4.1 Introduction

Carbon (C) occurs in the mantle in its elemental state in the form of graphite and diamond, but also as oxidized compounds that include carbonate minerals and carbonated magmas, as reduced components such as methane and carbide, and as gaseous phases in the C–O–H chemical system. The occurrence of C-bearing phases characterized by different oxidation states reflects magmatic processes occurring in Earth’s interior that link to its oxygenation through space and time.Reference Kasting, Eggler and Raeburn¹ Improving our understanding of the physical and chemical behavior of carbon at extreme conditions sheds light on the type and depth of possible reactions taking place in the interior of Earth and other planets over time and allows the identification of deep carbon reservoirs and mechanisms that move carbon among different reservoirs from the surface to the atmosphere, thereby affecting the total terrestrial budget of carbon ingassing and outgassing.

Carbon occurs in diverse forms depending on surrounding conditions such as pressure, temperature, oxygen fugacity (fO₂), and the availability of chemical elements that are particularly reactive with carbon to form minerals and fluids. Despite the low abundance of carbon within Earth,Reference McDonough and Sun² the stability of C-rich phases in equilibrium with surrounding minerals provides an important geochemical tracer of redox evolution in Earth and other planets, as well as an important economic resource in the form of diamonds.

Knowledge of carbon cycling through the mantle requires an understanding of the stable forms of carbon-bearing phases and their abundance at pressures, temperatures, and fO₂ values that are representative of Earth’s interior. Such information is necessary to identify potential carbon reservoirs and the petrogenetic processes by which carbon may be (re)cycled through the mantle over time, eventually being brought to the surface by magmas and to the atmosphere as dissolved gaseous species.

Accurate estimates of carbon abundance in Earth’s interior are challenging for many reasons, such as the unknown primordial budget of carbon,Reference Marty, Alexander and Raymond³ the low solubility of carbon in the dominant silicate minerals of the upper and lower mantle,Reference Keppler, Wiedenbeck and Shcheka^4–Reference Hayden and Watson⁷ the low modal abundance of accessory carbon-bearing minerals and graphite/diamond in mantle xenoliths, and because magmas occurring at shallow depths are the product of igneous differentiation, magma chamber processes, and degassing. Experimental studies conducted at high pressures and high temperatures help to constrain the initial carbon budget resulting from accretion and core–mantle differentiation processes. These estimates can then be used to determine the amount of carbon in the present-day terrestrial mantle by simulating possible reactions within simplified mantle mineral assemblages that identify the roles of pressure, temperature, and bulk chemistry on carbon speciation.

This chapter addresses fundamental questions about carbon within Earth: At which depths does carbon transform into different phases? How has the redox state of the mantle influenced carbon speciation throughout geological history? Are carbonate minerals more stable than diamonds or CO₂ fluids under certain conditions? Can minerals control the distribution of carbon within the mantle? Answers to these questions reveal how carbon has evolved in the mantle through time and where it may reside in the present-day mantle.

4.2 The Abundance, Speciation, and Extraction of Carbon from the Upper Mantle over Time

Estimates of carbon abundance in Earth’s interior can be made through analysis of mantle rocks sampled as peridotitic and eclogitic xenoliths carried to the surface by successively erupted lavas, combined with experimental investigations of the carbon contents of synthetic liquids and minerals at upper- and lower-mantle pressures and temperatures. Carbon abundance in upper-mantle rock-forming minerals such as olivine, orthopyroxene, clinopyroxene, and garnet in equilibrium with carbonated magmas (Na₂CO₃, Ref. Reference Keppler, Wiedenbeck and Shcheka4; olivine tholeiite with ~4 wt.% CO₂, Ref. Reference Rosenthal, Hauri and Hirschmann5) were shown to be in the range of a few ppm, as also detected in synthetic minerals representative of the transition zone and lower mantle (<1 ppm; Refs. Reference Shcheka, Wiedenbeck, Frost and Keppler6 and Reference Hayden and Watson7). These findings highlight the extreme geochemical incompatibility of carbon and the role of magmas as its main carriers in space and time.

Experimental investigation of carbon solubility in magmas has revealed that most carbon is generally present as molecular CO₂ and CO₃^2– molecules. Their concentrations follow a linear positive trend with pressure and alkali content (K₂O + Na₂O) and show a negative correlation with SiO₂ from alkali basalts to rhyolites and the water content of the melt.Reference Ni and Keppler⁸ Among the diverse suites of effusive products, basaltic lavas that have erupted along mid-ocean ridges have dissolved CO₂ concentrations that are inherited from deep mantle source rock and can therefore be used to estimate the mantle abundance of CO₂. However, due to the low solubility of CO₂ in magmas during ascent and decompression, the possibility of tracking its history from the carbonated source rock to the surface is limited to few known undegassed lavas (e.g. Siqueiros and 2πD43 popping rocks). Using the observed correlation of undegassed CO₂ versus trace elements (e.g. Rb, Ba, and Nb) from olivine-hosted melt inclusions, LeVoyer et al.Reference LeVoyer, Kelley, Cottrell and Hauri⁹ determined a global average CO₂ content of 137 ± 54 ppm, corresponding to an average flux out of mid-ocean ridges (60,864 km length) of 1.8 × 10¹² mol·yr^–1. This estimate pertains to a depleted mantle source, given that the carbon content of the bulk silicate Earth, generally determined from mantle plume-like magmas, is higher, ranging from 500 to 1000 ppm.Reference Marty, Alexander and Raymond³ In addition, the LeVoyer value is higher than the 72 ppm measured from Siqueiros melt inclusions by Saal et al.,Reference Saal, Hauri, Langmuir and Perfit¹⁰ but much lower than the 1300 ± 800 ppm measured in the 1990s by Dixon et al.Reference Dixon, Clague, Wallace and Poreda¹¹ on alkalic Atlantic lavas. Whether these carbon contents reflect those of the primordial mantle strongly depends on the origin of carbon, its initial budget at the time of Earth’s accretion, and the petrological processes capable of mobilizing deep carbon.

