3.18 Oneviewofthegeochemistryof Subduction-Related Magmatic Arcs
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The Evolution of a Heterogeneous Martian Mantle: Clues from K, P, Ti, Cr, and Ni Variations in Gusev Basalts and Shergottite Meteorites
Earth and Planetary Science Letters 296 (2010) 67–77 Contents lists available at ScienceDirect Earth and Planetary Science Letters journal homepage: www.elsevier.com/locate/epsl The evolution of a heterogeneous Martian mantle: Clues from K, P, Ti, Cr, and Ni variations in Gusev basalts and shergottite meteorites Mariek E. Schmidt a,⁎, Timothy J. McCoy b a Dept. of Earth Sciences, Brock University, St. Catharines, ON, Canada L2S 3A1 b Dept. of Mineral Sciences, National Museum of Natural History, Smithsonian Institution, Washington, DC 20560-0119, USA article info abstract Article history: Martian basalts represent samples of the interior of the planet, and their composition reflects their source at Received 10 December 2009 the time of extraction as well as later igneous processes that affected them. To better understand the Received in revised form 16 April 2010 composition and evolution of Mars, we compare whole rock compositions of basaltic shergottitic meteorites Accepted 21 April 2010 and basaltic lavas examined by the Spirit Mars Exploration Rover in Gusev Crater. Concentrations range from Available online 2 June 2010 K-poor (as low as 0.02 wt.% K2O) in the shergottites to K-rich (up to 1.2 wt.% K2O) in basalts from the Editor: R.W. Carlson Columbia Hills (CH) of Gusev Crater; the Adirondack basalts from the Gusev Plains have more intermediate concentrations of K2O (0.16 wt.% to below detection limit). The compositional dataset for the Gusev basalts is Keywords: more limited than for the shergottites, but it includes the minor elements K, P, Ti, Cr, and Ni, whose behavior Mars igneous processes during mantle melting varies from very incompatible (prefers melt) to very compatible (remains in the shergottites residuum). -
Kinematic Reconstruction of the Caribbean Region Since the Early Jurassic
Earth-Science Reviews 138 (2014) 102–136 Contents lists available at ScienceDirect Earth-Science Reviews journal homepage: www.elsevier.com/locate/earscirev Kinematic reconstruction of the Caribbean region since the Early Jurassic Lydian M. Boschman a,⁎, Douwe J.J. van Hinsbergen a, Trond H. Torsvik b,c,d, Wim Spakman a,b, James L. Pindell e,f a Department of Earth Sciences, Utrecht University, Budapestlaan 4, 3584 CD Utrecht, The Netherlands b Center for Earth Evolution and Dynamics (CEED), University of Oslo, Sem Sælands vei 24, NO-0316 Oslo, Norway c Center for Geodynamics, Geological Survey of Norway (NGU), Leiv Eirikssons vei 39, 7491 Trondheim, Norway d School of Geosciences, University of the Witwatersrand, WITS 2050 Johannesburg, South Africa e Tectonic Analysis Ltd., Chestnut House, Duncton, West Sussex, GU28 OLH, England, UK f School of Earth and Ocean Sciences, Cardiff University, Park Place, Cardiff CF10 3YE, UK article info abstract Article history: The Caribbean oceanic crust was formed west of the North and South American continents, probably from Late Received 4 December 2013 Jurassic through Early Cretaceous time. Its subsequent evolution has resulted from a complex tectonic history Accepted 9 August 2014 governed by the interplay of the North American, South American and (Paleo-)Pacific plates. During its entire Available online 23 August 2014 tectonic evolution, the Caribbean plate was largely surrounded by subduction and transform boundaries, and the oceanic crust has been overlain by the Caribbean Large Igneous Province (CLIP) since ~90 Ma. The consequent Keywords: absence of passive margins and measurable marine magnetic anomalies hampers a quantitative integration into GPlates Apparent Polar Wander Path the global circuit of plate motions. -
Tardi-Magmatic Precipitation of Martian Fe/Mg-Rich Clay Minerals Via Igneous Differentiation
