Carbon from Crust to Core

Total Page:16

File Type:pdf, Size:1020Kb

Carbon from Crust to Core Poster EGU2017 – 10193 GPMV2.3 Simon Mitton St Edmund’s College, CARBON FROM CRUST TO CORE University of Cambridge, Cambridge CB3 0BN, UK A Brief History of Deep Carbon Science European Geosciences Union General Assembly [email protected] 23–28 April 2017, Vienna, Austria Agricola 1546 Gilbert 1600 Hooke 1665 Hutton 1788 Lyell 1830 Sedgwick 1839 Wegner 1912 Holmes 1911 ZoBell 1930s Goldschmidt 1930s Bridgman 1946 Ringwood 1975 Mineralogy Geomagnestism Microscope Modern Geology Geological Principles Devonian System Continental Drift Geochronology Deep Life: biofilms Geochemistry High Pressure Physics Mantle Petrology Before 2009 … discovering Deep Earth Finding the Pioneers Finding solutions to deep puzzles . After 2009 Recounting five centuries of progress in the discovery of the I am on the trail of high impact authors and their papers, tell me your nominations and suggestions The foundation of the Deep Carbon Observatory in 2009 revolutionised geophysical, geochemical and biological properties of the Earth, deep Earth research and has given us a decade of significant deep Carbon From Crust to Core will document the vital discoveries that carbon discoveries. The history synthesis project Carbon From Crust to revealed the interior dynamics of our planet. Engaging stories of Whom do you want to Core recounts a remarkable story of how a community of scientists, from biologists to physicists, geologists to chemists, broke traditional remarkable scientists who first explored Earth’s deep interior will be see in the index? revealed. boundaries and built a new integrative field: deep carbon science. Nominate a colleague! Deep Life Reservoirs & Fluxes Deep Life exerts a vital influence on By identifying the deep reservoirs and their Earth's elemental fluxes and reservoirs. fluxes we can unlock many of the secrets This was recognised by pioneers such as of the deep carbon cycle. Research from Claude ZoBell the ‘Father of Marine What’s your deep authors such as McKenzie, Barnes and Microbiology’ credited with discovering Giggenbach has allowed for links between biofilms. The Deep Carbon Observatory carbon story? carbon emissions and volcanic and continues to assess the abundance and Could you be my next tectonic activity to be made, as well as diversity of the subsurface realm, The deep carbon pioneer? giving insights into important cycling Census of Deep Life developed through processes such as mantle convection. DCO will us find the environmental limits to Deep Carbon Observatory aims to deep life. The Great Oxidation Event had a produce quantitative models of global huge effect on the history of life on Earth. How do these deep carbon cycling at the planetary, tectonic Photosynthesis by cyanobacteria helped to lifeforms survive? What and reservoir scales, as well as assessing produce the organic carbon that became impact do they have on the evolution of the cycle over time. Deep fossil fuels. the carbon cycle? Carbon Observatory early career Geodynamics of Deep Carbon How is carbon recycled researchers recently conducted the Trail Deep carbon science explores how much carbon is in Earth, how it moves, what form it takes, where between the atmosphere by Fire expedition to make a snapshot of and how it originated, and how it has changed over billions of years. and Earth’s crust, mantle, volatile degassing along an entire Extreme Physics & Chemistry and core? subduction zone. Deep carbon is often stored at extremely high temperatures and pressures, such as in the mantle and core of Earth and other Deep Energy planets. Bridgman pioneered the Carbon-based fuels supply most of society’s application of high pressure physics to energy, whilst atmospheric carbon dioxide is mineralogy, paving the way for the primary cause of climate change. We must investigations into the physical and understand more about these deep sources of chemical behaviour of different elements energy if we are to continue to exploit them. and compounds in extreme conditions. Gold daringly proposed the deep gas Using both theoretical and experimental hypothesis, suggesting fossil fuel formation via approaches the Deep Carbon Observatory abiogenic processes and tectonic driven has been developing databases and migration. The Deep Carbon Observatory uses simulations of deep carbon material observation and experimentation to quantify the properties and seeking new carbon environmental conditions and processes that bearing minerals. Earth in Five Reactions control the origins, forms, quantities and Ancient inclusions of What are the physical and is a DCO project that will identify the five movements of carbon, abiogenic hydrocarbons garnet in diamond from chemical properties of most important reactions that govern the and organic compounds in the deep earth over transformation of carbon in Earth. geologic time. Deep Carbon Observatory B o t s w a n a re v e a l t h e carbon in Earth’s interior? scientists are probing diamonds and their carbon cycle of early Earth. Acknowledgments: Fiona Iddon, Marie Edmonds, Craig Schiffries (advice), Deep Carbon Observatory (images). inclusions to quantify temporal changes in the ( p h o t o M . G r e s s / V U This history of science project for Deep Carbon Observatory will be published by Cambridge University Press in 2019 deep carbon cycle. Amsterdam) .