Based on recent experimental studies, it was proposed that mantle carbon was inherited at the time of accretion from a Mercury-sized oxidized C-bearing S-rich body, which established the partitioning of carbon between the metallic core and silicate magma ocean during solidification of the terrestrial mantle.Reference Li, Dasgupta, Tsuno, Monteleone and Shimizu¹² An initially delivered carbon content ranging from 700 to 1000 ppm has been proposed for a reduced or S-rich impactor with a mass of 5–30% of Earth in order to match the current carbon concentration in the mantle. The mobilization of this primordial carbon, likely in the form of elemental carbon in Fe(Ni) alloys and CH₄ in the magma ocean as proposed by Li et al.,Reference Li, Dasgupta, Tsuno, Monteleone and Shimizu¹² links to the evolution of the mantle redox state over time. This issue remains controversial, however, and there is still an open debate on the different C species (CH₄, CO₂, and CO) that can be transported by mantle magmas (Ref. Reference Ni and Keppler8 and references therein).

Late addition of oxidized meteoritic bodies and enrichment of the post-core formation mantle in Fe₂O₃ consequent to the loss of Fe to the metallic core have been proposed, among a plethora of other processes, to explain the increase of fO₂ from conditions where C would be stable as diamond and in Fe(Ni) alloys (fO₂ ≈ iron–wüstite buffer (IW) – 2; Refs. Reference Frost, Mann, Asahara and Rubie13 and Reference Scaillet and Gaillard14) to conditions where C⁴⁺ is the dominant species incorporated in carbonate minerals and melts (IW + 1 < fO₂ < IW + 5). Geochemical tracers such as Ce in zircons believed to have crystallized in equilibrium with Hadaean magmasReference Trail, Watson and Tailby¹⁵ and the V/Sc ratio of erupted continental basaltsReference Li and Lee¹⁶ have been used to argue in favor of a constant mantle redox state over the last 4.4 billion years at values where C⁴⁺ is stable, and therefore able to mobilize carbon as CO₂ and/or CO₃^2– dissolved in magmas. In contrast, based on the reconstruction of the mantle redox state over time using the V/Sc ratio of Archean spreading ridge-derived metabasalts, Aulbach and StagnoReference Aulbach and Stagno¹⁷ found that the ambient mantle became gradually more oxidized by ~1.5 log units between ca. 3 Ga and 1.9 Ga, when fO₂ values similar to modern mid-ocean ridge basalts (MORBs) are recorded (Figure 4.1a). Figure 4.1b illustrates how a reduced asthenospheric Archaean mantle expected to host C in the form of diamond (or graphite) and CH₄ becomes more oxidized along a decompression path (Figure 4.1b, red line) as a result of the pressure effect on the equilibrium:Reference Stagno, Ojwang, McCammon and Frost¹⁸

until the local fO₂ at which carbon turns into carbonateReference Stagno and Frost¹⁹ is reached (fayalite–magnetite–quartz buffer (FMQ) – 2 log units; Figure 4.1b, blue line) at ~100 km depth. In Eq. (4.1), Fe³⁺ and Fe²⁺ refer to the ferric and ferrous iron of the bulk peridotite mantle rock, respectively. A similar equilibrium could be written to explain the distribution and fate of other important magmatic volatiles like H₂ and H⁺, N^3– and N₂, and S^2– and S⁶⁺ in igneous systems dominated by Fe-bearing silicates, with dramatic implications for volcanic outgassing and atmospheric composition over time.

Figure 4.1

(a) fO₂ as a function of time calculated from V/Sc of mid-ocean ridge-derived basalts and metabasalts occurring in ophiolites, as orogenic eclogites, or mantle eclogites (data in Aulbach and StagnoReference Aulbach and Stagno¹⁷). fO₂ values were projected to 1 GPa to avoid bias due to deeper onset of partial melting in warmer ancient convecting mantle. Shown for comparison are results for komatiites from Nicklas et al.Reference Nicklas, Puchtel and Ash²⁵ (b) Thermodynamic prediction of the variation in the mantle oxidation state upon decompression, obtained using oxy-thermobarometry for garnet-bearing peridotite.Reference Stagno, Ojwang, McCammon and Frost¹⁸ The graph shows the depth at which melting would occur as soon as 10 ppm C, expected in the Archean convecting mantle and hosted in diamonds, is oxidized to carbonate by the redox reaction shown. A source mantle with 2% Fe₂O₃ would generate a melt at the local temperature corresponding to the solidus of a carbonated peridotite that would have the fO₂ calculated for the igneous protolith of the Lace eclogite suite shown in (a) (after Aulbach and StagnoReference Aulbach and Stagno¹⁷).

At these depths, carbonate–silicate melts are likely to have formed by redox melting of graphite-bearing mantle at the near-constant fO₂ favored by hotter temperatures during the Archaean, until all carbon (~10 ppm in the case of reduced early EarthReference Dasgupta²⁰) was oxidized. Upon further decompression, the Archaean mantle would have continued to become more oxidized until the oxidation state of Archean MORBs, represented by a metabasaltic eclogite suite from Lace in the Kaapvaal craton,Reference Aulbach and Viljoen²¹ is reached below the spreading ridge. Given that redox melting – today as well as in the early mantle – requires the reduction of Fe₂O₃ (i.e. Eq. 4.1), the oxidation state of MORBs does not directly reflect the mantle oxidation state at the source, a concept introduced by Ballhaus and FrostReference Ballhaus and Frost²² in 1994 when they proposed the oxidation of MORBs from a more reduced mantle source due to the coupling between C/carbonate reactions and Fe³⁺/Fe²⁺ variations upon decompression as represented by Eq. (4.1). This was demonstrated in recent experiments where measured fO₂ values of synthetic MORBs appeared different from the fO₂ of the coexisting spinel-bearing peridotite rock source by up to ~3 log units.Reference Sorbadere, Laurenz, Frost, Wenz, Rosenthal, McCammon and Rivard²³ Nevertheless, a gradual increase of Fe³⁺ in the bulk asthenospheric mantle over time has been corroborated by the finding of extremely low Fe³⁺/∑Fe in mantle eclogites, which is not correlated with indices of subsequent melt depletion,Reference Aulbach, Jacob, Cartigny, Stern, Simonetti and Viljoen²⁴ as well as V-based estimates of fO₂ in komatiites, picrites, and basalts of various ages showing a clear trend in the Archaean that levels out at ca. 2 Ga.Reference Nicklas, Puchtel and Ash²⁵

4.3 The Stability of Reduced and Oxidized Forms of Carbon in the Upper Mantle: Continental Lithosphere versus Convective Mantle