©2020TheAuthors Published by the European Association of Geochemistry ▪ Tardi-magmatic precipitation of Martian Fe/Mg-rich clay minerals via igneous differentiation J.-C. Viennet1*, S. Bernard1, C. Le Guillou2, V. Sautter1, P. Schmitt-Kopplin3, O. Beyssac1, S. Pont1, B. Zanda1, R. Hewins1, L. Remusat1 Abstract doi: 10.7185/geochemlet.2023 Mars is seen as a basalt covered world that has been extensively altered through hydrothermal or near surface water-rock interactions. As a result, all the Fe/Mg-rich clay minerals detected from orbit so far have been interpreted as secondary, i.e. as products of aqueous alteration of pre-existing silicates by (sub)surface water. Based on the fine scale petrographic study of the evolved mesostasis of the Nakhla mete- orite, we report here the presence of primary Fe/Mg-rich clay minerals that directly precipitated from a water-rich fluid exsolved from the Cl-rich parental melt of nakhlites during igneous differentiation. Such a tardi-magmatic precipitation of clay minerals requires much lower amounts of water compared to production via aque- ous alteration. Although primary Fe/Mg-rich clay minerals are minor phases in Nakhla, the contribution of such a process to Martian clay formation may have been quite significant during the Noachian given that Noachian magmas were richer in H2O. In any case, the present discovery justifies a re-evaluation of the exact origin of the clay minerals detected on Mars so far, with potential consequences for our vision of the early magmatic and climatic histories of Mars. Received 26 January 2020 | Accepted 27 May 2020 | Published 8 July 2020 Letter mafic crustal materials (Smith and Bandfield, 2012; Ehlmann and Edwards, 2014). -
Lunar Silica-Bearing Diorite: a Lithology from the Moon with Implications for Igneous Differentiation
50th Lunar and Planetary Science Conference 2019 (LPI Contrib. No. 2132) 2008.pdf LUNAR SILICA-BEARING DIORITE: A LITHOLOGY FROM THE MOON WITH IMPLICATIONS FOR IGNEOUS DIFFERENTIATION. T. J. Fagan1* and S. Ohkawa1, 1Dept. Earth Sci., Waseda Univ., 1-6-1 Nishi- waseda, Shinjuku, Tokyo, 169-8050, Japan (*[email protected]). Introduction: Silica-rich igneous (“granitic”) ratios and relatively high F concentrations indicate that rocks are rare on the Moon, but have been detected by the analyzed grains are apatite (not merrillite). remote sensing on the lunar surface [e.g., 1], and in Results: The silica-bearing diorite (Sil-Di) is dom- Apollo samples and lunar meteorites [e.g., 2-5]. To date, inated by pyroxene (55 mode%), plagioclase feldspar lunar granitic samples have been characterized by high (36%), silica (4.4%), ilmenite (3.9%) and K-feldspar concentrations of incompatible elements and/or mafic (0.3%) (Fig. 2). Apatite and troilite also occur. The Sil- silicates with high Fe# (atomic Fe/[Fe+Mg]x100) [2-5], Di exhibits interlocking, igneous textures with elongate both features consistent with origin from late-stage re- plagioclase feldspar (Fig. 2). Plagioclase feldspar has sidual liquids or very low degree partial melting. Fur- nearly constant composition of An88Ab11, but pyroxene thermore, silica-rich rocks detected by remote sensing has a wide range of zoning (Fig. 3). often combine the Christiansen feature in infra-red spec- The modal composition of the Sil-Di is plagioclase- tra with high incompatible element concentrations (e.g., rich compared to many silica-bearing igneous rocks Th detected by gamma-ray spectroscopy [1]), again re- from the Moon (Fig. -
Episodic Nature of Continental Arc Activity Since 750 Ma: a Global Compilation ∗ Wenrong Cao A, , Cin-Ty A
Earth and Planetary Science Letters 461 (2017) 85–95 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl Episodic nature of continental arc activity since 750 Ma: A global compilation ∗ Wenrong Cao a, , Cin-Ty A. Lee a, Jade Star Lackey b a Department of Earth Science, Rice University, 6100 Main Street, MS-126, Houston, TX 77005, United States b Geology Department, Pomona College, 185 East 6th Street, Claremont, CA 91711, United States a r t i c l e i n f o a b s t r a c t Article history: Continental arcs have been recently hypothesized to outflux large amounts of CO2 compared to island Received 15 October 2016 arcs so that global flare-ups in continental arc magmatism might drive long-term greenhouse events. Received in revised form 3 December 2016 Quantitative testing of this hypothesis, however, has been limited by the lack of detailed studies on Accepted 27 December 2016 the spatial distribution of continental arcs through time. Here, we compile a worldwide database of Available online xxxx geological maps and associated literature to delineate the surface exposure of granitoid plutons, allowing Editor: A. Yin reconstruction of how the surface area addition rate of granitoids and the length of continental arcs have Keywords: varied since 750 Ma. These results were integrated into an ArcGIS framework and plate reconstruction continental arcs models. We find that the spatial extent of continental arcs is episodic with time and broadly matches episodicity the detrital zircon age record. Most vigorous arc magmatism occurred during the 670–480 Ma and the plate tectonics 250–50 Ma when major greenhouse events are recognized. -
