Geosciences 2013, 3(4), 633-667; doi:10.3390/geosciences3040633

Article
Modification of the Continental Crust by Subduction Zone Magmatism and Vice-Versa: Across-Strike Geochemical Variations of Silicic Lavas from Individual Eruptive Centers in the Andean Central Volcanic Zone
Gary S. Michelfelder 1,*,, Todd C. Feeley 1, Alicia D. Wilder 1 and Eric W. Klemetti 2
1
Department of Earth Sciences, Montana State University, Bozeman, MT 59717, USA; E-Mails: tfeeley@montana.edu (T.C.F.); alicia.wilder@msu.montana.edu (A.D.W.)
2
Department of Geosciences, Denison University, Granville, OH 43023, USA; E-Mail: klemettie@denison.edu
Present Address: Department of Geography, Geology and Planning, Missouri State University, Springfield, MO 65897, USA.
*
Author to whom correspondence should be addressed; E-Mail: gary.michelfelder@msu.montana.edu; Tel.: +1-406-994-6916; Fax: +1-406-994-6923.
Received: 2 May 2013; in revised form: 8 November 2013 / Accepted: 14 November 2013 /
Published: 27 November 2013

Abstract

: To better understand the origin of across-strike K2O enrichments in silicic volcanic rocks from the Andean Central Volcanic Zone, we compare geochemical data for Quaternary volcanic rocks erupted from three well-characterized composite volcanoes situated along a southeast striking transect between 21° and 22° S latitude (Aucanquilcha, Ollagüe, and Uturuncu). At a given SiO2 content, lavas erupted with increasing distance from the arc front display systematically higher K2O, Rb, Th, Y, REE and HFSE contents; Rb/Sr ratios; and Sr isotopic ratios. In contrast, the lavas display systematically lower Al2O3, Na2O, Sr, and Ba contents; Ba/La, Ba/Zr, K/Rb, and Sr/Y ratios; Nd isotopic ratios; and more negative Eu anomalies toward the east. We suggest that silicic magmas along the arc front reflect melting of relatively young, mafic composition amphibolitic source rocks and that the mid- to deep-crust becomes increasingly older with a more felsic bulk composition in which residual mineralogies are progressively more feldspar-rich toward the east. Collectively, these data suggest the continental crust becomes strongly hybridized beneath frontal arc localities due to protracted intrusion of primary, mantle-derived basaltic magmas with a diminishing effect behind the arc front because of smaller degrees of mantle partial melting and primary melt generation.
Keywords:
across-strike geochemical variation; Central Volcanic Zone; Aucanquilcha; Ollagüe; Uturuncu

1. Introduction

Continental arc volcanoes represent a dramatic surface expression of one of the most significant and fundamental phenomena in global tectonics: subduction of an oceanic plate beneath a more buoyant continental plate. The subduction of an oceanic plate results in recycling of crustal material into the convecting mantle, partial melting, and primary basalt production. Moreover, during passage through thick continental crust, subduction zone magmas may substantially differentiate and melt crustal rocks giving rise to the great diversity of igneous lithologies characteristic of Earth. These are important processes that must be understood in detail in order to interpret the long-term evolution of subduction zone systems on Earth and the generation of continental crust.

Although exceptions exist, one of the most remarkable features of arc magmatism is the systematic increase in the contents of K2O and other incompatible trace elements in volcanic rocks erupted with increasing vertical distance to the Benioff zone [1,2,3,4]. Understanding the significance of these trends has long been a major objective of petrologists due to the broader implications for regional tectonic complexities and magma generation processes, in addition to advancing understanding of arc magmatism. Despite decades of intense study, the origins of across-strike geochemical variations in intra-oceanic arcs are still vigorously debated; they are considerably less understood in continental arcs. As emphasized by Dickinson [5], interpreting the origin of these variations is inherently difficult in continental arcs due to the scarcity of primary, or near-primary basalts and the complicating effects of crustal contamination. For these reasons most of the better studied examples are from arcs underlain by relatively thin and, or, young continental crust where the potential for contamination is reduced [3,6,7,8,9,10,11,12,13,14,15,16,17,18,19].

Much has been learned about arc magmatism since publication of Gill’s [2] classic book on the subject, although much remains to be learned. Because of its exceptionally thick continental crust and numerous well preserved volcanic centers, the Central Volcanic Zone (CVZ) presents a unique opportunity to advance understanding of fundamental problems such as how silicic magmas are generated in continental arcs, how the continental crust may modify the compositions of primary arc magmas in space and time [7,17,20,21,22], and how arc magmas may, in turn, spatially and temporally modify the composition of the crust through which these magmas ascend and differentiate [23,24,25,26,27].

In this study we examine and interpret across-arc geochemical trends of <1 Ma silicic volcanic rocks (andesites to dacites) erupted from three composite volcanoes in the Andean Central Volcanic Zone (CVZ) of northern Chile and southwest Bolivia (21°–22° S latitude; Figure 1) and use this information to shed light on how the continental crust may influence across-arc trends in magma chemistry. Associated with active eastward subduction of the oceanic Nazca plate beneath the continental South American plate, the CVZ represents an end member in subduction zone systems on Earth because the continental crust is thicker (70–80 km) than at any other convergent margin setting [28,29,30,31,32,33,34,35]. The centers examined in this study were selected because of the young and limited range in ages (<1 Ma), quality and availability of comprehensive data sets (including isotopic data), and similarity in eruptive histories (i.e., effusive eruptions from andesitic to dacitic composite cones). In addition, we selected centers that span the range of volcanic activity in the arc, but show a small N-S coverage area, in order to minimize potential along-arc variations in magma sources and processes. Other volcanic centers are present within the study area that fit some of the above mentioned criteria, but no other centers were identified that fit all three of the controls. These restrictions allow for a more focused examination relative to larger regional studies (i.e., [22,36,37]). Previous regional-scale studies of magmatism in the southern Altiplano region documented eastward increases in K2O and related incompatible trace elements virtually identical to across-strike geochemical trends observed at many oceanic island arcs and continental arcs constructed on thin crust [38,39,40,41,42,43,44,45].

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Figure 1. Map showing location of Andean Central Volcanic Zone (CVZ). Shaded area shows the region where crustal thickness exceeds 60 km [30,32,33,46]; stippled region illustrates distribution of Quaternary volcanic rocks. Modified from Feeley and Hacker [47]. Red box highlights the region illustrated in Figure 2.

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Figure 1. Map showing location of Andean Central Volcanic Zone (CVZ). Shaded area shows the region where crustal thickness exceeds 60 km [30,32,33,46]; stippled region illustrates distribution of Quaternary volcanic rocks. Modified from Feeley and Hacker [47]. Red box highlights the region illustrated in Figure 2.
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Figure 2. Simplified geologic map of the southern Altiplano and surrounding region (modified from Sparks et al. [48]). Only potentially active volcanoes as defined by de Silva and Francis [49] and volcanoes on the southern Altiplano are illustrated. Labeled volcanic centers are those considered in this study due to the quality of data sets available for other volcanic centers within the study area. The thick dashed line trending NW-SE across the Bolivian-Argentine border is interpreted from Allmendinger et al. [28] and is considered to be the general boundary between the Bolivian Altiplano (north) and the Argentine Puna (south).