Thermodynamic prediction of the stable form of carbon in the upper mantle can be made using oxy-thermobarometry applied to mantle rocks such as peridotites and eclogites based on the relation between the ferric/ferrous iron ratio of minerals such as spinel and garnet and the buffering capacity of the host rocks. The decreasing fO₂ with depth shown in Figure 4.2 links to the volume change of the reactions used as oxy-thermobarometersReference Stagno, Ojwang, McCammon and Frost^18, Reference Stagno, Frost, McCammon, Mohseni and Fei^26, Reference Ballhaus, Berry and Green²⁷ and suggests that the Archaean continental lithospheric mantle down to ~270 km in depth might have equilibrated with elemental carbon in the form of diamond or graphite, plus a small volume of CO₂-bearing melts varying from carbonatitic (Figure 4.2, blue line) to kimberlitic (Figure 4.2, red region) in composition. The fO₂ at which diamond and CO₂-bearing melts can coexist with peridotite and eclogite depends on the effects that temperature (the local geotherm) and the presence of water have on the equilibria:Reference Stagno and Frost^19, Reference Stagno, Frost, McCammon, Mohseni and Fei²⁶

$\begin{array}{ccccccccccc}2{\mathrm{Mg}}_2{\mathrm{Si}}_2{\mathrm{O}}_6& +& \text{CaMg}{\left({\mathrm{CO}}_3\right)}_2& =& {\text{CaMgSi}}_2{\mathrm{O}}_6& +& 2{\mathrm{Mg}}_2{\mathrm{SiO}}_4& +& 2\mathrm{C}& +& 2{\mathrm{O}}_2\\ \text{enstatite}& & \text{dolomite}/\text{melt}& & \text{diopside}& & \text{olivine}& & \text{diamond}& & \end{array}$(4.2)

and

$\begin{array}{ccccccccc}\text{CaMg}{\left({\mathrm{CO}}_3\right)}_2& +& 2{\mathrm{SiO}}_2& =& {\text{CaMgSi}}_2{\mathrm{O}}_6& +& 2\mathrm{C}& +& 2{\mathrm{O}}_2.\\ \text{dolomite}/\text{melt}& & \text{coesite}& & \text{diopside}& & \text{diamond}& & \end{array}$(4.3)

Figure 4.2

Log fO₂ (normalized to the FMQ buffer) determined for peridotitic and eclogitic xenoliths using oxy-thermobarometry for spinel/garnet peridotite and eclogite.Reference Stagno, Ojwang, McCammon and Frost^18, Reference Stagno, Frost, McCammon, Mohseni and Fei^26, Reference Ballhaus, Berry and Green²⁷ The blue curve is the fO₂ calculated for Eq. (4.2) along a cratonic geotherm of 40 mW·m^–2 that defines the stability field between diamond (or graphite) and solid (liquid) carbonate within peridotite rocks. The orange curve indicates where Fe–Ni metallic alloys (with some C) are stable. The green line indicates the fO₂ buffered by Eq. (4.3) (see text).Reference Stagno, Frost, McCammon, Mohseni and Fei^26, Reference Luth³⁵ CO₂-bearing silicate melts are stable at lower fO₂ values than carbonatitic melts in equilibrium with diamantiferous peridotite due to the temperature effect on Eq. (4.1).Reference Stagno, Ojwang, McCammon and Frost¹⁸ The yellow arrow indicates the proposed oxidation state of a convective mantle contaminated by variable volumes of subducted carbonated lithologies.Reference Eguchi and Dasgupta³⁷ DCDD/G = dolomite–coesite–diopside–(diamond/graphite).

A direct sampling of deep carbon phases is represented by diamantiferous peridotite and eclogite of Archaean age (1–3% diamonds in the cratonic lithosphere),Reference Garber²⁸ while the observation of carbonated magmas of mantle origin, although predicted by experimental phase equilibria studies on synthetic carbonated peridotites and eclogites, appears quite rare (about 490 deposits)Reference Woolley and Kjarsgaard²⁹ due to a decreasing trend over time coupled to secular mantle cooling and late-stage fractionation and assimilation processesReference Tappe, Romer, Stracke, Steenfelt, Smart, Muehlenbachs and Torsvik^30, Reference Tappe, Smart, Torsvik, Massuyeau and de Wit³¹ that make these products difficult to identify. The decrease of fO₂ with depth in the case of eclogite is expected to result in carbonate minerals (or fluids) being reduced to diamond during subduction of a carbonated oceanic crust at variable depths through oxidation of coexisting garnet and clinopyroxene mineral phasesReference Stagno, Frost, McCammon, Mohseni and Fei²⁶ depending on the Fe³⁺ of the bulk rock.Reference Stagno, Frost, McCammon, Mohseni and Fei^26, Reference Aulbach, Woodland, Vasilyev, Galvez and Viljoen³²

The Fe(Ni) precipitation curve (Figure 4.2, orange line) marks the fO₂ conditions at which diamonds and Fe(Ni) alloys might coexist, therefore promoting the diffusion of carbon into adjacent metal or the formation of Fe(Ni)C intermetallic compounds depending on the local Fe(Ni)/C ratio.Reference Dasgupta and Hirschmann^33, Reference Rohrbach, Ghosh, Schmidt, Wijbrans and Klemme³⁴

The extent to which the redox state of the continental mantle resembles that of the convective mantle is highly debated. The model proposed in Figure 4.1b is based on conservative estimates in which a bulk silicate Earth compositionReference McDonough and Sun³⁶ is used as an analogue for the asthenospheric mantle. For this case, the convective mantle is predicted to follow an fO₂ trend similar to the one in Figure 4.2 for natural mantle peridotites along a decompression path. This model might apply to a convective early Earth mantle not equilibrated with subducted lithologies. However, correlations between geochemical tracers such as CO₂ versus Nb and Ba measured in modern natural oceanic basalts suggest a different trend. These correlations were used to constrain mixing models of two components: a residual mantle peridotitic partial melt plus graphite-saturated partial melts of subducted lithologies (e.g. pyroxenite, MORB-eclogites, sediments) in different proportions. These models, supported by melting experiments, show that generation of CO₂-rich basalts of up to ~6 wt.% in the melt like those from Atlantic popping rocksReference Eguchi and Dasgupta³⁷ requires the contribution of subduction-related melts originating from partial melting occurring in the carbonate stability field (fO₂ ≥ FMQ – 1; DCDD/G in Figure 4.2) rather than graphite/diamond-saturated sources. This results in a contaminated convective present-day mantle that is more oxidized than the Archaean continental lithospheric mantle (Figure 4.2).

