Stability of hydrous silicate at high pressures and water transport to the deep lower mantle

Size: px
Start display at page:

Download "Stability of hydrous silicate at high pressures and water transport to the deep lower mantle"

Transcription

1 Stability of hydrous silicate at high pressures and water transport to the deep lower mantle Supplementary Figure 1: Compositions of dense hydrous magnesium silicates on the H2O-MgO-SiO2 diagram. PhH, phase H; PhD, phase D; PhA, phase A; shb super hydrous phase B; Pv, MgSiO3 perovskite. DHMSs phases A G and superhydrous phase B have been reported 8. However, phase F and phase G were found to be identical to phase D 27, and it has been common practice that these three phases are called phase D. We named the new DHMS phase discovered here phase H to avoid possible confusion, as the names phase F and phase G were already used elsewhere, although these phases do not actually exist. NATURE GEOSCIENCE 1

2 Supplementary Figure 2: X-ray diffraction patterns of phase H at 42.0 GPa and 1000 C. The diffraction peaks were obtained by assuming orthorhombic symmetry with a space group P21nm (red lines), and cell parameters with theoretically predicted monoclinic symmetry (sub blue lines) are shown for comparison. PhH, phase H; St, stishovite; Br, brucite; Pe, periclase; D, phase D; *, Characteristic lines of Au (67.0 kev and 68.9 kev) and La (33.0 kev, 33.4 kev, and 37.8 kev). 2 NATURE GEOSCIENCE

3 SUPPLEMENTARY INFORMATION Supplementary Figure 3: Plots of Si and Mg against Al, based on 4 Oxygens showing the Tschermak substitution between phase H and -AlOOH (Si 4+ + M g2+ 2Al 3+ ). NATURE GEOSCIENCE 3

4 Supplementary Figure 4: Cross-sections of the sample assemblages used for quench experiments and in situ X-ray diffraction measurements. 4 NATURE GEOSCIENCE

5 SUPPLEMENTARY INFORMATION Supplementary Table 1: Experimental conditions and run products Run No. Mg(OH) 2 :SiO 2 : P (GPa) T ( C) t (hour) Run products in-situ, MgSiH 2 O 4 (Ph H) M : PhH M : PhH, Br*, St* quench, MgSi 1.5 H 2 O 5 (Ph D) MII193D 1 : PhD, Pe* MII197D 1 : Pv, St, Br, fluid MII213D 1 : PhD, PhH, St MII198D 1 : Pv, St, fluid MII203D 1 : PhH, St MII196D 1 : Pv, St, fluid quench, MgSiH 2 O 4 (Ph H) MII193H 1 : PhD, Br, Pe MII204H 1 : PhD, Br, Pv, fluid MII201H 1 : PhH, Pv* MII198H 1 : Pv, fluid MII199H 1 : PhH, Pe*, Pv* PhH, phase H; PhD, phase D; St, Stishovite; Br, Brucite; Pv, perovskite; *, trace amount. NATURE GEOSCIENCE 5

6 Supplementary Table 2: Experimental conditions and chemical compositions of phase H, phase D, and MgSiO 3 perovskite in the system Mg(OH) 2 -SiO 2 -Al 2 O 3 Run No. P (GPa) T ( C) Run products (chemical compositions) Partition MII214A 1) H ( Mg 0.49 Al 0.77 Si 0.58 H 2.4 O 4 ), Pv ( Mg 0.9 Al 0.16 Si 0.93 O 3 ) Al H /Al Pv = ~3.6 MII213A 2) H ( Mg 0.60 Al 0.71 Si 0.65 H 2.1 O 4 ), Pe*, St* MII199A 3) H ( Mg 0.26 Al 1.24 Si 0.33 H 2.4 O 4 ), D ( Mg 0.77 Al 0.27 Si 1.08 H 3.3 O 5 ), St Al H /Al D = ~6 The solubility of -AlOOH into phase H was investigated using the starting materials with various amounts of Al 2 O 3 added to the mixtures of Mg(OH) 2 and SiO 2. We confirmed that phase H can accommodate the -AlOOH component up to ~70 %. It is also found that alumina can be strongly partitioned into phase H relative to MgSiO 3 perovskite and phase D. Starting compositions: 1, 2) Mg(OH) 2 : SiO 2 : Al 2 O 3 = 1 : 1 : 1, 3) Mg(OH) 2 : SiO 2 : Al 2 O 3 = 1 : 2 : 0.5. Heating durations were 3-9 hours. H, aluminous phase H; D, aluminous phase D; Pv, MgSiO 3 perovskite; St, Stishovite; Pv, perovskite; *, trace amount; Al H, mol fraction of Al in aluminous phase H; Al D, mol fraction of Al in aluminous phase D; Al Pv, mol fraction of Al in perovskite. 6 NATURE GEOSCIENCE

7 SUPPLEMENTARY INFORMATION Supplementary Notes: X-ray diffraction pattern of phase H A clear X-ray profile of phase H at ambient conditions was only obtained immediately after pressure release (Fig. 3E), and the diffraction peaks weakened with time after retrieval from the high-pressure cell. Moreover, attempts to observe the electron diffraction pattern with a transmission electron microscope failed because of rapid amorphization of the sample during observations. Formation of phase H in the subducting plates Phase H should be formed by the reaction of phase D and MgO periclase somewhere between ~33 and 48 GPa if MgO-saturated systems such as pyrolite are assumed, while the direct transformation of phase D to phase H plus stishovite is expected to occur at pressures of ~48 GPa in MgO-undersaturated systems such as oceanic and continental crusts, which are more relevant to the present composition (A). Supplementary references: 28. Liu, L. Irifune, T. Comment on A new hydrous silicate, a water reservoir, in the upper part of the lower mantle by Eiji Ohtani, Hiroki Mizobata, Yasuhiro Kudoh, Toshiro Nagase, Haruo Arashi, Hisayoshi Yurimoto, and Isoji Miyagi. Geophy. Res. Lett. 25, 979 (1998). NATURE GEOSCIENCE 7