Recommended publications
  • Lipid Analysis of CO2-Rich Subsurface Aquifers Suggests an Autotrophy-Based Deep Biosphere with Lysolipids Enriched in CPR Bacteria
    The ISME Journal (2020) 14:1547–1560 https://doi.org/10.1038/s41396-020-0624-4 ARTICLE Lipid analysis of CO2-rich subsurface aquifers suggests an autotrophy-based deep biosphere with lysolipids enriched in CPR bacteria 1,2 3,4 1,3 3 3 Alexander J. Probst ● Felix J. Elling ● Cindy J. Castelle ● Qingzeng Zhu ● Marcus Elvert ● 5,6 6 1 7,9 7 Giovanni Birarda ● Hoi-Ying N. Holman ● Katherine R. Lane ● Bethany Ladd ● M. Cathryn Ryan ● 8 3 1 Tanja Woyke ● Kai-Uwe Hinrichs ● Jillian F. Banfield Received: 20 November 2018 / Revised: 5 February 2020 / Accepted: 25 February 2020 / Published online: 13 March 2020 © The Author(s) 2020. This article is published with open access Abstract Sediment-hosted CO2-rich aquifers deep below the Colorado Plateau (USA) contain a remarkable diversity of uncultivated microorganisms, including Candidate Phyla Radiation (CPR) bacteria that are putative symbionts unable to synthesize membrane lipids. The origin of organic carbon in these ecosystems is unknown and the source of CPR membrane lipids remains elusive. We collected cells from deep groundwater brought to the surface by eruptions of Crystal Geyser, sequenced 1234567890();,: 1234567890();,: the community, and analyzed the whole community lipidome over time. Characteristic stable carbon isotopic compositions of microbial lipids suggest that bacterial and archaeal CO2 fixation ongoing in the deep subsurface provides organic carbon for the complex communities that reside there. Coupled lipidomic-metagenomic analysis indicates that CPR bacteria lack complete lipid biosynthesis pathways but still possess regular lipid membranes. These lipids may therefore originate from other community members, which also adapt to high in situ pressure by increasing fatty acid unsaturation.
    [Show full text]
  • Carbonation and Decarbonation Reactions: Implications for Planetary Habitability K
    American Mineralogist, Volume 104, pages 1369–1380, 2019 Carbonation and decarbonation reactions: Implications for planetary habitability k E.M. STEWART1,*,†, JAY J. AGUE1, JOHN M. FERRY2, CRAIG M. SCHIFFRIES3, REN-BIAO TAO4, TERRY T. ISSON1,5, AND NOAH J. PLANAVSKY1 1Department of Geology & Geophysics, Yale University, P.O. Box 208109, New Haven, Connecticut 06520-8109, U.S.A. 2Department of Earth and Planetary Sciences, Johns Hopkins University, 3400 N. Charles Street, Baltimore, Maryland 21218, U.S.A. 3Geophysical Laboratory, Carnegie Institution for Science, 5251 Broad Branch Road NW, Washington, D.C. 20015, U.S.A. 4School of Earth and Space Sciences, MOE Key Laboratory of Orogenic Belt and Crustal Evolution, Peking University, Beijing 100871, China 5School of Science, University of Waikato, 101-121 Durham Street, Tauranga 3110, New Zealand ABSTRACT The geologic carbon cycle plays a fundamental role in controlling Earth’s climate and habitability. For billions of years, stabilizing feedbacks inherent in the cycle have maintained a surface environ- ment that could sustain life. Carbonation/decarbonation reactions are the primary mechanisms for transferring carbon between the solid Earth and the ocean–atmosphere system. These processes can be broadly represented by the reaction: CaSiO3 (wollastonite) + CO2 (gas) ↔ CaCO3 (calcite) + SiO2 (quartz). This class of reactions is therefore critical to Earth’s past and future habitability. Here, we summarize their signifcance as part of the Deep Carbon Obsevatory’s “Earth in Five Reactions” project. In the forward direction, carbonation reactions like the one above describe silicate weathering and carbonate formation on Earth’s surface. Recent work aims to resolve the balance between silicate weathering in terrestrial and marine settings both in the modern Earth system and through Earth’s history.
