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探索月球水循环。

Exploring the lunar water cycle.

作者信息

Reiss Philipp

机构信息

Technical University of Munich, School of Engineering and Design, Department of Aerospace and Geodesy, Ottobrunn 85521, Germany.

出版信息

Proc Natl Acad Sci U S A. 2024 Dec 24;121(52):e2321065121. doi: 10.1073/pnas.2321065121. Epub 2024 Dec 16.

Abstract

The presence of water on the Moon has been indicated by various remote-sensing observations and analyses of returned samples. Several missions are planned to conduct new in situ research on the lunar surface to directly observe and characterize lunar water. A comprehensive characterization of the present forms of water, their abundance, spatial distribution, temporal variation, and possible origin is required to understand the lunar water cycle and the relevance of individual source and sink mechanisms and transformations between the involved volatile species. These processes extend over vastly different scales, and the governing parameters are often insufficiently constrained by experimental and observational data. Here, I present a brief overview of the current state of knowledge on the lunar water cycle, its relevance for lunar science and exploration, and some of the main challenges of modeling and future in situ analyses aiming to substantially advance the understanding of lunar water occurrences.

摘要

各种遥感观测以及对带回样本的分析表明月球上存在水。计划开展多项任务,在月球表面进行新的实地研究,以直接观测和描述月球水。需要对水的现有形态、丰度、空间分布、时间变化以及可能的来源进行全面描述,以便了解月球水循环以及各个源汇机制的相关性,以及所涉及挥发性物种之间的转化。这些过程跨越了截然不同的尺度,而控制参数往往没有得到实验和观测数据的充分约束。在此,我简要概述一下月球水循环的当前知识状态、其对月球科学和探索的相关性,以及旨在大幅推进对月球水存在情况理解的建模和未来实地分析的一些主要挑战。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/1134/11670188/d244d6083643/pnas.2321065121fig01.jpg

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