Abbreviation | DCO |
---|---|
Formation | 2009 |
Purpose | Transforming our understanding of carbon in Earth's interior |
Membership | 957 scientists from 47 countries (as of January 2017) [1] |
Website | "deepcarbon.science". |
The Deep Carbon Observatory (DCO) is a global research program designed to transform understanding of carbon's role in Earth. DCO is a community of scientists, including biologists, physicists, geoscientists and chemists, whose work crosses several traditional disciplinary lines to develop the new, integrative field of deep carbon science. To complement this research, the DCO's infrastructure includes public engagement and education, online and offline community support, innovative data management, and novel instrumentation development. [2]
In December 2018, researchers announced that considerable amounts of life forms, including 70% of bacteria and archea on Earth, comprising up to 23 billion tonnes of carbon, live up to at least 4.8 km (3.0 mi) deep underground, including 2.5 km (1.6 mi) below the seabed, according to a ten-year Deep Carbon Observatory project. [3] [4] [5]
In 2007, Robert Hazen, a Senior Staff Scientist at the Carnegie Institution’s Geophysical Laboratory (Washington, DC) spoke at the Century Club in New York, on the origins of life on Earth and how geophysical reactions may have played a critical role in the development of life on Earth. Jesse Ausubel, a faculty member at Rockefeller University and Program Director at the Alfred P. Sloan Foundation, was in attendance and later sought out Hazen's book, Genesis: The Scientific Quest for Life’s Origins.
After two years of planning and collaboration, Hazen and colleagues officially launched the Deep Carbon Observatory (DCO) in August 2009, with its secretariat based at the Geophysical Laboratory of the Carnegie Institution of Washington, DC. Hazen and Ausubel, along with input from over 100 scientists invited to participate in the Deep Carbon Cycle Workshop in 2008, expanded their original idea. No longer focused solely on the origin of life on Earth, the group instead clarified their position to further human understanding of Earth, carbon, that critical element, had to take center stage. [2]
The Deep Carbon Observatory's research considers the global carbon cycle beyond Earth's surface. It explores high-pressure and extreme temperature organic synthesis, complex interactions between organic molecules and minerals, conducts field observations of deep microbial ecosystems and of anomalies in petroleum geochemistry, and constructs theoretical models of lower crust and upper mantle carbon sources and sinks.
The Deep Carbon Observatory is structured around four science communities focused on the topics of reservoirs and fluxes, deep life, deep energy, and extreme physics and chemistry.
The Reservoirs and Fluxes Community explores the storage and transport of carbon in Earth's deep interior. The subduction of tectonic plates and volcanic outgassing are primary vehicles for carbon fluxes to and from deep Earth, but the processes and rates of these fluxes, as well as their variation throughout Earth's history, remain poorly understood. In addition DCO research on primitive chondritic meteorites indicates that Earth is relatively depleted in highly volatile elements compared to chondrites, though DCO's research is further examining whether large reservoirs of carbon may be hidden in the mantle and core. Members of the Reservoirs and Fluxes Community are conducting research as a part of the Deep Earth Carbon Degassing Project to make tangible advances towards quantifying the amount of carbon outgassed from the Earth's deep interior (core, mantle, crust) into the surface environment (e.g. biosphere, hydrosphere, cryosphere, atmosphere) through naturally occurring processes.
The Deep Life Community documents the extreme limits and global extent of subsurface life in our planet, exploring the evolutionary and functional diversity of Earth's deep biosphere and its interaction with the carbon cycle. The Deep Life Community maps the abundance and diversity of subsurface marine and continental microorganisms in time and space as a function of their genomic and biogeochemical properties, and their interactions with deep carbon.
