Molecular Cell Physiology, Faculty of Earth and Life Sciences, VU University Amsterdam, de Boelelaan 1085, 1081 HV Amsterdam, The Netherlands.
Leiden Observatory, Leiden University, P.O. Box 9513, NL-2300 RA Leiden, The Netherlands.
Life (Basel). 2014 Oct 13;4(4):535-65. doi: 10.3390/life4040535.
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.
生命存在的三个主要条件是有机化合物、液态水和自由能。在地球上的所有生命形式中都存在几类有机化合物(如氨基酸、碱基、脂质),它们被用作诊断分子,即生物标志物,用于描述现存或已灭绝生命的特征。由于这些生物标志物对地球上的生命是不可或缺的,因此它们也是在火星上寻找生命的主要目标。生物标志物会随着时间的推移而降解;当地环境条件会影响这些分子的保存。尽管如此,在受到屏蔽(例如被矿物表面屏蔽)的情况下,某些生物标志物可以持续数十亿年,这使得它们在回答有关早期地球和火星生命起源和极限的问题方面变得至关重要。在火星上寻找有机物质和生物特征特别具有挑战性,因为火星的环境恶劣,会对表面附近的有机化合物产生影响。为了支持在火星上进行生命探测,调查地球的类似环境至关重要,这些环境最能反映过去和现在的火星条件。地球的极端环境为我们提供了丰富的信息来源,使我们能够确定极端条件如何影响生命及其相关分子。嗜极生物已经适应了地球上最恶劣的条件,生活在具有独特地质和化学特征的环境中。在检测生物标志物时,面临的一个挑战是优化提取方法,因为有机分子的丰度可能很低,并且可能强烈吸附在矿物表面上。生命科学领域的方法和分析工具在不断改进。扩增方法对于检测低浓度的基因组物质非常有用,但大多数其他有机分子并不适合扩增方法。因此,很大程度上取决于提取效率。“寻找什么”、“在哪里寻找”和“如何寻找”的问题需要我们更加关注,以确保未来在火星上进行生命探测任务的成功。