Journal of Petrology Advance Access originally published online on March 7, 2006
Journal of Petrology 2006 47(6):1147-1175; doi:10.1093/petrology/egl006
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Geochemical Constraints on the Origin of Volcanic Rocks from the Andean Northern Volcanic Zone, Ecuador
1 DEPARTMENT OF GEOLOGICAL SCIENCES, UNIVERSITY OF SOUTH CAROLINA, 701 SUMTER STREET, COLUMBIA, SC 29208, USA
2 INSTITUTO GEOFISICO, ESCUELA POLITECNICA NACIONAL (IG-EPN), APARTADO 17-01-2759 QUITO, ECUADOR
3 EARTH SCIENCES DIVISION, LAWRENCEBERKELEY NATIONAL LABORATORY, 1 CYCLOTRON ROAD, MAIL STOP 90-1116, BERKELEY, CA 94720, USA
4 DEPARTMENT OF GEOSCIENCES, HAMILTON COLLEGE, CLINTON, NY 13323, USA
RECEIVED JULY 25, 2004; ACCEPTED JANUARY 27, 2006
| ABSTRACT |
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Whole-rock geochemical data on basaltic to rhyolitic samples from 12 volcanic centers are used to constrain the role of continental crust in the genesis of magmas formed beneath the anomalously wide subduction-related volcanic arc in Ecuador. Relatively homogeneous, mantle-like, isotopic compositions across the arc imply that the parental magmas in Ecuador were produced largely within the mantle wedge above the subduction zone and not by extensive melting of crustal rocks similar to those upon which the volcanoes were built. Cross-arc changes in 143Nd/144Nd and
7/4Pb are interpreted to result from assimilation of geochemically mature continental crust, especially in the main arc area, 330360 km from the trench. Mixing calculations limit the quantity of assimilated crust to less than
10%. Most andesites and dacites in Ecuador have adakite-like trace element characteristics (e.g. Y <18 ppm, Yb <2 ppm, La/Yb >20, Sr/Y >40). Available whole-rock data do not provide a clear basis for distinguishing between slab-melting and deep crustal fractionation models for the genesis of Ecuador adakites; published data highlighting geochemical evolution within individual volcanoes, and in magmatic rocks produced throughout Ecuador since the Eocene, appear to support the deep fractionation model for the genesis of most evolved Ecuadoran lavas. A subset of andesites, which display a combination of high Sr (>900 ppm),
Nd >4·1 and
7/4Pb <6·0, appear to be the best candidates among Ecuador lavas for slab-melts associated with the subduction of the relatively young, over-thickened, oceanic crust of the Carnegie Ridge. KEY WORDS: andesite; Ecuador; trace elements; isotopes; adakite
| INTRODUCTION |
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It is widely believed that subduction-related andesites form predominantly through the differentiation of basaltic melts and their interaction with arc crust (e.g. Gill, 1981
An alternative view of arc magmatism and andesite genesis has recently grown out of the recognition that in some arcs, especially in places where the subducting lithosphere is young and/or warm, calc-alkaline andesites and dacites may form not only through the differentiation of basaltic magmas, but also through partial melting of basaltic rocks at high pressures in subducting oceanic crust (Kay, 1978
; Saunders et al., 1987
; Defant & Drummond, 1990
; Kay et al., 1993
; Yogodzinski et al., 1995
; Stern & Killian, 1996
; Rapp et al., 1999
; Kelemen et al., 2003
). Andesites and dacites thought to have formed by this mechanism have unusual trace element characteristics, including high Sr/Y (>40) and La/Yb (>20), and low concentrations of Y (<18 ppm) and Yb (<1·9 ppm) compared with common island arc lavas of intermediate composition (Defant & Drummond, 1990
). The geochemically distinctive class of andesites and dacites with these features, now commonly termed adakites (Defant & Drummond, 1990
), was first recognized by Kay (1978)
, who argued that they were formed through a two-step process that involved melting of the subducting oceanic crust in the presence of garnet (to produce the highly fractionated trace element patterns), followed by the interaction of the resulting silicic melt with peridotite in the hot mantle wedge (to form the andesitic and high Mg-number characteristics).
This model has been relatively successful in explaining the genesis of adakitic lavas in island arcs or other arc settings where the crust is relatively thin (Saunders et al., 1987
; Defant et al., 1991
; Morris, 1995
; Yogodzinski et al., 1995
; Stern & Killian, 1996
; Abratis & Wörner, 2001
). Recently however, the model has been applied in areas of thickened continental crust, where the mineral garnet, which plays the central role in generating the highly fractionated trace element patterns seen in adakites (Kay, 1978
; Defant & Drummond, 1990
; Rapp et al., 1999
), may be stable not only in the subducting oceanic plate, but also in the deep crust (e.g. Gutscher et al., 2000
; Beate et al., 2001
; Bourdon et al., 2002
, 2003
). Not surprisingly, studies in this geological setting, in particular in Ecuador, have produced a divergence of opinions, with some researchers focusing on the crust as a major component of northern Andean magmatism (Kilian & Pichler, 1989
; Arculus et al., 1999
; Monzier et al., 1999
), and others advocating processes within the subducting slab and mantle wedge (Barragan et al., 1998
; Gutscher et al., 1999
; Bourdon et al., 2002
, 2003
). Reconciliation of this issue will ultimately determine the extent to which we view widespread andesitedacite volcanism in the northern Andes as juvenile additions to the continental crust, or as recycling of old crust via intra-crustal melting and differentiation.
