Naukowcy znajdują rdzę i diamenty na granicach warstwy jądra Ziemi.
Na powierzchni Ziemi stal rdzewieje pod wpływem wody i powietrza. Ale co z głębinami wnętrza ziemi?
Największym zasobem węgla na Ziemi jest jądro Ziemi, w którym zakopane jest 90% węgla. Naukowcy wykazali, że skorupa oceaniczna, która znajduje się na płytach tektonicznych i opada w głąb lądu, zawiera uwodnione minerały i czasami może osiągnąć granicę między jądrem a płaszczem. Na granicy jądra i płaszcza temperatura jest co najmniej dwa razy wyższa niż lawy i jest wystarczająco wysoka, aby woda mogła uciec z uwodnionych minerałów. W rezultacie w pobliżu granicy płaszcza Ziemi może zachodzić reakcja chemiczna podobna do rdzewienia stali.
Byungkwan-koo, niedawno doktorant wyjście z Uniwersytet Stanu Arizona, a koledzy niedawno donieśli o swoich odkryciach na granicy między rdzeniem a płaszczem w czasopiśmie Geophysical Research Letters. Przeprowadzili eksperymenty z zaawansowanym źródłem fotonów w Narodowe Laboratorium ArgonneI ciśnienie i woda grzewcza oraz żelazko węglowe[{” attribute=””>alloy to conditions similar to those at the Earth’s core-mantle boundary, melting the iron-carbon alloy.
The scientists discovered that water and metal react to form iron oxides and iron hydroxides, just like rusting on Earth’s surface. However, they observed that at the core-mantle boundary conditions, carbon separates from the liquid iron-metal alloy and forms diamonds.
“Temperature at the boundary between the silicate mantle and the metallic core at 3,000 km depth reaches to roughly 7,000 F, which is sufficiently high for most minerals to lose H2O captured in their atomic-scale structures,” said Dan Shim, professor at ASU’s School of Earth and Space Exploration. “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 the solubility of other light elements in the core,” said Shim. “Therefore, the solubility of carbon, which likely exists in the Earth’s core, decreases locally where hydrogen enters into the core from the mantle (through dehydration). The stable form of carbon at the pressure-temperature conditions of 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,” said Ko. “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. 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 that diamonds are extremely incompressible and less dense than other materials at the core-mantle boundary,” said Shim.
Ko and the team will continue investigating how the reaction can also change the concentration of other light elements in the core, such as silicon, sulfur, and oxygen, and how such changes can impact the mineralogy of the deep mantle.
Reference: “Water-Induced Diamond Formation at Earth’s Core-Mantle Boundary” by Byeongkwan Ko, Stella Chariton, Vitali Prakapenka, Bin Chen, Edward J. Garnero, Mingming Li and Sang-Heon Shim, 11 August 2022, Geophysical Research Letters.
DOI: 10.1029/2022GL098271
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