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欧洲潜水:一项寻找生命的倡议。

Dive Europa: a search-for-life initiative.

作者信息

Naganuma T, Uematsu H

机构信息

Faculty of Applied Biological Science, Hiroshima University, Higashi-hiroshima, Japan.

出版信息

Biol Sci Space. 1998 Jun;12(2):126-30. doi: 10.2187/bss.12.126.

Abstract

Liquid water, underwater volcanoes and possibly life forms have been suggested to be present beneath the estimated 10 km-thick ice shell of Europa the Jovian satellite J2. Europa's possible ocean is estimated to be 100-200km deep. Despite the great depth of the Europa's ocean, hydrostatic pressure at the seafloor would be 130-260 MPa, corresponding to 13-26 km depth of a theoretical Earth's ocean. The hydrostatic pressure is not beyond the edge of existing deep-sea technology. Here we propose exploration of Europa's deep-sea by the use of current technologies, taking a symbolic example of a deep submergence vehicle Shinkai 6500 which dives to a depth of 6.5 km deep (50 km depth of Europa's ocean). Shinkai 6500 is embarkable in the payload bay of the Space Shuttles in terms of size and weight for the transportation to a Low Earth Orbit (LEO). Secondary boost is needed for interplanetary flight from the LEO. On-orbit assembly of the secondary booster is a technological challenge. The International Space Station (ISS) and ISS-related technologies will facilitate the secondary boost. Also, ice shell drilling is a challenge and is needed before the dive into Europa's ocean. These challenges should be overcome during a certain leading time for matured experience in the ISS operation.

摘要

液态水、水下火山以及可能存在的生命形式被认为存在于木卫二(木星的卫星J2)估计10千米厚的冰壳之下。木卫二可能存在的海洋估计有100 - 200千米深。尽管木卫二的海洋深度很大,但海底的静水压力将为130 - 260兆帕,相当于理论上地球海洋13 - 26千米深度处的压力。这种静水压力并未超出现有深海技术的范围。在此,我们提议利用现有技术探索木卫二的深海,以深潜器“深海6500”为例,它能下潜到6.5千米深处(相当于木卫二海洋50千米深处)。就尺寸和重量而言,“深海6500”可搭载于航天飞机的有效载荷舱内,以便运输至近地轨道(LEO)。从近地轨道进行行星际飞行需要二次助推。二次助推器的在轨组装是一项技术挑战。国际空间站(ISS)及与ISS相关的技术将有助于二次助推。此外,冰壳钻探是一项挑战,在潜入木卫二海洋之前就需要进行。在国际空间站运行积累成熟经验的一定准备阶段,应克服这些挑战。

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