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Remarks on Chinese Autonomous Exploration of the Liquid Oceans beneath the Icy Moons’Surfaces of Jupiter System
- XU Xiyu1,2, ZHU Di1, YANG Shuangbao1
Author information
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1. The Key Laboratory of Microwave Remote Sensing, National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China;
2. State Key Laboratory of Remote Sensing Science, Institute of Remote Sensing and Digital Earth, Chinese Academy of Sciences, Beijing 100094, China
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History
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Received |
Revised |
21 Dec 2018 |
09 May 2019 |
Issue Date |
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20 May 2022 |
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Icy Moons of Jupiter System (especially Europa) have abundant exploring value,and they are among the hottest objectives in solar system exploration throughout the world. In this paper,the recent advances in pertinent exploration technology in the international community are summarized, and some science issues, such as sub-surface model, temperature profile, penetration depth,and the influence of icy moons' ionosphere,are addressed. A few new ideas are presented,a preliminary system framework is proposed,and some simulation results of the sub-surface dielectric property are shown. The forthcoming Chinese autonomous Jupiter system exploration mission focusing on the exploration of the liquid oceans beneath the icy moons' surfaces is expected to benefit much from the investigation of new methodology and new configuration in this paper.
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