Journal of Petrology Advance Access originally published online on February 21, 2006
Journal of Petrology 2006 47(5):929-964; doi:10.1093/petrology/egi101
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Petrology and Geochemistry of Eclogite Xenoliths from the Colorado Plateau: Implications for the Evolution of Subducted Oceanic Crust
1 PHEASANT MEMORIAL LABORATORY FOR GEOCHEMISTRY AND COSMOCHEMISTRY, INSTITUTE FOR STUDY OF THE EARTH'S INTERIOR, OKAYAMA UNIVERSITY AT MISASA, TOTTORI, 682-0193, JAPAN
2 DEPARTMENT OF GEOLOGICAL SCIENCES AND GEOLOGICAL ENGINEERING, QUEEN'S UNIVERSITY, KINGSTON, ONT., K7L 3N6, CANADA
RECEIVED DECEMBER 9, 2004; ACCEPTED DECEMBER 19, 2005
| ABSTRACT |
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Eclogite xenoliths from the Colorado Plateau, interpreted as fragments of the subducted Farallon plate, are used to constrain the trace element and SrNdPb isotopic compositions of oceanic crust subducted into the upper mantle. The xenoliths consist of almandine-rich garnet, Na-clinopyroxene, lawsonite and zoisite with minor amounts of phengite, rutile, pyrite and zircon. They have essentially basaltic bulk-rock major element compositions; their Na2O contents are significantly elevated, but K2O contents are similar to those of unaltered mid-ocean ridge basalt (MORB). These alkali element characteristics are explained by spilitization or albitization processes on the sea floor and during subduction-zone metasomatism in the fore-arc region. The whole-rock trace element abundances of the xenoliths are variable relative to sea-floor-altered MORB, except for the restricted Zr/Hf ratios (36·937·6). Whole-rock mass balances for two Colorado Plateau eclogite xenoliths are examined for 22 trace elements, Rb, Cs, Sr, Ba, Y, rare earth elements, Pb, Th and U. Mass balance considerations and mineralogical observations indicate that the whole-rock chemistries of the xenoliths were modified by near-surface processes after emplacement and limited interaction with their host rock, a serpentinized ultramafic microbreccia. To avoid these secondary effects, the Sr, Nd and Pb isotopic compositions of minerals separated from the xenoliths were measured, yielding 0·704530·70590 for 87Sr/86Sr, 3·1 to 0·5 for
Nd and 18·92819·063 for 206Pb/204Pb. These isotopic compositions are distinctly more radiogenic for Sr and Pb and less radiogenic for Nd than those of altered MORB. Our results suggest that the MORB-like protolith of the xenoliths was metasomatized by a fluid equilibrated with sediment in the fore-arc region of a subduction zone and that this metasomatic fluid produced continental crust-like isotopic compositions of the xenoliths. KEY WORDS: Colorado Plateau; eclogite xenolith; geochemistry; subducted oceanic crust
| INTRODUCTION |
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Material recycling through subduction zones is one of the most important processes controlling the chemical evolution of the Earth, and materials from the Earth's surface are likely to have been reintroduced into its interior throughout geological history. Although most of the subducting plate is made of mantle material returning to depths from which it originated, hydrated and altered upper oceanic crust, as well as overlying sediments, carry a record of low-temperature interactions with continents, oceans and the atmosphere into the deep mantle. Subduction of surface and near-surface components can change the volatile contents, trace element abundances, amounts of heat-producing elements and radiogenic isotope systematics in the mantle.
A number of geochemical models have been developed to estimate the integrated trace element and isotopic composition of a hypothetical slab-derived component in arc and ocean island basalt (OIB) lavas (e.g. Zindler & Hart, 1986
; McCulloch & Gamble, 1991
; Ishikawa & Nakamura, 1994
; Hofmann, 1997
; Taylor & Nesbitt, 1998
; Stracke et al., 2003
). However, contributions from individual sources are difficult to assess from lava compositions alone, because element fractionations during slab dehydration and mass fluxes from the various subducted lithologies are poorly constrained. Nevertheless, most models have used a geochemical component estimated from rock compositions prior to subduction (e.g. samples from ocean-floor drilling). Therefore, understanding the trace element and isotopic compositions of individual rock types subducted into the sub-arc mantle is indispensable for constraining geochemical models for subduction-zone material recycling.
One approach to constrain material cycling involves high-pressure experimental studies that simulate processes such as dehydration of the subducting slab under controlled conditions (e.g. Schmidt & Poli, 1998
; Okamoto & Maruyama, 1999
; Poli & Schmidt, 2002
). Such experiments provide important constraints on the water contents and metamorphic phase relations in the subducting slab as a function of temperature and pressure. Other experiments have investigated the solubility of elements in fluids at high pressures, as well as element partitioning between the fluids and the constituent minerals in potential slab materials such as eclogites, blueschists and serpentinites (e.g. Brenan et al., 1994
, 1995
, 1998
; Iizuka & Nakamura, 1995
; Ayers et al., 1997
; Kogiso et al., 1997
; Stalder et al., 1998
). However, microanalytical and mass balance studies of subduction-related metamorphic rocks have shown that many so-called trace elements are preferentially partitioned into accessory minerals such as allanite, rutile, apatite, and zircon, and that elemental partitioning commonly does not reach equilibrium because of the relatively low-temperature environment envisaged in the subducting oceanic lithosphere (e.g. Sorensen & Grossman, 1989
, 1993
; Sorensen, 1991
; Tribuzio et al., 1996
; Zack et al., 2002a
, 2002b
; Spandler et al., 2003
). This suggests that partition coefficient data for trace elements may not be appropriate for evaluating trace element behaviors in subducting oceanic crust.
Thermomechanical studies indicate that subducting oceanic crust in cold subduction zones passes through the blueschist to lawsonite eclogite transition, and that the most important dehydration process for inducing island arc volcanism occurs in the lawsonite eclogite facies (Peacock, 1993
). Thus, lawsonite eclogites are critical to investigating trace element and isotopic behavior in subducted oceanic crust. However, data for trace element distributions among the mineral assemblages in the lawsonite eclogite facies are limited, because lawsonite eclogite terranes are rare (Zack et al., 2004
), and commonly much overprinted by high-T/P retrogression.
Lawsonite-bearing eclogite xenoliths from the Colorado Plateau of the southwestern USA present an important opportunity to study the trace element and isotopic systematics of this lithology. Helmstaedt & Doig (1975)
showed that these xenoliths resemble eclogites of the Franciscan Complex of the California Coast Ranges, western USA, in many aspects of their petrography and geochemistry. The Franciscan Complex represents fragments of a fossil subduction-zone plate boundary from the Jurassic to the Paleogene (e.g. Ernst, 1970
; Maruyama & Liou, 1989
). Offshore magnetic anomalies demonstrate that thousands of kilometers of oceanic crust have been subducted beneath the western US continental margin since the Late Cretaceous (Hamilton, 1969
). Usui et al. (2003)
used ion microprobe techniques to determine the UPb ages of zircons from the Colorado Plateau eclogite xenoliths, which yielded concordant ages from 81 to 33 Ma. Those workers interpreted the two extremes in age to reflect zircon crystallization during subduction-related metamorphism and zircon recrystallization during intrusion of the host rock. Combining geotectonic reasoning with the zircon geochronology and petrographic similarities to subduction-related eclogites led Usui et al. (2003)
to conclude that the Colorado Plateau eclogite xenoliths originated as fragments of the subducted Farallon plate that had resided in the upper mantle since the Late Cretaceous. Owing to their rapid transport to the surface, the eclogite xenoliths show few effects of retrograde overprinting compared with crustal eclogites exhumed by tectonic processes. Thus, they may preserve important chemical information about their subduction-related metamorphic history.
