Dehydration Melting Below the Undersaturated Transition Zone W Panero, C Thomas, R
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Density Difference Between Subducted Oceanic Crust and Ambient Mantle in the Mantle Transition Zone Density Difference Between S
Density Difference between Subducted Oceanic Crust and Ambient Mantle in the Mantle Transition Zone Since the beginning of plate tectonics, the were packed separately into NaCl or MgO sample oceanic lithosphere has been continually subducted chamber with a mixture of gold and MgO, and into the Earth’s deep mantle for 4.5 Gy. The compressed in the same high-pressure cell. The oceanic lithosphere consists of an upper basaltic pressure was determined by the cell volume for layer (oceanic crust) and a lower olivine-rich gold using an equation of state of gold [2], and the peridotitic layer. The total amount of subducted temperature was measured by a thermocouple. oceanic crust in this 4.5 Gy period is estimated to The cell volumes of garnet and ringwoodite were be at least ~3 × 1 0 23 kg, which is about 8% of the determined by least squares calculations using the weight of the present Earth’s mantle. Thus, the positions of X-ray diffraction peaks. The samples oceanic crust, which is rich in pyroxene and garnet, were compressed to the desired pressure at room may be the source of very important chemical temperature and heated to the maximum temperature heterogeneity in the olivine-rich Earth’s mantle. To to release non-hydrostatic stress. clarify behavior of the oceanic crust in the deep Pressure-volume-temperature data were collected mantle, accurate information about density under 47 different conditions. Figure 1 shows P -V - differences between the oceanic crust and the T data for garnet. The data collected by using an ambient mantle is very important. -
Mantle Transition Zone Structure Beneath Northeast Asia from 2-D
RESEARCH ARTICLE Mantle Transition Zone Structure Beneath Northeast 10.1029/2018JB016642 Asia From 2‐D Triplicated Waveform Modeling: Key Points: • The 2‐D triplicated waveform Implication for a Segmented Stagnant Slab fi ‐ modeling reveals ne scale velocity Yujing Lai1,2 , Ling Chen1,2,3 , Tao Wang4 , and Zhongwen Zhan5 structure of the Pacific stagnant slab • High V /V ratios imply a hydrous p s 1State Key Laboratory of Lithospheric Evolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, and/or carbonated MTZ beneath 2 3 Northeast Asia Beijing, China, College of Earth Sciences, University of Chinese Academy of Sciences, Beijing, China, CAS Center for • A low‐velocity gap is detected within Excellence in Tibetan Plateau Earth Sciences, Beijing, China, 4Institute of Geophysics and Geodynamics, School of Earth the stagnant slab, probably Sciences and Engineering, Nanjing University, Nanjing, China, 5Seismological Laboratory, California Institute of suggesting a deep origin of the Technology, Pasadena, California, USA Changbaishan intraplate volcanism Supporting Information: Abstract The structure of the mantle transition zone (MTZ) in subduction zones is essential for • Supporting Information S1 understanding subduction dynamics in the deep mantle and its surface responses. We constructed the P (Vp) and SH velocity (Vs) structure images of the MTZ beneath Northeast Asia based on two‐dimensional ‐ Correspondence to: (2 D) triplicated waveform modeling. In the upper MTZ, a normal Vp but 2.5% low Vs layer compared with L. Chen and T. Wang, IASP91 are required by the triplication data. In the lower MTZ, our results show a relatively higher‐velocity [email protected]; layer (+2% V and −0.5% V compared to IASP91) with a thickness of ~140 km and length of ~1,200 km [email protected] p s atop the 660‐km discontinuity. -
Deep Earth Structure: Lower Mantle and D"
