Carbon-saturated COH fluids in the upper mantle: a review of high-pressure and high-temperature ex situ experiments
- 1Institut für Mineralogie, Westfälische Wilhelms-Universität Münster, 48149 Münster, Germany
- 2Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC 20015, USA
- 3Dipartimento di Scienze della Terra, Università Degli Studi di Milano, Via Mangiagalli 34, 20133 Milan, Italy
Correspondence: Carla Tiraboschi (email@example.com)
High-pressure COH fluids have a fundamental role in a variety of geological processes. Their composition in terms of volatile species can control the solidus temperature and carbonation/decarbonation reactions, as well as influence the amount of solutes generated during fluid–rock interaction at depth. Over the last decades, several systems have been experimentally investigated to unravel the effect of COH fluids at upper-mantle conditions. However, fluid composition is rarely tackled as a quantitative issue, and rather infrequently fluids are analyzed in the same way as the associated solid phases in the experimental assemblage. A comprehensive characterization of carbon-bearing aqueous fluids in terms of composition is hampered by experimental difficulties in synthetizing and analyzing high-pressure fluids without altering their composition upon quenching.
Recently, improved techniques have been proposed for the analyses of experimental carbon-saturated COH fluids, leading to a significant advancement in synthetic fluid characterization. Here, we present a review of carbon-bearing aqueous fluid experiments conducted at lower-crust and upper-mantle P–T (pressure and temperature) conditions, in which fluids have been characterized quantitatively through ex situ techniques. We review the experimental background of the most commonly employed thermodynamic models for COH fluids, together with the techniques to synthetize them and analyze their composition when the fluid coexists with solid phases. We highlight how a quantitative approach to COH fluid analyses is a fundamental step to understand the effect of these fluids at upper-mantle conditions and to provide a strong experimental foundation to thermodynamic models to ultimately unravel the deep cycling of elements.
Aqueous fluids are involved in many geological processes, from controlling the location and extent of melting to hydrothermal ore genesis, earthquake generation, arc volcanism, and rock-forming processes in general (e.g., Green, 1973; Tatsumi et al., 1986; Taylor and McLennan, 1995; Poli and Schmidt, 2002). In subduction zones, aqueous fluids derived from devolatilization processes of the oceanic lithosphere and its sedimentary cover (Schmidt and Poli, 2014, and references therein) are major vectors of mass transfer from the slab to the mantle wedge (Kawamoto et al., 2013; Kogiso et al., 1997; Manning, 2004; Sanchez-Valle, 2013; Scambelluri and Philippot, 2001) and contribute to the recycling of elements and their geochemical cycles.
In this setting CO2 is the second most abundant volatile species, as testified by fluid inclusions in mantle wedge peridotites (Andersen and Neumann, 2001; Frezzotti and Touret, 2014; Kawamoto et al., 2013; Scambelluri et al., 2009) and by volcanic arc emissions (Wallace, 2005; Mason et al., 2017). CO2 is transferred from the oceanic lithosphere to the mantle wedge through dissolution of carbonates (Caciagli and Manning, 2003; Sanchez-Valle et al., 2003), diapirism of slab rock (Marschall and Schumacher, 2012; Tumiati et al., 2013), and carbonatitic melts (Hammouda and Keshav, 2015; Poli, 2015; Stagno, 2019). Recent experimental data indicate that the CO2 content fluxing from the slab to the mantle wedge could be higher than previously thought due to the effect of silicate dissolution in the presence of graphite, independently from carbonates occurrence (Tumiati et al., 2017). Graphite, previously considered a refractory phase (e.g., Manning et al., 2013), can effectively increase the CO2 budget of the mantle wedge by oxidation processes favored by the dissolution of minerals such as forsterite, enstatite (Tiraboschi et al., 2018), and quartz (Tumiati et al., 2017).
Graphite is brought to depth as carbonaceous material in subducted sedimentary rocks and exhibits a progressive increase in crystallinity with pressure and temperature, from poorly crystallized to almost crystalline graphite (e.g., Beyssac et al., 2002). These forms of carbon are commonly identified as disordered graphitic carbon (Aoya et al., 2010; Beyssac and Rumble, 2014) and may be representative of carbonaceous material at forearc to sub-arc metamorphic conditions. At high temperature and pressure conditions, up to approximately 5 GPa, crystalline graphite is considered the most common form of carbon (Beyssac et al., 2002) before its transition to diamond (e.g., Day, 2012).
The important role of graphite, and its variable degrees of crystallinity in the subduction zone, has been also pointed out by recent studies (Tumiati et al., 2020; Vitale Brovarone et al., 2020). For instance, Tumiati et al. (2020) showed that in subducted sediments flushed by aqueous fluids, the removal of disordered graphitic carbon is more efficient compared to crystalline graphite. By considering disordered graphitic carbon as a proxy for subducted organic matter, the authors suggested that carbon can be effectively removed from the subducting slab, prompting metasomatic processes in the mantle wedge. Vitale Brovarone et al. (2020) observed an analogous process in blueschist facies rocks from Alpine Corsica and the Western Alps, where subducted carbonaceous material is mobilized at forearc conditions by channelized fluid pathways.
The presence of graphite in rock assemblages brings strong constraints to possible COH fluid compositions (Holloway, 1984). Conventional thermodynamic modeling (e.g., PERPLE_X: Connolly and Cesare, 1993; COH: Huizenga, 2001; Gfluid: Zhang and Duan, 2009) allows for the retrieval of the volatile speciation of the COH fluid associated with graphite or diamond as a function of P (pressure), T (temperature), and fO2. However, these models rely on equations of state (EoS) that only consider pure molecular species (e.g., H2O, CO2, CH4, CO). Recent advances in thermodynamic modeling, represented for instance by the Deep Earth Water (DEW) model (Huang and Sverjensky, 2019; Sverjensky et al., 2014b), allow not only molecular species but also charged species to be investigate, such as carbonate or bicarbonate ions and organic dissolved compounds (Pan and Galli, 2016; Sverjensky et al., 2014a; Tiraboschi et al., 2018). However, additional constraints on the speciation of solutes are required to properly calibrate thermodynamic models in more complex systems.