Two problematic issues remain concerning the origin of the Colorado Plateau eclogite xenoliths. One is whether they represent fragments of relatively young Phanerozoic subducted oceanic crust (Helmstaedt & Doig, 1975
; Usui et al., 2003
) or remnants of the much older, Proterozoic basement of the Colorado Plateau (Roden et al., 1990
; Wendlandt et al., 1993
; Smith et al., 2004
). The contrasting hypotheses for their ages may be considered to result, in part, from the application of different geochronological methods to date them. UPb zircon ages by ion microprobe analysis have yielded Phanerozoic ages (Usui et al., 2003
), whereas SmNd isotopic data (Roden et al., 1990
; Wendlandt et al., 1993
) give Proterozoic model ages in the range of 15001800 Ma. In addition, UPb analyses of multigrain zircon fragments by the isotope dilution method with thermal ionization mass spectrometry (ID-TIMS) resulted in a linear discordant line that intersected the concordia at 1514 Ma (Smith et al., 2004
).
The other debated issue is whether the Colorado Plateau eclogite xenoliths were formed by prograde metamorphism during subduction of oceanic lithosphere or by magmatic recrystallization processes in the upper mantle. Based on mineral textures and compositional zoning of garnet and clinopyroxene, Helmstaedt & Schulze (1988
, 1991
) concluded the former. They estimated two metamorphic temperatures for the eclogite xenoliths, corresponding to crystallization of garnet cores and peak metamorphic conditions, respectively, and concluded that the garnet rims formed at
100°C higher temperatures than the garnet cores. However, these estimates are unlikely to be conclusive because: (1) they depend on calculating the Fe2+/Fe3+ of clinopyroxene, a parameter that cannot be determined by electron microprobe; (2) it is difficult to determine the clinopyroxene coregarnet core temperature by using clinopyroxene with an oscillatory zoned structure. Smith & Zientek (1979)
suggested that the oscillatory zoning of clinopyroxene may represent disequilibrium growth in the presence of fluid phases, and that the Colorado Plateau eclogite xenoliths formed coexisting with a fluid phase during cooling and metasomatism of basaltic dikes in a cool upper mantle.
In this paper, we report whole-rock and mineral data for major, minor, and trace elements, and Sr, Nd, and Pb isotopic data for a suite of Colorado Plateau eclogite xenoliths. The geochemical data are complemented by observations of the modes of constituent minerals, their textures and chemical zoning structures. We reassess the contrasting hypotheses for the origin of the Colorado Plateau eclogite xenoliths and demonstrate that these rocks can be used as proxies to understand the geochemical evolution of subducted oceanic crust. These data allow us to develop a model for the trace element and isotopic (Sr, Nd and Pb) composition of subducted oceanic crust in the sub-arc region.
| GEOLOGICAL SETTING |
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The Colorado Plateau is a broadly elevated region,
1500 m above sea level, in the southwestern interior of the USA. Unmetamorphosed and little deformed Paleozoic to Cenozoic sedimentary rocks are well exposed on Precambrian basement (1·41·8 Ga; Condie, 1982
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Eight diatremes of serpentinized ultramafic microbreccia and numerous minette diatremes, the products of intra-plate magmatism, are exposed in the Navajo Volcanic Field of the Colorado Plateau (Fig. 1b). The microbreccia diatremes occur as two structurally controlled clusters (McGetchin et al., 1977
The diatreme rocks that host the eclogite xenoliths lack primary igneous textures and consist of finely crushed fragments of strongly serpentinized ultramafic rocks. Although initially described as kimberlites (e.g. McGetchin et al., 1977
), these rocks are not true kimberlites (e.g. Clement et al., 1984
) but serpentinized ultramafic microbreccias (SUM; Roden, 1981
). The microbreccia diatremes were emplaced between 25 and 35 Ma (Naeser, 1971
; Helmstaedt & Doig, 1975
; Roden et al., 1979
), contemporaneous with the numerous minette diatremes of the Navajo Volcanic Field (Ehrenberg, 1982
). The diatremes contain several types of eclogite, as well as a broad spectrum of possible upper mantle rocks that include variously hydrated spinel- and garnet-bearing peridotites, pyroxenites and serpentinites. The eclogite xenoliths are found mainly in three microbreccia diatremes in the Comb Ridge cluster (Garnet Ridge, Moses Rock, Mule Ear), and are absent from the Green Knobs and Buell Park pipes near the Defiance uplift (McGetchin et al., 1977
; Selverstone et al., 1999
). The samples used for this study were collected from the Moses Rock and Garnet Ridge diatremes.
| ANALYTICAL METHODS |
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Major element compositions of minerals were determined using a JEOL JXA-8800 electron microprobe at ISEI (Institute for Study of the Earth's Interior). Analyses were carried out at 15 kV and 20 nA sample current for all silicate minerals. Counting times of 30 s were used, and matrix corrections were performed by ZAF methods. The standards are synthetic oxides and natural minerals. The modal abundance of zircon was determined by digital image analysis of 25 randomly selected back-scattered electron images (each 1000 µm) per sample.
Trace element analyses of garnet, clinopyroxene, lawsonite and zoisite were performed using a CAMECA ims-5f ion microprobe at the PML (Pheasant Memorial Laboratory) in the ISEI, using techniques described by Nakamura & Kushiro (1998)
. Clinopyroxene from mantle xenoliths and basaltic natural glass were used as standard minerals for trace element calibrations. Trace element concentrations in these standards were chemically determined by inductively coupled plasma mass spectrometry (ICP-MS; Makishima & Nakamura, 1997
). The homogeneity of these standards was confirmed by optical microscope, electron microprobe and ion microprobe analysis. Trace element contents of garnet and clinopyroxene were calibrated on the basis of the clinopyroxene standard, and those of lawsonite and zoisite were calibrated using the basaltic glass standards. Minerals in thin sections were sputtered with an O primary beam of 1020 nA intensity, resulting in 1020 µm beam diameter. Clinopyroxene and lawsonite inclusions <30 µm in diameter were measured by an O primary beam of
6 nA intensity, which produced a beam <10 µm in diameter. Positive secondary ions were collected by ion counting using an energy offset of 60 V from 4500 V acceleration with an energy bandpass of ±10 V. These operating conditions resulted in (11·5) x 105 c.p.s. for 30Si secondary ions. The secondary ion intensities of atomic masses of interest were normalized to 30Si. For each analysis spot, 15 trace elements were determined in a run that took
40 min, including presputtering. The analytical reproducibility (relative standard deviation % for n = 10) for trace element measurements is generally <10% for the clinopyroxene standard and <5% for the basaltic glass standard, except for Er and Lu (710%).
To prepare whole-rock powders for analysis, eclogite samples were broken into chips
2 mm in diameter. Fresh pieces were hand-picked and washed with deionized water in an ultrasonic bath for 30 min. After drying at 60°C overnight, the chips were pulverized using a silicon nitride triturator to a grain size <400 mesh. To separate minerals, rock powders obtained using the silicon nitride triturator were sieved to capture grain sizes between 80 and 100 mesh (an average grain size of
200 µm). This sieved fraction was processed with an isodynamic separator, and the resulting mineral fractions were hand-picked.
