Implications for Global-Scale Plate Tectonics Hamed Gamal El Dien1,2 ✉ , Luc S
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State Party Response to the Supplimentary Information Requested by Iucn for the Barberton Makhonjwa Mountains World Heritage
STATE PARTY RESPONSE TO THE SUPPLIMENTARY INFORMATION REQUESTED BY IUCN FOR THE BARBERTON MAKHONJWA MOUNTAINS WORLD HERITAGE NOMINATION 21 FEBRUARY 2018 GOVERNMENT OF THE REPUBLIC OF SOUTH AFRICA Barberton Makhonjwa Mountains is a site that South Africa submitted to Unesco for inscription as a World Heritage Site. An IUCN Evaluation Mission was successfully undertaken in September 2017. The aim of this Evaluation Mission was for IUCN to evaluate whether or not the property has Outstanding Universal Value, meet the conditions of integrity and (where relevant) of authenticity and meet the requirements of protection and management. Following the Evaluation Mission, IUCN wrote a letter to South Africa dated 20 December 2017, requesting supplementary information before finalising its recommendations to the World Heritage Committee. South Africa was requested to address the following aspects and to submit responses by 28 February 2018: Page: 1. Global Comparative analysis; 3 2. Legal protection; 3 3. Mining; 3 4. Buffer zones; 4 5. Relocation of people; 5 6. Threats; 5 7. Private Landowners; 5 8. Transboundary collaboration. 6 What follows below are the responses by South Africa, addressing the above points in chronological order, together with relevant attachments where indicated. 2 1. Global Comparative analysis As proposed by IUCN in terms of the Global Comparative Analysis, further review as requested has been submitted by Christoph Heubeck1, Carl Anhaeusser2 and Dion Brandt3. This new addendum has been integrated with the existing comparative analysis to provide a consolidated statement of the comparative values of the nominated property relative to other sites globally provided within the updated Nomination Dossier. -
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. -
Geology of the Eoarchean, >3.95 Ga, Nulliak Supracrustal
ÔØ ÅÒÙ×Ö ÔØ Geology of the Eoarchean, > 3.95 Ga, Nulliak supracrustal rocks in the Saglek Block, northern Labrador, Canada: The oldest geological evidence for plate tectonics Tsuyoshi Komiya, Shinji Yamamoto, Shogo Aoki, Yusuke Sawaki, Akira Ishikawa, Takayuki Tashiro, Keiko Koshida, Masanori Shimojo, Kazumasa Aoki, Kenneth D. Collerson PII: S0040-1951(15)00269-3 DOI: doi: 10.1016/j.tecto.2015.05.003 Reference: TECTO 126618 To appear in: Tectonophysics Received date: 30 December 2014 Revised date: 30 April 2015 Accepted date: 17 May 2015 Please cite this article as: Komiya, Tsuyoshi, Yamamoto, Shinji, Aoki, Shogo, Sawaki, Yusuke, Ishikawa, Akira, Tashiro, Takayuki, Koshida, Keiko, Shimojo, Masanori, Aoki, Kazumasa, Collerson, Kenneth D., Geology of the Eoarchean, > 3.95 Ga, Nulliak supracrustal rocks in the Saglek Block, northern Labrador, Canada: The oldest geological evidence for plate tectonics, Tectonophysics (2015), doi: 10.1016/j.tecto.2015.05.003 This is a PDF file of an unedited manuscript that has been accepted for publication. As a service to our customers we are providing this early version of the manuscript. The manuscript will undergo copyediting, typesetting, and review of the resulting proof before it is published in its final form. Please note that during the production process errors may be discovered which could affect the content, and all legal disclaimers that apply to the journal pertain. ACCEPTED MANUSCRIPT Geology of the Eoarchean, >3.95 Ga, Nulliak supracrustal rocks in the Saglek Block, northern Labrador, Canada: The oldest geological evidence for plate tectonics Tsuyoshi Komiya1*, Shinji Yamamoto1, Shogo Aoki1, Yusuke Sawaki2, Akira Ishikawa1, Takayuki Tashiro1, Keiko Koshida1, Masanori Shimojo1, Kazumasa Aoki1 and Kenneth D. -
