Geodynamic and Metabolic Cycles in the Hadean
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The Geologic Time Scale Is the Eon
Exploring Geologic Time Poster Illustrated Teacher's Guide #35-1145 Paper #35-1146 Laminated Background Geologic Time Scale Basics The history of the Earth covers a vast expanse of time, so scientists divide it into smaller sections that are associ- ated with particular events that have occurred in the past.The approximate time range of each time span is shown on the poster.The largest time span of the geologic time scale is the eon. It is an indefinitely long period of time that contains at least two eras. Geologic time is divided into two eons.The more ancient eon is called the Precambrian, and the more recent is the Phanerozoic. Each eon is subdivided into smaller spans called eras.The Precambrian eon is divided from most ancient into the Hadean era, Archean era, and Proterozoic era. See Figure 1. Precambrian Eon Proterozoic Era 2500 - 550 million years ago Archaean Era 3800 - 2500 million years ago Hadean Era 4600 - 3800 million years ago Figure 1. Eras of the Precambrian Eon Single-celled and simple multicelled organisms first developed during the Precambrian eon. There are many fos- sils from this time because the sea-dwelling creatures were trapped in sediments and preserved. The Phanerozoic eon is subdivided into three eras – the Paleozoic era, Mesozoic era, and Cenozoic era. An era is often divided into several smaller time spans called periods. For example, the Paleozoic era is divided into the Cambrian, Ordovician, Silurian, Devonian, Carboniferous,and Permian periods. Paleozoic Era Permian Period 300 - 250 million years ago Carboniferous Period 350 - 300 million years ago Devonian Period 400 - 350 million years ago Silurian Period 450 - 400 million years ago Ordovician Period 500 - 450 million years ago Cambrian Period 550 - 500 million years ago Figure 2. -
The Reaction Center of Green Sulfur Bacteria1
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Elsevier - Publisher Connector Biochimica et Biophysica Acta 1507 (2001) 260^277 www.bba-direct.com Review The reaction center of green sulfur bacteria1 G. Hauska a;*, T. Schoedl a, Herve¨ Remigy b, G. Tsiotis c a Lehrstuhl fu«r Zellbiologie und P£anzenphysiologie, Fakulta«tfu«r Biologie und Vorklinische Medizin, Universita«t Regensburg, 93040 Regenburg, Germany b Biozentrum, M.E. Mu«ller Institute of Microscopic Structural Biology, University of Basel, CH-4056 Basel, Switzerland c Division of Biochemistry, Department of Chemistry, University of Crete, 71409 Heraklion, Greece Received 9 April 2001; received in revised form 13 June 2001; accepted 5 July 2001 Abstract The composition of the P840-reaction center complex (RC), energy and electron transfer within the RC, as well as its topographical organization and interaction with other components in the membrane of green sulfur bacteria are presented, and compared to the FeS-type reaction centers of Photosystem I and of Heliobacteria. The core of the RC is homodimeric, since pscA is the only gene found in the genome of Chlorobium tepidum which resembles the genes psaA and -B for the heterodimeric core of Photosystem I. Functionally intact RC can be isolated from several species of green sulfur bacteria. It is generally composed of five subunits, PscA^D plus the BChl a-protein FMO. Functional cores, with PscA and PscB only, can be isolated from Prostecochloris aestuarii. The PscA-dimer binds P840, a special pair of BChl a-molecules, the primary electron acceptor A0, which is a Chl a-derivative and FeS-center FX. -
Convective Isolation of Hadean Mantle Reservoirs Through Archean Time
Convective isolation of Hadean mantle reservoirs through Archean time Jonas Tuscha,1, Carsten Münkera, Eric Hasenstaba, Mike Jansena, Chris S. Mariena, Florian Kurzweila, Martin J. Van Kranendonkb,c, Hugh Smithiesd, Wolfgang Maiere, and Dieter Garbe-Schönbergf aInstitut für Geologie und Mineralogie, Universität zu Köln, 50674 Köln, Germany; bSchool of Biological, Earth and Environmental Sciences, The University of New South Wales, Kensington, NSW 2052, Australia; cAustralian Center for Astrobiology, The University of New South Wales, Kensington, NSW 2052, Australia; dDepartment of Mines, Industry Regulations and Safety, Geological Survey of Western Australia, East Perth, WA 