In this paper we present whole-rock geochemical data, including Pb, Sr, and Nd isotope ratios, for Holocene and Late Pleistocene lavas collected from most of the length and width of the volcanic arc in Ecuador. Because the crust varies greatly in thickness and composition across the arc, from primitive oceanic terranes in the west (basalts and related volcaniclastic rocks) to geochemically mature continental lithologies in the east (granites and metapelites), these data provide a potentially powerful basis for evaluating the role of crustal melting and assimilation in the genesis of adakitic and other volcanic rocks in Ecuador.
| GEOLOGICAL SETTING |
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The spatial distribution of active volcanism in the northern Andes, which is controlled by the convergence of the Nazca and South American plates, undergoes a dramatic series of along-strike changes from central Colombia southward into northern Peru (Fig 1). In southern Colombia, the arc is a relatively narrow volcanic chain (4050 km wide), which is underlain by subducting oceanic lithosphere that dips to the SE at an angle of
30° (Gutscher et al., 1999
120 km, but ends a short distance to the south at Sangay Volcano, in central Ecuador (Fig. 1). In southernmost Ecuador and northern Peru, the subduction zone enters the non-volcanic/flat-slab region (Barazangi & Isacks, 1976
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The north Andean crust that underlies the currently active volcanoes in Colombia and Ecuador varies systematically across the margin with respect to thickness, age, rock type and geochemical maturity (Fig. 2). Estimates based on gravity data indicate that the crustal thickness across Ecuador changes from 2530 km beneath the volcanic front to >50 km beneath the highest elevations of the Eastern Cordillera, with progressive thinning of the basement eastward toward the craton (Feininger & Seguin, 1983
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The geological settings of individual volcanoes in Ecuador can be divided into three cross-arc zones, based on their distance from the trench and on the age, composition, and thickness of the crust upon which they were built (Figs 1 and 2). We refer to these zones as (1) the volcanic front, which lies in the Western Cordillera, 260300 km from the trench, (2) the main arc, which encompasses the Inter-Andean Graben and Eastern Cordillera and lies 300380 km from the trench, and (3) the back-arc area, which lies in the eastern foothills of the Northern Andes at distances greater than
380 km from the trench (Fig. 1).
Surface exposures of basement rocks at the volcanic front are composed primarily of geochemically primitive oceanic basalts and volcanoclastic rocks that were accreted to the northern Andean margin since the mid-Cretaceous. These oceanic terranes include fragments of the Caribbean Plateau as well as geochemically primitive, island-arc-type crustal blocks (Fig. 2; e.g. Feininger, 1987
; Megard, 1989
; Jaillard et al., 1990
, 1997
; Reynaud et al., 1999
; Hughes & Pilatasig, 2002
; Kerr & Tarney, 2005
). The geochemistry of the oceanic basalts is broadly similar to those of the Galapagos and the Carnegie Ridge (Dupré & Echeverria, 1984
; Lapierre et al., 2000
; Kerr et al., 2002
, 2004
; Mamberti et al., 2003
). To the east, the crust beneath the main arc and back-arc becomes progressively older on average, and geochemically more mature, consisting increasingly of granites, schists, and gneisses of mostly late Mesozoic to Paleozoic age (Fig. 2; Aspden et al., 1992
; Aspden & Litherland, 1992
; Litherland et al., 1994
; Noble et al., 1997
). Beneath the back-arc of Ecuador, the volcanoes appear to lie above Precambrian basement. Precambrian rocks are absent from surface exposures, but have been recovered in cuttings from deep oil wells (Feininger, 1987
).