4.4 The Redox State and Speciation of C in the Transition Zone and Lower Mantle

4.4.2 Carbonate Minerals in Earth’s Interior

In contrast to the view that bulk mantle redox conditions are reduced at transition-zone and lower-mantle depths, inclusions hosted in super-deep (sublithospheric) diamonds have also shown the presence of solid carbonates.Reference Brenker^47, Reference Kaminsky, Ryabchikov and Wirth⁴⁸ These observations raise important questions: (1) Do these inclusions reflect local fO₂ heterogeneities of the deep mantle? (2) What transformations do solid carbonates experience to preserve their stability at high pressures and temperatures to act as main carbon hosts? The latter question links to the possibility that the fO₂ of the transition zone and lower mantle could be buffered by an influx of oxidized carbon in the form of solid carbonate, but questions remain as to which carbonates these might be. The speciation of carbon at conditions from the upper to the lower mantle, whether in the form of diamond or carbonate (either liquid or solid), has been a focus of investigations over the last decades. All experimental studies and theoretical calculations suggest that solid carbonates (i.e. the end members CaCO₃, MgCO₃, FeCO₃, and their solid solutions) are stabilized at conditions of Earth’s lower mantle through a series of high-pressure phase transitions that are summarized below. This conclusion is also supported by the observations of extremely low solubility of carbon in deep mantle silicates such as wadsleyite, ringwoodite, bridgmanite, and ferropericlase in experimental studies conducted at high pressures and high temperatures.Reference Shcheka, Wiedenbeck, Frost and Keppler^6, Reference Hayden and Watson⁷

4.4.2.1 Dolomite and Its High-Pressure Polymorphs

It is generally accepted that dolomite, CaMg(CO₃)₂, is the dominant carbonate mineral up to about 4 GPa within simplified CaO–MgO–Al₂O₃–SiO₂ + CO₂ igneous systems, and is then replaced in dominance by magnesite at higher pressures.Reference Hammouda and Keshav⁴⁹ However, both the bulk Ca/(Ca + Mg) ratio of the rock and the presence of a small amount of Fe in the structure that reduces the cation-sized misfit between Ca and Mg may play important roles in stabilizing high-pressure polymorphs at the conditions of Earth’s lower mantle. Upon compression at ambient temperature, the rhombohedral dolomite structure is stable up to 17 GPa.Reference Santillan, Williams and Knittle⁵⁰ Above this pressure, a transition to dolomite-II with triclinic symmetry is observed with no observable volume change. Dolomite-II is stable upon heating to 1500 K;Reference Mao, Armentrout, Rainey, Manning, Dera, Prakapenka and Kavner⁵¹ however, it decomposes between 2000 and 2400 K below 35 GPa to form a mixture of oxides and diamond.Reference Merlini, Crichton, Hanfland, Gemmi, Mueller, Kupenko and Dubrovinsky⁵² Dolomite-II is stable up to 35 GPa, whereupon a second phase transition is observed to triclinic dolomite-III.Reference Mao, Armentrout, Rainey, Manning, Dera, Prakapenka and Kavner^51, Reference Merlini, Crichton, Hanfland, Gemmi, Mueller, Kupenko and Dubrovinsky⁵² Heating dolomite-III above 35 GPa to its melting point without evidence of decomposition demonstrates that dolomite-III can be a stable C-bearing mineral at Earth’s mantle conditions. Theoretical computations indicate that dolomite transforms into a ring-carbonate structure at 115 GPa and 2500°C that features tetrahedrally coordinated carbon and threefold carbonate rings,Reference Merlini⁵³ as shown in Figure 4.3.

Figure 4.3

Crystal structure of dolomite-IV based on experimental single-crystal X-ray data collected in a diamond anvil cell at 115 GPa after annealing at 2500°C. The structure is based on threefold-ring carbonate units, with carbon in tetrahedral coordination.

In a recent experimental study conducted using a laser-heated diamond anvil cell, Dorfman and coauthorsReference Dorfman, Badro, Nabiei, Prakapenka, Cantoni and Gillet⁵⁴ explored chemical reactions occurring at the boundary between dolomite and Fe metal to simulate subducted carbonates penetrating the reduced lower mantle saturated in Fe metal (about 1 wt.%Reference Frost, Liebske, Langenhorst and McCammon³⁸) at ~51–113 GPa and 1800–2400 K. Their results suggest that the MgCO₃ component of subducted crustal dolomite would react with iron metal to form a mixture of diamond + Fe₇C₃ + ferropericlase, while CaCO₃ with a post-aragonite structure would be preserved. This study supports previous experimental observations on the formation of diamond + carbide by reduction of subsolidus carbonates,Reference Palyanov, Bataleva, Sokol, Borzdov, Kupriyanov, Reutsky and Sobolev⁴⁵ and it demonstrates the potential role of dolomite as a deep carbon reservoir. So far, however, its transport to the lower mantle appears limited to exotic Ca-rich, Si-poor thick portions of the oceanic slab, likely related to the subduction of sedimentary lithologies.Reference Liu⁵⁵

4.4.2.2 Deep Carbon Stored as CaCO₃-like Phases

Calcite (the rhombohedral form of CaCO₃) and aragonite (orthorhombic CaCO₃) undergo a series of structural transitions toward denser phases with increasing pressure. Above 15 GPa, a new calcite polymorph, CaCO₃-IV, was discovered that shows stability at least up to 40 GPa.Reference Merlini, Hanfland and Crichton⁵⁶ The density of CaCO₃-IV is higher than aragonite (3.78 g/cm³ at 30.4 GPa), which suggests that it might replace aragonite at intermediate mantle depths.Reference Merlini, Hanfland and Crichton⁵⁶ At pressures of more than ~40 GPa, CaCO₃ undergoes yet another phase transition into a so-called post-aragonite phase.Reference Ono, Kikegawa and Ohishi⁵⁷ Compression to pressures of more than ~100 GPa leads to a different polymorph with a pyroxene-like structure based on CO₄ groups with sp³-hybridized carbon.Reference Ono, Kikegawa and Ohishi^57–Reference Lobanov⁶⁰ Chemical bonding in sp³-carbonates is different from bonding in carbonates based on sp²-hybridized carbon; thus, sp²–sp³ crossover, if it occurs in mantle carbonates, may disrupt the silicate–carbonate chemical equilibrium. To date, however, the geochemical and geophysical consequences of sp²–sp³ transitions are not well understood. It is noteworthy, however, that calcite was found as an inclusion in a sublithospheric diamond,Reference Brenker⁴⁷ confirming its stability in the lower mantle as a potential carbon reservoir and candidate for potential redox reactions through which diamond itself could form.