By integrating in situ and in vitro assessments of biomolecules and cells, the Deep Life Community explores the environmental limits to the survival, metabolism and reproduction of deep life. The resulting data informs experiments and models that study the impact of deep life on the carbon cycle, and the deep biosphere's relation to the surface world. [6] Members of the Deep Life Community are conducting research as a part of the Census of Deep Life, which seeks to identify the diversity and distribution of microbial life in continental and marine deep subsurface environments and to explore mechanisms that govern microbial evolution and dispersal in the deep biosphere. [7]
In December 2018, researchers announced that considerable amounts of life forms, including 70% of bacteria and archea on Earth, comprising up to 23 billion tonnes of carbon, live up to at least 4.8 km (3.0 mi) deep underground, including 2.5 km (1.6 mi) below the seabed, according to a ten-year Deep Carbon Observatory project. [3] [4] [5]
The Deep Energy Community is dedicated to quantifying the environmental conditions and processes from the molecular to the global scale that control the origins, forms, quantities and movements of reduced carbon compounds derived from deep carbon through deep geologic time. The Deep Energy Community uses field-based investigations of approximately 25 globally representative terrestrial and marine environments to determine processes controlling the origin, form, quantities and movements of abiotic gases and organic species in Earth's crust and uppermost mantle. Deep Energy also uses DCO-sponsored instrumentation, especially revolutionary isotopologue measurements, to discriminate between the abiotic and biotic methane gas and organic species sampled from global terrestrial and marine field sites. Another research activity of Deep Energy is to quantify the mechanisms and rates of fluid-rock interactions that produce abiotic hydrogen and organic compounds as a function of temperature, pressure, fluid and solid compositions. [8]
As a result of a series of workshops, the DCO initiated an additional Science Community to examine the physics and chemistry of carbon under extreme conditions. The overarching goal of the Extreme Physics and Chemistry Community is to improve the understanding of the physical and chemical behavior of carbon at extreme conditions, as found in the deep interiors of Earth and other planets. Extreme Physics and chemistry research explores thermodynamics of carbon-bearing systems, chemical kinetics of chemical deep carbon processes, high-pressure biology and biophysics, physical properties of aqueous fluids, theoretical modeling for carbon and its compounds at high pressures and temperatures, and solid-fluid interactions under extreme conditions. The Extreme Physics and Chemistry Community also seeks to identify possible new carbon-bearing materials in Earth and planetary interiors, to characterize the properties of these materials and to identify reactions at conditions relevant to Earth and planetary interiors. [9]
As the DCO nears its completion in 2020, it is integrating the discoveries made by its research communities into an overarching model of carbon in Earth, as well as other models and products aimed at both the scientific community and wider public. [10]
Research highlights to date include:
Carbon in Earth is Volume 75 of Reviews in Mineralogy and Geochemistry (RiMG). It was released as an open access publication on March 11, 2013. Each chapter of Carbon in Earth synthesizes what is known about deep carbon, and also outlines unanswered questions that will guide future DCO research. [19] The Deep Carbon Observatory encourages open access publication, and is striving to become a leader in Earth sciences in this regard. DCO funding can be used to defray the costs of open access publication. [20]
Recent advances in data generation techniques lead to increasingly complex data. At the same time, science and engineering disciplines are rapidly becoming more and more data driven with the ultimate aim of better understanding and modeling the dynamics of complex systems. However complex data requires integration of information and knowledge across multiple scales and spanning traditional disciplinary boundaries. Significant advances in methods, tools and applications for data science and informatics over the last five years can now be applied to multi- and inter-disciplinary problem areas. Given these challenges, it is clear that each DCO Research Community faces diverse data science and data management needs to fulfill both their overarching objectives and their day-to-day tasks. The Deep Carbon Observatory Data Science Team handles the data science and data management needs for each DCO program and for the DCO as a whole, using a combination of informatics methods, use case development, requirements analysis, inventories and interviews. [21]
A list of some of the scientists involved in the Deep Carbon Observatory:
On 11 April 2020, the Australian Broadcasting Corporation's Science Show broadcast a 37 minute radio documentary on the DCO. [22]
The carbon cycle is that part of the biogeochemical cycle by which carbon is exchanged among the biosphere, pedosphere, geosphere, hydrosphere, and atmosphere of Earth. Other major biogeochemical cycles include the nitrogen cycle and the water cycle. Carbon is the main component of biological compounds as well as a major component of many minerals such as limestone. The carbon cycle comprises a sequence of events that are key to making Earth capable of sustaining life. It describes the movement of carbon as it is recycled and reused throughout the biosphere, as well as long-term processes of carbon sequestration (storage) to and release from carbon sinks.
