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Biota and Biomolecules in Extreme Environments on Earth: Implications for Life Detection on Mars

机译:地球极端环境中的生物区系和生物分子:对火星生命探测的意义

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摘要

The three main requirements for life as we know it are the presence of organic compounds, liquid water, and free energy. Several groups of organic compounds (e.g., amino acids, nucleobases, lipids) occur in all life forms on Earth and are used as diagnostic molecules, i.e., biomarkers, for the characterization of extant or extinct life. Due to their indispensability for life on Earth, these biomarkers are also prime targets in the search for life on Mars. Biomarkers degrade over time; in situ environmental conditions influence the preservation of those molecules. Nonetheless, upon shielding (e.g., by mineral surfaces), particular biomarkers can persist for billions of years, making them of vital importance in answering questions about the origins and limits of life on early Earth and Mars. The search for organic material and biosignatures on Mars is particularly challenging due to the hostile environment and its effect on organic compounds near the surface. In support of life detection on Mars, it is crucial to investigate analogue environments on Earth that resemble best past and present Mars conditions. Terrestrial extreme environments offer a rich source of information allowing us to determine how extreme conditions affect life and molecules associated with it. Extremophilic organisms have adapted to the most stunning conditions on Earth in environments with often unique geological and chemical features. One challenge in detecting biomarkers is to optimize extraction, since organic molecules can be low in abundance and can strongly adsorb to mineral surfaces. Methods and analytical tools in the field of life science are continuously improving. Amplification methods are very useful for the detection of low concentrations of genomic material but most other organic molecules are not prone to amplification methods. Therefore, a great deal depends on the extraction efficiency. The questions “what to look for”, “where to look”, and “how to look for it” require more of our attention to ensure the success of future life detection missions on Mars.
机译:我们知道,生命的三个主要要求是有机化合物,液态水和自由能的存在。几类有机化合物(例如氨基酸,核碱基,脂质)以地球上的所有生命形式存在,并被用作诊断分子(即生物标记),以表征现存或已灭绝的生命。由于它们对地球生命的不可或缺,因此这些生物标记物也是寻找火星生命的主要目标。生物标记会随着时间而降解;原位环境条件会影响这些分子的保存。但是,通过屏蔽(例如,通过矿物表面),特定的生物标记物可以持续数十亿年,这对于回答有关地球早期和火星生命起源和极限的问题至关重要。由于恶劣的环境及其对地表附近有机化合物的影响,在火星上寻找有机材料和生物特征特别具有挑战性。为了支持火星上的生命探测,至关重要的是研究地球上最类似于过去和现在的火星状况的模拟环境。陆地极端环境提供了丰富的信息资源,使我们能够确定极端条件如何影响生命及其相关分子。在通常具有独特地质和化学特征的环境中,极端嗜热生物已经适应了地球上最令人震惊的条件。检测生物标志物的挑战之一是优化提取,因为有机分子的丰度低并且可以强烈吸附到矿物表面。生命科学领域的方法和分析工具正在不断改进。扩增方法对于检测低浓度的基因组物质非常有用,但是大多数其他有机分子不倾向于扩增方法。因此,很大程度上取决于提取效率。 “寻找什么”,“寻找哪里”和“如何寻找”这些问题需要我们的更多关注,以确保火星上未来的生命探测任务取得成功。

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