利用激光辅助质谱法确定侏罗纪碳酸盐岩中富硫微生物有机物的特征。

IF 3.5 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Astrobiology Pub Date : 2024-01-01 Epub Date: 2023-12-18 DOI:10.1089/ast.2023.0008
Siveen Thlaijeh, Kevin Lepot, Yvain Carpentier, Armelle Riboulleau, Dumitru Duca, Marin Vojkovic, Anuradha Tewari, Johan Sarazin, Mathilde Bon, Nicolas Nuns, Nicolas Tribovillard, Cristian Focsa
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引用次数: 0

摘要

激光解吸电离质谱法(MS)在行星表面的原位分子分析和太空返回样品或(微)化石的微观分析方面显示出巨大的潜力。该技术与欧空局ExoMars项目中的热解气相色谱-质谱联用,有助于进一步评估最近在火星上探测到的含硫有机物(OM)的来源。为了揭示这一潜力,我们利用激光解吸电离质谱法(单步和两步:LDI-MS 和 L2MS),与飞行时间二次离子质谱法(ToF-SIMS)、气相色谱-质谱法(GC-MS)和 Py-GC-MS 进行了比较,分析了约 1.5 亿年前碳酸盐岩中的硫化微生物 OM。我们的研究表明,LDI-MS 和 L2MS 可以轻松检测出(烷基)噻吩和(烷基)苯并噻吩等含硫分子。然而,在我们的 L2MS 实验中,矿物基质给含硫分子的鉴定带来了挑战。在提取的可溶性和不可溶性 OM 以及大块岩石的 LDI-MS 和 L2MS 中,芳香族小碳氢化合物(≤14 个碳原子)占主导地位,这与沉积物的低热成熟度相一致,并与使用这些技术在陨石中通常观察到的较大的多环芳香族结构占主导地位形成鲜明对比。我们在脱矿 OM 中检测到了无机离子,特别是 VO+,这些离子很可能来自地卟啉,而地卟啉是沉积物成岩过程中叶绿素的衍生物。最后,与提取的可溶性 OM 相比,不溶性 OM 的组成截然不同,质量电荷比(m/z)超过 175 的离子更为丰富,并增加了 N 原子。这凸显了激光辅助质谱技术在破译大分子 OM 成分,特别是研究微化石中生物大分子保存情况方面的潜力。需要对各种生物源和非生物源 OM 进行比较研究,以进一步评估该技术在寻找生物特征方面的应用。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Characterization of Sulfur-Rich Microbial Organic Matter in Jurassic Carbonates Using Laser-Assisted Mass Spectrometry.

Laser desorption-ionization mass spectrometry (MS) shows great potential for in situ molecular analysis of planetary surfaces and microanalysis of space-returned samples or (micro)fossils. Coupled with pyrolysis gas chromatography-mass spectrometry (Py-GC-MS) in ESA's ExoMars project, this technique could help assess further the origin of sulfur-bearing organic matter (OM) recently detected on Mars. To unravel this potential, we analyzed sulfurized microbial OM from ca. 150 million year-old carbonates with laser desorption-ionization mass spectrometry (single- and two-step: LDI-MS and L2MS), in comparison with time-of-flight secondary-ion mass spectrometry (ToF-SIMS), gas chromatography-mass spectrometry (GC-MS), and Py-GC-MS. We show that LDI-MS and L2MS readily detect sulfur-bearing moieties such as (alkyl)thiophenes and (alkyl)benzothiophenes. The mineral matrix, however, made the identification of sulfur-bearing molecules challenging in our L2MS experiment. The dominance of small aromatic hydrocarbons (≤14 carbons) in the LDI-MS and L2MS of the extracted soluble and insoluble OM and of the bulk rock is consistent with the low thermal maturity of the sediment and contrasts with the predominance of larger polycyclic aromatic structures commonly observed in meteorites with these techniques. We detected inorganic ions, in particular VO+, in demineralized OM that likely originate from geoporphyrins, which derive from chlorophylls during sediment diagenesis. Finally, insoluble OM yielded distinct compositions compared with extracted soluble OM, with a greater abundance of ions of mass-to-charge ratio (m/z) over 175 and additional N-moieties. This highlights the potential of laser-assisted MS to decipher the composition of macromolecular OM, in particular to investigate the preservation of biomacromolecules in microfossils. Studies comparing diverse biogenic and abiogenic OM are needed to further assess the use of this technique to search for biosignatures.

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来源期刊
Astrobiology
Astrobiology 生物-地球科学综合
CiteScore
7.70
自引率
11.90%
发文量
100
审稿时长
3 months
期刊介绍: Astrobiology is the most-cited peer-reviewed journal dedicated to the understanding of life''s origin, evolution, and distribution in the universe, with a focus on new findings and discoveries from interplanetary exploration and laboratory research. Astrobiology coverage includes: Astrophysics; Astropaleontology; Astroplanets; Bioastronomy; Cosmochemistry; Ecogenomics; Exobiology; Extremophiles; Geomicrobiology; Gravitational biology; Life detection technology; Meteoritics; Planetary geoscience; Planetary protection; Prebiotic chemistry; Space exploration technology; Terraforming
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