Effect of water on the spinel-postspinel transformation in Mg 2 SiO 4

Effect of water on the spinel-postspinel transformation in Mg 2 SiO 4 Effect of water on the spinel-postspinel transformation in Mg 2 SiO 4 * Pressures for spinel postspinel phase boundary has been subject of debate - XRD measurements indicates that the transition pressure

More information

Petrogenetic grid in the system MgO-SiO 2 -H 2 O up to 30 GPa, 1600 C: Applications to hydrous peridotite subducting into the Earth s deep interior

Petrogenetic grid in the system MgO-SiO 2 -H 2 O up to 30 GPa, 1600 C: Applications to hydrous peridotite subducting into the Earth s deep interior JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 109,, doi:10.1029/2003jb002651, 2004 Petrogenetic grid in the system MgO-SiO 2 -H 2 O up to 30 GPa, 1600 C: Applications to hydrous peridotite subducting into the

More information

Physics of the Earth and Planetary Interiors

Physics of the Earth and Planetary Interiors Physics of the Earth and Planetary Interiors 175 (2009) 106 114 Contents lists available at ScienceDirect Physics of the Earth and Planetary Interiors journal homepage: www.elsevier.com/locate/pepi High-pressure

More information

GSA DATA REPOSITORY

GSA DATA REPOSITORY GSA DATA REPOSITORY 2013019 Supplemental information for The Solidus of Alkaline Carbonatite in the Deep Mantle Konstantin D. Litasov, Anton Shatskiy, Eiji Ohtani, and Gregory M. Yaxley EXPERIMENTAL METHODS

More information

Interpreting Geophysical Data for Mantle Dynamics. Wendy Panero University of Michigan

Interpreting Geophysical Data for Mantle Dynamics. Wendy Panero University of Michigan Interpreting Geophysical Data for Mantle Dynamics Wendy Panero University of Michigan Chemical Constraints on Density Distribution Atomic Fraction 1.0 0.8 0.6 0.4 opx cpx C2/c garnet il olivine wadsleyite

More information

Revision 4. A Possible New Al-bearing Hydrous Mg-silicate (23 Å phase) in. the Deep Upper Mantle

Revision 4. A Possible New Al-bearing Hydrous Mg-silicate (23 Å phase) in. the Deep Upper Mantle 1 Revision 4 2 3 A Possible New Al-bearing Hydrous Mg-silicate (23 Å phase) in the Deep Upper Mantle 4 5 Nao CAI 1*, Toru INOUE 1, Kiyoshi FUJINO 1, Hiroaki OHFUJI 1, Hisayoshi YURIMOTO 2 6 7 1 Geodynamics

More information

NMR in Mineralogy. Sharon Ashbrook School of Chemistry, University of St Andrews

NMR in Mineralogy. Sharon Ashbrook School of Chemistry, University of St Andrews NMR in Mineralogy Sharon Ashbrook School of Chemistry, University of St Andrews Structure of the Earth Study of minerals is important for determining the physical and chemical properties of the Earth O

More information

Phase Transitions in the Lowermost Mantle

Phase Transitions in the Lowermost Mantle Phase Transitions in the Lowermost Mantle S.-H. Dan Shim 1, B. Grocholski 2, K. Catalli 3, and V. Prakapenka 4 1 Arizona State University, 2 Smithsonian Institution, 3 Livermore National Lab 4 University

More information

SUPPLEMENTARY INFORMATION

SUPPLEMENTARY INFORMATION SUPPLEMENTARY INFORMATION doi:10.1038/nature11294 Review of previous works on deep-liquid properties The major parameters controlling the buoyancy of deep-mantle melts are (i) the changes in atomic packing

More information

Fluids, melts, and supercriticality in the MSH system and element transport in subduction zones

Fluids, melts, and supercriticality in the MSH system and element transport in subduction zones cosmic rays Fluids, s, and supercriticality in the MSH system and element transport in subduction zones 10 Be volcanic front N, O 10 Be ocean water + CO 2 tracing petrologic and geotectonic processes (trace)

More information

Hydration of Olivine and. Earth s Deep Water Cycle

Hydration of Olivine and. Earth s Deep Water Cycle Hydration of Olivine and Earth s Deep Water Cycle IASPEI October 5, 2005 Olivine Hydration and Earth s Deep Water Cycle J. R. Smyth, (University of Colorado) Dan Frost and Fabrizio Nestola (Bayerisches

More information

Description of Supplementary Files

Description of Supplementary Files Description of Supplementary Files File Name: Supplementary Information Description: Supplementary Figures, Supplementary Tables and Supplementary References File Name: Peer Review File Supplementary figure

More information

Why cold slabs stagnate in the transition zone

Why cold slabs stagnate in the transition zone GSA Data Repository 2015085 Model 1 Model 2 Model 3 Model 4 Model 5 Model 6 Why cold slabs stagnate in the transition zone Scott D. King 1,2, Daniel J. Frost 2, and David C. Rubie 2 1 Department of Geosciences,

More information

Mantle-wide sequestration of carbon in silicates and the structure of magnesite II