Whole-rock major element compositions, along with Cr and Ni, were determined by X-ray fluorescence (XRF) spectrometry at the PML, on glass beads fluxed from mixing 100 mg of powdered sample and 5 g of lithium tetraborate (Takei, 2002
). Trace element compositions were measured by ICP-MS at the PML, based on the methods of Makishima & Nakamura (1997)
for Y, Cs, Ba, rare earth elements (REE), Pb, Th and U, those of Makishima et al. (1999)
for Zr, Hf and Nb, and of Moriguti et al. (2004)
for Li. Powdered samples (20 mg) for ICP-MS analysis were decomposed in 1·0 ml of HF and 0·1 ml of HNO3 in Teflon bombs at 210°C for 2 days, because acid-resistant minerals such as zircon and rutile are present in the eclogite samples. Analytical errors for trace element were generally 3% for Zr, Hf, and Li, and 5% for other elements.
The analytical procedures for mass spectrometry followed Yoshikawa & Nakamura (1993)
for Sr isotopic ratios and abundances of Rb and Sr, Makishima & Nakamura (1991)
for Nd isotopic ratios and abundances of Sm and Nd, Kuritani & Nakamura (2002
, 2003
) for Pb isotopic ratios and Pb abundances, and Yokoyama et al. (1999
, 2003
) for abundances of U and Th, employing TIMS in static multi-collection mode [modified Finnigan MAT261: Kiji (Nakano & Nakamura, 1998
), MAT262: Taro and MAT262: INU]. All of these elements (Rb, Sr, Sm, Nd, U, Th and Pb) were successively separated from each of the whole-rock and mineral samples, using a multi-ion exchange column chemistry approach modified after Nakamura et al. (2002)
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Basaltic standard JB3 from the Geological Survey of Japan (GSJ) yields typical analytical reproducibility of 0·005%, 0·005% and 0·02% for Sr, Nd and Pb isotopic ratios, respectively, and <1% for Rb, Sr, Sm, Nd, U, Th and Pb abundances. Accuracies of the isotopic and concentration analyses were confirmed by repeated measurement of JB3. We obtained data for this standard consistent with the previously published data within the analytical reproducibility (see Appendix, Table A1). Isotopic fractionation during analysis was corrected using 86Sr/88Sr = 0·1194 and 146Nd/144Nd = 0·7219 as normalizing factors. Pb isotopic fractionation was corrected by the two-double spikes method with 205Pb204Pb and 207Pb204Pb enriched spikes following the technique of Kuritani & Nakamura (2003)
. The composition of the spike was calibrated by assuming that the 208Pb/206Pb ratio of NBS982 is 1·00016 (Catanzaro et al., 1968
). Instrumental mass discrimination of TIMS analyses was corrected by the following values of standards: 87Sr/86Sr = 0·71024 (NIST987), 143Nd/144Nd = 0·511839 (La Jolla), and 206Pb/204Pb = 16·9424, 207Pb/204Pb = 15·5003, 208Pb/204Pb = 36·7266 (NBS981).
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| RESULTS |
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Mineral assemblage and classification of eclogite xenoliths
The Colorado Plateau eclogite xenoliths investigated in this study were previously described and referred to as metabasic eclogite and jadeite-clinopyroxenite, based not only on their mineral assemblages and basaltic bulk compositions, but also on their textural similarity to crustal examples of eclogites (Helmstaedt & Schulze, 1988
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Metabasic eclogites consist mainly of various proportions of almandine-rich garnet and omphacitic clinopyroxene with some lawsonite and zoisite (Fig. 2). They are either lawsonite-eclogite or zoisite-eclogite, according to the major constituent mineral assemblages (Table 1). Zoisite-eclogite is distinguished from lawsonite-eclogite only by its lack of lawsonite, although trace amounts of lawsonite crystals occur as small (
10 µm) inclusions in garnet in zoisite-eclogites (Fig. 3c). With a decrease in garnet content (approximately <10 vol. %) and an increase of the jadeite component in the clinopyroxene (approximately >70 mol %), the metabasic eclogites grade continuously into jadeitic-clinopyroxenites. Other minerals that occur in trace amounts in both xenolith types are phengite, pyrite, rutile, zircon and apatite. Rare chlorite, albite and barite occur as <5 µm crystals around garnet and clinopyroxene. In both eclogite types, coesite occurs as <20 µm inclusions in garnet crystals, but not in the matrix (Fig. 3a; Usui et al., 2002
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Occurrence, textures and compositions of minerals
Garnet
Garnet commonly occurs in small clusters or in thin layers accompanied by lawsonite and zoisite; these generally have euhedral to subhedral outlines with maximum diameters of
0·11·0 mm (Figs 2a and 3a). They are commonly color-zoned, from pink cores to reddish brown rims under plane-polarized light (Fig. 2d). Some grains exhibit rotation textures and contain fine-grained curved inclusion trails of coesite and rutile, indicating that deformation continued after the development of a planar tectonic fabric (Fig. 2d) (see also Helmstaedt & Schulze, 1991Garnets have compositions of Alm (Almandine)5070, Sps (Spessartine)<1, Pyr (Pyrope)1030, Grs (Grossular)20, except for locally developed pyrope-rich rims (Table 3 and Fig. 4). These pyrope-rich rims have distinctively different compositions from the other parts of the garnet, indicating a sharp compositional boundary (Fig. 2a). The compositions of these pyrope-rich rims are about Alm40Sps<1Pyr50Grs10 for the lawsonite-eclogite and Alm40Sps<1Pyr40Grs20 for the zoisite-eclogite. The rims may have formed under higher temperature conditions when the xenoliths were entrained in the microbreccia host rock, as will be discussed later, and are called reaction rims, to distinguish them from normal rims the composition of which is almost identical to those of the core and mantle (Table 4).
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In some particularly zoisite-rich eclogites (e.g. MR4, see Table 2), wide reaction rims are present around most garnet crystals, and also penetrate into the garnet cores along cracks (Fig. 3b). The chemical compositions of these garnets in the zoisite-rich eclogites trend toward those of the reaction rims in the (Alm + Sps)PyrGrs diagram (Fig. 4b). In contrast, no reaction rims were observed in jadeitic-clinopyroxenites, which have little or no lawsonite and zoisite, although some garnets have slightly pyrope-rich compositions (Figs 4c and 5a).
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The major element compositions of the garnet, except for the reaction rims, are more similar to those from eclogites in subduction-related metamorphic terranes (Low-Temperature eclogite) than to those from diamondiferous kimberlite pipes (High-Temperature eclogite) (Carswell, 1990
Clinopyroxene
Clinopyroxene is generally prismatic, and its orientation defines the rock fabric. In thin section it varies in color from colorless to pale green under plane-polarized light. The grain size varies as a result of deformation and synkinematic recrystallization (Helmstaedt & Schulze, 1988
). Clinopyroxene grains in the eclogites have compositions near Jd (Jadeite)4050, Aug (Augite)5060, Ac (Acmite)08, falling into the range of omphacite compositions (Table 4, Fig. 6a and b). On the other hand, clinopyroxenes in the jadeitic-clinopyroxenites have compositions of Jd65Aug20Ac15 to Jd75Aug20Ac5. This variation suggests relatively linear jadeite to acmite substitution (Fig. 6c). Clinopyroxene occurs both as inclusions in garnet (referred as included clinopyroxene)and in the matrix (referred to as matrix clinopyroxene; Figs 2c and 3a). Included clinopyroxene grains are richer in Ac and poorer in Jd components than matrix clinopyroxene grains, and their composition varies linearly between Jd35Aug50Ac15 and Jd40Aug55Ac5 (Fig. 6a and b).This trend is also a jadeite to acmite substitution but it differs from the compositional variations of the matrix clinopyroxene.