4.4.2.3 Magnesite and Fe-Bearing Solid Solutions as Deep Carbon Reservoirs

Magnesite and ferro-magnesite solid solutions have been found to occur as inclusions in diamonds that likely originated in Earth’s lower mantle.Reference Kaminsky, Ryabchikov and Wirth⁴⁸ Despite the lack of evidence of siderite inclusions hosted in such super-deep diamonds, the role of iron in the stability of Fe-carbonates appears relevant in the mid-lower mantle, where spin crossover of Fe²⁺ from high spin (HS) to low spin (LS) changes the physical and chemical properties of these carbonates,Reference Cerantola^61–Reference Lobanov, Holtgrewe and Goncharov⁶³ with important implications for their seismic detectability (discussed below).

Magnesite remains stable at up to 100 GPa and 2200 K without decomposition or associated phase transformations.Reference Isshiki⁶⁴ Congruent melting of magnesite was reported between 2100 and 2650 K at pressures between 12 and 84 GPa, whereas decomposition to MgO and diamond was observed only above ~3000 K at similar pressures.Reference Solopova⁶⁵ Isshiki et al.Reference Isshiki⁶⁴ first reported the transformation of magnesite to its high-pressure polymorph, magnesite-II, at ~115 GPa and ~2200 K. Maeda et al.Reference Maeda, Ohtani, Kamada, Sakamaki, Hirao and Ohishi⁶⁶ discussed phase relations in the MgCO₃–SiO₂ system up to 152 GPa and 3100 K. They reported a reaction between MgCO₃ phase II and SiO₂ (CaCl₂-type SiO₂ or seifertite) to form diamond and MgSiO₃ (bridgmanite or post-perovskite) at deep lower-mantle conditions via the following possible reaction:

SiO₂ + MgCO₃ → MgSiO₃ + C + O₂,

${\mathrm{SiO}}_2+{\text{MgCO}}_3\to {\text{MgSiO}}_3+\mathrm{C}+{\mathrm{O}}_2,$(4.4)

indicating that CO₂ dissociates above ~33 GPa and at >1700–1800 K to form diamond plus free oxygen and bridgmanite. These results describe a possible mechanism of formation of super-deep diamond in cold slabs descending into the deep lower mantle resulting from the instability of magnesite phase II in the presence of exotic assemblages.

The physical and chemical properties of Fe-bearing carbonates, such as their density, Fe content, elasticity, and optical properties, may have important geological consequences. Melting of FeCO₃ was investigated experimentally at high pressures and temperatures equal to or above the terrestrial geotherm. Experiments indicate that iron carbonates melt incongruently up to ~70 GPa and at >2000 K to produce a minor quenched Fe³⁺-rich phase and CO₂ in the liquid.Reference Cerantola^67, Reference Kang⁶⁸ At higher pressures and similar temperatures, new carbonates were observed with tetrahedral C₃O₉ rings.Reference Boulard⁶⁹ Merlini et al.Reference Merlini, Hanfland, Salamat, Petitgirard and Müller⁷⁰ reported the transformation of Mg-siderite at pressures and temperatures corresponding to the top of the D´´ layer (i.e. ~135 GPa and ~2650 K), with formation of Mg₂Fe^(III)₂(C₄O₁₃) and a new oxide phase, Fe₁₃O₁₉, thus demonstrating that self-oxidation–reduction reactions can preserve carbonates in Earth’s lower mantle to 2500 km in depth.

When slabs penetrate the lower mantle, redox reactions take place between the hotter outer part of the slab and the surrounding bulk mantle in order to balance the high Fe³⁺ content of bridgmanite (~80% in equilibrium with magnesite and diamonds),Reference Stagno, Tange, Miyajima, McCammon, Irifune and Frost⁷¹ similar to Eq. (4.1). The origin of diamonds in the lower mantle might be therefore linked to redox reactions involving Fe³⁺-bearing minerals, which could also account for the high proportion of ferropericlase in lower-mantle diamond inclusions.Reference McCammon⁷² At greater depths, the high degree of trivalent iron incorporation into high-pressure carbonate structures and iron oxides can influence redox processes in the deep mantle, where changes in fO₂ could be buffered by the activity of carbon (Eq. 4.5) or oxygen (Eq. 4.6) rather than being controlled by charge balance between iron cations.

4FeCO₃ = Fe₄C₃O₁₂ + C,

$4{\text{FeCO}}_3={\mathrm{Fe}}_4{\mathrm{C}}_3{\mathrm{O}}_{12}+\mathrm{C},$(4.5)

8Fe₄C₃O₁₂ = 6 Fe₄C₄O₁₃ + 4 Fe₂O₃ + 3 O₂.

$8{\mathrm{Fe}}_4{\mathrm{C}}_3{\mathrm{O}}_{12}=6{\mathrm{Fe}}_4{\mathrm{C}}_4{\mathrm{O}}_{13}+4{\mathrm{Fe}}_2{\mathrm{O}}_3+3{\mathrm{O}}_2.$(4.6)

4.4.3 Toward Oxy-Thermobarometry of the Deep Mantle and Implications for Carbon Speciation

Through the number of redox reactions that can be written to explore the mechanisms of diamond formation in the transition zone and lower mantle, a fundamental question arises: Is the deep mantle intrinsically buffered by abundant Fe-bearing minerals similarly to the upper mantle? A recent estimate of the deep-mantle redox state was proposed by Kiseeva et al.,Reference Kiseeva⁷³ who measured the ferric iron content of majorite inclusions and developed an oxy-thermobarometer based on the self-redox capacity of majorite as a function of pressure. Figure 4.4 shows the fO₂ values calculated using Eq. (4.7):

Ca₃Al₂Si₃O₁₂ + 4/3 Fe₃Al₂Si₃O₁₂ + 2.5 Mg₄Si₄O₁₂ + O₂ = 2 Ca₃Fe₂Si₃O₁₂ + 10/3 Mg₃Al₂Si₃O₁₂ + 4 SiO₂

