Clark Benton C, Kolb Vera M, Steele Andrew, House Christopher H, Lanza Nina L, Gasda Patrick J, VanBommel Scott J, Newsom Horton E, Martínez-Frías Jesús
Space Science Institute, Boulder, CO 80301, USA.
Department of Chemistry, University of Wisconsin-Parkside, Kenosha, WI 53141, USA.
Life (Basel). 2021 Jun 9;11(6):539. doi: 10.3390/life11060539.
Although the habitability of early Mars is now well established, its suitability for conditions favorable to an independent origin of life (OoL) has been less certain. With continued exploration, evidence has mounted for a widespread diversity of physical and chemical conditions on Mars that mimic those variously hypothesized as settings in which life first arose on Earth. Mars has also provided water, energy sources, CHNOPS elements, critical catalytic transition metal elements, as well as B, Mg, Ca, Na and K, all of which are elements associated with life as we know it. With its highly favorable sulfur abundance and land/ocean ratio, early wet Mars remains a prime candidate for its own OoL, in many respects superior to Earth. The relatively well-preserved ancient surface of planet Mars helps inform the range of possible analogous conditions during the now-obliterated history of early Earth. Continued exploration of Mars also contributes to the understanding of the opportunities for settings enabling an OoL on exoplanets. Favoring geochemical sediment samples for eventual return to Earth will enhance assessments of the likelihood of a Martian OoL.
尽管早期火星的宜居性现已得到充分证实,但其是否适合生命独立起源(OoL)所需的条件仍不太确定。随着探索的不断深入,越来越多的证据表明,火星上存在广泛多样的物理和化学条件,这些条件与那些被假设为地球上生命最初起源环境的条件相似。火星还具备水、能源、CHNOPS元素、关键的催化过渡金属元素,以及硼、镁、钙、钠和钾,所有这些都是我们所知的与生命相关的元素。早期潮湿的火星拥有极为有利的硫含量和陆地/海洋比例,在许多方面优于地球,仍是其自身生命独立起源的主要候选星球。火星相对保存完好的古老表面有助于了解早期地球现已消失的历史中可能存在的类似条件范围。对火星的持续探索也有助于理解系外行星上生命独立起源的环境机会。支持采集地球化学沉积物样本并最终带回地球,将提高对火星生命独立起源可能性的评估。