Melt–rock interactions in a veined mantle: pyroxenite–peridotite reaction experiments at 2 GPa
- 1Dipartimento di Scienze della Terra, University of Milan, via Botticelli 23, 20133 Milano, Italy
- 2DISTAV, University of Genova, 16132 Genova, Italy
Correspondence: Giulio Borghini (firstname.lastname@example.org)
Interaction between peridotite and pyroxenite-derived melts can significantly modify the mineralogy and chemistry of the upper mantle, enhancing its heterogeneity, by creating re-fertilized peridotites and secondary-type pyroxenites. We experimentally investigated the reaction between a fertile lherzolite and MgO-rich basaltic andesite produced by partial melting of an olivine-free pyroxenite at 2 GPa and 1300–1450 ∘C. The aim was to constrain the rate and style of melt–peridotite reaction mostly as a function of temperature, i.e. assuming variable physical status of the host peridotite. Experiments juxtaposed pyroxenite on a synthesized fertile lherzolite to evaluate the modal and mineral compositional changes in the fertile lherzolite resulting from the reaction with pyroxenite-derived melt. At 1300 and 1350 ∘C, the reaction produces a thin orthopyroxene-rich reaction zone confined between partially molten pyroxenite and modally unmodified subsolidus lherzolite. Chemical changes in minerals of the pyroxenite crystal mush suggest that element diffusion across the pyroxenite–peridotite interface, coupled with orthopyroxene precipitation, plays a role in the reactive crystallization of mantle pyroxenite veins. At 1380 and 1400 ∘C, infiltration of pyroxenite-derived melt significantly modifies the mineralogy and chemistry of the host peridotite by creating orthopyroxene-rich websterites and pyroxene-rich lherzolite. At 1450 ∘C, pyroxenitic melt fluxes into molten peridotite, enhancing peridotite melting and creating a melt-bearing dunite associated with a refractory harzburgite. At a given pressure, bulk compositions of hybrid rocks originating through melt–peridotite interaction are mostly controlled by the chemistry of the reacting melt. Interaction between pyroxenitic melt and peridotite causes and decrease and TiO2 increase in pyroxenes and spinel across the pyroxenite–peridotite boundary. Similar chemical gradients in minerals are observed in pyroxenite–peridotite associations from natural mantle sequences. The comparison with mineral chemistry variations derived by reaction experiments potentially represents a petrologic tool to discriminate between low- versus high-temperature melt–peridotite reactions.
Melt–peridotite reactions play an important role in the mineralogical and chemical modification of the upper mantle within a considerable range of depth (e.g. Rampone et al., 2020, and reference therein). Interaction between peridotites and pyroxenite-derived melts at the lithosphere–asthenosphere boundary is thought to enhance mantle heterogeneity creating hybrid rocks, such as re-fertilized peridotites and secondary-type pyroxenites (e.g. Lambart et al., 2013). Several lines of evidence have suggested that mafic or pyroxenitic heterogeneities are preserved in the deep mantle, likely resulting from the recycling of crustal material (e.g. Allègre and Turcotte, 1986; Phipps Morgan and Morgan, 1999). During the adiabatic (or near-adiabatic) upwelling of a heterogeneous mantle, such low-solidus lithologies encounter partial melting at significantly higher pressure than the host peridotite and experience a much higher degree of melting (e.g. Hirschmann and Stolper, 1996; Phipps Morgan, 2001; Kogiso et al., 2004a, b). Partial melts produced by pyroxenitic lithologies, significantly different from peridotite-derived liquids, are much more reactive with the surrounding peridotite (e.g. Yaxley and Green, 1998; Spandler et al., 2008; Rosenthal et al., 2014). A large variety of melt–peridotite reactions modify significantly the peridotite by forming a wide range of reaction products as a function of pressure (P), temperature (T) and melt composition (e.g. Herzberg, 2011; Rosenthal et al., 2018). Recent models have proposed that veined mantle resulting from melt–peridotite reactions represents the source of most oceanic basalts (e.g. Donnelly et al., 2004; Sobolev et al., 2007; Lambart et al., 2012; Mallik and Dasgupta, 2012).
Several experimental works have been recently dedicated to melt–peridotite reactions in upwelling mantle (Yaxley and Green, 1998; Lambart et al., 2012; Mallik and Dasgupta, 2012, 2013), as well as in subduction zone environments (Rapp et al., 1999; Mitchel and Grove, 2016; Wang et al., 2016; Gervasoni et al., 2017; Corgne et al., 2018) or in cratonic lithospheric mantle (Sen and Dunn, 1994; Rapp et al., 2010; Wang et al., 2010; Yu et al., 2014; Wang et al., 2013, 2016, 2020). In addition, basalt–peridotite reaction experiments at pressure P≤1 GPa provide evidence of the role of dissolution/reprecipitation processes in melt transport and the mineralogical/chemical modification of the lithospheric mantle (Daines and Kohlstedt, 1994; Morgan and Liang, 2003, 2005; Van Den Bleeken et al., 2010, 2011; Tursack and Liang, 2012; Saper and Liang, 2014; Borghini et al., 2018).
In order to simulate melt–peridotite reactions, various experimental strategies have been followed, mostly differing in terms of composition of starting materials and geometrical set-up (e.g. Yaxley and Green, 1998; Lo Cascio et al., 2004; Tursack and Liang, 2012; Saper and Liang, 2014). Overall, the nature of the reaction products is mostly controlled by the composition of reacting melt, pressure and, to a minor extent, the mineralogy of the infiltrated peridotite. On the other hand, temperature plays a key role in controlling not only elements' diffusion across the interface between the two reactants but also the physical status of peridotite (solid versus partially molten) that defines its porosity and, in turn, the amount of melt infiltration (Lambart et al., 2012; Wang et al., 2020), i.e. the melt rock ratio.
In terms of experimental set-up, melt–peridotite reaction processes have been investigated by adopting two different set-ups, i.e. mixed and layered experiments. Running homogeneous mixtures of glass and minerals (mixed experiments) simulates the complete infiltration of the peridotite, thus assuming reactive porous flow within a very high-porosity mantle. On the other hand, in layered experiments the melt–peridotite reactions mostly occur along the boundary between the reactants, simulating the interaction at the wall rock of melt-rich veins (channelized flow).
Although in layered experiments the interaction between melt and peridotite is limited and confined to the reactants' interface, they represent the more realistic simulation of pyroxenite–peridotite exchange in a veined mantle domain. Examples of such heterogeneous pyroxenite-bearing mantle were documented in many orogenic and ophiolitic ultramafic massifs (Bodinier and Godard, 2014, and references therein), as well as in mantle xenoliths (e.g. Lu et al., 2018). Most of these studies have reported significant chemical and modal changes in peridotites caused by interaction with pyroxenite-derived melts (e.g. Bodinier et al., 1990, 2004; Pearson et al., 1993; Zanetti et al., 1996; Mukasa and Shervais, 1999; Borghini et al., 2020). On the other hand, the origin itself of several pyroxenites has been ascribed to the replacement of peridotite by interaction with melts at deep lithospheric mantle levels (e.g. Garrido and Bodinier, 1999; Marchesi et al., 2013; Borghini et al., 2016; Tilhac et al., 2016).
