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Editorial12 November 2020
Editorial: Deep Carbon Science

reconstructions, and highlight CO2 fluxes from continental rift settings post-Pangea. The volcanic flux of CO2 has been successfully reconstructed by direct study of CO2 flux through lakes and adjacent soils (Hughes et al., 2019), an important and often overlooked CO2 valve linking lithosphere, atmosphere, and hydrosphere. From perspectives rooted deeper in the tectonic system, the important roles that serpentinites play in the carbon cycle are evaluated in two senses: (1) serpentinite as a carbon vector to the deep mantle (Merdith et al., 2019), and (2) serpentine mud volcanoes as sites of carbon mobilization through organic acid release (Eickenbusch et al., 2019), in a Mariana Trench case study.The physical properties of carbonaceous melt migration and chemical exchange are experimentally examined as reduced metallic melts (Dong et al, 2019) and oxidized carbonate melts (Sanloup et al., 2019note corrigendum). Regarding carbon-bearing metallic melts in the mid-mantle, Dong et al. (2019) apply experimental data to predict immobility of metallic carbon, meaning deep Fe-C melts will remain isolated. experimentally determine the viscosity of Fe-carbonate melt (FeCO3) in the mid-to lower-mantle, and find that such melts are polymerized and highly viscous, not readily reacting in the lower mantle. Both studies show deep carbon to be immobile and unreactive, under the very specific conditions of their experimental designs.Linking geological and biological aspects of carbon cycling reveal emerging challenges. The drawdown of atmospheric carbon into rock reservoirs is examined through the lens of Urey reactions and the efficiency of carbon deposition in the continental crust reservoir (Kellogg et al., 2019); the authors argue that carbon stored in Earth's continental crust could have been extracted either from the early atmosphere or from the mantle (over a longer period of time)--or both. Kellogg et al. (2019) challenge the community to prioritize better constraints on the concentration of carbon in the atmosphere and continental crust over geologic time. Their work also addresses the recovery (relaxation time) of Earth's climate to volcanicallyforced climate change, using the Paleocene-Eocene thermal maximum as a case study; the calculated relaxation time is ~50,000 yrs. This timeframe is certainly of modern concern, given anthropogenic injections of carbon into the atmosphere.Shales are known to be large carbon sinks in low pressure settings. Basu et al. (2019) ask whether shales can retain significant carbon during low pressure-temperature and high pressure-temperature processes during the subduction of Earth's crust. In a custom-built high vacuum line, they incrementally heat shale samples from 200 to 1400°C in the presence of O2 gas and record the carbon and nitrogen abundances, δ 13 C values, and the atomic C/N ratios for the gas at each stage of heating. Basu et al. (2019) propose that carbon silicate minerals, biomineralized and/or occluded, can be efficiently retained as a refractory phase and transferred into Earth's mantle through subduction.The important role of serpentinization is emphasized in this context also: Barbier et al. (2020) offer a detailed review of hydrogen, methane, and hydrocarbon formation through experimental serpentinization, informed by network analysis. The relevance of the frequently invoked Fischer-Tropsch-type (FTT) reactions to produce methane from the abiotic reduction of oxidized carbon by H2 is questioned. Barbier et al. (2020) follow the forms and movement of carbon through the near ubiquitous, extensive serpentinization process, operating beneath most past and present seabeds.Carbon cycling mediated by the deep biosphere is tracked also, in terms of function, detection, and novel findings. The Deep Mine Microbial Observatory in South Dakota, USA, described by Osburn et al. (2019), is a stable portal to the continental deep subsurface, with a rich, initial database on which future studies can pivot. In the marine realm, Cario et al. (2019) offer a perspective on the state of the science exploring the deep biosphere beneath the seabed. Aspects of the growth and resilience of subseafloor crustal biofilms are documented (Ramirez et al., 2019), and methods enabling new discernment of virus abundance in the subseafloor sedimentary blanket are shared (Pan et al., 2019). A new serpentinite-influenced organism, Petrocella atlantisensis, cultured from Atlantis Massif oceanic core complex rocks sampled during IODP Expedition 357 is described, observed at controlled hydrostatic pressure (Quemeneur et al., 2019).The findings reported in Deep Carbon Science underscore the need for multidisciplinary commitment to open questions related to Earth's carbon cycle. It is clear that the processes driven by, and driving, plate tectonics buffer the carbon fluxes on which life has been dependent for billions of years (e.g., fluctuations in atmosphere-ocean geochemistry). Important work includes methodical application of current techniques, but much work requires new ways of thinking: multifaceted investigations that connect the deep and shallow biospheres, and/or describe links between the whole biosphere and points of contact with geosphere have the potential to transform our thinking. The breadth of disciplines and scientific approaches collated in Deep Carbon Science provides exciting insight into a future where the traditional boundaries of classic disciplines become blurred. This, we argue, is the only way to reveal the true nature and extent of carbon cycle phenomena that are both vast and diminutive, slow yet fast, known but inaccessible, and everywhere all at once.