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. -
The Archean Geology of Montana
THE ARCHEAN GEOLOGY OF MONTANA David W. Mogk,1 Paul A. Mueller,2 and Darrell J. Henry3 1Department of Earth Sciences, Montana State University, Bozeman, Montana 2Department of Geological Sciences, University of Florida, Gainesville, Florida 3Department of Geology and Geophysics, Louisiana State University, Baton Rouge, Louisiana ABSTRACT in a subduction tectonic setting. Jackson (2005) char- acterized cratons as areas of thick, stable continental The Archean rocks in the northern Wyoming crust that have experienced little deformation over Province of Montana provide fundamental evidence long (Ga) periods of time. In the Wyoming Province, related to the evolution of the early Earth. This exten- the process of cratonization included the establishment sive record provides insight into some of the major, of a thick tectosphere (subcontinental mantle litho- unanswered questions of Earth history and Earth-sys- sphere). The thick, stable crust–lithosphere system tem processes: Crustal genesis—when and how did permitted deposition of mature, passive-margin-type the continental crust separate from the mantle? Crustal sediments immediately prior to and during a period of evolution—to what extent are Earth materials cycled tectonic quiescence from 3.1 to 2.9 Ga. These compo- from mantle to crust and back again? Continental sitionally mature sediments, together with subordinate growth—how do continents grow, vertically through mafi c rocks that could have been basaltic fl ows, char- magmatic accretion of plutons and volcanic rocks, acterize this period. A second major magmatic event laterally through tectonic accretion of crustal blocks generated the Beartooth–Bighorn magmatic zone assembled at continental margins, or both? Structural at ~2.9–2.8 Ga. -
Origin of Archean Subcontinental Lithospheric Mantle: Some Petrological Constraints
Lithos 109 (2009) 61–71 Contents lists available at ScienceDirect Lithos journal homepage: www.elsevier.com/locate/lithos Origin of Archean subcontinental lithospheric mantle: Some petrological constraints N.T. Arndt a,⁎, N. Coltice b, H. Helmstaedt c, M. Gregoire d a LGCA, UMR 5025 CNRS, Université de Grenoble, 1381 rue de la Piscine, 38401 Grenoble, France b Laboratoire de Sciences de la Terre, Université de Lyon, Université Lyon1, Ecole Normale Supérieure de Lyon, CNRS, 2 rue Raphaël Dubois, 69622 Villeurbanne Cedex, France c Department of Geological Sciences, Queen's University, Kingston, Canada d Observatoire Midi-Pyrenées, Université de Toulouse 4 Ave. E. Belin 31400, Toulouse, France article info abstract Article history: The longevity of the continental lithosphere mantle is explained by its unusual composition. This part of the Received 9 June 2008 mantle is made up mainly of forsterite-rich olivine (Fo92–94), with or without orthopyroxene, and it is Accepted 17 October 2008 essentially anhydrous. The former characteristic makes it buoyant, the latter makes it viscous, and the Available online 5 November 2008 combination of these features that allow it to remain isolated from the convecting mantle. Highly forsteritic olivine is not normally produced during mantle melting. Possible explanations for its abundance in old Keywords: Archean subcontinental lithospheric mantle include: (a) high-degree mantle melting in a plume or at an Mantle Lithosphere Archean ocean ridge; (b) accretion of this material to older lithosphere and its reworking in a subduction Olivine zone; (c) redistribution of material to eliminate high-density, low-viscosity lithologies. Following an Archean evaluation of these models based on petrological and numerical modeling, we conclude that the most likely explanation is the accumulation of the residues of melting of one or more mantle plumes following by gravity-driven ejection of denser, Fe-rich components. -