Mantle-wide sequestration of carbon in silicates and the structure of magnesite II GEOPHYSICAL RESEARCH LETTERS, VOL. 35, L14307, doi:10.1029/2008gl034442, 2008 Mantle-wide sequestration of carbon in silicates and the structure of magnesite II Wendy R. Panero 1 and Jason E. Kabbes 1

More information

Deep and persistent melt layer in the Archaean mantle

Deep and persistent melt layer in the Archaean mantle SUPPLEMENTARY INFORMATION Articles https://doi.org/10.1038/s41561-017-0053-9 In the format provided by the authors and unedited. Deep and persistent melt layer in the Archaean mantle Denis Andrault 1 *,

More information

phase H in deep subducted oceanic crust

phase H in deep subducted oceanic crust 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 Revision 3 Stability of the hydrous phases of Al-rich phase D and Al-rich phase H in deep subducted oceanic crust Xingcheng Liu 12*, Kyoko N. Matsukage

More information

Post-perovskite 1. Galley Proofs

Post-perovskite 1. Galley Proofs 16 September 2005 21:39 YB061180.tex McGraw Hill YB of Science & Technology Keystroked: 29/08/2005 Initial MS Page Sequence Stamp: 02350 Article Title: Post-perovskite Article ID: YB061180 1st Classification

More information

Subsolidus and melting experiments of a K-rich basaltic composition to 27 GPa: Implication for the behavior of potassium in the mantle

Subsolidus and melting experiments of a K-rich basaltic composition to 27 GPa: Implication for the behavior of potassium in the mantle American Mineralogist, Volume 84, pages 357 361, 1999 Subsolidus and melting experiments of a K-rich basaltic composition to 27 GPa: Implication for the behavior of potassium in the mantle WUYI WANG* AND

More information

doi: /nature09369

doi: /nature09369 doi:10.1038/nature09369 Supplementary Figure S1 Scanning electron microscope images of experimental charges with vapour and vapour phase quench. Experimental runs are in the order of added water concentration

More information

The role of Al-defects on the equation of state of Al (Mg,Fe)SiO 3 perovskite

The role of Al-defects on the equation of state of Al (Mg,Fe)SiO 3 perovskite Available online at www.sciencedirect.com Earth and Planetary Science Letters 263 (2007) 167 179 www.elsevier.com/locate/epsl The role of Al-defects on the equation of state of Al (Mg,Fe)SiO 3 perovskite

More information

Trace element partitioning between silicate perovskites and ultracalcic melt

Trace element partitioning between silicate perovskites and ultracalcic melt Physics of the Earth and Planetary Interiors 124 (2001) 25 32 Trace element partitioning between silicate perovskites and ultracalcic melt Hiroshi Taura a,1, Hisayoshi Yurimoto b,, Takumi Kato c,2, Shigeho

More information

Absence of density crossover between basalt and peridotite in the cold slabs passing through 660 km discontinuity

Absence of density crossover between basalt and peridotite in the cold slabs passing through 660 km discontinuity GEOPHYSICAL RESEARCH LETTERS, VOL. 31, L24607, doi:10.1029/2004gl021306, 2004 Absence of density crossover between basalt and peridotite in the cold slabs passing through 660 km discontinuity Konstantin

More information

WATER IN THE EARTH S MANTLE:

WATER IN THE EARTH S MANTLE: WATER IN THE EARTH S MANTLE: NATHALIE BOLFAN-CASANOVA LABORATOIRE MAGMAS ET VOLCANS => Heterogeneous distribution of water in the mantle > 10000 pmm wt H2O ~ 10000 pmm wt H2O ~ 1000 pmm wt H2O On what

More information

The Effect of H 2 O on the 410-km Seismic Discontinuity

The Effect of H 2 O on the 410-km Seismic Discontinuity The Effect of H 2 O on the 410-km Seismic Discontinuity B.J. Wood Science Paper (1995) Presented by HuajianYao Background Seismic discontinuities at 410 km and 660 km ------ important jumps in mantle density

More information

Sorosilicates, Colors in Minerals (cont), and Deep Earth Minerals. ESS212 January 20, 2006

Sorosilicates, Colors in Minerals (cont), and Deep Earth Minerals. ESS212 January 20, 2006 Sorosilicates, Colors in Minerals (cont), and Deep Earth Minerals ESS212 January 20, 2006 Double tetrahedron Sorosilicate is defined by the Si 2 O 7 group. Three groups of minerals, commonly, Epidote Zoisite

More information

α phase In the lower mantle, dominant mineralogy is perovskite [(Mg,Fe)SiO 3 ] The pyrolite mantle consists of: 60% olivine and 40% pyroxene.

α phase In the lower mantle, dominant mineralogy is perovskite [(Mg,Fe)SiO 3 ] The pyrolite mantle consists of: 60% olivine and 40% pyroxene. Summary of Dan Shim s lecture on 3/1/05 Phase transitions in the Earth s mantle In this lecture, we focused on phase transitions associated with the transition zone 1. 410 km alpha olivine beta wadsleyite

More information

doi: /nature09940

doi: /nature09940 LETTER doi:10.1038/nature09940 Spin crossover and iron-rich silicate melt in the Earth s deep mantle Ryuichi Nomura 1,2, Haruka Ozawa 1,3, Shigehiko Tateno 1, Kei Hirose 1,3, John Hernlund 4, Shunsuke

More information

Chemical Composition of the Lower Mantle: Constraints from Elasticity. Motohiko Murakami Tohoku University

Chemical Composition of the Lower Mantle: Constraints from Elasticity. Motohiko Murakami Tohoku University Chemical Composition of the Lower Mantle: Constraints from Elasticity Motohiko Murakami Tohoku University Acknowledgements Jay D. Bass (University of Illinois) Stanislav V. Sinogeikin (University of Illinois)

