Trace metal and organic biosignatures in digitate stromatolites from terrestrial siliceous hot spring deposits: Implications for the exploration of martian life

IF 3.6 2区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS Chemical Geology Pub Date : 2024-05-29 DOI:10.1016/j.chemgeo.2024.122194
Ema E. Nersezova , Michael C. Rowe , Kathleen A. Campbell , Andrew Langendam , Cherie Tollemache , Barbara Lyon , Amanda Galar , Diego M. Guido , Bronwyn L. Teece , Trinity L. Hamilton
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Abstract

Novel biosignatures of laminated, microbial, digitate sedimentary structures – stromatolites – from modern geothermal fields of the Taupō Volcanic Zone, New Zealand, and from El Tatio, Chile, provide an opportunity to investigate evidence of extremophile life preserved in siliceous hot spring deposits, or sinters, interpreted as analogs for early life on Earth and possibly Mars. Synchrotron-μXRF, electron microprobe analysis, Raman spectroscopy, and optical microscopy are used in a coordinated approach to identify corroborating textural and chemical (organic, inorganic) evidence of life in these modern, opaline (amorphous) siliceous materials. Fluid mobile elements, such as As and Sr, track the growth history of the digitate structures. Trace element enrichments of Ca, Al, Ga, +/− Fe, Mn, As, Rb, Cs, and Sr, are identified in silicified sheaths of microbial filaments embedded within the sinter. In contrast, silicified diatoms in some sinter samples show no trace element enrichment. Gallium enrichments have also been observed in other 16 ka and Jurassic (150 Ma) microbial palisade sinter textures, suggesting the potential for preservation through geologic time, even after recrystallization to quartz. Raman analysis reveals spectra of organics, consistent with pigments for UV protection in cyanobacteria, in silicified sheaths around microbial filaments and are co-located with trace metal enrichments in digitate structures. Due to spectral bands, the location of these molecules (i.e., in the sheaths), and the sampling locations, we ascribe the spectra to scytonemin and carotenoid class molecules. The combined analytical approach outlined here provides a robust means to assess the validity of novel biosignatures, with application to the exploration of Mars, where preservation of opaline silica in >3.6 Ga deposits has the potential to preserve a range of microbial biosignatures.

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来自陆地硅质温泉矿床的岩屑叠层石中的痕量金属和有机生物特征:对探索火星生命的影响
新西兰陶波火山区和智利埃尔塔蒂奥现代地热区的层状、微生物、岩屑沉积结构--叠层石--的新生物特征,为研究硅质温泉沉积物或沉积物中保存的嗜极端生物的证据提供了机会,这些沉积物被解释为地球早期生命的类似物,也可能是火星早期生命的类似物。同步辐射-μXRF、电子微探针分析、拉曼光谱和光学显微镜被协调使用,以确定这些现代乳白(无定形)硅质材料中生命的纹理和化学(有机、无机)证据。流体流动元素,如 As 和 Sr,可追踪岩屑结构的生长历史。在嵌入烧结矿中的微生物菌丝的硅化护套中发现了钙元素、铝元素、镓元素、+/-铁元素、锰元素、砷元素、铷元素、铯元素和锶元素的富集。相比之下,一些烧结矿样本中的硅化硅藻没有显示出微量元素富集。在其他 16 ka 和侏罗纪(150 Ma)微生物栅栏烧结矿纹理中也观察到镓元素富集,这表明即使在重结晶为石英之后,镓元素仍有可能通过地质时间保存下来。拉曼分析显示,在微生物菌丝周围的硅化护套中存在有机物光谱,与蓝藻中用于保护紫外线的色素一致,并与岩屑结构中富集的痕量金属位于同一位置。根据光谱带、这些分子的位置(即在鞘中)和取样位置,我们将光谱归结为鞘氨醇和类胡萝卜素类分子。本文概述的综合分析方法为评估新型生物特征的有效性提供了有力的手段,并可应用于火星探测,因为在 3.6 Ga 沉积物中保存的乳白硅石有可能保存一系列微生物生物特征。
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来源期刊
Chemical Geology
Chemical Geology 地学-地球化学与地球物理
CiteScore
7.20
自引率
10.30%
发文量
374
审稿时长
3.6 months
期刊介绍: Chemical Geology is an international journal that publishes original research papers on isotopic and elemental geochemistry, geochronology and cosmochemistry. The Journal focuses on chemical processes in igneous, metamorphic, and sedimentary petrology, low- and high-temperature aqueous solutions, biogeochemistry, the environment and cosmochemistry. Papers that are field, experimentally, or computationally based are appropriate if they are of broad international interest. The Journal generally does not publish papers that are primarily of regional or local interest, or which are primarily focused on remediation and applied geochemistry. The Journal also welcomes innovative papers dealing with significant analytical advances that are of wide interest in the community and extend significantly beyond the scope of what would be included in the methods section of a standard research paper.
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