6004, Australia; eSchool of Earth and Ocean Sciences, Cardiff University, Cardiff CF10 3AT, United Kingdom; and fInstitut für Geowissenschaften, Universität zu Kiel, 24118 Kiel, Germany Edited by Richard W. Carlson, Carnegie Institution for Science, Washington, DC, and approved November 18, 2020 (received for review June 19, 2020) Although Earth has a convecting mantle, ancient mantle reservoirs anomalies in Eoarchean rocks was interpreted as evidence that that formed within the first 100 Ma of Earth’s history (Hadean these rocks lacked a late veneer component (5). Conversely, the Eon) appear to have been preserved through geologic time. Evi- presence of some late accreted material is required to explain the dence for this is based on small anomalies of isotopes such as elevated abundances of highly siderophile elements (HSEs) in 182W, 142Nd, and 129Xe that are decay products of short-lived nu- Earth’s modern silicate mantle (9). Notably, some Archean rocks clide systems. Studies of such short-lived isotopes have typically with apparent pre-late veneer like 182W isotope excesses were focused on geological units with a limited age range and therefore shown to display HSE concentrations that are indistinguishable only provide snapshots of regional mantle heterogeneities. -
Geologic Time Lesson Guide Lesson Guide | Description
Geologic Time Lesson Guide Lesson Guide | Description Instructor: Dr. Michael T. Lewchuk Grade Level: 6 - 12 Subject: Earth & Physical Science Students will investigate the subdivisions of the Geologic Time Scale. Wonder How: Have you ever wondered how scientists and geologists know how old something is? Goal: Students will gather data and use ratios that will help them create a scale model of Geological time using simple materials found at home. Lesson Guide | Lesson Guide Agenda Lesson Guide Agenda: v Vocabulary v Materials List v Geologic Time Scale v Activity Instructions v Challenge! v Additional Resources v Oklahoma Academic Standards Lesson Guide | Vocabulary Eon – An Eon is the fundamental division of time in Geology. The Earth’s 4.6-billion- year history is divided into four Eons: Hadean, Archean, Proterozoic and Phanerozoic. Precambrian Supereon – This is the combination of the Hadean, Archean and Proterozoic Eons. It is subdivided based on the physical properties of the Earth’s surface and atmosphere. Hadean Eon – The Hadean is the oldest Eon. It is generally described as the time when the Earth was so hot that it was all, or mostly all, molten liquid. Archean Eon – The Archean Eon is generally described as the time when solid rock existed on the surface of the Earth, but little or no free oxygen existed in the atmosphere. Proterozoic Eon – The Proterozoic is generally considered the Eon when free oxygen began to appear in the atmosphere. Microscopic life developed during the Proterozoic. Lesson Guide | Vocabulary Phanerozoic Eon – The Phanerozoic Eon is the most recent Eon in geologic history. -
Horizontal Operon Transfer, Plasmids, and the Evolution of Photosynthesis in Rhodobacteraceae
The ISME Journal (2018) 12:1994–2010 https://doi.org/10.1038/s41396-018-0150-9 ARTICLE Horizontal operon transfer, plasmids, and the evolution of photosynthesis in Rhodobacteraceae 1 2 3 4 1 Henner Brinkmann ● Markus Göker ● Michal Koblížek ● Irene Wagner-Döbler ● Jörn Petersen Received: 30 January 2018 / Revised: 23 April 2018 / Accepted: 26 April 2018 / Published online: 24 May 2018 © The Author(s) 2018. This article is published with open access Abstract The capacity for anoxygenic photosynthesis is scattered throughout the phylogeny of the Proteobacteria. Their photosynthesis genes are typically located in a so-called photosynthesis gene cluster (PGC). It is unclear (i) whether phototrophy is an ancestral trait that was frequently lost or (ii) whether it was acquired later by horizontal gene transfer. We investigated the evolution of phototrophy in 105 genome-sequenced Rhodobacteraceae and provide the first unequivocal evidence for the horizontal transfer of the PGC. The 33 concatenated core genes of the PGC formed a robust phylogenetic tree and the comparison with single-gene trees demonstrated the dominance of joint evolution. The PGC tree is, however, largely incongruent with the species tree and at least seven transfers of the PGC are required to reconcile both phylogenies. 1234567890();,: 1234567890();,: The origin of a derived branch containing the PGC of the model organism Rhodobacter capsulatus correlates with a diagnostic gene replacement of pufC by pufX. The PGC is located on plasmids in six of the analyzed genomes and its DnaA- like replication module was discovered at a conserved central position of the PGC. A scenario of plasmid-borne horizontal transfer of the PGC and its reintegration into the chromosome could explain the current distribution of phototrophy in Rhodobacteraceae. -
