Elsevier

Chemical Geology

Volume 586, 30 December 2021, 120500
Chemical Geology

Mass-independent fractionation of oxygen isotopes during thermal decomposition of divalent metal carbonates: Crystallographic influence, potential mechanism and cosmochemical significance

https://doi.org/10.1016/j.chemgeo.2021.120500Get rights and content

Abstract

Few physical or chemical processes defy well-established laws of mass-dependent isotopic fractionation. A surprising example, discovered two decades ago, is that thermal decomposition of calcium and magnesium carbonate minerals (conducted in vacuo, to minimise back-reaction and isotopic exchange) causes the oxygen triple-isotope compositions of the resulting solid oxide and CO2 to fit on parallel mass-dependent fractionation lines in ln(1 + δ17O) versus ln(1 + δ18O) space, with anomalous depletion of 17O in the solid and equivalent enrichment of 17O in the CO2. By investigating the thermal decomposition of other natural divalent metal carbonates and one synthetic example, under similar conditions, we find that the unusual isotope effect occurs in all cases and that the magnitude of the anomaly (Δ′17O) seems to depend on the room temperature crystallographic structure of the carbonate. A lower cation coordination number (as associated with smaller cation radius) correlates with a Δ′17O value closer to zero. Local symmetry considerations may therefore be influential. Relative to a reference fractionation line of slope 0.524 and passing through VSMOW, solid oxides produced by thermal decomposition of orthorhombic carbonates were characterised by Δ′17O = −0.367 ± 0.004‰ (standard error). The comparable figure from rhombohedral examples was −0.317 ± 0.010‰, whereas from the sole monoclinic (synthesised) specimen it was −0.219 ± 0.011‰. The numerical values are, to some extent, dependent on details of the experimental procedure. We discuss potential origins of the isotopic anomaly, including the possibility of hyperfine coupling between 17O nuclei and unpaired electrons of transient radicals (the ‘magnetic isotope effect’). A new mechanism based on the latter process is proposed. The associated transition state is compatible with that suggested by recent quantum chemical and kinetic studies of the thermal decompositions of calcite and magnesite. An earlier suggestion based on the magnetic isotope effect is shown to be incompatible with the generation of a 17O anomaly, regardless of the identity of the carbonate. We cannot exclude the possibility that a Fermi resonance between states leading to dissociation may additionally affect the magnitude of Δ′17O in some cases. Our findings have cosmochemical implications, with thermal processing of carbonates providing a potential mechanism for the mass-independent fractionation of oxygen isotopes in protoplanetary systems.

Introduction

With few – though important – exceptions, chemical or physical processes that modify oxygen stable isotope distributions in nature, whether under equilibrium conditions or by kinetic mechanisms, cause the 17O/16O ratio to change by approximately half the corresponding change in 18O/16O. This is related to the mass difference between 17O and 16O (1.0042 Da) being approximately half that between 18O and 16O (2.0042 Da). Isotope ratio modifications that follow this pattern of proportionality are usually referred to as ‘mass-dependent’ fractionations and are described by well-established laws (Urey, 1947; Bigeleisen and Goeppert-Mayer, 1947; Bigeleisen and Wolfsberg, 1957; Young et al., 2002; Dauphas and Schauble, 2016). In contrast, Thiemens and Heidenreich (1983) reported that ozone generated by electrical discharge in molecular oxygen deviates from this relationship, with the 17O/16O and 18O/16O ratios changing by an equal amount. Since this discovery of a chemically produced ‘mass independent’ (or ‘non-mass-dependent’) isotope effect, several other examples have been documented, usually involving gas phase photochemistry. These include the reaction of CO with the ∙OH radical in Earth's atmosphere (Huff and Thiemens, 1998; Röckmann et al., 1998); photodissociation of CO2 (Bhattacharya et al., 2000) and of CO (Chakraborty et al., 2012). The occurrence of mass independent isotope effects in nature provides useful tracers and insights to the present and past atmosphere, climate and even the origin of life (Thiemens, 2013; Thiemens and Lin, 2019, Thiemens and Lin, 2021).