More information

Plate Tectonics. Why Continents and Ocean Basins Exist

Plate Tectonics. Why Continents and Ocean Basins Exist Plate Tectonics Plate Tectonics Why Continents and Ocean Basins Exist Topics Density Structure of Earth Isostasy Sea-Floor Spreading Mechanical Structure of Earth Driving Mechanism of Plate Tectonics Lithospheric

More information

University of Bristol - Explore Bristol Research. Peer reviewed version. Link to published version (if available): /j.epsl

University of Bristol - Explore Bristol Research. Peer reviewed version. Link to published version (if available): /j.epsl Walter, M. J., Tronnes, R. G., Armstrong, L. S., Lord, O. T., Caldwell, W. A., & Clark, S. M. (2006). Subsolidus phase relations and perovskite compressibility in the system MgO AlO1.5 SiO2 with implications

More information

Laboratory Electrical Conductivity Measurement of Mantle Minerals

Laboratory Electrical Conductivity Measurement of Mantle Minerals Laboratory Electrical Conductivity Measurement of Mantle Minerals Takashi Yoshino Institute for Study of the Earth s Interior, Okayama University Outline 1. Brief introduction 2. Conduction mechanisms

More information

Phase relations and equation of state of a natural MORB: Implications for the density profile of subducted oceanic crust in the Earth s lower mantle

Phase relations and equation of state of a natural MORB: Implications for the density profile of subducted oceanic crust in the Earth s lower mantle JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 115,, doi:10.1029/2009jb006709, 2010 Phase relations and equation of state of a natural MORB: Implications for the density profile of subducted oceanic crust in the

More information

Introduction. Geoffrey D. Bromiley Æ Alison R. Pawley

Introduction. Geoffrey D. Bromiley Æ Alison R. Pawley Contrib Mineral Petrol (2002) 142: 714 723 DOI 10.1007/s00410-001-0318-5 Geoffrey D. Bromiley Æ Alison R. Pawley The high-pressure stability of Mg-sursassite in a model hydrous peridotite: a possible mechanism

More information

Pressure Volume Temperature Equation of State

Pressure Volume Temperature Equation of State Pressure Volume Temperature Equation of State S.-H. Dan Shim ( ) Acknowledgement: NSF-CSEDI, NSF-FESD, NSF-EAR, NASA-NExSS, Keck Equations relating state variables (pressure, temperature, volume, or energy).

More information

Determination of the hyperfine parameters of iron in aluminous (Mg,Fe)SiO 3 perovskite

Determination of the hyperfine parameters of iron in aluminous (Mg,Fe)SiO 3 perovskite Determination of the hyperfine parameters of iron in aluminous (Mg,Fe)SiO 3 perovskite Jennifer M. Jackson Seismological Laboratory, Geological & Planetary Sciences California Institute of Technology VLab

More information

Elasticity of single crystal and polycrystalline MgSiO 3 perovskite by Brillouin spectroscopy

Elasticity of single crystal and polycrystalline MgSiO 3 perovskite by Brillouin spectroscopy GEOPHYSICAL RESEARCH LETTERS, VOL. 31, L06620, doi:10.1029/2004gl019559, 2004 Elasticity of single crystal and polycrystalline MgSiO 3 perovskite by Brillouin spectroscopy Stanislav V. Sinogeikin Department

More information

Geos 306, Mineralogy Final Exam, Dec 12, pts

Geos 306, Mineralogy Final Exam, Dec 12, pts Name: Geos 306, Mineralogy Final Exam, Dec 12, 2014 200 pts 1. (9 pts) What are the 4 most abundant elements found in the Earth and what are their atomic abundances? Create a reasonable hypothetical charge-balanced

More information

N = N 0 e -λt D* = N 0 -N D* = N 0 (1-e -λt ) or N(e λt -1) where N is number of parent atoms at time t, N 0

N = N 0 e -λt D* = N 0 -N D* = N 0 (1-e -λt ) or N(e λt -1) where N is number of parent atoms at time t, N 0 N = N 0 e -λt D* = N 0 -N D* = N 0 (1-e -λt ) or N(e λt -1) where N is number of parent atoms at time t, N 0 is initial number of parents, D* is number of radiogenic daughter atoms, and λ is the decay

More information

Synthesis of high-pressure hydrous magnesium silicates: Observations and analysis

Synthesis of high-pressure hydrous magnesium silicates: Observations and analysis American Mineralogist, Volume 81, pages 317-326, 1996 Synthesis of high-pressure hydrous magnesium silicates: Observations and analysis PAMELA C. BURNLEY. AND ALEXANDRA NA VROTSKY Center for High Pressure

More information

The primitive nature of large low shear-wave velocity provinces

The primitive nature of large low shear-wave velocity provinces The primitive nature of large low shear-wave velocity provinces Frédéric Deschamps 1, Laura Cobden 3, and Paul J. Tackley 2 1 Institute of Earth Sciences, Academia Sinica, 128 Academia Road Sec. 2, Nangang,

More information

T-X Diagrams C:\Courses\320\fall2007\in class\5000-t-x Exercise.wpd; September 25, 2003 (11:45am)

T-X Diagrams C:\Courses\320\fall2007\in class\5000-t-x Exercise.wpd; September 25, 2003 (11:45am) 1 T-X Diagrams C:\Courses\320\fall2007\in class\5000-t-x Exercise.wpd; September 25, 2003 (11:45am) T-X diagrams are most often used for describing metamorphism of carbonate-rich rocks (marbles or marls)