The Mars 2020 Candidate Landing Sites: a Magnetic Field Perspective
The Mars 2020 Candidate Landing Sites: A Magnetic Field Perspective The MIT Faculty has made this article openly available. Please share how this access benefits you. Your story matters. Citation Mittelholz, Anna et al. “The Mars 2020 Candidate Landing Sites: A Magnetic Field Perspective.” Earth and Space Science 5, 9 (September 2018): 410-424 © 2018 The Authors As Published http://dx.doi.org/10.1029/2018EA000420 Publisher American Geophysical Union (AGU) Version Final published version Citable link http://hdl.handle.net/1721.1/118846 Terms of Use Creative Commons Attribution-NonCommercial-NoDerivs License Detailed Terms http://creativecommons.org/licenses/by-nc-nd/4.0/ Earth and Space Science RESEARCH ARTICLE The Mars 2020 Candidate Landing Sites: A Magnetic 10.1029/2018EA000420 Field Perspective Key Points: • Mars 2020 offers the opportunity Anna Mittelholz1 , Achim Morschhauser2 , Catherine L. Johnson1,3, to acquire samples that record the Benoit Langlais4 , Robert J. Lillis5 , Foteini Vervelidou2 , and Benjamin P. Weiss6 intensity and direction of the ancient Martian magnetic field 1 • Laboratory paleomagnetic Department of Earth, Ocean and Atmospheric Sciences, The University of British Columbia, Vancouver, British Columbia, 2 3 measurements of returned samples Canada, GFZ German Research Center for Geosciences, Potsdam, Germany, Planetary Science Institute, Tucson, AZ, USA, can address questions about the 4Laboratoire de Planétologie et Geodynamique, UMR 6112 CNRS & Université de Nantes, Nantes, France, 5Space Science history of the -
Chronology of Late Cretaceous Igneous and Hydrothermal Events at the Golden Sunlight Gold-Silver Breccia Pipe, Southwestern Montana
Chronology of Late Cretaceous Igneous and Hydrothermal Events at the Golden Sunlight Gold-Silver Breccia Pipe, Southwestern Montana U.S. GEOLOGICAL SURVEY BULLETIN 2155 T OF EN TH TM E R I A N P T E E D R . I O S . R U M 9 A 8 4 R C H 3, 1 a Chronology of Late Cretaceous Igneous and Hydrothermal Events at the Golden Sunlight Gold-Silver Breccia Pipe, Southwestern Montana By Ed DeWitt, Eugene E. Foord, Robert E. Zartman, Robert C. Pearson, and Fess Foster T OF U.S. GEOLOGICAL SURVEY BULLETIN 2155 EN TH TM E R I A N P T E E D R . I O S . R U M 9 A 8 4 R C H 3, 1 UNITED STATES GOVERNMENT PRINTING OFFICE, WASHINGTON : 1996 a U.S. DEPARTMENT OF THE INTERIOR BRUCE BABBITT, Secretary U.S. GEOLOGICAL SURVEY Gordon P. Eaton, Director For sale by U.S. Geological Survey, Information Services Box 25286, Federal Center Denver, CO 80225 Any use of trade, product, or firm names in this publication is for descriptive purposes only and does not imply endorsement by the U.S. Government Library of Congress Cataloging-in-Publication Data Chronolgy of Late Cretaceous igneous and hydrothermal events at the Golden Sunlight gold-silver breccia pipe, southwestern Montana / by Ed DeWitt . [et al.]. p. cm.—(U.S. Geological Survey bulletin ; 2155) Includes bibliographical references. Supt. of Docs. no. : I 19.3 : 2155 1. Geology, Stratigraphic—Cretaceous. 2. Rocks, Igneous—Montana. 3. Hydrothermal alteration—Montana. 4. Gold ores—Montana. 5. Breccia pipes—Montana. -
Arc-Continent Collision and the Formation of Continental Crust: a New Geochemical and Isotopic Record from the Ordovician Tyrone Igneous Complex, Ireland
