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Fe3+ -hosting carbon phases in the deep Earth

Authors :
Albers, C
Sakrowski, R
Libon, L
Spiekermann, G
Winkler, B
Schmidt, C
Bayarjargal, L
Cerantola, V
Chariton, S
Giordano, N
Gretarsson, H
Kaa, J
Liermann, H
Sundermann, M
Thiering, N
Tolan, M
Wilke, M
Christian Sternemann, A
Christian Albers
Robin Sakrowski
Lélia Libon
Georg Spiekermann
Björn Winkler
Christian Schmidt
Lkhamsuren Bayarjargal
Valerio Cerantola
Stella Chariton
Nico Giordano
Hlynur Gretarsson
Johannes Kaa
Hanns-Peter Liermann
Martin Sundermann
Nicola Thiering
Metin Tolan
Max Wilke
and Christian Sternemann
Albers, C
Sakrowski, R
Libon, L
Spiekermann, G
Winkler, B
Schmidt, C
Bayarjargal, L
Cerantola, V
Chariton, S
Giordano, N
Gretarsson, H
Kaa, J
Liermann, H
Sundermann, M
Thiering, N
Tolan, M
Wilke, M
Christian Sternemann, A
Christian Albers
Robin Sakrowski
Lélia Libon
Georg Spiekermann
Björn Winkler
Christian Schmidt
Lkhamsuren Bayarjargal
Valerio Cerantola
Stella Chariton
Nico Giordano
Hlynur Gretarsson
Johannes Kaa
Hanns-Peter Liermann
Martin Sundermann
Nicola Thiering
Metin Tolan
Max Wilke
and Christian Sternemann
Publication Year :
2022

Abstract

Iron-bearing carbonates play an important role in Earth's carbon cycle. Owing to their stability at mantle conditions, recently discovered iron carbonates with tetrahedrally coordinated carbon atoms are candidates for carbon storage in the deep Earth. The carbonates' iron oxidation and spin state at extreme pressure and temperature conditions contribute to the redox conditions and element partitioning in the deep mantle. By laser heating FeCO3 at pressures of about 83 GPa, Fe43+C3O12 and Fe22+Fe23+C4O13 were synthesized and then investigated by x-ray emission spectroscopy to elucidate their spin state, both in situ and temperature quenched. Our experimental results show both phases in a high-spin state at all pressures and over the entire temperature range investigated, i.e., up to 3000 K. The spin state is conserved after temperature quenching. A formation path is favored where Fe43+C3O12 forms first and then reacts to Fe22+Fe23+C4O13, most likely accompanied by the formation of oxides. Density functional theory calculations of Fe22+Fe23+C4O13 at 80 GPa confirm the experimental findings with both ferric and ferrous iron in high-spin state with antiferromagnetic order at 80 GPa. As the intercrystalline cation partitioning between the Fe-bearing carbonates and the surrounding perovskite and ferropericlase depends on the spin state of the iron, an understanding of the redox conditions prevalent in subducted slab regions in the lower mantle has to take the latter into account. Especially, Fe22+Fe23+C4O13 may play a key role in subducted material in the lower mantle, potentially with a similar role as silicate perovskite.

Details

Database :
OAIster
Notes :
STAMPA, English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1354526925
Document Type :
Electronic Resource