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Lawsonite and zoisite
Lawsonite is transparent in plane-polarized light. Except for minute inclusions in garnet crystals in the zoisite-eclogite (Fig. 3c), lawsonite is restricted to lawsonite-eclogite. It is invariably rimmed by fine-grained zoisite aggregates (Fig. 2b). Lawsonite grains display relatively uniform compositions close to the ideal formula of CaAlSi2O7(OH)2·H2O, with limited substitution of Fe3+ for Al and (Na + K) for Ca (Table 5; e.g. Moore & Liou, 1979
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Zoisite invariably occurs as fine-grained, fibrous and radiating crystal aggregates in eclogite and some jadeitic-clinopyroxenites (Figs 2 and 3). Whereas the zoisite crystals themselves are transparent, the aggregates are dark brown in plane-polarized light. The grain size of zoisite is generally <10 µm along the major axis and <1 µm along the minor axis, and is much smaller than that of the other constituent minerals, garnet, clinopyroxene, lawsonite, phengite and rutile. It contains 39·740·2 wt % SiO2, 32·632·3 wt % Al2O3, 23·624·2 wt % CaO, and trace amounts of Fe2O3, MgO, TiO2, Na2O and Cr2O3 (Table 5). The textures and major element composition of zoisite are almost identical in lawsonite-eclogite, zoisite-eclogite and jadeitic-clinopyroxenite. Zoisite aggregates also occur as inclusions in fractured garnet preserving the sharp crystal boundaries of euhedral lawsonite pseudomorphs (Fig. 3d), suggesting that the zoisite aggregates originated by replacement of lawsonite.
Other minerals
Phengite occurs in one eclogite (GR1) and two jadeitic-clinopyroxenite (MR21 and MR3B) samples. Grains are platy and up to 0·5 mm in diameter, have relatively homogeneous major element compositions and are characterized by Si values of
7·5 p.f.u. (per formula unit, O = 22; Table 6). In jadeitic-clinopyroxenite samples, albite occurs as a secondary phase along clinopyroxene grain boundaries and rarely along cleavages. The mode of albite is <0·1 vol. %, and it contains <1 % of Or and An components. Orthoclase is present only as inclusions in the core of a garnet from eclogite MR7. Its composition is close to the ideal formula of KAlSi3O8 (Table 6). Amphibole does not occur in any of our metabasic eclogite xenoliths.
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Trace element compositions of minerals
Garnets from eclogites and jadeitic-clinopyroxenites are characterized by extreme LREE (light rare earth element) depletion and HREE (heavy rare earth element) enrichment, exceeding a chondrite-normalized Yb/Ce ratio of 104 (Fig. 8). Garnets have REE patterns that appear to increase progressively from La to Dy and are convex-upward from Dy to Lu, except for the reaction rim. The REE patterns of the reaction rims differ in shape from those in other parts of the garnet; they are characteristically convex-upward from La to Dy and concave-downward from Dy to Lu. LREE (La, Ce, Pr and Nd) and MREE (middle rare earth elements: Sm, Eu, Gd and Dy) contents are mostly uniform throughout the crystal, whereas HREE (Er, Yb and Lu) contents are markedly zoned (Fig. 8). The HREE are more abundant in the core relative to the rim, and show a strong correlation with Mn contents (Fig. 9). Garnets in all of the xenoliths are rich in Y, which decreases from core to rim, similar to the HREE (Table 7). Other trace element data for garnet measured by ICP-MS are listed in Table 10.
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The clinopyroxenes show two groups of trace element compositions (Fig. 8). The LREE, MREE and Sr contents of clinopyroxenes are higher in eclogite than jadeitic-clinopyroxenite. On the other hand, the HREE and Y contents of clinopyroxenes in eclogite are slightly lower than those of counterparts in jadeitic-clinopyroxenite (Table 8 and Fig. 8). Clinopyroxene in eclogite has REE patterns that are convex-upward from La to Dy and concave-downward from Dy to Lu. Such HREE characteristics are only weakly developed in clinopyroxene from the jadeitic-clinopyroxenites. In particular, no HREE depletion is observed in jadeitic-clinopyroxenite MR47 that contains <0·1 vol. % of garnet. Clinopyroxenes in both eclogite and jadeitic-clinopyroxenite are poor in HFSE (Zr <1 ppm and Nb <0·001 ppm; Table 8). Other trace element data for clinopyroxene measured by ICP-MS are listed in Table 10.
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Lawsonite and zoisite are rich in incompatible trace elements, especially U, Th, Pb, LREE and Sr. They are poor in high field strength elements (HFSE), similar to clinopyroxene (Tables 9 and 10). Matrix lawsonite from the lawsonite-eclogite sample has trace element abundances similar to those of matrix zoisite (Fig. 8e). The matrix lawsonites appear unzoned in trace elements, and the trace element abundances are almost identical among the matrix lawsonite grains in each sample. However, matrix and included lawsonites display different REE patterns. Matrix lawsonites exhibit gently convex-upward LREE-enriched patterns from La to Er and relatively unfractionated patterns from Er to Lu. Included lawsonite grains have fairly flat REE patterns that decease slightly from La to Lu (Fig. 8). The trace element patterns of zoisite grains in eclogite and jadeitic-clinopyroxenite vary from sample to sample. For example, zoisite from apatite-bearing zoisite-eclogite MR7 contains less LREE than other zoisites (Fig. 8). This may reflect equilibration with apatite that is REE-rich (Usui, 2004
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Whole-rock chemistry
Major element whole-rock compositions (Table 11) are plotted against SiO2 contents in Fig. 10. Compositions of fresh and altered mid-ocean ridge basalt (MORB) from ocean-floor drilling holes 504B and 417D (Tual et al., 1985
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Whole-rock chondrite-normalized REE patterns of eclogite and jadeitic-clinopyroxenite xenoliths are shown in Fig. 12; altered MORB from ocean-floor drilling hole 504B is shown as a shaded field for comparison. Eclogites have LREE-enriched patterns that decrease progressively from La to Lu, resulting in chondrite-normalized abundance ratios [La/Lu]N = 6·011 and [La/Sm]N = 2·53·3 that are distinctively greater than those of altered MORB (Table 11). In addition to the higher abundance ratios, LREE concentrations are higher in the eclogite than in altered MORB. Jadeitic-clinopyroxenites display V-shaped REE patterns with the lowest normalized abundances at Eu. Although jadeitic-clinopyroxenites exhibit variable LREE contents, which are lower than those of the eclogites, their chondrite-normalized [La/Sm]N ratios are relatively constant and similar to those of the eclogite xenoliths. The REE patterns of eclogite and jadeitic-clinopyroxenite xenoliths are probably controlled by the modes of garnet and zoisite (or lawsonite), which have extremely different REE characteristics (Fig. 8). HFSE abundances are almost identical between eclogite and jadeitic-clinopyroxenite. The Zr/Hf and Nb/Ta ratios of the xenoliths vary from 36·9 to 37·6 and from 10·9 to 15·0, respectively. Both fall in the range of altered MORB, although the contents of these elements in the xenoliths are slightly higher than those of altered MORB (David et al., 2000
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SrNdPb isotopic compositions
Whole-rock Sr, Nd and Pb isotopic data were age-corrected to 30 Ma (Table 12), the emplacement age of the host rock at Moses Rocks and Garnet Ridge (Naeser, 1971
Nd,
Nd206Pb/204Pb, 206Pb/204Pb207Pb/204Pb and 206Pb/204Pb208Pb/204 diagrams (Fig. 13). The isotopic compositions of Juan de Fuca MORB and Phanerozoic Cordilleran crust, which represent Farallon MORB and its sedimentary cover, respectively, are shown for comparison.