| ANALYTICAL METHODS |
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Whole-rock major and trace element concentrations were determined from fresh samples that were crushed in a steel jaw crusher and ground in agate or Al-ceramic containers. Major elements and some trace elements (Ni, Cr, Cu, V) were determined by X-ray fluorescence (XRF) at the Washington State Geoanalytical Laboratory on a low dilution Li-tetraborate fused bead (Johnson et al., 1999
absolute on all data in Table 2) are dominated by fractionation uncertainty of 0·06%/a.m.u. Seventy-two runs of the NBS-987 isotope standard yielded an average 87Sr/86Sr value of 0·710263 ± 0·000009 (2
). Data listed in Table 2 are corrected to a value of 0·710240 for NBS-987. Twenty runs of the JNdi-1 isotope standard solution yielded an average 143Nd/144Nd value of 0·512110 ± 0·000016 (2
). Data in Table 2 are corrected to a 143Nd/144Nd value of 0·512115 for JNdi-1, consistent with a CHUR value of 0·512635 and an
Nd value of 15·15 for the La Jolla Nd standard, and implying an
Nd value of 10·13 for the JNdi-1 standard (Lugmair & Carlson, 1978
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| RESULTS |
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Basalts and basaltic andesites (Sumaco Volcano)
Basalts and basaltic andesites are rare in the northern Andes, occurring in significant numbers only at Sumaco Volcano (4354 wt % SiO2, Table 1, Fig. 3), located in the back-arc of Ecuador (Fig. 2)
400 km from the trench (Beate et al., 2001
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Based on the above it is clear that the lavas from Sumaco are readily distinguished from all others in Ecuador with respect to major and trace elements (Figs 37). In contrast, the isotopic compositions of the Sumaco samples fall generally within the relatively narrow range of compositions observed in Ecuador (e.g. Harmon et al., 1984
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Andesites and dacites
Medium-K, calc-alkaline andesites and dacites (SiO2 = 55·7665·98%, FeO*/MgO = 1·391·76) are the predominant magma types erupted in Ecuador (Table 1, Fig. 3). Major element contents of MgO (2·006·40 wt %), CaO (4·537·80 wt %), FeO* (3·517·75 wt %) and Na2O (3·184·68 wt %) all show coherent linear trends when plotted against SiO2 (Fig. 3). In contrast, K2O (0·872·99 wt %) varies two-fold across the andesitedacite compositional range and is not correlated with increasing SiO2 (Fig. 3).
Highly incompatible trace elements in the andesites and dacites (Rb, Ba, Ta, Nb, La, etc.) are generally correlated with one another (Fig. 7), but like K2O, are not well correlated with major element differentiation indicators such as SiO2 or MgO (e.g. Fig. 4). Strontium (Sr) and Y, which typically exhibit moderately incompatible behavior in subduction-related lavas, are highly variable in abundance (Sr = 4501200 ppm; Y = 923 ppm), but show no clear relationship when plotted against strongly incompatible elements such as Cs, Rb or Ba. Strontium is similarly uncorrelated with SiO2 but does decrease systematically with decreasing Mg-number [Mg/(Mg + Fe), Fig. 6b]. Yttrium (Y), which is relatively low in abundance in most samples (commonly <15 ppm), generally decreases with increasing SiO2 between 56% and 64% SiO2, indicating that it has behaved as a moderately compatible element during the evolution of these lavas (see also Monzier et al., 1999
, fig. 11). Abundances of strongly compatible trace elements, such as Cr and Ni, are highly variable in the andesites and dacites (Cr up to 240 ppm), and like many of the most incompatible elements, also appear to be largely independent of SiO2 (e.g. Fig. 4).
Ratios among the incompatible elements in the andesites and dacites are clearly characteristic of a subduction zone setting, and in most respects are typical of andesites and dacites throughout the Andes. Ratios of LILE to HFSE (e.g. Rb/Ta, Ba/Nb) are elevated in the andesites and dacites compared with oceanic basalts (Fig. 7). The REE are highly variable with regard to both elemental abundance and pattern shape (Fig. 5). The total range for La/Yb is high (4·338·8; Fig. 10, Table 1), but there is a strong clustering of samples at relatively low La/Yb (610) with a few more highly fractionated samples (only four samples with La/Yb >20; Fig. 10). Among the samples with La/Yb >10, some are clearly depleted in the HREE (Yb <1·0) and have fractionated HREE patterns with normalized Dy/Yb >2·0, whereas others are primarily enriched in the light REE (LREE) and have flatter HREE patterns (Fig. 5a). The most common andesites and dacites have straight and modestly fractionated patterns with La/Yb = 610 and normalized Dy/Yb <2·0 (Fig. 5b). Overall, these REE characteristics do not stand out as unusual compared with andesites and dacites from other parts of the Andes (Fig. 10). Barium (Ba) concentrations are also variable, and Ba/La ratios are relatively high in the andesites and dacites (Ba/La = 2080); in this respect the Ecuadoran lavas are similar to lavas in island arcs but are unlike andesites and dacites of the central and southern Andes, which typically have Ba/La <25 (Fig. 10; Hildreth & Moorbath, 1988
; Davidson et al., 1990
). In addition, nearly all of the andesites and dacites from Ecuador have high Sr/Y (2270; Figs 6a and 10), and according to the criteria of Defant & Drummond (1990)
most would be classified as adakites (see also Beate et al., 2001
; Bourdon et al., 2002
, 2003
; Samaniego et al., 2002
). In this regard again, the rocks from Ecuador are also typical of andesites and dacites from throughout the Andes (Figs 6 and 10).