In this review, we will present recent experimental data on carbon-saturated COH fluids. We will address the following: (i) the volatile speciation of graphite-saturated COH fluids (hereafter GCOH fluids); (ii) the volatile speciation and solute content of GCOH fluids in equilibrium with different solid phases; and (iii) the different dissolution behavior of disordered graphitic carbon and crystalline graphite in aqueous fluids.
1.1 GCOH fluids: thermodynamic constraints and theoretical background on molecular neutral species
The volatile speciation in the pure COH system is often represented by means of ternary C–O–H chemographic diagrams, in which the main molecular neutral species (i.e., H2O, CO2, CH4, CO, H2, and O2) are plotted together with the solid carbon phase (i.e., graphite or diamond). The COH ternary diagram presents a two-phase field delimited from a one-phase field by the graphite-saturation surface (Connolly, 1995; bold solid line in Fig. 1), which is the locus of points representing the composition of a COH fluid phase coexisting with a solid carbon phase, in this case graphite. The position of the graphite-saturation surface varies with pressure and temperature: decreasing temperatures shift the curve toward H2O, while decreasing pressure leads to the opposite effect (Huizenga, 2011).
Considering the Gibbs phase rule the two-phase field, graphite + COH fluid, is univariant if pressure and temperature are fixed. Accordingly, the composition of a COH fluid in equilibrium with graphite would lie on the tie-line (dashed lines in Fig. 1) that connects the graphite vertex to the graphite-saturation surface. As graphite is a phase of fixed composition, the composition of the COH fluid would lie on the graphite-saturation surface.
In a closed fluid system (i.e., no mass is gained or lost by the system), the GCOH fluid speciation will be determined uniquely by the molar ratio. This ratio can be expressed by the variable X(O) (Connolly, 1995; Labotka, 1991), i.e., the atomic fraction of oxygen relative to oxygen + hydrogen, which is in turn related to oxygen fugacity (fO2). The GCOH systems can be described through the reactions occurring among the main species within the diagram and their relative equilibrium constants (French, 1966; Ohmoto and Kerrick, 1977):
where fi is the fugacity of the species i (e.g., H2O, CO2, CH4) and ac is the activity of the carbon solid phase (ac=1 in GCOH fluids). The four equations present six unknowns, i.e., the fugacities of H2, O2, H2O, CO2, CO, and CH4. To solve the system two compositional constraints are required. The first constraint is given by the assumption that the total fluid pressure is equal to the sum of partial pressures of the fluid volatile species:
Moreover, the sum of all molar fractions of the fluid must equal a unit:
Therefore, the total fluid pressure can be expressed as follows:
The additional constraint needed to solve the system, at fixed pressure and temperature, is given by fO2, which can be controlled in experimental runs employing redox buffering assemblages (e.g., fayalite–magnetite–quartz (FMQ), hematite–magnetite (HM)), also known as oxygen buffers. Experimentally controlling the fO2 allows us to determine the composition of carbon-saturated fluids by means of thermodynamic modeling since the composition of the fluid will be uniquely defined at fixed P and T (white dots in Fig. 1). Nevertheless, this approach relies on some concepts which have to be considered when the COH volatile speciation is calculated (French, 1966):
The calculation is valid only for a homogeneous COH fluid and does not apply if additional elements are present in the gas (e.g., N, S, and Cl) or if the fluid reacts with the associated mineral assemblage, except for graphite. The presence of solutes will increase the solvus temperature of the system (e.g., Bowers and Helgeson, 1983) and will affect the activity of H2O (e.g., Aranovich and Newton, 1997; Tumiati et al., 2017).
The gas phase is assumed to exhibit ideal behavior under all conditions.
The fluid is assumed to be in continuous equilibrium with graphite. Disequilibria with graphite, or the presence of disordered graphite, will change the thermodynamic properties of the fluid (see Tumiati et al., 2020).
The uncertainty of the fO2 calculated with thermodynamic models for different external buffers, such as FMQ or HM, might lead to different results in term of volatile speciation, as COH fluid composition is extremely sensitive to changes in oxygen fugacity (Huizenga, 2001).
The calculation can be performed only in a closed system. The direct application of the results to natural fluid systems, which might not represent closed systems, should be carefully evaluated.
Consequently, for a comprehensive characterization of COH fluids, these issues must be considered, especially in more complex chemical systems where the combined effect of these factors could significantly affect the volatile speciation.
1.2 Experimental data behind the thermodynamic modeling
At the current state thermodynamic modeling represents a viable way to predict fluid speciation for simple chemical systems at specific pressure and temperature conditions, and several programs based on different computational languages are available. The majority of the programs rely on the equilibrium-constant mass balance technique (French, 1966) to perform the calculations. The model is based on the chemical equilibria between the existing species and the relatives' equilibrium constants. The latter can be calculated using different equations, as well as thermodynamic datasets. Assuming ideal mixing a direct relation between the mole fraction and the fugacity of species can be established and used to determine the equilibrium constants (e.g., Huizenga, 2001). Ohmoto and Kerrick (1977) provide a set of Pfluid–T equations for the equilibrium constants with thermodynamic data from previous authors (i.e., Holland, 1965; Huebner, 1971). Furthermore, the same equilibrium constants can be calculated with the Gibbs free energy of the reaction, obtained with the enthalpy, entropy, and isobaric heat capacity of the fluid species (Huizenga, 2001, and references therein). Modeling COH fluids at high-pressure and high-temperature conditions also requires a reliable equation of state. Several formalisms have been developed for fluid phases (e.g., Zhang and Duan, 2009) relying on standard formalisms for the evolution of volume with pressure or combining pressure and temperature. Sometimes temperature can be accounted for in modified versions of standard equations of state (e.g., Fried and Howard, 2000). EoS are usually based on experimental data collected in a limited pressure and temperature range or even obtained a priori and fitted afterward to a specific dataset. For these reasons it represents a significant source of uncertainty in models. In recent years also molecular dynamic (MD) simulations have emerged as a means to study fluid speciation at non-ambient conditions (e.g., Huizenga, 2001; Zhang and Duan, 2009) and generate data to be used for equation state fitting.