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The Sr isotopic ratios of the eclogites and jadeitic-clinopyroxenites vary (87Sr/86Sr = 0·70500·7084) and are greater than those of MORB. The jadeitic-clinopyroxenites have much higher Sr isotopic ratios than the eclogites. In contrast, the Nd isotopic compositions are similar in both eclogites and jadeitic-clinopyroxenites;
Nd values vary from 3·1 to 1·2, much less than those of MORB, but similar to those of crustally derived sediments. Eclogites and jadeitic-clinopyroxenites have Pb isotopic compositions (206Pb/204Pb = 18·9119·38, 207Pb/204Pb = 15·6215·68, and 206Pb/204Pb = 38·6838·92) that fall in the compositional field of sedimentary rocks in 206Pb/204Pb207Pb/204Pb and 206Pb/204Pb208Pb/204Pb diagrams (Fig. 13). In addition to the whole-rock data, RbSr, SmNd and UThPb isotopic studies were also performed on garnet, clinopyroxene and zoisite mineral separates from the xenoliths (Table 13). The Pb isotopic compositions of garnet were not measured because of its extremely low Pb contents (0·0380·087 ppm; see Table 10). Reference isochrons at 30 Ma were calculated to pass through each mineral in the 87Sr/86Sr87Rb/86Sr, 143Nd/144Nd147Sm/144Nd and 206Pb/204Pb238U/204Pb isotopic systems to distinguish isotopic equilibrium and disequilibrium at 30 Ma (Fig. 14). If one mineral was isotopically in equilibrium with another when the host diatremes were emplaced, the reference isochrons for the two minerals should be coincident within error. The slope of the reference isochron for the RbSr system is almost horizontal because of the small variation of Rb/Sr ratio.
|
|
Figure 14a and b shows RbSr isochron diagrams for representative eclogite sample MR19 and jadeitic-clinopyroxenite sample MR26; the diagrams include both mineral and whole-rock data. Both whole-rock values of 87Sr/86Sr are greater than those of the constituent minerals, although the minerals in the eclogite xenolith have almost identical Sr isotopic compositions. Individual minerals in the jadeitic-clinopyroxenite have different isotopic compositions, suggesting that they were not in equilibrium with each other at 30 Ma.
The reference SmNd isochrons for all minerals and the whole-rock of eclogite are coincident within error (Fig. 14c), but garnet from the jadeitic-clinopyroxenite has a different Nd isotopic composition from the other minerals and the whole-rock (Fig. 14d). Zoisites display almost identical Sm/Nd abundance ratios and Nd isotopic compositions to those of the whole-rocks because they are the dominant reservoir for LREE in both eclogite and jadeitic-clinopyroxenite (as discussed later; see Fig. 15).
|
The Pb isotopic compositions of clinopyroxene in the eclogite xenoliths are almost in equilibrium with zoisite at 30 Ma (Fig. 14e). In contrast, the Pb isotopic compositions of clinopyroxene and zoisite in jadeitic-clinopyroxenite are not in equilibrium with each other at 30 Ma. Such features are weakly observed in the other U-series isochron diagrams (207Pb/204Pb235U/204Pb and 208Pb/204Pb232Th/204Pb). Although zoisite is the dominant host of U and Pb, it has distinctively different Pb isotopic compositions and U/Pb abundance ratios from those of the whole-rocks. This might be explained by the presence of zircons with extremely high 238U/204Pb (>106) and 206Pb/204Pb (>103) (Usui, 2004
| DISCUSSION |
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Evidence for high-P/T prograde metamorphism
The compositional zoning structure of garnet and the inclusion assemblages within garnet grains in eclogites and jadeitic-clinopyroxenites preserve information about a certain range of the PT history of the xenoliths. The Sps component of garnet in both xenolith types is markedly zoned and preserves a fine euhedral structure (Fig. 5). Mn zoning of this type is not observed in other mantle-derived eclogite xenoliths; however, it is common in garnet-bearing regional metamorphic rocks that have undergone prograde metamorphism (e.g. Atherton & Edmunds, 1966
Included clinopyroxenes are richer in Ac and poorer in Jd contents than matrix clinopyroxene (Fig. 6). This probably reflects jadeiteacmite substitution. Clinopyroxene generally becomes more jadeitic and less acmitic with increasing pressure and temperature in the upper blueschist to eclogite facies (Maruyama & Liou, 1988
). Most included lawsonite grains have higher Fe2O3 and lower Al2O3 contents than matrix lawsonite (Fig. 7). Maruyama & Liu (1988)
reported negative correlations between Fe3+ and Al molar abundances in lawsonite during progressive metamorphism at blueschist facies: Fe3+ content decreases with increasing pressure and temperature. Thus, included clinopyroxene and lawsonite probably formed in a lower pressure and temperature metamorphic environment than matrix clinopyroxene and lawsonite.
Garnet grains from the Colorado Plateau eclogites contain curved trails of fine-grained coesite and rutile inclusions (Fig. 2d), indicating the former presence of a planar tectonic fabric (see also Helmstaedt & Schulze, 1988
, 1991
). Such textures do not commonly form by magmatic processes, but are commonly found in regional metamorphic suites, such as those of Corsica and the Franciscan metamorphic complex of the western USA, which are known for their occurrences of high-pressure and low-temperature eclogites (Caron & Pèquignot, 1986
; Maruyama & Liou, 1988
). Thus, the inclusions indicate that the immediate protolith of the eclogite xenoliths was a fine-grained foliated rock, probably a blueschist.
In summary, garnet crystals grew during prograde metamorphism, and successively captured minerals such as clinopyroxene and lawsonite, reaching peak metamorphic conditions ranging from 560 to 700°C at 3 GPa and to 600 to 760°C at 5 GPa (Usui et al., 2003
). Such high-Plow-T environments, which are colder than typical mantle geotherms, can be achieved only in subducted oceanic lithosphere. Therefore, we propose that the Colorado Plateau eclogite xenoliths formed by prograde metamorphic recrystallization of subducted oceanic crust.
Retrogression of eclogite xenoliths during emplacement
The Colorado Plateau eclogites were entrained within and rapidly transported to the surface by the host ultramafic microbreccia diatremes during the Tertiary (
30 Ma). The eclogite xenoliths exhibit less retrograde overprinting than subduction-related eclogites from high-pressure metamorphic terranes, as indicated by the absence of amphibole. However, some modifications resulting from xenolithhost-rock interaction are observed. In the lawsonite-eclogite xenoliths, the lawsonite grains are invariably rimmed by zoisite, and, in the zoisite-eclogite xenoliths, the lawsonite is totally replaced by zoisite. Although similar replacement reactions of lawsonite are commonly observed in lawsonite-bearing eclogites from regional metamorphic belts (e.g. Zack et al., 2004
), the mineral products and their textures in the regional metamorphic eclogites are different from those in the Colorado Plateau eclogite xenoliths. Whereas lawsonite pseudomorphs in the Colorado Plateau eclogite xenoliths contain only fibrous and radiating zoisite aggregates, those in regional metamorphic eclogites are replaced by well-crystallized multiple mineral phases, such as epidote, paragonite, phengite and albite (Zack et al., 2004
). Because lawsonite is stable at lower-T and higher-P conditions than these replacing minerals (e.g. Schmidt & Poli, 1998
; Poli & Schmidt, 2002
), breakdown of lawsonite could occur as a result of increasing temperature and/or decreasing pressure during a retrogression event. The petrographical difference in lawsonite pseudomorphs between the Colorado Plateau eclogite xenoliths and regional metamorphic eclogites may reflect the nature of the PT path of retrograde metamorphism. The radiating and fibrous textures of zoisite and preservation of lawsonite in the Colorado Plateau eclogite xenoliths suggest that the zoisite crystallized rapidly by replacement of lawsonite under disequilibrium conditions, probably during the transport of the lawsonite-eclogites in the host rocks.
