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作 者:Xiuqi Shang Ruifang Huang Weidong Sun
机构地区:[1]Center of Deep Sea Research,Key Laboratory of Ocean Observation and Forecasting,Institute of Oceanology,Chinese Academy of Sciences,Qingdao 266071,China [2]Key Laboratory of Tropical Oceanography,South China Sea Institute of Oceanology,Chinese Academy of Sciences,Guangzhou 510301,China [3]Laboratory for Marine Mineral Resources,Ocean Sciences and Interdisciplinary Frontiers,Laoshan Laboratory,Qingdao 266237,China [4]University of Chinese Academy of Sciences,Beijing 100049,China
出 处:《The Innovation》2024年第6期13-14,共2页创新(英文)
基 金:funded by the Chinese Academy of Sciences(XDA22050103);the Laoshan Laboratory(LSKJ202204100);the National Key Research and Development Program of China(2023YFF0807101);the Taishan Scholar Program(tspd20230609);R.H.is supported by the National Natural Science Foundation of China(41873069).
摘 要:Aromatic compounds have been detected by the Curiosity and Perseverance rovers,suggesting their familiar presence on theMartian surface.1 These organic compounds were previously attributed to water-rock reactions.However,according to our knowledge,no experimental or theoretical evidence substantiates the formation of aromatic compounds purely throughwater-rock reactions in natural conditions.
关 键 词:CONDITIONS SURFACE purely
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