The Lau Backarc Basin (S.W. Pacific) hosts numerous spreading centers and rifts, including the Rochambeau Rifts (RR), Northwest Lau Spreading Center (NWLSC), and Central Lau Spreading Center (CLSC). Samples from the NWLSC, RR and CLSC show no evidence for a subduction-derived component in their mantle source regions or evidence for S loss during eruption. The contents of S in glasses from the NWLSC and many from the CLSC and the RR are lower than MORB at a given FeOTOT, indicating melts were initially sulfide-undersaturated. During differentiation, the decrease in Cu and Ag contents at ∼7 wt% MgO and the concomitant change in chalcophile element ratios marks the onset of sulfide saturation. The initially sulfide-undersaturated compositions of samples from the NWLSC are attributed to partial melting at pressures higher than parental MORB. The NWLSC and some of the CLSC and RR samples are strikingly enriched in Cu and Ag compared with MORB. This is a characteristic shared by basalts generated in many plume-related tectonic settings. The only plume-related samples that appear to be sulfide-saturated during differentiation and plot within the MORB array are alkaline basalts from the nearby Samoan islands. RR and CLSC basalts have a range in Cu contents, which can be explained by variable mixing between a high-Cu NWLSC-type melt with low-Cu sources from the Samoan plume (RR) and MORB-type mantle (CLSC). The RR alone of these three suites have markedly positive Pb, As, Tl and subtle Mo anomalies, possibly related to assimilation of old, hydrothermally altered, Vitiaz Arc crust.
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 Although the mixing of Pacific- and Indian-Type mantle in the northern Lau Basin is generally accepted [Hergt and Woodhead, 2007], the nature and extent of the overprinting OIB signature remains enigmatic. Anomalously high 3He/4He (up to ∼28 Ra), elevated 20Ne/22Ne at a given 21Ne/22Ne and a range of other geochemical proxies have been used to argue for a Samoan plume contribution to magmas erupting at Rochambeau Bank, the Rochambeau Rifts (RR), the Northwest Lau Spreading Centre (NWLSC), Niuafo'ou Island and the Peggy Ridge [Lupton and Craig, 1975; Volpe et al., 1988; Poreda and Craig, 1992; Turner and Hawkesworth, 1998; Falloon et al., 2007; Regelous et al., 2008; Lupton et al., 2009; Tian et al., 2011; Hahm et al., 2012; Lupton et al., 2012a]. The absence of high 3He/4He in magmas erupting at the Central Lau Spreading Center (CLSC) indicates the Samoan plume influence is confined to the northern parts of the Basin. The lateral migration of plume material from the Samoan hot spot (see red arrow on Figure 1b) could follow the western motion of the Pacific Plate at a rate of ∼7 cm/yr [e.g., Koppers et al., 2011, and references therein] and become entrained into the Lau Basin by toroidal flow around the edges of the downgoing Pacific Plate [Schellart, 2004; Stegman et al., 2006; Schellart et al., 2007]. The absence of high 3He/4He in samples from the Mangatolu Triple Junction indicates that the northeastern part of the Lau Basin is isolated from the Samoan plume component by the northern terminus of the Tonga Trench (shown on Figure 1), in accord with tectonic studies of this region [Zellmer and Taylor, 2001; Richards et al., 2011]. Hence, the eastern limit of the opening between the northern Lau Basin and Pacific mantle is likely located only slightly east of the RR, where high 3He/4He values have been reported.
 The high 3He/4He and elevated 20Ne/22Ne at a given 21Ne/22Ne of magmas presently erupting at the NWLSC, the RR and surrounding area can be used to argue for a primitive undegassed mantle component beneath the northern Lau Basin. However, understanding the origin of this component using isotopic systematics (e.g., Sr-Nd-Pb) is complicated, because the composition of primitive mantle lies within the convergence, or focus zone (FOZO [Hart et al., 1992]) of the four mantle end-member compositions (i.e., depleted mantle, HIMU, EM1 and EM2 [seeWorkman et al., 2004, Figure 5]. Hence, alternative tracers are required to understand the origin and distribution of the sources of the RR and NWLSC magmas, which are independent from those of the CLSC magmas. Mixing of a Samoan component with the surrounding Indian-Type mantle (seeTian et al.  for an example of possible mixing models) should affect numerous trace element characteristics, but this is not observed or is unconvincing. For example, samples from the Mangatolu Triple Junction, Peggy Ridge, Rochambeau Bank and Niuafo'ou Island have Gd/Yb comparable to MORB [see Tian et al., 2011, Figure 4] as opposed to the extremely high Gd/Yb typical of Samoan magmas with residual garnet in the mantle source [see Jackson et al., 2010, Figure 4].
 In addition to mixing of source components, the compositions of the magmas erupting at the RR and vicinity could be complicated by crustal contamination. The areas shallower (water depth) than 2000 m in the northern part of the Lau Basin trend approximately parallel to the paleo-Vitiaz Trench (Figure 1a) at comparable distances to those observed between the Tonga Ridge and the Tonga Trench. Conceivably, the ocean floor in the northern part of the Lau Basin is the stretched and boudinaged basement of the Paleogene-early Neogene Vitiaz Arc. The absence of clear correlation between3He/4He and other isotopic systems in magmas erupting at and around the RR may indicate the parental magmas are contaminated by variable mixing with a basement of crustal material produced during the active stage of the Vitiaz Arc. The trend to high-87Sr/86Sr and low-143Nd/144Nd of some magmas erupting at Rochambeau Bank and Niuafo'ou Island is consistent with ingress of a Samoan plume component [i.e., Tian et al., 2011]. Alternatively, this component may have been inherited by introduction of Samoan-derived, high-87Sr/86Sr volcaniclastic sediments to the mantle wedge during previous stages of subduction along the Vitiaz Trench, and/or crustal contamination during ascent of the parental magmas from high 87Sr/86Sr arc magmas comprising the Vitiaz Arc crust. Indeed, the diffusively extended topography of the RR indicates the evolution of this area is not just a simple spreading ridge, unlike the linear structure observed at the NWLSC (Figure 2), which is more distal from the Paleo-Vitiaz Trench (Figure 1). Hence, samples from the NWLSC, which also have elevated 3He/4He ranging from 7.4 to 20.8 Ra, provide an ideal opportunity for constraining the nature of the OIB component, which can be compared with the potentially more complicated RR samples.
 Here we present major and trace element compositions for samples from the RR, NWLSC, and CLSC (Table S1 in the auxiliary material). Samples were recovered during the SS07/2008 research voyage (NoLauVE) of the Australian Marine National Facility RV Southern Surveyor.Major (EMPA) and trace element analyses (LA-ICP-MS) for these samples were undertaken at the Research School of Earth Sciences, Australian National University, following methods described in previous contributions [Jenner et al., 2009; Jenner and O'Neill, 2012b, 2012a]. The data presented here for samples from the RR, NWLSC, and CLSC contain the typical set of trace elements used to understand the petrogenesis of basaltic magmas (i.e., rare earth elements (REE), large ion lithophile elements (LILE), high field strength elements (HFSE), the first row transition elements (FRTE), and a selection of less commonly analyzed elements (i.e., Li, Be, Ge, Ga, As, Se, Mo, Ag, Cd, In, Sn, Sb, W, Re, Tl, and Bi), which are used here to provide additional constraints on mantle source characteristics. The tectonic setting in which the samples from the RR, NWLSC, and CLSC are generated is complex: backarc basin samples with potential plume, MORB-source, subduction-related and crustal inputs. Hence, data for samples from these centers and rifts are compared against a complementary data set of analyses of ocean floor basalts from a range of fracture zones and spreading ridges from the Pacific, Atlantic, and Indian Oceans (data fromJenner and O'Neill [2012a]), collectively referred to here as mid-ocean ridge basalts (MORB), for ease of reference. Data sets of analyses that include the total range in trace elements reported herein are currently unavailable for samples from the Samoa subaerial and submarine chain. Hence, we present new analyses of ten sub-aerially erupted volcanic glasses from a single lava flow of the Pu'u'O'o eruption (11.30 A.M., 1 November 2000), Kilauea volcano, Hawaii [seeGarcia et al., 2000; Pietruszka et al., 2006] as an example of typical OIB (Table S1). We include for comparison, selected elemental data (Nb, Yb and Th; Table S2) for samples from ridges and rifts in the eastern Lau Basin (Valu Fa and Fonualei) with a well-defined subduction input.
