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Return to Europa: Overview of the Jupiter Europa orbiter mission

机译:返回欧罗巴:木星欧罗巴轨道器任务概述

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Missions to explore Europa have been imagined ever since the Voyager mission first suggested that Europa was geologically very young. Subsequently, the Galileo spacecraft supplied fascinating new insights into this satellite of Jupiter. Now, an international team is proposing a return to the Jupiter system and Europa with the Europa Jupiter System Mission (EJSM). Currently, NASA and ESA are designing two orbiters that would explore the Jovian system and then each would settle into orbit around one of Jupiter's icy satellites, Europa and Ganymede. In addition, the Japanese Aerospace exploration Agency (JAXA) is considering a Jupiter magnetospheric orbiter and the Russian Space Agency is investigating a Europa lander. The Jupiter Europa Orbiter (JEO) would be the NASA-led portion of the EJSM; JEO would address a very important subset of the complete EJSM science objectives and is designed to function alone or in conjunction with ESA's Jupiter Ganymede Orbiter (JGO). The JEO mission concept uses a single orbiter flight system that would travel to Jupiter by means of a multiple-gravity-assist trajectory and then perform a multi-year study of Europa and the Jupiter system, including 30 months of Jupiter system science and a comprehensive Europa orbit phase of 9 months. The JEO mission would investigate various options for future surface landings. The JEO mission science objectives, as defined by the international EJSM Science Definition Team, include: A. Europa's ocean: Characterize the extent of the ocean and its relation to the deeper interior. B. Europa's ice shell: Characterize the ice shell and any subsurface water, including their heterogeneity, and the nature of surface-ice-ocean exchange. C. Europa's chemistry: Determine global surface compositions and chemistry, especially as related to habitability. D. Europa's geology: Understand the formation of surface features, including sites of recent or current activity, and identify and characterize candidate sites for future in situ exploration. E. Jupiter system: Understand Europa in the context of the Jupiter system. The JEO orbital mission would provide critical measurements to support the scientific and technical selection of future landed options. The primary challenge of a Europa mission is to perform in Jupiter's radiation environment, radiation damage being the life-limiting parameter for the flight system. Instilling a system-level radiation-hardened-by-design approach very early in the mission concept would mitigate the pervasive mission and system-level impacts (including trajectory, configuration, fault protection, operational scenarios, and circuit design) that can otherwise result in runaway growth of cost and mass. This paper addresses the JEO mission concept developed by a joint team from JPL and the Applied Physics Laboratory to address the science objectives defined by an international science definition team formed in 2008, while designing for the Jupiter environment. Published by Elsevier Ltd. on behalf of COSPAR.
机译:自旅行者号首次提出欧罗巴在地质学上还很年轻以来,就一直在想像探索欧罗巴的任务。随后,伽利略号航天器对木星卫星提供了令人着迷的新见解。现在,一个国际团队正提议通过木卫二木星系统任务(EJSM)返回木星系统和木卫二。目前,美国宇航局和欧空局正在设计两个轨道器,它们将探索木星系统,然后每个轨道器将围绕木星的一颗冰卫星(欧罗巴和木卫三)进入轨道。此外,日本航空航天局(JAXA)正在考虑使用木星磁层轨道器,俄罗斯航天局正在研究欧罗巴着陆器。木星欧罗巴轨道器(JEO)将是EJSM的NASA主导部分; JEO将解决整个EJSM科学目标的一个非常重要的子集,并且可以单独运行或与ESA的木星木卫三轨道器(JGO)结合使用。 JEO任务概念使用单轨道飞行系统,该系统将通过多重力辅助轨迹到达木星,然后对欧罗巴和木星系统进行为期多年的研究,包括30个月的木星系统科学和全面的研究。欧罗巴轨道运行阶段为9个月。 JEO任务将研究各种选择,以备将来登陆地面。国际EJSM科学定义团队定义的JEO任务科学目标包括:A.欧罗巴的海洋:表征海洋的范围及其与更深内部的关系。 B.欧罗巴的冰壳:表征冰壳和任何地下水,包括它们的非均质性以及表层-冰层-海洋交换的性质。 C.欧罗巴的化学性质:确定总体表面成分和化学性质,尤其是与可居住性有关的化学成分。 D.欧罗巴的地质:了解表面特征的形成,包括最近或当前活动的地点,并识别和表征候选地点,以供将来进行原位勘探。 E.木星系统:在木星系统的背景下了解欧罗巴。 JEO轨道飞行任务将提供关键的测量数据,以支持对未来着陆方案的科学和技术选择。欧罗巴任务的主要挑战是在木星的辐射环境中执行任务,辐射损害是飞行系统的寿命限制参数。在任务概念的早期就灌输系统级辐射硬化设计方法,将减轻普遍存在的任务和系统级影响(包括轨迹,配置,故障保护,操作场景和电路设计),否则可能会导致成本和质量的失控增长。本文讨论了由JPL和应用物理实验室的联合团队开发的JEO任务概念,以解决2008年成立的国际科学定义小组为木星环境设计时确定的科学目标。由Elsevier Ltd.代表COSPAR发布。

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