This article was originally published in Treatise on Geophysics, Second Edition, published by Elsevier, and the attached copy is provided by Elsevier for the author's benefit and for the benefit of the author's institution, for non-commercial research and educational use including without limitation use in instruction at your institution, sending it to specific colleagues who you know, and providing a copy to your institution’s administrator. All other uses, reproduction and distribution, including without limitation commercial reprints, selling or licensing copies or access, or posting on open internet sites, your personal or institution’s website or repository, are prohibited. For exceptions, permission may be sought for such use through Elsevier's permissions site at: http://www.elsevier.com/locate/permissionusematerial Lay T Deep Earth Structure: Lower Mantle and D″. In: Gerald Schubert (editor-in-chief) Treatise on Geophysics, 2nd edition, Vol 1. Oxford: Elsevier; 2015. p. 683-723. Author's personal copy 00 1.22 Deep Earth Structure: Lower Mantle and D T Lay, University of California Santa Cruz, Santa Cruz, CA, USA ã 2015 Elsevier B.V. All rights reserved. 1.22.1 Lower Mantle and D00 Basic Structural Attributes 684 1.22.1.1 Elastic Parameters, Density, and Thermal Structure 684 1.22.1.2 Mineralogical Structure 685 1.22.2 One-Dimensional Lower Mantle Structure 686 1.22.2.1 Body-Wave Travel Time and Slowness Constraints 687 1.22.2.2 Surface-Wave/Normal-Mode Constraints 688 1.22.2.3 Attenuation Structure 688 1.22.3 Three-Dimensional -
50 Years of Petrology
spe500-01 1st pgs page 1 The Geological Society of America 18888 201320 Special Paper 500 2013 CELEBRATING ADVANCES IN GEOSCIENCE Plates, planets, and phase changes: 50 years of petrology David Walker* Department of Earth and Environmental Sciences, Lamont-Doherty Earth Observatory, Columbia University, Palisades, New York 10964, USA ABSTRACT Three advances of the previous half-century fundamentally altered petrology, along with the rest of the Earth sciences. Planetary exploration, plate tectonics, and a plethora of new tools all changed the way we understand, and the way we explore, our natural world. And yet the same large questions in petrology remain the same large questions. We now have more information and understanding, but we still wish to know the following. How do we account for the variety of rock types that are found? What does the variety and distribution of these materials in time and space tell us? Have there been secular changes to these patterns, and are there future implications? This review examines these bigger questions in the context of our new understand- ings and suggests the extent to which these questions have been answered. We now do know how the early evolution of planets can proceed from examples other than Earth, how the broad rock cycle of the present plate tectonic regime of Earth works, how the lithosphere atmosphere hydrosphere and biosphere have some connections to each other, and how our resources depend on all these things. We have learned that small planets, whose early histories have not been erased, go through a wholesale igneous processing essentially coeval with their formation. -
The Akimotoite–Majorite–Bridgmanite Triple Point Determined in Large Volume Press and Laser-Heated Diamond Anvil Cell
Preprints (www.preprints.org) | NOT PEER-REVIEWED | Posted: 12 December 2019 doi:10.20944/preprints201912.0177.v1 Peer-reviewed version available at Minerals 2020, 10, 67; doi:10.3390/min10010067 Article The Akimotoite–Majorite–Bridgmanite Triple Point Determined in Large Volume Press and Laser-Heated Diamond Anvil Cell Britany L. Kulka1, Jonathan D. Dolinschi1, Kurt D. Leinenweber2, Vitali B. Prakapenka3, and Sang-Heon Shim1 1 School of Earth and Space Exploration, Arizona State University, Tempe, Arizona, USA 2 Eyring Materials Center, Arizona State University, Tempe, Arizona, USA 3 GeoSoilEnviroCars, University of Chicago, Chicago, Illinois 60439, USA * Correspondence: [email protected] Abstract: The akimotoite–majorite–bridgmanite (Ak–Mj–Bm) triple point in MgSiO3 has been measured in large-volume press (LVP; COMPRES 8/3 assembly) and laser-heated diamond anvil cell (LHDAC). For the LVP data, we calculated pressures from the calibration by Leinenweber et al. [1]. For the LHDAC data, we conducted in situ determination of pressure at high temperature using the Pt scale by Dorogokupets and Dewaele [2] at synchrotron. The measured temperatures of the triple point are in good agreement between LVP and LHDAC at 1990–2000 K. However, the pressure for the triple point determined from the LVP is 3.9±0.6 GPa lower than that from the LHDAC dataset. The triple point determined through these experiments will provide an important reference point in the pressure-temperature space for future high-pressure experiments and allow mineral physicists to compare the pressure–temperature conditions measured in these two different experimental methods. Keywords: triple point; bridgmanite; akimotoite; majorite; large-volume press; laser-heated diamond anvil cell 1. -