View metadata, citation and similar papers at core.ac.uk brought to you by CORE provided by Woods Hole Open Access Server Arc-Continent Collision and the Formation of Continental Crust: A New Geochemical and Isotopic Record from the Ordovician Tyrone Igneous Complex, Ireland Amy E. Draut U.S. Geological Survey, Santa Cruz, CA 95060, U.S.A. [email protected] Peter D. Clift School of Geosciences, University of Aberdeen, Aberdeen AB24 3UE, United Kingdom Jeffrey M. Amato Department of Geological Sciences, New Mexico State University, Las Cruces, NM 88003, U.S.A. Jerzy Blusztajn and Hans Schouten Department of Geology and Geophysics, Woods Hole Oceanographic Institution, Woods Hole, MA 02543, U.S.A. Abstract Collisions between oceanic island-arc terranes and passive continental margins are thought to have been important in the formation of continental crust throughout much of Earth’s history. Magmatic evolution during this stage of the plate-tectonic cycle is evident in several areas of the Ordovician Grampian-Taconic Orogen, as we demonstrate in the first detailed geochemical study of the Tyrone Igneous Complex, Ireland. New U– Pb zircon dating yields ages of 493 ± 2 Ma from a primitive mafic intrusion, indicating intra-oceanic subduction in Tremadoc time, and 475 ± 10 Ma from a light-rare-earth- element (LREE)-enriched tonalite intrusion that incorporated Laurentian continental material by early Arenig time (Early Ordovician, Stage 2) during arc-continent collision. Notably, LREE enrichment in volcanism and silicic intrusions of the Tyrone Igneous Draut et al. page 1 of 27 Complex exceeds that of average Dalradian (Laurentian) continental material which would have been thrust under the colliding forearc and potentially recycled into arc magmatism. -
Magma Mixing Interaction Between Rhyolitic and Basaltic Melt
Magma Mixing Interaction Between Rhyolitic and Basaltic Melt Daniele Morgavi München 2013 Magma Mixing Interaction Between Rhyolitic and Basaltic Melts Daniele Morgavi Dissertation an der Fakultat fur Geowissenschaften der Ludwig-Maximilians-Universität München vorgelegt von Daniele Morgavi aus Roma, Italia München, den May, 2013 Erstgutachter: DONALD B. DINGWELL Zweitgutachter: DIEGO PERUGINI Tag der mündlichen Prüfung: 14. 01. 2014 To all the Friend and lovers that have shared a peace of their life with me In my life (Lennon and McCartney) There are places I remember All my life, though some have changed Some forever not for better Some have gone and some remain All these places have their moments With lovers and friends I still can recall Some are dead and some are living In my life I've loved them all But of all these friends and lovers There is no one compares with you And these memories lose their meaning When I think of love as something new Though I know I'll never lose affection For people and things that went before I know I'll often stop and think about them In my life I love you more Though I know I'll never lose affection For people and things that went before I know I'll often stop and think about them In my life I love you more In my life I love you more i Table of content Table of content……………………………………………………………………ii List of figures………………………………………………………………………iv List of tables………………………………………………………………………..v Preamble…………………………………………………………………………...vi Summary…………………………………………………………………………..vii Zusammenfassung………………………………………………………………...viii Chapter 1. Introduction…………………………………………………………….1 1.1 Magma mixing theory the idea of Bunsen…………………………………2 1.2 Magma mixing in the modern times……………………………………….4 1.3 Numerical and experimental stady a new light for understanding magma mixing………………………………………………………………5 1.4 Chaotic Mixing Experiment………………………………………………..6 Chapter 2. -
Chemical and Isotopic Fractionation of Wet Andesite in a Temperature Gradient: Experiments and Models Suggesting a New Mechanism of Magma Differentiation
Available online at www.sciencedirect.com Geochimica et Cosmochimica Acta 73 (2009) 729–749 www.elsevier.com/locate/gca Chemical and isotopic fractionation of wet andesite in a temperature gradient: Experiments and models suggesting a new mechanism of magma differentiation F. Huang a, C.C. Lundstrom a,*, J. Glessner a, A. Ianno a, A. Boudreau b,J.Lia, E.C. Ferre´ c, S. Marshak a, J. DeFrates a a Department of Geology, University of Illinois at Urbana-Champaign, 245 NHB, 1301 W. Green St., IL 61801, USA b Nicholas School of the Environment and Earth Sciences, Box 90227, Duke University, Durham, NC 27708, USA c Department of Geology, Southern Illinois University, Carbondale, IL 62901-4324, USA Received 6 August 2008; accepted in revised form 4 November 2008; available online 18 November 2008 Abstract Piston–cylinder experiments were conducted to investigate the behavior of partially molten wet andesite held within an imposed temperature gradient at 0.5 GPa. In one experiment, homogenous andesite powder (USGS rock standard AGV-1) with 4 wt.% H2O was sealed in a double capsule assembly for 66 days. The temperature at one end of this charge was held at 950 °C, and the temperature at the other end was kept at 350 °C. During the experiment, thermal migration (i.e., diffusion in a thermal gra- dient) took place, and the andesite underwent compositional and mineralogical differentiation. The run product can be broadly divided into three portions: (1) the top third, at the hot end, contained 100% melt; (2) the middle-third contained crystalline phases plus progressively less melt; and (3) the bottom third, at the cold end, consisted of a fine-grained, almost entirely crystalline solid of granitic composition. -
