Mechanical softening and enhanced elasticity of lunar olivine probed via nanoindentation and high-pressure X-ray diffraction measurements

TL;DR

This study combines nanoindentation and high-pressure X-ray diffraction to reveal that lunar olivine in meteorite NWA 12008 is softer and more elastic than terrestrial olivine, providing insights into planetary mineral properties.

Contribution

It introduces a combined experimental approach to analyze the mechanical and elastic properties of lunar meteorite olivine, highlighting differences from terrestrial samples.

Findings

Lunar olivine is softer than terrestrial olivine.

Olivine in meteorite NWA 12008 shows higher elastic modulus softening.

Differences are linked to macroscopic and chemical-bond effects.

Abstract

The mechanical properties of minerals in planetary materials are not only interesting from a fundamental point of view but also critical to the development of future space missions. Here we present nanoindentation experiments to evaluate the hardness and reduced elastic modulus of olivine, (Mg, Fe)2SiO4, in meteorite NWA 12008, a lunar basalt. Our experiments suggest that the olivine grains in this lunaite are softer and more elastic than their terrestrial counterparts. Also, we have performed synchrotron-based high-pressure X-ray diffraction (HP-XRD) measurements to probe the compressibility properties of this meteorite and, for comparison purposes, of three ordinary chondrites. The HP-XRD results suggest that the axial compressibility of the orthorhombic $b$ lattice parameter of olivine relative to terrestrial olivine is higher in NWA 12008 and also in the highly-shocked Chelyabinsk meteorite. The origin of the observed differences is discussed. A simple model combining the results of both our nanoindentation and HP-XRD measurements allows us to describe the contribution of macroscopic and chemical-bond related effects, both of which are necessary to reproduce the observed elastic modulus softening. Such joint analysis of the mechanical and elastic properties of meteorites and returned samples opens up a new avenue for characterizing these highly interesting materials.