Phase transitions in MgSiO3 post-perovskite in super-Earth mantles
- Tokyo Inst. of Technology, Tokyo (Japan). Earth-Life Science Inst.; Univ. of Minnesota, Minneapolis, MN (United States). Dept. of Earth Sciences; Ames Lab. and Iowa State Univ., Ames, IA (United States). Dept. of Physics and Astronomy
- Columbia Univ., New York, NY (United States). Dept. of Applied Physics and Applied Mathematics; Columbia Univ., New York, NY (United States). Dept. of Earth and Environmental Sciences; Columbia Univ., New York, NY (United States). Lamont–Doherty Earth Observatory
- Ames Lab. and Iowa State Univ., Ames, IA (United States). Dept. of Physics and Astronomy; Xiamen Univ., Xiamen (China). Dept. of Physics
- Ames Lab. and Iowa State Univ., Ames, IA (United States). Dept. of Physics and Astronomy
The highest pressure form of the major Earth-forming mantle silicate is MgSiO3 post-perovskite (PPv). Understanding the fate of PPv at TPa pressures is the first step for understanding the mineralogy of super-Earths-type exoplanets, arguably the most interesting for their similarities with Earth. Modeling their internal structure requires knowledge of stable mineral phases, their properties under compression, and major element abundances. Several studies of PPv under extreme pressures support the notion that a sequence of pressure induced dissociation transitions produce the elementary oxides SiO2 and MgO as the ultimate aggregation form at ~3 TPa. However, none of these studies have addressed the problem of mantle composition, particularly major element abundances usually expressed in terms of three main variables, the Mg/Si and Fe/Si ratios and the Mg#, as in the Earth. Here we show that the critical compositional parameter, the Mg/Si ratio, whose value in the Earth’s mantle is still debated, is a vital ingredient for modeling phase transitions and internal structure of super-Earth mantles. Specifically, we have identified new sequences of phase transformations, including new recombination reactions that depend decisively on this ratio. This is a new level of complexity that has not been previously addressed, but proves essential for modeling the nature and number of internal layers in these rocky mantles.
- Research Organization:
- Ames Laboratory (AMES), Ames, IA (United States); Lawrence Berkeley National Laboratory, Berkeley, CA (United States). National Energy Research Scientific Computing Center (NERSC)
- Sponsoring Organization:
- USDOE Office of Science (SC), Basic Energy Sciences (BES) (SC-22). Materials Sciences & Engineering Division; National Natural Science Foundation of China (NSFC); USDOE Office of Science (SC), Advanced Scientific Computing Research (ASCR); USDOE Office of Science (SC), Basic Energy Sciences (BES)
- Grant/Contract Number:
- 1047629; 1319368; 1348066; 11004165; AC02-07CH11358
- OSTI ID:
- 1464467
- Alternate ID(s):
- OSTI ID: 1463298; OSTI ID: 1495541
- Report Number(s):
- IS-J-9482; PII: S0012821X1730479X; TRN: US1902387
- Journal Information:
- Earth and Planetary Science Letters, Vol. 478, Issue C; ISSN 0012-821X
- Publisher:
- ElsevierCopyright Statement
- Country of Publication:
- United States
- Language:
- English
Web of Science
Similar Records
Stability of MgSio[subscript 3] Perovskite in the Lower Mantle
Thermodynamic properties of at super-Earth mantle conditions