Origin of water in the Moon  

作　　者：Hejiu Hui Ziyan Han Kang Shuai 

机构地区：[1]State Key Laboratory of Mineral Deposits Research&Lunar and Planetary Science Institute,School of Earth Sciences and Engineering,Nanjing University,China [2]CAS Center for Excellence in Comparative Planetology,China [3]CAS Key Laboratory of Earth and Planetary Physics,Institute of Geology and Geophysics,China

出　　处：《National Science Review》2024年第6期3-5,共3页国家科学评论（英文版）

基　　金：supported by the National Natural Science Foundation of China(42125303);the B-type Strategic Priority Program of the Chinese Academy of Sciences(XDB41000000);the China National Space Administration(D020205).

摘　　要：It has been well known since the Apollo era that the Moon is relatively depleted in volatiles as a result of the Moonformation impact and the subsequent planetary differentiation.The lunar interior was believed to have been extremely dry[1].The discovery of indigenous water(a collective term for H-bearing species OH,H_(2)O,etc.)in various lunar materials[2–5]has driven a paradigm shift in our knowledge of water in the Moon,from a dry to a wet Moon.These discoveries have invoked investigations on the consequences of indigenous water in the lunar interior for the origin of the Moon in the context of giant-impact formation theory[6–8].The origin of this indigenous water in the lunar interior has become key to understanding the formation of the Moon.

关 键 词：INTERIOR COLLECTIVE consequences 

分 类 号：Q935[生物学—微生物学]