The COSPAR planetary protection policy for missions to Icy Worlds: A review of history, current scientific knowledge, and future directions

IF 2.9 3区 生物学 Q2 ASTRONOMY & ASTROPHYSICS Life Sciences in Space Research Pub Date : 2024-02-08 DOI:10.1016/j.lssr.2024.02.002
P.T. Doran , A. Hayes , O. Grasset , A. Coustenis , O. Prieto-Ballesteros , N. Hedman , O. Al Shehhi , E. Ammannito , M. Fujimoto , F. Groen , J.E. Moores , C. Mustin , K. Olsson-Francis , J. Peng , K. Praveenkumar , P. Rettberg , S. Sinibaldi , V. Ilyin , F. Raulin , Y. Suzuki , B. Schmidt
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Abstract

Recent discoveries related to the habitability and astrobiological relevance of the outer Solar System have expanded our understanding of where and how life may have originated. As a result, the Icy Worlds of the outer Solar System have become among the highest priority targets for future spacecraft missions dedicated to astrobiology-focused and/or direct life detection objectives. This, in turn, has led to a renewed interest in planetary protection concerns and policies for the exploration of these worlds and has been a topic of discussion within the COSPAR (Committee on Space Research) Panel on Planetary Protection. This paper summarizes the results of those discussions, reviewing the current knowledge and the history of planetary protection considerations for Icy Worlds as well as suggesting ways forward. Based on those discussions, we therefore suggest to (1) Establish a new definition for Icy Worlds for Planetary Protection that captures the outer Solar System moons and dwarf planets like Pluto, but excludes more primitive bodies such as comets, centaurs, and asteroids: Icy Worlds in our Solar System are defined as all bodies with an outermost layer that is believed to be greater than 50 % water ice by volume and have enough mass to assume a nearly round shape. (2) Establish indices for the lower limits of Earth life with regards to water activity (LLAw) and temperature (LLT) and apply them into all areas of the COSPAR Planetary Protection Policy. These values are currently set at 0.5 and -28 °C and were originally established for defining Mars Special Regions; (3) Establish LLT as a parameter to assign categorization for Icy Worlds missions. The suggested categorization will have a 1000-year period of biological exploration, to be applied to all Icy Worlds and not just Europa and Enceladus as is currently the case. (4) Have all missions consider the possibility of impact. Transient thermal anomalies caused by impact would be acceptable so long as there is less than 10−4 probability of a single microbe reaching deeper environments where temperature is >LLT in the period of biological exploration. (5) Restructure or remove Category II* from the policy as it becomes largely redundant with this new approach, (6) Establish that any sample return from an Icy World should be Category V restricted Earth return.

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空间研委会冰雪世界任务行星保护政策:历史回顾、当前科学知识和未来方向
有关外太阳系可居住性和天体生物学相关性的最新发现,扩大了我们对生命可能起源于何处和如何起源的认识。因此,外太阳系的冰雪世界已成为未来航天器任务的最优先目标之一,这些任务致力于天体生物学和/或直接生命探测目标。这反过来又引起了人们对行星保护问题和探索这些世界的政策的重新关注,并成为 COSPAR(空间研究委员会)行星保护小组讨论的一个主题。本文总结了这些讨论的结果,回顾了当前的知识和冰雪世界行星保护考虑因素的历史,并提出了前进的方向。根据这些讨论,我们建议 (1) 为行星保护制定一个冰雪世界的新定义,该定义涵盖太阳系外的卫星和矮行星(如冥王星),但不包括更原始的天体(如彗星、半人马和小行星):太阳系中的冰雪世界被定义为所有最外层水冰含量超过 50%(按体积计算)的天体,其质量足以形成近似圆形的形状。(2) 建立地球生命在水活性(LLAw)和温度(LLT)方面的下限指数,并将其应用于 COSPAR 行星保护政策的所有领域。这些数值目前设定为 0.5 和 -28 °C,最初是为界定火星特殊区域而设定的;(3) 将 LLT 确定为参数,以便对冰雪世界任务进行分类。建议的分类将有 1000 年的生物探索期,适用于所有冰雪世界,而不仅仅是目前的木卫二和土卫二。(4) 所有任务都要考虑撞击的可能性。只要在生物探索期间,单个微生物到达温度为低温层的更深环境的概率小于 10-4,就可以接受撞击造成的瞬时热异常。(5) 重新调整或删除政策中的第二类*,因为采用这种新方法后,第二类在很大程度上变得多余, (6) 规定从冰雪世界返回的任何样本都应属于第五类受限制的地球返回样本。
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来源期刊
Life Sciences in Space Research
Life Sciences in Space Research Agricultural and Biological Sciences-Agricultural and Biological Sciences (miscellaneous)
CiteScore
5.30
自引率
8.00%
发文量
69
期刊介绍: Life Sciences in Space Research publishes high quality original research and review articles in areas previously covered by the Life Sciences section of COSPAR''s other society journal Advances in Space Research. Life Sciences in Space Research features an editorial team of top scientists in the space radiation field and guarantees a fast turnaround time from submission to editorial decision.
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