Editorial: Deep Carbon Science

Department of Geosciences, University of Rhode Island, Kingston, RI, United States, Center for Space and Habitability (CSH), University of Bern, Bern, Switzerland, Univ Lyon, Univ Lyon 1, ENSL, CNRS, LGL-TPE, Villeurbanne, France, Faculty of Environmental Science and Engineering, Babes-Bolyai University, Cluj-Napoca, Romania, Department of Physics and Geology, University of Perugia, Perugia, Italy, School of Earth and Environmental Sciences, University of St Andrews, St Andrews, United Kingdom, Department of Earth Sciences, Franklin College of Arts and Sciences, University of Georgia, Athens, GA, United States, Earth Byte Group, School of Geosciences, The University of Sydney, Darlington, NSW, Australia

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 volcanically-forced climate change, using the Paleocene-Eocene thermal maximum as a case study; the calculated relaxation time is ∼50,000 years. 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 1,400°C in the presence of O 2 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 H 2 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, United States, 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.

AUTHOR CONTRIBUTIONS
DC drafted a first version of this editorial. All authors contributed to and approved the final version.