V14C-04
Iron carbonates in the Earth’s lower mantle: reality or imagination?

Monday, 14 December 2015: 16:45
103 (Moscone South)
Valerio Cerantola1,2, Catherine A McCammon2, Marco Merlini3, Elena Bykova2, Ilya Kupenko1, Leyla Ismailova2, Alexander I Chumakov1, Innokenty Kantor1, Leonid S Dubrovinsky4 and Clemens Prescher5, (1)ESRF European Synchrotron Radiation Facility, Grenoble, France, (2)University of Bayreuth, Bayreuth, Germany, (3)University of Milano, Milano, Italy, (4)Bayerisches Geoinsitut, Bayreuth, Germany, (5)University of Chicago, Center for Advanced Radiation Sources, Chicago, IL, United States
Abstract:
Carbonates play a fundamental role in the recycling of carbon inside our planet due to their presence in oceanic slabs that sink through the Earth’s interior. Through this process, iron carbonates are potential stable carbon-bearing minerals in the deep mantle in part due to spin crossover of ferrous iron. Our goal is to identify which minerals may be the dominant carriers of carbon into the deep mantle at the relevant conditions of fO2, P and T. All experiments were performed using synthetic FeCO3 and MgFeCO3 single crystals in laser heated diamond anvil cells up to 100 GPa and 3000 K in order to simulate the conditions prevailing in the Earth’s lower mantle. Transformation and decomposition products of the original carbonates were characterized at different synchrotron facilities by means of single-crystal XRD, synchrotron Mössbauer source spectroscopy and XANES techniques. At deep lower mantle conditions, we observed the transformation of FeCO3 to two new HP-carbonate structures, monoclinic Fe22+Fe23+C4O13 and trigonal Fe43+(CO4)3, both characterized by the presence of CO4 tetrahedra with different degrees of polymerization. At shallower depths in the lower mantle where temperatures are lower following the geotherm, Fe-carbonates decompose to different Fe-oxides instead of new HP-carbonates. However, at slab temperatures several hundred degrees lower than the surrounding mantle, carbonates could be stabilized until reaching conditions that trigger their transformation to HP-structures. We postulate that Fe-rich carbonates could exist in regions down to the core-mantle boundary in the proximity of subducting slabs, i.e., a “cold” environment with relatively high fO2.