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Figure 2. Simplified geologic map of the southern Altiplano and surrounding region (modified from Sparks et al. [48]). Only potentially active volcanoes as defined by de Silva and Francis [49] and volcanoes on the southern Altiplano are illustrated. Labeled volcanic centers are those considered in this study due to the quality of data sets available for other volcanic centers within the study area. The thick dashed line trending NW-SE across the Bolivian-Argentine border is interpreted from Allmendinger et al. [28] and is considered to be the general boundary between the Bolivian Altiplano (north) and the Argentine Puna (south).
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2. Background: Tectonic and Geologic Setting

2.1. Regional Setting

The Andes are generally considered the classic example of a modern Cordilleran type orogen formed by long-term subduction of oceanic lithosphere beneath continental lithosphere. The central Andes, in particular, represent the type locality for this process owing to the great width of the orogen and immense crustal thicknesses (up to 70–80 km; [29]) and high elevations (~4–6 km; [50]) that occur over vast areas (Figure 1). The region composes one of the youngest and largest active silicic volcanic provinces on Earth with recent caldera formation. It contains over 20 calderas and numerous ignimbrites (large ash flow sheets) less than 10 Ma as well as an estimated 50 active or recently active composite volcanoes [51,52,53].

The modern central Andes at 21°–22° S latitude are divided into three north- to north-west striking geological and upper crustal provinces. From west to east these are: (1) the Western Cordillera: an active volcanic arc bounded on the west by a westward dipping monocline; (2) the Altiplano: a broad, elevated plateau (>3800 m) where undeformed late-Miocene and younger volcanic rocks overlie variably folded and faulted mid-Miocene and older sedimentary and volcanic rocks; and (3) the Eastern Cordillera: a major east-verging thrust complex involving Paleozoic to Mesozoic sedimentary and metamorphic rocks. The largest volumes of intermediate composition lavas at 21°–22° S latitude erupted from composite volcanoes that form the peaks of the Western Cordillera. Baker and Francis [53] estimated that the Western Cordillera contains ~3000 km3 of these lavas between 21° and 22° S latitude. Lavas associated with composite volcanoes extend for ~200 km eastward onto the Altiplano, although volumes decrease sharply to <800 km3 [53].

The youngest rocks in the southern Altiplano region of the CVZ were erupted following relatively recent changes in the subduction history of the CVZ. These changes are related to breakup of the Farallon plate into the Cocos and the Nazca plates, which increased the rate of subduction beneath the South American plate [16,54,55,56]. Between 15° and 28° S latitude the present day subduction angle of ~30° allows for an expression of magmatism that is absent from 2° to 15° S where the subduction angle is between 5° and 10° [57]. Uplift of the Altiplano and thickening of the CVZ crust are believed to be related, in part, to the recent steepening of the subducting slab [16,58,59]. In this study we focus on compositional variations of rocks on and behind the Quaternary arc-front that erupted after the last major episode of regional crustal thickening and shortening in the region.

2.2. Individual Volcanic Centers

Aucanquilcha is a long lived (11 Ma) volcanic complex located on the volcanic front in northern Chile (Figure 1 and Figure 2; [27]). The Aucanquilcha Volcanic Complex consists of 4 distinct volcanic groups: the Alconcha Group (11 to 8 Ma), the Gordo Group (6 to 4 Ma), the Polan Group (~4 to 2 Ma), and Volcán Aucanquilcha (<1 Ma; [27,60]). There are long hiatuses between the Aconcha and Gordo Groups and between the Polan Group and Volcán Aucanquilcha. This paper focuses exclusively on the eruptive products of Volcán Aucanquilcha.

Eruptive products from Volcán Aucanquilcha range in age from 1.04 to 0.24 Ma [60]. Volcán Aucanquilcha experienced four stages of growth as defined by Klemetti and Grunder [60]: the Azufrera, Rodado, Cumbre Negra and Angulo stages. These stages are not uniquely distinguished on the basis of location or time, and all are dominantly dacitic in composition. Eruptive units of the Azufrera stage (1.04 to 0.94 Ma) make up the main edifice of the volcano [60]. These units are mainly blocky two-amphibole (with the exception of the Rodado Stage) plus biotite dacitic lava flows [60,61]. Nearly all lavas contain undercooled basaltic andesitic to andesitic magmatic inclusions that compose 1%–10% of the total volume of the lavas [27,60].

Volcán Ollagüe straddles the Bolivia-Chile border approximately 25 km to the east of the arc front (Figure 1 and Figure 2; [41]). It is a composite volcano with no Holocene eruptions [62]. Feeley et al. [63] described four eruptive series (Vinta Loma, Chasca Orkho, La Celosa, and post-collapse) and a debris avalanche deposit resulting from sector collapse of the western flank of the volcano. These series were subsequently sub-divided into ten sequences by Wörner et al. [64], Clavero et al. [65], and Vezzoli et al. [66].

Ollagüe was primarily active between 1.2 Ma and 130 ka. Currently the volcano shows signs of activity through active degassing of fumaroles that vent from a young dacitic dome on the upper western flank [63,65]. Compositions of eruptive products range from basaltic andesitic to dacitic lava flows and domes covering an estimated area of ~230 km2 with a volume of ~85 km3 [63]. In addition, basaltic andesitic to andesitic magmatic inclusions are present in varying proportions in nearly all lava flows, although they are more abundant in younger units. The volcano is built upon 8 to 5 Ma ignimbrite deposits [47].

Cerro Uturuncu is an andesitic to mainly dacitic composite volcano located in the southern Altiplano region of the CVZ in southwest Bolivia, approximately 120 km east of the arc front (Figure 1 and Figure 2; [48]). The volcano was primarily active between 890 and 271 ka. Eruptive products define two series as described by Sparks et al. [48]. The first series is more extensive older material ranging from 890 to 549 ka. These flows and domes rest directly on approximately 5 Ma ignimbrites [49]. The second series consists of younger flows covering about 10 km2, mostly located on the upper flanks of the edifice. These flows range from 427 to 271 ka and are built upon the first series flows and domes [48]. Most flows and domes sampled by Sparks et al. [48] and in this study contain undercooled andesitic magmatic inclusions that compose no more than a few volume percent of the host rocks. In many older rocks magmatic inclusions are rarer [48]. This relationship is similar to that seen at Aucanquilcha [60] and Ollagüe [63] where magmatic inclusions are typically more abundant in younger lavas.

3. Methods

New whole rock analyses for Uturuncu rocks were performed at Washington State University, Pullman. Major and trace element analyses on 121 samples were performed by X-ray Fluorescence Spectrometry (XRF) on a ThermoARL Advant’XP+ automated sequential wavelength spectrometer (ThermoARL, Waltham, MA, USA). Methods and errors for the XRF analyses are described in Johnson et al. [67]. 65 distinct geochemical samples were further analyzed for trace elements, including the rare earth elements, by Inductively Coupled Plasma Mass Spectrometry (ICP-MS) on an Agilent Technologies 7700 ICP-MS (Agilent Technologies, Conesus, NY, USA). Methods and errors for trace element analyses are detailed in Jarvis [68].

