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火星生命与环境的协同演化:基于生物特征机器人探测的生态系统视角。

The Coevolution of Life and Environment on Mars: An Ecosystem Perspective on the Robotic Exploration of Biosignatures.

机构信息

The SETI Institute Carl Sagan Center , Mountain View, California.

出版信息

Astrobiology. 2018 Jan;18(1):1-27. doi: 10.1089/ast.2017.1756. Epub 2017 Dec 18.

DOI:10.1089/ast.2017.1756
PMID:29252008
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC5779243/
Abstract

Earth's biological and environmental evolution are intertwined and inseparable. This coevolution has become a fundamental concept in astrobiology and is key to the search for life beyond our planet. In the case of Mars, whether a coevolution took place is unknown, but analyzing the factors at play shows the uniqueness of each planetary experiment regardless of similarities. Early Earth and early Mars shared traits. However, biological processes on Mars, if any, would have had to proceed within the distinctive context of an irreversible atmospheric collapse, greater climate variability, and specific planetary characteristics. In that, Mars is an important test bed for comparing the effects of a unique set of spatiotemporal changes on an Earth-like, yet different, planet. Many questions remain unanswered about Mars' early environment. Nevertheless, existing data sets provide a foundation for an intellectual framework where notional coevolution models can be explored. In this framework, the focus is shifted from planetary-scale habitability to the prospect of habitats, microbial ecotones, pathways to biological dispersal, biomass repositories, and their meaning for exploration. Critically, as we search for biosignatures, this focus demonstrates the importance of starting to think of early Mars as a biosphere and vigorously integrating an ecosystem approach to landing site selection and exploration. Key Words: Astrobiology-Biosignatures-Coevolution of Earth and life-Mars. Astrobiology 18, 1-27.

摘要

地球的生物和环境演化是相互交织、不可分割的。这种共同演化已成为天体生物学的一个基本概念,也是寻找地球以外生命的关键。就火星而言,是否发生了共同演化尚不清楚,但分析其中的作用因素表明,每个行星实验都是独特的,无论它们之间存在相似性。早期的地球和火星具有相似的特征。然而,如果火星上存在任何生物过程,它们也必须在独特的环境中进行,包括不可逆转的大气崩溃、更大的气候变化和特定的行星特征。在这方面,火星是一个重要的试验台,可用于比较一组独特的时空变化对类地行星的影响,尽管这颗行星与地球有所不同。关于火星早期环境仍有许多问题尚未得到解答。然而,现有数据集为一个知识框架提供了基础,可以在该框架中探索假设的共同演化模型。在这个框架中,焦点从行星尺度的可居住性转移到了栖息地、微生物生态过渡带、生物扩散途径、生物量储存库及其对探索的意义。至关重要的是,当我们寻找生物特征时,这种焦点表明,开始将早期火星视为一个生物圈并大力整合生态系统方法来选择着陆点和进行探索非常重要。

关键词

天体生物学-生物特征-地球与生命的共同演化-火星。天体生物学 18,1-27。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/398c/5779243/63a6131ddfcb/fig-3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/398c/5779243/3504d59d56b6/fig-1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/398c/5779243/c7a44b5260a5/fig-2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/398c/5779243/63a6131ddfcb/fig-3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/398c/5779243/3504d59d56b6/fig-1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/398c/5779243/c7a44b5260a5/fig-2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/398c/5779243/63a6131ddfcb/fig-3.jpg

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