Carbon Flow of Heliobacteria Is Related More
Supplemental Material can be found at: http://www.jbc.org/content/suppl/2010/08/31/M110.163303.DC1.html THE JOURNAL OF BIOLOGICAL CHEMISTRY VOL. 285, NO. 45, pp. 35104–35112, November 5, 2010 © 2010 by The American Society for Biochemistry and Molecular Biology, Inc. Printed in the U.S.A. Carbon Flow of Heliobacteria Is Related More to Clostridia than to the Green Sulfur Bacteria*□S Received for publication, July 14, 2010, and in revised form, August 30, 2010 Published, JBC Papers in Press, August 31, 2010, DOI 10.1074/jbc.M110.163303 Kuo-Hsiang Tang‡§1,2, Xueyang Feng¶1, Wei-Qin Zhuangʈ, Lisa Alvarez-Cohenʈ, Robert E. Blankenship‡§, and Yinjie J. Tang¶3 From the Departments of ‡Biology, §Chemistry, and ¶Energy, Environment, and Chemical Engineering, Washington University, St. Louis, Missouri 63130 and the ʈDepartment of Civil and Environmental Engineering, University of California, Berkeley, California 94720 The recently discovered heliobacteria are the only Gram-pos- cultured heliobacteria (2), Heliobacterium modesticaldum is itive photosynthetic bacteria that have been cultured. One of the the only one that can grow at temperatures of Ͼ50 °C. Madigan unique features of heliobacteria is that they have properties of and co-workers (1, 3) reported that pyruvate, lactate, acetate both the photosynthetic green sulfur bacteria (containing the (ϩHCOϪ), or yeast extract can support the phototrophic 3 Downloaded from type I reaction center) and Clostridia (forming heat-resistant growth of H. modesticaldum, and our recent studies demon- endospores). Most of the previous studies of heliobacteria, strated that D-sugars can also support the growth of H. -
The World Turns Over: Hadean–Archean Crust–Mantle Evolution
Lithos 189 (2014) 2–15 Contents lists available at ScienceDirect Lithos journal homepage: www.elsevier.com/locate/lithos Review paper The world turns over: Hadean–Archean crust–mantle evolution W.L. Griffin a,⁎, E.A. Belousova a,C.O'Neilla, Suzanne Y. O'Reilly a,V.Malkovetsa,b,N.J.Pearsona, S. Spetsius a,c,S.A.Wilded a ARC Centre of Excellence for Core to Crust Fluid Systems (CCFS) and GEMOC, Dept. Earth and Planetary Sciences, Macquarie University, NSW 2109, Australia b VS Sobolev Institute of Geology and Mineralogy, Siberian Branch, Russian Academy of Sciences, Novosibirsk 630090, Russia c Scientific Investigation Geology Enterprise, ALROSA Co Ltd, Mirny, Russia d ARC Centre of Excellence for Core to Crust Fluid Systems, Dept of Applied Geology, Curtin University, G.P.O. Box U1987, Perth 6845, WA, Australia article info abstract Article history: We integrate an updated worldwide compilation of U/Pb, Hf-isotope and trace-element data on zircon, and Re–Os Received 13 April 2013 model ages on sulfides and alloys in mantle-derived rocks and xenocrysts, to examine patterns of crustal evolution Accepted 19 August 2013 and crust–mantle interaction from 4.5 Ga to 2.4 Ga ago. The data suggest that during the period from 4.5 Ga to ca Available online 3 September 2013 3.4 Ga, Earth's crust was essentially stagnant and dominantly maficincomposition.Zirconcrystallizedmainly from intermediate melts, probably generated both by magmatic differentiation and by impact melting. This quies- Keywords: – Archean cent state was broken by pulses of juvenile magmatic activity at ca 4.2 Ga, 3.8 Ga and 3.3 3.4 Ga, which may Hadean represent mantle overturns or plume episodes. -
Tracking Molecular Evolution of Photosynthesis by Characterization