Continental Flood Basalts Derived from the Hydrous Mantle Transition Zone
ARTICLE Received 4 Sep 2014 | Accepted 1 Jun 2015 | Published 14 Jul 2015 DOI: 10.1038/ncomms8700 Continental flood basalts derived from the hydrous mantle transition zone Xuan-Ce Wang1, Simon A. Wilde1, Qiu-Li Li2 & Ya-Nan Yang2 It has previously been postulated that the Earth’s hydrous mantle transition zone may play a key role in intraplate magmatism, but no confirmatory evidence has been reported. Here we demonstrate that hydrothermally altered subducted oceanic crust was involved in generating the late Cenozoic Chifeng continental flood basalts of East Asia. This study combines oxygen isotopes with conventional geochemistry to provide evidence for an origin in the hydrous mantle transition zone. These observations lead us to propose an alternative thermochemical model, whereby slab-triggered wet upwelling produces large volumes of melt that may rise from the hydrous mantle transition zone. This model explains the lack of pre-magmatic lithospheric extension or a hotspot track and also the arc-like signatures observed in some large-scale intracontinental magmas. Deep-Earth water cycling, linked to cold subduction, slab stagnation, wet mantle upwelling and assembly/breakup of supercontinents, can potentially account for the chemical diversity of many continental flood basalts. 1 ARC Centre of Excellence for Core to Crust Fluid Systems (CCFS), The Institute for Geoscience Research (TIGeR), Department of Applied Geology, Curtin University, GPO Box U1987, Perth, Western Australia 6845, Australia. 2 State Key Laboratory of Lithospheric Evolution, Institute of Geology and Geophysics, Chinese Academy of Sciences, P.O.Box9825, Beijing 100029, China. Correspondence and requests for materials should be addressed to X.-C.W. -
Scientific Research of the Sco Countries: Synergy and Integration 上合组织国家的科学研究:协同和一体化
SCIENTIFIC RESEARCH OF THE SCO COUNTRIES: SYNERGY AND INTEGRATION 上合组织国家的科学研究:协同和一体化 Materials of the Date: International Conference November 19 Beijing, China 2019 上合组织国家的科学研究:协同和一体化 国际会议 参与者的英文报告 International Conference “Scientific research of the SCO countries: synergy and integration” Part 1: Participants’ reports in English 2019年11月19日。中国北京 November 19, 2019. Beijing, PRC Materials of the International Conference “Scientific research of the SCO countries: synergy and integration”. Part 1 - Reports in English (November 19, 2019. Beijing, PRC) ISBN 978-5-905695-74-2 这些会议文集结合了会议的材料 - 研究论文和科学工作 者的论文报告。 它考察了职业化人格的技术和社会学问题。 一些文章涉及人格职业化研究问题的理论和方法论方法和原 则。 作者对所引用的出版物,事实,数字,引用,统计数据,专 有名称和其他信息的准确性负责 These Conference Proceedings combine materials of the conference – research papers and thesis reports of scientific workers. They examines tecnical and sociological issues of research issues. Some articles deal with theoretical and methodological approaches and principles of research questions of personality professionalization. Authors are responsible for the accuracy of cited publications, facts, figures, quotations, statistics, proper names and other information. ISBN 978-5-905695-74-2 © Scientific publishing house Infinity, 2019 © Group of authors, 2019 CONTENTS ECONOMICS 可再生能源发展的现状与前景 Current state and prospects of renewable energy sources development Linnik Vladimir Yurievich, Linnik Yuri Nikolaevich...........................................12 JURISPRUDENCE 法律领域的未命名合同 Unnamed contracts in the legal field Askarov Nosirjon Ibragimovich...........................................................................19 -
INTERIOR of the EARTH / an El/EMEI^TARY Xdescrrpntion