Geomicrobiology is the scientific field at the intersection of geology and microbiology and is a major subfield of geobiology. It concerns the role of microbes on geological and geochemical processes and effects of minerals and metals to microbial growth, activity and survival. Such interactions occur in the geosphere, the atmosphere and the hydrosphere. Geomicrobiology studies microorganisms that are driving the Earth's biogeochemical cycles, mediating mineral precipitation and dissolution, and sorbing and concentrating metals. The applications include for example bioremediation, mining, climate change mitigation and public drinking water supplies.
A biogeochemical cycle, or more generally a cycle of matter, is the movement and transformation of chemical elements and compounds between living organisms, the atmosphere, and the Earth's crust. Major biogeochemical cycles include the carbon cycle, the nitrogen cycle and the water cycle. In each cycle, the chemical element or molecule is transformed and cycled by living organisms and through various geological forms and reservoirs, including the atmosphere, the soil and the oceans. It can be thought of as the pathway by which a chemical substance cycles the biotic compartment and the abiotic compartments of Earth. The biotic compartment is the biosphere and the abiotic compartments are the atmosphere, lithosphere and hydrosphere.
Isotope geochemistry is an aspect of geology based upon the study of natural variations in the relative abundances of isotopes of various elements. Variations in isotopic abundance are measured by isotope-ratio mass spectrometry, and can reveal information about the ages and origins of rock, air or water bodies, or processes of mixing between them.
Crustal recycling is a tectonic process by which surface material from the lithosphere is recycled into the mantle by subduction erosion or delamination. The subducting slabs carry volatile compounds and water into the mantle, as well as crustal material with an isotopic signature different from that of primitive mantle. Identification of this crustal signature in mantle-derived rocks is proof of crustal recycling.
Katrina Jane Edwards was a pioneering geomicrobiologist known for her studies of organisms living below the ocean floor, specifically exploring the interactions between the microbes and their geological surroundings, and how global processes were influenced by these interactions. She spearheaded the Center for Dark Energy Biosphere Investigation (C-DEBI) project at the University of Southern California, which is ongoing. Edwards also helped organize the deep biosphere research community by heading the Fe-Oxidizing Microbial Observatory Project on Loihi Seamount, and serving on several program steering committees involving ocean drilling. Edwards taught at the Woods Hole Oceanographic Institution (WHOI) and later became a professor at the University of Southern California.[1][2]
The Carbon Mineral Challenge is a citizen science project dedicated to accelerating the discovery of carbon-bearing minerals. The program launched in 2015 December with sponsorship from the Deep Carbon Observatory. The project ended in 2019 September, with 31 new carbon-bearing minerals found from 27 locations.
The Deep Earth Carbon Degassing (DECADE) project is an initiative to unite scientists around the world to make tangible advances towards quantifying the amount of carbon outgassed from the Earth's deep interior into the surface environment through naturally occurring processes. DECADE is an initiative within the Deep Carbon Observatory (DCO).
Marine biogeochemical cycles are biogeochemical cycles that occur within marine environments, that is, in the saltwater of seas or oceans or the brackish water of coastal estuaries. These biogeochemical cycles are the pathways chemical substances and elements move through within the marine environment. In addition, substances and elements can be imported into or exported from the marine environment. These imports and exports can occur as exchanges with the atmosphere above, the ocean floor below, or as runoff from the land.
Craig E. Manning is a professor of geology and geochemistry in the Department of Earth, Planetary, and Space Sciences at the University of California, Los Angeles, where he served as department chair between 2009 and 2012. Manning's research interests include water chemistry, thermodynamics, gas chemistry, geochemistry, igneous petrology, and metamorphic petrology.
