N-Alkane Biosignatures in a High Arctic Mars Analogue Gossan Deposit

Hiba Aoid, Richard Léveillé, Peter Douglas, Myriam Lemelin, Marie-Claude Williamson
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Abstract

If past life ever existed on Mars, what are the multiple ways it could have been preserved in the Martian geological record? This crucial question is becoming especially relevant the more we uncover about the planet’s ancient wet history. Different acidic and sulfur rich analog environments have been proposed that are comparable to the alteration environments of iron oxides and sulfate minerals on Mars. However, some authors have hypothesized that these past Martian environments might have been cold and semi-dry, similar to polar regions on Earth. As part of the T-MARS team, we studied reactive gossans in the Canadian High Arctic, on Axel Heiberg Island, as an analog environment to similar deposits on Mars. We hypothesized that n-alkane lipids could potentially be an important form of molecular fossils entombed in varying mineral assemblages of sulphates, iron oxides, and phyllosilicates in Arctic gossans, because of their excellent preservation potential relative to most other forms of organic molecules. To determine the preservation potential of lipids in mineralogically varying acidic sulfur rich gossan deposits, this study extracted and quantified n-alkane biomarkers from three different Arctic gossans with gas chromatography–mass spectrometry (GC-MS). Total organic carbon, pH, and mineralogy were also determined. Organic matter was found to be very low in all samples (<1% wt.%). N-alkane analysis also revealed preserved even-over-odd distribution patterns in short chain n-alkanes, most likely from a microbial source, along with evidence for long-chain n-alkanes with odd-over-even distribution from higher plant sources. The presence of these unique chemical biosignatures in low organic, highly acidic, and sulfur rich Mars analog gossans of varying maturity provides evidence that sulfur deposits linked to paleo hydrothermal systems on Mars can be promising targets for preserved organic biosignatures, specifically lipid n-alkanes. The significant diversity in biosignature patterns across samples of varying mineralogy, pH, and oxidation levels within each gossan suggests that n-alkane preservation varies on a small scale in these environments. These factors alone do not definitively account for the variability of n-alkane concentrations and distributions in this study, and additional investigations of these and other influencing factors are needed to determine which specific targets to choose for biosignature search on Mars in future space missions. This exploratory study provides novel insights into the lipid biosignature content in high Arctic Mars analogue gossan deposits.
高北极火星模拟砂岩矿床的正构烷烃生物特征
如果过去的生命曾经在火星上存在过,那么在火星地质记录中有哪些保存方式呢?随着我们对火星古代湿润历史的了解越来越多,这个关键问题变得尤为重要。人们提出了不同的酸性和富硫模拟环境,可与火星上氧化铁和硫酸盐矿物的蚀变环境相媲美。然而,一些作者假设,这些过去的火星环境可能是寒冷和半干燥的,类似于地球上的极地地区。作为T-MARS团队的一员,我们研究了加拿大高北极地区阿克塞尔海伯格岛上的活性蛛丝,作为火星上类似沉积物的模拟环境。我们假设,正烷脂可能是埋藏在北极蛛丝中硫酸盐、氧化铁和层状硅酸盐矿物组合中的一种重要的分子化石形式,因为它们相对于大多数其他形式的有机分子具有良好的保存潜力。为了确定矿物学变化的酸性富硫棉质沉积物中脂质的保存潜力,本研究利用气相色谱-质谱联用技术(GC-MS)从三种不同的北极棉质中提取并定量了正烷烃生物标志物。测定了总有机碳、pH值和矿物学。所有样品中的有机物含量都很低(1% wt.%)。正构烷烃分析还揭示了短链正构烷烃中保存的偶比奇分布模式,这些短链正构烷烃很可能来自微生物来源,同时也有证据表明,长链正构烷烃来自高等植物来源,具有奇比奇分布模式。在不同成熟度的低有机、高酸性和富硫的火星模拟蛛丝中存在这些独特的化学生物特征,这表明与火星古热液系统有关的硫沉积物可能是保存有机生物特征的有希望的目标,特别是脂质正构烷烃。不同矿物学、pH值和氧化水平的样品中生物特征模式的显著差异表明,在这些环境中,正构烷烃的保存在小范围内存在差异。这些因素本身并不能明确解释本研究中正构烷烃浓度和分布的变异性,需要对这些因素和其他影响因素进行进一步调查,以确定在未来的太空任务中选择哪些具体目标进行火星生物特征搜索。这项探索性研究为北极火星高模拟松质沉积物的脂质生物特征含量提供了新的见解。
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