Submicron-scale detection of microbes and smectite from the interior of a Mars analogue basalt sample by optical-photothermal infrared spectroscopy
Author(s)
Type
Journal Article
Abstract
For near-future missions planed for Mars Sample Return (MSR), an international working group organized by the Committee on Space Research (COSPAR) developed the sample safety assessment framework (SSAF). For the SSAF, analytical instruments were selected by taking the practical limitations of hosting them within a facility with the highest level of biosafety precautions (biosafety level 4) and the precious nature of returned samples into account. To prepare for MSR, analytical instruments of high sensitivity need to be tested on effective Mars analogue materials. As an analogue material, we selected a rock core of basalt, a prominent rock type on the Martian surface. Two basalt samples with aqueous alteration cached in Jezero crater by the Perseverance rover are planned to be returned to Earth. Our previously published analytical procedures using destructive but spatially sensitive instruments such as nanoscale secondary ion mass spectrometry (NanoSIMS) and transmission electron microscopy coupled to energy-dispersive spectroscopy revealed microbial colonization at clay-filled fractures. With an aim to test the capability of an analytical instrument listed in SSAF, we now extend that work to conventional Fourier transform infrared (FT-IR) microscopy with a spatial resolution of 10 μm. Although Fe-rich smectite called nontronite was identified after crushing some portion of the rock core sample into powder, the application of conventional FT-IR microscopy is limited to a sample thickness of <30 μm. In order to obtain IR-based spectra without destructive preparation, a new technique called optical-photothermal infrared (O-PTIR) spectroscopy with a spatial resolution of 0.5 μm was applied to a 100 μm thick section of the rock core. By O-PTIR spectroscopic analysis of the clay-filled fracture, we obtained in-situ spectra diagnostic to microbial cells, consistent with our previously published data obtained by NanoSIMS. In addition, nontronite identification was also possible by O-PTIR spectroscopic analysis. From these results, O-PTIR spectroscopy is suggested be superior to deep ultraviolet fluorescence microscopy/μ-Raman spectroscopy, particularly for smectite identification. A simultaneous acquisition of the spatial distribution of structural motifs associated with biomolecules and smectites is critical for distinguishing biological material in samples as well as characterizing an abiotic background.
Date Issued
2025-02-19
Date Acceptance
2025-01-07
Citation
International Journal of Astrobiology, 2025, 24
ISSN
1473-5504
Publisher
Cambridge University Press
Journal / Book Title
International Journal of Astrobiology
Volume
24
Copyright Statement
© The University of Tokyo, 2025. Published by Cambridge University Press. This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution and reproduc tion, provided the original article is properly cited
License URL
Sponsor
Science and Technology Facilities Council (STFC)
UKSA- UK Space Agency
Department for Business Innovation and Skills
UK Space Agency
Identifier
10.1017/S1473550425000011
Grant Number
EACPR_P89346
ST/V006134/1
AMS 1900529
ST/Y006194/1
Subjects
0201 Astronomical and Space Sciences
0403 Geology
Astronomy & Astrophysics
Publication Status
Published
Article Number
e1
Date Publish Online
2025-02-19