Sound velocities in lunar mantle aggregates at simultaneous high pressures and temperatures suggests the presence of garnet in the deep lunar interior

Researchers at the Geodynamics Research Center (GRC), Ehime University, were able to determine the sound velocities in a synthetic lunar mantle rock, containing a high percentage of garnet, by means of synchrotron radiation and ultrasonic measurements in a large volume press apparatus. Their results suggest that significant amounts of garnet could be present in the deep lunar interior, the presence of which has important implications for the formation, composition, and internal dynamics of the Moon.

Our present-day Moon has an interior structure containing a central metallic core, overlain by a mantle comprised of minerals such as olivine and pyroxene (e.g. Ol+Px mantle) underneath a shell of crust (e.g. Wieczorek et al. 2006). Such a picture of the Moon’s interior has been formed from analyses of returning lunar samples and records of deep seismic events collected during missions to the Moon (e.g. Weber et al., 2011). Despite the wealth of literature, there is still a longstanding debate as to the existence of garnet (Gt) within the deeper part of the lunar mantle. Reflecting upon the existence of garnet, the pivotal question first posited fifty years ago (e.g. Anderson, 1975) has remained unanswered: are laboratory measured sound velocities in realistic lunar aggregates containing garnet compatible with the seismic profiles of the deep lunar interior?
To provide answers to this question Ehime’s researchers first synthesized garnet-rich lunar rock assemblages (Ol+Px+Gt sample) at high pressures and high temperatures using the multi-anvil press apparatus “ORANGE-2000” at the Geodynamics Research Center. These samples were then transported to SPring-8, the Large-scale Synchrotron Radiation Facility, located in Hyogo Prefecture, where experiments were carried out at the High Pressure and High Temperature beamline BL04B1. Here the researchers subjected the lunar rock assemblage to pressure and temperature conditions similar to those of the Moon’s deep interior while they measured the propagation speed of sound waves in the lunar rock assemblage. Combining the results of their experiment with a modelling component, the researchers concluded that the sound velocities in lunar assemblages containing large amounts of garnet were compatible with the seismic and density profiles of the Moon’s deep interior, between depths of 740-1260 km. Furthermore, they found that rock assemblages containing little to no garnet are unlikely to explain the observed seismic velocities and densities of the lunar mantle at those depths.
These intriguing results have significant implications for the Moon and its interior dynamics, including its composition and formation (e.g. Jing et al., 2022), the interior temperature, as well as implications for the lunar core and the now defunct lunar dynamo.

Reference URL: https://www.sciencedirect.com/science/article/pii/S0012821X24002255?via%3Dihub

Bibliographic Information

Sound velocities in lunar mantle aggregates at simultaneous high pressures and temperatures: Implications for the presence of garnet in the deep lunar interior,
Marisa C. Wood, Steeve Gréaux, Yoshio Kono, Sho Kakizawa, Yuta Ishikawa, Sayako Inoué, Hideharu Kuwahara, Yuji Higo, Noriyoshi Tsujino, Tetsuo Irifune,
Earth and Planetary Science Letters, 641, 118792,
https://doi.org/10.1016/j.epsl.2024.118792, 2024 (September 1st).

Fundings

• Japan Society for the Promotion of Science(JSPS) KAKENHI Grant Number 19H02002
• Japan Society for the Promotion of Science(JSPS) Postdoctoral Fellowship

Media

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  A deep garnet-rich layer in the lunar mantle

  Schematic representation of the Moon’s interior featuring a garnet-rich lunar mantle atop the core-mantle-boundary, and a picture of the synthetic lunar mantle aggregate investigated in this study.

  credit : Geodynamics Research Center, Ehime University
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