the elasticity of (fe,ni) alloys and the composition of the earth’s core

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The Elasticity of (Fe,Ni) Alloys and the Composition of the Earth’s Core Owen Boberg Dave Emery, Boris Kiefer Department of Physics

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The Elasticity of (Fe,Ni) Alloys and the Composition of the Earth’s Core. Owen Boberg Dave Emery, Boris Kiefer. Department of Physics. Planetary Cores and Astronomical Observations. Earth’s Moment of Inertia not consistent with a homogeneous sphere. - PowerPoint PPT Presentation

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Page 1: The  Elasticity of (Fe,Ni) Alloys  and the Composition of the Earth’s Core

The Elasticity of (Fe,Ni) Alloys and the Composition of the Earth’s Core

Owen Boberg

Dave Emery, Boris Kiefer

Department of Physics

Page 2: The  Elasticity of (Fe,Ni) Alloys  and the Composition of the Earth’s Core

Planetary Cores and Astronomical Observations

• Earth’s Moment of Inertia not consistent with a homogeneous sphere.

• For a homogeneous sphere I = 0.4, IEarth= 0.33.• Suggests heavy material is concentrated toward the center of the

Earth.

Heavy element toward the center of the Earth.

I = r2dm∫

Page 3: The  Elasticity of (Fe,Ni) Alloys  and the Composition of the Earth’s Core

Nuclear Synthesis

• Iron is very abundant• Iron is very dense• Iron will sink due to

gravity.

Iron is abundant and heavy.http://www.fas.org

Relative to Sun

Iron

Page 4: The  Elasticity of (Fe,Ni) Alloys  and the Composition of the Earth’s Core

Local Magnetic FieldPrerequisites:• Liquid.• Rotating.• Electrical conductor.

Abundant metal like ironis a prime candidate for acore material.

Iron is a good candidate for core materials.

http://www.physics.ubc.ca/

Page 5: The  Elasticity of (Fe,Ni) Alloys  and the Composition of the Earth’s Core

Cosmochemistry• Iron meteorites are

remnants of planetary cores.

• Their composition is ≈90% iron and ≈10% nickel.

• Small perforations contain other elements.

Iron meteorites suggest iron-rich (Fe,Ni)-alloy in the Earth’s core.

http://www.amgueddfacymru.ac.uk

Page 6: The  Elasticity of (Fe,Ni) Alloys  and the Composition of the Earth’s Core

Earth Core Conditions

http://www.nature.com

http://matdl.org/

fcc

bcc

hcp

• Temperature: 5000K-6000K• Pressure: 136-360 GPa• Approximately 3 million

times the pressure felt at sea level.

• Known structures of iron: Face Centered Cubic (fcc). Body Centered Cubic (bcc). Hexagonal Closed Packing (hcp).

Page 7: The  Elasticity of (Fe,Ni) Alloys  and the Composition of the Earth’s Core

Exploration of Planetary Interiors

• Using state of the art computers we can simulate the Earth’s core.

• No Assumptions about the nature of chemical bonding.

It is possible to recreate the conditions of planetary cores in the lab or on computers.

https://wci.llnl.gov

http://upload.wikimedia.org/wikipedia/commons/

http://www.newmexicosupercomputer.com

New MexicoSupercomputerEncanto

Page 8: The  Elasticity of (Fe,Ni) Alloys  and the Composition of the Earth’s Core

Chemical Compositions

2x2x18 atomsx=0.125

1x1x12 atomsx=0.50

Double x, y

Triple x, yDouble z

Supercells: Fe1-XXX

Host atomAlloying element

Different cell sizes simulate different chemical compositions.

Page 9: The  Elasticity of (Fe,Ni) Alloys  and the Composition of the Earth’s Core

Iron-Nickel Alloys

• We are interested in how nickel (Ni) affects the elasticity of Fe,Ni alloys.

• Specifically we studied alloys containing 12.5% Nickel.

• A much needed knowledge baseline.

Understanding the properties of iron-nickel alloys forms a baseline for further research.

Page 10: The  Elasticity of (Fe,Ni) Alloys  and the Composition of the Earth’s Core

Iron-Nickel Alloy Stability700

600

500

400

300

200

100

0

-100

del

H (m

eV/a

t)

4003002001000

Pressure (GPa)

bcc

fcc

hcp

Fe7Ni (hcp-SS-221) Fe15Ni (hcp-SS-222) Fe7Ni (fcc-SS-211) Fe15Ni (fcc-SS-221) Fe7Ni (bcc-SS-SC221) Fe15Ni (bcc-SS-SC222)

Fe31Ni - fcc - SC(222)

•hcp is the most stable.•bcc is the least stable.

bcc favored:Belonoshko et al. (2008)

fcc favored:Mikhaylushkin et al. (2007)

hcp favored by Stixrude et al. (1995)

Page 11: The  Elasticity of (Fe,Ni) Alloys  and the Composition of the Earth’s Core

Elasticity of hcp: (Fe0.875Ni0.1257)2500

2000

1500

1000

500

0

C33

C11

C13

C12

600

500

400

300

200

10010.09.08.07.0

Volume (Å3/atom)

C44

C66Ela

stic

Con

stan

ts (G

Pa)

A)

B)

12

10

8

6

4

2

0

Wav

e S

peed

(km

/s)

14131211109

Density (gm/cm3)

Vp

Vs

• C44 is most greatly affected.• Shear properties are mostly affected.

Page 12: The  Elasticity of (Fe,Ni) Alloys  and the Composition of the Earth’s Core

Isotropic Velocities14

12

10

8

6

4

2

0

Agg

rega

te V

eloc

ities

(km

/s)

1614121086

Density (g/cm3)

Theory: hcp-(Fe0.875Si0.125) hcp-(Fe0.875S0.125) hcp-(Fe0.937O0.063) hcp-(Fe0.875Ni0.125) hcp-Fe; Steinle-Neumann (1999)

Experiment: hcp-Fe; Mao et al. (1998) hcp-(Fe0.92Ni0.08); Lin et al. (2003) PREM (1989)

• Oxygen affects elastic properties more than Si and S.• Candidate for light element in the Earth’s core.

Page 13: The  Elasticity of (Fe,Ni) Alloys  and the Composition of the Earth’s Core

Summary

• Hcp-type (Fe,Ni) alloy is most stable structure at least at low temperatures.

• Nickel affects mainly shear elasticity of (Fe,Ni) alloys.

• Small amounts of oxygen are possible without affecting stability.

• Oxygen may be prime candidate for light element.

Page 14: The  Elasticity of (Fe,Ni) Alloys  and the Composition of the Earth’s Core

Future Research

• Complete a knowledge baseline of the Iron-Nickel alloys.

• Extend research to high temperaturesNewton’s 2nd Law: F = m a.Dynamics (MD).

• Determine chemical conditions at formation of the core: oxidizing (O) vs. reducing (Si, S).

• Better understand the evolution of the Earth and other planets.