Whole rock Nd and Sr isotopic analyses on 30 samples were acquired by Thermal Ionization Mass Spectrometry (TIMS) on a VG Sector 54 (VG, Santa Clara, CA, USA) and analyzed by five Faraday collectors in dynamic mode at New Mexico State University, Las Cruces. Calibration of 87Sr/86Sr ratios was calculated using the 86Sr/88Sr ratio analyzed at 3.0 V aiming intensity and normalized to 0.1194 using NBS 987 Standard (0.710298 + 0.000010) to monitor the precision of the analyses. Sr was isolated using Sr-Spec resin column chromatography by the method described in Ramos and Reid [69]. Nd was separated using REE resin column chromatography using the digested split of prepared sample for Sr chromatography. Nd isotopes were normalized to 146Nd/144Nd = 0.7219 and results for JNDi-1 were 146Nd/144Nd = 0.512137 ± 0.000009 for five analyses. Pb isotopes were separated from the same digested samples used for Sr and Nd isotope ratios. Pb separations used ~2 mL of anion exchange resin in a high-aspect ratio glass column with an eluent of 1N HBr and 7N HNO3. Purified samples were then dried and re-dissolved in 1 mL of 2% HNO3 containing 0.01 ppm Tl. Samples were analyzed on a ThermoFinnigan Neptune multi-collector ICP-MS (ThermoFinnigan, Waltham, MA, USA) equipped with nine Faraday collectors and an ion counter. The standard NBS 981 (208Pb/204Pb ≈ 36.662 ± 0.002, 207Pb/204Pb ≈ 15.462 ± 0.001, 206Pb/204Pb ≈ 16.928 ± 0.001) was used for accuracy corrections and to monitor precision of the analyses. The values measured for NBS 981 were within the error of published ratios for NBS 981 [70] and therefore corrections were not applied to unknown sample ratios. Given the young ages of all rocks examined in this study, no age corrections were performed for the radiogenic isotope data.

δ18O values were determined for 30 Uturuncu samples by the laser fluorination method described by Takeuchi and Larsen [71] at Washington State University, Pullman. Quartz and plagioclase phenocryst separates were analyzed twice to insure reproducibility. The standard UWG-2 was measured with a difference of 0.2‰ from the published value of 5.89‰ [71,72]. Data are illustrated in figures and presented in Table 1 in permil using standard delta notation relative to Vienna Standard Mean Ocean Water (VSMOW).

Table 1. Representative new whole rock samples from Cerro Uturuncu.

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Table 1. Representative new whole rock samples from Cerro Uturuncu.
SampleDM10ADM58A2GSM17GSM29GSM-50
SiO265.5562.3066.5963.6564.84
TiO21.081.131.000.991.08
Al2O316.1617.1915.8416.1116.25
FeO*4.815.734.475.244.93
MnO0.070.090.060.070.07
MgO1.872.601.613.072.11
CaO4.144.953.644.694.11
Na2O2.372.212.412.232.29
K2O3.703.494.113.674.01
P2O50.250.300.280.280.32
LOI (%)0.990.430.530.510.95
Sum100.00100.00100.00100.00100.00
La5359696170
Ce109118140120141
Pr1314171517
Nd5053615462
Sm1010111011
Eu1.801.981.891.901.97
Gd7.688.238.107.798.36
Tb1.111.251.111.101.18
Dy5.896.965.655.746.07
Ho1.031.310.931.031.04
Er2.443.292.182.632.40
Tm0.330.450.290.370.31
Yb1.902.721.642.251.76
Lu0.270.400.240.330.25
Ba686776850814866
Th1919252025
Nb1821191922
Y2733252727
Hf6.66.47.36.47.3
Ta1.41.51.41.31.5
Rb167146193161184
Sr305474338391388
Zr250241277230276

Note: Total Fe reported as FeO*.

4. Results

4.1. Summary of Petrology and Petrogenetic Processes at 21°–22° S Latitude

Rocks from all three centers are porphyritic with 30% to 60% by volume phenocrysts (average ~40%). Plagioclase is the most abundant phenocryst phase in all samples, accounting for 50% to 75% of the mineral assemblage in many of the samples. Other phenocryst phases are present in variable amounts and include orthopyroxene, clinopyroxene, amphibole, biotite, quartz, magnetite, and ilmenite. In general, phenocryst assemblages are similar for rocks from the three centers, except that amphibole and clinopyroxene are typically more abundant in young rocks from Aucanquilcha, whereas biotite is progressively more abundant in young rocks from Ollagüe and Uturuncu. The latter probably reflects the higher K2O contents of Ollagüe and Uturuncu rocks relative to rocks from Aucanquilcha.

Petrographic similarities such as those described above and the presence of undercooled magmatic inclusions that are slightly more mafic than the host lavas, suggest that Uturuncu magmas experienced similar petrogenetic processes to magmas erupted at Ollagüe and Aucanquilcha. Specifically, recent geochemical modeling of Uturuncu rocks suggests that the magmas were produced by complex processes involving magma mixing and mingling with more mafic magmas following assimilation of crustal rocks coupled with fractional crystallization (AFC) in multiple reservoirs within both the mid-deep and shallow crust [73,74]. This is consistent with the work of Sparks et al. [48] who, on the basis of geochemical and petrologic data, concluded that dacitic magmas at Uturuncu formed by fractional crystallization of andesite forming norite cumulates and involving partial melting and assimilation of the continental crust. Furthermore, phenocryst compositions and zoning patterns indicate that more detailed compositional variations of the dacites reflect magma mixing with silicic andesite at shallow crustal levels. The latter conclusion is supported by geophysical evidence that indicates magma accumulation and seismicity clusters at sea level beneath Uturuncu (6 km depth; [75,76,77]).

The petrologic model for Uturuncu rocks [48,73,74] is nearly identical to those proposed by Feeley and Davidson [25] and Feeley and Hacker [47] for production of magmas at Ollagüe and Klemetti and Grunder [60] and Walker et al. [78] for production of magmas at Aucanquilcha. These authors argue that magma mixing with a component of mid-deep crustal AFC were responsible for producing the rock compositions observed at these two centers. Therefore, mid-deep crustal AFC is considered the dominant process in producing the dacitic rocks erupted at the three centers followed by mixing and mingling with more mafic melts and undercooled inclusions, respectively, in shallow reservoirs to produce rocks lower in SiO2 contents. The most silicic rocks erupted at the three centers are thus all considered to contain a significant crustal component derived from melting and assimilation of mid-deep crustal local basement lithologies.

4.2. Across-Arc Geochemical Variations

In this section we describe across-arc geochemical and isotopic variations of silicic volcanic rocks (i.e., >60 wt % SiO2) erupted from the three centers. We focus on silicic rocks because more mafic rocks are generally rare or non-existent at the three centers and the silicic rocks better record the compositions of crustal rocks through which the magmas ascended and interacted. Data for magmas erupted at Ollagüe and Aucanquilcha are in Feeley and Davidson [25], Feeley and Hacker [47], Feeley and Sharp [26], Mattoli et al. [79], Grunder et al. [27], Klemetti and Grunder [60], and Vezzoli et al. [66]. New whole rock and isotopic data are illustrated in this paper for Uturuncu rocks with representative analyses presented in Table 1, Table 2 and Table 3. A complete dataset for new analyses is available in the supplementary information. Additional major and trace element data for Uturuncu rocks are in Sparks et al. [48].

Table 2. Representative new whole rock trace element ratios from Cerro Uturuncu.

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Table 2. Representative new whole rock trace element ratios from Cerro Uturuncu.
SampleDM10ADM58A2GSM17GSM29GSM-50
K2O + Na2O5.995.686.465.876.20
Rb/Sr0.550.310.570.410.47
Sr/Y11.4814.2513.5914.4814.54
Ce/Y4.093.565.634.435.29
Ce/Yb57.2443.4385.3853.2380.06
Ba/La12.9113.2712.3413.3412.37
Ba/Zr2.753.223.073.533.13
K/Rb184.42199.17176.59189.74180.83
Nb/Zr0.070.090.070.080.08
Dy/Dy*0.810.730.800.680.81
Dy/YbN2.011.662.241.662.23
La/YbN18.8714.4728.3618.2926.75
Eu Anomaly0.570.580.560.580.63

Note: Dy/Dy* = DyN/(LaN4/13YbN9/13).

