Steel rusts by water and air on the Earth’s surface. But what about deep inside the Earth’s interior?
The Earth’s core is the largest carbon storage on Earth – roughly 90% is buried there. Scientists have shown that the oceanic crust that sits on top of tectonic plates and falls into the interior (in a process called subduction) contains hydrous minerals and can sometimes descend all the way to the core-mantle boundary.
The temperature at the core-mantle boundary is at least twice as hot as lava, and high enough that water can be released from the hydrous minerals. Therefore, a chemical reaction similar to rusting steel could occur at Earth’s core-mantle boundary.
Byeongkwan Ko, a recent Arizona State University (ASU) Ph.D. graduate, and his collaborators have been conducting experiments at the U.S. Department of Energy’s Advanced Photon Source (APS) at Argonne National Laboratory, where they compressed iron-carbon alloy and water together to the pressure and temperature expected for Earth’s core-mantle boundary, melting the iron-carbon alloy, and carried out in situ x-ray diffraction experiments at the GeoSoilEnviroCARS 13-ID-D x-ray beamline of the APS.
The team found that water and metal react and make iron oxides and iron hydroxides, just like rusting at Earth’s surface. However, they found that for the conditions of the core-mantle boundary, unlike rusting at Earth’s surface, carbon comes out of the liquid iron metal alloy and forms diamond (Fig. 1).
Ko and his team published their findings in a paper in the journal Geophysical Research Letters.
“Temperature at the boundary between the silicate mantle and the metallic core at 3,000 km depth reaches to (about 7,000 degrees Fahrenheit), which is sufficiently high for most minerals to lose H2O captured in their atomic-scale structures,” says Dan Shim, a professor at ASU's School of Earth and Space Exploration and a co-author on the paper. “In fact, the temperature is high enough that some minerals should melt at such conditions.”
Because carbon is an iron-loving element, significant carbon is expected to exist in the core, while the mantle is thought to have relatively low carbon. However, scientists have found that much more carbon exists in the mantle than expected.
“At the pressures expected for the Earth's core-mantle boundary, hydrogen alloying with iron metal liquid appears to reduce solubility of other light elements in the core. Therefore, solubility of carbon, which likely exists in the Earth's core, decreases locally where hydrogen enters into the core from the mantle (through dehydration),” Shim said. “The stable form of carbon at the pressure-temperature conditions of the Earth's core-mantle boundary is diamond. So, the carbon escaping from the liquid outer core would become diamond when it enters into the mantle.”
“Carbon is an essential element for life and plays an important role in many geological processes. The new discovery of a carbon transfer mechanism from the core to the mantle will shed light on the understanding of the carbon cycle in the Earth’s deep interior,” Ko says. “This is even more exciting given that the diamond formation at the core-mantle boundary might have been going on for billions of years since the initiation of subduction on the planet.”
Ko's new study shows that carbon leaking from the core into the mantle by this diamond formation process may supply enough carbon to explain the elevated carbon amounts in the mantle. Ko and his collaborators also predicted that diamond-rich structures can exist at the core-mantle boundary and that seismic studies might detect the structures because seismic waves should travel unusually fast for the structures.
“The reason that seismic waves should propagate exceptionally fast through diamond-rich structures at the core-mantle boundary is because diamond is extremely incompressible and less dense than other materials at the core-mantle boundary,” Shim says.
Ko and his team will continue investigating how the reaction can also change the concentration of the other light elements in the core, such as silicon, sulfur and oxygen, and how such changes can impact the mineralogy of the deep mantle.
See: Byeongkwan Ko1‡*, Stella Chariton2, Vitali Prakapenka2, Bin Chen3, Edward J. Garnero1, Mingming Li1, and Sang-Heon Shim1**, “Water-Induced Diamond Formation at Earth's Core-Mantle Boundary,” Geophys. Res. Lett. 49, e2022GL098271 (2022). DOI: 10.1029/2022GL098271
Author affiliations: 1Arizona State University, 2The University of Chicago, 3University of Hawaii at Manoa ‡Present address Michigan State University,
Correspondence: * kobyeong@msu.edu, ** sshm5@asu.edu
This work has been supported by National Science Foundation (NSF) EAR-CSEDI-1855624 and EAR-1921298 and the National Aeronautics and Space Administration (NASA) Exoplanet 80NSSC18K0353. B. Chen acknowledges the support from NSF grants EAR-1555388 and EAR-2127807. GeoSoilEnviroCARS is supported by the National Science Foundation (NSF)—Earth Sciences (EAR-1634415). This research used resources of the Advanced Photon Source, a U.S. Department of Energy (DOE) Office of Science user facility operated for the DOE Office of Science by Argonne National Laboratory under Contract No. DE-AC02-06CH11357.
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