Shock and shock-ramp compression of iron-rich (Mg,Fe)O at Earth's core conditions
ORAL
Abstract
Where Earth’s iron core and silicate mantle meet is a region of the Earth’s interior that is still poorly understood. Seismological results suggest the presence of ultra-low velocity zones (ULVZ’s) sitting directly atop the core. One possible explanation for these features is that they are regions of highly iron-enriched ferropericlase (Mg,Fe)O (Wicks et al. 2010), however the thermodynamic properties at near-core conditions are poorly constrained. Here we present the results of combined ab-initio calculations and shock measurements of (Mg,Fe)O containing 25 and 50 mol% Fe. The results are being used to design shock-ramp experiments on the Z machine at Sandia National Laboratories.
Wicks, J. K., Jackson, J. M., & Sturhahn, W. (2010) Very low sound velocities in iron‐rich (Mg, Fe) O: Implications for the core‐mantle boundary region. Geophysical Research Letters, 37(15).
Wicks, J. K., Jackson, J. M., & Sturhahn, W. (2010) Very low sound velocities in iron‐rich (Mg, Fe) O: Implications for the core‐mantle boundary region. Geophysical Research Letters, 37(15).
*Sandia National Laboratories is a multimission laboratory managed and operated by National Technology & Engineering Solutions of Sandia, LLC, a wholly owned subsidiary of Honeywell International Inc., for the U.S. Department of Energy National Nuclear Security Administration under contract DE-NA0003525.This work was supported by the US Department of Energy — National Nuclear Security Administration through the Chicago / DOE Alliance Center.
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Presenters
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Hannah Bausch
- Northwestern University