 Since the publication of the Pual Ridge and vicinity, Eastern Manus Backarc Basin data set (Jenner et al. referred to in the following text as the Manus Basin), there have been improvements in calibration values (NIST SRM 612) and analytical protocols for LA-ICP-MS techniques [seeJenner and O'Neill, 2012b]. Hence, the data presented in Jenner et al.  are updated and presented here (Table S3) as an example of an arc-proximal backarc sample suite with a strong subduction influence, and as a complementary extension to the global ocean floor basaltic data file ofJenner and O'Neill [2012a]. Pervasive degassing during eruption of samples from the Manus Basin resulted in loss of S to levels close to the limit of detection of the electron microprobe [Jenner et al., 2010]. Hence, we present more precise data for low S contents in samples from the Manus Basin (Table S3), together with Cl, CO2, H2O and F, using the Cameca IMS 6f ion microprobe housed at the Department of Terrestrial Magnetism, following the techniques described in Hauri et al. .
 Samples from the NWLSC are basaltic in composition, except NLD39 and NLD41, which are classified as basaltic andesite and andesite, respectively. FeOTOT, TiO2, V, Re, S and Se in the NWLSC show a systematic increase in contents with decreasing MgO, until ∼5 wt.% MgO, followed by a marked drop in contents with further decreases in MgO (Figure 3). Glasses from the NWLSC are characterized by very high Cu contents, and consistently higher Ag, and Re at a given MgO compared with MORB (Figure 3) and primitive mantle values (PM values from Palme and O'Neill ) of Re (0.32 ppb), Cu (20 ppm) and Ag (4 ppb). Cu and Ag contents show a subtle increase with decreasing MgO from 8.7 to ∼7 wt.% MgO, followed by a progressive decrease in samples with <7 wt.% MgO (Figure 3). Basaltic glasses from the RR and CLSC have a more limited range in MgO contents compared to samples from the NWLSC (Figure 3). Additionally, the most MgO-rich samples from the RR have slightly higher TiO2 and S, lower V and Cu, and display less coherent trends in compositions compared to samples from the NWLSC (Figure 3). Samples from the CLSC can be distinguished from those collected from the NWLSC and the RR by the consistently lower TiO2 contents at a given MgO (Figure 3b), have a similar range in Cu contents to samples from the RR (Figure 3g) and lack a coherent fractionation trend. Our limited sample set from Hawaii has a restricted compositional range that can be distinguished from samples from the NWLSC, RR and CLSC by the higher TiO2 at a given MgO, but with FeOTOT and V contents comparable to those from the RR (Figure 3). In addition to samples from the NWLSC and a number of samples from both the RR and CLSC, samples from Hawaii have elevated Cu and Ag contents compared to the MORB array.
 Trace element abundances normalized to PM of samples from the NWLSC, RR, CLSC and Hawaii are shown in Figure 4. In addition to the typical range in elements presented on PM-normalized diagrams, we have extended the list to include analyses of Be, Zn, Ge, Ga, As, Mo, Cd, In, Sn, Sb, W, Tl and Bi to establish whether these elements can be used to place further constraints on the petrogenesis of the suites of samples from the NWLSC, RR, and CLSC. To avoid additional congestion, the trace elements displayed inFigure 3 are not included in Figure 4. The additional elements have been added to the traditional sequence (intended to span from highly to mildly incompatible relative to a peridotite assemblage) in their ‘approximate’ positions with respect to their incompatibility relative to refractory lithophile elements (i.e., As, Mo, Sn, Sb and Pb between refractory lithophile elements Ce and Pr [e.g., Palme and O'Neill, 2003]. However, the overall ordering of the chalcophile/siderophile elements that are displayed on Figure 4 (i.e., Mo, As, Sb, Ge, Sn, In, Bi, Pb and Tl positioned between Ce and Pr) is chosen as a means for demonstrating the range in compositions of samples presented here by achieving a coherent trend between Sb and Mo on Figure 4 for samples from the NWLSC, RR and CLSC compared with MORB, as opposed to providing a definitive ordering with regards to compatibility.
 NWLSC glasses have flat HREE patterns (Gd/YbPM ranging from 0.99 to 1.15), are variably depleted in LREE (La/SmPM ranging from 0.33 to 0.95), have positive Nb anomalies relative to Ta and U, variable enrichments in Rb and Ba relative to Cs and W, and depletions in Pb and As relative to In and Pr (Figure 4a). With decreasing MgO content, samples show progressively increasing negative Sr, Eu and Ti anomalies compared to neighboring REE on primitive mantle-normalized plots, and an overall increase in abundances of trace elements. RR glasses display a narrower range in trace element contents and higher Gd/YbPM (1.15–1.48) compared to samples from the NWLSC (Figure 4b), are LREE-depleted to enriched (La/SmPM = 0.68–1.73), have Nb enrichments relative to U and Ta comparable to samples from the NWLSC and MORB, and show variable enrichments in Rb, Ba, and Sr, and depletions in Y compared to samples from the NWLSC. A striking feature of the RR samples are the positive Tl spikes and the less pronounced, or absent, Pb and As depletions relative to In and Pr when compared to both MORB and samples from the NWLSC (Figures 4c and 4d).
 The CLSC samples are broadly similar to the most depleted MORB in terms of the range from incompatible to relatively compatible trace element abundances (Figure 4e), with a range in La/SmPM from 0.30 to 0.51, and depleted to enriched HREE patterns (Gd/YbPM range form 0.87–1.06). Samples from the CLSC show depletions in Pb and As relative to In and Pr, and enrichments in Nb relative to U and Ta, similar to MORB and samples from the NWLSC. The NWLSC and CLSC samples have considerably smoother trace element patterns from Sb to In, and RR from Sb to As, compared to the MORB array (MORB show pronounced depletions in Sb, Ge and Bi relative to Zn and Cd, and typically more pronounced depletions in As relative to Tl). In addition, samples from the NWLSC, Hawaii, and many of the samples from the CLSC lack the distinctive positive Mo anomalies relative to Tl and Pr of MORB. In contrast, the RR have enrichments in Mo relative to Pr. Hawaiian basalts have trace element patterns from Cs to In similar to samples from the NWLSC (Figure 4e) and the more LREE-enriched MORB samples. However, the HREE patterns are highly fractionated (Gd/YbPM = 2.12–2.21) compared to the NWLSC, RR, and CLSC (Figure 4e). Hawaiian glasses show depletions in Tl relative to As and Mo, and subtle enrichments of Sr relative to Be and Sn.
3. Source Characteristics of MORB, Hawaii and the Manus Basin Magmas
 The spectrum of MORB compositions (Figure 4) with a continuum from LREE-enriched to depleted character provides an important comparator for the Lau Basin samples. We note this continuum renders any presentation of a normal-MORB (NMORB), enriched MORB (EMORB), or average MORB value for normalization purposes as likely misleading [Hofmann, 2003; Jenner and O'Neill, 2012a]. Hence, we use the entire MORB array plotted against PM to embrace the entire range in compositions generated at mid-ocean ridges (Figure 4) for comparison with samples generated in other tectonic settings, as opposed to the use of NMORB-normalized plots.