    [Show full text]
  • Earth Catastrophes and Their Impact on the Carbon Cycle
    Earth Catastrophes and their Impact on the Carbon Cycle Celina A. Suarez1, Marie Edmonds2, and Adrian P. Jones3 1811-5209/19/0015-0301$2.50 DOI: 10.2138/gselements.15.5.301 arbon is one of the most important elements on Earth. It is the basis search for catastrophic causes of of life, it is stored and mobilized throughout the Earth from core to perturbations in the carbon cycle ranges from the tipping points Ccrust and it is the basis of the energy sources that are vital to human reached during slow accretion civilization. This issue will focus on the origins of carbon on Earth, the roles of tectonic plates into megacon- played by large-scale catastrophic carbon perturbations in mass extinctions, tinents, to shifts in atmospheric or ocean circulation, to instanta- the movement and distribution of carbon in large igneous provinces, and neous megaenergy events deliv- the role carbon plays in icehouse–greenhouse climate transitions in deep ered by Earth’s inevitable orbital time. Present-day carbon fluxes on Earth are changing rapidly, and it is of space encounters with bolides, utmost importance that scientists understand Earth’s carbon cycle to secure to large-scale volcanism. These major events are often associated a sustainable future. with biological diversity crises and KEYWORDS: impacts, Earth’s origin, extinction, climate change, volcanism, mass extinctions. Deciphering the large igneous province complex and often faint signals of distant catastrophes requires a INTRODUCTION multidisciplinary effort and the most innovative analytical technology. Great strides have been made in quantifying the diverse world of carbon in Earth.
    [Show full text]
  • Deep Carbon Emissions from Volcanoes Michael R
    Reviews in Mineralogy & Geochemistry Vol. 75 pp. 323-354, 2013 11 Copyright © Mineralogical Society of America Deep Carbon Emissions from Volcanoes Michael R. Burton Istituto Nazionale di Geofisica e Vulcanologia Via della Faggiola, 32 56123 Pisa, Italy [email protected] Georgina M. Sawyer Laboratoire Magmas et Volcans, Université Blaise Pascal 5 rue Kessler, 63038 Clermont Ferrand, France and Istituto Nazionale di Geofisica e Vulcanologia Via della Faggiola, 32 56123 Pisa, Italy Domenico Granieri Istituto Nazionale di Geofisica e Vulcanologia Via della Faggiola, 32 56123 Pisa, Italy INTRODUCTION: VOLCANIC CO2 EMISSIONS IN THE GEOLOGICAL CARBON CYCLE Over long periods of time (~Ma), we may consider the oceans, atmosphere and biosphere as a single exospheric reservoir for CO2. The geological carbon cycle describes the inputs to this exosphere from mantle degassing, metamorphism of subducted carbonates and outputs from weathering of aluminosilicate rocks (Walker et al. 1981). A feedback mechanism relates the weathering rate with the amount of CO2 in the atmosphere via the greenhouse effect (e.g., Wang et al. 1976). An increase in atmospheric CO2 concentrations induces higher temperatures, leading to higher rates of weathering, which draw down atmospheric CO2 concentrations (Ber- ner 1991). Atmospheric CO2 concentrations are therefore stabilized over long timescales by this feedback mechanism (Zeebe and Caldeira 2008). This process may have played a role (Feulner et al. 2012) in stabilizing temperatures on Earth while solar radiation steadily increased due to stellar evolution (Bahcall et al. 2001). In this context the role of CO2 degassing from the Earth is clearly fundamental to the stability of the climate, and therefore to life on Earth.