More information

Constitution of Magmas. Magmas. Gas Law. Composition. Atomic Structure of Magma. Structural Model. PV = nrt H 2 O + O -2 = 2(OH) -

Constitution of Magmas. Magmas. Gas Law. Composition. Atomic Structure of Magma. Structural Model. PV = nrt H 2 O + O -2 = 2(OH) - Constitution of Magmas Magmas Best, Ch. 8 Hot molten rock T = 700-1200 degrees C Composed of ions or complexes Phase Homogeneous Separable part of the system With an interface Composition Most components

More information

Computational support for a pyrolitic lower mantle containing ferric iron

Computational support for a pyrolitic lower mantle containing ferric iron SUPPLEMENTARY INFORMATION DOI: 1.138/NGEO2458 Computational support for a pyrolitic lower mantle containing ferric iron Xianlong Wang, Taku Tsuchiya and Atsushi Hase NATURE GEOSCIENCE www.nature.com/naturegeoscience

More information

Weidner and Wang (1999) Phase transformations - implications for mantle structure

Weidner and Wang (1999) Phase transformations - implications for mantle structure Weidner and Wang (1999) Phase transformations - implications for mantle structure The Transition Zone Complex Interactions among Minerals in the Transition Zone Mg-Si-O Mg-Fe-Si-O Mg-Fe-Ca-Al-Si-O (this

More information

Defects, Diffusion, Deformation and Thermal Conductivity in the Lower Mantle and D

Defects, Diffusion, Deformation and Thermal Conductivity in the Lower Mantle and D Defects, Diffusion, Deformation and Thermal Conductivity in the Lower Mantle and D John Brodholt UCL Thanks to: Michael Ammann, Simon Hunt, James Wookey, Kai Wang, Andrew Walker and David Dobson College

More information

Nitrogen speciation in upper mantle fluids and the origin of Earth s nitrogen-rich atmosphere

Nitrogen speciation in upper mantle fluids and the origin of Earth s nitrogen-rich atmosphere Supporting Online Material for Nitrogen speciation in upper mantle fluids and the origin of Earth s nitrogen-rich atmosphere Sami Mikhail & Dimitri Sverjensky S1. Supplementary discussion S1.1 The selection

More information

Supplementary Materials for

Supplementary Materials for advances.sciencemag.org/cgi/content/full/2/3/e1501725/dc1 Supplementary Materials for Discovery of natural MgSiO3 tetragonal garnet in a shocked chondritic meteorite The PDF file includes: Naotaka Tomioka,

More information

PerovskitePhaseRelationsintheSystem CaO^MgO^TiO 2^SiO 2 and Implications for Deep Mantle Lithologies

PerovskitePhaseRelationsintheSystem CaO^MgO^TiO 2^SiO 2 and Implications for Deep Mantle Lithologies JOURNAL OF PETROLOGY VOLUME 53 NUMBER 3 PAGES611^635 2012 doi:10.1093/petrology/egr073 PerovskitePhaseRelationsintheSystem CaO^MgO^TiO 2^SiO 2 and Implications for Deep Mantle Lithologies L. S. ARMSTRONG

More information

Investigating Causes of D Anisotropy

Investigating Causes of D Anisotropy Investigating Causes of D Anisotropy J.-M. Kendall and P. G. Silver in: The Core-Mantle Boundary Region, AGU, 1998. MDL 3/15/04 Although most of the lower mantle (below 660km) appears to be isotropic,

More information

Layer Composition Thickness State of Matter

Layer Composition Thickness State of Matter Unit 4.2 Test Review Earth and Its Layers 1. Label the layers of the earth. oceanic crust continental crust lithosphere asthenosphere mantle outer core inner core 2. Complete the Following Table about

More information

First results of the UHV system 'LIFE' (Light Irradiation Facility for Exochemistry)

First results of the UHV system 'LIFE' (Light Irradiation Facility for Exochemistry) Osservatorio Astronomico di Palermo (INAF-OAPa) First results of the UHV system '' (Light Irradiation Facility for Exochemistry) Antonio Jimenez-Escobar Angela Ciaravella Cesare Cecchi-Pestellini Giuliana

More information

Chapter 7 Plate Tectonics

Chapter 7 Plate Tectonics Chapter 7 Plate Tectonics Earthquakes Earthquake = vibration of the Earth produced by the rapid release of energy. Seismic Waves Focus = the place within the Earth where the rock breaks, producing an earthquake.

More information

(4) Give an example of important reactions that are responsible for the composition of river water.

(4) Give an example of important reactions that are responsible for the composition of river water. Lecture 12 Global Biogeochemical Cycles (1) If rivers are the chief source of the dissolved salts in seawater, why is seawater not simply a concentrated version of average composition of all rivers? The

More information

Planetary Accretion Models and the

Planetary Accretion Models and the Planetary Accretion Models and the Mineralogy of Planetary Interiors DanFrost & DaveRubie Bayerisches Geoinstitut John Hernlund Earth Life Science Institute, Institute of TechnologyTokyo Alessandro Morbidelli

More information

Stability of MgSiO, Perovskite in the Lower Mantle

Stability of MgSiO, Perovskite in the Lower Mantle Stability of MgSiO, Perovskite in the Lower Mantle Sang-Heon Shim Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, Massachusetts As it is expected

More information

Cloud Condensation Chemistry. in Low-Mass Objects. Katharina Lodders Washington University, St. Louis

Cloud Condensation Chemistry. in Low-Mass Objects. Katharina Lodders Washington University, St. Louis Cloud Condensation Chemistry in Low-Mass Objects Katharina Lodders Washington University, St. Louis For a recent review on this topic, see Lodders & Fegley 2006, Astrophysics Update 2, Springer, p. 1 ff.

