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 ...
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
- Page 2 and 3: The 410- and 520-km Discontinuities
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- Page 8 and 9: The 410-km Discontinuity in the Ear
- Page 10 and 11: The 410-km Discontinuity in the Ear
- Page 12 and 13: The 520-km Discontinuity in the Ear
- Page 14 and 15: The 520-km Discontinuity in the Ear
- Page 16 and 17: The 520-km Discontinuity in the Ear
- Page 18 and 19: The 520-km Discontinuity in the Ear
- Page 20 and 21: The 520-km Discontinuity in the Ear
- Page 22: The 410- and 520-km Discontinuities
<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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