Archean Subduction Or Not? Evidence from Volcanic Geochemistry
Archean Subduction or Not? Evidence from Volcanic Geochemistry Julian Pearce (Cardiff, UK) including collaboration with Hugh Smithies and David Peate Plan Part 1: Theory: Fingerprinting Subduction Volcanism Part 2: Life Cycles of Volcanic Arcs Part 3: Identification of Subduction Volcanism in the Palaeoproterozoic Part 4: Identification of Subduction Volcanism in the Middle to Late Archean Part 5: Identification of Subduction Volcanism in the Early Archean Plan Part 1: Theory: Fingerprinting Subduction Volcanism Part 2: Life Cycles of Volcanic Arcs Part 3: Identification of Subduction Volcanism in the Palaeoproterozoic Part 4: Identification of Subduction Volcanism in the Middle to Late Archean Part 5: Identification of Subduction Volcanism in the Early Archean Arc-aeology: Fingerprinting Arc Lavas in the Geological Record 1. Selective element mantle depletion by episodic enrichment In the mantle melt extraction towards arc front wedge. volcanic back-arc rear-arc intraplate arc ridge seamount volcano 2. Distinctive mantle flow pattern constrained by the F lithosphere B’ A’ subducting slab. C LT a sthenosphere HT B 3. Effects of high water UHT content on melting of the mantle wedge A 3. Effects of high water content in magmas on crystallization history and vesicularity/explosivity Arc-aeology: Fingerprinting Arc Lavas in the Geological Record 1. Selective element mantle depletion by episodic enrichment In the mantle melt extraction towards arc front wedge. volcanic back-arc rear-arc intraplate arc ridge seamount volcano 2. Distinctive mantle flow pattern constrained by the F lithosphere B’ A’ subducting slab. C LT a sthenosphere HT B 3. Effects of high water UHT content on melting of the mantle wedge A 3. -
Petrogenesis of 3.15 Ga Old Banasandra Komatiites from the Dharwar Craton, India: Implications for Early Mantle Heterogeneity
Accepted Manuscript Petrogenesis of 3.15 Ga old Banasandra komatiites from the Dharwar craton, India: Implications for early mantle heterogeneity J.M. Maya, Rajneesh Bhutani, S. Balakrishnan, S. Rajee Sandhya PII: S1674-9871(16)30025-1 DOI: 10.1016/j.gsf.2016.03.007 Reference: GSF 443 To appear in: Geoscience Frontiers Received Date: 5 November 2015 Revised Date: 1 March 2016 Accepted Date: 3 March 2016 Please cite this article as: Maya, J.M., Bhutani, R., Balakrishnan, S., Sandhya, S.R., Petrogenesis of 3.15 Ga old Banasandra komatiites from the Dharwar craton, India: Implications for early mantle heterogeneity, Geoscience Frontiers (2016), doi: 10.1016/j.gsf.2016.03.007. This is a PDF file of an unedited manuscript that has been accepted for publication. As a service to our customers we are providing this early version of the manuscript. The manuscript will undergo copyediting, typesetting, and review of the resulting proof before it is published in its final form. Please note that during the production process errors may be discovered which could affect the content, and all legal disclaimers that apply to the journal pertain. ACCEPTED MANUSCRIPT MANUSCRIPT ACCEPTED ACCEPTED MANUSCRIPT 1 Petrogenesis of 3.15 Ga old Banasandra komatiites from the Dharwar 2 craton, India: Implications for early mantle heterogeneity * 3 J. M. Maya, Rajneesh Bhutani , S. Balakrishnan, S. Rajee Sandhya 4 Department of Earth Sciences, Pondicherry University, Puducherry-605014, India 5 6 *Corresponding author. Phone: +919443636422; 7 E-mail address: [email protected] 8 9 MANUSCRIPT ACCEPTED ACCEPTED MANUSCRIPT 10 Abstract 11 Spinifex-textured, magnesian (MgO >25 wt.%) komatiites from Mesoarchean 12 Banasandra greenstone belt of the Sargur Group in the Dharwar craton, India were 13 analysed for major and trace elements and 147,146 Sm-143,142 Nd systematics to constrain 14 age, petrogenesis and to understand the evolution of Archean mantle. -
