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高盐湖泊冰的生物负荷和离子组成:地球上的新型栖息地及其天体生物学意义。

The Bioburden and Ionic Composition of Hypersaline Lake Ices: Novel Habitats on Earth and Their Astrobiological Implications.

机构信息

Thayer School of Engineering, Dartmouth College, Hanover, NH, USA.

School of Earth and Space Exploration, Arizona State University, Pheonix, AZ, USA.

出版信息

Astrobiology. 2022 Aug;22(8):962-980. doi: 10.1089/ast.2021.0078. Epub 2022 Jun 7.

Abstract

We present thermophysical, biological, and chemical observations of ice and brine samples from five compositionally diverse hypersaline lakes in British Columbia's interior plateau. Possessing a spectrum of magnesium, sodium, sulfate, carbonate, and chloride salts, these low-temperature high-salinity lakes are analogs for planetary ice-brine environments, including the ice shells of Europa and Enceladus and ice-brine systems on Mars. As such, understanding the thermodynamics and biogeochemistry of these systems can provide insights into the evolution, habitability, and detectability of high-priority astrobiology targets. We show that biomass is typically concentrated in a layer near the base of the ice cover, but that chemical and biological impurities are present throughout the ice. Coupling bioburden, ionic concentration, and seasonal temperature measurements, we demonstrate that impurity entrainment in the ice is directly correlated to ice formation rate and parent fluid composition. We highlight unique phenomena, including brine supercooling, salt hydrate precipitation, and internal brine layers in the ice cover, important processes to be considered for planetary ice-brine environments. These systems can be leveraged to constrain the distribution, longevity, and habitability of low-temperature solar system brines-relevant to interpreting spacecraft data and planning future missions in the lens of both planetary exploration and planetary protection.

摘要

我们介绍了来自不列颠哥伦比亚内陆高原五个组成不同的高盐湖泊的冰和盐水样本的热物理、生物和化学观测结果。这些低温高盐湖泊拥有一系列镁、钠、硫酸盐、碳酸盐和氯化物盐,是行星冰盐水环境的模拟物,包括欧罗巴和恩克拉多斯的冰壳以及火星上的冰盐水系统。因此,了解这些系统的热力学和生物地球化学可以为高优先级天体生物学目标的演化、可居住性和可探测性提供见解。我们表明,生物量通常集中在冰盖底部附近的一层,但化学和生物杂质存在于整个冰中。我们结合生物负荷、离子浓度和季节性温度测量,证明了冰中的杂质夹带与冰的形成速率和母体流体组成直接相关。我们强调了一些独特的现象,包括盐水过冷、盐水合物沉淀和冰盖内的盐水层,这些对于行星冰盐水环境是重要的过程,需要加以考虑。这些系统可以用来限制低温太阳系盐水的分布、寿命和可居住性,这对于解释航天器数据和在行星探索和行星保护的视角下规划未来任务都具有重要意义。

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