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Trace element characteristics in the andesites and dacites also change systematically from west to east across the magmatic arc in Ecuador. In general, the average incompatible element concentrations are higher in the main arc and back-arc areas, at greater distances from the trench (Fig. 11a and b). Certain incompatible-element ratios (e.g. Ba/Nb and La/Yb) also change systematically across the arc (Fig. 11c and d; see also Hörmann & Pichler, 1982
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Isotopically, the andesites and dacites from Ecuador define a relatively narrow range of values that fall within the SrNd mantle array and overlap somewhat with Galapagos plume basalts for each of the isotopic systems studied (Sr, Nd, Pb; Figs 8 and 9). Isotope ratios for Sr and Nd (87Sr/86Sr = 0·70400·7044, 143Nd/144Nd = 0·512730·51295; Table 2) lie at the high 143Nd/144Nd end of the field of modern Andean lavas (Fig. 8), and encompass nearly the full range of published values for the Northern Volcanic Zone (Harmon et al., 1984
7/4 Pb, which is a quantitative expression of the deviation in 207Pb/204Pb from the mantle reference line at the 206Pb/204Pb composition of the sample (Hart, 1984
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The isotopic compositions of the andesites and dacites change both east-to-west across the magmatic arc in Ecuador, and with changes in certain trace element parameters. Specifically, 87Sr/86Sr and
7/4 Pb in the Ecuadoran lavas reach their highest values in lavas erupted in the main-arc region (330360 km from the trench), along the crest of the Andes, where the crust is likely to be thickest (Fig. 13). Conversely, 143Nd/144Nd (
Nd) is lowest across this region. It should be noted, however, that the alkali basalts and basaltic andesites from Sumaco Volcano in the back-arc area do not follow the cross-arc isotopic trends of the andesites and dacites (Fig. 13). The isotopic compositions of the andesites and dacites in Ecuador also change systematically with increasing incompatible element concentrations (e.g. decreasing 143Nd/144Nd with increasing Nb, Ba, Rb, La; Fig. 14), and with changes in certain trace element ratios, especially Ba/Nb and La/Yb, and to a lesser extent Ba/La (Fig. 15). In general, the trace elementisotope relationships are clearest for Nd and Pb isotopes, but are absent or less clear when they involve either Sr or 87Sr/86Sr. Finally, there appears to be no clear systematic relationship between any of the isotopic systems and any major element parameter (e.g. SiO2) in the andesitedacite compositional range (Fig. 16).
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Rhyolites
Rhyolites reported here are from Chacana, Chalupas, and Cotopaxi volcanoes, which are all located in the main-arc area, along the crest of the Andes in northern Ecuador (Table 1, Figs 1 and 2). Apart from the obvious gap in silica between approximately 66% and 71% SiO2 (Fig. 3), the major and trace element compositions of the rhyolites from Ecuador appear, in a broad sense, to be extensions of the andesitedacite compositional trends (Figs 35). One exception is in the REE patterns, which are clearly much flatter in the HREE (normalized Dy/Yb <1·50) and have 1857% negative Eu anomalies (i.e. Eu/Eu* = 0·430·82; Fig. 5c). The broad similarity with respect to trace elements does not extend to the isotopic compositions, which on average, are more radiogenic in Pb and Sr and less radiogenic in Nd in the rhyolites than in the andesites and dacites (Figs 8, 9 and 1315). This is to be expected in high-SiO2 melts containing a relatively high proportion of geochemically evolved crustal rock relative to mantle components.
| DISCUSSION |
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Isotopic constraints on crustal components in Ecuadoran lavas
Compared with the central and southern Andes, where the case for substantial melting and assimilation of geochemically evolved crustal rocks has been well documented (e.g. Hildreth & Moorbath, 1988
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Arculus et al. (1999)
It remains possible, of course, based on isotopic data alone, that partial melts of a newly underplated mafic layer at Moho depths (formed from basalts generated in the modern subduction zone and, therefore, isotopically similar to the modern arc lavas), could have contributed significantly to the source of the Ecuadoran lavas. Such an origin, which involves rapid remelting of a recently created (i.e. newly underplated) basaltic layer, has been proposed for Ecuador (Monzier et al., 1999
) and for other areas of thickened crust in the Andes, in particular in the case of the Miocene Cordillera Blanca Batholith in Peru (Petford & Atherton, 1996
). At some level, this process seems inevitable in any vigorously active magmatic arc. It is unlikely, however, that this process has exerted a major influence on magma genesis in the modern volcanic arc in Ecuador, where the lavas are mostly medium-K, calc-alkaline andesites whose major element compositions are unlike those of the silicic, alkali-rich, leucocratic granites that dominate the Cordillera Blanca in Peru (SiO2 >70%, Na2O >4% K2O >3%, MgO <2%, FeO* <2%). The latter appear to have formed by regional-scale melting of underplated basalt during the Miocene (Petford & Atherton, 1996
). The rhyolites of Ecuador have major element compositions that are similar to the Cordillera Blana leucogranites, but they constitute only a small proportion of the surface eruptive rocks, and unlike leucogranites from the Cordillera Blanca, the Ecuadoran rhyolites have relatively flat HREE patterns, which also contrast strongly with Cordillera Blanca mafic and intermediate rocks (e.g. compare Fig. 5 with Petford & Atherton, 1996
, fig. 9).
