@article{115bd9baa94c4822a2301f826f3256ed,
title = "A new hydrous iron oxide phase stable at mid-mantle pressures",
abstract = "The amount of hydrogen stored in the Earth's interior is important for a range of issues, including the volatile incorporation during the Earth formation and the co-evolution of the atmosphere, the hydrosphere, and the interior. Recent experiments found titanium bearing ε-FeOOH in a hydrous basaltic system at 12–19 GPa and 1300 K. Pyrite-type FeOOH was found to be stable at pressures higher than 80 GPa. These discoveries suggest possible hydrogen storage in the mantle transition zone and in the mantle below 1800 km depths, respectively. However, it remains uncertain how the potential deep hydrogen storage can be connected to the shallower storage. Here, we report a new hydrous iron oxide (η-Fe12O18+x/2Hx, x≈2) stable at pressures between the stability fields of the ε- and the pyrite-type FeOOH. Our experiment also shows that the new η phase can exist together with the major lower mantle minerals including bridgmanite and periclase, making it an important hydrogen-bearing phase in the Earth's deep interior. Because of its limited H2O storage capacity, which is less than 1/6 of the storage capacity of the pyrite-type phase and the ε phase, the stability of the η phase would result in H2O loss during water transport in the mid mantle and therefore limit the amount of H2O potentially stored in the Fe–O–H system of the lower mantle. The large channel in the crystal structure of the η phase could provide potential storage sites for other volatile elements in the deep mantle.",
keywords = "crystal structure, hydrogen, hydrous iron oxide, lower mantle",
author = "Huawei Chen and Xie, {Sheng Yi} and Byeongkwan Ko and Taehyun Kim and Carole Nisr and Vitali Prakapenka and Eran Greenberg and Dongzhou Zhang and Wenli Bi and Ercan, {Alp E.} and Yongjae Lee and Shim, {Sang Heon}",
note = "Funding Information: This work was supported by NSF grants EAR1321976 and EAR1401270 and a NASA grant (80NSSC18K0353) to S.H.S. H.C. was supported by the Keck Foundation (PI: P. Buseck). Y. L. thanks the Leader Researcher program (NRF-2018R1A3B1052042) of the Korean Ministry of Science and ICT. We thank Kurt Leinenweber and Andrew Chizmeshya for discussions. The results reported herein benefit from collaborations and/or information exchange within NASA's Nexus for Exoplanet System Science (NExSS) research coordination network sponsored by NASA's Science Mission Directorate. The synchrotron experiments were conducted at GSECARS, Advanced Photon Source (APS). GSECARS is supported by NSF-Earth Science (EAR-1128799) and DOE-GeoScience (DE-FG02-94ER14466). APS is supported by DOE, under contracts DE-AC02-06CH11357. The experimental data included in this paper are available by contacting SHDShim@asu.edu or hchen156@asu.edu. Funding Information: This work was supported by NSF grants EAR1321976 and EAR1401270 and a NASA grant ( 80NSSC18K0353 ) to S.H.S. H.C. was supported by the Keck Foundation (PI: P. Buseck). Y. L. thanks the Leader Researcher program ( NRF-2018R1A3B1052042 ) of the Korean Ministry of Science and ICT . We thank Kurt Leinenweber and Andrew Chizmeshya for discussions. The results reported herein benefit from collaborations and/or information exchange within NASA's Nexus for Exoplanet System Science (NExSS) research coordination network sponsored by NASA's Science Mission Directorate. The synchrotron experiments were conducted at GSECARS, Advanced Photon Source (APS). GSECARS is supported by NSF -Earth Science ( EAR-1128799 ) and DOE -GeoScience ( DE-FG02-94ER14466 ). APS is supported by DOE , under contracts DE-AC02-06CH11357 . The experimental data included in this paper are available by contacting SHDShim@asu.edu or hchen156@asu.edu. Publisher Copyright: {\textcopyright} 2020 Elsevier B.V.",
year = "2020",
month = nov,
day = "15",
doi = "10.1016/j.epsl.2020.116551",
language = "English (US)",
volume = "550",
journal = "Earth and Planetary Science Letters",
issn = "0012-821X",
publisher = "Elsevier",
}