2,950 views

Exploring Carbon Mineral Systems: Recent Advances in C Mineral Evolution, Mineral Ecology, and Network Analysis
REVIEW
27 August 2020
Exploring Carbon Mineral Systems: Recent Advances in C Mineral Evolution, Mineral Ecology, and Network Analysis
Shaunna M. Morrison, 17 more and Robert M. Hazen
Large and growing data resources on the spatial and temporal diversity and distribution of the more than 400 carbon-bearing mineral species reveal patterns of mineral evolution and ecology. Recent advances in analytical and visualization techniques leverage these data and are propelling mineralogy from a largely descriptive field into one of prediction within complex, integrated, multidimensional systems. These discoveries include: (1) systematic changes in the character of carbon minerals and their networks of coexisting species through deep time; (2) improved statistical predictions of the number and types of carbon minerals that occur on Earth but are yet to be discovered and described; and (3) a range of proposed and ongoing studies related to the quantification of network structures and trends, relation of mineral ‘natural kinds’ to their genetic environments, prediction of the location of mineral species across the globe, examination of the tectonic drivers of mineralization through deep time, quantification of preservational and sampling bias in the mineralogical record, and characterization of feedback relationships between minerals and geochemical environments with microbial populations. These aspects of Earth’s carbon mineralogy underscore the complex co-evolution of the geosphere and biosphere and highlight the possibility for scientific discovery in Earth and planetary systems.

22,202 views

48 citations

ORIGINAL RESEARCH
19 November 2019
Stability of Organic Carbon Components in Shale: Implications for Carbon Cycle
Sudeshna Basu, 3 more and Anne-Lise Jourdan

5,305 views

19 citations

ORIGINAL RESEARCH
1 November 2019
On the Role of the Urey Reaction in Extracting Carbon From the Earth's Atmosphere and Adding It to the Continental Crust
Louise H. Kellogg, 1 more and Harsha Lokavarapu

10,968 views

6 citations

Understanding Degassing Pathways Along the 1886 Tarawera (New Zealand) Volcanic Fissure by Combining Soil and Lake CO2 Fluxes
The 1886 eruption of Tarawera, New Zealand, produced a ~17 km long fissure across the Tarawera Volcanic Complex (TVC), Lake Rotomahana (LR), and the Waimangu Geothermal System (WGS). We combine new soil CO2 flux and isotope measurements of TVC with previous data from LR and WGS to fingerprint the CO2 source, understand the current pathways for degassing, and quantify the CO2 released along the entire fissure. The total CO2 emissions from the fissure are 1227 t·d-1 (742–3398 t·d-1). The CO2 flux from WGS and LR is far higher than from TVC (>549 vs. ~4 t·d-1 CO2), likely influenced by a shallow silicic body at depth and caldera rim faults increasing permeability at the southern end of the fissure. Highly localised regions of high CO2 flux occur along the fissure and are likely caused by cross-cutting faults that focus the flow. One of these areas occurs in the TVC, which is emitting ~1 t·d-1 CO2 with a δ13CO2 of -5.5 ± 0.5 ‰, and comparison with previous observations shows that activity is declining over time. Future CO2 flux surveys could be compared to this baseline survey to understand changes in volcanic activity.

