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Marine Ecosystems Research Department - jamstec japan agency ...

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JAMSTEC 2002 Annual Report<br />

Institute for Frontier <strong>Research</strong> on Earth Evolution (IFREE)<br />

143Nd/144Nd<br />

207Pb/204Pb<br />

0.5142<br />

0.5134<br />

HIMU<br />

0.5126 2 Ga<br />

0.5118<br />

17.5<br />

17.0<br />

16.5<br />

2 Ga<br />

dehydrated<br />

MORB<br />

1 Ga<br />

DMM<br />

OIB<br />

3 Ga<br />

4 Ga<br />

EMI<br />

2 Ga<br />

fresh MORB<br />

dehydrated MORB<br />

subducted<br />

sediments<br />

2 Ga 1 Ga<br />

0.702 0.706 0.710 0.714<br />

subducted<br />

sediments<br />

PM<br />

EMII<br />

87Sr/86Sr<br />

2 Ga<br />

1 Ga<br />

16.0<br />

EMII<br />

1 Ga<br />

PM<br />

HIMU<br />

15.5<br />

OIB fresh<br />

EMI DMM<br />

MORB<br />

15 20 25 30 35 40<br />

206Pb/ 204 Pb<br />

Fig.14 Isotopic evolution of subducted oceanic crust and sediment.<br />

Variation of isotopic compositions of subducted fresh<br />

MORB, dehydrated residue of hydrous MORB and sediments.<br />

Ages of subduction are shown with symbols and<br />

lines. Compositions of the fresh MORB are calculated with<br />

Rb/Sr and Nd/Sm ratios 1% (upper curve) to 10% (lower<br />

curve) higher than the MORB source. U/Pb ratios of the<br />

fresh MORB are assumed to be same as the source. The<br />

MORB source is assumed to be derived from the primitive<br />

mantle at 4.0 Ga with parent/daughter ratios which<br />

changed continuously from 4 Ga to present. Present isotopic<br />

composition of the MORB source is: 87 Sr/ 86 Sr=0.7026,<br />

143<br />

Nd/ 144 Nd=0.5131, 206 Pb/ 204 Pb=17.5, 207 Pb/ 204 Pb=15.4.<br />

are likely to be significatly greater than that of the<br />

HIMU component, implying that subducted dehydrated<br />

basaltic crust may contribute to the genesis of this<br />

mantle component. The Sr and Nd isotopic evolution<br />

of the dehydrated crust is dependent on Rb-Sr and<br />

Sm-Nd ratio changes during partial melting at<br />

mid-oceanic ridges and dehydration reactions in<br />

subduction zones. Although it is difficult to estimate<br />

quantitatively, suitable parent-daughter ratios to<br />

produce HIMU-like Sr and Nd isotopic ratios could<br />

be explained through the above two processes,<br />

including accumulation of both fresh and dehydrated<br />

MORB crust (Fig.).<br />

The role of subducting sediments in the formation<br />

of EMII, one of the enriched geochemical reservoirs in<br />

the mantle, has been emphasized by several authors<br />

because oceanic sediments generally have high<br />

<br />

Sr/ Sr and relatively low Nd/ Nd values (e.g.,<br />

Devey et al., ; Weaver, ). However, oceanic<br />

sediments that are subducted into the mantle contain<br />

significant amounts of hydrous phases, all of which<br />

will decompose to release fluids, ultimately causing<br />

significant fractionation of trace elements through<br />

fluid migration. Experiments on sediment dehydration<br />

have demonstrated that ancient subducted oceanic sediments,<br />

while experiencing compositional modification<br />

in the subduction factory, may evolve to an<br />

enriched component with high Sr/ Sr and Pb/ Pb<br />

values. They further indicated that the isotopic signature<br />

of the EMII component can be achieved by the<br />

addition of small amounts (~wt.%) of dehydrated<br />

sediment to DMM-like mantle or primitive mantle<br />

(Fig.).<br />

Trace element modeling by IFREE suggests that the<br />

geochemical characteristics of bulk continental crust<br />

can be reasonably explained by mixing of mantlederived<br />

basaltic and crust-derived felsic magmas.<br />

In order to make an andesitic continental crust, the<br />

melting residue after extraction of felsic melts should<br />

be removed and delaminated from the initial crust.<br />

It is thus of interest to examine the isotopic evolution<br />

of a delaminated 'anti-crust' component, based on<br />

inferred parent-daughter element concentrations, and<br />

to compare such signatures with those of the mantle<br />

reservoirs.<br />

The results of the calculation are shown in Figure<br />

, together with the isotope compositions of the mantle<br />

geochemical reservoirs. Quite distinct evolutionary<br />

curves with large variations in isotope ratio are<br />

obtained, due to differences in the degrees of involve-<br />

96

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