Table 3. Representative new whole rock Sr, Nd, Pb whole rock isotopic ratios and 18O/16O ratios from mineral separates from Cerro Uturuncu.

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Table 3. Representative new whole rock Sr, Nd, Pb whole rock isotopic ratios and 18O/16O ratios from mineral separates from Cerro Uturuncu.
SampleDM10ADM58A2GSM17GSM29GSM-50
87Sr/86Sr0.714570.7112940.713850.711410.71247
144Nd/143Nd0.512150.5121790.512140.512230.51216
208/204Pb38.9438.9238.9438.938.93
207/204Pb15.6515.6515.6515.6515.64
206/204Pb18.8718.8418.8418.8418.86
δ18O-QTZ7.268.957.607.98
δ18O-PLG9.328.75

Notes: δ18O-QTZ represents mineral separate analyses of quartz phenocrysts; δ18O-PLG represents mineral separate analyses of plagioclase phenocrysts.

Volcanic rocks at Aucanquilcha, Ollagüe, and Uturuncu are high-K, calc-alkaline andesites/trachyandesites and dacites/trachytes, together with less abundant basaltic andesites (Figure 3). Total alkali concentrations of rocks from Aucanquilcha and Ollagüe with 61–68 wt % SiO2 are restricted, ranging from 5.1 to 7.9 wt %, such that they plot along the border of the andesite-dacite/trachyte-trachyandesite fields (Figure 3; [27,60]). Ollagüe also contains a few rocks that plot in the trachyte and trachyandesite fields, but these are rare (Figure 3; [23,25]). Silicic rocks at Uturuncu with SiO2 contents from 61 to 68 wt % have lower total alkali concentrations of 5.5–6.7 wt % (as a result of low Na2O concentrations; see below); classifying them as andesitic to dacitic (Figure 3; [23,25,48]).

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Figure 3. Total alkalis vs. SiO2 contents and classification of silicic rocks from Aucanquilcha, Ollagüe and Uturuncu [80].

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Figure 3. Total alkalis vs. SiO2 contents and classification of silicic rocks from Aucanquilcha, Ollagüe and Uturuncu [80].
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Systematic differences exist in the major and trace element compositions of rocks erupted with increasing distance from the arc front. At a given SiO2 content, K2O, FeO, P2O5, and TiO2 concentrations increase toward the east, particularly in the most silicic composition rocks, with the highest concentrations in rocks at Uturuncu (Figure 4). In contrast, contents of CaO, Al2O3, and, particularly, Na2O, decrease in concentration toward the east, with very low concentrations of the latter in Uturuncu rocks (Figure 4). In more detail, trends for P2O5 and TiO2 decrease with increasing SiO2 for lavas from Aucanquilcha and Ollagüe, whereas they increase with increasing SiO2 for lavas from Uturuncu.

At a given SiO2 content, all trace elements analyzed increase in rocks erupted progressively toward the east with the exception of Sr and Ba (Figure 5). In contrast, Sr (and to a lesser degree, Ba) concentrations decrease toward the east at a given SiO2 concentration (Figure 5). Chondrite-normalized REE patterns for rocks from Aucanquilcha and Ollagüe have similar slopes, although Ollagüe rocks have higher concentrations of REE compared to Aucanquilcha (Figure 6). In contrast, Uturuncu REE patterns have steeper slopes for middle to heavy REE compared to patterns for Ollagüe or Aucanquilcha rocks and higher concentrations (Figure 6). In these regards, with increasing SiO2 contents, (La/Yb)n (when “n” refers to chondrite normalized values) ratios increase for rocks from all centers and broadly overlap (although the most silicic rocks from Uturuncu have the highest ratios; Figure 7). In contrast, with increasing SiO2 concentrations, trends for (Dy/Yb)n ratios are variable: they decrease in Aucanquilcha rocks, are roughly constant for the Ollagüe suite, and increase for Uturuncu rocks (Figure 7). Furthermore, negligible Eu anomalies are observed in REE patterns for rocks from Aucanquilcha (0.8–0.85) compared to small negative Eu anomalies in Ollagüe rocks (0.61–0.88; ratios close to one are considered small). Relatively large negative Eu anomalies (0.49–0.69) are observed for all Uturuncu rocks (Figure 6 and Figure 7; Table 2).

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Figure 4. Major element diagrams for volcanic rocks from Aucanquilcha, Ollagüe and Uturuncu rocks vs. SiO2.

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Figure 4. Major element diagrams for volcanic rocks from Aucanquilcha, Ollagüe and Uturuncu rocks vs. SiO2.
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Figure 5. Plots of selected trace element compositions of Aucanquilcha, Ollagüe, and Uturuncu rocks vs. SiO2.

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Figure 5. Plots of selected trace element compositions of Aucanquilcha, Ollagüe, and Uturuncu rocks vs. SiO2.
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Figure 6. Rare earth element fields for whole rock samples from each volcanic center. Chondrite normalization values from Sun and Mcdonough [81].

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Figure 6. Rare earth element fields for whole rock samples from each volcanic center. Chondrite normalization values from Sun and Mcdonough [81].
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LILE to HFSE ratios (e.g., Ba/Zr and Rb/Nb; the latter not illustrated), K/Rb, Ba/La, and Eu/Eu* decrease toward the east for a given SiO2 (Figure 7). Nb/Zr and Rb/Sr ratios increase toward the east with the highest ratios observed in Uturuncu rocks for a given SiO2 (Figure 7). Aucanquilcha rocks contain the highest Sr/Y ratios for a given Y concentration (Figure 8). This ratio is lower in Ollagüe rocks and the lowest ratios are observed in Uturuncu rocks. Ratios of La/Ta show no correlation with distance from the arc front with the exception that there are no observed ratios for Aucanquilcha that fall below La/Ta = 40. Ba/Ta ratios decrease towards the east. Ba/La ratios for all observed rocks from Aucanquilcha and most rocks for Ollagüe are above the Ba/La = 20 ratio indicative of their arc affiliation [17,82].

Across-arc variations in Sr, Nd, and O isotope ratios generally parallel those observed for K2O and incompatible trace elements (with the exceptions of Sr and Ba), particularly for the most silicic rocks erupted at any given center. In this regard, 87Sr/86Sr and 18O/16O ratios of Uturuncu rocks (Table 3) are highly elevated and become progressively lower in rocks erupted towards the arc front, whereas 143Nd/144Nd ratios increase (Figure 9). In detail, with increasing SiO2 contents, Sr and Nd isotopic ratios of rocks from Aucanquilcha decrease and increase, respectively, show small variations for rocks from Ollagüe, and increase and decrease, respectively, for rocks from Uturuncu.