Having emphasized that the crustal rocks of the northern Andes have played a limited role in the genesis of Ecuadoran lavas, compared with other parts of Andes where assimilation and wholesale melting of the crust appears to be common, it is important to point out that the SrNdPb isotope systematics clearly indicate that, similar to the case in Colombia (James & Murcia, 1984
), at least some assimilation of continental crust has affected many of the samples from Ecuador that we have analyzed. This is particularly clear from Pb and Nd isotope data, which are well correlated and appear to define mixing lines between Galapagos PlumeCarnegie Ridge basalts (i.e. probable subducting plate and mantle wedge compositions) and the local, geochemically mature continental crustal rocks (probable assimilants) that underlie many of the volcanoes in central Ecuador (Fig. 12). Bulk mixing calculations based on this PbNd correlation indicate that most lavas in Ecuador contain no more than 510% of the local crust (Fig. 12). Assimilation of geochemically mature continental crustal material by the Ecuadoran lavas is well supported by the observed spatialgeochemical shifts in isotopic compositions across the arc, which reach maximum values for 87Sr/86Sr and
7/4Pb, and minimum values for 143Nd/144Nd, over the crest of the northern Andes in the main arc area at distances of 330360 km from the trench (Fig. 13). Based on the high elevations and the presence of rhyolitic volcanism at Cotapaxi, Chalupas and Chacana, this area around the Inter-Andean depression appears to be the part of the Northern Andes where the crust is thickest, warmest, and where it is therefore most likely to contribute an assimilant to melts that are in transit from the subduction zone to the surface. Our estimate of the extent of the crustal contamination in Ecuadoran lavas, which is somewhat lower than some previous estimates (e.g. Kilian et al., 1995
; Barragan et al., 1998
), does not constrain the possible role of geochemically primitive accreted oceanic terranes as a crustal assimilant, because those terranes are isotopically similar to the anticipated subducting plate and mantle wedge composition (Carnegie Ridge, Galapagos Plume, Figs 8 and 9).
The above interpretation implies that a significant proportion of the Ecuadoran lavas have remained unaffected or minimally affected by assimilation of geochemically mature continental crust (e.g. samples with
7/4Pb <6·80 and
Nd >4·0, Figs 8 and 9). We cannot, of course, rule out the possibility that all of the lavas have been modified by assimilation of isotopically primtive crustal rocks, or that isotopically more primitive parental magmas were never erupted at the surface and, therefore, have not been sampled. We do not believe this is the case for two reasons. First, a large number of the Ecuadoran andesites and dacites have Pb, Sr and Nd isotopic compositions that are tightly clustered and partially overlap with (in Nd and Pb isotopes) likely subducting plate compositions in the form of Galapagos Plume and Carnegie Ridge basalts. This is similar to what is observed in many island arcs where the Pb, Nd and Sr isotopic compositions of the lavas approach those of MORB and are therefore widely believed to be controlled largely by geochemical components that originate in subducted MORB, marine sediment and seawater (Kay, 1980
; Plank & Langmuir, 1993
; Elliott et al., 1997
; Class et al., 2000
). Second, the alkali basalts and basaltic andesites at Sumaco, which appear, based on major and trace element compositions, to be low-percentage melts of mantle peridotite that has been less affected by subduction metasomatism than the associated andesites and dacites (Barragan et al., 1998
; Bourdon et al., 2003
), have extraordinarily high concentrations of Pb (1229 ppm), Sr (>2000 ppm) and Nd (>80 ppm). Such high concentrations would have caused these melts to be much more resistant to isotopic modification during crustal assimilation compared with the andesites and dacites, which have lower concentrations of these elements, are more evolved (lower Mg-number) and were erupted at lower temperatures. Assuming that the more silicic and cooler lavas are more likely to have assimilated crust on their way to the surface (DePaolo, 1981
), the broad isotopic overlap between the mafic alkaline lavas at Sumaco and the andesites and dacites implies that control over the composition of most Ecuadoran lavas lies primarily in the subduction zone, and not in the continental crust through which the melts passed (see also Barragan et al., 1998
; Bourdon et al., 2003
).