N \ N I 1i/ / ' /' \ \ 1/ / / s v N N I ' / ' f , / X GEOLOGICAL SURVEY CIRCULAR 532 / N X \ i INTERIOR OF THE EARTH / AN El/EMEI^TARY xDESCRrPNTION The Interior of the Earth An Elementary Description By Eugene C. Robertson GEOLOGICAL SURVEY CIRCULAR 532 Washington 1966 United States Department of the Interior CECIL D. ANDRUS, Secretary Geological Survey H. William Menard, Director First printing 1966 Second printing 1967 Third printing 1969 Fourth printing 1970 Fifth printing 1972 Sixth printing 1976 Seventh printing 1980 Free on application to Branch of Distribution, U.S. Geological Survey 1200 South Eads Street, Arlington, VA 22202 CONTENTS Page Abstract ......................................................... 1 Introduction ..................................................... 1 Surface observations .............................................. 1 Openings underground in various rocks .......................... 2 Diamond pipes and salt domes .................................. 3 The crust ............................................... f ........ 4 Earthquakes and the earth's crust ............................... 4 Oceanic and continental crust .................................. 5 The mantle ...................................................... 7 The core ......................................................... 8 Earth and moon .................................................. 9 Questions and answers ............................................. 9 Suggested reading ................................................ 10 ILLUSTRATIONS -
The Upper Mantle and Transition Zone
The Upper Mantle and Transition Zone Daniel J. Frost* DOI: 10.2113/GSELEMENTS.4.3.171 he upper mantle is the source of almost all magmas. It contains major body wave velocity structure, such as PREM (preliminary reference transitions in rheological and thermal behaviour that control the character Earth model) (e.g. Dziewonski and Tof plate tectonics and the style of mantle dynamics. Essential parameters Anderson 1981). in any model to describe these phenomena are the mantle’s compositional The transition zone, between 410 and thermal structure. Most samples of the mantle come from the lithosphere. and 660 km, is an excellent region Although the composition of the underlying asthenospheric mantle can be to perform such a comparison estimated, this is made difficult by the fact that this part of the mantle partially because it is free of the complex thermal and chemical structure melts and differentiates before samples ever reach the surface. The composition imparted on the shallow mantle by and conditions in the mantle at depths significantly below the lithosphere must the lithosphere and melting be interpreted from geophysical observations combined with experimental processes. It contains a number of seismic discontinuities—sharp jumps data on mineral and rock properties. Fortunately, the transition zone, which in seismic velocity, that are gener- extends from approximately 410 to 660 km, has a number of characteristic ally accepted to arise from mineral globally observed seismic properties that should ultimately place essential phase transformations (Agee 1998). These discontinuities have certain constraints on the compositional and thermal state of the mantle. features that correlate directly with characteristics of the mineral trans- KEYWORDS: seismic discontinuity, phase transformation, pyrolite, wadsleyite, ringwoodite formations, such as the proportions of the transforming minerals and the temperature at the discontinu- INTRODUCTION ity. -
Subduction-Transition Zone Interaction: a Review
Research Paper THEMED ISSUE: Subduction Top to Bottom 2 GEOSPHERE Subduction-transition zone interaction: A review Saskia Goes1, Roberto Agrusta1,2, Jeroen van Hunen2, and Fanny Garel3 1Department of Earth Science & Engineering, Royal School of Mines, Imperial College, London SW7 2AZ, UK GEOSPHERE; v. 13, no. 3 2Department of Earth Sciences, Durham University, Science Labs, Durham DH1 3LE, UK 3Géosciences Montpellier, Université de Montpellier, Centre national de la recherche scientifique (CNRS), 34095 Montpellier cedex 05, France doi:10.1130/GES01476.1 9 figures ABSTRACT do not; (2) on what time scales slabs are stagnant in the transition zone if they have flattened; (3) how slab-transition zone interaction is reflected in plate mo- CORRESPONDENCE: s .goes@ imperial .ac .uk As subducting plates reach the base of the upper mantle, some appear tions; and (4) how lower-mantle fast seismic anomalies can be correlated with to flatten and stagnate, while others seemingly go through unimpeded. This past subduction. CITATION: Goes, S., Agrusta, R., van Hunen, J., variable resistance to slab sinking has been proposed to affect long-term ther- Over the past 20 years since the last Subduction Top to Bottom volume and and Garel, F., 