In spite of an increasing number of experimental works focused on melt–peridotite reaction, the mineralogical and chemical changes in peridotites due to interaction with pyroxenite-derived melt are still poorly known. In particular, experimental constraints are needed to shed light on the mutual effects of this interaction and to discriminate the role of melt–peridotite reactions in the origin of pyroxenites from natural settings.
In this study, we present the results of reaction experiments, at 2 GPa and 1300–1450 ∘C, between lherzolite and partial melts derived from an olivine-free websterite. The major goal of this work is to investigate how the melt–rock reactions modify a pyroxenite–peridotite association as a function of temperature. We simulate the different extent of pyroxenite partial melting, thus varying the composition of reacting melt, and the variable physical status of the host peridotite as this is expected to control the rate and style of melt–peridotite reaction (Lambart et al., 2012; Wang et al., 2020). At the same time, coupling a partially molten pyroxenite to peridotite provides insights on the evolution of pyroxene-rich crystal mush within the upper mantle, which has relevant implications for the reactive crystallization of pyroxenites in the lithospheric mantle.
2.1 Starting materials
We performed eight pyroxenite–peridotite reaction experiments by juxtaposing olivine-free pyroxenite powder (Px1; Sobolev et al., 2005, 2007) to a layer of fertile lherzolite (Fig. 1a). Bulk compositions of starting materials are reported in Table 1.
The starting peridotite is a fertile lherzolite (FLZ; studied by Borghini et al. 2010) (Table 1), prepared in the anhydrous complex system TiO2-Cr2O3-Na2O-CaO-FeO-MgO-Al2O3-SiO2 (Ti,Cr-NCFMAS) from a gel (Table 2). We performed a first set of exploratory experiments in order to investigate the texture and mineral chemistry of FLZ at 2 GPa and 1300, 1350, 1380, 1400 and 1450 ∘C. Then, we repeated the same runs in order to prepare the synthesized FLZ to be used as the starting lherzolite layer in the reaction experiments at the same pressure and temperature. After the second set of experiments, the synthesized FLZ was carefully extracted from the capsule and grounded in a mortar to obtain a fine powder to be loaded in the capsule together with Px1. This procedure allowed a better estimate (by direct comparison) of the modal and mineral compositions in the peridotite modified after reaction with pyroxenite-derived melt.
t (h) is run duration in hours. a Starting material proportions. b Modal proportions in the reaction zone (RZ) and partially molten pyroxenite layer estimated by image analysis. c It includes the amount of quenched clinopyroxene. Modal abundances in FLZ runs were computed by weighted least squares mass balance calculations; in parentheses modal fraction and error calculated by Monte Carlo simulation are shown. R2 is the sum of the squares of residuals: ol, olivine; opx, orthopyroxene; cpx, clinopyroxene; sp, spinels; gl, glass.
Px1 is an olivine-free pyroxenite modelled by Sobolev et al. (2005, 2007) through the reaction between high-Si eclogite-derived melt and peridotite until the complete consumption of olivine. Px1 is a synthetic starting material prepared by blending high purity oxides and carbonates at the Australian National University, which was kindly provided by Gregory M. Yaxley. Px1 has relatively high XMg (XMg = molar = 0.81) coupled with high SiO2, moderate Al2O3 and low CaO contents (Table 1). Melting-phase relations and partial-melt compositions for pyroxenite Px1 at 2 GPa have been investigated in a separated paper by Borghini and Fumagalli (2020). At 2 GPa, Px1 is an olivine-free garnet websterite, and its solidus is located between 1250 and 1280 ∘C. At increasing melting degree, the sequence of mineral-phase disappearance is garnet, clinopyroxene and orthopyroxene, this latter completely consumed at 1480 ∘C. At 2 GPa and investigated temperatures (T = 1300–1450 ∘C), pyroxenite Px1 is above its solidus (Borghini and Fumagalli, 2020), thus representing the source of melt in these reaction experiments. In the range 1300–1450 ∘C, Px1 produces MgO-rich basaltic andesites (Fig. 2), matching the composition of eclogitic melts in terms of silica and alkali contents but with significantly higher XMg values. These melts differ from those produced by lherzolite melting at 2 GPa, having higher SiO2 and lower CaO contents. Moreover, due to their relatively high silica activities, Px1 melts are expected to react with the associated peridotite (Borghini and Fumagalli, 2020).
2.2 Experimental and analytical techniques
Experiments were carried out at 2 GPa and temperatures from 1300 to 1450 ∘C (Table 2) in an end-loaded piston cylinder at the Laboratorio di Petrologia Sperimentale, Dipartimento di Scienze della Terra “Ardito Desio”, University of Milano (Italy), using a 0.5 in. talc–pyrex–MgO assembly. Pressure correction for friction of 10 % was experimentally calibrated using the quartz–coesite transition (Bohlen and Boettcher, 1982). FLZ syntheses lasted from 46 to 175 h, and reaction couple experiments were run for 24 h (Table 2). We applied the graphite-lined platinum capsule technique (Ulmer and Luth, 1991) to minimize Fe loss toward the noble metal capsule. Layers of pyroxenite Px1 and lherzolite FLZ were loaded into a graphite container (2.7 mm o.d., 2 mm i.d.), placed in a welded Pt capsule (3 mm o.d.) (Fig. 1a). The weight proportions between pyroxenite and lherzolite are reported in Table 2. The graphite–Pt assembly keeps the oxygen fugacity below the graphite–C–O vapour buffer (e.g. Ulmer and Luth 1991; Médard et al., 2008).
In order to maintain anhydrous conditions, the platinum-graphite capsule loaded with the starting material was dried overnight in an oven at 250 ∘C before being rapidly welded shut. The thermocouple tip was separated from the platinum capsule by a 0.5 mm thick hard corundum disc. Assemblies were kept in oven at about 200 ∘C for several hours before running the experiments. Temperature was measured by S-type thermocouples and is considered to be accurate to ±5 ∘C. An initial pressure of 0.25 GPa was applied, then the sample was first heated to 400 ∘C for 10 min in order to soften the Pyrex, and pressure was raised to the experimental value before reaching the desired temperature. The centre of the sample was located in the hotspot of the assembly that was about 2 mm far from the thermocouple; according to Watson et al. (2002), this set-up is expected to introduce a maximum temperature gradient of less than 10 ∘C. We terminated the runs by turning off the power. Capsules were enclosed in epoxy, sectioned lengthwise, polished and carbon-coated.
We investigated the run products by performing back-scattered electron (BSE) images and microanalyses using a JEOL JXA-8200 SuperProbe equipped with five wavelength-dispersive spectrometers (WDSs) and one energy dispersive spectrometer (EDS) at the Dipartimento di Scienze della Terra “Ardito Desio”, University of Milan. BSE images and X-ray element maps represented useful tools in textural examination of the experimental charges. Analyses on mineral phases were performed using 1 µm beam size and beam conditions of 15 kV and 5 nA. Counting time was 30 s for peak and 10 s for background.