    [Show full text]
  • Jesse H. Ausubel the Liberation of the Environment
    Jesse H. Ausubel The Liberation of the Environment Di Renzo Dialogues in Science The Dialogues: Science The books of this series result from extensive discussions with the author, who, stimulated by our questions, similar to those which a reader might wish to pose, develops clearly the themes of his professional career. ©2014 Di Renzo Editore Viale Manzoni 59 00185 Roma Tel. 06/77 20 90 20 Fax 06/70 47 40 67 E‐mail: [email protected] Internet: http://www.direnzo.it JESSE H. AUSUBEL La liberazione dell’ambiente Di Renzo Editore Table of Contents My Roots..................................................................................................................................1 My Childhood...........................................................................................................................4 University Years........................................................................................................................8 The US National Academy of Sciences and the First United Nations World Climate Conference..............................................................12 A Bridge over the Cold War: The International Institute for Applied Systems Analysis ........14 Global Warming and Climate Change............................................................. .......................17 The mid‐80s: A General Theory of Environmental Problems.................................................20 A Question of Efficiency.........................................................................................................22
    [Show full text]
  • Diamond Formation in the Deep Lower Mantle
    www.nature.com/scientificreports OPEN Diamond formation in the deep lower mantle: a high-pressure reaction of MgCO3 and SiO2 Received: 30 August 2016 Fumiya Maeda1, Eiji Ohtani1,2, Seiji Kamada1,3, Tatsuya Sakamaki1, Naohisa Hirao4 & Accepted: 07 December 2016 Yasuo Ohishi4 Published: 13 January 2017 Diamond is an evidence for carbon existing in the deep Earth. Some diamonds are considered to have originated at various depth ranges from the mantle transition zone to the lower mantle. These diamonds are expected to carry significant information about the deep Earth. Here, we determined the phase relations in the MgCO3-SiO2 system up to 152 GPa and 3,100 K using a double sided laser- heated diamond anvil cell combined with in situ synchrotron X-ray diffraction. MgCO3 transforms from magnesite to the high-pressure polymorph of MgCO3, phase II, above 80 GPa. A reaction between MgCO3 phase II and SiO2 (CaCl2-type SiO2 or seifertite) to form diamond and MgSiO3 (bridgmanite or post-perovsktite) was identified in the deep lower mantle conditions. These observations suggested that the reaction of the MgCO3 phase II with SiO2 causes formation of super-deep diamond in cold slabs descending into the deep lower mantle. Carbon is circulated around the surface and interior of the Earth with subducting slabs and volcanic eruptions; subduction carries carbon-bearing rocks to the Earth’s interior and volcanic eruption expels carbon-bearing gas, lavas and rocks from the interior of the Earth1. The flux of subducted carbon within oceanic plates is estimated to be more than 5 Tmol/yr, almost twice as large as the expelled-carbon flux, 2–3 Tmol/yr, through arc magmatism2.
    [Show full text]
  • Jie (Jackie) Li
    Jie (Jackie) Li Jie (Jackie) Li Department of Earth and Environmental Sciences, University of Michigan 1100 N. University Ave., Ann Arbor MI 48109 +1 734 6157317, [email protected] http:/www.earth.lsa.umich.edu/jackieli/ EDUCATION 1992 University of Science and Technology of China, B.S. Geochemistry 1997 Harvard University, M.A. Geophysics 1998 Harvard University. Ph.D. Earth and Planetary Sciences POSITIONS HELD University of Michigan 2016- Professor 2010-2016 Associate Professor University of Illinois 2009 Associate Professor 2003-2009 Assistant Professor Carnegie Institution for Science 2000-2003 Postdoctoral Associate, 1998-2000 Gilbert Postdoctoral Fellow 2018 Stanford University, Blaustein Visiting Adjunct Professor, 2013 University of Western Australia, Short-Stay Visitor, Institute of Advanced Studies, 2012 Tohoku University, Japan Global Center of Excellence Scholar, 2012 