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首页> 外文期刊>Planetary and space science >Explorer of Enceladus and Titan (E~2T): Investigating ocean worlds' evolution and habitability in the solar system
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Explorer of Enceladus and Titan (E~2T): Investigating ocean worlds' evolution and habitability in the solar system

机译:土卫二和土卫六探险家(E〜2T):研究海洋世界在太阳系中的演化和宜居性

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Titan, with its organically rich and dynamic atmosphere and geology, and Enceladus, with its active plume, both harbouring global subsurface oceans, are prime environments in which to investigate the habitability of ocean worlds and the conditions for the emergence of life. We present a space mission concept, the Explorer of Enceladus and Titan (E2T), which is dedicated to investigating the evolution and habitability of these Saturnian satellites. E2T is proposed as a medium-class mission led by ESA in collaboration with NASA in response to ESA's M5 Cosmic Vision Call. E2T proposes a focused payload that would provide in-situ composition investigations and high-resolution imaging during multiple flybys of Enceladus and Titan using a solar-electric powered spacecraft in orbit around Saturn. The E2T mission would provide high-resolution mass spectrometry of the plume currently emanating from Enceladus' south polar terrain and of Titan's changing upper atmosphere. In addition, high-resolution infrared (IR) imaging would detail Titan's geomorphology at 50–100 m resolution and the temperature of the fractures on Enceladus' south polar terrain at meter resolution. These combined measurements of both Titan and Enceladus would enable the E2T mission scenario to achieve two major scientific goals: 1) Study the origin and evolution of volatile-rich ocean worlds; and 2) Explore the habitability and potential for life in ocean worlds. E2T's two high-resolution time-of-flight mass spectrometers would enable resolution of the ambiguities in chemical analysis left by the NASA/ESA/ASI Cassini-Huygens mission regarding the identification of low-mass organic species, detect high-mass organic species for the first time, further constrain trace species such as the noble gases, and clarify the evolution of solid and volatile species. The high-resolution IR camera would reveal the geology of Titan's surface and the energy dissipated by Enceladus' fractured south polar terrain and plume in detail unattainable by the Cassini mission.
机译:土卫六拥有丰富的有机和动态的大气和地质学,土卫二拥有活跃的羽状生物,它们都具有全球地下海洋,是研究海洋世界的宜居性和生命出现条件的主要环境。我们提出了一个太空任务概念,即土卫二和土卫六(E2T)探险家,致力于研究这些土星卫星的演化和可居住性。 E2T是ESA与NASA共同发起的一项中型任务,旨在响应ESA的M5 Cosmic Vision Call。 E2T提出了一种集中的有效载荷,该载荷将使用土星周围轨道上的太阳能航天器在土卫二和土卫六的多次飞越过程中提供原位成分研究和高分辨率成像。 E2T任务将对当前从土卫二的南极地形和土卫六不断变化的高层大气中喷出的烟流进行高分辨率质谱分析。此外,高分辨率的红外(IR)成像将以50-100m的分辨率详细显示泰坦的地貌,并以米的分辨率详细显示土卫二的南极地形上的裂缝温度。泰坦和土卫二的这些综合测量将使E2T任务场景实现两个主要的科学目标:1)研究富含挥发物的海洋世界的起源和演化; 2)探索海洋世界中的可居住性和生命潜力。 E2T的两台高分辨率飞行时间质谱仪将能够解决NASA / ESA / ASI卡西尼-惠更斯飞行任务在鉴定低质量有机物种,检测高质量有机物种方面留下的化学分析中的歧义。第一次,进一步限制稀有气体等微量物质,并澄清固体和挥发性物质的演变。高分辨率的红外热像仪将详细显示土卫六表面的地质情况以及土卫二破裂的南极地形和羽流所消耗的能量,这是卡西尼号任务无法实现的。

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