The 410- and 520-km Discontinuities in the Earth's Mantle ...

The 410- and 520-km Discontinuities in the Earth's Mantle ... The 410- and 520-km Discontinuities in the Earth's Mantle ...

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The 410- and 520-km Discontinuities in the Earth’s Mantle: Experiments and Thermodynamic modelling Fiorenza Deon, Maria Mrosko, Monika Koch-Müller Deutsches GeoForschungsZentum, GFZ, Department 3, Telegrafenberg, 14473, Potsdam 3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel (Mg, Fe) 2 SiO 4 olivine, wadsleyite, ringwoodite H incorporation in the range of wt% if expressed as H 2 O

<strong>The</strong> <strong>410</strong>- <strong>and</strong> <strong>520</strong>-<strong>km</strong> <strong>Discont<strong>in</strong>uities</strong> <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Experiments <strong>and</strong> <strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

Fiorenza Deon, Maria Mrosko, Monika Koch-Müller<br />

Deutsches GeoForschungsZentum, GFZ, Department 3, Telegrafenberg, 14473, Potsdam<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

(Mg, Fe) 2 SiO 4<br />

oliv<strong>in</strong>e, wadsleyite, r<strong>in</strong>gwoodite<br />

H <strong>in</strong>corporation <strong>in</strong> <strong>the</strong> range of wt%<br />

if expressed as H 2 O


<strong>The</strong> <strong>410</strong>- <strong>and</strong> <strong>520</strong>-<strong>km</strong> <strong>Discont<strong>in</strong>uities</strong> <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Experiments <strong>and</strong> <strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

d<strong>410</strong>-<strong>km</strong>:<br />

oliv<strong>in</strong>e to wadsleyite<br />

Seismology: Wide range of<br />

thicknesses from about 4 <strong>km</strong><br />

to 35 <strong>km</strong><br />

Related to water<br />

<strong>in</strong>corporation <strong>in</strong> <strong>the</strong><br />

coexist<strong>in</strong>g m<strong>in</strong>erals ol <strong>and</strong><br />

wads?<br />

Experiments <strong>in</strong>dicate shift of<br />

<strong>the</strong> transformation to lower<br />

P <strong>in</strong> <strong>the</strong> presence of water.<br />

Experimental studies: Frost<br />

<strong>and</strong> Dolejs, 2007; Chen et<br />

al., 2002; Frost <strong>and</strong><br />

McCammon, 2009<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

No clear picture<br />

(Mg, Fe) 2 SiO 4<br />

d<strong>520</strong>-<strong>km</strong>:<br />

wadsleyite to r<strong>in</strong>gwoodite<br />

Seismology: large variation<br />

<strong>in</strong> <strong>the</strong> depth <strong>and</strong> very sharp<br />

Related to water<br />

<strong>in</strong>corporation <strong>in</strong> <strong>the</strong><br />

coexist<strong>in</strong>g m<strong>in</strong>erals ol <strong>and</strong><br />

wads?<br />

Experiments <strong>in</strong>dicate shift of<br />

<strong>the</strong> transformation to<br />

higher P <strong>in</strong> <strong>the</strong> presence of<br />

water.<br />

Contrary to <strong>the</strong> d<strong>410</strong> <strong>the</strong><br />

reason for this variation is<br />

<strong>the</strong>rmodynamically<br />

completely unclear.


<strong>The</strong> <strong>410</strong>- <strong>and</strong> <strong>520</strong>-<strong>km</strong> <strong>Discont<strong>in</strong>uities</strong> <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Experiments <strong>and</strong> <strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

Experiments <strong>in</strong> a rotat<strong>in</strong>g/rock<strong>in</strong>g multi-anvil press <strong>in</strong> <strong>the</strong> system (Mg,Fe) 2 SiO 4 - H 2 O,<br />

buffered with opx <strong>and</strong> water <strong>in</strong> excess under reduc<strong>in</strong>g conditions us<strong>in</strong>g multi-anvil<br />

sets 14/8 <strong>and</strong> 10/5.<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel


<strong>The</strong> <strong>410</strong>- <strong>and</strong> <strong>520</strong>-<strong>km</strong> <strong>Discont<strong>in</strong>uities</strong> <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Experiments <strong>and</strong> <strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

Experiments <strong>in</strong> a rotat<strong>in</strong>g/rock<strong>in</strong>g multi-anvil press <strong>in</strong> <strong>the</strong> system (Mg,Fe) 2 SiO 4 - H 2 O,<br />

buffered with opx <strong>and</strong> water <strong>in</strong> excess us<strong>in</strong>g multi-anvil sets 14/8 <strong>and</strong> 10/5.<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

Reduc<strong>in</strong>g conditions: Fe/FeO buffer


<strong>The</strong> <strong>410</strong>- <strong>and</strong> <strong>520</strong>-<strong>km</strong> <strong>Discont<strong>in</strong>uities</strong> <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Experiments <strong>and</strong> <strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

static rock<strong>in</strong>g<br />

Experiments <strong>in</strong> a rotat<strong>in</strong>g/rock<strong>in</strong>g multi-anvil press <strong>in</strong> <strong>the</strong> system (Mg,Fe) 2 SiO 4 - H 2 O,<br />

buffered with opx <strong>and</strong> water <strong>in</strong> excess us<strong>in</strong>g multi-anvil sets 14/8 <strong>and</strong> 10/5.<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

water <strong>in</strong> excess


<strong>The</strong> <strong>410</strong>- <strong>and</strong> <strong>520</strong>-<strong>km</strong> <strong>Discont<strong>in</strong>uities</strong> <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Experiments <strong>and</strong> <strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

JEOL JXA 8500 F:<br />

chemical composition<br />

Horiba Job<strong>in</strong> Yvon Laser Raman,<br />

Water quantification<br />

Phase identification, chemical analyses,<br />

quantification of water <strong>and</strong> Fe 3+<br />

Synchrotron FIR: vibrational mod.<br />

SIMS,<br />

Water quantification<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

Bruker, NIR <strong>and</strong> MIR<br />

Fei TEM <strong>and</strong> FIB:<br />

EELS for Fe 3+<br />

Co-operation with<br />

Dr. Alex<strong>and</strong>ra Friedrich for X-RDA


<strong>The</strong> <strong>410</strong>-<strong>km</strong> Discont<strong>in</strong>uity <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Results - Mg2SiO4 +/- H2O Mg 2 SiO 4<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

Systematic occurrence of hydrous<br />

Wadsleyite <strong>in</strong> <strong>the</strong> stability field of dry<br />

oliv<strong>in</strong>e.<br />

In <strong>the</strong> presence of water <strong>the</strong><br />

oliv<strong>in</strong>e-wadsleyite phase boundary<br />

is shifted 0.6 GPa to lower P.<br />

This is due to a stronger fractionation<br />

of water <strong>in</strong>to wadsleyite ra<strong>the</strong>r than<br />

oliv<strong>in</strong>e - <strong>in</strong>crease of <strong>the</strong><br />

configurational entropy of hydrous<br />

wadsleyite.


<strong>The</strong> <strong>410</strong>-<strong>km</strong> Discont<strong>in</strong>uity <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Results - (Mg, Fe) 2SiO 4<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

P-x projection<br />

1200 °C


<strong>The</strong> <strong>410</strong>-<strong>km</strong> Discont<strong>in</strong>uity <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Results - (Mg, Fe) 2SiO 4 + H 2O<br />

Triple po<strong>in</strong>t at 12.2 GPa, 1200°C<br />

ol: 2700 wt ppm H 2 O<br />

wad:10000 wt ppm H 2 O<br />

r<strong>in</strong>g: 4000 wt ppm H 2 O<br />

BSE image<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

EEL-Spectra<br />

FIB-Foil<br />

Coexist<strong>in</strong>g<br />

ol-wad-r<strong>in</strong>g<br />

Fe 3+ pfu:<br />

Wad:<br />

0.07(2)<br />

R<strong>in</strong>g:<br />

0.02(1)