Columbia University, Tharp Fellow 1996-1997 Harvard University, Resident Tutor, Winthrop House AWARDS AND HONORS 2013 Kavli Fellow, National Academy of Sciences 2010 Fellow, Mineralogical Society of America 2009-2010 COMPRES (Consortium for Materials Properties Research) Distinguished Lecturer 2009 Helen Corley Petit Scholar, University of Illinois, College of Liberal Arts and Sciences 2009-2010 Center for Advanced Study Fellow, University of Illinois 2003-2008 Teachers Ranked as Excellent by Their Students, University of Illinois 1992 Presidential Guo Morou Prize, University of Science and Technology of China PROFESSIONAL SOCIETY MEMBERSHIP 2016- American Association
    [Show full text]
  • Nature and Extent of the Deep Biosphere Frederick S
    Reviews in Mineralogy & Geochemistry Vol. 75 pp. 547-574, 2013 17 Copyright © Mineralogical Society of America Nature and Extent of the Deep Biosphere Frederick S. Colwell College of Earth, Ocean, and Atmospheric Sciences Oregon State University Corvallis, Oregon 97331-5503, U.S.A. [email protected] Steven D’Hondt Graduate School of Oceanography University of Rhode Island Narragansett, Rhode Island 02882, U.S.A. [email protected] INTRODUCTION In the last three decades we have learned a great deal about microbes in subsurface envi- ronments. Once, these habitats were rarely examined, perhaps because so much of the life that we are concerned with exists at the surface and seems to pace its metabolic and evolutionary rhythms with the overt planetary, solar, and lunar cycles that dictate our own lives. And it cer- tainly remains easier to identify with living beings that are in our midst, most obviously strug- gling with us or against us for survival over time scales that are easiest to track using diurnal, monthly or annual periods. Yet, research efforts are drawn again and again to the subsurface to consider life there. No doubt this has been due to our parochial interests in the resources that exist there (the water, minerals, and energy) that our society continues to require and that in some cases are created or modified by microbes. However, we also continue to be intrigued by the scientific curiosities that might only be solved by going underground and examining life where it does and does not exist. But really, is life underground just a peculiarity of most life on the planet and only a re- cently discovered figment of life? Or is it actually a more prominent and fundamental, if unseen, theme for life on our planet? Our primary purpose in this chapter is to provide an incremental assembly of knowledge of subsurface life with the aim of moving us towards a more complete conceptual model of deep life on the planet.
    [Show full text]
  • Commodore of a Global DNA Census
    Commodore of a Global DNA Census Tue Apr 26 2011 Page: D1 / Science Times Byline: NICHOLAS WADE Column: SCIENTIST AT WORK JESSE H. AUSUBEL Length: 1,704 words Ad Value: $940,680 Circulation: 1,126,190 "Dinochelus ausubeli" was the name conferred earlier this year on a strange deep sea monster, a lobster discovered off the Philippine coast whose right claw is elongated into a fearsome pincer. The new species was named not after its discoverer, but in honor of the person under whose auspices a fleet of 540 ships from 80 nations has found the lobster and 6,000 other new marine species in the last 10 years. He is Jesse H. Ausubel, a Rockefeller University environmental researcher who is also vice president of the Alfred P. Sloan Foundation of New York. With his academic hat, Mr. Ausubel, 59, writes and thinks about the environment. Under his foundation hat, he has so far started four major international programs to survey the planet and catalog its biological diversity. He began the Census of Marine Life in 2000 after discussions with Fred Grassle, a deep-sea biologist at Rutgers University. The project began as a census of the fishes, but as more biologists got involved it expanded to include invertebrates, a wide range of habitats from shoreline to the ocean abysses, and a system for monitoring the distribution of ocean species. The Sloan Foundation invested $75 million in the census, but all the ship time was paid for by the participating institutions. By the time the first census finished, in 2010, total investment in the project had reached $650 million.
