CIDER 12 Deep Time - University of California, …...CIDER 12 Deep Time Earth Materials I...

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CIDER 12 Deep Time Earth Materials I Introduction to Earth Materials (Hirschmann) Earth Materials II Exp. Studies Related to Early Earth Proc (Rubie) Earth Materials III The Mantle (Li) Tutorial IV: Equations of State (Li) Earth Materials IV Accretion, Magma Oceans, Core Formation (Rubie) Tutorial V: Molecular Dynamics (Caracas) Earth Materials V Transport Properties (Williams) Earth Materials VI The Core (Li) July 16-28, 2012 KITP, Santa Barbara CA

Transcript of CIDER 12 Deep Time - University of California, …...CIDER 12 Deep Time Earth Materials I...

Page 1: CIDER 12 Deep Time - University of California, …...CIDER 12 Deep Time Earth Materials I Introduction to Earth Materials (Hirschmann) Earth Materials II Exp. Studies Related to Early

CIDER 12 Deep Time

Earth Materials I Introduction to Earth Materials (Hirschmann) Earth Materials II Exp. Studies Related to Early Earth Proc (Rubie) Earth Materials III The Mantle (Li) Tutorial IV: Equations of State (Li) Earth Materials IV Accretion, Magma Oceans, Core Formation (Rubie) Tutorial V: Molecular Dynamics (Caracas) Earth Materials V Transport Properties (Williams) Earth Materials VI The Core (Li)

July 16-28, 2012 KITP, Santa Barbara CA

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Earth’s Mantle

P: 136 GPa T: 3000 K x: ? t: ?

How are Earth processes controlled by material properties?

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Interpret 1D Seismic Profile + Rock Records: X-T-t

Dziewonski and Anderson 81 PEPI

LAB Melt, water TZ Discontinuities Depth: Phase transitions Width: Fe partition, phase equilibria Magnitude: Density, velocity Topography: Clapeyron slope, kinetics D” Phase transitions Deep time MO overturn: Density

Frost 08 Element

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Explain Seismic Tomography + Geochemical Domains: X-T-t

Garnero/McNamara 08 Science

Kellogg et al. 99

Stracke 05 G3

Plate Tectonics Slab, Plume: Density, viscosity, conductivity Mantle Convection Rayleigh #: Density, viscosity, conductivity, heat capacity CMB Interaction Partition, transport

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Iron Plays a Critical Role in Mantle Evolution

Jie (Jackie) Li, University of Michigan

Phase transition Partitioning Oxidation state Spin crossover Density, velocity, elasticity Transport properties

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Phase Transition: Coordination Number

Fei 98 UHPM

Pauling’s Rules

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Phase Transition Affects Density and Velocities

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Phase Transition in Mg2SiO4 Produces Density/Velocity Jumps

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Clausius-Clapeyron Slope G = U + PV -TS GA = UA + PVA -TSA GB = UB + PVB –TSB

For an infinitesimal change in P and T dGA = VAdP - SAdT dGB = VBdP - SBdT

Along the boundary GA = GB dGA = dGB i.e. VAdP - SAdT = VBdP – SBdT ΔVB-AdP = ΔSB-AdT dP/dT = ΔSB-A/ΔVB-A

Phase boundary (curve) dP/dT = Slope of tangent to curve Sign and value of slope

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Sign of Clapeyron Slope Indicates Thermal Effect

dT/dP = ΔV/ΔS

α to β transition (410 km) Positive Clapeyron slope (common) β  smaller molar volume, smaller molar entropy Exothermic

γ to PV+FP transition (660 km) Negative Clapeyron slope (uncommon) PV+FP smaller molar volume larger molar entropy Endothermic

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TZ Topography / Barriers to Convection

gamma

Pv+Fp 660 km

resistance to plume rising

resistance to slab sinking

gamma

Pv+Fp gamma

Pv+Fp

boundary pushed downwards

boundary pushed upwards

dT/dP = ΔV/ΔS = 769 K/GPa�Assuming linear slope�

For slab dT ~ -500 K, dP ~ 0.6 GPa (15 km)�For plume dT ~ +200 K, dP ~ -0.3 GPa (7.5 km)

Fei et al. 2004

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D” Topography and Structure

Shim 08 AREPS Lay et al. 08 Nature Geo.

