Abstract

The upcoming Mars Sample Return (MSR) mission aims to deliver small quantities of Martian rocks to the Earth. Investigating these precious samples requires the development and application of techniques that can extract the greatest amount of high quality data from the minimum sample volume, thereby maximising science return from MSR. Atom probe tomography (APT) and transmission electron microscopy (TEM) are two complementary techniques that can obtain nanoscale structural, geochemical and, in the case of atom probe, isotopic information from small sample volumes. Here we describe how both techniques operate, as well as review recent developments in sample preparation protocols. We also outline how APT has been successfully applied to extraterrestrial materials in the recent past. Finally, we describe how we have studied Martian meteorites using TEM and APT in close coordination in order to characterise the products of water/rock interactions in t h e cru st of Ma r s – a k ey sc ie n ce goal of MSR. Our results provide new insights into the Martian hydrosphere and the mechanisms of anhydrous-hydrous mineral replacement. In light of the unique results provided by these tools, APT and TEM should form a crucial part at the culmination of a correlative analytical pipeline for MSR mission materials.

Highlights

  • Rocks from Mars are among the rarest meteorites and are the only physical samples we currently have of the red planet

  • A brief history of atom probe tomography in planetary science The first paper on non-conductive geological materials using laser assisted atom probe microscopy was by Valley et al [34] who demonstrated that the 207Pb/206Pb isotopic abundances can be measured in zircon using Atom probe tomography (APT)

  • Through measurements at the atomicscale using transmission electron microscopy (TEM) and APT we can provide new insights into Martian and Solar System processes that act on length scales over 20 orders of magnitude larger than the sample volume analysed such as action of water on Mars that has implications for past and future habitability of the red planet

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Summary

Introduction

Rocks from Mars are among the rarest meteorites and are the only physical samples we currently have of the red planet. Atom probe tomography (APT) and transmission electron microscopy (TEM) are two complementary techniques that can obtain nanoscale structural, geochemical and, in the case of atom probe, isotopic information from small sample volumes. We describe how we have studied Martian meteorites using TEM and APT in close coordination in order to characterise the products of water/rock interactions in the crust of Mars – a key science goal of MSR.

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