Centro de Astrobiología (CAB, CSIC-INTA), 28850 Torrejón de Ardoz, Spain.
Centro de Astrobiología (CAB, CSIC-INTA), 28850 Torrejón de Ardoz, Spain.
Sci Total Environ. 2023 Apr 20;870:161765. doi: 10.1016/j.scitotenv.2023.161765. Epub 2023 Jan 23.
Subaerial hydrothermal systems are of great interest for paleobiology and astrobiology as plausible candidate environments to support the origin of life on Earth that offer a unique and interrelated atmosphere-hydrosphere-lithosphere interface. They harbor extensive sinter deposits of high preservation potential that are promising targets in the search for traces of possible extraterrestrial life on Hesperian Mars. However, long-term quality preservation is paramount for recognizing biosignatures in old samples and there are still significant gaps in our understanding of the impact and extent of taphonomy processes on life fingerprints. Here, we propose a study based on lipid biomarkers -highly resistant cell-membrane components- to investigate the effects of silicification on their preservation in hydrothermal opaline sinter. We explore the lipid biomarkers profile in three sinter deposits of up to ~3000 years from El Tatio, one of the best Martian analogs on Earth. The lipid profile in local living biofilms is used as a fresh counterpart of the fossil biomarkers in the centuries-old sinter deposits to qualitatively assess the taphonomy effects of silicification on the lipid's preservation. Despite the geological alteration, the preserved lipids retained a depleted stable-carbon isotopic fingerprint characteristic of biological sources, result highly relevant for astrobiology. The data allowed us to estimate for the first time the degradation rate of lipid biomarkers in sinter deposits from El Tatio, and to assess the time preservation framework of opaline silica. Auxiliary techniques of higher taxonomic resolution (DNA sequencing and metaproteomics) helped in the reconstruction of the paleobiology. The lipids were the best-preserved biomolecules, whereas the detection of DNA and proteins dropped considerably from 5 cm depth. These findings provide new insights into taphonomy processes affecting life fingerprints in hydrothermal deposits and serves as a useful baseline for assessing the time window for recovering unambiguous signs of past life on Earth and beyond.
陆上热液系统对于古生物学和天体生物学具有重要意义,因为它们是支持地球上生命起源的合理候选环境,提供了独特且相互关联的大气-水圈-岩石圈界面。这些系统中存在广泛的高保存潜力的烧结矿床,是在赫斯珀里得斯火星上寻找可能的外星生命痕迹的有前途的目标。然而,对于识别旧样本中的生物特征,长期的质量保存至关重要,并且我们对于化石化作用对生命指纹的影响和程度的理解仍然存在重大差距。在这里,我们提出了一项基于脂质生物标志物的研究——高度抵抗细胞膜成分——以调查硅化作用对热液蛋白石烧结中其保存的影响。我们探索了三个烧结矿床的脂质生物标志物谱,这些矿床来自于地球上最好的火星模拟区之一的埃尔塔蒂奥,距离现在有长达 3000 年的历史。当地活体生物膜中的脂质谱被用作数百年烧结矿床中化石生物标志物的新鲜对照,以定性评估硅化作用对脂质保存的化石化作用影响。尽管经历了地质变化,但保留下来的脂质仍保留了生物来源的稳定碳同位素指纹特征,这对于天体生物学具有重要意义。这些数据首次允许我们估计来自埃尔塔蒂奥的烧结矿床中脂质生物标志物的降解速率,并评估蛋白石硅的保存时间框架。辅助的高分类分辨率技术(DNA 测序和宏蛋白质组学)有助于古生物学的重建。脂质是保存最完好的生物分子,而从 5 厘米深度开始,DNA 和蛋白质的检测数量则大大减少。这些发现为热液沉积物中影响生命指纹的化石化作用过程提供了新的见解,并为评估在地球和其他星球上恢复过去生命明确迹象的时间窗口提供了有用的基准。