Currently, several computer programs (e.g., PERPLE_X: Connolly and Cesare, 1993; COH: Huizenga, 2001; Gfluid: Zhang and Duan, 2009) offer the possibility of calculating COH fluid speciation at specific pressure and temperature conditions, provided that the system under examination meets the necessary requirements (see Sect. 1.1).
Analyzing volatiles at high-pressure and high-temperature conditions is not trivial. A variety of analytical techniques are available and routinely employed for the characterization of solid phases and for the analysis of fluids in natural or synthetic inclusions (Frezzotti et al., 2012; Lamadrid et al., 2014; Li, 2017; Pasteris and Wanamaker, 1988; Pawley et al., 1992; Roedder, 1965). Even though the study of natural fluid systems is of fundamental importance, the trapped fluid may experience different post-entrapment processes, such as H diffusion through the host mineral (e.g., olivine), or undergo composition modifications upon decompression and cooling. Consequently, the development of experimental and analytical strategies involving synthetic fluids is crucial to provide solid benchmarks for high-pressure fluid characterization.
Over the years different approaches, either in situ or ex situ, have been established. For the purpose of this review, we will briefly mention the most common in situ techniques and then focus solely on the ex situ approach.
In situ techniques (Sanchez-Valle, 2013, and references therein) are generally achieved through hydrothermal diamond anvil cells (HDAC; Bassett et al., 1993; Schmidt and Chou, 2012) associated with different analytical approaches, such as Raman and Fourier transform infrared (FTIR) spectroscopy (e.g., McCubbin et al., 2014; Mysen and Yamashita, 2010). HDAC can be also coupled with laser or synchrotron X-ray spectroscopies (Louvel et al., 2013; Mookherjee et al., 2014; Wilke et al., 2012; Zotov and Keppler, 2002). These approaches allow the retrieval of information about the speciation of volatiles directly during the experimental run, together with the speciation of major solutes and trace elements, but do not provide the total amount of volatile present in the experimental charge or the amount of dissolved species in the fluid in terms of molar concentration. This information can be retrieved through ex situ techniques, which provide quantitative analyses of volatile species (e.g., Miozzi and Tumiati, 2020; Tiraboschi et al., 2016; Tumiati et al., 2017) or the concentration of dissolved species in the fluid (e.g., Kessel et al., 2004; Tiraboschi et al., 2018).
Ex situ experimental works on COH fluids have required the development of original strategies (e.g., Akaishi and Yamaoka, 2000; Chepurov et al., 2012; Matveev et al., 1997; Morgan et al., 1992; Truckenbrodt et al., 1997; Truckenbrodt and Johannes, 1999) to recover the fluid phase from the experimental capsule and measure the fluid composition afterwards through a variety of analytical approaches. COH fluids can be synthetized in a wide range of P–T composition conditions through piston cylinders and multi-anvil apparatus; however, quenching the fluids to room conditions might represent a drawback. The bulk composition of the quenched fluid in terms of C, O, and H is considered to be representative of the experimental P–T conditions when high quench rates are attained (i.e., > 20 ∘C min−1; Matveev et al., 1997). Conversely, for low quench rates, possible modifications in the speciation of volatiles can only be ruled out by confronting the volatile speciation with complementary in situ studies (e.g., Schmidt, 2014) or by thermodynamic modeling (see Tiraboschi et al., 2016). Ex situ experiments have the fundamental advantage of allowing the oxygen fugacity conditions to be accurately controlled through the double capsule technique (Eugster, 1957; Eugster et al., 1966), a strategy employed to keep the sample physically separated from the oxygen buffer. This technique consists of employing an inner capsule permeable to hydrogen (e.g., AuPd, AgPd), which contains the sample and the GCOH fluid source (i.e., graphite and a compound that generates a COH fluid at the experimental conditions). The outer capsule contains the inner capsule, an oxygen buffer, and H2O. Due to H2 permeability of the capsule material, the hydrogen fugacity conditions (fH2) will be the same in the inner and in the outer capsule. Indirectly, also the other species in the COH fluid will be fixed by the oxygen buffer, including O2. However, as the inner capsule contains a mixed COH fluid and not pure water only, the fO2 in the inner capsule will be lower compared to the fO2 in the outer capsule (Luth, 1989).
For what concerns fluid sources, different solid organic compounds (e.g., stearic acid, oxalic acid dihydrate) can be employed to generate COH fluids in experimental runs (see Fig. 1). Usually, the choice of the fluid source depends on the ratio, assuming that this ratio will be maintained at the experimental P–T conditions (Table 1) or that the initial volatile speciation is adequate to provide the expected equilibrium speciation if oxygen buffers are employed.
The first ex situ analysis of COH fluids was performed by Holloway et al. (1968). The authors investigated the decomposition of oxalic acid dihydrate (OAD; H2C2O4•2H2O) in cold seal and internally heated pressure vessels at 0.1 to 0.7 GPa and 500 to 1005 ∘C. OAD was employed to generate a COH fluid (Boettcher et al., 1973; Eugster et al., 1966; Eugster and Skippen, 1967) as it decomposes at high temperatures to H2O, CO2, and H2. After quenching, the capsule was punctured in an evacuated chamber and the fluid was analyzed through a gas chromatograph for CO2, CO, and CH4.
Eggler et al. (1979) implemented the capsule-piercing technique of Holloway et al. (1968) by modifying the gas chromatograph, using a thermal conductivity detector and an electronic peak integrator. The authors investigated the solubility of CO2 and CO in different silicate melts synthesized in piston cylinder experiments at 3 GPa and 1700 ∘C. To extract the fluid, the capsule was placed at the bottom of a vacuum valve connected to a gas chromatograph. The valve was then rapidly closed to puncture the capsule, and the gases were swept to the chromatographic column. The analyzed CO2 concentrations were systematically higher compared to the calculated values through Redlich–Kwong EoS (Redlich and Kwong, 1948). The effect was attributed to CO formation due to low-temperature re-equilibration reactions between graphite and CO2.