3.1 Phase assemblages and textures
3.1.1 Run products in FLZ lherzolite syntheses
At 1300 and 1350 ∘C (P=2 GPa) FLZ starting material produced a four-phase subsolidus lherzolite made of olivine, orthopyroxene, clinopyroxene and spinel. The mineral chemistry in FLZ experiments is reported in Tables S1–S4 in the Supplement. Run products show well-developed polygonal mineral aggregates (Fig. 1b) in which olivine forms rounded crystals up to 10 µm in size, pyroxenes are up to 30 µm in length, and spinel is present as small rounded bright crystals up to 5 µm in diameter. The occurrence of several triple points involving both olivine and pyroxenes suggests a well-equilibrated texture (Fig. 1b). Weighted least squares mass balance calculation by a weighted least squares method provided phase abundances typical of mantle lherzolite with clinopyroxene and orthopyroxene ranging 15 wt %, 17 wt % and 22 wt %–25 wt %, respectively, and spinel around 2 wt % (Table 2). Error propagation has been performed by Monte Carlo simulation. Very low residual sums of squares (R2<0.6) strongly support the attainment of equilibrium in subsolidus experiments at 1300–1350 ∘C.
At 1380–1400 ∘C the appearance of interstitial glass among mineral phases (Fig. 1c) indicates that the lherzolite is above its solidus at incipient partial melting. In these runs, the grain size of olivine and pyroxenes increases up to 50–60 µm (Fig. 1c). At 1450 ∘C, quenched glass is accumulated at the rim of the capsule (Fig. 1d); coarse olivine and orthopyroxene are associated with an interstitial matrix made of glass and fine-grained quenched clinopyroxene (Fig. 1d). In this run, both textural observations and mineral chemistry of clinopyroxene indicate that it formed by quenching of melt and cannot be considered a stable residual mineral. In order to avoid the inclusion of a large amount of disequilibrated quenched material in the capsule, in the reaction experiment at 1450 ∘C we coupled the pyroxenite Px1 to the FLZ synthesized at 1400 ∘C.
3.1.2 Run products in pyroxenite–peridotite reaction experiments
At 1300 and 1350 ∘C (P=2 GPa) reaction experiments were run for 24 h. Both runs show similar textures, well evidenced in BSE images and X-ray elemental maps (Figs. 3 and 4). A thin orthopyroxene-rich reaction zone bounds the layers consisting of partially molten pyroxenite and subsolidus lherzolite at the top and bottom of the capsule, respectively. The opx-rich (orthopyroxene) reaction zone has a thickness ranging from 50 to 100 µm at 1300 ∘C (Fig. 3a, b) and from 100 to 150 µm at 1350 ∘C (Fig. 3c, d). Lherzolite layers after reaction contain olivine, pyroxenes and tiny spinels of <5 µm in size and show textural features similar to those observed in the analogous experiment on FLZ (Fig. 1b). The pyroxenite layer consists of clinopyroxene, orthopyroxene and interstitial glass (Fig. 3b, d). Remarkably, garnet is absent among the residual phases, although it was observed as residual phase in the partial melting experiment on Px1 at 1300 ∘C and 2 GPa (Borghini and Fumagalli, 2020).
At 1380 and 1400 ∘C, pyroxenite–lherzolite interaction generates a thicker reaction zone, ranging from 650 to 950 µm, made of orthopyroxene, clinopyroxene, minor olivine and interstitial glass (Fig. 5a). Thin interstitial glass is associated with well-crystallized clinopyroxene and mostly occurs in the upper part of the websteritic reaction zone at the contact with the partially molten pyroxenite (Fig. 5c). The modal proportion of olivine tends to increase toward the bottom of the capsule up to the contact with the lherzolite layer. Differently from experiments on FLZ showing very low melt fractions (Table 2, Fig. 1c), in reaction experiments at 1380–1400 ∘C the lherzolite layer does not contain glass and displays slightly higher clinopyroxene modal abundances compared to unreacted FLZ (Fig. 5d). The molten pyroxenite layer contains orthopyroxene, clinopyroxene and melt at 1380 ∘C and orthopyroxene and melt at 1400 ∘C (Fig. 5b). In reaction experiment at 1400 ∘C, clinopyroxene occurs only in quenched textures (Fig. 5b), therefore not being a residual phase, whereas it is still stable in the analogous partial melting experiment (Borghini and Fumagalli, 2020).
At 1450 ∘C, pyroxenite is completely molten, and a large portion of glass plus quenched minerals is still preserved at the top of the capsule (Fig. 5e, f). Most of pyroxenitic melt is fluxed into partially molten peridotite, creating a glass-bearing dunite with interstitial glass amount decreasing downwards (Fig. 5e). Glass-bearing dunite almost covers the whole charge in its central portion (Fig. 5e). The remnant of original lherzolite is represented by a thin (<400 µm) layer of glass-free harzburgite at the bottom of the charge (Fig. 5e).
3.2 Mineral chemistry of interaction products
The phase compositions in experiments on FLZ and reaction runs are reported in Tables S1–S4 and S5–S8, respectively. The predominant textural occurrence of melt in very thin interstitial patches did not allow us to collect reliable compositions except for the reaction experiment at 1450 ∘C in which glass has been analysed in the large pool at the top of the capsule (Table S9). In all experiments, we observed distinct mineral chemistry variations as a function of distance (d) along the capsule. We distinguished three zones: (i) molten pyroxenite at the top of the capsule, (ii) reaction zone, identified as the first appearance of an orthopyroxene-rich layer whose width is dependent on experimental temperature, and (iii) the peridotite layer at the bottom. Mineral chemistry profiles are plotted against distance (Figs. 6–8), taking as reference (d=0 µm) the interface between the partially molten pyroxenite and the orthopyroxene-rich reaction zone. Major element analyses of pyroxenes (Figs. 6, 7) were performed in core grains having variable size (>5 µm). We did not observe any significant core-to-rim chemical zoning in pyroxenes of both low- and high-T experiments (Fig. S1 in the Supplement). In Figs. 6–8, mineral compositions in reaction experiments are compared with those documented in equilibrium FLZ experiments (dashed coloured bars at the bottom; data in Tables S1–S4) and in equilibrium partial melting experiments on pyroxenite Px1 (coloured bars on top of the diagrams, data from Borghini and Fumagalli, 2020).