Surprisingly, thermal decomposition of calcium and magnesium carbonates is also associated with mass-independent fractionation of the oxygen isotopes (Miller et al., 2002), if the decomposition is conducted under vacuum, to minimise the potential for back-reaction and isotopic exchange between the resulting solid oxide and CO2. Anomalous depletion of 17O in the solid oxide is accompanied by a corresponding enrichment of 17O in the CO2. No generally accepted explanation for this finding has since been proposed. Here, we report an investigation of whether the unusual fractionation pattern occurs during thermal decomposition of other anhydrous divalent metal carbonates and consider whether the magnitude of the isotopic anomaly relates to specific characteristics of the individual carbonates. Most of the empirical data were obtained shortly after the initial report, but have not been published hitherto. Some years later, we also tested a hypothesis based on a hyperfine coupling mechanism (proposed and subsequently published by Buchachenko, 2013) for explaining the experimental findings. Although that test and its outcome were mentioned at a conference (Miller et al., 2012), no data were reported in the abstract; neither have they been published since. We therefore present the details here, together with the (also hitherto unpublished) oxygen triple-isotope measurements of oxides from thermal decomposition of eight different divalent carbonate minerals, for comparison with the Ca and Mg examples reported by Miller et al. (2002).

On the basis of the Buchachenko (2013) mechanism, details of which are discussed below (Section 5.6), all divalent metal carbonates would be expected to exhibit mass-independent fractionation of the oxygen isotopes during the thermal decomposition process, unless the corresponding cation in the univalent state contains no unpaired electrons. In this case, the intermediate cannot be a radical pair and therefore its reactions are not spin-state selective. Because Cu+ has electronic configuration [Ar]3d10, a definitive empirical test of the hypothesis was to perform controlled thermal decomposition of CuCO3 in vacuo and measure the oxygen triple-isotope compositions of the resulting CuO and CO2. If the proposed mechanism is correct, no 17O anomaly would be produced.

Unfortunately, CuCO3 does not occur in nature. The first reliable synthesis – from heating the hydroxycarbonate minerals azurite and malachite at 500 ± 10 °C for approximately 21 h duration in CO2 atmosphere at 20 ± 1 kb pressure – was reported by Ehrhardt et al. (1973), with the structure being published the following year (Seidel et al., 1974). CuCO3 is a grey, monoclinic crystalline solid (space group Pa-C2S, cation coordination number 5), reputedly stable in dry air at room temperature for several months. To conduct the experimental test, it was therefore necessary to first prepare a small quantity (~20 mg) of CuCO3, based on the Ehrhardt et al. (1973) procedure.

Section snippets

Definitions and notation

Measurements of oxygen triple-isotope ratios are, by convention, reported as δ17O and δ18O values relative to a specific reference material, usually Vienna Standard Mean Ocean Water (VSMOW). With 17R and 18R as the abundances of the respective minor isotopes relative to the 16O abundance, then by definition:δO=17RsampleRreference1717Rreference17andδO=18RsampleRreference1818Rreference18

Because the magnitudes of the dimensionless quantities δ17O and δ18O are << 1 in natural systems, their

Samples

Apart from CuCO3, which was synthesised for this investigation, most of the single carbonate mineral specimens used in this study were supplied by the Natural History Museum, London. Sample details are given in Table 1. The use of natural samples ensured that the relationship between the 17O/16O and 18O/16O ratios would conform to mass-dependent norms, prior to the commencement of thermal decomposition. Oxygen triple-isotope characterisation of carbonates at high precision (to ~10 ppm or better

Oxides formed from the rhombohedral and orthorhombic carbonates

A compilation of the oxygen triple-isotope data from this investigation is provided in Table 2. From the respective mean values of replicate measurements of the ten solid oxides produced by thermal decomposition of the natural anhydrous carbonates, a linear array of slope 0.5243 ± 0.0011 (standard error) can be derived in 103ln(1 + δ17O) versus 103ln(1 + δ18O) space, with ordinate intercept of −0.343 ± 0.023 relative to VSMOW, as shown in Fig. 1. The slope of the array is in accord with