Taylor and Green (1987) employed a capsule-piercing device connected to a mass spectrometer to investigate reducing GCOH fluids in the model peridotite system nepheline–forsterite–silica. The device was composed of a modified Whitey regulating valve with a redesigned stem tip into a harder needlepoint. To obtain low background levels, especially due to absorbed molecules of H2O on the metal surface, the system was evacuated for 12 h prior to measurements. The technique allowed methane, ethane, and trace amounts of C3−4 hydrocarbons to be measured. The strategy was then described in detail in the work of Taylor and Foley (1989), in which the authors assessed the composition of COH fluids buffered by WC–WO2–graphite (WCWO). Experiments were performed at pressures from 0.9 to 3.5 GPa and temperatures from 1000 to 1260 ∘C. The device allowed CH4, H2O, C2H6, and CO2 generated from stearic acid (C18H36O2) in equilibrium with graphite to be analyzed, and it provided a suitable buffering strategy for experiments at reduced oxygen fugacity conditions.
Jakobsson and Oskarsson (1990) modified the vacuum valve of the gas chromatography–thermal conductivity detector (GC–TCD) previously employed by Eggler et al. (1979) by connecting it to a quadrupole mass spectrometer (QMS). The capsule-piercing device was modified to allow the analysis of H2O by heating the inlet system to 80 ∘C. The authors retrieved the speciation of a GCOH fluid at iron–wuestite (IW) oxygen buffer conditions, at pressures from 0.5 to 1 GPa and temperatures from 900 to 1200 ∘C, analyzing H2, CH4, H2O, C2H6, CO, and CO2 through a Faraday cup detector. Since results were close to the calculated values, the authors suggested that equilibrium was reached during the experimental run and preserved upon quenching. In a subsequent work the same authors (Jakobsson and Oskarsson, 1994) investigated GCOH fluids in equilibrium with graphite from 0.7 to 2 GPa and 1100 to 1500 ∘C. The detected species were CO, CO2, and H2O, while H2, CH4, and C2H6 were absent (i.e., below detection limit of 0.1 mol %). Different quench rates showed decreasing CO with increased quench time, suggesting CO2 formation from CO, as previously proposed by Eggler et al. (1979).
Morgan et al. (1992) employed silica glass capsules and Raman spectroscopy to analyze the COH fluid generated by thermal dissociation of oxalic acid dihydrate. However, due to the brittleness of the capsule material, the investigated conditions of pressure and temperatures were limited to pressures lower than 0.13 GPa and temperatures below 750 ∘C. This approach allowed CO2, CH4, CO, and H2 to be measured, while H2O was estimated through mass balance calculation due to its weak Raman activity.
Matveev et al. (1997) analyzed redox-buffered, graphite-saturated COH fluids at 2.4 GPa and 1000 ∘C, over 7.5 orders of magnitude in oxygen fugacity, from −10.9 (CO–CoO buffer) to 24 logfO2 (SiC–SiO2–C buffer). The capsule was placed in a helium-flushed piercing device connected to a gas chromatograph. Lines were heated to 150 ∘C to prevent water condensation on the tubes. The system was calibrated to analyze H2O, CO2, C2H6, CH4, CO, and H2. Similarly, also Truckenbrodt et al. (1997) employed a gas chromatograph connected to a heated capsule-puncturing system to investigate the GCOH volatile speciation. The technique allowed them to obtain quantitative analyses of H2, CO, C2H6, CO2, CH4, and H2O generated from different organic compounds (C4H4O4, C9H10O2, and C14H22O) at 1 GPa and 900 ∘C.
Akaishi et al. (2000) synthesized diamonds from 13C-graphitic carbon and oxalic acid dihydrate at 7.7 GPa and 1600 ∘C. H2O and CO2 were analyzed through a QMS by piercing the platinum capsule. However, H2O could not be determined quantitatively because the inlet system was not heated, and thus the removal of the adsorbed water in the vacuum chamber was reported to be particularly difficult.
Dvir et al. (2013) determined the H2O and CO2 content at oxidizing conditions, employing diamond traps (Baker and Stolper, 1994; Hirose and Kushiro, 1993) to collect COH fluids from rocking multi-anvil experiments at 6 GPa and 1000 ∘C. The capsules were frozen at −90 ∘C in liquid nitrogen and open to expose the diamond trap. Fluids were conducted to an infrared gas analyzer by heating the diamond trap at 900 ∘C in a quartz tube.
Sokol et al. (2017a, b) investigated reduced N-poor and N-rich graphite-saturated COH fluids at pressures from 5.5 to 7.8 GPa and temperatures ranging from 1100 to 1500 ∘C, employing a Thermo Scientific FOCUS GS/DSQ II series single quadrupole MS analyzer, previously employed for the analysis of fluid inclusion (Sokol et al., 2014). The gas mixture was extracted by piercing the capsule and then injected into the analytical column at 300 ∘C. Analytical uncertainty for H2O, NH3, and CO2 was less than 10 % and in most cases less than 5 %.
