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Trace element modeling of aqueous пuid · peridotite interaction in the mantle wedge of subduction zones. Received: 6 October 1997 / Accepted: 8 May 1998.
Contrib Mineral Petrol (1998) 132: 390±404

Ó Springer-Verlag 1998

John Ayers

Trace element modeling of aqueous ¯uid ± peridotite interaction in the mantle wedge of subduction zones

Received: 6 October 1997 / Accepted: 8 May 1998

Abstract Recently measured partition coecients for Rb, Th, U, Nb, La (Ce), Pb, Sr, Sm, Zr, and Y between lherzolite assemblage minerals and H2O-rich ¯uid (Ayers et al. 1997; Brenan et al. 1995a,b) are used in a two-component local equilibrium model to assess the e€ects of interaction between slab-derived aqueous ¯uids and wedge lherzolite on the trace element and isotopic composition of island arc basalts (IAB). The model includes four steps representing chemical processes, with each process represented by one equation with one adjustable parameter, in which aqueous ¯uid: (1) separates from eclogite in the subducted slab (Rayleigh distillation, mass fraction of ¯uid released F ¯uid); (2) ascends through the mantle wedge in isolated packets, exchanging elements and isotopes with depleted lherzolite (zone re®ning, the rock/¯uid mass ratio n); (3) mixes with depleted lherzolite (physical mixing, the mass fraction of ¯uid in the mixture X ¯uid); (4) induces melting to form primitive IAB (batch melting, mass fraction of melt F melt). The amount of mantle lherzolite processed by the ¯uid in step (2) determines its isotopic and trace element signature and the relative contributions of slab and wedge to primitive IAB. Assuming an average depleted lherzolite composition and mineralogy (70% olivine, 26% orthopyroxene, 3% clinopyroxene and 1% ilmenite) and using nonlinear regression to adjust parameter values to obtain an optimal ®t to the average composition of IAB (McCulloch and Gamble 1991) yields values of F ¯uid ˆ 0.20, n ˆ 26, X ¯uid ˆ 0.17, and F melt ˆ 0.15, with r 2 ˆ 0.995 and the average relative error in trace element concentration ˆ 6%. The average composition of IAB can also e€ectively be modeled with no contribution from the slab other than H2O (i.e., skip model step 1): n ˆ 27, X ¯uid ˆ 0.21, J. Ayers Department of Geology, P.O. Box 105B, Vanderbilt University, Nashville, TN 37235, USA; E-mail: [email protected]; Fax: 615-322-2138; Tel.: 615-322-2158 Editorial responsibility: T.L. Grove

F melt ˆ 0.17, with r 2 ˆ 0.992. By the time the ¯uid reaches the IAB source, exchange with depleted wedge lherzolite reduces the 87Sr/86Sr ratio isotopic composition to near-mantle values and the slab contribution to 5 wt%) must be added to lherzolite in the IAB source. Decreasing X ¯uid below 0.05 causes model results to have unacceptably high levels of error and petrologically unreasonable values of F melt. That H2O contents of IAB are generally 5 wt%) be added to lherzolite in the IAB source to obtain the observed composition for average IAB, no matter what assumptions are made in the trace element models. Although the trace element patterns of ¯uids in equilibrium with wedge lherzolite have appropriate trace element signatures for metasomatizing the IAB source, their low solute contents require high mass fractions of ¯uid to a€ect signi®cantly the composition of the source. Either all of the mineral/¯uid partition coecients measured by Ayers et al. (1997), Brenan et al. (1995) and Stalder et al. (1998) are systematically high (which seems unlikely since di€erent experimental and analytical methods were used in each study), or some complexing agent that uniformly increases D wedge/ ¯uid values has not been accounted for, or most of the ¯uid escapes from the source region while leaving behind its dissolved load. Clearly, more work must be done to reconcile the results of trace element modeling with those from studies of H2O contents of IAB (e.g., Sisson and Layne 1993) and melting of hydrous peridotite to form IAB (Kushiro 1990).

Acknowledgements Thanks to James Brenan and Terry Plank for organizing the ``Fluxes in Subduction Zones'' symposium at the Seventh Annual V.M. Goldschmidt Conference that prompted me to start this study. Funding was provided by NSF grant #EAR9317105. Ocial reviews by Je€ Ryan and an anonymous reviewer, informal reviews by Jim Meen, James Brenan, and Roland Stalder, and comments from Bill Leeman and Frank Dorendorf all helped to improve the manuscript.

After Nabalek (1987) Derivation of equation for concentration of trace element in ¯uid Cf during the zone re®ning process as function of n, the rock/ ¯uid mass ratio, with input of trace element-containing ¯uid Cfi at the base of the column (symbols same as used by Nabalek, 1987): Closed system: Co ˆ X f Cff ‡ …1 ÿ X f †Crf ˆ X f Cfi ‡ …1 ÿ X f †Cri Dˆ

Crf Cff

Co ˆ X f Cff ‡ …1 ÿ X f †DCff ˆ X f Cff ‡ DCff ÿ X f D Cff ˆ Cff …X f ‡ D ÿ X f D† Cff ˆ

Co (batch equilibrium) X f ‡ D…1 ÿ X f † Let N ˆ Cff ˆ

Cff ÿ Cfi ˆ

Cfi

‡

Mr 1 ÿ X f ˆ ; substitute for Co : Mf Xf i i Cf ‡ NCr ND ‡ 1

NCri Cfi …ND

ND ‡ 1 Cri ÿ Cfi D dCf ˆ dN … DN ‡ 1†2

‡ 1†

ND ‡ 1

ˆ

In the limit that N ˆ Mr/Mf ˆ 0,   dCf ˆ Cri ÿ Cfi D dN f

ZCf



Cff

dCf Cri ÿ Cfi D

ˆN

" # Cri ÿ Cfi D 1 ln D Cri ÿ Cff D   Cri ÿ Cff D exp N D ˆ Cri ÿ Cfi D



NCri ÿ Cfi ND ND ‡ 1

403 Since exp ()1) * exp (1) ˆ 1, multiply both sides by exp ()N D)  i  Cri Cr ÿ Cff ˆ ÿ Cfi exp…ÿND† D D  i  Cri Cr f Cf ˆ ÿ ÿ Cfi exp…ÿND† D D Compare to zone re®ning equation of Harris (1974):   Cff 1 1 ÿ ÿ 1 exp…ÿN D† ˆ D D Co If Co ˆ Cri as we assumed,  i  Ci Cr Cff ˆ r ÿ ÿ Cri exp…ÿND† D D In Eq. 3 )Cif replaces the term )Cir in the parentheses. This term represents the initial concentration in the material at the bottom of the column. In normal zone re®ning, this is a zone where the solid is completely molten, so that the initial concentration of the trace elements in this zone must equal that in the unmodi®ed bulk rock Cir . In our model, it is a ¯uid with initial trace element concentration Cif that enters the base of the column.

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