Figure 6 displays the variations in XMg, , Ca and Ti (a.p.f.u.: atoms per formula weight) in orthopyroxene along the capsule. Profiles also report the compositions of orthopyroxenes from the harzburgite layer in the run at 1450 ∘C (PPR8), at which temperature pyroxenite is completely molten, and the interaction produced a melt–harzburgite–dunite layering. Overall, from molten pyroxenite towards the reaction zone and peridotite, XMg and XCr of orthopyroxenes increase, and Ti contents decrease (Fig. 6). At fixed run duration, temperature has the effect of reducing the gap observed for XMg in orthopyroxene between pyroxenite and peridotite: at 1300 ∘C, XMg varies from 0.86 in the pyroxenite to 0.91 in the peridotite, whereas it ranges from 0.89 to 0.92 at 1400 ∘C (Fig. 6). XCr in orthopyroxene increases from 0.021 in molten pyroxenite to 0.072 in the peridotite layer at 1300 ∘C and varies towards higher values (XCr = 0.037–0.112) at 1400 ∘C (Fig. 6). Remarkably, in reaction experiments at 1380 and 1400 ∘C, orthopyroxenes in the peridotite layer show an average XMg and XCr lower than equilibrium orthopyroxenes in FLZ runs at the same P–T conditions (dashed lines at the bottom in Fig. 6). In these experiments, higher XMg (0.91 and 0.92 at 1380 and 1400 ∘C, respectively) and XCr (0.12 and 0.14 at 1380 and 1400 ∘C, respectively) in orthopyroxene are explained by incipient melting of FLZ. On the other hand, at the same temperatures (1380 and 1400 ∘C) XMg and XCr of orthopyroxenes in molten pyroxenite are, on average, slightly higher than those of orthopyroxene in partial melting experiments on Px1 (Fig. 6). The highest XMg and XCr values have been found in orthopyroxenes from the harzburgite layer in reaction experiment at 1450 ∘C (Fig. 6).
At 1300–1350 ∘C, orthopyroxenes exhibit very low Ti content in the peridotite layers (<0.001 a.p.f.u.), as observed in the subsolidus experiments on FLZ at the same P–T conditions. Ti abundance in orthopyroxenes abruptly increases across the reaction zone showing values between 0.006 and 0.008 a.p.f.u., in agreement with values of the residual orthopyroxenes in Px1 melting experiments (Borghini and Fumagalli, 2020). At 1380–1400 ∘C, orthopyroxenes in the peridotite layer of reaction experiments have systematically higher Ti content with respect to orthopyroxene stable in FLZ in subsolidus experiments, whereas orthopyroxenes in the molten pyroxenite layers show lower Ti contents compared to residual orthopyroxene in Px1 melting experiments (Fig. 6). Low Ti contents are found in orthopyroxenes from harzburgite at 1450 ∘C (0.001–0.002 a.p.f.u.).
Ca content does not vary linearly along the capsule, and data are scattered along the chemical profiles, except for the run at 1400 ∘C in which the Ca content of orthopyroxenes in the molten pyroxenite layer is systematically higher (up to 0.090 a.p.f.u.) than in melting experiments at the same conditions ( a.p.f.u.) (Fig. 6). A large variation in Ca content, from 0.072 to 0.085 a.p.f.u., is found in orthopyroxene from harzburgite at 1450 ∘C (Fig. 6).
Similar to what is observed for orthopyroxene, clinopyroxenes along the capsule in reaction experiments show significant increase in the XMg and XCr and detectable decrease in Ti content from pyroxenite to peridotite (Fig. 7). At 1300 and 1350 ∘C, XMg follows a cotangent diffusion curve varying from 0.85 in the molten pyroxenite to 0.90 in the peridotite. While the XMg values of clinopyroxene in the peridotite layers reflect those in FLZ subsolidus experiments, in the molten pyroxenite layers they are higher than those in melting experiments (Fig. 7, data from Borghini and Fumagalli, 2020). At 1380 ∘C, XMg varies rather linearly from about 0.86 in pyroxenite to 0.91 in peridotite, suggesting that diffusion reaches the end of the charge. Clinopyroxenes in the peridotite layer after the reaction at 1380–1400 ∘C show slightly lower XMg values with respect to those in FLZ experiments (Fig. 7).
XCr values of clinopyroxene increase from 0.020 in molten pyroxenite to 0.073 in the peridotite layer at 1300 ∘C and vary towards higher values (similar to those in FLZ experiments) in the peridotite layers at 1350 and 1380 ∘C (0.096 and 0.110, respectively) (Fig. 7). At 1400 ∘C, XCr values of clinopyroxene in the peridotite layer are slightly lower (0.071–0.109) than those of clinopyroxene in the FLZ experiments (0.121±0.002) (Fig. 7).
At 1300 and 1350 ∘C, Ti contents of clinopyroxene in the peridotite layers are quite low (<0.002 a.p.f.u.), similar to clinopyroxene in FLZ experiments (<0.001 a.p.f.u.), whereas significantly higher Ti contents are observed in clinopyroxene of the peridotite layers at 1380 and 1400 ∘C (up to 0.005 and 0.006, respectively) (Fig. 7). Ti abundances of clinopyroxene in molten pyroxenite layers are systematically lower than those documented in Px1 melting experiments at all investigated temperatures (Fig. 7).
In reaction experiments at 1300 and 1380 ∘C, the Na contents of clinopyroxene decrease from the molten pyroxenite to the peridotite layer, whereas they are rather homogeneous along the profile in the reaction experiment at 1350 ∘C (Fig. 7). Remarkably, clinopyroxenes in molten pyroxenite show lower Na content than clinopyroxenes in Px1 melting experiments at 1300–1350 ∘C, whereas the opposite is observed at 1380 ∘C. Moreover, in the reaction experiment at 1380 ∘C clinopyroxenes in the peridotite layer have higher Na content than in the equilibrium FLZ run at the same conditions (Fig. 7). Na in clinopyroxene at 1400 ∘C is low as in FLZ experiments. The Ca content is low in clinopyroxenes from molten pyroxenite, and it increases with temperature (0.277–0.416 a.p.f.u. at 1300–1350 ∘C; 0.459–0.553 a.p.f.u. at 1380 ∘C), in agreement with the composition of clinopyroxenes in Px1 partial melting experiments (Borghini and Fumagalli, 2020). Higher Ca contents (0.508–0.669 a.p.f.u.) are found in clinopyroxene from the peridotite layer after reaction runs; they are comparable to Ca contents of clinopyroxene from FLZ experiments (Table S2).
In reaction experiments, spinels were only found in the peridotite layer. Their chemical features are shown in Fig. 8, compared to the compositional ranges of spinels in equilibrium FLZ experiments. In the reaction runs, the XMg of spinels increases from the bottom of the capsule towards the top of the peridotite layer, up to the reaction zone boundary. In reaction experiments, spinels show larger variations in XMg relative to what was observed in corresponding FLZ experiments. Furthermore, at 1300, 1350 and 1400 ∘C spinels have higher XMg, whereas they show lower values at 1380 ∘C (Fig. 8).
The XCr values of spinel in reaction experiments at 1300–1380 ∘C show an opposite behaviour with respect to XMg. XCr is highest at the bottom of the capsule, overlapping those documented in spinels from FLZ runs, and progressively decreases towards the reaction zone boundary (Fig. 8). Spinels analysed adjacent to the reaction zones display significantly lower XCr values with respect to those in the corresponding FLZ experiments (Fig. 8). Spinels in reaction experiment at 1400 ∘C exhibit lower XCr values (XCr = 0.133–0.166) than those in the corresponding FLZ run (XCr = 0.193±0.006) but differently from what was observed in lower temperature reaction runs; no correlation with distance is observed (Fig. 8).