Tiraboschi et al. (2016) developed a capsule piercing device connected to a QMS to determine the speciation of major volatiles in synthetic COH fluids. OAD was employed as the starting material, and experiments were performed at ambient pressure and 250 ∘C in single capsules heated in a furnace and at 1 GPa and 800 ∘C using a piston cylinder apparatus. The double capsule technique and the rhenium–rhenium oxide (RRO) oxygen buffer were employed to control the redox conditions. After the experimental run, the inner capsule was retrieved and placed in a reactor connected to a QMS. The connecting lines and the reactor were heated to 80 ∘C in order to avoid water condensation and to allow all volatiles released from the capsule after the piercing, including H2O, to be transported to the QMS by the gas carrier. The capsule-piercing technique provided quantitative analysis of the main volatile species in the COH system: H2O, CO2, CH4, CO, H2, and O2. The amount of volatiles in the capsule was retrieved using standard gas mixtures, with detection limits lower than 1 µmol. Moreover, the technique allowed air and/or N2 contained in the capsule or leaking into the line to be measured. Results indicated that the COH fluid speciation (in terms of neutral molecular species only, such as H2O and CO2) is preserved during and after quenching as the experimental data closely mimic the results from conventional thermodynamic modeling (see Tiraboschi et al., 2016), both in terms of bulk composition and fluid speciation. The same technique was employed for the characterization of COH fluid in equilibrium with silicates (Tumiati et al., 2017) and to investigate ordered and disordered graphitic carbon dissolution in subduction zones (Tumiati et al., 2020).
2.1 GCOH volatile speciation as a highly sensitive oxybarometer
The link between COH fluid speciation and the molar ratio can be exploited both ways: first, to calculate COH fluid speciation through thermodynamic models but also to determine the molar ratio and consequently the oxygen fugacity of the system under examination. The topic of assessing oxygen fugacity in experimental charges has been already addressed in the past, and oxybarometers of diverse nature have been calibrated. Metallic alloys (e.g., Ir–Fe; Stagno and Frost, 2010), metal-oxide couples (e.g., rutile–ilmenite; Tao et al., 2017), and mineral assemblages (e.g., olivine–orthopyroxene–spinel; Ballhaus et al., 1991) have been proven to be suitable for the use once the relation between their composition and activity is accurately described (e.g., Balta et al., 2011; Woodland and O'Neill, 1997). Over the years, solid redox sensors have been recognized to be extremely useful; however, the limitations related to their use (e.g., phase transitions, melting) have caused a push toward the definition and calibration of redox sensors based on non-solid phases (i.e., melts and fluids). For instance, Stagno and Frost (2010) have calibrated an oxybarometer based on the CO2 content of the melt in carbon–carbonate systems, while Miozzi and Tumiati (2020) calibrated an oxybarometer based on the CO2 content of aqueous fluids. The latter exploits the properties of the GCOH system and establishes a mathematical relation between XCO2 (= CO[CO2+H2O]) and the oxygen fugacity through a polynomial equation, whose coefficients were determined for both crystalline graphite and glass-like carbon (see Sect. 4). The susceptibility of COH fluid composition to fO2 conditions makes it an ideal oxybarometer as also the smallest variation is recorded with extreme precision (see Miozzi and Tumiati, 2020).
2.2 COH volatile speciation analyses in equilibrium with mantle minerals
So far, the speciation of COH fluids in equilibrium with rock assemblages has been often estimated through thermodynamic models that rely on equations of state of simple H2O–non-polar gas systems (e.g., equations of state of Connolly and Cesare, 1993, and Zhang and Duan, 2009). These models have been largely employed to constrain the composition of COH fluids in equilibrium with solid phases (Frost and McCammon, 2008; Goncharov and Ionov, 2012; Malaspina et al., 2010; Malaspina and Tumiati, 2012; Poli et al., 2009; Tumiati et al., 2013; Woodland and Koch, 2003), with the latter being routinely analyzed by means of electron microprobe. Recently, more complex models including dissolved species have been developed (Facq et al., 2014; Galvez et al., 2015; Huang and Sverjensky, 2019; Menzel et al., 2020; Pan et al., 2013; Sverjensky et al., 2014b) to account for the interaction between fluid and coexisting solid phases. However, these models still rely on a very limited experimental dataset due to the lack of quantitative analyses of synthetic COH fluid in equilibrium with minerals and the relative solubility data for the associated solid phases.
After the pioneering work of Eggler et al. (1979), which investigates the solubility of carbon monoxide in silicate melts, Taylor and Green (1988) analyzed the composition of reduced COH fluids in equilibrium with a peridotite at 3.5 GPa buffered employing the WCWO buffer (Taylor and Foley, 1989). The capsule-piercing device was heated at 150 ∘C which allowed them to determine the ratio in the fluid to range from 1000 to 1250 ∘C. This method enabled to assess a rapid change in fluid composition with increasing pressure, from a CH4-dominated fluid to a mainly aqueous fluid.
Dvir and Kessel (2017) investigated unbuffered garnet peridotite at 4–6 GPa and 900–1100 ∘C in equilibrium with H2O and CO2. The technique allowed them to obtain the ratio in the fluid or melt but not the total amount of volatiles.
Martin and Hermann (2018) and Sieber et al. (2018, 2020) employed the GC–TCD proposed by Eggler et al. (1979) to quantify the amount of CO2, H2O, and alkanes (from methane to hexane) in altered mafic oceanic crust. The measured XCO2 was found to be in agreement but slightly higher compared to thermodynamic modeling, suggesting the influence of additional charged species such as HCO (Sverjensky et al., 2014a). Sieber et al. (2020) investigate the carbonation of serpentinites by GCOH fluids at 1.5–2.5 GPa and 375–700 ∘C. Time series experiments indicated that after 96 h at 2 GPa and 600 ∘C, the carbonation of serpentinites is completed, showing how this process is efficient in sequestering CO2 from the interacting fluid into newly formed magnesite.
Tumiati et al. (2017) investigate the volatile speciation of COH fluids in equilibrium with mantle minerals in a carbonate-free compositional range at 800 ∘C and pressures of 1 and 3 GPa in order to focus on the role of graphite and silicates. GCOH fluids were synthesized in equilibrium with minerals representative of subduction mélanges, i.e., Mg-silicates (forsterite + enstatite), representative of the mantle component, and quartz, representative of the sedimentary component. Three different systems were compared: (i) COH, (ii) SiO2–COH, and (iii) MgO–SiO2–COH, all buffered at the same oxygen fugacity conditions (either nickel–nickel oxide (NNO) or fayalite–magnetite–quartz (FMQ)). Redox conditions were constrained employing the double capsule technique (Eugster, 1957; Eugster et al., 1966) in order to keep the starting material separated from the oxygen buffer. Depending on the experimental conditions investigated the fO2 conditions in the inner capsule corresponded to −14.28 at 1 GPa and 800 ∘C (NNO), −14.31 at 1 GPa and 800 ∘C (FMQ), and −11.66 at 3 GPa and 800 ∘C (FMQ) (see Tumiati et al., 2017).