The textures and major element compositions of zoisite are almost identical in both lawsonite- and zoisite-eclogite xenoliths (Figs 2 and 3 and Table 5). Moreover, zoisite-eclogite xenoliths lack matrix lawsonite but contain included lawsonite in unfractured garnet (Fig. 3c). Thus, the textural and mineralogical differences between the lawsonite- and zoisite-eclogites could reflect varying extents of recrystallization induced by the host rock. Both types of eclogite xenoliths could, therefore, have been originally lawsonite-eclogites.
Garnet compositions are almost uniform within individual mineral grains, except for variations in the Mg/Fe ratio in some reaction rims (Figs 2a and 5). Such rims display extremely pyrope-rich compositions relative to other parts of the garnet, suggesting that they crystallized at higher temperature conditions than the rest of the grain. The reaction rims are well developed in zoisite-rich eclogite. Moreover, the pyrope-rich compositions are also observed along cracks within the garnet grains that connect to lawsonite pseudomorphs (Fig. 3b). On the other hand, such reaction rims are not found in jadeitic-clinopyroxenite xenoliths, which have little or no zoisite aggregate after lawsonite. Formation of the reaction rim was probably related to the alteration of lawsonite to zoisite, which liberated fluid that catalyzed the reaction.
Heterogeneous trace element distributions in the subducted oceanic crust
Colorado Plateau eclogite xenoliths have been interpreted to represent fragments of the subducted Farallon plate (probably altered oceanic crust) that underwent high-P/T metamorphism in the lawsonite eclogite facies (Usui et al., 2003
). Therefore, the compositions of the xenoliths should carry a record of the trace element characteristics of the subducted oceanic crust in the Farallon plate. In this study, we have determined element distributions of Rb, Sr, Sm, Nd, U, Th and Pb between the constituent minerals, garnet, clinopyroxene and zoisite. RbSr, SmNd and UPb isotopic systematics of both constituent minerals and whole-rocks allows the degree of isotopic equilibrium and disequilibrium to be evaluated.
Mass balance calculations were performed by comparing the measured whole-rock data with calculated whole-rock data. The calculated whole-rock data were obtained by multiplying density-weighted modal abundances of the constituent minerals by their trace element concentrations, and summing each mineral's contribution. The ICP-MS analyses for separated minerals were used as average values for the trace element contents of each mineral (Table 10). Differences between measured and calculated whole-rock compositions may point to undetected accessory phases. The calculations also indicate the dominant carriers of each trace element. Figure 15 shows the results of the calculations for zoisite-eclogite MR19 and jadeitic-clinopyroxenite xenolith MR26.
Mass balance can be achieved only for HREE; garnet controls the HREE and Y budgets of the whole-rock. Although zoisite hosts the other REE (especially LREE), Sr, Th and Pb, the calculated whole-rock compositions of these elements are more than twice as much as those of the measured whole-rock compositions. These overestimates of calculated compositions against measured compositions might be caused by overestimates of the modal proportions of zoisite. For modal proportion determinations by optical microscope, areas of lawsonite pseudomorphs that were totally replaced by zoisite aggregates were defined as zoisite. Because fine-grained and radiating zoisite aggregates cannot be completely embedded in the lawsonite pseudomorphs owing to their morphology (Figs 2 and 3), the modal proportion of zoisite is likely to be overestimated. The obvious deficits of Cs, Rb and Ba can be explained by the lack of analyses of phengite for Cs, Rb and Ba, and barite for Ba. These deficits are observed in the jadeitic-clinopyroxenite (Fig. 15). Barite could have been formed by surface weathering after exhumation of the xenoliths to the surface by the host-rock emplacement, because it has not been found as part of the primary mineral assemblage of the eclogites and occurs only as fine-grained crystals along the grain boundaries of the other primary minerals, such as garnet and clinopyroxene. The deficit for U cannot be explained and might be attributed to the presence of an unknown U-enriched phase.
Our results for trace element distributions in the Colorado Plateau eclogite xenoliths are generally consistent with previous studies regarding eclogite samples from regional metamorphic belts (Tribuzio et al., 1996
; Zack et al., 2002a
, 2002b
; Spandler et al., 2003
). In some regional metamorphic eclogites and garnet-amphibolites, allanite dominates the whole-rock REE, U and Th budgets, instead of lawsonite and zoisite (Sorensen & Grossman, 1989
, 1993
; Tribuzio et al., 1996
). This reflects the difference in metamorphic pressure and temperature conditions between these regional metamorphic eclogites and the Colorado Plateau eclogite xenoliths. The regional metamorphic eclogites underwent lower-P and/or higher-T metamorphic conditions than our xenoliths, in which neither lawsonite nor zoisite was stable.
We tested for isotopic equilibrium among the constituent minerals by examining the RbSr, SmNd and UThPb systematics of both minerals and whole-rocks. The mass balance calculations suggest that, except for U, these elements are concentrated almost exclusively in the zoisite that crystallized during xenolith emplacement (Fig. 15). This means that zoisite and the whole-rock should plot close together in the isochron diagrams or, if this is not the case, another phase with extremely different isotopic compositions and element ratios, not accounted for in the mass balance, must be suspected in the rocks. The former case was observed in the SmNd isochron diagram, and the latter in both the RbSr and UPb diagrams.
As seen in the RbSr isochron diagrams (Fig. 14a and b), the whole-rock 87Sr/86Sr isotopic ratios are distinctly higher than those of zoisite. This discrepancy could be explained by the presence of barite crystals, which contain abundant Sr (up to 20 wt % as Sr oxide). Differences in 87Sr/86Sr between whole-rock and zoisite are much larger in the jadeitic-clinopyroxenite. This may reflect differences in the contributions of barite to the whole-rock Sr budget between eclogite and jadeitic-clinopyroxenite, because eclogite contains more zoisite, which dominates the whole-rock Sr, than jadeitic-clinopyroxenite.
For the 238U206Pb isochron diagrams, the whole-rocks of both zoisite-eclogite and jadeitic-clinopyroxenite plot far from the zoisites and their reference isochrons (Fig. 14e and f). This discrepancy is explained by the presence of young zircons (3381 Ma) with high 238U/204Pb (>106) and 206Pb/204Pb (>103) ratios (Usui, 2004
). Although these zircons should also affect the whole-rock data for 235U207Pb and 232Th208Pb systematics, their isotopic signatures are not clearly observed in the 235U207Pb and 232Th208Pb isochron diagrams, because the natural abundance ratio of 235U/238U is low (1/137·88) and contents of Th are lower than those of U.
The zoisite-eclogite xenolith MR19 consists of garnet, clinopyroxene and zoisite that equilibrated at 30 Ma, the age of emplacement of the host diatreme, although the Sr isotopic composition of the zoisite is slightly higher than those of the other minerals (Fig. 14a, c and e). The mineral isochron ages for zoisite-eclogite xenoliths are 39 ± 11 Ma for the 147Sm/144Nd143Nd/144Nd isochron diagram, and 33 ± 20 Ma for the 238U/206Pb207Pb/206Pb isochron diagram. Despite large errors, both of the mineral isochron ages are consistent with the UPb ages of zircons in the zoisite-eclogites (Usui et al., 2003
), and with the emplacement ages of the host diatremes (Naeser, 1971
; Helmstaedt & Doig, 1975
; Roden et al., 1979
). On the other hand, it is difficult to obtain meaningful isotopic ages from the 87Rb/86Sr87Sr/86Sr, 147Sm/144Nd143Nd/144Nd and 238U/206Pb207Pb/206Pb isochron diagrams for jadeitic-clinopyroxenite xenolith MR26 (Fig. 14b, d and f). If clinopyroxene and garnet in MR26 were isotopically homogenized, the pair should yield identical isochron ages among the different isotopic systems. However, this is not the case, and the ages obtained for 87Rb/86Sr87Sr/86Sr and for 147Sm/144Nd143Nd/144Nd are 492 ± 27 Ma and 42·4 ± 6·7 Ma, respectively. Moreover, mineral isochron ages obtained for zoisite combined with garnet and clinopyroxene are geologically unreasonable (for example, the zoisiteclinopyroxene mineral isochron age in the 87Rb/86Sr87Sr/86Sr system is 13 400 ± 700 Ma).
