Stability of iron-bearing carbonates in the deep Earth's interior

Valerio Cerantola, Elena Bykova, Ilya Kupenko, Marco Merlini, Leyla Ismailova, Catherine McCammon, Maxim Bykov, Alexandr I. Chumakov, Sylvain Petitgirard, Innokenty Kantor, Volodymyr Svitlyk, Jeroen Jacobs, Michael Hanfland, Mohamed Mezouar, Clemens Prescher, Rudolf Ruffer, Vitali B. Prakapenka, Leonid Dubrovinsky

Research output: Contribution to journalJournal articleResearchpeer-review

133 Downloads (Pure)


The presence of carbonates in inclusions in diamonds coming from depths exceeding 670 km are obvious evidence that carbonates exist in the Earth's lower mantle. However, their range of stability, crystal structures and the thermodynamic conditions of the decarbonation processes remain poorly constrained. Here we investigate the behaviour of pure iron carbonate at pressures over 100 GPa and temperatures over 2,500 K using single-crystal X-ray diffraction and Mossbauer spectroscopy in laser-heated diamond anvil cells. On heating to temperatures of the Earth's geotherm at pressures to similar to ∼50 GPa FeCO3 partially dissociates to form various iron oxides. At higher pressures FeCO3 forms two new structures-tetrairon(III) orthocarbonate Fe34+C3O12, and diiron(II) diiron(III) tetracarbonate Fe22+Fe32+C4O13, both phases containing CO4 tetrahedra. Fe4C4O13 is stable at conditions along the entire geotherm to depths of at least 2,500 km, thus demonstrating that self-oxidation-reduction reactions can preserve carbonates in the Earth's lower mantle.
Original languageEnglish
Article number15960
JournalNature Communications
Number of pages9
Publication statusPublished - 2017
Externally publishedYes


Dive into the research topics of 'Stability of iron-bearing carbonates in the deep Earth's interior'. Together they form a unique fingerprint.

Cite this