2017, Subduction-transition zone inter- action: A review: Geosphere, v. 13, no. 3, p. 1– mal and chemical mantle circulation. A review of observational constraints several reviews of subduction through the transition zone (Lay, 1994; Chris- 21, doi:10.1130/GES01476.1. and dynamic models highlights that neither the increase in viscosity between tensen, 2001; King, 2001; Billen, 2008; Fukao et al., 2009), information about upper and lower mantle (likely by a factor 20–50) nor the coincident endo- the nature of the transition zone and our understanding of how slabs dynami- Received 6 December 2016 thermic phase transition in the main mantle silicates (with a likely Clapeyron cally interact with it has increased substantially. -
The Nakhlite Meteorites: Augite-Rich Igneous Rocks from Mars ARTICLE
ARTICLE IN PRESS Chemie der Erde 65 (2005) 203–270 www.elsevier.de/chemer INVITED REVIEW The nakhlite meteorites: Augite-rich igneous rocks from Mars Allan H. Treiman Lunar and Planetary Institute, 3600 Bay Area Boulevard, Houston, TX 77058-1113, USA Received 22 October 2004; accepted 18 January 2005 Abstract The seven nakhlite meteorites are augite-rich igneous rocks that formed in flows or shallow intrusions of basaltic magma on Mars. They consist of euhedral to subhedral crystals of augite and olivine (to 1 cm long) in fine-grained mesostases. The augite crystals have homogeneous cores of Mg0 ¼ 63% and rims that are normally zoned to iron enrichment. The core–rim zoning is cut by iron-enriched zones along fractures and is replaced locally by ferroan low-Ca pyroxene. The core compositions of the olivines vary inversely with the steepness of their rim zoning – sharp rim zoning goes with the most magnesian cores (Mg0 ¼ 42%), homogeneous olivines are the most ferroan. The olivine and augite crystals contain multiphase inclusions representing trapped magma. Among the olivine and augite crystals is mesostasis, composed principally of plagioclase and/or glass, with euhedra of titanomagnetite and many minor minerals. Olivine and mesostasis glass are partially replaced by veinlets and patches of iddingsite, a mixture of smectite clays, iron oxy-hydroxides and carbonate minerals. In the mesostasis are rare patches of a salt alteration assemblage: halite, siderite, and anhydrite/ gypsum. The nakhlites are little shocked, but have been affected chemically and biologically by their residence on Earth. Differences among the chemical compositions of the nakhlites can be ascribed mostly to different proportions of augite, olivine, and mesostasis. -
Cleavage Induced Akimotoite Transformation in Shocked Chondrites
Modern Analytical Methods I (2014) 4009.pdf CLEAVAGE INDUCED AKIMOTOITE TRANSFORMATION IN SHOCKED CHONDRITES. SZ. Nagy 1, I. Gyollai 2, A. Gucsik 3, SZ. Bérczi 4 1Szeged University, Department of Mineralogy, Geochemistry and Petrology, Egyetem u. 2-4., 6720 Szeged, Hunga- ry. 2Geochemical Research Institute, Budaörsi út 45., 1112 Budapest, Hungary. 3MTA Konkoly-Thege Miklós Astronomical Research Institute, Konkoly-Thege Miklós út 15-17., 1121 Budapest, Hungary. 4Eötvös Lorand University, Department of Material Physics, Pázmány Péter sétány 1/A, 1117 Budapest, Hungary. Introduction: Shock-events by asteroidal colli- very high melting point (2450 °C) of oldhamite infers sions may cause the effect of high-pressure metamor- its formation as an early nebular condensate. In the phism on the mineral assemblages [1]. The low-Ca shocked chondrites the oldhamite phase has been pro- pyroxene can transform to its high-pressure phases duced by shock vein formation. The present of the old- including the followings of jadeite, majorite-pyrope ss , hamite is an evidence for the very high-temperature majorite, akimotoite, Mg-perovskite and pyroxene condition during the shock-vein formation rather that glass depending on the shock-metamorphic conditions. supposed in earlier work [2]. A mixed-type pyroxene In this study we have examined a new microstructure chondrule (~1 mm in diameter) contains a number of form of akimotoite in NWA 5011 meteorite to clarify subchondrules observed in the sample. One of the sub- pyroxene-akimotoite phase transformation during chondrules exhibits a dense cleavage network, where shock-metamorphism. the angle between two directions of the cleavages is nearly perpendicular (87 °) (Fig.