火星探测计划
菱铁矿
大气(单位)
地质学
天体生物学
碳酸盐
碳纤维
碳酸盐矿物
火星大气层
地球化学
撞击坑
矿物学
化学
火星人
方解石
材料科学
物理
复合材料
有机化学
复合数
热力学
作者
Benjamin M. Tutolo,Elisabeth M. Hausrath,Edwin S. Kite,E. B. Rampe,T. F. Bristow,Robert T. Downs,A. H. Treiman,T. Peretyazhko,M. T. Thorpe,J. P. Grotzinger,Amelie L. Roberts,P. D. Archer,David J. Des Marais,D. F. Blake,D. T. Vaniman,Shaunna M. Morrison,S. J. Chipera,Robert M. Hazen,R. V. Morris,Valerie Tu
出处
期刊:Science
[American Association for the Advancement of Science]
日期:2025-04-17
卷期号:388 (6744): 292-297
标识
DOI:10.1126/science.ado9966
摘要
Ancient Mars had surface liquid water and a dense carbon dioxide (CO 2 )–rich atmosphere. Such an atmosphere would interact with crustal rocks, potentially leaving a mineralogical record of its presence. We analyzed the composition of an 89-meter stratigraphic section of Gale crater, Mars, using data collected by the Curiosity rover. An iron carbonate mineral, siderite, occurs in abundances of 4.8 to 10.5 weight %, colocated with highly water-soluble salts. We infer that the siderite formed in water-limited conditions, driven by water-rock reactions and evaporation. Comparison with orbital data indicates that similar strata (deposited globally) sequestered the equivalent of 2.6 to 36 millibar of atmospheric CO 2 . The presence of iron oxyhydroxides in these deposits indicates that a partially closed carbon cycle on ancient Mars returned some previously sequestered CO 2 to the atmosphere.
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