17,740 views

15 citations

Carbon is a key control on the surface chemistry and climate of Earth. Significant volumes of carbon are input to the oceans and atmosphere from deep Earth in the form of degassed CO2 and are returned to large carbon reservoirs in the mantle via subduction or burial. Different tectonic settings (e.g. volcanic arcs, mid-ocean ridges, and continental rifts) emit fluxes of CO2 that are temporally and spatially variable, and together they represent a first-order control on carbon outgassing from the deep Earth. Changes in the relative importance of different tectonic settings throughout Earth's history has therefore played a key role in balancing the deep carbon cycle on geological timescales. Over the past ten years the Deep Carbon Observatory has made enormous progress in constraining estimates of carbon outgassing flux at different tectonic settings. Using plate boundary evolution modelling and our understanding of present-day carbon fluxes, we develop time series of carbon fluxes into and out of the Earth’s interior through the past 200 million years. We highlight the increasing importance of carbonate-intersecting subduction zones over time to carbon outgassing, and the possible dominance of carbon outgassing at continental rift zones, which leads to maxima in outgassing at 130 and 15 Ma. To a first-order, carbon outgassing since 200 Ma may be net positive, averaging ~50 Mt C yr-1 more than the ingassing flux at subduction zones. Our net outgassing curve is poorly correlated with atmospheric CO2, implying that surface carbon cycling processes play a significant role in modulating carbon concentrations and/or there is a long-term crustal or lithospheric storage of carbon which modulates the outgassing flux. Our results highlight the large uncertainties that exist in reconstructing the corresponding in- and outgassing fluxes of carbon. Our synthesis summarizes our current understanding of fluxes at tectonic settings and their influence on atmospheric CO2, and provides a framework for future research into Earth’s deep carbon cycling, both today and in the past.

27,974 views

85 citations

Origin of Short-Chain Organic Acids in Serpentinite Mud Volcanoes of the Mariana Convergent Margin
ORIGINAL RESEARCH
26 July 2019
Origin of Short-Chain Organic Acids in Serpentinite Mud Volcanoes of the Mariana Convergent Margin
Philip Eickenbusch, 11 more and Mark Alexander Lever
Serpentinitic systems are potential habitats for microbial life due to frequently high concentrations of microbial energy substrates, such as hydrogen (H2), methane (CH4), and short-chain organic acids (SCOAs). Yet, many serpentinitic systems are also physiologically challenging environments due to highly alkaline conditions (pH>10) and elevated temperatures (>80C). To elucidate the possibility of microbial life in deep serpentinitic crustal environments, International Ocean Discovery Program (IODP) Expedition 366 drilled into the Yinazao, Fantangisña and Asùt Tesoru serpentinite mud volcanoes on the Mariana Forearc. These mud volcanoes differ in temperature (80, 150, 250C, respectively) of the underlying subducting slab, and in the porewater pH (11.0, 11.2, 12.5, respectively) of the serpentinite mud. Increases in formate and acetate concentrations across the three mud volcanoes, which are positively correlated with temperature in the subducting slab and coincide with strong increases in H2 concentrations, indicate a serpentinization-related origin. Thermodynamic calculations suggest that formate is produced by equilibrium reactions with dissolved inorganic carbon (DIC) + H2, and that equilibration continues during fluid ascent at temperatures below 80C. By contrast, the mechanism(s) of acetate production are not clear. Besides formate, acetate, and H2 data, we present concentrations of other SCOAs, methane, carbon monoxide, and sulfate, δ13C-data on bulk carbon pools, and microbial cell counts. Even though calculations indicate a wide range of microbial catabolic reactions to be thermodynamically favorable, concentration profiles of potential energy substrates and very low cell numbers suggest that microbial life is scarce or absent. We discuss the potential roles of temperature, pH, pressure, and dispersal in limiting the occurrence of microbial life in deep serpentinitic environments.

8,503 views

35 citations