Effects of crustal assimilation on trace elements
Ecuador andesites and dacites that have relatively high
7/4Pb and 87Sr/86Sr, and low 143Nd/144Nd (i.e. those that appear to have assimilated a significant quantity of continental crust), generally have more variable and higher concentrations of the most incompatible trace elements, including Rb, Cs, Nb, Zr, Ba, Pb, and La. For example, as seen in Fig. 14, among the andesites and dacites with 143Nd/144Nd <0·51285 (
Nd <4·1), four samples out of five have Zr >100 ppm, whereas no sample with 143Nd/144Nd >0·51285 has Zr >100 ppm. A similar relationship can be seen in the Nb concentrations, which show a clear inverse correlation with 143Nd/144Nd, but not for Y or Yb, where the elemental concentrations are not correlated with isotope ratios (Fig. 14). Not surprisingly, the rhyolites generally also have elevated concentrations of the highly incompatible elements and concomitantly higher 87Sr/86Sr and
7/4Pb, and lower 143Nd/144Nd, consistent with relatively higher degrees of crustal contamination (Fig. 14). For most incompatible elements, however, the correlation with isotopic composition is relatively weak.
Isotopic shifts attributable to crustal contamination are also accompanied by shifts in certain incompatible element ratios (Fig. 15). This is particularly clear for La/Yb, which is generally higher, and for Ba/La and Ba/Nb, which are generally lower in samples with relatively low 143Nd/144Nd and high 87Sr/86Sr (i.e. those that appear to have assimilated continental crust). These relationships suggest that cross-arc changes in La/Yb, Ba/Nb, etc., for the andesites and dacites are produced at least in part, by combined fractional crystallization and assimilation (AFC) of thickened continental crust, and not exclusively (as has been consistently argued in the literature) by increased depth and/or decreased percentage melting or by a decrease in the slabfluid input to the mantle wedge. It is an important point, however, that the back-arc mafic and alkaline lavas at Sumaco (which anchor the cross-arc trends with high La/Yb and low Ba/Nb) retain the high 143Nd/144Nd and low
7/4Pb that is characteristic of lavas at the volcanic front, and so do not appear to have been significantly modified by AFC processes (Fig. 13). We agree with the interpretation of the Sumaco lavas as deep, low-percentage, alkaline-series melts of mantle peridotite (Barragan et al., 1998
; Bourdon et al., 2003
), and emphasize that, as such, they represent relatively hot and dry melts with low viscosities, that are physically and chemically distinct from the felsic and intermediate-composition calc-alkaline lavas (andesitedaciterhyolite) that dominate volcanism in Ecuador.
In contrast to La/Yb and Ba/Nb, which appear to be significantly affected by crustal assimilation, the full range of Sr/Y observed in the Ecuador andesites and dacites appears to be present among samples with relatively primitive isotopic composition (e.g. 143Nd/144Nd >0·51285,
7/4 Pb <7·0; Fig. 15). This suggests that Sr/Y, a key ratio in the adakite characterization, is not substantially affected by crustal assimilation in andesite and dacite lavas. In fact, for individual volcanoes where significant crustal assimilation has occurred, and where several andesite and dacite samples have been analyzed (e.g. Antisana, Imbabura), Sr/Y and Sr concentration appear to be inversely correlated with
7/4Pb, suggesting that, at some volcanoes, these quantities are highest in the samples that have assimilated the least amount of continental crust (Fig. 17).
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We conclude that crustal assimilation has significantly changed the trace element abundances of some Ecuadoran lavas, but that assimilation does not play a clear and consistent role in the genesis of the adakitic trace element characteristics, which are ubiquitous in the andesites and dacites in Ecuador.
Origin of the adakitic trace element characteristics in Ecuadoran lavas
Most andesites and dacites in Ecuador have REE characteristics that are adakitic; that is, they are enriched in the LREE, lack significant Eu anomalies, and are strongly fractionated between the middle REE (MREE) and HREE (Fig. 5). Unusually high concentrations of LREE in some Ecuadoran lavas may have been produced by assimilation of crustal rocks (as discussed above); however, assimilation alone cannot explain the low concentrations of Yb and Lu and the strongly fractionated MREE to HREE patterns (normalized Gd/Yb >> 1·0) that distinguish andesites and dacites in Ecuador from those in island arcs (Fig. 5d). Assuming that the melt source beneath the Northern Andes is approximately chondritic with respect to the HREE (i.e. normalized Gd/Yb
1·0), it is clear that garnet must have played a major role in the genesis of the Ecuadoran lavas. This role for garnet could be as a residual phase left after melt extraction or through removal by crystal fractionation under high pressures.
