有機化合物の発見が土星の衛星エンセラダスの生命可能性を支持(Discovery of organic compounds bolsters case that Saturn’s moon Enceladus could support life)

2025-10-03 ワシントン大学 (UW)

NASA探査機カッシーニのデータを再解析した結果、土星の衛星エンケラドスの噴出物中に新たな有機化合物(エステル、アルケン、エーテル類)が確認された。これらは脂質の構成要素でもあり、生命維持に必要な分子群を示唆する。噴出物は衛星内部の海から放出されたもので、熱水噴出孔の存在も示されている。発見はNature Astronomy誌に掲載され、エンケラドスが生命居住可能環境を備える可能性を一段と強めた。研究はワシントン大学、ベルリン自由大学などの国際チームが実施。

有機化合物の発見が土星の衛星エンセラダスの生命可能性を支持(Discovery of organic compounds bolsters case that Saturn’s moon Enceladus could support life)
Jets of icy water and gas erupt from Enceladus’ south pole. The Cassini space probe captured this photograph and also performed a close flyby of the jets to study their contents. A new analysis of Cassini’s data reveals organic compounds never before identified in the Saturn system.NASA/JPL-Caltech/Space Science Institute

<関連情報>

エンケラドゥスの海から新たに噴出した氷粒中の有機化合物の検出 Detection of organic compounds in freshly ejected ice grains from Enceladus’s ocean

Nozair Khawaja,Frank Postberg,Thomas R. O’Sullivan,Maryse Napoleoni,Sascha Kempf,Fabian Klenner,Yasuhito Sekine,Maxwell Craddock,Jon Hillier,Jonas Simolka,Lucía Hortal Sánchez & Ralf Srama
Nature astronomy  Published:01 October 2025
DOI:https://doi.org/10.1038/s41550-025-02655-y

Abstract

Saturn’s moon Enceladus ejects a plume of ice grains and gases originating from a subsurface ocean via fractures near its south pole. The chemical characterization of organic material in such ice grains was previously conducted via the analysis of mass spectra obtained in Saturn’s E ring by Cassini’s Cosmic Dust Analyzer at impact speeds below 12 km s−1. Here we present a comprehensive chemical analysis of organic-bearing ice grains sampled directly from the plume during a Cassini fly-by of Enceladus (E5) at an encounter speed of nearly 18 km s−1. We again detect aryl and oxygen moieties in these fresh ice grains, as previously identified in older E-ring grains. Furthermore, the unprecedented high encounter speed revealed previously unobserved molecular fragments in Cosmic Dust Analyzer spectra, allowing the identification of aliphatic, (hetero)cyclic ester/alkenes, ethers/ethyl and, tentatively, N- and O-bearing compounds. These freshly ejected species are derived from the Enceladus subsurface, hinting at a hydrothermal origin and involvement in geochemical pathways towards the synthesis and evolution of organics.

1702地球物理及び地球化学
ad
ad
Follow
ad
タイトルとURLをコピーしました