Ti contents in spinels of reaction runs at 1300–1350 ∘C are low in the internal part of the peridotite layers (<0.001 a.p.f.u.), with values similar to those in FLZ runs, and drastically increase approaching the reaction zones (Fig. 8). The largest variation is shown in the experiment at 1300 ∘C (Fig. 8). In 1380–1400 ∘C experiments, Ti contents of spinel in the peridotite layers are systematically higher than those in FLZ runs (Fig. 8). Spinels in FLZ experiments have average ratio slightly increasing with temperature from 0.13 at 1300 ∘C to 0.21 at 1400 ∘C (Fe3+ and Fe2+ derived from stoichiometric recalculation). More variable ratios are found in spinels from reaction experiments, with values spanning from 0 to 0.44, without any correlation with temperature or distance within single experimental charges.
Figure 9 exhibits the XMg values and Ca contents of olivine in the reaction runs (compared to olivine composition in FLZ experiments) as a function of temperature. In all runs XMg increases with temperature. In the reaction experiments olivine shows rather homogeneous compositions within the peridotite layer and no correlation with distance from the reaction zone; XMg varies from 0.90 at 1300 ∘C to 0.94 at 1450 ∘C. As compared with FLZ runs at the same conditions, olivine in the peridotite layer at 1350–1400 ∘C has slightly lower XMg values (Fig. 9).
Ca is positively correlated with temperature in both reaction and FLZ experiments (Fig. 9), in agreement with previous melt-bearing experiments (e.g. Libourel, 1999; Borghini et al., 2017, 2018). Ca content is only slightly higher in the reaction experiments as compared with FLZ runs; it varies from about 0.005 a.p.f.u. at 1300 ∘C to 0.009 a.p.f.u. at 1450 ∘C (Fig. 9).
4.1 Pyroxenite–peridotite interactions at low temperature (1300–1350 ∘C)
At 1300–1350 ∘C (2 GPa), FLZ is at subsolidus condition (Fig. 1b, Table 2). At the same P–T values, pyroxenite is partially molten and produces liquids that are basaltic andesites with XMg ranging from 0.61 (1300 ∘C) to 0.67 (1350 ∘C) and high silica activities (0.51–0.52; Borghini and Fumagalli, 2020). Interaction between pyroxenite-derived melts and peridotite mostly forms orthopyroxenite at the lherzolite–molten-pyroxenite boundary, according to the following reaction:
The same reaction has been documented in previous experimental studies investigating the interaction between peridotite and eclogite-derived or andesitic melts within a range of pressure (P = 1–4 GPa). Orthopyroxene is the main reaction product in the pioneer experimental work of Yaxley and Green (1998), who investigated melt–peridotite interaction by layered eclogite–peridotite experiments and obtained thin orthopyroxenite bands separating garnet lherzolite and garnet clinopyroxenite at 3.5 GPa. Orthopyroxene plus garnet (± clinopyroxene) resulted from reactions between peridotite and slab-derived melts at 3.8 GPa (Rapp et al., 1999) and eclogite-derived melts at 2.5–3 GPa (Mallik and Dasgupta, 2012). Wang et al. (2016) documented the development of the orthopyroxenite layers in reaction experiments coupling peridotite and hydrous basaltic melts at 2 GPa. In these experiments, the liquidus-phase relation drives the formation of orthopyroxenite because orthopyroxene is on the liquidus of the reacting melts, and it crystallizes at the expense of olivine at the melt–rock interface. Noteworthy, Wang et al. (2016) found that orthopyroxenite formation is further enhanced by hydrous melting of the adjacent lherzolite, via water infiltration from the reacting melt. Mixing of peridotite-derived melt with hydrous reactive basalt increases orthopyroxene oversaturation of hybrid melt, promoting the orthopyroxene precipitation at the melt–rock interface. Orthopyroxene-rich lithologies have been also observed at the melt–peridotite contact in dissolution experiments at 2 GPa, mostly using the same starting compositions (Wang et al., 2013).
At 1300 and 1350 ∘C the mineral mode within the lherzolite layer is unmodified, and the orthopyroxene-rich reaction zone mostly grows at the expense of the molten pyroxenite (Fig. 3). This is clearly evidenced by X-ray mapping (Fig. 4), which shows the development of orthopyroxene starting from the lherzolite towards the molten pyroxenite. This is in agreement with the experimental results of Wang et al. (2020) showing that at 1300–1350 ∘C, peridotite dissolution in the reacting melt is limited, and the reaction mostly induces modifications in the pyroxenite crystal mush. They observed garnet and clinopyroxene precipitation at the interface with subsolidus peridotite according to the liquidus-phase relationships of reacting melts in their experiments. There are two major differences between our reaction experiments and those of Wang et al. (2020). First, we used a powder-to-powder set-up, whereas a synthesized rod-to-rod set-up was used in Wang et al. (2020). A powder-to-powder set-up could have enhanced melt infiltration at the beginning of the reaction, producing a hybrid boundary layer made by pyroxenite + peridotite powder. Second, we used a partially molten pyroxenite as the reacting melt source instead of a glass rod (Wang et al., 2020); therefore, pyroxenite crystal mush, rather than a totally molten layer, could have limited melt infiltration and reaction with the adjacent peridotite.
The predominant crystallization of orthopyroxene along the peridotite in our 1300–1350 ∘C runs suggests that orthopyroxene is the liquidus phase of MgO-rich reacting basaltic andesites (Table 1). As discussed by Lambart et al. (2012), olivine dissolution and orthopyroxene precipitation reflect high silica activity () of the reacting melt. The crystallization of the orthopyroxene-rich layer at the contact with the lherzolite wall rock modifies the composition of pyroxenite-crystallizing melt toward lower Si, Fe and Mg and higher Ca contents. This could explain the lack of residual garnet in the molten pyroxenite at 1300 ∘C, which instead is observed in the Px1 partial melting experiments (Borghini and Fumagalli, 2020). Fe decrease in crystallizing melt could indeed inhibit garnet crystallization (see Borghini and Fumagalli, 2018). At the same time, the lower Si and higher Ca of melt favour the crystallization of clinopyroxene in the inner part of molten pyroxenite. In the reaction experiments at 1300 and 1350 ∘C the cpx opx (clinopyroxene and orthopyroxene) modal ratios are 2.29 and 1.86 (Fig. S2), respectively, i.e. significantly higher than the cpx opx ratios in the Px1 partial melting experiments at the same P–T conditions (1.11 and 0.96; see Borghini and Fumagalli, 2020).
The reactive crystallization of pyroxenite at the peridotite interface is illustrated in Fig. 10a. Notably, in this model the crystallization of pyroxenite in its inner side is assisted by interaction with the peridotite, and after some extent of crystallization residual melts can flux away or be extracted by compaction. In this way, the final result of reactive crystallization is the mineralogical “layering” made by the clinopyroxene-rich domain at the centre and orthopyroxene-rich bands along the contact with the host peridotite (Fig. 10a). Similar mineralogical zoning was widely described in pyroxenite dikes and layered mantle sequences from ultramafic massifs (e.g. Pearson et al., 1993; Takazawa et al., 1999; Fabries et al., 2001; Mazzucchelli et al., 2010; Borghini et al., 2016). In the Beni Bousera ultramafic massif, Pearson et al. (1993) described rather sharp contact between pyroxenite and peridotite and showed that the first 10 cm of thick pyroxenite layers were chemically modified by interaction with host peridotite through a combined process of melt–rock reaction and diffuse equilibration, similar to what we observed in chemical profiles along reaction experiments.
