Proposed Missions to Collect Samples for Analyzing Evidence of Life in the Venusian Atmosphere.

IF 3.5 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Astrobiology Pub Date : 2024-04-01 Epub Date: 2023-10-18 DOI:10.1089/ast.2022.0134
Dirk Schulze-Makuch, Louis N Irwin, Troy Irwin
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Abstract

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 in situ 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 in situ 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.

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收集样本以分析金星大气中生命证据的拟议任务。
最近在金星大气中检测到磷化氢的说法仍然存在争议,这重新引发了人们对微生物生命是否存在于云层中的思考。如果微生物生命存在于金星的云层中,这些微生物必须是封闭在云层气溶胶颗粒中的多极端微生物。解决云粒子存在问题的最直接方法是获取云粒子的样本并分析其内部。虽然技术的发展使复杂的现场分析成为可能,但可以通过在专用地面设施中使用仪器检查样本来获得更详细的信息。因此,最终可能需要金星云层级别的样本返回任务来解决金星云层中是否存在生物的问题。目前正在开发两个多阶段任务概念,用于将现场分析与样本返回组件相结合。Venus Life Finder架构建议在一个悬浮在气球上的隔间中收集云粒子,气球在所需高度漂浮数周,而“金星探测和月球开发新解决方案”(NUVOLE)概念涉及一架滑翔机,该滑翔机在云层中巡航1200 公里,通过感兴趣的关键区域收集云气溶胶颗粒。这两种结构都提出了一种火箭驱动的上升方式,将采集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,但它们的实现还有几十年的时间。同时,我们建议,可以在更短的开发时间内以更低的成本简化滑翔机云级样本采集场景。即使云粒子不是有机的,也没有显示出活生物体的证据,它们也会揭示出对金星自然历史和进化的重要见解。
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来源期刊
Astrobiology
Astrobiology 生物-地球科学综合
CiteScore
7.70
自引率
11.90%
发文量
100
审稿时长
3 months
期刊介绍: Astrobiology is the most-cited peer-reviewed journal dedicated to the understanding of life''s origin, evolution, and distribution in the universe, with a focus on new findings and discoveries from interplanetary exploration and laboratory research. Astrobiology coverage includes: Astrophysics; Astropaleontology; Astroplanets; Bioastronomy; Cosmochemistry; Ecogenomics; Exobiology; Extremophiles; Geomicrobiology; Gravitational biology; Life detection technology; Meteoritics; Planetary geoscience; Planetary protection; Prebiotic chemistry; Space exploration technology; Terraforming
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