Cite abstracts as
Eos Trans. AGU, 82(47), Fall Meet. Suppl., Abstract xxxxx-xx,
2001
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churikova
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HR: 09:15h AN: T31F-04 TI: The HFSE budget of arc
magmas: new models from Hf isotopes and isotope dilution measurements of
Nb/Ta, Zr/Hf and Lu/Hf in Kamchatka arc rocks AU: * M\"{u}nker, C EM: [email protected] AF: Institut
f\"{u}r Mineralogie, Corrensstr. 24 , M\"{u}nster, 48149 Germany
AU: W\"{o}rner, G AF: Geowissenschaftliches Zentrum der Universitt G\"{o}ttingen GZG),
Abt. Geochemie, Goldschmidtstr. 1, G\"{o}ttingen, 37077 Germany
AU: Churikova, T AF: Institute of Volcanology and Geochemistry, Piip Avenue 9,
Petropavlowsk, Russian Federation AU: Mezger, K
AF: Institut f\"{u}r Mineralogie, Corrensstr. 24
, M\"{u}nster, 48149 Germany AB: There is still
no consensus as to whether the HFSE depletion in subduction rocks is
caused by the immobile behaviour of these elements during slab dehydration
or by the presence of residual accessory phases in the magma sources. To
assess this problem, we analysed Nb/Ta, Zr/Hf and Lu/Hf by isotope
dilution, together with Hf isotopes, in arc rocks from Kamchatka. Using a
mixed $^{180}$Ta-$^{94}$Zr-$^{180}$Hf-$^{176}$Lu tracer and the MC-ICPMS
in Mnster, we are able to achieve external precisions and accuracies of
$\pm$0.5 to $\pm$1$\%$ for Lu/Hf and Zr/Hf and of $\pm$5$\%$ for Nb/Ta
(2$\sigma$ uncertainties). In contrast to older techniques (e.g.
quadropole ICPMS), this analytical protocol results in a nearly 10-fold
improvement in analytical resolution. The investigated suite of Kamchatka
arc rocks comprises a cross-arc transect at $56\deg$ (element budget
largely controlled by variable fluid flux into the subarc mantle,
Dohrendorf et al. 2000) and a suite from volcanoes in the Northern Central
Kamchatka depression (NCKD, largely controlled by slab melts, Yogodzinski
et al. 2001). Coupled Hf-Nd isotope variations ($\epsilon$Hf = 12-18,
$\epsilon$Nd = 6-10) in all samples from the central Kamchatka depression
(CKD) and from the back-arc suggest mixing between an OIB source and a
MORB source in the wedge. However, samples from the arc front are slightly
displaced from the Hf-Nd array towards less radiogenic Nd, indicating
selective addition of minor sediment derived Nd to the mantle wedge by
fluids high in Nd/Hf. The Zr/Hf (30-42) in all arc rocks are
anti-correlated with Lu/Hf ($^{176}$Lu/$^{177}$Hf= 0.01-0.03), suggesting
that the budget of Zr and Hf is controlled by the degree of mantle
depletion rather than by the slab component. NCKD samples are slightly
offset from the southern array towards lower Lu/Hf-Zr/Hf, suggesting that
Zr-Hf is controlled by slab melts. The back-arc samples show
superchondritic Zr/Hf ($>$35), consistent with the presence of an OIB
source component (typical Zr/Hf$>$35) in their source. Nb/Ta in the
Kamchatka rocks range from 11-18 and are decoupled from Zr/Hf and Lu/Hf.
The samples from the arc front show an increase in Nb/Ta with Sr/Nd and
Ba/Th, indicating that the Nb-Ta budget in these samples is controlled by
fluids derived from the subducted slab. Samples from the NCKD (slab melt
controlled) overlap in their Nb/Ta and Zr/Hf with samples from the CKD
further south (fluid controlled). Such overlapping HFSE patterns, similar
in range to MORB, suggest that accessory phases in the slab, if present,
can only cause minor Zr/Hf and Nb/Ta fractionation in the subarc fluids or
melts. References Dorendorf, F., Wiechert, U. and Worner, G. (2000): Earth
and Planetary Science Letters 175: 69-86. Yogodzinski, G.M., Lees, J.M.,
Churikova, T., Dorenforf, F., Worner, G., and Volynets, O.N., (2000):
Nature 409, 500-504. DE: 1040 Isotopic
composition/chemistry DE: 1065 Trace elements
(3670) DE: 3640 Igneous petrology SC:
T MN: 2001 AGU Fall
Meeting