 In the context of this contribution, we note MORB are characterized by enrichments in Rb and Ba relative to Cs and W, enrichments in Nb relative to Ta and U, and depletions in chalcophile elements Sb, Ge, Bi, Pb, As and Tl relative to Ce when compared to PM. MORB show a striking enrichment in Mo relative to both Ce (Mo/CePM = 2.26 ± 0.49) and Pr (Mo/PrPM = 2.15 ± 0.49), despite their similar incompatibilities during differentiation of basaltic melts [Newsom et al., 1986; Sims et al., 1990; Fitton, 1995; Jenner and O'Neill, 2012a], indicating the higher incompatibility of Mo compared to both Ce and Pr during melting of the MORB source mantle. Alternatively, the high Mo/Ce and Mo/Pr of MORB compared to PM may indicate the PM value for Mo is too high, and the method for estimating the Mo content of PM needs to be reassessed. Samples from Hawaii have trace element patterns comparable with the most LREE-enriched MORB (Figure 4e), with the exception of the highly fractionated HREE patterns of the former, demonstrating the presence of residual garnet in their mantle source region during melt extraction at high pressures [e.g., Chen et al., 1991]. A notable difference between the trace element patterns of MORB compared to samples from Hawaii are the absence of Mo anomalies relative to Ce (Mo/CePM = 1.06–1.15) and Pr (Mo/PrPM = 1.13–1.25), possibly indicating the compatibility of Mo in garnet, although to the authors' knowledge, appropriate partition coefficients for Mo between garnet and silicate melt are currently unavailable to test this hypothesis.
 In contrast to MORB and Hawaii, arc-proximal Manus Basin samples (Figure 4f) show enrichments in Cs, U and Pb compared to LREE, Sr relative to Nd, and pronounced depletions in Nb and Ta relative to La, typical of convergent margin basalts [e.g., Plank and Langmuir, 1988; Chauvel et al., 1995; Morris and Ryan, 2003; Pearce et al., 2005; Plank, 2005]. In addition, subduction-related basalts from the Manus Basin have enrichments in Bi relative to Ga, As, and Tl relative to Pr, and substantially higher Sb/Ce compared to PM, MORB, and Hawaii. The enrichment of As, Tl and Sb in subduction- related magmas compared to MORB is consistent with previous studies [Noll et al., 1996; Hattori et al., 2002]. In contrast, Mo is not enriched in the Manus Basin suite: the Mo/CePM ranges from 1.60 to 2.69, and Mo/PrPMfrom 1.62 to 2.94, similar to the range of MORB values, indicating only limited mobility of Mo during subduction-related processes. The enrichment of some chalcophile/siderophile trace elements in samples from the Manus Basin (As, Sb, Tl, Bi and Pb), but depletions or MORB-like abundances in others (S, Se, Cu, Ag and Mo;Figures 3 and 4), indicates the processes controlling the behavior of these elements in the subducted slab and mantle wedge are distinct from the mantle source region of MORB. Geochemical studies of pristine and hydrothermally altered oceanic crust, and black smoker-type hydrothermal fluids have shown Tl is particularly susceptible to leaching during hydrothermal alteration by high temperature (>250–300°C) fluids [Nielsen et al., 2006]. Similarly, trace element analyses of sulfides associated with black smokers and other types of hydrothermal deposits have noted enrichments in As, Sb, Tl, Bi and Pb [Hannington et al., 1991; Shin et al., 2004; Kristall et al., 2011]. Hence, enrichment of the mantle wedge via subduction of hydrothermally altered oceanic crust and associated low-temperature As-Sb-Tl-Bi-Pb sulfides, as previously suggested to explain the enrichments in Pb in arc magmas and the continental crust compared to MORB [Chauvel et al., 1995], could explain the enrichment of the source region of the Manus Basin magmas in these chalcophile elements relative to others such as Cu, Ag. Alternatively, the processes taking place during black-smoker type hydrothermal alteration may be resulting in the leaching of As, Sb, Tl, Bi and Pb relative to the REE from the oceanic crust during subduction, but on a considerably larger scale than observed on the seafloor.
 During differentiation of MORB magmas, the contents of both Cu and Ag decrease with decreasing MgO, consistent with the removal of sulfide liquid during differentiation (Figure 3). The lack of enrichment of Cu and Ag in the primitive Manus Basin samples compared to MORB, as previously demonstrated by Jenner et al. , may indicate these magmatic sulfides reside in the gabbroic layers of the oceanic crust (∼1–2 km depth beneath the ocean floor [see Klein, 2003]) and as a consequence, have little impact on the budget of chalcophile elements supplied to the mantle wedge during subduction (i.e., they are located too deep in the oceanic crust).
4. Source Characteristics of the Northwestern Lau Basin Magmas
 On PM-normalized plots, samples from the NWLSC, CLSC, and RR show a number of notable geochemical characteristics compared with the MORB spectrum. For example, samples from the NWLSC lack positive Zn, Cd and Mo anomalies; the CLSC basalts show only subtle enrichments in Mo; and RR basalts have distinctively smooth trace element patterns between Sb and As compared to MORB (Figure 4). Similarly, the elevated Re, Cu, and Ag contents at a given MgO indicate the petrogenesis of the samples from the NWLSC and a number of samples from the RR and CLSC was distinct from that of MORB (Figure 3). In contrast to Hawaiian basalts, the most primitive samples from the NWLSC (>8 wt.%) have relatively flat HREE patterns, which are comparable to typical MORB (Gd/YbPM = 1.00–1.15), indicating that garnet was not a residual phase in the mantle source region during partial melting. However, the most primitive samples from the CLSC (Gd/YbPM = 0.87–1.06) and the RR (Gd/YbPM = 1.15–1.48), have a range in HREE abundances, indicating the involvement of residual garnet in their mantle source regions at some stage during their petrogenesis, either in the source mantle (i.e., prior melting of the mantle source region of the CLSC magmas within the garnet stability field to achieve the low Gd/YbPM during subsequent melting) or during melt extraction (i.e., to achieve the high Gd/YbPM of a number of samples from the RR). Nevertheless, the elevated Gd/YbPM of samples from the RR are less pronounced than samples from Hawaii and Samoa (Figure 4e). Hence, samples from the NWLSC, CLSC, and RR are geochemically distinct from MORB and Hawaiian basalts. However, we note the samples from Hawaii are also enriched in Cu and Ag at a given MgO compared to the MORB array, which is a distinctive feature of samples presented here from the NWLSC (Figure 3).