The differences in mineral isochron ages between the zoisite-eclogite and the jadeitic-clinopyroxenite are related to the amount of fluid that was generated by lawsonite breakdown to zoisite aggregates during diatreme emplacement. Fluid not only catalyzes metamorphic reactions, but it also facilitates rapid mass transport. In the zoisite-eclogite xenoliths, the availability of fluids evidently allowed the recrystallization of zircons, which yield UPb concordia ages almost identical to those of microbreccia intrusion (Usui et al., 2003
). Because the zoisite-eclogite contains abundant zoisite aggregates that were originally lawsonite, isotopic homogenization was probably facilitated by the presence of fluids, which evidently induced recrystallization of parts of garnet and clinopyroxene and caused diffusive isotopic resetting preferentially along cracks and grain boundaries. Petrographic observations indicate that almandine-rich garnet in the zoisite-eclogites recrystallized pyrope-rich compositions not only at the rim, but also along cracks into the garnet cores (Fig. 3b). Thus, all the mineral isochron ages and the UPb zircon ages in the zoisite-eclogite represent the emplacement age of the microbreccia diatreme.
In contrast, the jadeitic-clinopyroxenites contain little or no zoisite, reflecting a lawsonite-poor precursor. This lack of prograde lawsonite resulted in little or no fluid production during retrogression associated with the microbreccia emplacement. The experimentally determined volume diffusion rates for Pb and Nd in clinopyroxene (Sneeringer et al., 1984
; van Orman et al., 1998
; Cherniak, 2001
) are too slow to have changed the isotopic ratios during diatreme emplacement without a fluid phase. In the absence of fluids, minerals have been shown to preserve their isotopic signatures far above their commonly accepted closure temperatures, even for time scales of entire orogenic metamorphic episodes (Farquhar et al., 1996
; Tilton et al., 1997
; Kelley & Wartho, 2000
). Therefore, the constituent minerals in the jadeitic-clinopyroxenite xenoliths were probably not in equilibrium, and their mineral isochron ages are, thus, meaningless. Fortunately, however, the isotopic compositions of these minerals allow us to infer the pristine isotopic compositions of subducted oceanic crust prior to isotopic homogenization by diatreme emplacement.
Infiltration of metasomatizing fluids derived from sedimentary rocks
Although the chemical compositions of lithologies likely to be subducted (i.e. variably altered oceanic crust and overlying sedimentary cover) have been well investigated by ocean-floor drilling (e.g. Alt, 1995
), chemical characterization of the subducted lithologies remains relatively poorly studied. In particular, there are few reliable datasets for the Sr, Nd and Pb isotopic compositions of subducted materials (e.g. Bernard-Griffiths & Cornichet, 1985
; Thöni & Jagoutz, 1992
; Becker et al., 2000
). Such data could be used to constrain whole-mantle and individual subduction-zone chemical recycling models, and to explain the enriched isotopic signatures of OIB and island arc magmas (e.g. Hofmann, 1997
; Shibata & Nakamura, 1997
; Taylor & Nesbitt, 1998
; van Keken et al., 2002
). In this section, we discuss the isotopic and trace element compositions of the subducted materials, based on the geochemical datasets obtained from the Colorado Plateau eclogite xenoliths.
Both the eclogite and jadeitic-clinopyroxenite xenoliths from the Colorado Plateau, which are interpreted to represent subducted oceanic crust, exhibit geochemicallyenriched Sr, Nd and Pb isotopic compositions and whole-rock trace element patterns (Figs 12 and 13).Because the whole-rock trace element abundances of the xenoliths are likely to have been modified by hydrothermal alteration at the mid-ocean ridge, where the MORB protolith formed, and by metasomatism during subduction (Becker et al., 1999
, 2000
), they cannot be used to constrain their protoliths, e.g. normal-type MORB (N-MORB) or enriched-MORB (E-MORB). In addition, we cannot discount the possibility that the xenoliths represent fragments of OIB, similar to Hawaiian tholeiites and associated subalkaline rocks, which probably occurred sporadically on the Farallon plate. However, the eclogite and the jadeitic-clinopyroxenite xenoliths have almost constant Zr/Hf ratios ranging from 36·9 to 37·6 (Table 11). Such values are consistent with all types of MORB, but not with OIB (David et al., 2000
). The MORB-like Zr/Hf ratios of the xenoliths are evidence against a seamount origin, because Zr and Hf are relatively immobile elements, and the Zr/Hf ratios should not change during subduction. Even if any of the different MORB-types are protoliths for the xenoliths, their Sr, Nd and Pb isotopic signatures reflect the addition of an enriched geochemical component to the xenoliths.
The Sr, Nd and Pb isotopic compositions of the constituent minerals of the Colorado Plateau eclogite xenoliths are used to identify the source of the enriched component, because the whole-rock isotopic data were probably contaminated by surface weathering and/or interaction with the microbreccia host rock. A surface weathering effect is seen in the difference between the Sr isotopic compositions of the whole-rocks and those of the constituent minerals (Fig. 13a) and is best explained by the presence of late barite along grain boundaries. Differences in Pb isotopic compositions between whole-rocks and minerals were also observed (e.g. Fig. 13c). If abundant geochemical components originating in the microbreccia transport medium were added to the xenoliths, the mineral isotopic compositions of the eclogite xenoliths would be unusable, because, in contrast to the jadeitic-clinopyroxenite xenoliths, the eclogite minerals reached isotopic equilibrium during diatreme emplacement. However, judging from the REE element patterns of garnet and clinopyroxene (Fig. 8), such magmatic influences on the geochemistry of the constituent minerals of the xenoliths were probably small. Therefore, the mineral isotopic signatures observed not only the jadeitic-clinopyroxenite but also in the eclogite xenolith could represent the Sr, Nd and Pb isotopic compositions of the subducted basaltic oceanic crust.
The Sr, Nd and Pb isotopic compositions of the constituent minerals in the xenoliths are thought to reflect mixing between an altered MORB component and a sedimentary component, based on considerations of the possible lithologies subducted with the protolith of the xenoliths in the Farallon plate (Fig. 13). The isotopic variations could have resulted from combining heterogeneous sedimentary components with variably altered MORB in variable mixing ratios. Such mixing cannot be explained by mechanical mixing between metasedimentary rocks and altered MORB crust, because a mechanical mixing model is inconsistent with the basaltic bulk-rock major element composition of the xenoliths. Instead, it requires metasomatic alteration induced by migration of a fluid from sedimentary layers to the basaltic protolith. Because the quantity of fluids and fluid mobility are limited in high-grade metamorphic conditions (e.g. Scambelluri & Philippot, 2001
) metasomatism probably occurred at an early stage of subduction. At shallow levels (<10 km depth), large volumes of predominantly sedimentary rock and detritus accumulate in accretionary wedges, occurring in many subduction complexes as mélange-like material between the slab and the hanging wall (Shreve & Cloos, 1986
). Such subduction mélanges contain mafic and ultramafic blocks showing varying extents of metasomatic alteration as a result of infiltrating aqueous fluids (Sorensen, 1988
; Sorensen & Grossman, 1989
, 1993
). Although the Colorado Plateau eclogite xenoliths might not have been derived from mafic blocks in a mélange unit, studies of mélanges yield insights into the metasomatic mixing process. Detailed isotopic studies of a subduction mélange unit (Bebout, 1991
) have suggested that large amounts of aqueous fluid, previously equilibrated with metasedimentary rocks, enter the maficultramafic mélange, and produce large-scale stable isotopic homogenization and pervasive metasomatism. Therefore, in the fore-arc region, the protolith of the eclogite and jadeitic-clinopyroxenite xenoliths could have been metasomatized by large volumes of fluid derived from associated metasedimentary units.
