地球上可能保存生物特征的火星相关水文火山环境全球数据库

Geosphere Pub Date : 2024-01-26 DOI:10.1130/ges02712.1
Catheryn H. Ryan, Mariek E. Schmidt, Gordon R. Osinski, Erica A. Massey
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引用次数: 0

摘要

地球上的玄武岩水文火山环境产生丰富的玻璃(菱锰矿),这些玻璃很容易发生变化,是岩石微生物重要的化学能源来源;因此,这些地点对于潜在的生命起源和早期生命研究具有重要意义。在火星上也发现了类似的环境,应将其视为天体生物学研究的潜在目标。地球上更新世到近代的喷火和冰川火山结构包括凝灰岩锥、凝灰岩环、火山口、土雅斯和丁达尔。这些水火山沉积物含有丰富的玻璃,这些玻璃经过不同程度的水热膨胀,有些区域已公布的证据表明存在假定的微生物居住和微生物介导的蚀变,包括微管和颗粒蚀变。我们分析了有关陆地热液火山环境的文献,并创建了一个全球数据库,其中包含 45 个地球上的火山区,其成分、蚀变历史和结构与火星相关。这些地点的地球化学、矿物学以及同期和爆发后的环境条件使它们成为火星类天体生物学研究的合适目标。相关的蚀变产物包括帕拉贡石、沸石、粘土和方解石。其中七个地点有微生物介导的蚀变证据,这可被视为火星模拟背景下的一种有用的生物特征。这些地点是加拿大的威尔斯-格雷-清水火山场;美国的洛克堡火山场、西蛇河平原火山场和乌普萨尔-霍格贝克;冰岛的雷克雅内斯火山场和西部火山区;以及南极洲的卡拉帕斯-努纳塔克。根据这些已确认地点的特性,并将其余 38 个地球火山区与火星上的火山岩进行比较,我们从数据库中特别推荐了 11 个火山区供未来研究之用:新西兰奥克兰和南奥克兰火山区;美国奥胡岛、黑岩沙漠和黑角;加拿大图亚火山区;土耳其卡拉佩纳尔火山区;冰岛韦斯特曼纳埃亚群岛;阿根廷兰卡内洛火山区;亚速尔群岛圣米格尔火山区;以及南极洲努纳塔克冰瀑。我们建议,除了进行地球化学和矿物学分析以确定其岩浆和蚀变特性外,还应对这些地点的钙钛矿凝灰岩样本进行审查,以寻找微生物蚀变的证据。通过研究地球上热液火山环境的岩石记录来推断可居住性和生物改变,我们有助于确定火星相关环境中生命起源、生存和增殖的有利条件。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A global database of Mars-relevant hydrovolcanic environments on Earth with potential biosignature preservation
Basaltic hydrovolcanic environments on Earth produce abundant glass (sideromelane), which readily alters and acts as an important source of chemical energy for lithotrophic microorganisms; as such, these sites are significant for potential origins-of-life and early life research. Similar environments were identified on Mars and should be considered potential targets for astrobiological investigation. Pleistocene to recent phreatomagmatic and glaciovolcanic structures on Earth include tuff cones, tuff rings, maars, tuyas, and tindars. Such hydrovolcanic deposits contain abundant glass that is variably hydrothermally altered, and some areas contain published evidence of putative microbial habitation and microbially mediated alteration, including microtubules and granular alteration. We analyzed the literature on terrestrial hydrovolcanic environments and created a global database of 45 volcanic fields on Earth with compositions, alteration histories, and structures relevant to Mars. These sites have geochemistry, mineralogy, and syn- and post-eruptive environmental conditions that make them suitable targets for Mars-analogue astrobiological research. Relevant alteration products include palagonite, zeolites, clays, and calcite. Seven of these sites have evidence of microbially mediated alteration, which could be considered a useful biosignature in a Mars-analogue context. The sites are Wells Gray–Clearwater Volcanic Field, Canada; Fort Rock Volcanic Field, Western Snake River Plain Volcanic Field, and Upsal Hogback, USA; Reykjanes Volcanic Field and Western Volcanic Zone, Iceland; and Carapace Nunatak, Antarctica. Based on the properties of these already confirmed sites, along with comparing the remaining 38 Earth volcanic fields to volcanic rocks on Mars, we recommend 11 volcanic fields in particular from our database for future investigations: Auckland and South Auckland volcanic fields, New Zealand; O’ahu, Black Rock Desert, and Black Point, USA; Tuya Volcanic Field, Canada; Karapınar Volcanic Field, Türkiye; Vestmannaeyjar Archipelago, Iceland; Llancanelo Volcanic Field, Argentina; São Miguel Volcanic Field, Azores; and Icefall Nunatak, Antarctica. We recommend reviewing palagonitized tuff samples from these sites for evidence of microbial alteration, in addition to performing geochemical and mineralogical analyses to constrain their magmatic and alteration properties. By studying the rock record of hydrovolcanic environments on Earth to infer habitability and biological alteration, we contribute to establishing the conditions favorable for the origination, survival, and proliferation of life in a Mars-relevant setting.
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