On a plot of 143Nd/144Nd vs. 87Sr/86Sr, rocks from all three centers form a slightly scattered curvilinear array, becoming isotopically more “crustal-like” (i.e., plotting lower and further to the right from Bulk Earth (BE; 143Nd/144Nd = 0.51263; 87Sr/86Sr = 0.7052; [83])) with increasing distance from the arc front (Figure 10). This is a long observed trend in the CVZ as outlined by Kay et al. [17] and references within. Furthermore, on Figure 10, there is a distinct gap between magmas erupted at Uturuncu versus those erupted on or just to the east of the arc front. In a similar manner, δ18O values for the rocks as a group are elevated relative to generally accepted mantle values [24,84,85,86], thus requiring the incorporation of a significant crustal component during the petrogenesis of all studied suites. δ18O values of mineral separates are extremely variable for Uturuncu rocks (δ18O = 7.3‰–9.6‰) compared to Ollagüe (δ18O = 7.3‰–8.3‰) and Aucanquilcha rocks (δ18O = 7‰–7.3‰), in part reflecting that values for both plagioclase and quartz are illustrated for Uturuncu rocks. Nevertheless, Aucanquilcha rocks contain the lowest δ18O values and, while values for Uturuncu and Ollagüe overlap, 18O/17O ratios become on-average more crustal-like toward the east (Figure 9).

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Figure 7. Plots of selected trace element abundance ratios for Aucanquilcha, Ollagüe, and Uturuncu rocks vs. SiO2. Lines through data points without arrowheads illustrate inferred trends for individual eruptive centers.

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Figure 7. Plots of selected trace element abundance ratios for Aucanquilcha, Ollagüe, and Uturuncu rocks vs. SiO2. Lines through data points without arrowheads illustrate inferred trends for individual eruptive centers.
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Figure 8. Plots of trace element ratios for Aucanquilcha, Ollagüe, and Uturuncu rocks vs. Y, La contents and La/Yb ratios.

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Figure 8. Plots of trace element ratios for Aucanquilcha, Ollagüe, and Uturuncu rocks vs. Y, La contents and La/Yb ratios.
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Figure 9. Plots of 87Sr/86Sr, 143Nd/144Nd, and 18O/16O (as δ18O values of mineral separates) ratios of Aucanquilcha, Ollagüe and Uturuncu rocks vs. SiO2. Lines through data points illustrate inferred trends for individual eruptive centers.

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Figure 9. Plots of 87Sr/86Sr, 143Nd/144Nd, and 18O/16O (as δ18O values of mineral separates) ratios of Aucanquilcha, Ollagüe and Uturuncu rocks vs. SiO2. Lines through data points illustrate inferred trends for individual eruptive centers.
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Figure 10. (a) 143Nd/144Nd vs. 87Sr/86Sr ratios of Aucanquilcha, Ollagüe and Uturuncu rocks. Arrow labeled BE illustrates direction toward position of “Bulk Earth”, which plots off of figure; (b) 87Sr/86Sr vs. Sr/Y ratios of Aucanquilcha, Ollagüe and Uturuncu rocks.

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Figure 10. (a) 143Nd/144Nd vs. 87Sr/86Sr ratios of Aucanquilcha, Ollagüe and Uturuncu rocks. Arrow labeled BE illustrates direction toward position of “Bulk Earth”, which plots off of figure; (b) 87Sr/86Sr vs. Sr/Y ratios of Aucanquilcha, Ollagüe and Uturuncu rocks.
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Rocks from Aucanquilcha and Ollagüe have extremely variable Pb isotopic ratios and show no distinct arrays with varying SiO2 concentrations (not shown). Uturuncu rocks (Table 3) have very restricted 207Pb/204Pb, 208Pb/204Pb, and 206Pb/204Pb ratios, although they are higher on average than for Ollagüe or Aucanquilcha rocks (Figure 11).

Pb isotopic ratios for all three centers lie within the southern sector Pb isotopic domain defined by Wörner et al. [22]. Aucanquilcha and Ollagüe Pb isotopic values lie in the Southern Altiplano Pb isotopic domains (207Pb/204Pb > 15.64, 208Pb/204Pb < 38.89 but >38.5 and 206Pb/204Pb > 18.6) defined by Aitcheson et al. [87] and Uturuncu lies within the Eastern Cordilleran domain (207Pb/204Pb > 15.64, 208Pb/204Pb > 38.9 and 206Pb/204Pb > 18.6).

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Figure 11. 208Pb/204Pb vs. 206Pb/204Pb and 207Pb/204Pb vs. 206Pb/204Pb. Pb isotopic ratios for all three centers lie within the southern Altiplano Pb isotopic domain defined by Wörner et al. [22] and Aitcheson et al. [87]. Grey field defines the boundary between the Eastern Cordilleran domain and the Southern Altiplano domain [87].

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Figure 11. 208Pb/204Pb vs. 206Pb/204Pb and 207Pb/204Pb vs. 206Pb/204Pb. Pb isotopic ratios for all three centers lie within the southern Altiplano Pb isotopic domain defined by Wörner et al. [22] and Aitcheson et al. [87]. Grey field defines the boundary between the Eastern Cordilleran domain and the Southern Altiplano domain [87].
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5. Discussion: Origin of Across-Arc Geochemical Variations in the Central Andes at 21°–22° S Latitude

Major and trace element across-arc variations at 21°–22° S latitude described in the previous section are similar in several respects to trends observed at many other convergent margin settings where there is thin (Southern Andes) or no overlying continental crust (oceanic arcs; as described by Gill [2]; p. 209, and Tatsumi and Eggins [4]; pp. 80–81). These include increases in K2O and most incompatible trace elements with increasing distance from the active arc front. Notable exceptions are that whole rock Na2O, Sr, and Ba contents decrease to the east for a given SiO2 concentration (Figure 4 and Figure 5). These trends are contrary to the across-arc behavior of these elements observed at other oceanic arcs (e.g., New Zealand, Java, Japan, and the Aleutians; [2,3,4,5,88]).

It has been repeatedly demonstrated that K and incompatible trace elements tend to increase in arc magmas with distance behind the volcanic front (there is, however, no general rule for isotopic ratios [2,3,4,5,89]). Much of our perspective on the origin of these trends comes from study of intra-oceanic arcs or arcs constructed over young, thin continental crust [6,90,91,92]. In these settings, across-arc geochemical trends are nearly always linked to systematic changes in mantle source compositions, degrees of partial melting, and, or, slab dehydration reactions. This is because they are typically expressed in the most primitive rocks of any given suite and they frequently correlate with other petrologic features such as inferred primary magmatic H2O contents [11,12,93,94,95].

The Andean CVZ offers the opposite perspective to island arcs: thick continental crust producing or enhancing across-arc trace element variations in subduction zone magmas. A result of the anomalously thick crust beneath the CVZ is that the across-arc increases in K2O and incompatible trace element concentrations do not directly reflect variations in mantle source compositions or degrees of partial melting. Baseline Sr and O isotopic ratios of the volcanic rocks are highly elevated relative to primitive intra-oceanic arc magmas, implying a contribution from the continental crust during magma petrogenesis [96]. Furthermore, 87Sr/86Sr and 18O/16O ratios become more variable and increase towards the east for a given SiO2 concentration while 143Nd/144Nd ratios decrease (Figure 9). These trends parallel the incompatible trace element trends for each of the three volcanic centers (Figure 5, Figure 6 and Figure 7). This suggests that the sources become more variable/complex towards the east. The thick continental crust thus modifies primary arc magmas generated across the transect (Figure 10 and Figure 11), yet many of the universal across-arc trace element trends observed at oceanic arcs are maintained (Figure 5). How is this possible?