Double Crossing PPv lens

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Iron Lowers and Broadens Phase Boundaries Mw or Fp Phase Rule f = c + 2 – p

Fei 1998 UHPM

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Iron Shifts and Broadens Pv-PPv Transition

Mao 07 AGU mono Mao et al. 06 Science Mao et al. 06 PNAS

Pv contains more iron than PPv Hirose 08 AM

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Iron Increases Density and Lowers Sound Velocities

Stixrude 07 ToG

ρ = m/V ρVp2 = K + 4G/3 ρVS

2 = G

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Iron’s Valence State / Oxidation State

Fe [Ar]3d64s2

metallic

Fe2+ [Ar]3d6

ferrous Fe3+ [Ar]3d5

ferric

3Fe2+ = 2Fe3+ + Fe0

Wood et al. 06 Nature

Fe3+ + Al3+ = Mg2+ + Si4+

Fe3+ + Fe3+ = Mg2+ + Si4+

McCammon 97 Nature

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Crystal Field Splitting in Iron

Cubic, octahedral site

Spherical, degeneracy

Orthorhombic 8-12 C.N. site

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Pressure-Induced Spin Crossover in Fe2+

Δ Π

High Spin

Low Spin

Δ

Π

HS IS LS

Intermediate Spin

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Probe Electronic Structure Mössbauer spectroscopy • Conventional • Synchrotron - Energy domain - Time domain Nuclear Forward Scattering

X-ray emission spectroscopy • Local moment • Kβ’/Kβ

Isomer shift

Quadrupole splitting

Struzhkin 04, JPCM

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Pressure-Induced Spin Crossover in Fp and Pv

HS LS

Badro et al. 03 Science

1.5

1.0

0.5

0.0

Nor

mali

zed

inten

sity,

a.u.

70707060705070407030

Energy, eV

Al free, low spin Al free, 2 GPa Al free, 100 GPa Al bearing, 100 GPa

Lin et al. 07 Science Badro et al. 04 Science

Li et al. 04 PNAS

Lin et al. 08 Nature Geo

McCammon et al. 08 Nature Geo

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Spin Crossover Influences Physical Properties

Density & elasticity Lin et al. 05, 07 - Fp Fei et al. 05 – Pv

Radiative conductivity - Fp Badro et al 04 - blue shift Tsuchiya et al. 06 - red shift Goncharov et al 06 - red shift

Electric conductivity - Fp Ohta et al. 07

Vs

Pressure

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Limited Effects of Spin Crossover on Partitioning

Badro et al 03, 05 - Pv/Fp Li et al. 04; Li 07 - Pv/Fp Irifune et al. 10 - Pyrolite

Spin crossover gradual Fe3+ strongly prefers pV

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Birch-Murnaghan EoS

Finite strain theory: Eulerian strain Thermodynamics Macroscopic view

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“Hot” BM EoS T

P

T0

Isobaric heating

Isothermal compression

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Elasticity: Atomic Potential and Lattice Dynamics

Lattice dynamics: The Core

Microscopic view Bulk modulus Thermal expansion

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Mie-Grüneisen-Debye EoS - γ

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Mie-Grüneisen-Debye EoS – γ, q

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Modified Mie-Grüneisen-Debye EoS – γ, q0, q1

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Post-Spinel Transition and 660-km Discontinuity

Fei et al. 04 JGR Fei et al. 04 PEPI

Page 30: CIDER 12 Deep Time - University of California, …...CIDER 12 Deep Time Earth Materials I Introduction to Earth Materials (Hirschmann) Earth Materials II Exp. Studies Related to Early

Perovskitic Lower Mantle

Murakami et al. 12 Science

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Conclusions and Outlook

Material properties under deep mantle P-T-x-t conditions key to understanding the state and history of the mantle but poorly constrained

State of the art Experimental: ~ 4 Mbar (400 GPa), ~ 6000 K Analytical: time second spatial 10 nm

Planetary perspectives

CIDER

Brooks Bays Weber et al. 11 Science