Reassessment of Precambrian model ages
The Colorado Plateau eclogite xenoliths have distinctively lower
Nd values than MORB at any time in the Phanerozoic (Roden et al., 1990
; Wendlandt et al., 1993
; this study). Wendlandt et al. (1993)
applied SmNd isotope systematics to determine the age of oceanic lithosphere that could have contributed to the protolith of the Colorado Plateau eclogite xenoliths. The Nd isotopic compositions and Sm/Nd ratios of the xenolith samples were used to calculate the time at which the xenolith would have the
Nd value of the depleted mantle evolution curve proposed by DePaolo et al. (1991)
. However, the Nd isotopic compositions as well as the Sm/Nd ratios of MORB can be modified by subduction-related metasomatic events after extraction of the MORB melts from the depleted mantle at a mid-ocean ridge (e.g. Jahn et al., 1996
). As discussed above, the Colorado Plateau eclogite xenoliths were metasomatized by large amounts of fluid that were isotopically equilibrated with metasedimentary rocks. To obtain accurate Nd model ages, Wendlandt et al. (1993)
selected less altered eclogite xenoliths based on their whole-rock chemistries. Nevertheless, these eclogite xenoliths have weak V-shaped REE patterns and distinctively higher [La/Sm]N ratios (0·971·29) than those of MORB, suggesting that even they have undergone metasomatism. Thus, Nd model ages are an unsatisfactory measure of the protolith age for the Colorado Plateau eclogite xenoliths.
Smith et al. (2004)
reported Proterozoic UPb zircon ages from the Colorado Plateau eclogite xenoliths. Nine multigrain zircon fractions were analyzed with TIMS following the chemical separation of Pb and U. Four of the nine multigrain zircon fractions almost plot on the concordia growth curve and yield ages from 35 to 70 Ma, consistent with the age range reported by Usui et al. (2003)
. The other five multigrain zircon fractions were discordant. Smith et al. (2004)
selected seven multigrain zircon fractions from the nine fractions, and then obtained a poorly fit discordia (MSWD = 92) between 34·9 ± 3·3 and 1514 ± 74 Ma. The discordant zircon fractions were interpreted to establish that Colorado Plateau eclogites contained inherited mid-Proterozoic zircons. From this Smith et al. (2004)
concluded that the Colorado Plateau eclogites represent fragments of Proterozoic lithosphere, and that the concordant young ages between 35 and 70 Ma record episodic zircon growth as a result of Mesozoic or Cenozoic eclogite-facies recrystallization of Proterozoic mantle. However, the reliability of the Proterozoic discordant UPb age must be further investigated, because all discordant multigrain zircon fractions plot close to the lower intercept (<10% of concordance from the upper intercept). The Smith et al. (2004)
model is also inconsistent with the euhedral zoning structure of Mn in garnet and the garnet inclusion assemblages described in this paper. These petrographic features are incompatible with the postulated eclogite-facies recrystallization processes in the upper mantle but are better explained by subduction-related prograde metamorphism.
| CONCLUSIONS |
|---|
|
|
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Eclogite and jadeitic-clinopyroxenite xenoliths from the Colorado Plateau consist of garnet, clinopyroxene, lawsonite and zoisite with minor amounts of phengite, rutile, pyrite and zircon. The xenoliths have basaltic whole-rock major element compositions, but significantly higher Na2O with increasing SiO2 contents compared with those of altered MORB. These major element characteristics are interpreted to reflect spilitization during hydrothermal alteration in a mid-ocean ridge environment, followed by subduction-related metasomatism in the fore-arc. Euhedral garnet zoning structures and the major element compositions of included clinopyroxene and lawsonite indicate that the xenoliths underwent subduction-related prograde metamorphism. Fine-grained zoisite aggregates crystallized rapidly, formed by replacement of lawsonite during the transport of lawsonite-eclogite to the surface in the microbreccia host. These petrographic results are consistent with those of Usui et al. (2003)
The whole-rock chemistry of the xenoliths has variable trace element enrichment compared with MORB or altered MORB, except for the Zr/Hf ratio, which ranges from 36·9 to 37·6. Whole-rock mass balance analysis demonstrates the trace element distributions among the constituent minerals in the xenoliths. Garnet is the principal residence site for HREE and Y, and zoisite hosts the other REE (especially LREE), Sr, Th and Pb. In the eclogite xenoliths, garnet, clinopyroxene and zoisite were in approximate isotopic equilibrium at the time of emplacement (
30 Ma). These minerals yield 147Sm143Nd mineral isochron ages of 39 ± 11 Ma and 238U206Pb ages of 33 ± 20 Ma. In contrast, the same minerals in the jadeitic-clinopyroxenite xenoliths were not in isotopic equilibrium at the time of diatreme emplacement. The fluid released by the breakdown of lawsonite during the entrainment by the microbreccia host may have facilitated isotopic equilibration in the eclogite xenoliths.
Based on the SrNdPb isotope systematics of their constituent minerals, the xenoliths underwent metasomatism by a fluid in equilibrium with sediments in the fore-arc region of the subducting Farallon plate. The metasomatism resulted in the xenoliths acquiring distinctively different isotopic compositions from those of altered MORB despite their altered MORB protoliths; Sr and Pb have more radiogenic and Nd less radiogenic isotopic compositions than those of altered MORB. This suggests that basaltic oceanic crust with an isotopic composition reflecting metasomatism by a fluid in equilibrium with a sedimentary component can be introduced into the sub-arc mantle through subduction zones and could, therefore, explain the sediment-like isotopic signatures of some island arc basalt and ocean island basalts.
| APPENDIX |
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| ACKNOWLEDGEMENTS |
|---|
We are very grateful to S. Maruyama, G. E. Bebout and all of the PML members for their scientific guidance, technical support and valuable discussion. I. Buick and R. L. King are also acknowledged for improving the quality of this paper. We thank J. Selverstone, S. S. Sorensen and T. Zack for constructive reviews of this manuscript, and M. Wilson for editorial handling. This study was financially supported in part by grants from the Ministry of Education, Science, Sports and Culture of Japan (E.N.) and by the program Center of Excellence for the 21st Century in Japan (E.N.).
* Corresponding author. Present address: Department of Earth and Planetary Sciences, University of Tennessee, 1412 Circle Drive, Knoxville, TN 37996, USA. Telephone: +1-865-974-3874. Fax: +1-865-974-2368. E-mail: tusui{at}utk.edu
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, serpentinized ultramafic microbreccia diatremes. Major monoclines with dip directions are also shown. ME, Mule Ear; MR, Moses Rock; CN, Cane Valley; GR, Garnet Ridge; RM, Red Mesa; BP, Buell Park; GK, Green Knobs; SF, San Francisco; LA, Los Angeles.








, jadeitic-clinopyroxenite. Compositional fields of fresh MORB and altered MORB are based on data from Tual et al. (1985)



) in Table A1.