$2{\mathrm{Ca}}_3{\mathrm{Al}}_2{\mathrm{Si}}_3{\mathrm{O}}_{12}+4/3{\mathrm{Fe}}_3{\mathrm{Al}}_2{\mathrm{Si}}_3{\mathrm{O}}_{12}+2.5{\mathrm{Mg}}_4{\mathrm{Si}}_4{\mathrm{O}}_{12}+{\mathrm{O}}_2=2{\mathrm{Ca}}_3{\mathrm{Fe}}_2{\mathrm{Si}}_3{\mathrm{O}}_{12}+10/3{\mathrm{Mg}}_3{\mathrm{Al}}_2{\mathrm{Si}}_3{\mathrm{O}}_{12}+4{\mathrm{SiO}}_2,$(4.7)

from majoritic inclusions in super-deep diamonds from the Jagersfontein kimberlite (South Africa).Reference Beyer and Frost⁷⁴ The carbon/carbonate equilibrium bufferReference Stagno, Tange, Miyajima, McCammon, Irifune and Frost⁷¹ refers to experimental measurements of the fO₂ at which diamond and magnesite coexist with transition-zone (wadsleyite/ringwoodite and clino-enstatite) and lower-mantle (bridgmanite and ferropericlase) mineral phases.Reference Stagno, Tange, Miyajima, McCammon, Irifune and Frost⁷¹ The results indicate the heterogeneity of mantle fO₂ in the transition zone, varying from about IW to IW + 3, where the high concentration of Fe³⁺ in majorite (between 8% and 30%) is linearly correlated with pressure and likely related to the oxidizing effect of CO₂-rich fluids rather than FeO disproportionation. This suggests that carbonate is, at least locally, a stable phase in Earth’s deep mantle, stabilized at an fO₂ value about 2 log units above the iron–wüstite buffer. Carbonate could therefore participate in melting processes depending on the local geotherm and promote carbon mobility through the formation of carbonatitic to kimberlitic melts. At higher pressures, ferropericlase and bridgmanite are expected to play major roles in buffering redox conditions through chemical reactions that involve the Fe³⁺-bearing mineral end members. However, the crystal chemistry of these phases has been shown to be extremely complex due to simultaneous element substitution in different sites.Reference Ismailova⁷⁵

Figure 4.4

fO₂ stability of carbon phases at high pressures based on experimental studies,Reference Stagno, Tange, Miyajima, McCammon, Irifune and Frost⁷¹ as well as majorite inclusions in diamondsReference Kiseeva⁷³ and metal-bearing “CLIPPIR” diamonds.Reference Smith, Shirey, Nestola, Bullock, Wang, Richardson and Wang⁴⁰ The blue dashed line indicates the fO₂ values at which diamonds and carbonate (magnesite) are in equilibrium.Reference Stagno, Tange, Miyajima, McCammon, Irifune and Frost⁷¹

4.5 Seismic Detectability of Reduced and Oxidized Carbon in Earth’s Mantle

The presence of carbon within the mantle may be detectable using seismic data. A recent multidisciplinary study conducted by Garber and coauthorsReference Garber²⁸ showed that diamondiferous lithologies may be responsible for elevated shear-wave velocities (V_S; ≥4.7 km/s) detected at 120–150‑km depths in cratonic lithospheric mantle. Diamond and eclogite (known to contain higher concentrations of diamond compared to peridotite)Reference Luth³⁵ are the most likely high-V_S candidates that could explain the observed seismic anomalies, implying the presence of up to about 3 vol.% diamond, depending on the peridotite and eclogite compositions and the local geotherm.

The seismic detectability of carbonates in the upper mantle and transition zone is related primarily to their crystal structure. Sanchez-Valle et al.Reference Sanchez-Valle, Ghosh and Rosa⁷⁶ measured the elastic tensor of Mg_1–xFe_xCO₃ with four compositions extending from pure magnesite to pure siderite using single-crystal Brillouin scattering spectroscopy at ambient conditions. They found that Fe substitution has a negligible effect on the adiabatic bulk modulus, K_S, of Mg–Fe carbonates, whereas the shear modulus, μ, decreases by 34% from MgCO₃ to FeCO₃. They concluded that, based on current seismic resolution (with a threshold of 2%), detection of carbonated regions from seismic velocity contrast would require high carbonate contents (~15 wt.% CO₂) in eclogite and >20 wt.% CO₂ in peridotite. These results are supported by the work of Yang et al.,Reference Yang, Mao, Lin and Prakapenka⁷⁷ who measured the full elastic stiffness tensor of MgCO₃ up to 14 GPa at ambient temperature and up to 750 K at ambient pressure using Brillouin scattering in the diamond anvil cell.

In Fe-bearing carbonates, the pressure-induced splitting of iron 3d energy levels into two leads to the possibility of two different spin configurations for Fe²⁺: (1) the HS state with four unpaired and two paired electrons; and (2) the LS state with six paired electrons. The spin pairing of electrons causes a volume collapse of the iron atomic volume, followed by shrinking of the octahedral site and ultimately of the unit cell. The first experimental observation of the HS–LS transition of Fe²⁺ in siderite was reported by Mattila et al.Reference Mattila⁷⁸ using X-ray emission spectroscopy. They observed the transition to occur at ~50 GPa and at ambient temperature in natural siderite powder. Subsequent experimental and theoretical work provided further evidence of the spin transition in Fe-carbonates at ~45 GPa, as well as insights into how the spin transition affects the physical and chemical properties of carbonates.Reference Shi, Luo, Johansson and Ahuja^79–Reference Weis⁸⁶

The spin transition causes changes in the thermoelastic properties of carbonates and may enhance the seismic detectability of carbon in the lower mantle. Liu et al.Reference Liu, Lin, Mao and Prakapenka⁸⁷ observed anomalous thermoelastic behavior in natural magnesiosiderite at high pressure and high temperature across the spin transition, including a dramatic increase in the thermal expansion coefficient and decreases in the isothermal bulk modulus and the bulk sound velocity by 75% and 50%, respectively. When compared to MgCO₃ at relevant pressure–temperature conditions of subducted slabs, HS magnesiosiderite with 65 mol.% FeCO₃ is approximately 21–23% denser and its unit-cell volume is 2–4% larger, whereas the LS state is 28–29% denser and 2% smaller than end-member magnesite. These results indicate that dense LS ferromagnesite can become more stable than HS ferromagnesite at pressures above ~50 GPa, providing a mechanism for (Mg,Fe)-bearing carbonate to be a major carbon host in the deeper lower mantle. Fu et al.Reference Fu, Yang and Lin⁸⁸ measured the full elastic stiffness tensor of Mg_0.35Fe_0.65CO₃ up to 70 GPa at ambient temperature using Brillouin light scattering and impulsive stimulated light scattering in a diamond anvil cell. They observed a dramatic softening of the C₁₁, C₃₃, C₁₂, and C₁₃ moduli and stiffening of the C₄₄ and C₁₄ moduli across the spin transition in the mixed spin state. Outside the region of the spin transition, they observed a linear increase of all elastic moduli with pressure. Based on their work, mixed spin-state ferromagnesite is expected to exhibit abnormal elasticity in the mid-lower mantle, including a negative Poisson’s ratio and a drastically reduced compressional wave velocity (V_P). Similar results were obtained by Stekiel et al.,Reference Stekiel⁸⁹ who determined the elastic stiffness moduli of FeCO₃ across the spin transition up to 60 GPa and at ambient temperature by inelastic X-ray scattering and density functional theory calculations. Based on calculations employing a pyrolitic mantle model and considering varying amounts of Mg_1–xFe_xCO₃, the presence of magnesioferrite solid solutions changed the V_S more than the V_P. At least 3 vol.% of FeCO₃ would be needed to produce a shear velocity contrast of more than 1% due to the spin transition, and 8 vol.% of Mg_0.85Fe_0.15CO₃ would be needed to produce the same contrast between carbonated and non-carbonated pyrolitic mantle.