The Link Between Volcanism and Tectonics in the Southern Volcanic Zone of the Chilean Andes: a Review
Tectonophysics 471 (2009) 96–113 Contents lists available at ScienceDirect Tectonophysics journal homepage: www.elsevier.com/locate/tecto The link between volcanism and tectonics in the southern volcanic zone of the Chilean Andes: A review José Cembrano a,⁎, Luis Lara b a Universidad Católica del Norte Avda. Angamos 0610, Antofagasta, Chile b Servicio Nacional de Geología y Minería, Avda. Santa María 0104, Santiago, Chile article info abstract Article history: The nature of the interplay between tectonics and volcanism is a major question in continental margin Received 7 January 2008 tectonics. The Southern Andes volcanic zone (SVZ), located at the obliquely convergent Nazca–South America Received in revised form 16 January 2009 plate margin between 33°S and 46°S, offers a unique opportunity to address this question because of along- Accepted 26 February 2009 strike changes in crustal thickness, tectonic style and well-constrained long-term and short-term kinematic Available online 13 March 2009 history. The complex interaction between tectonic and magmatic processes is evidenced by both the architecture and geochemical signature of volcanic systems. Main first-order factors accounting for the Keywords: Southern Andes along-strike variations in the nature and composition of volcanism are crustal thickness and the existence of Volcanism a major, intra-arc fault system, the Liquiñe–Ofqui fault zone (LOFZ). Second order factors include the local Arc tectonics nature of the volcanic arc basement. Liquiñe-Ofqui fault zone Two main categories of volcano–tectonic associations have been identified, according to the spatial Dykes distribution and internal organization of individual volcanoes and clusters of volcanoes with respect to both the overall strike of the volcanic arc and the first and second-order active/inactive basement faults. -
IGNEOUS ROCKS Where Do Igneous Rocks Form?
FUNDAMENTALS OF EARTH SCIENCE I FALL SEMESTER 2018 IGNEOUS ROCKS Where do igneous rocks form? Understanding Earth 6th Ed. Classification of igneous rocks 1. TEXTURE Cooling of magma/lava Crystallization of minerals Formation of an igneous rock Slow cooling Rapid within the cooling lithosphere near or on Earth’s surface INTRUSIVE IGNEOUS ROCKS EXTRUSIVE IGNEOUS ROCKS Coarser-grained texture Finer-grained texture e.g. granite e.g. basalt Understanding Earth 6th Ed. Different types of igneous rocks identified based on the texture Understanding Earth 6th Ed. 2. CHEMICAL AND MINERALOGICAL COMPOSITION Felsic vs. mafic compositions Felsic : feldspar-silica Mafic : magnesium-ferric FELSIC MAFIC Igneous rocks enriched in SiO2 and Igneous rocks enriched in silicates silicates rich in Al, K, Na rich in Fe, Mg Quartz (SiO2) Biotite (mica) Orthoclase (K-rich feldspar) Amphibole group Plagioclase (Na/Ca-rich feldspar) Pyroxene group Muscovite (K-rich mica) Olivine Example: granite (continental crust) Example: basalt (oceanic crust) Light color Dark color CONTINUUM Pyroxene Anorthite: Quartz: SiO CaAl2Si2O8 2 Ca-rich plagioclase Granite Basalt Orthoclase: KAlSi3O8 Continental crust 0-7 km Fe, Mg > 3.0 g/cm3 Oceanic crust 35-60 km Al, K, Na > Fe, Mg >> 3.4 g/cm3 2.8 g/cm3 Mantle Peridotite Olivine: (Mg, Fe)2SiO4 Pyroxene: XY(Si,Al)2O6 Enstatite (MgSiO3) and ferrosilite (FeSiO3) Augite (Ca,Na)(Mg,Fe,Al,Ti)(Si,Al)2O6 DOMINANT IN EARTH’S UPPER MANTLE Intrusive Extrusive Anorthite CaAl2Si2O8 KAlSi O ABUNDANT IN 3 8 ABUNDANT IN THE THE CONTINENTAL OCEANIC CRUST SiO2 CRUST (underlying ocean floor) NaAlSi O 3 8 (Mg, Fe)SiO Albite 3 (Mg, Fe)2SiO4 LIGHT color DARK color Crystallize and melt at different T !!! http://www.gso.uri.edu/lava/MagmaProperties/properties.html Understanding Earth 6th Ed.