 Neither the CLSC, NWLSC, nor the RR samples have the strong enrichments in Cs and U or depletions in Nb and Ta relative to neighboring elements on PM-normalized plots, characteristic of subduction-related volcanic rocks, such as those from the Manus Basin (Figure 4f). Additionally, PM-normalized patterns for samples from the NWLSC and CLSC (Figures 4a and 4e) show depletions in Pb, As, and Tl relative to In and Pr, which are completely different to the geochemical signatures of subduction-related magmas from the Manus Basin. The lack of a subduction-derived input to the source region of the CLSC, NWLSC, and RR magmas can also be demonstrated on a plot of Th/Yb versus Nb/Yb (Figure 5). The majority of these samples plot within the MORB array, from relatively depleted (CLSC) through moderate (NWLSC) to enriched character (RR), whereas volcanic glasses from the Pual Ridge region of the Manus Basin, the Fonualei and Valu Fa Rifts (eastern Lau Basin) have elevated Th/Yb at a given Nb/Yb compared to the MORB array, resulting from the mobility of Th relative to Nb during subduction-related processes [e.g.,Pearce, 2008]. Trace element compositions of samples from the CLSC, NWLSC, and RR show no evidence in terms of established trace element criteria for crustal contamination and/or enrichment of the mantle source region by a subduction-derived component. The lack of evidence for a subduction component to the mantle source region of the NWLSC and the RR magmas is in agreement with plate reconstructions based on earthquake distributions [Benz et al., 2011; Richards et al., 2011], which indicate the northern limit of the subducting Pacific Plate is located south of both the NWLSC and the RR (Figure 1b). Samples from the RR are geochemically distinct from those retrieved from the NWLSC and the CLSC because of the elevated Pb and As relative to In and Pr, and pronounced spikes in Tl and Mo relative to Pr on PM-normalized plots (Figures 4b and 4d). These specific characteristics are comparable to those displayed by the subduction-related samples from the Manus Basin. However, the lack of other diagnostic trace element patterns of subduction-related basaltic magmatism suggests an alternative origin for these specific chalcophile element enrichments, which will be discussed below. In contrast to the RR and NWLSC, the CLSC is located directly above the subducting Pacific Plate (Figure 1b) and despite the highly depleted compositions of the erupting magmas (i.e., the extremely low incompatible element contents, making them particularly susceptible to overprinting by subduction-derived fluids or melts;Figure 4), these samples also show no trace element evidence of a subduction-zone signature. Hence, we infer the Pacific Plate surface temperature increased from ∼730°C below the Tonga arc (slab depth = 123 km) to ≥900°C by a depth of ∼300 km, resulting in the destruction of the key volatile-hosting phases such as phengite, allanite and monazite [Hermann and Spandler, 2008; Klimm et al., 2008; Skora and Blundy, 2010; Syracuse et al., 2010; Cooper et al., 2012; Ruscitto et al., 2012]. We conclude there is no unequivocal evidence for involvement of subducted Pacific Plate components in the mantle source regions as west as the RR, NWLSC or the CLSC.
5. Mantle Source Variability
 Samples from the CLSC, NWLSC, and RR have a large range in incompatible element contents and ratios (Figures 4 and 5). Even within the NWLSC sample set containing >8 wt.% MgO, there is a high degree of variability in trace element patterns (Figure 4c). In terms of Nb/Yb versus Th/Yb, the most primitive magmas from the NWLSC (>8 wt.% MgO) have a range in compositions spanning almost half the entire MORB array (Figure 5). The lack of a subduction-related input to the source region of the CLSC, NWLSC, and RR magmas indicates the variability can be attributed either to progressive depletion of the mantle source region, variations in the degree of partial melting, and/or variable mixing with an enriched OIB end-member composition (the Samoan plume).
 The high MgO contents of the most mafic samples (>8 wt.%), which occur along the length of the NWLSC (Figure 6a), indicates the parental magmas were generated by similar degrees of partial melting. The range in LREE patterns (e.g., La/Sm from 0.33 to 0.95) within the five most mafic samples is too large to be attributed to single magma chamber processes, such as fractional crystallization, because of the limited range in MgO contents. Figure 6b shows the melts erupting along the NWLSC, in particular the samples with >8 wt.% MgO, have systematically lower La/Sm in the central, relatively shallow parts of the Center (Figure 2, samples enclosed within the white circle), compared to the deeper northeastern and southwestern tips. The distribution in La/Sm (shaded fields on Figure 6b) indicates melt production/extraction was greater toward the middle of the NWLSC, resulting in a more rapid short-term depletion of the mantle source region feeding magmatism in this area compared with the propagating tips. Alternatively, the high La/Sm, Nb/Yb and Th/Yb could be attributed to mixing with a Samoan OIB component, as suggested for samples from the RR and surrounding area [Tian et al., 2011]. If lateral migration of the Samoan component is responsible for the range in La/Sm, Nb/Yb, and Th/Yb of NWLSC samples, these ratios would be expected to decrease from NE to SW along the rift. This is not observed so we attribute the range in La/Sm, Nb/Yb and Th/Yb of NWLSC samples to variable degrees of melt extraction and depletion of the underlying mantle source region.
 In contrast to La/Sm, 3He/4He remains approximately constant along the length of the Center, at values notably higher than typical MORB [see Lupton et al., 2009], consistent with variable degrees of partial melting of a specific source mantle. Trace element abundances of samples from the Lau Basin show only weak correlations with variations in radiogenic isotopic systems, such as Nd, Sr, and Hf [e.g., Pearce et al., 2007; Tian et al., 2011]. We suggest rapid opening of the Lau Basin, resulting in pervasive melt extraction and localized variations in trace element proxies of mantle depletion, as exemplified by samples from the NWLSC, is likely the major variable contributing to the weak correlations between trace element and isotopic systematics.
 Samples from the southern parts of the overlapping rifts forming the CLSC (white symbols, Figure 2) have slightly higher Gd/YbPM and lower La/SmPM (Gd/YbPM ranging from 0.98 to 1.06 and La/SmPM of 0.30–0.43, respectively) compared to samples from the northern parts of the CLSC (Gd/YbPM of 0.87–0.92 and La/SmPM of 0.38–0.51, respectively; red symbols on Figure 2). Additionally, northern samples from the CLSC have consistently higher Cu and Ag contents at a given MgO compared to southern samples (distinguished on Figures 3g and 4e). The subtle geochemical differences for samples from the CLSC, which can be related to their geographic locations, indicate slight variations in the petrogenesis of magmas erupting along the CLSC, which may be linked to the ages of the rifts. Samples from the RR show no clear correlations between La/Sm and Gd/Yb with either latitude or longitude. The samples with Cu contents at a given MgO that plot above the MORB array are typically erupting in the southern parts of the RR (closest to the NWLSC; yellow and red symbols on Figure 2), however the correlation is less pronounced compared to the systematic geochemical variations of CLSC and NWLSC magmas. Hence, samples from the NLWSC, CLSC and RR preserve evidence for complex trace element systematics, which can be linked to either compositional differences between the mantle source regions (e.g., the CLSC and the RR) or the evolution of the mantle source region during progressive melt extraction (e.g., the NWLSC). Additionally, RR samples have consistently lower V and higher Ti contents at a given MgO (notably comparable to Hawaiian basalts, Figure 3), indicating the parental magmas of the NWLSC and the RR were compositionally distinct, possibly as a result of redox variability [Mallmann and O'Neill, 2009] and/or source mixing. The lower TiO2 of the CLSC samples (Figure 3b), coupled with the extremely low Nb/Yb and Th/Yb (Figure 5) demonstrates the mantle source region of the CLSC magmas was more depleted than the source of both the NWLSC and RR magmas.
 Using the highest MgO samples from each spreading center, their respective Nb contents and the lack of discernable differences in primary CO2/Nb between mantle sources characterized by high 3He/4He and MORB-like ratios in samples from the Lau Basin [Hahm et al., 2012], we can calculate CO2 fluxes assuming a mantle source CO2/Nb of 530 similar to average undegassed MORB [Cartigny et al., 2008]. With magma production rates estimated for each area of 0.033 km3/yr (RR and NWLSC) to 0.12 km3/yr for CLSC [Taylor et al., 1996; Crawford et al., 2003], we can calculate CO2 fluxes from the RR (1.2 × 109 mol/yr), CLSC (1.5 × 109 mol/yr), and NWLSC (4.3 × 109mol/yr). Scaled to the 377 km total length of these three back-arc ridge segments, this represents a CO2flux per km of ridge that is similar to that estimated for depleted mid-ocean ridges [Saal et al., 2002], suggesting that most of the CO2subducted beneath the Lau Basin is either delivered efficiently to Tonga arc volcanoes, or is subducted beyond the depths of back-arc magma generation.