Our knowledge of the iron spin state of FeCO₃ is limited to near-room temperature conditions, as probing different electronic structures at combined high pressure–temperature conditions is challenging. Temperature broadens the pressure range of the HS to LS transition, but the depth range over which spin transitions take place remains uncertain (Figure 4.5). In addition, siderite is unstable at greater than ~1500 K (greater than ~40 GPa) and decomposes into iron oxides and C-bearing phases. As a result, FeCO₃ is unlikely to occur in the lower mantle at depths greater than ~1200 km. Instead, solid solutions involving iron oxides and sp³-bonded novel Fe-carbonates (Fe₄C₄O₁₃ and Fe₄C₃O₁₂) may be the most common carbon-bearing phases at sufficiently oxidizing conditions.

Figure 4.5

Stability and spin-state diagram of FeCO₃ at high pressure–temperature. Mixed blue–red circles depict the spin transition pressure in siderite at 300 K as observed in a soft pressure medium (e.g. Ne) at 40.5 GPa and in more rigid media (KCl, Ar, etc.) at ~44 GPa. Pink and blue regions are high and low spin-state regions, respectively. The pressure–temperature conditions of mixed-spin iron (0.1–0.9 LS) in FeCO₃ are uncertain (shown by different green-shaded areas). High-temperature transformations in the FeCO₃ system are shown after Cerantola et al.Reference Cerantola⁶⁷

4.6 Conclusion

In contrast to the immobile behavior of carbon in the Archaean lithospheric mantle, the deep carbon cycle in modern Earth linked with carbon transport through the convective mantle at varying pressure–temperature–fO₂ conditions over time shows evidence of large heterogeneities in mantle redox state, both vertically and laterally, which likely result from the contribution of subducted lithologies with varying degrees of oxidation through space and time. We conclude that the movement of carbon over geologic time is fundamentally controlled by the level of oxygenation of Earth’s interior, which causes elemental carbon to oxidize to CO₂-bearing magmas, whose rheology mainly controls their transport properties.Reference Kono^91, Reference Stagno, Stopponi, Kono, Manning and Irifune⁹² The observation of both oxidized carbon and metal trapped as inclusions in sublithospheric diamonds testifies to the heterogeneity of mantle fO₂, thereby implying the stability of carbon in various redox states and phases (mineral, melt, or fluid), and even favored by the presence of additional elements like sulfur. The relation between iron oxidation state in mineral inclusions in diamonds and fO₂ is an important tool for determining the local redox conditions needed to model carbon speciation. Fluids in equilibrium with reduced mantle regions would be methane dominated and may precipitate diamonds by reduction of Fe, liberating water that could induce partial melting. On the other hand, the possible presence of carbonate as a source of carbon in natural diamond-forming processes is supported by experimental studies at high pressure and temperature that demonstrate the stability of diverse geologically relevant carbonates (and their solid solutions) such as magnesite, calcite/aragonite, and siderite down to the lower mantle. Redox reactions of these carbonates with Fe-bearing minerals in the bulk mantle under initially reducing conditions have been demonstrated to promote the formation of diamond as well as the crystallization of carbide phases, leading to mantle oxidation. Such “conditioned” mantle regions may eventually allow carbonated melts and fluids to be mobilized along ascending (plumes) or descending (slabs) redox fronts, facilitating melt-mediated carbon transfer between different terrestrial reservoirs. Finally, elemental carbon transported upwards in upwelling mantle regions will be subjected to redox melting upon oxidation due to decompression. The resulting carbonated melts eventually erupt at the surface, where they interact with the hydrosphere and atmosphere. Figure 4.6 summarizes the stability of different carbon species through space and (indirectly) time with a particular focus on the asthenospheric mantle, the continental lithosphere, and subducted slabs.

Figure 4.6

Simplified cartoon showing the distribution and forms of carbon inside Earth. Carbon has low solubility in mantle minerals;Reference Keppler, Wiedenbeck and Shcheka^4–Reference Hayden and Watson⁷ hence, it occurs primarily in the form of gas (red circles), fluids or melts (orange circles), and accessory solid phases (green circles), including diamonds (octahedra). Reactions involving carbon include redox melting (diamond consuming) and freezing (diamond producing),Reference Aulbach and Stagno^17, Reference Stagno, Ojwang, McCammon and Frost¹⁸ reduction of carbonate to diamond,Reference Stagno, Frost, McCammon, Mohseni and Fei^26, Reference Aulbach, Woodland, Vasilyev, Galvez and Viljoen³² growth of diamond from metallic liquids,Reference Dasgupta and Hirschmann^33, Reference Rohrbach, Ghosh, Schmidt, Wijbrans and Klemme^34, Reference Smith, Shirey, Nestola, Bullock, Wang, Richardson and Wang^40, Reference Tsuno and Dasgupta⁴⁶ breakdown of carbonate under reduced conditions,Reference Palyanov, Bataleva, Sokol, Borzdov, Kupriyanov, Reutsky and Sobolev^45, Reference Dorfman, Badro, Nabiei, Prakapenka, Cantoni and Gillet^54, Reference Maeda, Ohtani, Kamada, Sakamaki, Hirao and Ohishi⁶⁶ redox reactions that produce tetracarbonates,Reference Cerantola^67, Reference Boulard⁶⁹ and reactions between carbonate and silicate.Reference Maeda, Ohtani, Kamada, Sakamaki, Hirao and Ohishi^66, Reference Stagno, Tange, Miyajima, McCammon, Irifune and Frost⁷¹ Numbers indicate the depth at which important phase transitions in carbonates have been proposed to occur: (1) calcite to aragonite,Reference Hammouda and Keshav⁴⁹ (2) dolomite to dolomite-II,Reference Santillan, Williams and Knittle^50, Reference Merlini, Crichton, Hanfland, Gemmi, Mueller, Kupenko and Dubrovinsky⁵² (3) aragonite to post-aragonite,Reference Ono, Kikegawa and Ohishi⁵⁷ (4) dolomite-II to dolomite-III,Reference Mao, Armentrout, Rainey, Manning, Dera, Prakapenka and Kavner^51, Reference Merlini, Crichton, Hanfland, Gemmi, Mueller, Kupenko and Dubrovinsky⁵² (5) Fe-carbonate to Fe-tetracarbonate,Reference Cerantola^67, Reference Boulard⁶⁹ (6) post-aragonite to CaCO₃ with sp³-hybridized carbon,Reference Ono, Kikegawa and Ohishi^57–Reference Lobanov⁶⁰ and (7) magnesite to magnesite-II.Reference Isshiki⁶⁴ Ferrous iron in carbonate undergoes a HS to LS transition in the mid-mantle.Reference Mattila^78–Reference Müller, Efthimiopoulos, Jahn and Koch-Müller⁹⁰ The thickness of the crust and slab is vertically exaggerated for clarity.