More information

Anderson RN, Uyeda S, Miyashiro A. (1976) Geophysical and geochemical constraints

Anderson RN, Uyeda S, Miyashiro A. (1976) Geophysical and geochemical constraints REFERENCES RELEVANT TO PERIDOTITE PARTIAL MELTING IN THE MANTLE WEDGE Anderson RN, Uyeda S, Miyashiro A. (1976) Geophysical and geochemical constraints at converging plate boundaries - I: Dehydration in

More information

Thermo-chemical structure, dynamics and evolution of the deep mantle: spherical convection calculations

Thermo-chemical structure, dynamics and evolution of the deep mantle: spherical convection calculations Thermo-chemical structure, dynamics and evolution of the deep mantle: spherical convection calculations Paul J. Tackley ETH Zürich, Switzerland With help from Takashi Nakagawa, Frédéric Deschamps, James

More information

SUPPLEMENTARY INFORMATION

SUPPLEMENTARY INFORMATION SUPPLEMENTARY INFORMATION Supplementary information: Our 1080 km x 360 km model setup includes a 7 km thick oceanic crust adjacent to a 60 km thick, 250 km wide orogenic crust. Both the oceanic and the

More information

High pressure crystal chemistry of hydrous ringwoodite and water in the Earth s interior

High pressure crystal chemistry of hydrous ringwoodite and water in the Earth s interior High pressure crystal chemistry of hydrous ringwoodite and water in the Earth s interior Joseph R. Smyth a, Christopher M. Holl a, Daniel J. Frost b, Steven D. Jacobsen b a Department of Geological Sciences,

More information

Equation of state of Ca 2 AlSiO 5.5 oxygen defect perovskite

Equation of state of Ca 2 AlSiO 5.5 oxygen defect perovskite Phys Chem Minerals (2015) 42:327 336 DOI 10.1007/s00269-014-0723-8 ORIGINAL PAPER Equation of state of Ca 2 AlSiO 5.5 oxygen defect perovskite Chaowen Xu Shuangmeng Zhai Lijin Ye Yuji Higo Received: 10

More information

High pressure crystal chemistry of hydrous ringwoodite and water in the Earth s interior

High pressure crystal chemistry of hydrous ringwoodite and water in the Earth s interior Physics of the Earth and Planetary Interiors xxx (2004) xxx xxx High pressure crystal chemistry of hydrous ringwoodite and water in the Earth s interior Joseph R. Smyth a,, Christopher M. Holl a, Daniel

More information

PY2N20 Material Properties and Phase Diagrams

PY2N20 Material Properties and Phase Diagrams PY2N20 Material Properties and Phase Diagrams Lecture 10 P. Stamenov, PhD School of Physics, TCD PY2N20-10 Modern CMOS pair structure Photolithographic Process CMOS Processing Steps Cu Damascene Process

More information

Along the center of the mid-ocean ridge is a rift valley that forms when the plates separate.

Along the center of the mid-ocean ridge is a rift valley that forms when the plates separate. Newly formed rock from rising magma rises above sea floor and forms mountain ranges known as midocean ridges. Along the center of the mid-ocean ridge is a rift valley that forms when the plates separate.

More information

How do we know about the different layers of Earth's interior when we've never been there?

How do we know about the different layers of Earth's interior when we've never been there? Layers of the Earth Layers of the Earth How do we know about the different layers of Earth's interior when we've never been there? Oct 11 6:41 AM Make a note: These layers are inferred based on seismic

More information

JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 117, B09205, doi: /2012jb009290, 2012

JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 117, B09205, doi: /2012jb009290, 2012 JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 117,, doi:10.1029/2012jb009290, 2012 High-P behavior of anorthite composition and some phase relations of the CaO-Al 2 O 3 -SiO 2 system to the lower mantle of the

More information

high and ultrahigh pressures.

high and ultrahigh pressures. Stability of hydrous phases in serpentinites to high and ultrahigh pressures. Study of fluid and multiphase solid inclusions in high, very high pressure rocks and metamorphic veins The crust to mantle

More information

University of Bristol - Explore Bristol Research

University of Bristol - Explore Bristol Research Armstrong, L. S., Walter, M. J., Tuff, J. R., Lord, O. T., Lennie, AR., Kleppe, AK., & Clark, SM. (). Perovskite Phase Relations in the System CaO MgO TiO SiO and Implications for Deep Mantle Lithologies.

More information

Continental Alkaline Magmatism. The East African Rift

Continental Alkaline Magmatism. The East African Rift Announcements No lecture on Friday Lab final begins at 1 PM Today s agenda: Lecture/Demo Go through field trip pics Call for pizza Lab review Lecture Review Make poster Continental Alkaline Magmatism.

More information

Imagine the first rock and the cycles that it has been through.