<strong>The</strong> <strong>410</strong>-<strong>km</strong> Discont<strong>in</strong>uity <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Results - (Mg, Fe) 2SiO4 +/- H2O P-x projections<br />

dry<br />

Extension of <strong>the</strong> stability field of hydrous wadsleyite to lower <strong>and</strong><br />

to higher pressures<br />

which br<strong>in</strong>gs us to <strong>the</strong> new project on:<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

hydrous


<strong>The</strong> <strong>520</strong>-<strong>km</strong> Discont<strong>in</strong>uity <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Experiments <strong>and</strong> <strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

Modell<strong>in</strong>g <strong>the</strong> stability of wadsleyite <strong>and</strong> r<strong>in</strong>gwoodite<br />

<strong>in</strong> dependence of <strong>the</strong> water content<br />

Experimental part:<br />

quenched Multi-Anvil-runs<br />

- effect of P, T, x<br />

- fractionation of water<br />

between wads <strong>and</strong> r<strong>in</strong>g<br />

- structural <strong>and</strong> crystalchemical<br />

analyses<br />

- vibrational spectroscopy<br />

- calorimetry<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

Different approach:<br />

<strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

- calculate vibrational spectra<br />

(DFPT)<br />

- calculate <strong>the</strong>rmodynamic<br />

properties on basis of<br />

vibrational DOS<br />

- model phase stabilities as<br />

f(H 2 O)


<strong>The</strong> <strong>520</strong>-<strong>km</strong> Discont<strong>in</strong>uity <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Experiments <strong>and</strong> <strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

Modell<strong>in</strong>g of phase stabilities<br />

Determ<strong>in</strong>e <strong>the</strong>rmodynamic data<br />

Calorimetry at University of Salzburg (E. Dachs)<br />

PPMS-System of Quantum Design<br />

PPMS (5-303K):<br />

- Sample <strong>and</strong> measur<strong>in</strong>g probe <strong>in</strong> liquid-Hebath<br />

- Resonance of sample to a heat-pulse is<br />

determ<strong>in</strong>ed at different temperatures<br />

- non-l<strong>in</strong>ear curve-fitt<strong>in</strong>g of data produces<br />

heat-capacities


<strong>The</strong> <strong>520</strong>-<strong>km</strong> Discont<strong>in</strong>uity <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Experiments <strong>and</strong> <strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

Modell<strong>in</strong>g of phase stabilities<br />

Determ<strong>in</strong>e <strong>the</strong>rmodynamic data<br />

Calorimetry at University of Salzburg (E. Dachs)<br />

PPMS-System of Quantum Design<br />

PPMS <strong>and</strong> DSC-measurements of<br />

anhydrous wadsleyite:<br />

C p (298) = 115.43 J/(mol*K)<br />

S (298) = 86.67 J/(mol*K)<br />

Cp (298) = 116.3 J/(mol*K) Akaogi et al 2007<br />

Cp (298) = 117.3 J/(mol*K) Ottonello et al 2009<br />

Values for hydrous wads differ clearly


<strong>The</strong> <strong>520</strong>-<strong>km</strong> Discont<strong>in</strong>uity <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Experiments <strong>and</strong> <strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

» use vDOS (determ<strong>in</strong>ed by vibrational spectroscopy) <strong>and</strong><br />

its pressure dependence to compute <strong>the</strong>rmodynamic data<br />

» <strong>the</strong> more modes can be characterized <strong>the</strong> better <strong>the</strong><br />

modell<strong>in</strong>g<br />

» complicate <strong>in</strong> <strong>the</strong> FAR-IR-region (loss of light due to<br />

diffraction)<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

Modell<strong>in</strong>g of phase stabilities<br />

Determ<strong>in</strong>e <strong>the</strong>rmodynamic data<br />

BUT: Calorimetric measurements not feasible for hydrous<br />

syn<strong>the</strong>ses (impurities of o<strong>the</strong>r phases)


<strong>The</strong> <strong>520</strong>-<strong>km</strong> Discont<strong>in</strong>uity <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Experiments <strong>and</strong> <strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

High brilliance of IR synchrotron light ma<strong>in</strong>ta<strong>in</strong>s<br />

enough <strong>in</strong>tensity<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel


<strong>The</strong> <strong>520</strong>-<strong>km</strong> Discont<strong>in</strong>uity <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Experiments <strong>and</strong> <strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

<strong>The</strong>refore we constructed a microscope to take pressure-depend<strong>in</strong>g<br />

FAR-IR-spectra <strong>in</strong> DAC at <strong>the</strong> Berl<strong>in</strong> Synchrotron source BESSY.<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

synchrotron<br />

IR light<br />

from<br />

<strong>in</strong>terferometer


<strong>The</strong> <strong>520</strong>-<strong>km</strong> Discont<strong>in</strong>uity <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Experiments <strong>and</strong> <strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

Merged spectrum (FAR <strong>and</strong> MID-IR) of anhydrous wadsleyite<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel


<strong>The</strong> <strong>520</strong>-<strong>km</strong> Discont<strong>in</strong>uity <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Experiments <strong>and</strong> <strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

Merged spectrum (FAR <strong>and</strong> MID-IR) of anhydrous wadsleyite<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

1<br />

2<br />

3 4 5 6 78<br />

9<br />

10<br />

11<br />

12<br />

1 ν as (SiO 3 )<br />

2 ν s (SiO 3 )<br />

3 ν s (SiOSi)<br />

4 ρ(Si 2 O 7 )<br />

5 ν(M3-O1)<br />

6 ν(M3-O1)<br />

7 ν(M3-O1)<br />

8 T(M)<br />

9 T(M)<br />

10 R<br />

11 T<br />

12 R


<strong>The</strong> <strong>520</strong>-<strong>km</strong> Discont<strong>in</strong>uity <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Experiments <strong>and</strong> <strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

Pressure-depend<strong>in</strong>g FAR-IR spectra<br />

of hydrous wadsleyite<br />

» <strong>the</strong> more modes one can<br />

observe <strong>the</strong> better one can<br />

compute <strong>the</strong>rmodynamic data<br />

us<strong>in</strong>g <strong>the</strong> vibrational modell<strong>in</strong>g<br />

» correct assignment of modes is<br />

essential (substitution experiments,<br />

pressure-dependence)


<strong>The</strong> <strong>520</strong>-<strong>km</strong> Discont<strong>in</strong>uity <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Experiments <strong>and</strong> <strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

Pressure-depend<strong>in</strong>g FAR-IR spectra<br />

of hydrous wadsleyite<br />

Vibrational modell<strong>in</strong>g after Kieffer<br />

(1979, 1980)<br />

#<br />

"<br />

0<br />

x<br />

e<br />

CV = 3Nk<br />

x<br />

( e $ 1)<br />

Cp = C V + TV a 2 K T<br />

2<br />

x<br />

2<br />

g(<br />

! ) d!<br />

» compare with experimental data


<strong>The</strong> <strong>520</strong>-<strong>km</strong> Discont<strong>in</strong>uity <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Experiments <strong>and</strong> <strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

Pressure-depend<strong>in</strong>g FAR-IR spectra<br />

of hydrous wadsleyite<br />

Changes <strong>in</strong> pressure-depend<strong>in</strong>g<br />

behaviour of FAR-IR-b<strong>and</strong>s<br />

» <strong>in</strong>dicate phase transition between<br />

7 <strong>and</strong> 8 GPa<br />

» transition <strong>in</strong> dry wadsleyite seems<br />

to appear at app. 10 GPa


<strong>The</strong> <strong>410</strong>- <strong>and</strong> <strong>520</strong>-<strong>km</strong> <strong>Discont<strong>in</strong>uities</strong> <strong>in</strong> <strong>the</strong> Earth’s <strong>Mantle</strong>:<br />

Experiments <strong>and</strong> <strong>The</strong>rmodynamic modell<strong>in</strong>g<br />

Fiorenza Deon, Maria Mrosko, Monika Koch-Müller<br />

Deutsches GeoForschungsZentum, GFZ, Department 3, Telegrafenberg, 14473, Potsdam<br />

3. Berichtskolloquium SPP 1236 10. - 12. 03.2010 Oberursel<br />

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