Residual pyroxenes (mostly cpx) in the crystal mush after reaction have XMg values higher than those in residual pyroxenite after Px1 partial melting experiments (Figs. 6 and 7). This feature cannot be explained only by the crystallization of the opx-rich reaction zone; rather, it suggests the role of element diffusion during the reaction from the lherzolite towards the molten pyroxenite. Experiments of orthopyroxene reaction rims grown at the olivine–quartz interface suggest that element diffusion is efficient during the SiO2 metasomatism of the mantle, in particular for the Fe–Mg redistribution across the orthopyroxene rim (Milke et al., 2011). In addition, the higher diffusion rate of the interstitial melt in the molten pyroxenite likely enhanced the element diffusion within the pyroxenite matrix (e.g. Liang, 2000).
The XMg profiles in pyroxenes and spinel across the reaction interface in the experimental charges (Figs. 6, 7, 8) resemble the chemical gradients across natural pyroxenite layers as documented in Balmuccia (Mukasa and Shervais, 1999), Lherz (Fabries et al., 2001) and External Liguride (Borghini et al., 2016). In mantle sequences, pyroxenite–peridotite chemical exchange is also indicated by the inverse relationship between dyke thickness and bulk-rock Mg number (e.g. Bodinier et al., 1987a, b, 2008; Fabries et al., 2001). The reactive crystallization of high-XMg pyroxenes in the pyroxenite layer observed in our experiments reinforces the idea that many mantle pyroxenites do not reflect the chemistry of parental melts; rather, they represent the result of interaction with the host peridotite. In our experiments at 1300–1350 ∘C, the mineralogy of the peridotite layer is unmodified and the chemical changes in the mineral phases are modest and confined to the pyroxenite–peridotite interface. On the other hand, the growth of the opx-rich reaction layer may constitute a low permeability barrier that potentially hinders melt extraction from the molten pyroxenite vein (Yaxley and Green, 1998; Kogiso et al., 2004b).
4.2 Pyroxenite–peridotite interactions at high temperature (1380–1450 ∘C)
Pyroxenite–peridotite interaction experiments at 1380 and 1400 ∘C produced wider reaction zones (up to 950 µm) and significant modal changes in the peridotite layer (Fig. 5). Incipient melting of the lherzolite, observed in FLZ experiments at 1380–1400 ∘C, induced a significant porosity in the peridotite layer, which was high enough to allow melt infiltration from the adjacent molten pyroxenite, as observed in previous experimental works (e.g. Saper and Liang, 2014; Wang et al., 2020). However, the determination of near-solidus low-melt-fraction composition is challenging in experimental studies on peridotite partial melting, and it would require the use of specific experimental techniques (e.g. Hirose and Kushiro, 1993; Laporte et al., 2004; Dasgupta and Hirschmann, 2007), which are beyond the aim of this study. As the chemistry of the thin films of interstitial glass collected in FLZ experiments has been presumably modified during the quench, mass balance calculations did not provide a reliable quantification of melt fractions. To circumvent this uncertainty, we derived the peridotite melt fraction using the equation proposed by Hellebrand et al. (2002), which is based on the composition of residual spinel. The calculation provided lherzolite melting degrees of 6 % at 1380 ∘C and 8 % at 1400 ∘C, consistent with the results of Wang et al. (2020) in melt–lherzolite reaction experiments at 2 GPa (5 % and 7 % at 1375 and 1425 ∘C, respectively).
The infiltration of a pyroxenite-derived melt into the peridotite layer is supported by textural and chemical observations. First, the thickness of the lherzolite layer after the experiments is significantly reduced, and its upper portion is substituted by a websteritic reaction zone (Fig. 5a). Secondly, the composition of minerals in the peridotite layer is modified throughout its thickness, as revealed by the increase in Ti content coupled with the decrease in XMg and XCr in pyroxenes and spinels (Figs. 6, 7 and 8). Indeed, the rather slow diffusion rate of Ti in both pyroxenes (e.g. Cherniak and Liang, 2012) precludes its mobility through the subsolidus peridotite, suggesting that the higher Ti content measured in pyroxenes and spinels from the peridotite layer must reflect melt migration towards the bottom of the charge.
The interaction between lherzolite and pyroxenite-derived melts produces an opx-rich websterite through the following reaction:
where (lherzolite + melt0) is assumed to be the starting melt-bearing lherzolite we synthesized in FLZ experiments, whereas melt1 is the andesitic melt resulting from the molten pyroxenite layer (Table 1). This reaction is similar to that derived by Wang et al. (2020) in melt–peridotite reaction experiments at 2 GPa using eclogite-derived melts, except for the presence of clinopyroxene among the reaction products.
Reaction (R2) is controlled by the composition of melt1, this latter varying with the Px1 melting degree as a function of temperature. The silica activity of Px1 partial melts decreases with increasing melt fraction (Borghini and Fumagalli, 2020). Melt1 reacts with the peridotite forming the opx-rich websterite, and, through interaction with partially molten peridotite, it acquires lower silica activities and precipitates clinopyroxene in the adjacent peridotite portion (Fig. 10b). Accordingly, mixed experiments have shown that strong mineralogical changes in infiltrated peridotites are strongly controlled by the composition of reacting melts (e.g. Lambart et al., 2012; Mallik and Dasgupta, 2012). Similar pyroxene enrichments in wall-rock peridotite were described in ultramafic massifs (e.g. Pearson et al., 1993; Varfalvy et al., 1997; Takazawa et al., 1999). In the External Liguride (EL) mantle sequences (northern Apennine, Italy), the interaction between pyroxenite-derived melt and host peridotites produces an opx-rich rim at the contact coupled with simultaneous modal pyroxenes enrichment in the adjacent peridotites (Hidas et al., 2021).
At 1450 ∘C the pyroxenite Px1 is almost completely molten (Borghini and Fumagalli, 2020), and peridotite FLZ has the high melt fraction with interconnected textures. Fluxing of pyroxenitic melt into molten porous peridotite further enhances peridotite melting creating a melt-bearing dunite associated with a refractory harzburgite. Partial melt produced by concomitant melting of pyroxenite Px1 and FLZ has a basaltic composition with XMg of 0.84 and low alkali contents (Na2O + K2O < 1.6 wt %; Table S9). In a more dynamic and open-system scenario, in which melt is expected to be extracted after the reaction, the pyroxenite–peridotite interaction at such a high temperature forms melt-bearing channels leaving a refractory peridotitic residue. This experimental result supports, therefore, the theoretical models proposing that melt released from a fertile heterogeneity could induce chemically isolated, channelized melt transport into the mantle (Weatherley and Katz, 2016, and references therein).