Relationship between Δ′17O of the metal oxides and crystallographic structure of the parent carbonate

Despite the variability between replicate Δ′17O measurements of individual metal oxides, there appears to be an association between the respective mean Δ′17O values and whether the parent carbonate has a rhombohedral, orthorhombic or monoclinic structure (at room temperature). This is illustrated in Fig. 5, with cation radius data from Shannon (1976). The carbonate structural type, which controls the cation coordination number, is determined by the cation radius. A rhombohedral structure is

Conclusions

We have demonstrated that anomalous fractionation of 17O/16O relative to 18O/16O occurs during the thermal decomposition of all (eleven) divalent metal carbonate examples investigated, regardless of the cation identity. The magnitude of the anomaly, quantified as Δ′17O, ranged from −0.20‰ to −0.43‰ in individual samples of solid oxide, when λRL is assigned as 0.524 and when a protracted, controlled heating protocol was utilised. The exact magnitude of the anomaly is dependent on the

Declaration of Competing Interest

The authors declare that they have no known competing financial interests or personal relationships that could have appeared to influence the work reported in this paper.

Acknowledgements

JRW identified the hitherto unrecognised problem with the Buchachenko (2013) mechanism and devised the alternative hypothesis presented in this paper (Sections 5.6, 5.7 and Fig. 7, Fig. 8, Fig. 9). The idea that Fermi resonance might be involved in the unusual isotope effect was suggested to MFM by John R. Hulston (lead author of Hulston and Thode, 1965, cited in the text). MFM is indebted to Open University colleagues Jenny M. Gibson for laboratory assistance and Andy G. Tindle for electron

References (93)

  • M.F. Miller

    Isotopic fractionation and the quantification of 17O anomalies in the oxygen three-isotope system: an appraisal and geochemical significance

    Geochim. Cosmochim. Acta

    (2002)
  • M.F. Miller et al.

    Standardizing the reporting of Δ′17O data from high precision oxygen triple-isotope ratio measurements of silicate rocks and minerals

    Chem. Geol.

    (2020)
  • D. Rumble et al.

    Oxygen three-isotope fractionation lines in terrestrial silicate minerals: an inter-laboratory comparison of hydrothermal quartz and eclogitic garnet

    Geochim. Cosmochim. Acta

    (2007)
  • T. Sharma et al.

    Measurement of O18/O16 ratios of total oxygen of carbonates

    Geochim. Cosmochim. Acta

    (1965)
  • J.A.G. Wostbrock et al.

    An internally consistent triple oxygen isotope calibration of standards for silicates, carbonates and air relative to VSMOW2 and SLAP2

    Chem. Geol.

    (2020)
  • E.D. Young et al.

    Kinetic and equilibrium mass-dependent isotope fractionation laws in nature and their geochemical and cosmochemical significance

    Geochim. Cosmochim. Acta

    (2002)
  • S.M. Antao et al.

    The orthorhombic structure of CaCO3, SrCO3, PbCO3 and CaCO3: linear structural trends

    The Canadian Mineral.

    (2009)
  • I. Arvanitidis et al.

    A study of the thermal decomposition of BaCO3

    Metall. Mater. Trans. B

    (1996)
  • M. Basire et al.

    Fermi resonance in CO2: mode assignment and quantum nuclear effects from first principles molecular dynamics

    J. Chem. Phys.

    (2017)
  • S.K. Bhattacharya et al.

    New evidence for symmetry dependent isotope effects: O + CO reaction

    Z. Naturforsch.

    (1989)
  • S.K. Bhattacharya et al.

    A new class of oxygen isotopic fractionation in photodissociation of carbon dioxide: potential implications for atmospheres of Mars and Earth

    Geophys. Res. Lett.

    (2000)
  • J. Bigeleisen et al.

    Calculation of equilibrium constants for isotopic exchange reactions

    J. Chem. Phys.

    (1947)
  • J. Bigeleisen et al.