A variety of models have been proposed to account for the across-arc trace element trends at 21°–22° S latitude. However, until recently these models have been difficult to test due to the absence of a comprehensive data set on magmas erupted from suitable back-arc locations. This is important in order to constrain the processes and contaminants that influence magmatic differentiation to a singular location rather than using multiple locations that may have undergone different processes or assimilated different crustal contaminants. Using data from multiple centers representing a “zone” would require additional analyses and comparison of the centers. Fernández et al. [42], Kussmaul et al. [44], Avila-Salinas [38], and Feeley [41] demonstrated that rocks with the highest K2O contents also have the highest 87Sr/86Sr ratios. These authors proposed that the eastward enrichments of incompatible trace elements require the involvement of some form of crustal melting or contamination. Further to the south, Kay et al. [17] suggested that the ignimbrites located on the Puna plateau are controlled by basement contaminants during the earliest stages of volcanism. Overtime, this contribution diminishes and compositions become increasingly controlled by mantle source compositions. Fernández et al. [42] and Kussmaul et al. [44] suggested that the observed compositional trends may reflect crustal melting or contamination of more mafic magmas at increasingly shallower depths eastward. These conclusions were reached without comprehensive trace element data, which was later suggested to play key roles in modeling the mineralogies and source compositions during magma differentiation and migration [41,97,98]. Avila-Salinas [38] suggested the trends may reflect an eastward increase in the degree of upper-crustal contamination, although little evidence was discussed to support this idea. Feeley [41] argued the trends may reflect assimilation of progressively less hybridized mid-deep crustal rocks eastward (e.g., Figure 5). Diminishing hybridization of the continental crust east of the volcanic front was inferred to reflect diminishing intrusion of subduction-derived basaltic magmas due to progressively lower degrees of mantle partial melting. In contrast to these models, Dostal et al. [99] suggested a more traditional model where the across-arc spatial variations were attributed to the degree of mantle partial melting with increasing depths to the Benioff zone and possibly systematic variations in mantle source compositions as a result of hydrous fluid fluxing. The temporal geochemical evolution of the Central Andes was discussed by Mamani et al. [36,37]. These authors used Sr/Y, Dy/Yb and Sm/Yb to describe changes in arc magma composition from the Triassic to the recent and discussed the observed changes these ratios have during arc migration. These authors suggested that along-strike variations from 18° to 28° S over time were caused by the onset of crustal thickening and changes in the depth of assimilation at ~30 Ma and again at ~3 Ma. The variation caused by the onset of crustal thickening at ~30 Ma resulted in higher ratios of Dy/Yb and Sm/Yb reflecting increased lithospheric pressures at the time of differentiation and crust-magma interaction. These depths were suggested to be where garnet and amphibole are stable [37].

The model by Kay et al. [17] is a hybrid model. In the early stages of eruption of the Puna ignimbrites the composition of the ignimbrites are controlled by variation in the crustal composition. Over time, these authors suggest that the composition of the crust becomes less important, and the controlling factor in the compositional variation between the back arc and the arc front volcanic rocks is variation in the mantle source and slab fluxes. Early stages of this model suggest hybridization and crustal assimilation similar to the model presented by Feeley [41], but does not suggest how geochemical variation occurs at a single point in time. The model of Kay et al. [17] requires a temporal component to observe similar across arc variations seen at 21°–22°.

Our preferred explanation for the across-arc geochemical and isotopic trends described in the previous section is that magmas assimilate continental crust that becomes increasingly more mafic toward the arc-front because of relatively recent intrusion and hybridization by primary, subduction-derived basaltic magmas. Several lines of evidence collectively support this hypothesis. First, the curvilinear array formed by 87Sr/86Sr and 143Nd/144Nd ratios on Figure 10, with magmas becoming isotopically more crustal-like with increasing distance from the arc front, cannot reflect a continuous differentiation trend formed by a common petrogenetic process given the similar bulk compositions (i.e., SiO2 and MgO contents) of the rocks at the three centers (a similar argument can be made for the across-arc trend in Sr vs. O isotope ratios). Instead, it is more likely related to local isotopic differences in the composition of the mid- deep-continental crust. In this regard, it is possible that magmas at Uturuncu assimilated crustal rocks similar in composition to un-hybridized Paleozoic granites and gneisses exposed in northwestern Argentina. These rocks have 87Sr/86Sr ratios between 0.71 and 0.80 [100,101,102,103,104]. Assimilation fractional crystallization modeling of Uturuncu magmatic inclusions and contaminants of similar composition to the Paleozoic granites described by Lucassen [36,37,73,100,102,103,105,106,107,108,109,110] suggest that very little contamination is required to produce the high Sr isotopic ratios while maintaining the moderate Sr concentrations observed at Uturuncu. Increasing Rb/Sr ratios (Figure 7) toward the east can thus be directly related to assimilation of progressively older, less-hybridized crustal rocks toward the east with high 87Sr/86Sr ratios due to protracted in-growth of radiogenic 87Sr in assimilated lithologies.

Second, across-arc increases in K2O, Rb, Th, Y, REE and HFSE contents can be interpreted to reflect assimilation of more silicic lithologies with higher incompatible trace element contents in which residual mineralogies are progressively more feldspar-rich. In the latter regard it is important to note that contrary to across-arc geochemical trends commonly observed at other arcs, the CVZ rocks display systematically lower Na2O, CaO, Al2O3, Sr, and Ba contents toward the east; stoichiometric components or trace elements with relatively high partition coefficients in feldspar-rich assemblages [83]. Furthermore, with increasing distance from the arc-front, the rocks have progressively more negative Eu anomalies (Figure 7), also consistent with more feldspar-rich residual mineralogies. In a similar manner, across-arc increases in δ18O can be interpreted to indicate assimilation of rocks with increasingly higher proportions of more silicic, 18O-concentrating minerals toward the east.

Third, more feldspar-rich residual mineralogies toward the east are supported by experimental studies. Specifically, Huang and Wyllie [111] demonstrated in tonalite melting experiments at low-H2O and high pressures (~15 kbar), similar to conditions assumed for the mid-deep crust beneath the southern CVZ, that K2O-rich silicic melts are produced with residual plagioclase and garnet. In contrast, during melting of mafic amphibolite under similar conditions, plagioclase becomes unstable, increasing Sr concentrations in the melt [20,98]. Moreover, high-pressure (e.g., ≥15 kbar) melting experiments by Litvinovsky et al. [112] on a variety of Archean silicic rock compositions (e.g., charnokite, granodiorite, and leuco-granite) under both wet and fluid-absent conditions in all cases produced silicic melts in equilibrium with residual garnet, Na-rich feldspar, and clinopyroxene. At low to moderate melt fractions (e.g., 5%–25%), derivative melts are characterized by low Na2O, but high K2O contents. Collectively, these experiments demonstrate that partial melting of mafic protoliths at high pressures leads to production of melts with high Sr/Y ratios, whereas high pressure melting of more silicic compositions leads to production of melts with low Sr/Y ratios (largely due to low Sr contents) and Na2O contents, but high K2O contents. The smooth, curvilinear array on Figure 8 with Sr/Y ratios decreasing with increasing Y contents to the east is therefore consistent with a progressive change to melting of more silicic bulk composition crustal rocks eastward and more feldspar-rich residual mineralogies (alternatively, this trend has also been ascribed to melting at progressively lower pressures in the absence of residual garnet, but we discount this below).

Kay et al. [17] suggested that the low Na2O concentrations observed in the Puna ignimbrites (Grandada-Orosmayo, Panizos, and Vilama) combined with high 87Sr/86Sr ratios (0.709861–0.715048; [113,114]) and δ18O (9.05–10.24; [113,114]) ratios are the result of crustal contamination by old shale-like components with similar interpretations for the Altiplano ignimbrites (e.g., Morococala; [115]). This is a possible alternative to the model described above, but still supports the model that the composition of the continental crust changes eastward.