4.7 Limits to Knowledge and Unknowns

Although great advances have been made, important limits to knowledge remain regarding the stability and mobility of carbon-bearing phases and their interaction with silicates and metals at pressure–temperature–fO₂ conditions relevant to the deep Earth. Redox melting and freezing reactions, as a function of fO₂, are critical in mediating transitions between the relatively refractory forms of carbon, such as diamond/graphite, carbide, and metal alloys, to highly mobile oxidized forms, such as carbonated melts and CO₂-bearing fluids.Reference Stagno, Ojwang, McCammon and Frost^18, Reference Frost and McCammon^93, Reference Rohrbach and Schmidt⁹⁴ However, the amount of carbon involved in these reactions, the participating minerals, and the fO₂ in the mantle with depth and through time remain highly uncertain. This uncertainty arises because most of our knowledge relies on indirect estimates based on mostly degassed magmas and direct estimates from mantle xenoliths and diamonds entrained in magmas that are irregularly distributed in space and time. Moreover, mantle xenoliths and diamonds are exclusively or dominantly derived from the lithospheric mantle and may sample multiply reactivated fluid and melt pathways that are not representative of the lithospheric mantle and even less so of the convective mantle.Reference O’Reilly and Griffin⁹⁵ The few sublithospheric diamonds available for study sample anomalous mantle domains characterized by strong compositional and redox gradients at the interface between deeply subducted slabs and ambient mantle.Reference Frost and McCammon^93, Reference Foley⁹⁶ Thus, although it is assumed that the fO₂ of the metal-saturated mantle below ~250–300 km in depth is effectively buffered close to the iron–wüstite redox buffer (where carbonates and carbonated melts are unstableReference Rohrbach and Schmidt⁹⁴), sublithospheric diamonds appear to record much higher fO₂ values, linked to the influx of slab-derived oxidizing agents.Reference Kiseeva⁷³ In addition, the CO₂ content of oceanic basalts has been suggested to require carbonated redox melting rather than graphite-saturated melting, implying higher fO₂ values than are inferred from lithospheric mantle xenoliths.Reference Eguchi and Dasgupta³⁷ The problem of constraining the dominant fO₂ and redox equilibria with depth is only exacerbated in deep time, where debate over appropriate sample material and redox proxies continues.Reference Trail, Watson and Tailby^15–Reference Aulbach and Stagno^17, Reference Litasov, Shatskiy, Kono and Sanloup⁹⁸

Progress on deciphering the speciation and distribution of carbon in modern Earth’s interior will be made by combining observations from experiments and theoretical studies with increasingly sophisticated remote-sensing tools. For example, the ponded products of redox melting may be increasingly traceable by geophysics due to the increasingly well-characterized melting relations of carbon-bearing mantleReference Sakamaki, Kono and Sanloup⁹⁹ and constraints on the physical properties of carbonated melts (e.g. viscosity, seismic velocity, and electrical conductivity),Reference Kono^91, Reference Stagno, Stopponi, Kono, Manning and Irifune^92, Reference Litasov, Shatskiy, Kono and Sanloup⁹⁸ and they have indeed been linked to low-velocity zones below the oceanic lithosphere.Reference Sifre’, Gardes, Massuyeau, Hashim, Hier-Majumder and Gaillard¹⁰⁰ The fate of carbonates in subducting slabs, however, remains poorly constrained, in part due to the unknown variation of mantle fO₂ with depth and time. Carbonates do show rich polymorphism at high-pressure, high-temperature conditions, which renders them stable along the geotherm. Therefore, studies that explore the interaction of carbonates with silicates at well-controlled pressure, temperature, and redox conditions will provide important insights into the survival and mobility of oxidized carbon species in the mantle. Recent advances in experimental design that allow fO₂ to be controlled and monitored at deep mantle pressuresReference Stagno, Tange, Miyajima, McCammon, Irifune and Frost^71, Reference Rohrbach and Schmidt⁹⁴ will enable the stabilities of various carbonate minerals to be mapped out as a function of depth for complex systems, combined with their predicted seismic velocities based on their crystal structure.Reference Sanchez-Valle, Ghosh and Rosa⁷⁶ Future improvements in the sensitivity of remote-sensing tools and data processing may allow deep carbonated mantle regions to be detected. Recent studies indicate that Fe-bearing carbonates show remarkably complex chemical and physical behavior at mid-lower mantle depths. The Fe spin transition may shift the chemical equilibrium in favor of Fe-rich carbonates, which in turn would significantly affect their physical properties, with potential implications for carbonate seismic detectability. However, the relevant depth range of spin transitions is not well constrained because of the immense technological challenge of probing spin transitions at combined high-pressure, high-temperature conditions. The iron oxides, oxygen, and elemental carbon that may be produced during reactions that take place when carbonate is transported to the deep mantle may also affect redox conditions and have important (but as yet unexplored) geological consequences.

Acknowledgments

VS acknowledges financial support from the Deep Carbon Observatory and Sapienza University of Rome through “Fondi di Ateneo.” SA is grateful for funding from the German Research Foundation (DFG) under grant AU 356/10. Thoughtful comments by the reviewer Arno Rohrbach and the editor Rajdeep Dasgupta helped to improve the quality of this chapter.

Questions for the Classroom