6. Chalcophile Element Systematics During Low-Pressure Differentiation
 In contrast to MORB, volcanic glasses from the Manus Basin record a muted increase in FeOTOT and TiO2 with decreasing MgO (Figure 3). Contrasting fractionation paths can be attributed to differences in the sequence of crystalline phase appearance on the liquidus of ‘dry’ MORB melts (olivine-plagioclase-clinopyroxene) compared to ‘wet’ subduction-related melts (olivine-clinopyroxene-Ca-rich plagioclase-amphibole), resulting in the evolution to typically higher SiO2 contents of the latter [see Arculus, 2004], and the lower frequency in eruption of high MgO compositions. Between 9 and 3 wt.% MgO, samples from the Manus Basin show an increase in Se, Cu, and Ag and relatively constant Cu/Se, Ag/Se and Ag/Se with decreasing MgO, indicating these melts were sulfide-undersaturated [Jenner et al., 2010]. The extremely low S contents and highly variable S/Se in Manus Basin samples with between 9 and 3 wt.% MgO (S/Se ranges from 291 to 639) indicate S was lost via degassing during eruption (Figure 3), complicating interpretations of the behavior of S during magma chamber processes. In addition to S loss, pervasive degassing of samples from the Manus Basin is evident from extremely low CO2 contents (2.00–4.35 ppm; Table S3) and the high relative standard deviation (1σ) in replicate (3) analyses of both CO2 (1–88%) and H2O (0.8–12%). Fortuitously Se mimics the behavior of S during differentiation (Figure 3f), but unlike S (and other volatile elements such as CO2), Se is not lost during degassing [Jenner et al., 2010], likely linked to differences in redox systematics between S and Se; sulfur transitions from S2− to S6+, whereas Se transitions from Se2− to Se4+ with increasing fO2 [Wykes et al., 2011]. Consequently, the measured content of Se ([Se]), in combination with an estimation of the initial S/Se of the melt prior to degassing, can be used to estimate the content of S (S*) in a melt prior to degassing and to constrain the behavior of S during differentiation in a crustal magma chamber prior to eruption [Jenner et al., 2010]. Assuming a S/Se of between 3000 (approximate S/Se of primitive MORB), S* in the most primitive Manus Basin sample (MD3; [Se] = 0.131 ppm) is 392 ppm (open triangles on Figure 3). However, the mantle source region of the Manus Basin magmas is typically considered to be highly depleted [Kamenetsky et al., 2001; Sinton et al., 2003; Jenner et al., 2010], consistent with the higher Cu/Se and Ag/Se of the most primitive samples from the Manus Basin compared to MORB (differences in the relative compatibility of the chalcohile elements in mantle sulfides (S < Se < Cu ≈ Ag) would result in an increase in Ag/Se, Cu/Se and decrease in S/Se with progressive depletion of the source [Hamlyn et al., 1985; Peach et al., 1990; Stimac and Hickmott, 1994; Jenner et al., 2010]. Consequently, the initial S/Se of the Manus Basin magmas is likely to be substantially lower than MORB. Using a lower S/Se of 1800 [see Jenner et al., 2010], S* of the most primitive Manus Basin sample is 235 ppm (open circles on Figure 3). Both estimates of S* indicate the primitive Manus Basin magmas would be sulfide undersaturated even if all the S in the melt was dissolved as S2− (Figure 8a), and both estimates are substantially lower than the levels required to achieve S-saturation in relatively oxidized magmas [Jugo et al., 2005].
 At ∼3 wt.% MgO and with further decreases in MgO, the contents of Se, Cu, Ag and the Cu/Se and Ag/Se suddenly decrease, coincident with onset of magnetite-fractionation (Figures 3 and 7). This decrease was attributed by Jenner et al. to magnetite-triggered sulfide saturation (the ‘Magnetite Crisis’), because a modest change in the Fe redox ratio of the melt, resulting from magnetite fractionation, has a dramatic effect on sulfur speciation; the dissolved S in the melt switches from mostly sulfate to sulfide, forcing the appearance of sulfide on the liquidus. Prior to the Magnetite Crisis, [Se] = 0.360 ppm (average of samples MD7a and MD7b), indicating an increase in the S content of the melt from 235 ppm in the most primitive sample to 648 ppm (assuming a S/Se of 1800), complemented by an increase in the contents of Cu and Ag from 88 to 281 ppm, and from 0.038 to 0.084 ppm, respectively.Jenner et al.  used the change in Ag/Cu following the Magnetite Crisis, which is not observed in MORB (Figure 7d), to suggest saturation in a crystalline Cu-rich sulfide phase, such as bornite, at this stage in the evolution of the Manus Basin melts, as opposed to the removal of sulfide melt during the differentiation of MORB melts. Hence, the drop in [Se] resulting from sulfide saturation (Δ[Se] = 0.160 ppm; calculated between samples MD7 and MD8) and the S/Se of bornite (S/Se of 904, from the average of four analyses of Cu rich sulfide fromCore et al. ) can be used to estimate the complementary drop in S (Δ[S*]) following sulfide saturation to be 145 ppm (Δ[S*] = Δ[Se] × (S/Se)bornite; see Jenner et al.  for further discussion). Hence, S* in the melt following the ‘Magnetite Crisis’ is 503 ppm (slight differences in the estimations of S* presented here for the Manus suite compared to those presented in Jenner et al. , result from improvements in LA-ICP-MS analytical techniques described in detail inJenner and O'Neill [2012b].
 Using a S/Se of 1800 for the parental melt, [S*] calculated both prior to and following the Magnetite Crisis (648 and 503 ppm, respectively) plot below the S-saturated MORB array (open and black circles;Figure 8a). However, because the melts evolved to high Cu contents prior to sulfide saturation, the compositions of the Manus Basin magmas at sulfide saturation plot within the Cu-rich, Ni poor, S-saturated melt array [Ripley et al., 2002; Jenner et al., 2010, Figure 8], indicating saturation in a Cu-rich sulfide phase was likely. Using the MORB S/Se of 3000 does give a S* prior to sulfide saturation that plots within the MORB S-saturated array (open triangles,Figure 8a). However, as explained above, it is likely that the S/Se of the parental melt of the Manus suite was substantially lower than MORB, indicating a S/Se value of 3000 is too high. To fully exploit the use of S* for tracking the behavior of S in degassed magmas, and in particular, for estimating the initial contents of S in mantle-derived melts, a systematic -study of the variations in S/Se of a melt with varying pressures, degrees of mantle depletion and a range infO2 is required.
6.2. Low-pressure Fractionation of Chalcophile Elements in the NWLSC Magmas Prior to Magnetite Fractionation
 Despite the overall spread in La/Sm, Th/Yb, and Nb/Yb, the most primitive samples from the NWLSC have a relatively limited range in major and minor element compositions (Figure 3). Additionally, samples from along the length of the NWLSC converge on a coherent fractionation path indicative of predominantly low-pressure fractional crystallization prior to eruption, from parental melts with similar major element compositions. In contrast to samples from the NWLSC, samples from the CLSC and RR have a larger range in major and minor element compositions at a given MgO content, and less well-defined fractionation trends, indicating the parental melt compositions were more variable. In particular, the CLSC and the RR have a large range in Cu and Ag contents that span the region between the NWLSC samples and the MORB array. Accordingly, here we focus on the better-defined low-pressure fractionation trend of the NWLSC suite that spans a larger range in MgO contents compared to the CLSC and RR.