4.3 Melt–peridotite interaction effect on mineral chemistry
Reaction experiments highlight mineral chemistry changes in the peridotite layer as a result of dissolution and reprecipitation coupled with element diffusion across the pyroxenite–peridotite boundary. The major chemical variations are recorded by pyroxene and spinels (Figs. 6, 7 and 8). The XMg and XCr decrease is correlated with the thickness of reaction layers, which is, in turn, temperature dependent. While at relatively lower T (1300–1350 ∘C) chemical variations in pyroxene are confined at the pyroxenite–peridotite contact, at higher temperature (T > 1350 ∘C) chemical and mineralogical variations within the peridotite are enhanced by local pyroxenitic melt infiltration. This is indicated by higher Ti contents in pyroxenes coupled with higher Na in cpx and Ca in orthopyroxene far from the reaction zone (Figs. 6, 7).
In the reaction zone, pyroxenes show a wider variability, and inferences can be drawn by comparing our results with previous experimental studies that investigated melt–peridotite interactions at similar P–T conditions (Fig. 11). Orthopyroxenes in our pyroxenite–peridotite reaction experiments have XCr and Ca positively correlated to XMg, whereas Ti contents increase at decreasing XMg (Fig. 11a, b, c). It is worth noting that such variations are strongly dependent on temperature as they reflect the interaction with melts resulting from variable degrees of melting of the starting pyroxenite Px1 as a function of T (see Table 1 and Fig. 2). In Fig. 11a, the XCr and XMg variations in orthopyroxene from our runs and the other reaction experiments at 2 GPa (Wang et al., 2013, 2016, 2020) define a trend with the highest values shown by orthopyroxene in reactive harzburgite at 1450 ∘C (this study). Ca contents in orthopyroxene are overall high and mostly reflect high experimental temperatures (Fig. 11b). Ti contents in orthopyroxene increase with decreasing T as a function of the TiO2 content of the reacting melts (Table 1). Very high TiO2 contents in orthopyroxene have been documented by reaction between peridotite and high-TiO2 eclogite-derived melt (Mallik and Dasgupta, 2012; Fig. 11c).
Clinopyroxenes show an XCr–XMg correlation similar to orthopyroxene (Fig. 11d) and comparable with clinopyroxenes produced by melt–peridotite reaction experiments using anhydrous (Wang et al., 2013) and hydrous (Wang et al., 2016) basaltic andesites at 1–2 GPa. Decrease in Na at increasing XMg in clinopyroxenes further reflects the interaction with melts produced by higher melting degrees of Px1, as also indicated by the Na–XMg trend defined by clinopyroxene compositions in melt–peridotite reaction experiments at 2.5–3 GPa (Mallik and Dasgupta, 2012) (Fig. 11e).
Spinels in experimental reacted peridotites show significant chemical changes mostly in terms of XCr values. The highest XCr values are found in the bottom of charges and are similar to those measured in spinels from unmodified peridotite (FLZ runs). In general, XCr of spinel progressively decreases toward the contact with the molten pyroxenite (Fig. 8). In the reaction run at 1400 ∘C, XCr values are similar to those documented in spinels of dissolution experiments reported by Wang et al. (2013) (Fig. 12). However, the increasing extent of melting or melt–peridotite reaction, as well as the increase in temperature, is expected to increase the XCr and decrease the XMg (Lo Cascio et al., 2008; Van den Bleeken et al., 2010; Tursack and Liang, 2012). Lowering of XCr in spinels of our high-T experiments reflects interaction between a Cr-bearing spinel (previously synthesized in FLZ experiments) with low Cr, high Al melts. Lambart et al. (2012) obtained similar low XCr (0.05–0.1) coupled with low XMg (0.61–0.76) in spinels from experiments of peridotite impregnation by pyroxenite-derived melts at 1 and 1.5 GPa. Remarkably, we observe low XCr in spinels also in 1300–1350 ∘C runs, not affected by significant infiltration of pyroxenite-derived melt. Although diffusion coefficients of Cr and Al are rather low when compared to Fe and Mg, Suzuki et al. (2008) showed that the diffusivity of Al is 1 order of magnitude higher than that of Cr. Therefore, Al diffusion from the melt-bearing pyroxenite layer could explain the low XCr in the neighbouring peridotites.
4.4 Comparison with natural occurrences
The systematic mineral chemistry variations related to pyroxenite–peridotite interactions, documented in our experiments, might provide a petrological guide to decipher natural occurrences. A comparison of experimental results with natural records from peridotites adjacent to pyroxenite veins and layers in ultramafic massifs is therefore mandatory.
Borghini et al. (2020) recently reported detailed chemical profiles across pyroxenite–peridotite associations from External Liguride (EL) mantle sequences (northern Apennine, Italy). They recorded systematic variations in XMg and XCr in pyroxenes and spinels in the wall-rock peridotite, in response to reactive percolation of pyroxenite-derived melt. These pyroxenites likely originated from high-pressure segregation of melts, partially derived from a silica-excess pyroxenite-bearing (Borghini et al., 2016) composition comparable with the starting pyroxenite Px1 used in this experimental study.
The composition of pyroxenes and spinels from metasomatised peridotite (EL wall rock) of External Liguride mantle sequences is reported in Figs. 11 and 12. Compositional fields defined by minerals in the EL metasomatised peridotite match the compositions of reaction minerals produced in our experiments at 1300–1350 ∘C. This suggests that the chemical changes in minerals of EL peridotite can be ascribed to interaction with andesite basalt-like melts, similar to Px1 partial melts, at temperatures near the peridotite solidus. Some discrepancies are observed for Ca in orthopyroxene and Ti in spinel. Lower Ca contents in orthopyroxene from EL peridotites (Fig. 11) presumably resulted from cooling of these ophiolitic mantle sequences, as clearly indicated by diffuse exolutions in pyroxene porphyroclasts (Borghini et al., 2020). High Ti contents in spinel observed in EL peridotites could reflect the richer Ti composition of infiltrating melt relative to the Px1 partial melts here investigated. Alternatively, Ti enrichment can derive by partial plagioclase-facies recrystallization that affected the EL mantle sequences (Borghini et al., 2011).
Similar chemical gradients within peridotite-hosting pyroxenite veins were widely documented in mantle sequences from ophiolites (e.g. Varfalvy et al., 1996, 1997) and orogenic massifs (e.g. Lherz: Fabries et al., 2001; Balmuccia: Rivalenti et al., 1995; Mukasa and Shervais, 1999). The most common chemical features are the lowering of XMg and XCr in pyroxenes and spinels in peridotites at the contact with pyroxenites, usually interpreted as the result of interaction between pyroxenite-derived melts and host peridotite. Woodland et al. (1996) reported a detailed study on the composition of spinel in Lherz peridotite adjacent to pyroxenite veins, nicely describing the development of local chemical gradient in spinel formed by non-pervasive metasomatism of peridotite along the contact with pyroxenite veins. Notably, they show the same systematic XCr lowering that we observed in spinels of peridotite after reaction experiments (Fig. 12).
The composition of experimental orthopyroxenes at 1450 ∘C closely overlaps the compositional field of orthopyroxenes in dunite channels from Balmuccia ultramafic massif (Fig. 11a, b, c), which was interpreted as the result of focused reactive percolation of MgO-rich melts produced by the whole pyroxenite melting into the adjacent peridotite (Mazzucchelli et al., 2009). Still, the lower Ca contents suggest a cooling effect recorded by these rocks in comparison to experimental temperatures (see above). Therefore, our experimental results support the potential role of pyroxenite in focusing melt percolation through the mantle responsible for the origin of refractory dunite–harzburgite channels.
