Water and other volatiles on Mars  

作　　者：Sen Hu Yubing Gao Zhan Zhou Liang Gao Yangting Lin 

机构地区：[1]Key Laboratory of the Earth and Planetary Physics,Institute of Geology and Geophysics,Chinese Academy of Sciences,China [2]College of Earth and Planetary Sciences,University of Chinese Academy of Sciences,China

出　　处：《National Science Review》2024年第6期5-7,共3页国家科学评论（英文版）

基　　金：supported by the National Key Research and Development Program(2022YFF0503202);the National Natural Science Foundation of China(41973062);the key research program of the Institute of Geology and Geophysics,Chinese Academy of Sciences(IGGCAS-202204 and 201904).

摘　　要：Mars,the intriguing red planet,is one of the planets most similar to the Earth in oursolarsystem.Itiswidely accepted that Mars could have had a warm and wet climate in its early history supported by numerous lines of evidence,e.g.topography,canyons,outflow channels,presence of phyllosilicates and evaporative salts,sedimentary formation,and many others(e.g.[1]),and thus Mars is believed to once have a potentially habitable environment which could be able to supply fundamental conditions for the evolution of potential lives.Therefore,discovery of biosignatures of potential life on Mars is becoming the top scientific objective in planetary sciences.

关 键 词：SEDIMENTARY TOPOGRAPHY PLANETARY 

分 类 号：V476.4[航空宇航科学与技术—飞行器设计]