 The trends in major element contents with decreasing MgO of the NWLSC suite are more comparable to nominally anhydrous MORB than the Manus Basin suite (Figure 3). FeOTOT, TiO2, V, and Re contents of NWLSC samples show an initial increase with decreasing MgO until ∼5 wt.% MgO, followed by a decrease in abundances with further differentiation, attributable to the appearance of magnetite on the liquidus (Figure 3). The complementary decrease in Re at the onset of magnetite saturation in samples from both the Manus Basin and NWLSC supports the conclusion of Jenner et al. that Re is magnetite-compatible during low-pressure differentiation.
 The contents of S and Se in primitive samples from the NWLSC are comparable to MORB and both elements mimic the behavior of FeOTOT during differentiation (Figures 3e and 3f). Unlike samples from the Manus Basin, and Hawaiian subaerially erupted magmas, samples from the NWLSC (plus CLSC and RR) show no evidence for S-loss during eruption. In contrast to S and Se, initial contents of Cu, Ag, and Re in NWLSC glasses are substantially higher than MORB. Further, unlike MORB, Cu and Ag initially increase until ∼7 wt.% MgO, at which stage contents of both elements decrease with further differentiation of the melts. The initial increase in Cu and Ag and the approximately constant Se/S, Cu/S, Cu/Se, and Ag/Se of samples from the NWLSC (Figure 7) indicates the parental melts were sulfide-undersaturated, similar to the Manus Basin. This conclusion is supported by consistently lower contents of S (∼100–200 ppm) at a given FeOTOTof NWLSC samples with >8 wt.% MgO compared to the sulfide-saturated MORB array (Figure 8a inset). The contents of Cu and Ag in samples from the NWLSC decrease with decreasing MgO in samples with <7 wt.%, indicating saturation in a sulfide phase was achieved by ∼7 wt.% MgO. This interpretation is supported by changes in Se/S, Cu/S, Cu/Se and Ag/Se at this stage in melt evolution. Notably, the Ag/Cu of samples with between 4 and 7 wt.% MgO remains constant, and Se/S, Cu/S, Cu/Se and Ag/Se decrease at a comparable rate to MORB, indicating removal of sulfide melt as opposed to a crystalline sulfide phase during early stages of differentiation of the melt (Figure 7). The content of Re continues to increase regardless of the decrease in Cu and Ag (Figure 3d), demonstrating Re is not compatible in the fractionating sulfide melt.
 The change in partitioning behavior of Cu and Ag coincides with the liquid line of descent for S versus FeOTOTmoving into the MORB sulfide-saturated array (evolution of the NWLSC melt shown by arrows onFigure 8a inset), demonstrating the higher bulk partition coefficient of FeOTOT compared to S prior to sulfide saturation. Unlike samples from the Manus Basin, sulfide saturation in samples from the NWLSC (∼7 wt.% MgO) is achieved prior to the onset of magnetite fractionation (∼5 wt.% MgO; Figure 3). Hence, magnetite-triggered-reduction of the evolving magma was not required to trigger sulfide saturation; i.e., the primitive melts generated in the NWLSC were less oxidized than samples from the Manus Basin and more similar to MORB.
 Unlike Cu and Ag, the content of S in samples from the NWLSC continues to increase between 7 wt.% MgO and ∼5 wt.% MgO (Figure 3e), because the solubility of S is predominantly controlled by the proportion of FeOTOT [O'Neill and Mavrogenes, 2002], with the net surplus of S relative to FeOTOT during differentiation removed by sulfide precipitation. Similarly, the content of Se also increases between 7 and 5 wt.% MgO (Figure 3f), which can likely be attributed to Se occupying the same site in the melt structure as S (i.e., the sulfur content at sulfide saturation (SCSS) is actually the sum of S+Se), resulting in the relatively constant, or subtle decrease in Se/S of MORB and the NWLSC samples with between 7 and 5 wt.% MgO; Figure 7). Hence, Cu and Ag are more useful for pinpointing the onset of sulfide saturation than S and Se.
6.3. Low-pressure Fractionation of Chalcophile Elements in the NWLSC Magmas After Magnetite Fractionation
 Curiously, the most evolved NWLSC samples (<4 wt.% MgO; Figure 8a) plot on a trend between S and FeOTOTat an angle and slightly below the field for sulfide-saturated MORB, indicating a drop in the SCSS compared to the MORB array. This drop in S contents at a given FeOTOT coincides with the onset of magnetite fractionation and the sudden increase in the Se/S, Cu/S, and Ag/Cu of erupted melt. The relative change in behavior of S, Se, Cu, and Ag at the onset of magnetite saturation, in particular Ag/Cu, which remains constant during the evolution of MORB melts, indicates a change in the composition of the sulfide phase (previously sulfide liquid) on the liquidus (Figure 7). This apparent drop in the SCSS may in turn be linked to reduction of the melt associated with the removal of magnetite. An increase in Ag/Cu is also observed in samples from the Manus Basin, following magnetite-triggered sulfide saturation, whichJenner et al. attributed to the appearance of a crystalline Cu-rich sulfide phase on the liquidus, such as bornite, as opposed to sulfide liquid. It is conceivable that magnetite saturation coupled with a decrease in temperature during continued differentiation in a crustal magma chamber, results in a change in phase composition on the liquidus of the NWLSC magmas from sulfide liquid, to a more Cu-rich composition. Alternatively, the increased compatibility of Cu relative to Ag at this stage in the fractionation sequence may indicate that Cu is slightly compatible in magnetite. However, the systematic changes in each of the chalcophile element ratios, including S and Se, which are unlikely to partition into magnetite, supports our conclusion that there is a change in the composition of the fractionating sulfide, potentially from a liquid to a crystalline sulfide phase with a stoichiometry capable of fractionating Cu from Ag.
7. Origin of Sulfide-Undersaturated Melts
Jenner and O'Neill [2012a]used Cu versus MgO to demonstrate submarine-quenched samples erupted along known hot spot tracks or close to areas associated with plume-related magmatism have higher Cu contents at a given MgO compared to the typical MORB array (compilation shown onFigure 9). Similarly, our data for Hawaii (Pu'u'O'o eruption of Kilauea), and compiled data from Ko'oalau and Moloka'i Hawaiian volcanoes, Iceland, Kwaimbaita-Type magmas from the Ontong Java Plateau and the Galápagos Islands have high Cu at a given MgO compared to the MORB array, indicating elevated Cu contents is a common characteristic of magmas associated with mantle plumes. The only samples presented inFigure 9that are generated by plume-related magmatism but do not have higher Cu contents compared to the MORB array are the primitive Kroenke-type magmas from the Ontong Java Plateau, and conspicuously, samples from the Samoan islands. The most straightforward explanation for the higher Cu contents at a given MgO of the majority of plume-related samples compared to MORB, is the parental melts, like the NWLSC magmas, were initially S-undersaturated and consequently, evolved to high Cu contents compared to sulfide-saturated MORB. The high Cu contents of the more evolved Kwaimbaita-type basalts indicate the Ontong Java Plateau melts were indeed S-undersaturated during differentiation (considered byFitton and Godard to be linked to the Kroenke-type magmas by fractional crystallization), consistent with conclusions of other studies [Ely and Neal, 2003; Chazey and Neal, 2004]. Hence, some part of the petrogenesis of parental magmas of each of these Cu-rich melts discussed above was likely similar to that of NWLSC samples consequent to parental magmas being S-undersaturated.
 S-undersaturated melts could be generated by high-degrees of partial melting if the sulfide phase in the mantle source region became exhausted. For example, komatiites-komatiitic basalts were S-undersaturated during low-pressure fractional crystallization [Puchtel and Humayun, 2000, 2001]. However, the most primitive samples retrieved from the NWLSC, RR and CLSC all have MgO contents <10 wt.%, indicating these were not high-degree partial melts. Additionally, samples from the NWLSC, RR and CLSC have REE patterns similar to MORB (Figure 4c) and plot within the MORB array with regards to Th/Yb versus Nb/Yb (Figure 5), indicating similar degrees of partial melting. Given the melt-depleted upper mantle sources of MORB are generally considered to contain residual sulfides [Peach et al., 1990], we can infer sulfide was also present in the mantle source region of these northwestern Lau Basin magmas.