AST 201 - Introduction to Astrobiology Script
AST 201 - Introduction to Astrobiology Script Samuel Gunz1 and Martin Emons1 1Department of Biosystems Science and Engineering, ETH Zurich Autumn 2020 1 What is Life? Note that also some non-living things satisfy some of these traits (e.g. Fire, snowflake). In addition, some living things The definition of Life is not simple. NASA defines life as (e.g. seed, bacteria) can undergo a period of dormancy. Are follows, “Life is a self-sustaining system capable of Dar- they dead during that time because they are not growing, winian evolution.”. However, this excludes for instance metabolising or interacting with the environment? mules as they are infertile. The definition might depend in which context it is asked. Different smart people came up with various definitions, however they could never agree 1.2 Physical definition of life upon a single definition. It is important that a definition Life is an ordered system of molecules that ‘disobeys’ the should apply to alien life as well. Reproduction/replication second law of thermodynamics – that entropy always in- needs to be imperfect to allow for natural selection of those creases. An isolated cell cannot violate the second law branches of life with beneficial traits, otherwise life would of thermodynamics, the only way it can maintain a low- have got stuck at the first replicating organism. entropy, nonequilibrium state characterised by a high de- gree of structural organisation is to increase the entropy of The chicken and egg problem illustrates the problem of its surroundings. A cell releases some of the energy that it the definition of life and species. -
Geology of the Nuvvuagittuq Belt
Earth’s Oldest Rocks Edited by Martin J. van Kranendonk, R. Hugh Smithies and Vickie C. Bennett Developments in Precambrian Geology, Vol. 15 (K.C. Condie, Series Editor) ©2007 Elsevier B.V. All rights reserved. THE GEOLOGY OF THE 3.8 GA NUVVUAGITTUQ (PORPOISE COVE) GREENSTONE BELT, NORTHEASTERN SUPERIOR PROVINCE, CANADA. Jonathan O’Neil1, Charles Maurice2, Ross K. Stevenson3,4, Jeff Larocque5, Christophe Cloquet6, Jean David3 & Don Francis1 1 Earth & Planetary Sciences, McGill University and GÉOTOP-UQÀM-McGill, 3450 University St. Montreal, QC, Canada, H3A 2A7 ([email protected]) 2 Bureau de l’exploration géologique du Québec, Ministère des Ressources naturelles et de la Faune, 400 boul. Lamaque Val d’Or, QC, J9P 3L4 3 GÉOTOP-UQÀM-McGill, Université du Québec à Montréal, C.P. 8888, succ. centre-ville, Montreal, QC, Canada H3C 3P8 4 Département des Sciences de la Terre et de l’Atmosphère, Université du Québec à Montréal, C.P. 8888, succ. centre-ville Montreal, QC, Canada H3C 3P8 5 School of Earth and Oceanic Sciences, University of Victoria, P.O. Box 3055 STN CSC, Victoria, BC, Canada, V8W 3P6 6 INW-UGent, Department of analytical chemistry, Proeftuinstraat 86, 9000 GENT, Belgium Abstract The Nuvvuagittuq greenstone belt is a 3.8 Ga supracrustal succession preserved as a raft in remobilised tonalities along the eastern coast of Hudson Bay. The dominant lithology of the belt is a quartz-ribboned grey amphibolite composed of variable proportions of cummingtonite, biotite and plagioclase. Although the amphibolites have mafic compositions, the presence of cummingtonite rather than hornblende in these rocks reflects their low Ca contents, which may result from the alteration and metamorphism of mafic pyroclastic rocks. -