Several studies have concluded that garnet is involved in magma genesis beneath Ecuador when melting occurs at the surface of the subducting slab (e.g. Beate et al., 2001
; Bourdon et al., 2002
, 2003
; Samaniego et al., 2005
). This is essentially an application of the Defant & Drummond (1990)
adakite model in Ecuador. Among the lavas in Ecuador, those that appear to present the strongest case for the slab-melt interpretation have >700 ppm Sr and relatively MORB-like isotopic compositions (Fig. 17). Lavas with these characteristics are well illustrated by our data from Imbabura Volcano, where there is a high-Sr liquid line of descent separate from the evolutionary pathway defined by lavas with 400600 ppm Sr over the same range of SiO2 and Mg-number (Fig. 17). High-Sr lavas of this type appear to be present at Antisana Volcano (Fig. 17) and at Puñalica Volcano, where high Sr (>850 ppm) and unradiogenic Sr isotopes (87Sr/87Sr <0·7039) define an end-member composition among the 23 samples from the Northern Andes studied by Harmon et al. (1984)
. Rocks of this geochemical type do not appear to exist among lavas of the central and southern Andes (Fig. 17) or in Colombia (James, 1982
). In combination, these observations support the idea that melts from oceanic crust of the subducting Carnegie Ridge play a significant roll in the genesis of at least some Ecuador lavas (Bourdon et al., 2003
, and references therein).
Despite the apparent control of the Carnegie Ridge on the surface expression of active volcanism in Ecuador (Fig. 1), and the clear presence of lavas with trace element and isotopic compositions appropriate to the slab-melt interpretation (Fig. 17), the existence of thickened continental crust beneath Ecuador (at least 50 km; Prévot et al., 1996
; Guillier et al., 2001
) allows an alternative scenario by which adakite geochemistry may be produced, involving mantle melting and high-pressure crystal fractionation.
The presence of thick crust allows only a short column of mantle rock above the subduction zone (Fig. 1). This in turn means that melting within the mantle wedge will be relatively low percentage beneath Ecuador, compared with arcs in which the crust is thin and the melting column is long (Plank & Langmuir, 1988
). In addition, we know from Sm/Nd and Lu/Hf systematics that melting in all of the major tectonic settings involves the stabilization of at least a small quantity of residual garnet (Salters, 1991
; Hirschmann & Stolper, 1996
). With these considerations in mind, it is reasonable to anticipate that Ecuador basalts, which are only rarely erupted in the volcanic front or main-arc areas, will generally have HREE patterns that are more strongly fractionated than those of common island arc basalts, which typically have Gd/Yb = 1·51·9 (e.g. Elliott et al., 1997
; George et al., 2003
). This expectation is confirmed by the few available analyses of basaltic rocks from Ecuador's main arc at Sangay Volcano, where four samples with SiO2 <54% have Gd/Yb = 2·63·2 (Monzier et al., 1999
), well within the range of the common Ecuadoran andesites and dacites, which typically have Gd/Yb = 2·03·7 (Table 1 and Samaniego et al., 2005
). These observations provide clear support for the idea that the physical conditions of melting within the mantle wedge beneath Ecuador may be conducive to the stabilization of small quantities of residual garnet and the formation of basaltic melts that have strongly fractionated trace element patterns with low Y and Yb.
Subsequent cooling and fractional crystallization in the deep crust beneath Ecuador are also likely to contribute to depletion of Y and HREE and enrichment in Sr to produce adakitic melts. This is true because basaltic to andesitic magmas with high H2O contents (56%) at pressures of 1520 kbar (4560 km depths) and at temperatures below 1100°C, will crystallize a mineral assemblage that is free of plagioclase and dominated by clinopyroxene and garnet ± amphibole (Green, 1972
, 1982
). Simple calculations using typical partition coefficients (McKenzie & O'Nions, 1991
) demonstrate that if garnet constitutes 1520% of the mineral assemblage, fractional crystallization will result in strongly compatible behavior for Y, Yb and Lu (DBULK = 1·52·0), progressively less compatible behavior for the MREE, and strongly incompatible behavior for La and Ce (DBULK < 0·20). This mechanism is clearly capable of producing the low concentrations of MREE to HREE that distinguish andesites and dacites in Ecuador from lavas of similar major element compositions produced in island arcs (Fig. 5d). These physical conditions for melt evolution (high-pressure and hydrous) will also suppress crystallization of plagioclase (Green, 1982
), which in turn will cause Sr to behave as an incompatible element that can be enriched to high concentration as the melts evolve by crystal fractionation. The experimental studies of Green (1972
, 1982
) have similarly demonstrated that the major element character of the calc-alkaline series (basalt, andesite, dacite) can be explained by crystal fractionation processes under high-pressure and hydrous condition (see also Hildreth & Moorbath, 1988
; Garrison & Davidson, 2003
).
More broadly, the deep crustal fractionation mechanism is consistent with the basic observation that the trace element characteristics of Ecuadoran lavas are highly variable, even though their Pb, Sr and Nd isotopic compositions are relatively primitive and homogeneous. This is true for lavas throughout Ecuador, and within individual volcanoes (Samaniego et al., 2002
, 2005
), and is consistent with the idea that melt batches may evolve by crystal fractionation to create either adakitic or classic calc-alkaline trace element characteristics, dependent on the depth/pressure of fractionation, and consequently on the presence or absence of garnet in the fractionating assemblage.