Proc. Natl. Acad. Sci. USA Vol. 95, pp. 14851–14856, December 1998 Evolution Tracking molecular evolution of photosynthesis by characterization of a major photosynthesis gene cluster from Heliobacillus mobilis (bacteriochlorophyll biosynthesisycytochrome bc complexyphylogenetic analysisyphotosystem origin) JIN XIONG*, KAZUHITO INOUE†, AND CARL E. BAUER*‡ *Department of Biology, Indiana University, Bloomington, IN 47405; and †Department of Biological Sciences, Kanagawa University, Hiratsuka, Kanagawa 259-1293, Japan Communicated by Norman R. Pace, University of California, Berkeley, CA, October 13, 1998 (received for review July 21, 1998) ABSTRACT A DNA sequence has been obtained for a With the aim of providing more substantive information on 35.6-kb genomic segment from Heliobacillus mobilis that con- the evolution of photosynthesis, we have undertaken an ex- tains a major cluster of photosynthesis genes. A total of 30 tensive characterization of photosynthesis genes from Helioba- ORFs were identified, 20 of which encode enzymes for bacte- cillus mobilis. A gene cluster was found to encode enzymes for riochlorophyll and carotenoid biosynthesis, reaction-center bacteriochlorophyll and carotenoid biosynthesis, as well as the (RC) apoprotein, and cytochromes for cyclic electron trans- RC core polypeptide and cytochromes involved in photosyn- port. Donor side electron-transfer components to the RC thetic electron transfer. Phylogenetic studies based on this new include a putative RC-associated cytochrome c553 and a sequence information provide important clues for the unique unique four-large-subunit cytochrome bc complex consisting evolutionary position of H. mobilis in the course of develop- of Rieske Fe-S protein (encoded by petC), cytochrome b6 ment of photosynthesis. (petB), subunit IV (petD), and a diheme cytochrome c (petX). -
Habitability of the Early Earth: Liquid Water Under a Faint Young Sun Facilitated by Strong Tidal Heating Due to a Nearby Moon
Habitability of the early Earth: Liquid water under a faint young Sun facilitated by strong tidal heating due to a nearby Moon Ren´eHeller · Jan-Peter Duda · Max Winkler · Joachim Reitner · Laurent Gizon Draft July 9, 2020 Abstract Geological evidence suggests liquid water near the Earths surface as early as 4.4 gigayears ago when the faint young Sun only radiated about 70 % of its modern power output. At this point, the Earth should have been a global snow- ball. An extreme atmospheric greenhouse effect, an initially more massive Sun, release of heat acquired during the accretion process of protoplanetary material, and radioactivity of the early Earth material have been proposed as alternative reservoirs or traps for heat. For now, the faint-young-sun paradox persists as one of the most important unsolved problems in our understanding of the origin of life on Earth. Here we use astrophysical models to explore the possibility that the new-born Moon, which formed about 69 million years (Myr) after the ignition of the Sun, generated extreme tidal friction { and therefore heat { in the Hadean R. Heller Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077 G¨ottingen, Germany E-mail: [email protected] J.-P. Duda G¨ottingenCentre of Geosciences, Georg-August-University G¨ottingen, 37077 G¨ottingen,Ger- many E-mail: [email protected] M. Winkler Max Planck Institute for Extraterrestrial Physics, Giessenbachstraße 1, 85748 Garching, Ger- many E-mail: [email protected] J. Reitner G¨ottingenCentre of Geosciences, Georg-August-University G¨ottingen, 37077 G¨ottingen,Ger- many G¨ottingenAcademy of Sciences and Humanities, 37073 G¨ottingen,Germany E-mail: [email protected] L. -
Geologic Time
Alles Introductory Biology Lectures An Introduction to Science and Biology for Non-Majors Instructor David L. Alles Western Washington University ----------------------- Part Three: The Integration of Biological Knowledge The Origin of our Solar System and Geologic Time ----------------------- “Out of the cradle onto dry land here it is standing: atoms with consciousness; matter with curiosity.” Richard Feynman Introduction “Science analyzes experience, yes, but the analysis does not yet make a picture of the world. The analysis provides only the materials for the picture. The purpose of science, and of all rational thought, is to make a more ample and more coherent picture of the world, in which each experience holds together better and is more of a piece. This is a task of synthesis, not of analysis.”