 Experimental studies have demonstrated SCSS decreases with increasing pressure [Mavrogenes and O'Neill, 1999]. During adiabatic upwelling of a melt, S-saturated melts generated at high pressures will be S-undersaturated at lower pressures. For example, using the experimental constraints presented inMavrogenes and O'Neill  for basaltic compositions, a melt with a temperature of 1200°C and 10 wt.% FeOTOT, the SCSS at 1.2 GPa is 750 ppm, at 0.9 GPa is 850 ppm, and at 0.3 GPa is 950 ppm. Given the parental magmas of the NWLSC have ∼100–200 ppm less S at a given FeOTOT compared to the MORB array (Figure 8), we suggest the former were generated at pressures at least ∼0.6–0.9 GPa higher than typical MORB, but at pressures lower than garnet stability (∼2.8 GPa [Robinson and Wood, 1998]) to prevent the fractionation of the HREE. Although in detail subtle differences in the composition of the parental melt, such as Cu content, also affects the SCSS [O'Neill and Mavrogenes, 2002; Ripley et al., 2002], these variables do not result in the production of S-undersaturated parental melts.
 Subsequent to partial melting, retention of higher-pressure (S-saturated) lower S contents compared to MORB, requires NWLSC parental magmas to have ascended rapidly, i.e., without equilibrating with surrounding mantle during ascent and maintaining S-saturation, resulting in parental melts that were S-undersaturated during initial stages of low-pressure fractional crystallization. This interpretation is supported by the geographic locations of the high-Cu samples plotted onFigure 9; each of the samples were erupted at locations linked to plume-related magmatism. Hence, we consider the S-undersaturated signatures of samples from the NWLSC and parts of the CLSC and RR, indicates the generation of the parental melts was more comparable to the petrogenesis of plume-related magmas as opposed to MORB, but at pressures less than the garnet stability field.
 Geophysical studies, including bathymetric and seismic constraints coupled with numerical modeling, have attributed the anomalously high topography of a region spanning the North Fiji Basin, North Fijian Plateau and northern Lau Basin to the upwelling of hot, buoyant mantle [Billen and Gurnis, 2003; Zhang and Pysklywec, 2006]. The presence of deep mantle upwelling(s) may account for the geochemical characteristics of the Northwest Lau Basin we have identified herein. An extremely high incidence of hydrothermal activity reported in this part of the Lau Basin [Lupton et al., 2012b], also indicates the area is anomalously hot. Although samples from the NWLSC lack the characteristic high-pressure garnet signature (i.e., high Gd/YbPM) typical of plume-related melts such as Hawaii and Samoa, this may not preclude the magmatism in the NWLSC being linked to a ‘deep’ upwelling of the mantle. For example, the physical upwelling resulting in the production of the NWLSC melts may have been present in the garnet stability field, but derived melts will only record high Gd/YbPM if the solidus was intersected at this depth. It is worth noting the petrogenesis of oceanic plateau basalts, (e.g., Ontong Java) which have Gd/Yb, Th/Yb, and Nb/Yb similar to the NWLSC (Figures 4 and 5), is typically linked to plume-related magmatism, but these samples also lack a garnet control signature [Fitton and Godard, 2004].
 The compilation presented in Figure 9shows a number of Samoan islands samples are S-saturated (i.e., the contents of Cu decrease with decreasing MgO), and plot almost entirely within the MORB array. This interpretation is supported by the occurrence of sulfides in the majority of submarine alkali basaltic glasses from the three youngest Samoan volcanoes, Ta'u, Malumalu and Vailulu'u [Workman et al., 2006]. The cause of the S-saturated characteristics of the magmas sourced by the Samoan plume, which contrasts with the S-undersaturated nature of the majority of plume-derived melts compiled inFigure 9is enigmatic, and beyond the scope of this contribution, but may be linked to their more alkali-rich compositions or magma ascent rates.
8. High Cu Contents in Samples from the Northwest Lau Basin
 The most primitive samples from the NWLSC and a number of samples from the RR and CLSC have the highest Cu contents of all of the samples compiled in Figure 9, implying either: (1) the parental melts were generated by high-degrees of partial melting, producing high-Mg parental melts that evolved to high Cu contents during extensive sulfide-undersaturated differentiation; or (2), the partial melts are anomalously rich in Cu. Th/Yb versus Nb/Yb systematics and the PM- normalized patterns of samples from the CLSC, NWLSC, and RR show no evidence for a subduction-derived input to the mantle source region of the NWLSC samples (Figures 4 and 5). Hence, it is unlikely that the high Cu and Ag contents resulted from subduction-related processes. Additionally, the contents of Cu, Ag, and Se in primitive samples from the Manus Basin plot either within or below the MORB array, despite the trace element evidence for a subduction component to their mantle source region, indicating minimal mobility of these elements compared to elements such as As, Sb, Tl, Bi and Pb.
Fitton and Godard demonstrated the range in major and trace element compositions of primitive Kroenke-type magmas from the Ontong Java Plateau can be generated by olivine-only fractionation. Additionally,Fitton and Godard [2004, Figure 10] used the range in Nb versus MgO contents to demonstrate the more pronounced enrichment of incompatible elements after the appearance of plagioclase and clinopyroxene on the liquidus, and the ability of fractional crystallization to generate the differences in compositions of the primitive Kroenke-type and the more evolved Kwaimbaita-type magmas. Olivine ± chromite are typically the only phases on the liquidus of melts with >8 wt. MgO [e.g.,Langmuir et al., 1992]. The approximately constant Cu contents with decreasing MgO of the Kroenke-type magmas (Figure 9a), demonstrates olivine ± chromite only fractionation is unable to generate the high-Cu contents of the most mafic NWLSC basalts from a picritic, low-Cu parental melt composition. Accordingly, the red line onFigure 9 indicates the likely Cu content of any parental NWLSC magmas at higher MgO contents. Thus we consider the high Cu contents of the NWLSC magmas and a number of samples from the RR and CLSC to be a diagnostic feature of the parental melts.
 In addition to the high Cu and Ag contents of the most primitive NWLSC samples and a number of samples from the CLSC and RR, the initially high Cu/Se, Cu/S, and Ag/S are distinctive. With progressive depletion of the mantle source region, the Cu/S, Cu/Se and Ag/Se of subsequent melts are expected to increase because of the higher compatibility of Cu and Ag in the residual mantle sulfide compared to both S and Se [Hamlyn et al., 1985; Peach et al., 1990; Jenner et al., 2010]. Given NWLSC have LREE compositions that plot within the range of MORB and are not markedly depleted, the Cu/S, Cu/Se and Ag/Se are expected to plot within the MORB array and not substantially above it. Similarly, other plume-related suites, such as the Hawaiian basalts (Figure 7), samples from the Réunion hot spot track and Cocos Ridge also have high Cu/Ag and Ag/Se compared to the MORB array. This behavior contrasts with the predicted chalcophile element behavior of samples from the Manus Basin (Figure 7) and data for boninites [Hamlyn et al., 1985], which are considered to have been derived from extremely depleted mantle source regions [Hamlyn et al., 1985; Kamenetsky et al., 2001; Sinton et al., 2003; Jenner et al., 2010] and in accord with our understanding of chalcophile element systematics, have elevated Cu/Se and Ag/Se compared to less depleted MORB. Hence, the high Cu and Ag contents of samples from the NWLSC and some samples from the CLSC and RR, and the high Cu/S, Cu/Se and Ag/Se appear to be diagnostic features resulting from the petrogenesis of the parental magmas.
