毅力号漫游车在火星杰泽罗陨坑沉积扇面采集的岩石的天体生物学潜力

IF 8.3 Q1 GEOSCIENCES, MULTIDISCIPLINARY
AGU Advances Pub Date : 2024-08-14 DOI:10.1029/2024AV001241
T. Bosak, D. L. Shuster, E. L. Scheller, S. Siljeström, M. J. Zawaski, L. Mandon, J. I. Simon, B. P. Weiss, K. M. Stack, E. N. Mansbach, A. H. Treiman, K. C. Benison, A. J. Brown, A. D. Czaja, K. A. Farley, E. M. Hausrath, K. Hickman-Lewis, C. D. K. Herd, J. R. Johnson, L. E. Mayhew, M. E. Minitti, K. H. Williford, B. V. Wogsland, M.-P. Zorzano, A. C. Allwood, H. E. F. Amundsen, J. F. Bell III, K. Benzerara, S. Bernard, O. Beyssac, D. K. Buckner, M. Cable, F. Calef III, G. Caravaca, D. C. Catling, E. Clavé, E. Cloutis, B. A. Cohen, A. Cousin, E. Dehouck, A. G. Fairén, D. T. Flannery, T. Fornaro, O. Forni, T. Fouchet, E. Gibbons, F. Gomez Gomez, S. Gupta, K. P. Hand, J. A. Hurowitz, H. Kalucha, D. A. K. Pedersen, G. Lopes-Reyes, J. N. Maki, S. Maurice, J. I. Nuñez, N. Randazzo, J. W. Rice Jr., C. Royer, M. A. Sephton, S. Sharma, A. Steele, C. D. Tate, K. Uckert, A. Udry, R. C. Wiens, A. Williams
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引用次数: 0

摘要

毅力号 "漫游车在火星杰泽罗陨石坑西部扇区的裸露底部采集了七个定向沉积岩样本,这些样本的年代可能都比地球上最古老的广泛生命迹象还要久远。这些样本包括含硫酸盐和粘土的泥岩和砂岩、扇前地层较低位置的河流砂岩以及沉积在含硫酸盐地层之上的含碳酸盐砂岩。所有样本都含有水沉淀物质,而且大部分或所有样本都是水沉积物。虽然漫游车仪器还不能确定在扇形前沿的岩石中检测到有机物,但灵敏度更高的地面仪器仍然能够在返回地球的样本中寻找前生物化学反应和过去生命的残留物,并研究火星过去的宜居性。含硫酸盐的水合泥岩最有可能保存有机物和生物特征,而含碳酸盐的砂岩则可用于确定杰泽罗陨石坑何时以及在多长时间内含有液态水。对在扇形前沿采集的样品中存在的硫酸盐、碳酸盐、粘土、磷酸盐和火成岩矿物以及痕量金属和挥发物进行返回样品科学分析,将为了解火星过去的宜居环境、其磁场、大气和气候的演变以及大气和地壳中水、硫和碳的过去和现在的循环提供变革性的见解。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Astrobiological Potential of Rocks Acquired by the Perseverance Rover at a Sedimentary Fan Front in Jezero Crater, Mars

Astrobiological Potential of Rocks Acquired by the Perseverance Rover at a Sedimentary Fan Front in Jezero Crater, Mars

The Perseverance rover has collected seven oriented samples of sedimentary rocks, all likely older than the oldest signs of widespread life on Earth, at the exposed base of the western fan in Jezero crater, Mars. The samples include a sulfate- and clay-bearing mudstone and sandstone, a fluvial sandstone from a stratigraphically low position at the fan front, and a carbonate-bearing sandstone deposited above the sulfate-bearing strata. All samples contain aqueously precipitated materials and most or all were aqueously deposited. Although the rover instruments have not confidently detected organic matter in the rocks from the fan front, the much more sensitive terrestrial instruments will still be able to search for remnants of prebiotic chemistries and past life, and study Mars's past habitability in the samples returned to Earth. The hydrated, sulfate-bearing mudstone has the highest potential to preserve organic matter and biosignatures, whereas the carbonate-bearing sandstones can be used to constrain when and for how long Jezero crater contained liquid water. Returned sample science analyses of sulfate, carbonate, clay, phosphate and igneous minerals as well as trace metals and volatiles that are present in the samples acquired at the fan front would provide transformative insights into past habitable environments on Mars, the evolution of its magnetic field, atmosphere and climate and the past and present cycling of atmospheric and crustal water, sulfur and carbon.

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