—Bronowski, 1977 • Because life on Earth is an effectively closed historical system, we must understand that biology is an historical science. One result of this is that a chronological narrative of the history of life provides for the integration of all biological knowledge. • The late Preston Cloud, a biogeologist, was one of the first scientists to fully understand this. His 1978 book, Cosmos, Earth, and Man: A Short History of the Universe, is one of the first and finest presentations of “a more ample and more coherent picture of the world.” • The second half of this course follows in Preston Cloud’s footsteps in presenting the story of the Earth and life through time. From Preston Cloud's 1978 book Cosmos, Earth, and Man On the Origin of our Solar System and the Age of the Earth How did the Sun and the planets form, and what lines of scientific evidence are used to establish their age, including the Earth’s? 1. -
Heterogeneous Hadean Crust with Ambient Mantle Affinity Recorded in Detrital Zircons of the Green Sandstone Bed, South Africa
Heterogeneous Hadean crust with ambient mantle affinity recorded in detrital zircons of the Green Sandstone Bed, South Africa Nadja Drabona,1,2, Benjamin L. Byerlyb,3, Gary R. Byerlyc, Joseph L. Woodend,4, C. Brenhin Kellere, and Donald R. Lowea aDepartment of Geological Sciences, Stanford University, Stanford, CA 94305; bDepartment of Earth Sciences, University of California, Santa Barbara, CA 93106; cDepartment of Geology and Geophysics, Louisiana State University, Baton Rouge, LA 70803; dPrivate address, Marietta, GA 30064; and eDepartment of Earth Sciences, Dartmouth College, Hanover, NH 03755 Edited by Albrecht W. Hofmann, Max Planck Institute for Chemistry, Mainz, Germany, and approved January 4, 2021 (received for review March 10, 2020) The nature of Earth’s earliest crust and the processes by which it While the crustal rocks in which Hadean zircon formed have formed remain major issues in Precambrian geology. Due to the been lost, the trace and rare earth element (REE) geochemistry of absence of a rock record older than ∼4.02 Ga, the only direct re- these zircons can be used to characterize their parental magma cord of the Hadean is from rare detrital zircon and that largely compositions. Zircon crystallizes as a ubiquitous accessory mineral from a single area: the Jack Hills and Mount Narryer region of in silica-rich, differentiated magmas formed in a number of crustal Western Australia. Here, we report on the geochemistry of environments. Since zircon compositions are influenced by varia- Hadean detrital zircons as old as 4.15 Ga from the newly discov- tions in melt composition, coexisting mineral assemblage, and trace ered Green Sandstone Bed in the Barberton greenstone belt, element partitioning as a function of magmatic processes, temper- South Africa. -
Early Earth - W
EARTH SYSTEM: HISTORY AND NATURAL VARIABILITY - Vol. I - Early Earth - W. Bleeker EARLY EARTH W. Bleeker Continental Geoscience Division, Geological Survey of Canada, Ottawa, Canada Keywords: early Earth, accretion, planetesimals, giant impacts, Moon, Hadean, Archaean, Proterozoic, late heavy bombardment, origin of life, mantle convection, mantle plumes, plate tectonics, geological time-scale, age dating Contents 1. Introduction 2. Early Earth: Concepts 2.1. Divisions of Geological Time 2.2. Definition of the“Early Earth” 2.3. Age Dating 3. Early Earth Evolution 3.1. Origin of the Universe and Formation of the Elements 3.2. Formation of the Solar System 3.3. Accretion, Differentiation, and Formation of the Earth–Moon System 3.4. Oldest Rocks and Minerals 3.5. The Close of the Hadean: the Late Heavy Bombardment 3.6. Earth’s Oldest Supracrustal Rocks and the Origin of Life 3.7. Settling into a Steady State: the Archean 4. Conclusions Acknowledgements Glossary Bibliography Biographical Sketch Summary The “ early Earth” encompasses approximately the first gigayear (Ga, 109 y) in the evolution of our planet, from its initial formation in the young Solar System at about 4.55 Ga to sometimeUNESCO in the Archean eon at about 3.5– Ga. EOLSS This chapter describes the evolution of the early Earth and reviews the evidence that pertains to this interval from both planetary and geological science perspectives. Such a description, even in general terms, can only be given with some background knowledge of the origin and calibration of the geological timescale, modernSAMPLE age-dating techniques, the foCHAPTERSrmation of solar systems, and the accretion of terrestrial planets.