The history of magmatism in Ecuador since the Eocene appears most consistent with the deep crustal fractionation model. Chiaradia et al. (2004)
recently showed that Eocene to Late Miocene andesites in Ecuador (509 Ma) have relatively flat REE patterns that contrast with the younger, Miocene to Recent lavas, which are adakitic (see Chiaradia et al., 2004
, fig. 8). The differences in REE characteristics imply that different processes operated in the genesis of these lavas of different ages. Available Pb isotope data, however, indicate that the magma source region beneath Ecuador has remained largely unchanged since the Eocene. Chiaradia et al. (2004)
argued that these observations imply that the magmatic plumbing systems beneath Ecuador shifted to depths within the stability field of garnet after
9 Ma, probably in response to a crustal thickening event, possibly caused by the initial collision and subduction of the Carnegie Ridge. The alternative interpretation involves a shift in source from the mantle wedge to the subducting plate at the point in time when subduction of the Carnegie Ridge began (i.e. Bourdon et al., 2003
, and references therein). This alternative remains possible, but appears less likely in the light of the new isotopic data, which suggest that the melt source beneath Ecuador has remained approximately constant since the Eocene (Chiaradia et al., 2004
).
One weakness of the deep crustal fractionation model described here for adakite genesis is that it requires fractional crystallization of garnet, even though garnet phenocrysts are not observed in Ecuadoran lavas. Garnets are not commonly found as phenocrysts in calc-alkaline lavas; they are, however, known from several localities and their potential role in the evolution of andesitic and dacitic lavas is well documented experimentally (Green & Ringwood, 1968
; Fitton, 1972
; Green, 1972
, 1982
; Hamer & Moyes, 1982
; Day et al., 1992
). If the deep crustal fractionation model is correct, this means simply that the plagioclasepyroxeneamphibole phenocryst assemblage in the Ecuadoran lavas is produced late in the magmatic evolution, during magma storage in shallow-level systems where garnet is unstable (e.g. Fitton, 1972
).
| CONCLUSIONS |
|---|
|
|
|---|
(i) Primitive and relatively homogeneous Sr, Nd and Pb isotopic compositions indicate that lavas throughout Ecuador are produced largely within the supra-subduction zone mantle wedge and not by extensive melting of the North Andean crust.
(ii) Changes in 143Nd/144Nd,
7/4Pb and La/Yb across the arc in Ecuador are interpreted to result from assimilation of geochemically mature continental crust, especially in the main-arc area, at distances of 330360 km from the trench. Mixing calculations limit the quantity of assimilated continental crust to less than
10%.
(iii) Possible assimilation of geochemically primitive crustal rock beneath the Western Cordillera remains poorly constrained; however, assimilation of crustal rocks does not appear to play a clear and consistent role in the genesis of the adakitic trace element patterns that are common in andesites and dacites in Ecuador.
(iv) Available whole-rock data do not provide a clear basis for distinguishing between slab-melting and deep crustal fractionation models for the genesis of adakitic lavas in Ecuador. Both models derive adakites from basalt, either by partial melting or fractional crystallization, and both explain the observed fractionation of REE patterns with garnet. None the less, the geochemical evolution within individual volcanoes (Samaniego et al., 2005
), and in magmatic rocks produced throughout Ecuador since the Eocene (Chiaradia et al., 2004
), appears to favor the deep crustal fractionation model for the genesis of most post-Miocene lavas in Ecuador.
| ACKNOWLEDGEMENTS |
|---|
This paper benefited substantially from thoughtful reviews by Henrietta Lapierre, Erwan Bourdon, Pablo Samaniego and Jennifer Garrison. We thank Nick Arndt and Marjorie Wilson for their thoughtful, thorough and timely handling of this work. Thanks also go to Drew Coleman for his assistance in acquiring the isotopic data. This paper also benefited from discussions with members of the University of South Carolina Solid-Earth Group. We thank in particular Jim Kellogg, Matt Kohn, Jim Knapp, and Bob Trenkamp. Thanks also go to Dennis Geist and Roberto Barragan, who generously provided samples from Sumaco, Antisana and Atacazo for this study, and to Sue Kay for many helpful discussions regarding Andean petrology and geochemistry.
* Corresponding author. Telephone: 001-803-777-9524. Fax: 001-803-777-6610. E-mail: gyogodzin{at}geol.sc.edu
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, locations of Quaternary volcanoes from the Smithsonian Global Volcanism database. Black arrows show the convergence direction and rate of movement of the Nazca Plate relative to stable South America from Trenkamp et al. (2002)

