Dimitri Alexander Sverjensky is a professor in Earth and Planetary Sciences at Johns Hopkins University where his research is focused on geochemistry.
Matthew Schrenk is an associate professor in geomicrobiology at Michigan State University. His research focuses on the diversity, distribution, and activities of microorganisms in the deep subsurface biosphere. His work couples molecular biological approaches and geochemical analyses to investigate microbial ecosystems. Schrenk investigates high pH environments fueled by underground serpentinization reactions between water and certain rock types and hydrothermal vent systems along the ocean floor that are driven by volcanic activity.
Mark Alexander Lever is a microbial ecologist and biogeochemist who studies the role of microorganisms in the global carbon cycle. He is a professor of biogeochemistry and geobiology at the Marine Science Institute of the University of Texas at Austin.
The geochemistry of carbon is the study of the transformations involving the element carbon within the systems of the Earth. To a large extent this study is organic geochemistry, but it also includes the very important carbon dioxide. Carbon is transformed by life, and moves between the major phases of the Earth, including the water bodies, atmosphere, and the rocky parts. Carbon is important in the formation of organic mineral deposits, such as coal, petroleum or natural gas. Most carbon is cycled through the atmosphere into living organisms and then respirated back into the atmosphere. However an important part of the carbon cycle involves the trapping of living matter into sediments. The carbon then becomes part of a sedimentary rock when lithification happens. Human technology or natural processes such as weathering, or underground life or water can return the carbon from sedimentary rocks to the atmosphere. From that point it can be transformed in the rock cycle into metamorphic rocks, or melted into igneous rocks. Carbon can return to the surface of the Earth by volcanoes or via uplift in tectonic processes. Carbon is returned to the atmosphere via volcanic gases. Carbon undergoes transformation in the mantle under pressure to diamond and other minerals, and also exists in the Earth's outer core in solution with iron, and may also be present in the inner core.
Mineral evolution is a recent hypothesis that provides historical context to mineralogy. It postulates that mineralogy on planets and moons becomes increasingly complex as a result of changes in the physical, chemical and biological environment. In the Solar System, the number of mineral species has grown from about a dozen to over 5400 as a result of three processes: separation and concentration of elements; greater ranges of temperature and pressure coupled with the action of volatiles; and new chemical pathways provided by living organisms.
Isabelle Daniel is a mineralogist at the Claude Bernard University Lyon 1 in Lyon, France. She studies minerals under extreme conditions, such as those that exist in Earth's mantle, as well as biosignatures of early life.
The deep carbon cycle is geochemical cycle (movement) of carbon through the Earth's mantle and core. It forms part of the carbon cycle and is intimately connected to the movement of carbon in the Earth's surface and atmosphere. By returning carbon to the deep Earth, it plays a critical role in maintaining the terrestrial conditions necessary for life to exist. Without it, carbon would accumulate in the atmosphere, reaching extremely high concentrations over long periods of time.
The deep biosphere is the part of the biosphere that resides below the first few meters of the surface. It extends down at least 5 kilometers below the continental surface and 10.5 kilometers below the sea surface, at temperatures that may reach beyond 120 °C (248 °F) which is comparable to the maximum temperature where a metabolically active organism has been found. It includes all three domains of life and the genetic diversity rivals that on the surface.
Peter H. Barry is an American geochemist who is an associate scientist in the marine chemistry and geochemistry department at the Woods Hole Oceanographic Institution. He uses noble gases and stable isotopes to understand the volatile history and chemical evolution of Earth, including the dynamic processes of subduction, mantle convection and surface volcanism, which control the redistribution of chemical constituents between the crust and mantle reservoirs. Barry’s main research focus has been on high-temperature geochemistry, crust-mantle interactions and the behavior of volatile fluids in the lithosphere. He also studies crustal systems, the origin of high helium deposits, including hydrocarbon formation and transport mechanisms.
Bénédicte Menez is a French geomicrobiologist and university professor in Earth Sciences at the Institut de Physique du Globe de Paris. In 2012, she received the Irène Joliot-Curie Prize in the “Young Female Scientist” category for her work.
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