    [Show full text]
  • Earth's Deep Carbon Cycle
    Earth’s Deep Carbon Cycle with an emphasis on subduction zones and continental lithospheric mantles Rajdeep Dasgupta CIDER 2013 July 16, 2013 http://earthobservatory.nasa.gov/Library/CarbonCycle ~1/3rd Depleted mantle 50‐200 ppm CO2 Enriched mantle up to 1000 ppm CO2 ~2/3rd Dasgupta and Hirschmann (2010) Deep Carbon – Estimating Flux and Concentration • Direct measurement of CO2 in mantle derived melts/ glasses (MORBs, OIBs, Arc lavas and melt inclusions) (e.g., Dixon et al., 1997; Bureau et al., 1998) • Direct measurement of CO2 in mantle-derived fluids (trapped gas bubbles in basalts, hydrothermal vent fluids, plumes) and gases (e.g., Aubaud et al., 2005) ● Measurement of CO2/Incompatible species ratio in glasses, fluids, gases and independent estimate of mantle He or Nb etc. 3 CO2/ He (e.g., Trull et al., 1993; Marty and Tolstikhin, 1998; Shaw et al., 2003; Resing et al., 2004) CO2/Ar (e.g., Tingle, 1998; Cartigny et al., 2001) CO2/Nb (e.g., Saal et al., 2002; Cartigny et al., 2008) CO2/Cl (e.g., Saal et al., 2002) Mantle derived Carbonatites and Kimberlites on Continents Belton (2004) Oldonyo Lengai, Tanzania - Active Carbonatite Volcano Kjarsgaard (2005) Primary magma –38‐45 wt.% CO2 Primary magma –25‐15 wt.% CO2 Subduction Zones loci of continent formation Does the present‐day subduction processes lead to efficient release of CO2 to exogenic system? Did the CO2 fluxes (in‐ and out‐) in subduction zones remain the same throughout the Earth’s history? sediment basalt peridotite Approaches ● Constraints on slab input and arc ouput
    [Show full text]
  • Carbonation and the Urey Reactionk
    American Mineralogist, Volume 104, pages 1365–1368, 2019 Carbonation and the Urey reactionk LOUISE H. KELLOGG1, HARSHA LOKAVARAPU2, AND DONALD L. TURCOTTE2,*,† 1Department of Earth and Planetary Science, University of California, Davis, 1 Shields Avenue, Davis, California 95616, U.S.A. Orcid 0000-0001-5874-0472 2Department of Earth and Planetary Science, University of California, Davis, 1 Shields Avenue, Davis, California 95616, U.S.A. ABSTRACT There are three major reservoirs for carbon in the Earth at the present time, the core, the mantle, and the continental crust. The carbon in the continental crust is mainly in carbonates (limestones, marbles, etc.). In this paper we consider the origin of the carbonates. In 1952, Harold Urey proposed that calcium silicates produced by erosion reacted with atmospheric CO2 to produce carbonates, this is now known as the Urey reaction. In this paper we first address how the Urey reaction could have scavenged a significant mass of crustal carbon from the early atmosphere. At the present time the Urey reaction controls the CO2 concentration in the atmosphere. The CO2 enters the atmosphere by volcanism and is lost to the continental crust through the Urey reaction. We address this process in some detail. We then consider the decay of the Paleocene-Eocene thermal maximum (PETM). We quantify how the Urey reaction removes an injection of CO2 into the atmosphere. A typical decay time is 100 000 yr but depends on the variable rate of the Urey reaction. Keywords: Urey reaction, deep carbon, chemical geodynamics, carbonation; Earth in Five Reac- tions: A Deep Carbon Perspective INTRODUCTION time are the core, mantle, and continental crust.
    [Show full text]
  • Second International Science Meeting
    DEEP CARBON OBSERVATORY SECOND INTERNATIONAL SCIENCE MEETING 26–28 March 2015 Munich, Germany PROGRAM COMMITTEE Craig Manning, Program Committee Chair DCO Executive Committee and DCO Extreme Physics and Chemistry Community Scientific Steering Committee, University of California Los Angeles Donald Dingwell, Local Host DCO Executive Committee, Ludwig Maximilian University Magali Ader DCO Deep Energy Community Scientific Steering Committee, Institut de Physique du Globe de Paris Liz Cottrell DCO Reservoirs and Fluxes Community Scientific Steering Committee, Smithsonian Institution National Museum of Natural History Craig Schiffries DCO Secretariat, Carnegie Institution of Washington Matt Schrenk DCO Deep Life Community Scientific Steering Committee, Michigan State University VENUES Conference Hotel (Included breakfast buffet begins each morning at 06:00) Holiday Inn Munich–City Centre, Hochstraße 3, 81669 Icebreaker (Wednesday, 25 March, 18:00 – 20:00) Holiday Inn Munich–City Centre, Hochstraße 3, 81669 Science Meeting (Thursday, 26 March, Registration and coffee, 08:00; Program 09:00 - 17:00; Friday and Saturday, 27–28 March, Registration and coffee, 08:30; Program 09:00 - 17:00) Deutsches Museum, Museumsinsel 1, 80538 DCO Community Dinners (Thursday, 26 March, 20:00 - 22:00) Deep Energy and Deep Life, Restaurant Alter Hof, Alter Hof 3, 80331 Reservoirs and Fluxes and Extreme Physics and Chemistry, Zum Spöckmeier, Rosenstraße 9 (direct by the Marienplatz), D-80331 Poster Sessions (Friday, 27 March and Saturday, 28 March, 17:00 - 19:00) Holiday
    [Show full text]