The volatile speciation of quenched fluids was analyzed employing the capsule-piercing QMS technique (Tiraboschi et al., 2016), and the results were compared with conventional thermodynamic models using different equations of state and mixing properties of H2O and non-polar species.
The measured XCO2 from experiments and the modeled compositions of the COH fluids coexisting only with graphite overlapped in both experiments buffered with NNO and FMQ (XCO2=0.73 at 1 GPa and 800 ∘C, NNO; XCO2=0.67 at 1 GPa and 800 ∘C, FMQ; XCO2=0.74 at 3 GPa and 800 ∘C, NNO). At the investigated conditions the COH fluid was mainly constituted of CO2 (66.9 mol % at 1 GPa and 800 ∘C, FMQ; 73.7 mol % at 3 GPa and 800 ∘C, FMQ) and H2O (25.5 mol % at 3 GPa and 800 ∘C, FMQ; 32.3 mol % at 1 GPa and 800 ∘C, FMQ). However, the volatile speciation of COH fluids coexisting with either quartz–coesite (SiO2–COH system) or forsterite + enstatite (MgO–SiO2–COH system) clearly displayed a significant increase in XCO2 compared to experiments in which silicates were not present (Fig. 2).
The amount of CO2 was up to + 28 % (SiO2–COH) and + 33 % (MgO–SiO2–COH) at 1 GPa and 800 ∘C and + 9 % (SiO2–COH) at 3 GPa and 800 ∘C in experiments buffered by FMQ buffer. In experiments buffered by NNO at 1 GPa and 800 ∘C the measured increased was + 14 % (SiO2–COH) and + 15 % (MgO–SiO2–COH). Since the run products showed no evidence of hydration and/or carbonation reactions, the observed CO2 increase was attributed to an effect of graphite and silicate dissolution reactions. As a matter of fact, if graphite is present in excess, silicate dissolution can modify the fluid speciation in both systems, SiO2–COH and MgO–SiO2–COH, as a consequence of a decrease in water activity associated with the formation of organic complexes containing Si–O–C and Si–O–Mg bonds.
The combined results from volatile speciation, coupled with mineral dissolution data (see Sect. 3), suggest that the silica component derived from the dissolution of either magnesium silicates (Tiraboschi et al., 2018) or quartz/coesite alone (Tumiati et al., 2017) controls the composition of deep COH fluids in equilibrium with graphite, in particular enhancing their CO2 content when compared to SiO2-free systems due to the polymerized nature of silica at high pressures and temperatures (Newton and Manning, 2009). This effect can be relevant for subduction mélanges, in which silicate minerals and graphite are thought to be abundant and flushed by aqueous fluids, originating from the dehydration of the subducted lithosphere. The dissolution of silicates can boost graphite oxidation in the subduction mélange in the form of volatile CO2 dissolved in COH fluids by up to +30 % compared to silicate-free systems, independently from the occurrence of carbonates. These CO2-rich fluids will interact with the overlying mantle rocks, influencing metasomatic processes, carbonation/decarbonation reactions, and the melting temperatures of rocks in the mantle wedge (Tumiati et al., 2017). The effect of COH fluids on mantle rocks has been also observed in metamorphic blueschist facies rocks from Alpine Corsica and the Western Alps (e.g., Piccoli et al., 2018; Vitale Brovarone et al., 2020), where abundant quartz precipitation in the presence of carbonaceous material and graphite has been attributed to fluid-mediated selective dissolution processes.
Studies on mineral solubility over the last 50 years have been essential to define the total amount of solutes derived from a variety of minerals in equilibrium with different fluids. Experimental constraints on mineral solubility in high-pressure fluids are in fact crucial to assess the mass transport of elements operated by fluids at depth. Most solubility studies have been conducted ex situ, meaning that the fluid is extracted and sampled after quenching the experiment from high-pressure and high-temperature conditions (see Sect. 2). Ex situ experiments have targeted major individual phases representative of the subducted oceanic crust, sediments, and the mantle wedge, including quartz (Manning, 1994), calcite (Caciagli and Manning, 2003; Fein and Walther, 1989), and forsterite (Nakamura and Kushiro, 1974; Newton and Manning, 2002). Experimental data on mineral dissolution in mixed H2O–CO2 fluids are however far more scarce and up to now only available for a few minerals, such as quartz (Newton and Manning, 2000, 2009; Shmulovich et al., 2006; Walther and Orville, 1983), albite, and diopside (Shmulovich et al., 2001). The results of these studies suggest that the presence of CO2 lowers the solute content in the fluid. In the system SiO2–H2O–CO2, mixed fluids show decreasing amounts of SiO2 with increasing content of CO2 in the fluid (i.e., increasing XCO2) and increasing temperatures likely due to the decrease in the activity of water (e.g., Newton and Manning, 2000). However, recent works (Tiraboschi et al., 2018; Tumiati et al., 2017) indicate that in the presence of graphite the amount of solutes increases with increasing temperature and XCO2, suggesting an alternative mechanism for dissolution processes in COH fluids.
To analyze the solubility of quartz in H2O–CO2 mixed fluids, Walther and Orville (1983) developed an extraction quench hydrothermal apparatus. The experiments were performed in cold seal vessels at low-pressure conditions (i.e., 0.2 GPa) and at T < 600 ∘C. Results showed a decrease in quartz solubility with increasing amounts of CO2 in the fluid.