Finally, observations by Baker and Francis [53] indicate that the greatest volumes of late Cenozoic, subduction-related rocks are located along the arc-front and decrease systematically toward the east. This may indicate that recent intrusion of subduction-derived mafic melts has been greatest in the mid- to deep-crust beneath the arc front and diminishes in a regular manner toward the east. A straightforward interpretation of this result is that the continental crust is likely younger and more mafic beneath the arc-front as a result of hybridization due to protracted intrusion of subduction-derived, primary basaltic magmas. A further implication of the higher magma volumes along the arc-front is that the degree of mantle partial melting and thus melt production may be greatest along the arc-front.

We discount other models to explain the observed across-arc geochemical trends. For example, Fernández et al. [42] and Kussmaul et al. [44] suggested the trends may reflect crustal melting or contamination of more mafic magmas at increasingly shallower depths eastward. This hypothesis is unlikely because Y and Yb contents, although high in Uturuncu rocks, probably as a result of assimilation of more incompatible element-enriched silicic crustal source rocks, decrease with increasing SiO2 contents for rocks from all centers (Figure 5). This suggests that garnet was in the high-pressure melt residue after assimilation for all three suites, consistent with the experimental studies cited above involving a wide-range of crustal source rock compositions [17]. Furthermore, with increasing SiO2 contents, (La/Yb)n ratios increase for rocks from all centers and broadly overlap or are higher in Uturuncu rocks, consistent with similar amounts of garnet in the residue during crustal melting for all centers and, by extension, comparable depths of differentiation (Figure 7; [116]). This is also consistent with the similar petrographic features of the rocks from all centers, which indicates comparable petrogenetic histories. There is thus no evidence for shallower depths of melting toward the east. In contrast, with increasing SiO2 contents, (Dy/Yb)n ratios (calculated by the method of [116]) decrease in Aucanquilcha rocks, are roughly constant for the Ollagüe suite, and increase for Uturuncu rocks (Figure 7). Similar trends are seen for TiO2 vs. SiO2 for rocks from Aucanquilcha and Uturuncu (Figure 4). Furthermore, FeO contents increase eastward at a given SiO2 content. Collectively these trends can be explained by more mafic, Ti- amphibole-rich lithologies (and residual mineralogies) in the mid-deep crust beneath the arc-front relative to the mid- to deep-crust beneath the back-arc, given that partition coefficients for middle-REE (e.g., Dy) are higher than for heavy-REE (e.g., Yb) in amphibole (see [116,117]). As a result, the trend of smoothly decreasing Sr/Y ratios with increasing Y contents and increasing Eu anomalies from west to east (Figure 5 and Figure 8) are best explained by assimilation in the mid- to deep-crust of progressively more felsic, incompatible trace element enriched crustal compositions (e.g., [118]), as opposed to progressively shallower depths of assimilation.

The presence of plagioclase, either in the source as a residual phase or as a result of fractionation during melt migration, plays a key role in controlling the variations observed in the Sr contents for all three centers. By normalizing Sr to an element such as Y we can observe the effects of plagioclase in the source or during melt migration. The increasing Eu anomalies observed from west to east suggest that beneath the arc front plagioclase is neither retained in the source or fractionated during melt migration. This can be explained by either the stability of plagioclase in the melt or in the source. As suggested by the middle-REE patterns for rocks from Aucanquilcha, a mafic amphibole-rich source explains why fractionation or retention of plagioclase is not observed in either the Sr/Y ratio or the Eu anomaly for these rocks. In contrast, at Uturuncu more pronounced Eu anomalies, lower Sr/Y ratios and middle-REE patterns are observed suggesting fractionation or retention of plagioclase is present either in the source or during migration of the melt.

La/Ta ratios show little correlation with distance from the arc front at 21°–22° S similar to the model proposed by Kay et al. [17] for the Puna ignimbrites. When Ba/Ta ratios are compared to Ta concentrations for the three centers, the highest Ba/Ta ratios coincide with the lowest Ta concentrations (Figure 12). Uturuncu rocks for a given SiO2 have lower Ba concentrations than observed at Aucanquilcha. This relationship further supports the inference made from the Sr/Y ratios that the source beneath Uturuncu is compositionally different than beneath Aucanquilcha. Ba/Ta ratios for Ollagüe overlap with both Uturuncu and Aucanquilcha suggesting that the variation may be more controlled by the Ta concentration of the rocks than the Ba concentration.

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Figure 12. Ba/Ta ratios vs. La/Ta ratios. The Ba/La ratio for rocks sampled at the three centers decreases with distance from the arc front. The grey shaded area labeled arc are the lower limits of ratios among La, Ba and Ta in mafic southern Andean volcanic arc rocks as interpreted by Hickey et al. [82] as inferred from Kay et al. [17]. Ratios observed at Uturuncu are similar to ratios observed by Kay et al. [17] for northern Puna small volume ignimbrites.

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Figure 12. Ba/Ta ratios vs. La/Ta ratios. The Ba/La ratio for rocks sampled at the three centers decreases with distance from the arc front. The grey shaded area labeled arc are the lower limits of ratios among La, Ba and Ta in mafic southern Andean volcanic arc rocks as interpreted by Hickey et al. [82] as inferred from Kay et al. [17]. Ratios observed at Uturuncu are similar to ratios observed by Kay et al. [17] for northern Puna small volume ignimbrites.
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Finally, Dostal et al. [99] suggested a more traditional model to explain the across-arc geochemical variations at 21°–22° S latitude. This model is similar in many respects to models often invoked for oceanic island arc settings or arcs constructed over thin continental crust [6,94,118]. Specifically, Dostal et al. [99] suggested that the proportion of a LILE-enriched hydrous fluid added to the mantle source region for the volcanic rocks decreases across the strike of the arc. Ultimately, this fluid is derived from the subducting, dehydrating Nazca plate. Concomitant with the across-arc decrease in the proportion of a slab-derived fluid is a decrease in the degree of mantle partial melting. This suggestion stems from the well-documented decrease in mantle solidus temperatures with progressive hydration (e.g., [119,120,121]). This model is initially attractive because it can account for the strongly west to east decreasing primary magma production rates as reflected in decreasing eruption volumes of the composite cones at 21°–22° S latitude. This, of course, assumes that magma production rates in the mantle and eruption rates at the surface correlate with the degree of mantle partial melting.

The geochemical implications of decreasing west to east fluid fluxing are two-fold. First, because contents of trace elements with low crystal/liquid partition coefficients (e.g., LILE, REE, HFSE) in primary basaltic melts are a strong function of the degree of partial melting of the mantle source, primary melts generated behind the arc-front will have progressively higher contents of incompatible elements, relative to arc-front magmas, because they derive from smaller degrees of partial melting (this accounts for the K-h relationship). Second, superposed on these first-order variations will be across-arc variations in the LILE contents of the mantle source due to their selective transport and enrichment in slab-derived hydrous fluids [12,122,123]. The LILE enrichments are highest at the arc-front where the proportion of fluid is greatest and they diminish behind the arc. The net effect of these two processes is to produce primary melts with relatively low incompatible trace element contents but high LILE/HFSE and LILE/REE along the arc-front where the mantle is fluxed by larger amounts of slab-derived fluid and partially melts to a greater extent than behind the arc (e.g., [8]). Further, there may also be additional complexities introduced by inherent across-arc variations in mantle source compositions, particularly radiogenic isotopic ratios, prior to or during slab dehydration- or melt-related metasomatism [124].

