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

被引:10
作者
Bosak, T. [1 ]
Shuster, D. L. [2 ]
Scheller, E. L. [1 ]
Siljestroem, S. [3 ]
Zawaski, M. J. [4 ]
Mandon, L. [5 ]
Simon, J. I. [6 ]
Weiss, B. P. [1 ]
Stack, K. M. [7 ]
Mansbach, E. N. [1 ]
Treiman, A. H. [8 ]
Benison, K. C. [9 ]
Brown, A. J. [10 ]
Czaja, A. D. [11 ]
Farley, K. A. [5 ]
Hausrath, E. M. [12 ]
Hickman-Lewis, K. [13 ,14 ]
Herd, C. D. K. [15 ]
Johnson, J. R. [16 ]
Mayhew, L. E. [17 ]
Minitti, M. E. [18 ]
Williford, K. H. [19 ]
Wogsland, B. V. [20 ]
Zorzano, M. -p. [21 ]
Allwood, A. C. [7 ]
Amundsen, H. E. F. [22 ]
Bell, J. F. [23 ]
Benzerara, K. [24 ]
Bernard, S. [24 ]
Beyssac, O. [24 ]
Buckner, D. K. [25 ]
Cable, M. [7 ]
Calef, F. [7 ]
Caravaca, G. [26 ]
Catling, D. C. [27 ]
Clave, E. [28 ]
Cloutis, E. [29 ]
Cohen, B. A. [30 ]
Cousin, A. [26 ]
Dehouck, E. [31 ]
Fairen, A. G. [21 ,32 ]
Flannery, D. T. [33 ]
Fornaro, T. [34 ]
Forni, O. [26 ]
Fouchet, T. [35 ]
Gibbons, E. [36 ]
Gomez, F. Gomez [21 ]
Gupta, S. [37 ]
Hand, K. P. [7 ]
Hurowitz, J. A. [38 ]
机构
[1] MIT, Dept Earth Atmospher & Planetary Sci, Cambridge, MA 02139 USA
[2] Univ Calif Berkeley, Dept Earth & Planetary Sci, Berkeley, CA 94720 USA
[3] RISE Res Inst Sweden, Stockholm, Sweden
[4] Texas A&M Univ, Dept Geol & Geophys, College Stn, TX USA
[5] CALTECH, Div Geol & Planetary Sci, Pasadena, CA USA
[6] NASA Johnson Space Ctr, Ctr Isotope Cosmochem & Geochronol, Houston, TX USA
[7] CALTECH, Jet Prop Lab, Pasadena, CA USA
[8] Lunar & Planetary Inst USRA, Houston, TX USA
[9] West Virginia Univ, Dept Geol & Geog, Morgantown, WV USA
[10] Plancius Res, Severna Pk, MD USA
[11] Univ Cincinnati, Dept Geosci, Cincinnati, OH USA
[12] Univ Nevada, Dept Geosci, Las Vegas, NV USA
[13] Nat Hist Museum, London, England
[14] Univ Bologna, Dipartimento Bigea, Bologna, Italy
[15] Univ Alberta, Dept Earth & Atmospher Sci, Edmonton, AB, Canada
[16] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA
[17] Univ Colorado, Dept Geol Sci, Boulder, CO USA
[18] Framework, Silver Spring, MD USA
[19] Blue Marble Space Inst Sci, Seattle, WA USA
[20] Univ Tennessee, Dept Earth & Planetary Sci, Knoxville, TN USA
[21] CSIC INTA, Ctr Astrobiol CAB, Madrid, Spain
[22] Univ Oslo, Ctr Space Sensors & Syst, Kjeller, Norway
[23] Arizona State Univ, Tempe, AZ USA
[24] Sorbonne Univ, Inst Mineral Phys Mat & Cosmochimie, Museum Natl Hist Nat, CNRS,UMR 7590,IMPMC, Paris, France
[25] Univ Florida, Dept Geol Sci, Gainesville, FL USA
[26] Univ Toulouse, Inst Rech Astrophys & Planetol, CNRS, CNES, Toulouse, France
[27] Univ Washington, Dept Earth & Space Sci, Seattle, WA USA
[28] DLR Inst Opt Sensor Syst, Berlin, Germany
[29] Univ Winnipeg, Winnipeg, MB, Canada
[30] NASA Goddard Space Flight Ctr, Greenbelt, MD USA
[31] Univ Claude Bernard Lyon1, LGL TPE, CNRS, UMR 5276,ENSL,UJM, Villeurbanne, France
[32] Cornell Univ, Dept Astron, Ithaca, NY USA
[33] Queensland Univ Technol, Brisbane, Qld, Australia
[34] INAF Astrophys Observ Arcetri, Florence, Italy
[35] Univ Paris, Sorbonne Univ, Univ PSL, CNRS,LESIA,Observ Paris, Meudon, France
[36] McGill Univ, Montreal, PQ, Canada
[37] Imperial Coll London, Dept Earth Sci & Engn, London, England
[38] SUNY Stony Brook, Dept Geosci, Stony Brook, NY USA
[39] Tech Univ Denmark, Dept Measurement & Instrumentat, DTU Space, Kongens Lyngby, Denmark
[40] Purdue Univ, Earth Atmospher & Planetary Sci, W Lafayette, IN USA
[41] Carnegie Inst Sci, Earth & Planetary Lab, Washington, DC USA
来源
AGU ADVANCES | 2024年 / 5卷 / 04期
基金
加拿大自然科学与工程研究理事会; 欧洲研究理事会; 美国国家航空航天局; 澳大利亚研究理事会;
关键词
Mars; sedimentary geochemistry; planetary geochemistry; origin of life; hydrothermal systems and weathering on other planets; hydrology and fluvial processes; BARBERTON GREENSTONE-BELT; MERIDIANI-PLANUM; GALE CRATER; ISOTOPE FRACTIONATION; MARTIAN METEORITES; ORGANIC-MOLECULES; MAGNESIUM-SULFATE; BURNS FORMATION; MICROBIAL MATS; CLAY-MINERALS;
D O I
10.1029/2024AV001241
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
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. The Perseverance rover collected seven oriented samples of bedrock at the front of the apron-like sediment deposit in the western side of Jezero crater, Mars. Grains and cements in these sedimentary rocks were likely deposited by water or formed in the presence of water in a range of past environments that predate the first signs of life on Earth. This study describes the geologic context and chemical composition of these samples and discusses how, upon return to Earth, they can be used to search for potential signs of past life, understand when and for how long Mars was habitable and why its climate changed. Studies of the returned samples would seek to detect and analyze organic compounds that may be present below the detection limit of the rover instruments, particularly in the finest-grained rocks, and look for the traces of prebiotic processes or past life in all collected samples of sedimentary rocks. Additional analyses can also constrain tell us when, why and for how long the rivers and lakes existed in Jezero crater. The presence of diverse materials in rocks that were deposited by or into water can transform current views of Mars science and habitability outside of Earth. The Perseverance rover has collected seven cores of aqueously deposited sandstones and siltstones at the front of Jezero's western fan Hydrated sulfate, clay and carbonate minerals in the cores record the history of Mars's volatiles and surface habitability The same minerals may preserve organic and inorganic signals of abiotic, prebiotic and biological processes
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页数:21
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