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A Maximum Subsurface Biomass on Mars from Untapped Free Energy: CO and H_2 as Potential Antibiosignatures

机译:利用未开发的自由能在火星上产生的最大地下生物量:CO和H_2作为潜在的抗生物签名

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Whether extant life exists in the martian subsurface is an open question. High concentrations of photochemically produced CO and H2 in the otherwise oxidizing martian atmosphere represent untapped sources of biologically useful free energy. These out-of-equilibrium species diffuse into the regolith, so subsurface microbes could use them as a source of energy and carbon. Indeed, CO oxidation and methanogenesis are relatively simple and evolutionarily ancient metabolisms on Earth. Consequently, assuming CO- or H2-consuming metabolisms would evolve on Mars, the persistence of CO and H2 in the martian atmosphere sets limits on subsurface metabolic activity. In this study, we constrain such maximum subsurface metabolic activity on Mars using a one-dimensional photochemical model with a hypothetical global biological sink on atmospheric CO and H2. We increase the biological sink until the modeled atmospheric composition diverges from observed abundances. We find maximum biological downward subsurface sinks of 1.5 × 108 molecules/(cm2·s) for CO and 1.9 × 108 molecules/(cm2·s1) for H2. These convert to a maximum metabolizing biomass of ≲1027 cells or ≤2 × 1011 kg, equivalent to ≤10−4–10−5 of Earth's biomass, depending on the terrestrial estimate. Diffusion calculations suggest that this upper biomass limit applies to the top few kilometers of the martian crust in communication with the atmosphere at low to mid-latitudes. This biomass limit is more robust than previous estimates because we test multiple possible chemoautotrophic ecosystems over a broad parameter space of tunable model variables using an updated photochemical model with precise atmospheric concentrations and uncertainties from Curiosity. Our results of sparse or absent life in the martian subsurface also demonstrate how the atmospheric redox pairs of CO-O2 and H2-O2 may constitute antibiosignatures, which may be relevant to excluding life on exoplanets.
机译:火星表面是否存在现存生命是一个悬而未决的问题。在否则会氧化的火星大气中,高浓度的光化学产生的CO和H2代表了未开发的生物学上有用的自由能来源。这些不平衡的物质扩散到重灰岩中,因此地下微生物可以将它们用作能量和碳的来源。确实,CO氧化和甲烷生成是地球上相对简单且进化上古老的新陈代谢。因此,假设消耗CO或H 2的新陈代谢会在火星上发生,那么火星大气中CO和H 2的持续存在会限制地下代谢活动。在这项研究中,我们使用一维光化学模型限制了火星上这种最大的地下代谢活性,该模型具有假设的全球生物沉入大气CO和H2的假设。我们增加了生物汇,直到模拟的大气成分与观测到的丰度发生偏差为止。我们发现,CO的最大生物向下表面下沉为1.5×108分子/(cm2·s),H2的最大生物向下沉为1.9×108分子/(cm2·s1)。这些转化为最大代谢生物量of1027个细胞或≤2×1011 kg,相当于地球生物量的≤10−4–10−5,这取决于地面估计。扩散计算表明,该生物量上限适用于与中低纬度大气连通的火星地壳的前几公里。该生物量极限比以前的估计值更可靠,因为我们使用具有精确大气浓度和好奇心的不确定性的更新光化学模型,在可调模型变量的广阔参数空间上测试了多种可能的化学自养生态系统。我们在火星地下的生命稀疏或缺乏生命的结果也表明,大气中的CO-O2和H2-O2氧化还原对可能构成抗生物签名,这可能与排除系外行星的生命有关。

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