Imagine the first rock and the cycles that it has been through. A rock is a naturally formed, consolidated material usually composed of grains of one or more minerals The rock cycle shows how one type of rocky material gets transformed into another The Rock Cycle Representation

More information

Solubility of water in pyrope-rich garnet at high pressures and temperature

Solubility of water in pyrope-rich garnet at high pressures and temperature Click Here for Full Article GEOPHYSICAL RESEARCH LETTERS, VOL. 37, L03310, doi:10.1029/2009gl041289, 2010 Solubility of water in pyrope-rich garnet at high pressures and temperature Mainak Mookherjee 1

More information

THE INTERIOR OF THE EARTH

THE INTERIOR OF THE EARTH THE INTERIOR OF THE EARTH Introduction: Nebular hypothesis and the origin of solar system, which indicates that there is a differentiation (layering) in the earth. * Sources of our knowledge about the

More information

Mg/Si ratios of aqueous fluids coexisting with forsterite and enstatite based on the phase relations in the Mg 2 SiO 4 -SiO 2 -H 2 O system

Mg/Si ratios of aqueous fluids coexisting with forsterite and enstatite based on the phase relations in the Mg 2 SiO 4 -SiO 2 -H 2 O system American Mineralogist, Volume 89, pages 1433 1437, 2004 Mg/Si ratios of aqueous fluids coexisting with forsterite and enstatite based on the phase relations in the Mg 2 SiO 4 -SiO 2 -H 2 O system TATSUHIKO

More information

INVESTIGATION ON GEOTHERMAL DRILLING MUDS WITH HIGH TEMPERATURE STABILITY

INVESTIGATION ON GEOTHERMAL DRILLING MUDS WITH HIGH TEMPERATURE STABILITY INVESTIGATION ON GEOTHERMAL DRILLING MUDS WITH HIGH TEMPERATURE STABILITY Umran Serpen ITÜ, Petroleum and Natural Gas Eng. Dept., Maslak, 80626, Istanbul, Turkey Key Words: Drilling-mud, geothermal, sepiolite,

More information

Structural study of the coherent dehydration of wadsleyite

Structural study of the coherent dehydration of wadsleyite American Mineralogist, Volume 96, pages 1760 1767, 2011 Structural study of the coherent dehydration of wadsleyite YU YE, 1, * JOSEPH R. SMYTH, 2 AND DANIEL J. FROST 3 1 Department of Physics, University

More information

Supplementary Information

Supplementary Information Supplementary Information Materials and Experiments 57 Fe-enriched enstatite sample [(Mg 0.6,Fe 0.4 )SiO 3 ] was synthesized by mixing powders of the oxides SiO 2, MgO, and 57 Fe 2 O 3 (90% enrichment

More information

Supporting Information

Supporting Information Supporting Information Bindi et al. 10.1073/pnas.1111115109 Fig. S1. Electron microprobe X-ray elemental maps for the grain reported in Fig. 1B. Experimental details are given in Experimental Methods.

More information

Silicate Atmospheres, Clouds, and Fractional Vaporization of Hot Earth-like Exoplanets

Silicate Atmospheres, Clouds, and Fractional Vaporization of Hot Earth-like Exoplanets Silicate Atmospheres, Clouds, and Fractional Vaporization of Hot Earth-like Exoplanets Laura Schaefer and Bruce Fegley, Jr. Planetary Chemistry Laboratory Department of Earth and Planetary Sciences Washington

More information

Formation of the Hawaiian Islands. Volcanoes, Magma, and Hot Spots

Formation of the Hawaiian Islands. Volcanoes, Magma, and Hot Spots Formation of the Hawaiian Islands Volcanoes, Magma, and Hot Spots Topics Hawai i Ring of Fire Hot Spots Decompression Melting The Hawai i Hot Spot Topics Hawai i Ring of Fire Hot Spots Decompression Melting

More information

Synchrotron facilities and the study of the Earth s deep interior

Synchrotron facilities and the study of the Earth s deep interior INSTITUTE OF PHYSICS PUBLISHING Rep. Prog. Phys. 68 (2005) 1811 1859 REPORTS ON PROGRESS IN PHYSICS doi:10.1088/0034-4885/68/8/r03 Synchrotron facilities and the study of the Earth s deep interior Thomas

More information

American Mineralogist, Volume 84, pages , Department of Earth Sciences, University of Oxford, Parks Road, Oxford, OX1 3PR U.K.

American Mineralogist, Volume 84, pages , Department of Earth Sciences, University of Oxford, Parks Road, Oxford, OX1 3PR U.K. American Mineralogist, Volume 84, pages 214 220, 1999 High-resolution synchrotron X-ray powder diffraction and Rietveld structure refinement of two (Mg 0.95,Fe 0.05 )SiO 3 perovskite samples synthesized

More information

Thomas S. Duffy, Thomas J. Ahrens, and Manfred A. Lange 1

Thomas S. Duffy, Thomas J. Ahrens, and Manfred A. Lange 1 JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 96, NO. Bll, PAGES 18,011-18,027, OCTOBER 10, 1991 SHOCK WAVE EQUATION OF STATE OF SERPENTINE TO 150 GPA: IMPLICATIONS FOR THE OCCURRENCE OF WATER IN THE EARTH'S LOWER

More information

Mantle Dynamics and Geochemical Cycle: What can Ocean Drilling contribute?

Mantle Dynamics and Geochemical Cycle: What can Ocean Drilling contribute? Mantle Dynamics and Geochemical Cycle: What can Ocean Drilling contribute? Geochemical Cycle: input and output Subduction Factory Carbon Transfer at Deep Mantle Diamond in Oceanic Mantle? Carbon/Water

More information

Composition of the Earth and its reservoirs: Geochemical observables

Composition of the Earth and its reservoirs: Geochemical observables Composition of the Earth and its reservoirs: Geochemical observables Cin-Ty A. Lee Rice University MYRES-I 2004 The Earth is dynamic and heterogeneous Atmosphere Midocean Ridge Plume Ocean Crust Oceanic

More information

Supporting Information

Supporting Information Supporting Information Structural Evidence for Strong Coupling between Polarization Rotation and Lattice Strain in Monoclinic Relaxor Ferroelectrics Hui Liu, Jun Chen,*, Longlong Fan, Yang Ren, Lei Hu,

