combined with comparable CO2 measurements carried out by Mauna Loa Observatory, Hawaii, USA, (1958- 2000). Measurement precision is +/- 3%. Based on thermometric measurements, the mean average temperature in- crease from 1850 to the present is 0.75oC (0.44oC/100 years) with the following fluctuations. From 1850 to 1940 the temperature increased by +0.6oC; while from 1941 to 1975 temperature dropped by -0.2oC. From 1976 to 1998, the tem- perature rose by +0.35oC. From 1999 to 2006 temperature increase was nil. Fi- nally, since 2007 the Mean Annual Temperature of earth’s surface has substan- tially decreased.
    [Show full text]
  • Timeline of Natural History
    Timeline of natural history Main articles: History of the Earth and Geological his- chondrules,[1] are a key signature of a supernova ex- tory of Earth plosion. See also: Geologic time scale and Timeline of evolution- ary history of life • 4,567±3 Ma: Rapid collapse of hydrogen molecular For earlier events, see Timeline of the formation of the cloud, forming a third-generation Population I star, Universe. the Sun, in a region of the Galactic Habitable Zone This timeline of natural history summarizes signifi- (GHZ), about 25,000 light years from the center of the Milky Way Galaxy.[2] • 4,566±2 Ma: A protoplanetary disc (from which Earth eventually forms) emerges around the young Sun, which is in its T Tauri stage. • 4,560–4,550 Ma: Proto-Earth forms at the outer (cooler) edge of the habitable zone of the Solar Sys- tem. At this stage the solar constant of the Sun was only about 73% of its current value, but liquid wa- ter may have existed on the surface of the Proto- Earth, probably due to the greenhouse warming of high levels of methane and carbon dioxide present in the atmosphere. Early bombardment phase begins: because the solar neighbourhood is rife with large planetoids and debris, Earth experiences a number of giant impacts that help to increase its overall size. Visual representation of the history of life on Earth as a spiral 2 Hadean Eon cant geological and biological events from the formation of the Earth to the rise of modern humans. Times are listed in millions of years, or megaanni (Ma).
    [Show full text]
  • A Negative Fold Test on the Lorrain Formation of The
    Earth and Planetary Science Letters 232 (2005) 315–332 www.elsevier.com/locate/epsl A negative fold test on the Lorrain Formation of the Huronian Supergroup: Uncertainty on the paleolatitude of the Paleoproterozoic Gowganda glaciation and implications for the great oxygenation event Isaac A. Hilburna, Joseph L. Kirschvinka,*, Eiichi Tajikab, Ryuji Tadab, Yozo Hamanob, Shinji Yamamotob aDivision of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California 91125, USA bDepartment of Earth and Planetary Science, University of Tokyo, 7-3-1 Hongo, Tokyo 113-0033, Japan Received 18 December 2003; received in revised form 4 September 2004; accepted 27 November 2004 Available online 13 March 2005 Editor: V. Courtillot Abstract Previous paleomagnetic studies of the glaciogenic Gowganda and Lorrain formations have identified several low-inclination magnetic components of high thermal stability, which suggest low-latitude glaciation during deposition of the Huronian Supergroup, Canada. While extraordinary claims demand extraordinary proof, prior authors have been unable to support their interpretations of these components conclusively with any of the classic field stability tests (e.g., conglomerate, fold, and baked contact) capable of demonstrating that the magnetization was acquired at or soon enough after the time of deposition to be used to constrain the paleolatitude of the Gowganda or Lorrain formations. We report here the results of a fold test from the bpurple siltstoneQ member of the Lorrain Formation near the town of Desbarats, Ontario, which indicate that none of the reported components dates to the time of deposition. Hence, the paleolatitude of the Gowganda glaciation is uncertain. Comparison of the lithostratigraphic, paleomagnetic, and radiometric constraints on the Huronian sequence and the Transvaal Supergroup of Southern Africa implies that the one verified low-latitude Paleoproterozoic glacial event (the Makganyene glaciation, Transvaal Supergroup, South Africa) is younger than the three glacial units of Canada.
    [Show full text]
  • The Huronian Glaciation
    1 Earth’s earliest global glaciation? Geochronology and carbonate geochemistry of the 2 Polisarka Sedimentary Formation, Kola Peninsula, Russia 3 4 A.T. Brasier1*, A.P. Martin2+, V.A. Melezhik3,4, A.R. Prave5, D.J. Condon2, A.E. Fallick6 and FAR- 5 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. 16 G75 0QF 17 18 *corresponding author ([email protected]) 19 + present address: GNS Science, Private Bag 1930, Dunedin, New Zealand 20 # present address: Department of Geology and Petroleum Geology, Meston Building, University of 21 Aberdeen, Scotland, UK. AB24 3UE. 22 23 Research highlights: 24 ICDP FAR-DEEP Hole 3A targeted Palaeoproterozoic diamictites of the Polisarka Sedimentary 25 Formation of Russian Fennoscandia ► Zircon U-Pb dating of a tuff above the diamictites yielded a 26 minimum age of 2434 Ma for the diamictites ► This new U-Pb age constrains the onset of the 1 27 Palaeoproterozoic glaciation in Fennoscandia to between ca. 2430 and ca. 2440 Ma suggesting it 28 was one of the earliest Palaeoproterozoic glaciations ► carbonate δ13C analyses of carbonate rocks 29 below the diamictites revealed two excursions to ca.
    [Show full text]
  • High Country Conservation Advocates the Wilderness Society Center
    High Country Conservation Advocates ● The Wilderness Society ● Center for Biological Diversity ● Rocky Smith ● EcoFlight ● Great Old Broads for Wilderness ● Rocky Mountain Wild ● Colorado Native Plant Society ● Rocky Mountain Recreation Initiative ● Wild Connections ● Quiet Use Coalition ● Central Colorado Wilderness Coalition ● San Luis Valley Ecosystem Council November 18, 2019 Brian Stevens Team Leader BLM Gunnison Field Office 210 West Spencer Ave., Suite A Gunnison, CO 81230 Via email to [email protected] Re: North Powderhorn Fuels Project Dear Mr. Stevens: The following are the comments of High Country Conservation Advocates (HCCA), The Wilderness Society, Center for Biological Diversity, Rocky Smith, EcoFlight, Great Old Broads for Wilderness, Rocky Mountain Wild, Colorado Native Plant Society, Rocky Mountain Recreation Initiative, Wild Connections, Quiet Use Coalition, Central Colorado Wilderness Coalition, Center for Biological Diversity, and San Luis Valley Ecosystem Council on the proposed North Powderhorn Fuels Project, as described in the Scoping Letter (SL) of October 18, 2019 and the Draft Proposed Action and Alternatives (DPAA). HCCA is located in Crested Butte, Colorado and has over 900 members. HCCA was founded in 1977 to protect the health and natural beauty of the land, rivers, and wildlife in and around Gunnison County now and for future generations. Thank you for the opportunity to comment on this proposal. We may be able to support Alternative C should the agency provide more information clearly indicating that treatments outside of the wilderness and WSAs could be justified and, with mitigation, be acceptable.1 We could also support an alternative that allows non-motorized prescribed burning in ponderosa stands within the Powderhorn Wilderness and Wilderness Study Areas, if such treatments would result in treated areas resembling what would exist if natural fire disturbances had been allowed to occur.
    [Show full text]