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Mars Extant Life: What's Next? Conference Report

机译:火星现存:下一步是什么?会议报告

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On November 5-8, 2019, the "Mars Extant Life: What's Next?" conference was convened in Carlsbad, New Mexico. The conference gathered a community of actively publishing experts in disciplines related to habitability and astrobiology. Primary conclusions are as follows: A significant subset of conference attendees concluded that there is a realistic possibility that Mars hosts indigenous microbial life. A powerful theme that permeated the conference is that the key to the search for martian extant life lies in identifying and exploring refugia ("oases"), where conditions are either permanently or episodically significantly more hospitable than average. Based on our existing knowledge of Mars, conference participants highlighted four potential martian refugium (not listed in priority order): Caves, Deep Subsurface, Ices, and Salts. The conference group did not attempt to reach a consensus prioritization of these candidate environments, but instead felt that a defensible prioritization would require a future competitive process. Within the context of these candidate environments, we identified a variety of geological search strategies that could narrow the search space. Additionally, we summarized a number of measurement techniques that could be used to detect evidence of extant life (if present). Again, it was not within the scope of the conference to prioritize these measurement techniques-that is best left for the competitive process. We specifically note that the number and sensitivity of detection methods that could be implemented if samples were returned to Earth greatly exceed the methodologies that could be used at Mars. Finally, important lessons to guide extant life search processes can be derived both from experiments carried out in terrestrial laboratories and analog field sites and from theoretical modeling.
机译:2019年11月5日至8日,“火星现存生活:下一步是什么?”会议在Carlsbad,新墨西哥卡尔斯巴德召开。会议聚集了与居住地和天体学相关的纪律的积极出版专家社区。主要结论如下:大量会议与会者的结论是,火星举办土着微生物生活具有现实的可能性。渗透会议的强大主题是,寻找火星利党的关键是识别和探索避难所(“果树”),其中条件是永久性的或显着更大的令人难以置信的人。基于我们对火星的现有知识,会议参与者强调了四个潜在的火星避难所(未按优先顺序列出):洞穴,深度地下,冰和盐。会议集团没有试图达成这些候选环境的合格优先级,而是认为可辩护的优先级需要未来的竞争过程。在这些候选环境的上下文中,我们确定了各种能够缩小搜索空间的地质搜索策略。此外,我们总结了许多可用于检测现存寿命(如果存在)的证据的数量测量技术。再次,它不在会议范围内,优先考虑这些测量技术 - 这是最适合竞争过程的留言。我们具体地注意到,如果样品返回地球,则可以实施的检测方法的数量和敏感性大大超过了可能在火星的方法。最后,可以从地面实验室和模拟现场网站和理论建模中源于在陆地实验室和模拟场地进行的实验来导出扩展寿命搜索过程的重要课程。

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