- Open Access
Direct sound speed measurements of MgO along planetary adiabats up to 400 GPa using shock-ramp compression
Phys. Rev. B 114, 274108 – Published 12 November, 2026
DOI: https://doi.org/10.1103/x7x6-16cs
Abstract
Accurate models of planetary formation and evolution rely on equation-of-state (EOS) models for their constituent materials across wide ranges of pressure, temperature, and density. Currently, estimates of thermoelastic properties along Earth-like pressure and temperature adiabats (the geotherm) require extrapolation of laboratory data, which confounds clear interpretation of the physical and chemical states of planetary interiors. We designed experiments on the Z Machine at Sandia National Laboratories to directly measure the EOS and sound speeds in dense oxides along quasi-isentropes close to the geotherm using shock-ramp compression. Here we demonstrate the method on magnesium oxide, representing the major nonsilicate mineral in the mantle, to pressures exceeding Earth's core. Our observations up to 400 GPa are confirmed by independent density functional theory and quantum Monte Carlo predictions and indicate the experimental compression path is close to a 1900 K geotherm. The results show excellent agreement with the preliminary reference Earth model (PREM), suggesting the technique can produce highly accurate thermoelastic data useful for interpreting the internal structure of terrestrial planets.
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