Schneider and Eggler (1986) extracted and collected the solutes from piston cylinder experiments performed at 1.5–2 GPa and 600–1100 ∘C. Solutes were mixed with LiBO2 and fused in graphite capsule at 1000 ∘C for 10 min. The resulting glasses were then analyzed through electron microprobe. The solubility of different types of peridotites (amphibole-, phlogopite-, and clinopyroxene-bearing peridotite) and single minerals in mixed H2O–CO2 fluids were retrieved. Results showed that the addition of 9 mol % of CO2 to the aqueous fluid has a strong effect in depressing the solubility of silicates by approximately 1 order of magnitude.
A modified version of the weight loss technique (Manning, 1994) was employed to determine the activity–composition relations in CO2–H2O solutions (Aranovich and Newton, 1999). The capsule was frozen in liquid nitrogen and punctured with a needle while still frozen. The immediate weight loss was ascribed to CO2 escape. The capsules were then dried and reweighed to retrieve the H2O content. This technique, applied on double capsules, was also used to investigate quartz dissolution in H2O–CO2 fluids at P=0.2–1.5 GPa and T=500–900 ∘C (Newton and Manning, 2000, 2009). The solubility of SiO2 in the fluid decreased strongly with increasing CO2, in agreement with previous experimental data. Similar results were also retrieved by Shmulovich et al. (2001, 2006), which investigated quartz and albite solubilities at 0.9 GPa and 800 ∘C by measuring the weight change in single crystals using the rapid-quench method modified from Manning (1994).
A more recent experimental study by Tiraboschi et al. (2018) showed that the solubility of silicate minerals such as forsterite and enstatite in graphite-saturated H2O–CO2 fluids is significantly higher compared to systems containing only H2O as the volatile component (Newton and Manning, 2002). Solubility experiments were conducted from 1 to 2.1 GPa and 700 to 1200 ∘C using a rocking piston cylinder apparatus. Redox conditions were buffered by NNO employing the double capsule technique (Eugster, 1957; Eugster et al., 1966). The dissolved solute loads were analyzed through a modified version of the cryogenic LA-ICP-MS (laser ablation inductively coupled plasma mass spectrometry) technique (Aerts et al., 2010; Kessel et al., 2004), employed for the first time on redox-buffered COH fluids. The results showed that forsterite + enstatite solubility in GCOH fluids is higher compared to pure water, both in terms of dissolved SiO2 and MgO (Fig. 3). The enhanced solubility in GCOH fluids, compared to pure water was related to the formation of C-, Mg-, and Si-bearing organic complexes, as suggested by thermodynamic calculations applying the DEW model (Sverjensky et al., 2014b). The effect of graphite-saturated COH fluids on the solubility of forsterite and enstatite was extendible to other systems such as SiO2 + GCOH fluid (Tumiati et al., 2017). The measured Si content at 1 GPa and 800 ∘C was lower than quartz solubility in pure water at the same conditions (Manning, 1994). However, the value was much higher than reported solubilities in graphite-free H2O–CO2 fluids with similar XCO2 (Newton and Manning, 2000, 2009) (Fig. 3).
The cryogenic LA-ICP-MS technique was also employed to investigate carbonate dissolution in GCOH fluids. The solubility of magnesite associated with enstatite has been investigated at 1.5 GPa and at temperatures of 800 and 900 ∘C (Tiraboschi et al., 2018). The amount of solutes derived from the dissolution of magnesite + enstatite in a GCOH fluid was comparable to the experimental data from Caciagli and Manning (2003) relative to calcite dissolution in H2O by considering Mg and Si as dissolved cations instead of Ca. Solute amounts for Mg and Ca were observed to be similar, suggesting an analogous behavior for calcite and magnesite at the investigated conditions.
For a comprehensive characterization of GCOH fluids it is pivotal to address also the solid carbon phase in equilibrium with the COH fluid. In experiments, crystalline graphite is employed at pressures ranging from lower-crust to upper-mantle conditions (e.g., Tumiati et al., 2017) to represent ordered carbonaceous materials in subduction zone sedimentary rocks. Other forms of carbon, such as glass-like carbon, can be also employed as a proxy for disordered carbonaceous material (e.g., Tumiati et al., 2020). Glass-like carbon, also known as glassy carbon, is a non-crystalline and non-graphitizing carbon, which will not develop graphite crystals up to 3000 ∘C at room pressure and up to 45 GPa at room temperature (Shiell et al., 2018). This form of amorphous carbon is considered an inert phase which will not react with the experimental assemblages and therefore can also serve as fluid/melt trap (e.g., Van Den Bleeken et al., 2010; Borghini et al., 2018; Dasgupta et al., 2005; Falloon et al., 2008; Robinson et al., 1998; Spandler et al., 2008; Wasylenki et al., 2003).
In principle, carbon saturation in COH fluids can be achieved by adding any carbon solid phases, from crystalline graphite to glassy carbon and diamond. However, one of the assumptions to calculate the volatile speciation of GCOH fluids through conventional thermodynamic modeling (see Sect. 1.1) is that graphite should be perfectly ordered. As a consequence, the volatile speciation of COH fluids in equilibrium with different forms of graphite, such as glass-like carbon, should be experimentally evaluated case by case. Moreover, investigating how different forms of carbon dissolve in aqueous and more complex fluids is fundamental to unravel how organic matter can be mobilized from the subducting slab to the mantle wedge.
Recently, Tumiati et al. (2020) investigated the dissolution of glass-like carbon and crystalline graphite in aqueous fluids at 800 ∘C and pressures of 1 and 3 GPa. Crystalline graphite was employed to represent the behavior of ordered carbon, while glass-like carbon was considered as an analogue for disordered graphitic carbon. Solid carbon was analyzed through scanning electron microscope (SEM), micro-Raman spectroscopy, and synchrotron X-ray diffraction, while GCOH fluids were characterized employing the capsule-piercing QMS technique (Tiraboschi et al., 2016).