Urakawa et al. showed the eutectic in the Fe-Ni-O-S system remains below 900°C to 15 GPa, indicating sulfides are molten throughout the mantle. Consequently, it is difficult to envisage why partitioning behavior would change with depth, or permit the production of variably Cu-rich parental melts. Alternatively, other experimental studies found that two sulfide phases are stable in the upper mantle, a crystalline Fe-S-rich monosulfide and a Cu-Ni enriched sulfide melt [Bockrath et al., 2004; Ballhaus et al., 2006]. These studies concluded that during melt segregation, monosulfide stays in the residual solid residue whereas the Cu-rich sulfide melt is entrained as immiscible droplets in the silicate melt, providing a means to fractionate the chalcophile and siderophile elements from each other during melting, as observed in the Lau Basin samples. Sulfide liquids are not quenchable to glass, even in rapidly quenched experiments, and instead crystallize on cooling to a variably complex phase assemblage depending on their exact composition, making interpretation of their results challenging. The two-phase field of monosulfide plus sulfide melt derived from textural relationships could merely be a quench texture. However, we note models presented byBockrath et al.  and Ballhaus et al.  are able to reproduce the PGE fractionated patterns of silicate melts. Alternatively, Ripley et al.  used sulfide liquid/silicate partition coefficients in experimental runs to demonstrate an increase in Cu solubility in the silicate melt with moderate increases in fO2. Hence, parental melts of the NWLSC basalts may have been slightly more oxidised than MORB, but not oxidized enough to prevent saturation in sulfide during differentiation of the melts at low pressure, and notably with regards to the differentiation of backarc basin magmas, before the Magnetite Crisis. Quantitatively resolving the cause of the initially high Cu contents of the NWLSC magmas and plume-related melts is beyond the scope of this contribution and likely requires further experimental studies regarding the partitioning of chalcophile elements at high pressure.
9. The use of Cu for Tracking the Ingress of the Samoan Plume
 We attribute the S-undersaturated compositions of the most primitive samples from the NWLSC and a number of samples along the RR and CLSC to partial melting at pressures greater than MORB. Previous studies have attributed a range of geochemical proxies in samples from the northern part of the Lau Basin to lateral entrainment of material from the Samoan Plume into and mixing with the local mantle [Lupton and Craig, 1975; Volpe et al., 1988; Poreda and Craig, 1992; Turner and Hawkesworth, 1998; Falloon et al., 2007; Regelous et al., 2008; Lupton et al., 2009; Tian et al., 2011; Hahm et al., 2012; Lupton et al., 2012a]. However, samples from Samoa plot almost exclusively within the MORB array on the plot of Cu versus MgO (Figure 9). Consequently the high Cu and Ag contents of the NWLSC are not easily attributable to ingress of the Samoan plume and in particular, mixing between two low-Cu sources, such as Samoan and MORB. We suggest the RR result from the mixing of two distinct end-member compositions; (1) a high-Cu, relatively high3He/4He (∼20) component beneath the NWLSC generated at pressures higher than MORB; (2) a low-Cu, Samoan plume (3He/4He ∼30) component invading beneath the RR (see mixing line on Figure 9b). Additionally, we note that the offset to higher Ag at a given Cu content of samples from the RR compared to both the NWLSC and CLSC is a feature shared by OIB samples from Hawaii (Figure 8c), indicating the Samoan plume material may share this characteristic. This interpretation is also supported by the subtly higher Gd/Yb, TiO2and lower V of the RR samples compared to those generated at the NWLSC, which is consistent with some extent of mixing with a Samoan-plume component. The ingress of Samoan material into the Northern Lau Basin (red arrow,Figure 1b) is likely facilitated by toroidal flow of the mantle around the northern limit of the Pacific Slab during rapid migration of the trench [Schellart, 2004; Stegman et al., 2006; Schellart et al., 2007].
 The presence of the Pacific Slab beneath the CLSC (∼300 km) possibly prevents the high-Cu signals in the northern parts of this spreading center being derived from a Transition Zone or a lower mantle-derived plume. Additionally, the consistently low3He/4He of ∼8 of both the high-Cu and low-Cu melts from the CLSC indicates mixing between the high3He/4He NWLSC and MORB-like source cannot be invoked to explain the geochemical compositions of the CLSC magmas. The high Cu contents of some of the samples from the CLSC indicates the parental magmas were generated by melting at higher pressures than MORB, lending support for models that have suggested the existence of subduction-triggered plume-like mantle upwellings in backarc basin regions [e.g.,Faccenna et al., 2010]. Similarly, the high Cu contents of samples from the NWLSC, which are comparable in magnitude to those generated in the CLSC, may indicate poloidal flow of material from beneath and around the edges of the flat-lying section of the Pacific Plate (yellow arrow,Figure 1b; the angle of subduction of the Pacific Plate shallows between ∼300–400 km, at a distance of ∼400–600 km from the Tonga Trench [Richards et al., 2011]) may have triggered upwelling of the mantle to produce the NWLSC magmas.
10. High Pb, Tl and As Signatures of the RR Magmas: The Remnant Vitiaz Arc?
 A notable feature of the RR samples are enrichments in Pb, As, and especially Tl on PM-normalized plots, compared to MORB and samples from the NWLSC and the CLSC (Figure 4). These distinctively high Pb, As, and Tl patterns may indicate the Samoan OIB magmas are also enriched in these elements, although to the best of our knowledge, relevant data are currently unavailable to test this hypothesis. However, we note there is no correlation between the magnitude of the Pb, As, and Tl anomalies with other indicators of mixing with the Samoan component, such as Gd/Yb, V, TiO2or the chalcophile elements. The enrichments in Pb, As, and Tl in samples from the RR are comparable to subduction-related samples from the Manus Basin, but the magnitude in the Tl enrichment compared to Pb, As, and Mo indicates differences in their petrogenesis. Additionally, samples from the RR lack other commonly recognized geochemical characteristics of subduction-related magmatism, such as depletions in Nb and Ta relative to La, enrichments in Cs relative to Rb, or elevated Th/Yb at a given Nb/Yb. In addition to Tl anomalies, samples from the RR have negative Y depletions relative to Ho on primitive mantle plots, which are not observed in samples from the NWLSC, the CLSC, the Manus Basin or samples defining the MORB array. Y and Ho are typically regarded as ‘geochemical twins’ and as such, are difficult to fractionate from each other during igneous processes [e.g.,Blundy and Wood, 2003; Pack et al., 2007]. However, hydrothermal alteration of oceanic crust, at temperatures between 100 and 400°C is capable of fractionating Y from Ho, as a result of chemical complexation and differences in electronic configuration between the two elements [Bau, 1996, and references therein]. Noting the basement of the RR may represent disrupted portions of the fossil Vitiaz Arc (Figure 1), we suggest the positive As, Tl and Mo anomalies and negative Y anomalies relative to Ho in the majority of samples from the RR may have resulted from variable assimilation of hydrothermally altered portions of this basement.
 We thank the officers, crew, and co-scientific staff of the SS07/2008 voyage for their professionalism and enthusiasm that ensured the success of the expedition. The post-voyage analytical costs were supported by an Australian Research Council Discovery Grant to RJA and JM. Erik Hauri acknowledges funding from the Deep Carbon Observatory. Rick Carlson provided sagacious advice ré content and balance of an early draft of this paper, and we thank Jianhua Wang for expert maintenance and assistance in the DTM SIMS lab. Jon Blundy and Andreas Audétat are thanked for their constructive and thoughtful reviews and Joel Baker for editorial handling.