Astrobiology Group, ZAA, Technical University Berlin, Berlin, Germany.
Section Geomicrobiology, GFZ German Research Center for Geosciences, Potsdam, Germany.
Astrobiology. 2024 Apr;24(4):397-406. doi: 10.1089/ast.2022.0134. Epub 2023 Oct 18.
The recent and still controversial claim of phosphine detection in the venusian atmosphere has reignited consideration of whether microbial life might reside in its cloud layers. If microbial life were to exist within Venus' cloud deck, these microorganisms would have to be multi-extremophiles enclosed within the cloud aerosol particles. The most straightforward approach for resolving the question of their existence is to obtain samples of the cloud particles and analyze their interior. While developing technology has made sophisticated analysis possible, more detailed information could be obtained by examining samples with instrumentation in dedicated ground-based facilities. Ultimately, therefore, Venus Cloud-level Sample Return Missions will likely be required to resolve the question of whether living organisms exist in the clouds of Venus. Two multiphase mission concepts are currently under development for combining analyses with a sample return component. The Venus Life Finder architecture proposes collection of cloud particles in a compartment suspended from a balloon that floats for weeks at the desired altitude, while the Novel solUtion for Venus explOration and Lunar Exploitation (NUVOLE) concept involves a glider that cruises within the cloud deck for 1200 km collecting cloud aerosol particles through the key regions of interest. Both architectures propose a rocket-driven ascent with the acquired samples transported to a high venusian orbit as a prelude to returning to Earth or the Moon. Both future conceptual missions with their combined phases will contribute valuable information relative to the habitability of the clouds at Venus, but their fulfillment is decades away. We suggest that, in the meantime, a simplification of a glider cloud-level sample collection scenario could be accomplished in a shorter development time at a lower cost. Even if the cloud particles are not organic and show no evidence of living organisms, they would reveal critical insights about the natural history and evolution of Venus.
最近,关于在金星大气中检测到磷化氢的争议性说法再次引发了人们的关注,即微生物是否可能存在于其云层中。如果微生物存在于金星的云层中,这些微生物必须是生活在云气溶胶粒子中的多极端微生物。解决它们存在问题的最直接方法是获取云层粒子样本并分析其内部。虽然技术的发展使得复杂的分析成为可能,但通过使用专用地面设施中的仪器检查样本,可以获得更详细的信息。因此,最终可能需要金星云层样本返回任务来解决金星云层中是否存在生物体的问题。目前正在开发两种多阶段任务概念,将分析与样本返回组件结合在一起。金星生命探测器架构提议在悬浮在气球中的舱室中收集云层粒子,该气球在所需的高度上漂浮数周,而 Novel solUtion for Venus explOration and Lunar Exploitation (NUVOLE) 概念则涉及在云层中巡航 1200 公里的滑翔机,通过关键的感兴趣区域收集云层气溶胶粒子。这两种架构都提议使用火箭驱动上升,将采集到的样本运送到高金星轨道,作为返回地球或月球的前奏。这两个未来的概念任务及其组合阶段将为金星云层的宜居性提供有价值的信息,但它们的实现还需要几十年的时间。我们建议,在此期间,可以在更短的开发时间内以更低的成本简化滑翔机云层样本收集方案。即使云层粒子不是有机的,也没有生命迹象,它们也将揭示金星自然历史和演化的关键见解。