At the investigated experimental P–T–fO2 conditions (NNO and FMQ buffers in double capsules), the dominant dissolution product was carbon dioxide, formed by the oxidation of solid carbon. At 1 GPa and 800 ∘C, oxidative dissolution of glass-like carbon produced 16–19 mol % more CO2 than crystalline graphite (Fig. 4). The COH volatile speciation in equilibrium with glass-like carbon consisted in 5.03 mmol of CO2 and 0.89 mmol of H2O at NNO conditions (XCO2=0.85), while in equilibrium with crystalline graphite the generated fluid was 4.87 mmol CO2 and 1.80 mmol H2O (XCO2=0.73). Similarly, COH fluids at FMQ conditions exhibited a difference in XCO2, from 0.80 when in equilibrium with glass-like carbon to 0.67 in equilibrium with crystalline graphite. In contrast, fluids interacting with glass-like carbon at 3 GPa showed only a limited increase in CO2 (XCO2=0.10; NNO) or even a lower CO2 content (XCO2=0.57; FMQ) with respect to fluids interacting with crystalline graphite (XCO2=0.10 for NNO and XCO2=0.74 for FMQ).
The discrepancies in the dissolution behavior were ascribable to differences in the thermodynamic properties of glass-like carbon and crystalline graphite (i.e., higher compressibility of glass-like carbon, differences in Gibbs free energy). As a result, disordered graphitic carbon appeared to be more prone to oxidation relative to ordered crystalline graphite, leading to fluids enriched in CO2 with respect to current estimates. The experimental data indicated that, in the presence of aqueous fluids that flush subducted sediments, the removal of poorly crystalline disordered graphitic carbon is more efficient than that of crystalline graphite (Fig. 5).
This occurs especially at shallow levels of subduction zones, where the difference in free energy between crystalline and disordered graphitic carbon is higher (i.e., +1.7(1) kJ mol−1 at 1 GPa–800 ∘C and +0.51(1) kJ mol−1 at 3 GPa–800 ∘C; see Tumiati et al., 2020) and the availability of poorly organized metastable carbonaceous matter and of aqueous fluids is maximized. The different dissolution susceptibility declines at pressure corresponding to 110 km in depth, where glass-like carbon is thought to be less soluble than crystalline graphite. This seems to be supported by ultra-high-pressure eclogitic and metasedimentary rocks from Cignana Lake in the Western Alps (Frezzotti, 2019; Frezzotti et al., 2014), which show the preservation of nano-crystalline disordered graphitic carbon in micro- and nano-sized diamonds. As glass-like carbon had been synthetized at diamond-stable conditions (i.e., 7.7 GPa and 1000 ∘C) (Yamaoka et al., 2002), further experimental work is vital to evaluate its role at ultra-high-pressure conditions (i.e., > 5 GPa).
The results summarized in this contribution emphasize how pivotal it is to quantitatively assess the volatile speciation in carbon-saturated COH fluid experiments. Even though conventional thermodynamic modeling represents a valuable tool to predict the volatile speciation at certain P, T, and fO2 conditions, care must be taken to extend the calculation to more complex systems.
The presence of silicates in equilibrium with GCOH fluid can significantly modify the speciation of volatiles mainly due to the generation of solute species, leading to significant differences between the calculated and the actual volatile speciation. Nevertheless, the mechanism controlling the solubility of silicate minerals is poorly understood, and experimental in situ confirmation of the formation and stability of the anticipated solute species in COH fluids is still missing. Likewise, the mechanism governing how graphite enhances the solute budget of GCOH fluids should be characterized, especially at conditions relevant to fluid processes in subduction zones, where graphite is a major carbon-bearing species.
The interactions generated by the presence of GCOH fluid in the subduction zone lead to significant modifications in the subduction mélange and in the overlying mantle wedge (Fig. 6), enhancing the amount of CO2 in the fluid and prompting metasomatic processes. Additional constraints are thus required to further calibrate thermodynamic models which also include charged species, such as the DEW model (Sverjensky et al., 2014b), and assess the complex dynamic of subduction zones. Recently, thanks to solubility data on simple and multicomponent systems, the DEW model has been extended (Huang and Sverjensky, 2019) to incorporate new equilibrium constants for aqueous bisilicate anion, silica trimer, silicate complexes of Ca, Fe, Al, and Mg, and formate complexes of Fe and Ca, providing new constraints to model fluid–rock interactions at upper-mantle conditions.
Investigating other carbon-bearing phases, such as carbonates, is another pivotal step in GCOH fluids studies. Carbonates represent a significant source of carbon at lower-crust and upper-mantle conditions (Caciagli and Manning, 2003). Extrapolated thermodynamic data indicate that at 1 GPa and 500 to 750 ∘C the dominant dissolved carbon species is CO2 (Caciagli and Manning, 2003), while at higher pressure conditions the main carbon-carrier species is CO (Pan et al., 2013). Quantitative analyses on the generation of C-bearing fluids would represent a significant step forward in understanding the contribution of carbonate dissolution to the global deep carbon cycle. Similarly, assessing the effect of diamond on COH fluid speciation will bring additional constraints to the carbon cycling at ultra-high-pressure conditions. Eventually, reducing oxygen fugacity conditions should be also evaluated to explore the genesis of CH4-rich fluids and their influence on silicate dissolution.
A joint effort from several geoscience branches and from ex situ and in situ experiments to thermodynamic modeling, assisted by evidence from natural samples, is then pivotal to fully characterize COH fluids and understand their behavior at upper-mantle conditions.
Data sharing is not applicable to this article as no datasets were generated or analyzed for this review.
CT and FM wrote the review. ST supervised the process.
The contact author has declared that neither they nor their co-authors have any competing interests.
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.
Reviews from Vincenzo Stagno and an anonymous reviewer significantly improved the manuscript. Monika Koch-Müller and Elisabetta Rampone are acknowledged for the editorial handling.
This research has been supported by the Ministero dell'Istruzione, dell'Università e della Ricerca (grant no. 2017ZE49E7_002). Carla Tiraboschi has been supported by the Wire fellowship from WWU Münster (Germany).
This paper was edited by Monika Koch-Müller and reviewed by Vincenzo Stagno and one anonymous referee.
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