We stress that the comparison of detailed chemical profiles in pyroxenite–peridotite mantle sequences with experimental data of this work provides valuable constrains to discriminate between melt–peridotite interaction processes occurring at low- and high-temperature conditions.
4.5 Insights on the composition of secondary pyroxenites
The experimental results of this study further confirmed that high-pressure melt–peridotite interaction is able to significantly modify the mineralogy and chemistry of mantle peridotite. In particular, the interaction between peridotite and pyroxenite-derived melt leads to mantle re-fertilization and triggers a new generation of pyroxenite. Lambart et al. (2012) have demonstrated that impregnation of peridotite by a finite amount of melts produced by partial melting of pyroxenite generates a large range of pyroxene-rich rocks that they named “secondary” or “stage2” pyroxenite (Lambart et al., 2013). They supported this hypothesis through experiments of peridotite impregnation by melts from two silica-deficient pyroxenites at 1 and 1.5 GPa. Assuming variable ratios between infiltrated peridotite and pyroxenite-derived melts, they elaborated a thermodynamic model to estimate the effect of peridotite modifications. The mineralogy and chemistry of reaction products are mostly affected by the composition of reaction melts (e.g. silica activity; Lambart et al., 2012) and by the physical state of the host peridotite (Wang et al., 2020), i.e. the ability of pyroxenite-derived melts to infiltrate the host peridotite (Lambart et al., 2012). At lithospheric mantle conditions (P = 1–3 GPa), pressure has a subordinate effect on the newly forming pyroxenites, mostly controlling the presence of plagioclase, spinel or garnet.
In this section, we use the compositions of experimental phases resulting from the interaction between the Px1 partial melts and the FLZ to derive the composition of a second generation of pyroxenites. We used the modal abundances estimated by image analysis on the reaction zones to recalculate the bulk compositions of secondary pyroxenites (Fig. S3). The resulting bulk compositions are projected from diopside (Di) in the pseudo-ternary diagram Fo–CaTs–Qz (forsterite, Ca-Tschermak's pyroxene and quartz, respectively) of Fig. 13, together with the compositions of selected pyroxenites from orogenic and ophiolitic ultramafic massifs. Secondary pyroxenites resulting from our reaction experiments at 2 GPa and 1300–1400 ∘C plot in a relatively narrow range near the lowest part of the En–CaTs (enstatite–Ca-Tschermak) join. Figure 13 also shows the compositional trends (grey arrows) calculated by modelling the reaction between melts produced by silica-deficient pyroxenites and lherzolite assuming variable melt rock ratios (Lambart et al., 2012). Secondary pyroxenites formed by the infiltration and reactive crystallization within peridotite of silica-rich melts, like Px1 partial melts of this study, have bulk compositions plotting towards the silica-rich part of the Fo–En–CaTs triangle (i.e. near to En apex). They differ from the Ronda pyroxenites (group ; Garrido and Bodinier, 1999), interpreted as reaction products from melt derived by silica-deficient pyroxenite (Lambart et al., 2012). This strongly reflects the major role of melt composition in the mineral modes resulting from the reactions, because reacting melts with higher Si contents (or higher silica activity) results in preferential precipitation of orthopyroxene, as shown in this study and previous experimental works using basaltic andesites or ferro-basalts (e.g. Wang et al., 2013, 2020).
Notably, computed secondary pyroxenite compositions are similar to those of orthopyroxene-rich spinel westerites documented in some natural mantle sequences, as in Beni Bousera (Pearson et al., 1993), Ronda (Garrido and Bodinier, 1999) and Lherz (Bodinier et al., 1987a, b). Moreover, orthopyroxene-rich pyroxenites with bulk compositions similar to those resulting from our reaction experiments are documented in supra-subduction ultramafic massifs (SSZ-py in Fig. 12). The origin of these pyroxenites was ascribed to the infiltration and interaction of Si-rich (boninite-like) melts with variably depleted mantle peridotites (Varfalvy et al., 1997; Tilhac et al., 2016; Rogkala et al., 2017). In summary, the bulk compositions of secondary pyroxenite can be used to evaluate the chemistry of melt involved in the reaction with the peridotite.
At relatively low temperature (1300–1350 ∘C), interactions between pyroxenite-Px1-derived melt and lherzolite FLZ is confined at the boundary between partially molten pyroxenite and subsolidus lherzolite. Precipitation of orthopyroxene-rich aureole from the lherzolite wall rock determines the development of modal layering forming orthopyroxenite or websterite at the periphery and clinopyroxene-rich domain in the inner portion of pyroxenite. Chemical changes in minerals are mostly observed in the phases of pyroxenite crystal mush as a result of orthopyroxenite precipitation coupled with element diffusion across the pyroxenite–peridotite interface. These results provide experimental proofs of the pyroxenite reactive crystallization that is responsible for modal and chemical zoning in pyroxenite emplaced in mantle peridotites, as widely documented from studies on natural pyroxenite–peridotite mantle sequences.
At higher temperatures (T = 1380–1400 ∘C), the onset of peridotite partial melting enhances pyroxenite-derived melt infiltration that significantly modifies the mineralogy and chemistry of the host peridotite by creating orthopyroxene-rich websterites and pyroxenite-rich lherzolite. Chemical gradients in minerals produced by pyroxenite–peridotite reaction experiments are comparable with those observed in mantle sequences from ultramafic massifs. The experimental data of this work can be used to discriminate between low- and high-temperature melt–peridotite reactions. Bulk compositions of rocks originating through the interaction between pyroxenite-derived melt and peridotite mostly reflect the chemistry of the reacting melt.
All data derived from this research are presented in the enclosed tables, figures and Supplement.
The supplement related to this article is available online at: https://doi.org/10.5194/ejm-34-109-2022-supplement.
GB, PF and ER conceptualized the project. GB and PF performed the experiments. GB characterized the samples and collected phase compositions. GB, PF and ER visualized, discussed and elaborated the data. GB wrote the original draft. PF and ER revised and edited the manuscript draft. Acquisition of the financial support for the project was provided by PF and ER.
At least one of the (co-)authors is a member of the editorial board of European Journal of Mineralogy. The peer-review process was guided by an independent editor, and the authors also have no other competing interests to declare.
Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.
This article is part of the special issue “Probing the Earth: experiments and mineral physics at mantle depths”. It is not associated with a conference.
We gratefully thank Chunguang Wang and Alexandre Corgne for their constructive reviews and Didier Laporte for the editorial handling. Andrea Risplendente is thanked for technical assistance during the work by electron microprobe.
Funding was provided by the Italian Ministry of Education, University and Research (MIUR) (grant no. PRIN-2015C5LN35) “Melt rock reaction and melt migration in the MORB mantle through combined natural and experimental studies”.
This paper was edited by Didier Laporte and reviewed by Chunguang Wang and Alexandre Corgne.
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