Cadmus: a Europa lander concept

R. Thompson, S. Francis, R. Olsen, M. Parsons, R. Coffman, R. Braun
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Abstract

The Cadmus mission responds to the need for a Europa surface exploration mission in the 2021 time frame that complements and extends the science performed by the Jupiter icy moons orbiter (JIMO) and Galileo spacecraft. Cadmus will help prepare for future subsurface and sample return missions. Europa is one of the most intriguing outer solar system planetary bodies due to the compelling evidence that an ocean of salty water exists approximately 20 km beneath the surface. This liquid water could make Europa a haven for life. The NASA Office of Space Science (OSS) has identified the search for life in the solar system and the resources necessary to support extraterrestrial life as an important area of study. The Cadmus mission investigates the habitability of Europa from the surface to determine the likelihood that life exists on the moon. By studying the crustal dynamics of the moon, the Cadmus mission assesses the extent to which a flux of water and ice exists between the possible subsurface ocean and the surface. Cadmus investigates the presence of nutrients and signs of energy resources in the crustal ice and also assesses the environmental suitability of the Europa environment to the evolution and sustainability of life. To reduce mission operations cost and complexity the mission architecture includes two landers that will land on the surface independently and utilize a high degree of autonomy.
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卡德摩斯:木卫二着陆器的概念
卡德摩斯任务响应了2021年木卫二表面探测任务的需求,补充和扩展了木星冰卫星轨道器(JIMO)和伽利略航天器所执行的科学。卡德摩斯将帮助为未来的地下和样本返回任务做准备。欧罗巴是太阳系外最有趣的行星体之一,因为有令人信服的证据表明,在地表下大约20公里处存在着一个咸水海洋。这些液态水可能使木卫二成为生命的天堂。美国宇航局空间科学办公室(OSS)已经确定在太阳系中寻找生命和支持外星生命所需的资源是一个重要的研究领域。卡德摩斯任务从表面调查木卫二的可居住性,以确定月球上存在生命的可能性。通过研究月球的地壳动力学,卡德摩斯任务评估了可能存在的地下海洋和地表之间的水和冰的流动程度。卡德摩斯调查了地壳冰中营养物质的存在和能量资源的迹象,并评估了木卫二环境对生命进化和可持续性的环境适应性。为了降低任务运行成本和复杂性,任务架构包括两个着陆器,它们将独立降落在地面上,并利用高度的自主性。
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