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《针对冰冷世界任务的 COSPAR 行星保护政策:历史回顾、当前科学知识和未来方向》。

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

机构信息

Department of Geology and Geophysics, Louisiana State, Baton Rouge, LA, USA.

Cornell University, Ithaca, NY, 14853-6801, USA.

出版信息

Life Sci Space Res (Amst). 2024 May;41:86-99. doi: 10.1016/j.lssr.2024.02.002. Epub 2024 Feb 8.

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 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.

摘要

最近在外太阳系的可居住性和天体生物学相关性方面的发现扩展了我们对生命可能起源的地点和方式的理解。因此,外太阳系的冰冷世界已成为未来专注于天体生物学和/或直接生命探测目标的航天器任务的最高优先目标之一。这反过来又重新引起了人们对这些世界探索的行星保护关注和政策的兴趣,并成为 COSPAR(空间研究委员会)行星保护小组讨论的主题。本文总结了这些讨论的结果,回顾了冰冷世界的行星保护考虑因素的当前知识和历史,并提出了前进的方向。基于这些讨论,我们因此建议:(1)为行星保护建立一个新的冰冷世界定义,该定义涵盖了外太阳系的卫星和矮行星,如冥王星,但不包括更原始的天体,如彗星、半人马座和小行星:我们太阳系中的冰冷世界定义为所有具有最外层体积大于 50%的水冰且具有足够质量以呈现近圆形的天体。(2)建立与水活性(LLAw)和温度(LLT)有关的地球生命下限指标,并将其应用于 COSPAR 行星保护政策的所有领域。这些值目前设定为 0.5 和-28°C,最初是为定义火星特殊区域而设定的;(3)将 LLT 作为为冰冷世界任务分配分类的参数。建议的分类将有 1000 年的生物探索期,适用于所有冰冷世界,而不仅仅是 Europa 和 Enceladus,就像目前的情况一样。(4)让所有任务都考虑到撞击的可能性。只要在生物探索期间,温度>LLT 的深部环境中单个微生物的到达概率小于 10%,则由撞击引起的短暂热异常是可以接受的。(5)根据这种新方法,使政策中的 II*类结构或移除,因为它变得冗余;(6)确定从冰冷世界返回的任何样本都应受 V 类限制,禁止返回地球。

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