土星の衛星タイタンに微量の生命可能性(Saturn’s Moon Titan Could Harbor Life, But Only a Tiny Amount, Study Finds)

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2025-04-07 アリゾナ大学

アリゾナ大学の研究によると、土星の衛星タイタンの地下海には、生命が存在できる可能性があるものの、生物量はわずか数キログラム程度と推定されました。生物エネルギーモデルを用いた分析では、地下に供給される有機物が限られているため、微生物レベルの生命しか存在できないと考えられています。この研究は、2028年に予定されているNASAのドラゴンフライ・ミッションにおける生命探査の重要な指針となることが期待されています。

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タイタンの地下海におけるグリシン発酵の生存可能性 The Viability of Glycine Fermentation in Titan’s Subsurface Ocean

Antonin Affholder, Peter M. Higgins, Charles S. Cockell, Catherine Neish, Krista M. Soderlund, Michael J. Malaska, Kendra K. Farnsworth, Rosaly M. C. Lopes, Conor A. Nixon, Mohit Melwani Daswani,…
The Planetary Science Journal  Published: 2025 April 7
DOI:10.3847/PSJ/adbc66

土星の衛星タイタンに微量の生命可能性(Saturn’s Moon Titan Could Harbor Life, But Only a Tiny Amount, Study Finds)

Abstract

Energy and nutrient sources for life could be delivered to Titan’s subsurface water ocean from both its surface above and its core below. Organic matter forming de novo in Titan’s atmosphere and depositing on the surface may hydrolyze upon descent into the ocean with impact-generated melt pools sinking through the ice, adding to a primordial inventory released by the core during differentiation and/or across geologic time. This raises the possibility that abiotic organic carbon could fuel heterotrophic carbon assimilation into biomass in Titan’s ocean if it is inhabited. Glycine fermentation is one possible metabolism of interest, because mechanisms exist to transport glycine to Titan’s ocean and anaerobic fermentations do not rely on additional strong oxidants which may not be present on Titan. Using bioenergetic modeling, we show that while conditions favorable to glycine fermentation may exist, they are highly dependent on temperature. Additionally, the ability of that metabolism to fuel a global biosphere is limited by the slow delivery of glycine by impact melt pools (<10 nmolal yr−1 optimistically, with a >1 mmolal primordial component). A total population of 1014–1017 cells (a few kilograms of carbon) can be sustained, amounting to less than 1 cell kg–1 water when diluted through the entire ocean. Constraining notionally detectable biospheres on Titan will therefore require (i) considering localized environments that may concentrate cells, (ii) better characterizing other candidate metabolisms (e.g., degradation of acetylene or polyaromatic hydrocarbons) for quantitative bioenergetic modeling, and (iii) resolving new mechanisms to deliver organics and oxidants for life.

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