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Deliquescence, liquid water, and the search for sources and sinks of methane on Mars

机译:潮解,液态水以及在火星上寻找甲烷的来源和汇

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The recent discoveries of evidence for liquid saline water1'2'3'4 and methane5 on Mars have excited the science community by reviving the possibility of extant microbial life in this nearby planet. Here we report recently discovered photometric and spectral evidence that liquid saline water exists on Mars4. We show that this finding indicates that deliquescence occurs seasonally on some areas of Mars' polar region4. These discoveries support the hypothesis that liquid saline water is ubiquitous in the shallow Martian subsurface. This has important implications for the search for extraterrestrial life because a diverse array of terrestrial microorganisms thrives in highly saline water or brines6'7. We conclude this article by describing in situ and remote sensing instruments for detecting brines in the Martian subsurface and studying their relationship with sources and sinks of trace gases.
机译:最近在火星上发现液态盐水1'2'3'4和甲烷5的证据,通过恢复附近这个星球上现存微生物生命的可能性,激发了科学界的兴趣。在这里,我们报道了最近发现的光度学和光谱学证据,表明Mars4上存在液态盐水。我们表明,这一发现表明潮解在火星极地4的某些区域发生。这些发现支持以下假设:液态火星水在浅层火星地下普遍存在。这对于寻找外星生命具有重要意义,因为各种各样的陆生微生物在高盐度的水或盐水中繁衍生息6'7。本文通过描述用于探测火星地下盐溶液的原位和遥感仪器并研究其与痕量气体源和汇的关系来结束本文。

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