More information

Earth s Interior and Geophysical Properties. Chapter 13

Earth s Interior and Geophysical Properties. Chapter 13 Earth s Interior and Geophysical Properties Chapter 13 Introduction Can we just go there? Deep interior of the Earth must be studied indirectly Direct access only to crustal rocks and upper mantle fragments

More information

Partitioning of iron between magnesian silicate perovskite and magnesiowüstite at about 1 Mbar

Partitioning of iron between magnesian silicate perovskite and magnesiowüstite at about 1 Mbar Physics of the Earth and Planetary Interiors 131 (2002) 295 310 Partitioning of iron between magnesian silicate perovskite and magnesiowüstite at about 1 Mbar S.E. Kesson, J.D. Fitz Gerald, H.St.C. O Neill,

More information

Physics of the Earth and Planetary Interiors

Physics of the Earth and Planetary Interiors Physics of the Earth and Planetary Interiors 177 (2009) 103 115 Contents lists available at ScienceDirect Physics of the Earth and Planetary Interiors journal homepage: www.elsevier.com/locate/pepi Structure

More information

Earth and Planetary Science Letters

Earth and Planetary Science Letters Earth and Planetary Science Letters 434 (2016) 264 273 Contents lists available at ScienceDirect Earth and Planetary Science Letters www.elsevier.com/locate/epsl High-pressure, temperature elasticity of

More information

Cation sites in Al-rich MgSiO 3 perovskites

Cation sites in Al-rich MgSiO 3 perovskites American Mineralogist, Volume 83, pages 1045 1053, 1998 Cation sites in Al-rich MgSiO 3 perovskites D. ANDRAULT, 1, * D.R. NEUVILLE, 1 A.-M. FLANK, 2 AND Y. WANG 3 1 Laboratoire des Géomatériaux, IPGP,

More information

Ch 6: Internal Constitution of the Earth

Ch 6: Internal Constitution of the Earth Ch 6: Internal Constitution of the Earth Mantle composition Geological background 88 elements found in the Earth's crust -- of these, only 8 make up 98%: oxygen, silicon, aluminum, iron, calcium, magnesium,

More information

Chapter 12 Lecture. Earth: An Introduction to Physical Geology. Eleventh Edition. Earth s Interior. Tarbuck and Lutgens Pearson Education, Inc.

Chapter 12 Lecture. Earth: An Introduction to Physical Geology. Eleventh Edition. Earth s Interior. Tarbuck and Lutgens Pearson Education, Inc. Chapter 12 Lecture Earth: An Introduction to Physical Geology Eleventh Edition Earth s Interior Tarbuck and Lutgens Earth s Internal Structure Earth s interior can be divided into three major layers defined

More information

Structural, vibrational and thermodynamic properties of Mg 2 SiO 4 and MgSiO 3 minerals from first-principles simulations

Structural, vibrational and thermodynamic properties of Mg 2 SiO 4 and MgSiO 3 minerals from first-principles simulations 1 2 3 4 5 6 7 8 Structural, vibrational and thermodynamic properties of Mg 2 SiO 4 and MgSiO 3 minerals from first-principles simulations E. R. Hernández,a, J. Brodholt b, D. Alfè b a Instituto de Ciencia

More information

SUPPLEMENTARY INFORMATION

SUPPLEMENTARY INFORMATION SUPPLEMENTARY INFORMATION DOI: 10.1038/NGEO1250 Intensive hydration of the mantle transition zone beneath China caused by ancient slab stagnation Takeshi Kuritani 1,2 *, Eiji Ohtani 1, and Jun-Ichi Kimura

More information

Silicates. The most common group of minerals forming the silicate Earth

Silicates. The most common group of minerals forming the silicate Earth Silicates The most common group of minerals forming the silicate Earth 25% of all minerals (~1000) 40% of rock forming minerals 90% of earth s crust i.e those minerals you are likely to find ~100 of earth

More information

Carbon and other light element contents in the Earth s core based on first-principles molecular dynamics

Carbon and other light element contents in the Earth s core based on first-principles molecular dynamics Carbon and other light element contents in the Earth s core based on first-principles molecular dynamics Yigang Zhang a and Qing-Zhu Yin b,1 a Key Laboratory of the Earth s Deep Interior, Institute of

More information

Igneous Rock Classification, Processes and Identification Physical Geology GEOL 100

Igneous Rock Classification, Processes and Identification Physical Geology GEOL 100 Igneous Rock Classification, Processes and Identification Physical Geology GEOL 100 Ray Rector - Instructor Major Concepts 1) Igneous rocks form directly from the crystallization of a magma or lava 2)

More information

First principles investigation of the structural and elastic properties of hydrous wadsleyite under pressure

First principles investigation of the structural and elastic properties of hydrous wadsleyite under pressure JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 114,, doi:10.1029/2008jb005841, 2009 First principles investigation of the structural and elastic properties of hydrous wadsleyite under pressure Jun Tsuchiya 1,2

More information

On the hydration of majoritic garnet

On the hydration of majoritic garnet University of Colorado, Boulder CU Scholar Geological Sciences Graduate Theses & Dissertations Geological Sciences Spring 1-1-2011 On the hydration of majoritic garnet David Andrew Brown University of

More information

Supplementary Materials for

Supplementary Materials for advances.sciencemag.org/cgi/content/full/4/5/eaar4378/dc1 Supplementary Materials for Discovery of moganite in a lunar meteorite as a trace of H2O ice in the Moon s regolith Masahiro Kayama, Naotaka Tomioka,

More information