    Theoretical and experimental aspects of isotope effects in chemical kinetics

    Adv. Chem. Phys.

    (1957)
  • C. Blondel et al.

    Electron affinities of 16O, 17O, 18O, the fine structure of 16O and the hyperfine structure of 17O

    Phys. Rev. A

    (2001)
  • A.L. Buchachenko

    Mass-independent isotope effects

    J. Phys. Chem. B

    (2013)
  • A. Buchachenko

    Magnetic isotopes as a means to elucidate Earth and environmental chemistry

    Russ. Chem. Rev.

    (2018)
  • A. Buchachenko et al.

    New possibilities for magnetic control of chemical and biochemical reactions

    Acc. Chem. Res.

    (2017)
  • A.L. Buchachenko et al.

    Isotope enrichment induced by magnetic interactions in chemical reactions

    Dokl. Akad. Nauk SSSR

    (1976)
  • P. Cartigny et al.

    On the mass independent fractionations of O, Hg, Si, Mg and Cd during open system evaporation or thermal decomposition. Sixth Internatnl. Symp. Isotopomers (ISI 2012)

    (2012)
  • C. Ceccarelli et al.

    Discovery of calcite in the solar type protostar NGC 1333-IRAS4

    Astron. Astrophys.

    (2002)
  • S. Chakraborty et al.

    Experimental test of self-shielding in vacuum ultraviolet photodissociation of CO

    Science

    (2012)
  • A. Chiavassa et al.

    The 90–110 mm dust features in low to intermediate mass protostars: calcite?

    Astron. Astrophys.

    (2005)
  • M. Chiesa et al.

    Carbon dioxide activation by surface excess electrons: an EPR study of the CO2 radical ion adsorbed on the surface of MgO

    Chem. Eur. J.

    (2007)
  • R.N. Clayton et al.

    Kinetic isotope effects in oxygen in the laboratory dehydration of magnesian minerals

    J. Phys. Chem. A

    (2009)
  • T.B. Coplen et al.

    Comparison of stable isotope reference samples

    Nature

    (1983)
  • R.T. Cygan et al.

    Atomistic models of carbonate minerals: bulk and surface structures, defects, and diffusion

    Mol. Simul.

    (2002)
  • N. Dauphas et al.

    Mass fractionation laws, mass-independent effects, and isotopic anomalies

    Annu. Rev. Earth Planet. Sci.

    (2016)
  • H. Ehrhardt et al.

    Hochdrucksynthese von Kupfer(II)-Carbonat

    Z. Naturforsch.

    (1973)
  • J. Farquhar et al.

    Atmosphere-surface interactions on Mars: Δ17O measurements of carbonate from ALH 84001

    Science

    (1998)
  • D.K. Fisler et al.

    Diffusion of Ca and Mg in calcite

    Am. Mineral.

    (1999)
  • D.K. Fisler et al.

    A shell model for the simulation of rhombohedral carbonate minerals and their point defects

    Amer. Mineral.

    (2000)
  • B.R. Fosu et al.

    Technical note: Developments and applications in triple oxygen isotope analysis of carbonates

    ACS Earth Space Chem.

    (2020)
  • I.A. Franchi et al.

    The oxygen-isotopic composition of Earth and Mars

    Meteorit. Planet. Sci.

    (1999)
  • P. Gillet et al.

    Raman spectroscopic studies of carbonates. Part I: High-pressure and high-temperature behaviour of calcite, magnesite, dolomite and aragonite

    Phys. Chem. Miner.

    (1993)
  • D.M. Goldin et al.

    On the dissociation mechanism of carbonates and their isomorphous mixture

    J. Therm. Anal.

    (1984)
  • R. Haberkorn et al.

    Isotope effects in interstellar molecules by chemical hyperfine interaction

    Astron. Astrophys.

    (1977)
  • Cited by (5)

    1

    Present address: Department of Chemical Engineering, Imperial College London, Imperial College Road, Kensington, London SW7 2AZ, UK

    View full text