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Water on Mars and the Prospect of Martian Life

机译:火星上的水与火星生命的前景

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Evidence of water on Mars dates back to the first observations of channeled landscapes made by Mariner 9 and Viking. More recent images from Mars Global Surveyor and Mars Express strikingly confirm that fluids have sculpted the Martian surface at least episodically through its history. The Mars Exploration Rovers Opportunity and Spirit have added evidence for extensive rock-water chemical interactions in the regions where these remote geologists landed, while OMEGA and THEMIS have shown that similar processes took place in many parts of the planet. Because of the close relationship between water and biological activity on Earth, such observations have been taken as hopeful sigps that Mars, as well, might once have supported life and, indeed, might still do so in subterranean oases. There is, however, much more to consider. Water appears to be necessary for life, at least as it exists on Earth and can be contemplated on Mars, but it does not, by itself, insure habitability. In this paper, we review the broader requirements for biological activity as they relate to water and use these to constrain astrobiological inferences about Mars.
机译:火星上水的证据可以追溯到水手9号和维京人对通道景观的首次观察。来自火星全球测量师和火星快车的最新图像惊人地证实,流体至少在其历史上已经在表面上对火星表面进行了雕刻。火星探测漫游者的机遇和精神为这些偏远的地质学家登陆的地区提供了广泛的岩水化学相互作用的证据,而OMEGA和THEMIS则表明在地球的许多地方也发生了类似的过程。由于水与地球上生物活动之间的密切关系,这种观察被认为是有希望的信号,火星也曾经曾经支持过生命,而且实际上仍然可以在地下绿洲中维持生命。但是,还有更多要考虑的问题。水似乎是生命所必需的,至少就像地球上存在的水一样,在火星上也可以考虑到水,但是水本身并不能确保可居住性。在本文中,我们回顾了与水有关的生物学活动的更广泛要求,并使用这些要求来约束有关火星的天体生物学推断。

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