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总结
一项基于NASA“卡西尼”号对土星最大卫星土卫六（泰坦）长期观测数据的再分析指出，其冰壳下可能不存在此前设想的全球性液态水海洋。研究认为潮汐形变与重力等证据更符合厚而刚性的冰层结构，内部或仅有局部“半融”泥状层。该结论将影响对土卫六可居住性、甲烷湖泊与地质活动机制的解释，并为后续探测任务制定观测重点提供参考。
正文
Absence Of A Subsurface Ocean On Titan Indicated By Cassini Data astrobiology.com ❄️ Nearly molten ice beneath Titan's surface Techno-Science.net The Ominous Kraken Mare, Titan's Largest Lake, Is Hiding Something Far Deeper Than Scientists Ever Expected The Daily Galaxy Goodbye to everything we thought we knew about Titan-NASA reveals data that completely changes our view of Saturn's moon Unión Rayo New Study Finds 'Slushy Tunnels' in Saturn's Titan International Business Times UK
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