Any subcrustal model such as that described above is inherently difficult to test and quantitatively model, given the strongly crustal isotopic compositions of the volcanic rocks at 21°–22° S latitude and lack of knowledge of deep-crustal compositions in the CVZ. Interaction of the silicic magmas with thick continental crust is thus expected to mask most of the influence of the slab dehydration fluids and any pre-metasomatic isotopic variations [118]. Geochemical variations consistent with such a model include lower LILE/HFSE and LILE/REE ratios at a given SiO2 content toward the east at the three centers (Figure 7). However, in more detail this model cannot account for numerous other features such as lower Na2O, Ba, and Sr contents (Figure 4 and Figure 5) and higher Sr/Y (where Sr is considered to be more fluid-mobile than Y) and 18O/16O ratios (Figure 8) ratios in Uturuncu rocks relative to those erupted on or slightly behind the arc-front. A subcrustal model invoking an across-arc variation in degrees of mantle partial melting also cannot account for relatively high Nb/Zr ratios in Uturuncu rocks relative to those at Aucanquilcha and Ollagüe, as the degrees of incompatibility between Nb and Zr in mantle solid assemblages are very small (DNb and DZr are estimated to be 0.04 and 0.08, respectively; [125]). Thus, this ratio is not expected to vary strongly with different degrees of mantle partial melting and is instead controlled by the crustal contaminant. Therefore, although decreasing degrees of mantle partial melting with increased distance from the arc front are expected to produce geochemical variations in parental magmas at 21°–22° S latitude (i.e., [126]), we consider the across-arc geochemical and isotopic variations documented for silicic rocks in this study to be largely, if not mostly, crustal in origin. We acknowledge, however, that the more “arc-like” nature (e.g., higher LILE/HFSE ratios) of the silicic rocks erupted on or just east of the arc-front may, in fact, partially reflect greater volumetric intrusion of primary mafic magmas with high LILE/HFSE beneath the arc-front relative to the back-arc, lowering the compositional distinctions between primary magmas and the arc-front crust with time.

Wörner et al. [22] and Harmon et al. [127] observed similar along-strike geochemical trends within the CVZ to the across strike trends. The northern CVZ has been shown to be more radiogenic compared to the south. These authors proposed that this relationship is a function of thicker crust and varying composition of the crust beneath the arc front of the northern CVZ compared to the southern CVZ. Across-arc geochemical variation at 21°–22° S latitude shows a similar relationship to the along-arc variations described by previous authors [22,36,37,96,128] in that variation in the continental crust composition and thickness of the crust is expressed in the volcanic products with increasing distance away from the arc front. Toward the east as the continental crust thickens the volcanic rocks record more radiogenic isotopic signatures inherited from the assimilation of older, less hybridized basement rocks. The source rock composition at the arc-front is less radiogenic as a direct result of intrusion of mafic magmas during the formation of the modern arc-front.

6. Broader Implications

An intriguing result of this study is that on first inspection across-arc geochemical variations at volcanic arcs constructed over thick continental crust, such as increasing K2O and incompatible trace element contents, resemble those observed at island arcs and arcs constructed over thin continental crust. However, on closer inspection there are significant differences, particularly involving systematic variations in isotopic ratios and other geochemical features that reflect interaction with variable composition continental crust with distance from the arc-front. This contrasts with the results of studies of island arcs where the occurrence of K2O-rich magmas in back-arc regions is often ascribed to decreasing additions of slab-derived, LILE-rich hydrous fluids to mantle source regions with concomitant decreases in the degree of mantle partial melting and volumetric production of primary mafic magmas. However, we argue based on the geochemical data presented in this paper and geologic relationships [53] that although across-arc geochemical variations at island arcs and arcs constructed over thick continental crust are produced by apparently fundamentally different processes, ultimately they are both related, directly and indirectly, respectively, to mantle processes associated with the subduction process itself. Specifically, at continental volcanic arcs greater time-integrated primary melt production beneath frontal arc regions has the potential to produce younger, more mafic crustal compositions due to repeated intrusion and hybridization by primary mantle-derived melts. Smaller degrees of mantle partial melting and volumetric melt production in back arc regions results in progressively less hybridized or modified continental crust that retains to a larger degree its more silicic, isotopically evolved composition. Production of intermediate to silicic composition magmas in continental arcs with more “arc-like” chemical (e.g., higher LILE/HFSE) and isotopic features (lower 87Sr/86Sr) in frontal-arc localities relative to back-arc magmas is therefore ultimately linked to higher degrees of mantle partial melting and melt production, as is inferred for island arcs as well. Thus, although subduction zone magmas may be substantially modified by the continental crust resulting in systematic across-arc geochemical trends, these trends are a manifestation that the continental crust has also been substantially modified by fundamental subduction zone processes similar to those proposed for island arcs. In short, the crust thus modifies the compositions of subduction zone magmas, but complimentary to this, subduction zone magmas modify the composition of the continental crust.

7. Conclusions

In an effort to better understand the origin of systematic across-arc geochemical variations in silicic volcanic rocks (60–68 wt % SiO2) from the Andean Central Volcanic Zone, we compared geochemical and isotopic compositions of Quaternary (<1.0 Ma) lava flows erupted at three well-characterized composite volcanoes situated along a narrow southeast striking transect between 21° and 22° S. Trends observed include the following. At a given SiO2 content lavas erupted with increasing distance from the arc-front display systematically higher K2O, P2O5, TiO2, Rb, Th, Y, REE and HFSE contents; Rb/Sr elemental ratios; and Sr and O isotopic ratios. In contrast, the lavas display systematically lower Al2O3, Na2O, Sr, and Ba contents; Ba/Nb, K/Rb, and Sr/Y elemental ratios; and Nd isotopic ratios. In addition, Eu anomalies become progressively more negative toward the east.

These variations are interpreted to indicate that mid- to deep-crustal source rocks for the lavas become progressively older and more feldspar-rich with increasing distance from the arc front. In this regard, silicic magmas erupted along the arc-front reflect melting of relatively young, mafic composition amphibolitic source rocks with garnet-rich, but feldspar-poor residual mineralogies. Towards the east, the lower crust becomes increasingly older with a more felsic bulk composition in which residual mineralogies are progressively more feldspar-rich. The implication of this interpretation is that large-scale regional trends in magma compositions at continental volcanic arcs may reflect a process wherein the continental crust becomes strongly hybridized beneath frontal arc localities due to protracted intrusion of subduction-derived basaltic magmas, with a diminishing effect behind the arc front because of smaller degrees of mantle partial melting and primary melt generation.

Acknowledgments

The authors wish to thank Frank Ramos for use of and assistance with the thermal ionization mass spectrometer at New Mexico State University; Peter Larson at Washington State University for assistance with the O-isotope analyses; Shan de Silva, Duncan Muir, and all members of the PLUTONS working group for insightful discussions; Jamie Kern for field assistance; and the residents of Quetena Chico, Bolivia, and Lipiko Tours for logistical support and hospitality. We thank three anonymous reviews for detailed comments that substantially improved this manuscript. This work was supported by U.S. National Science Foundation grant EAR-0901148 to TCF and grants to GSM from the Department of Earth Sciences at Montana State University.

Conflicts of Interest

The authors declare no conflict of interest.

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