RESEARCH a Non–Plate Tectonic
RESEARCH A non–plate tectonic model for the Eoarchean Isua supracrustal belt A. Alexander G. Webb1,*, Thomas Müller2, Jiawei Zuo1, Peter J. Haproff3, and Anthony Ramírez-Salazar2 1DEPARTMENT OF EARTH SCIENCES AND LABORATORY FOR SPACE RESEARCH, UNIVERSITY OF HONG KONG, POKFULAM ROAD, HONG KONG, CHINA 2SCHOOL OF EARTH AND ENVIRONMENT, UNIVERSITY OF LEEDS, MATHS/EARTH AND ENVIRONMENT BUILDING, LEEDS LS2 9JT, UK 3DEPARTMENT OF EARTH AND OCEAN SCIENCES, UNIVERSITY OF NORTH CAROLINA, WILMINGTON, NORTH CAROLINA 28403, USA ABSTRACT The ca. 3.8–3.6-b.y.-old Isua supracrustal belt of SW Greenland is Earth’s only site older than 3.2 Ga that is exclusively interpreted via plate- tectonic theory. The belt is divided into ca. 3.8 Ga and ca. 3.7 Ga halves, and these are interpreted as plate fragments that collided by ca. 3.6 Ga. However, such models are based on idiosyncratic interpretations of field observations and U-Pb zircon data, resulting in intricate, conflicting stratigraphic and structural interpretations. We reanalyzed published geochronological work and associated field constraints previously interpreted to show multiple plate-tectonic events and conducted field-based exploration of metamorphic and structural gra- dients previously interpreted to show heterogeneities recording plate-tectonic processes. Simpler interpretations are viable, i.e., the belt may have experienced nearly homogeneous metamorphic conditions and strain during a single deformation event prior to intrusion of ca. 3.5 Ga mafic dikes. Curtain and sheath folds occur at multiple scales throughout the belt, with the entire belt potentially representing Earth’s largest a-type fold. Integrating these findings, we present a new model in which two cycles of volcanic burial and resultant melt- ing and tonalite-trondhjemite-granodiorite (TTG) intrusion produced first the ca. -
Generation of Earth's Early Continents from a Relatively Cool Archean
RESEARCH ARTICLE Generation of Earth's Early Continents From a Relatively 10.1029/2018GC008079 Cool Archean Mantle Key Points: 1 2 1 3 • Geodynamic and thermodynamic Andrea Piccolo , Richard M. Palin , Boris J.P. Kaus , and Richard W. White modeling are applied to understand 1 2 the production of continental crust Institute for Geosciences, Johannes-Gutenberg University of Mainz, Mainz, Germany, Department of Geology and • Production of continental crust Geological Engineering, Colorado School of Mines, Golden, CO, USA, 3School of Earth and Environmental Sciences, produces dense residuum, which University of St Andrews, St Andrews, UK triggers Rayleigh instabilities that destabilize the lithosphere • The continental crust production via Rayleigh-Taylor instabilities Abstract Several lines of evidence suggest that the Archean (4.0–2.5 Ga) mantle was hotter than ◦ could work at low mantle potential today's potential temperature (TP) of 1350 C. However, the magnitude of such difference is poorly temperature (T ), supporting the ◦ P constrained, with TP estimation spanning from 1500 to 1600 C during the Meso-Archean (3.2–2.8 Ga). new T temperatures estimates P Such differences have major implications for the interpreted mechanisms of continental crust generation on the early Earth, as their efficacy is highly sensitive to the TP. Here we integrate petrological modeling Supporting Information: with thermomechanical simulations to understand the dynamics of crust formation during Archean. • Supporting Information S1 Our results predict that partial melting of primitive oceanic crust produces felsic melts with geochemical ◦ signatures matching those observed in Archean cratons from a mantle TP as low as 1450 C thanks Correspondence to: to lithospheric-scale RayleighTaylor-type instabilities.