Acoustic and electrical properties of Fe-Ti oxides with application to the deep lunar mantle

被引:6
作者
Pommier, Anne [1 ]
Walter, Michael J. [1 ]
Hao, Ming [1 ]
Yang, Jing [1 ]
Hrubiak, Rostislav [2 ]
机构
[1] Carnegie Inst Sci, Earth & Planets Lab, Washington, DC 20015 USA
[2] Argonne Natl Lab, Xray Sci Div, High Pressure Collaborat Access Team HPCAT, Lemont, IL 60439 USA
关键词
Fe -Ti oxides; Ilmenite-bearing cumulates; Lunar mantle; Seismic velocity; Electrical conductivity; ELASTIC-WAVE VELOCITY; HIGH-TEMPERATURE; HIGH-PRESSURES; MAGMA OCEAN; SINGLE-CRYSTAL; CONDUCTIVITY; CONSTRAINTS; ILMENITE; MODEL; MOON;
D O I
10.1016/j.epsl.2024.118570
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The overturn of titanium-rich mantle cumulates has been invoked to explain the structure and dynamics of the Moon. These dense cumulates are stable at the core-mantle boundary (CMB) and could explain field observations inferred from geophysical studies. We report acoustic and electrical experiments on natural ilmenite-rutile aggregates up to 4.5 GPa and 1920 K. Seismic velocities show a weak pressure and temperature dependence, with Vs similar to 4.2 (+/-0.2) km/s and Vp similar to 8.0 (+/-0.2) km/s at the CMB conditions. Conductivity increases by a factor of 10(4) from 373 to 1920 K and is >10(3) S/m above 1573 K. Seismic and electrical models for the lunar mantle based on our results, considering mixtures of Fe-Ti oxides and olivine, indicate that field velocity and conductivity estimates are reproduced satisfactorily with 3-16 vol.% Fe-Ti oxides and 20 vol.% melt. Interactions between a Ti-rich, melt-bearing layer and the adjacent core likely affect the cooling and magnetic history of the Moon.
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页数:9
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