Aqueously altered igneous rocks sampled on the floor of Jezero crater, Mars

被引：86

作者：

Farley, K. A. ^{[1
]}

Stack, K. M. ^{[2
]}

Shuster, D. L. ^{[3
]}

Horgan, B. H. N. ^{[4
]}

Hurowitz, J. A. ^{[5
]}

Tarnas, J. D. ^{[2
]}

Simon, J. I. ^{[6
]}

Sun, V. Z. ^{[2
]}

Scheller, E. L. ^{[1
]}

Moore, K. R. ^{[1
]}

McLennan, S. M. ^{[5
]}

Vasconcelos, P. M. ^{[7
]}

Wiens, R. C. ^{[8
,67
]}

Treiman, A. H. ^{[9
]}

Mayhew, L. E. ^{[10
]}

Beyssac, O. ^{[11
]}

Kizovski, T. V. ^{[12
]}

Tosca, N. J. ^{[13
]}

Williford, K. H. ^{[14
]}

Crumpler, L. S. ^{[15
]}

Beegle, L. W. ^{[2
]}

Bell, J. F., III ^{[16
]}

Ehlmann, B. L. ^{[1
]}

Liu, Y. ^{[2
]}

Maki, J. N. ^{[2
]}

Schmidt, M. E.

Allwood, A. C. ^{[2
]}

Amundsen, H. E. F. ^{[17
]}

Bhartia, R. ^{[18
]}

Bosak, T. ^{[19
]}

Brown, A. J. ^{[20
]}

Clark, B. C. ^{[21
]}

Cousin, A. ^{[22
]}

Forni, O. ^{[22
]}

Gabriel, T. S. J. ^{[2
]}

Goreva, Y. ^{[2
]}

Gupta, S. ^{[2
]}

Hamran, S. -E. ^{[24
]}

Herd, C. D. K. ^{[25
]}

Hickman-Lewis, K. ^{[26
,27
]}

Johnson, J. R. ^{[28
]}

Kah, L. C. ^{[29
]}

Kelemen, P. B. ^{[30
]}

Kinch, K. B. ^{[31
]}

Mandon, L. ^{[32
]}

Mangold, N. ^{[33
]}

Quantin-Nataf, C. ^{[34
]}

Rice, M. S. ^{[35
]}

Russell, P. S. ^{[36
]}

Sharma, S. ^{[2
]}

机构：

[1] CALTECH, Div Geol & Planetary Sci, Pasadena, CA USA

[2] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA

[3] Univ Calif Berkeley, Dept Earth & Planetary Sci, Berkeley, CA 94720 USA

[4] Purdue Univ, Dept Earth Atmospher & Planetary Sci, W Lafayette, IN 47907 USA

[5] SUNY Stony Brook, Dept Geosci, Stony Brook, NY 11794 USA

[6] NASA Johnson Space Ctr, Astromaterials Res & Explorat Sci Div, Ctr Isotope Cosmochem & Geochronol, Houston, TX 77058 USA

[7] Univ Queensland, Sch Earth & Environm Sci, Brisbane, Qld 4072, Australia

[8] Los Alamos Natl Lab, Planetary Explorat Team, Los Alamos, NM 87545 USA

[9] Univ Space Res Assoc, Lunar & Planetary Inst, Houston, TX 77058 USA

[10] Univ Colorado, Dept Geol Sci, Boulder, CO 80309 USA

[11] Sorbonne Univ, Ctr Natl Rech Sci, Inst Mineral Phys Mat & Cosmochimie, F-75005 Paris, France

[12] Brock Univ, Dept Earth Sci, St Catharines, ON L2S 3A1, Canada

[13] Univ Cambridge, Dept Earth Sci, Cambridge CB2 3EQ, England

[14] Blue Marble Space Inst Sci, Seattle, WA 98104 USA

[15] New Mexico Museum Nat Hist & Sci, Albuquerque, NM 87106 USA

[16] Arizona State Univ, Sch Earth & Space Explorat, Tempe, AZ 85287 USA

[17] Univ Oslo, Ctr Space Sensors & Syst, N-2007 Kjeller, Norway

[18] Photon Syst Inc, Covina, CA 91725 USA

[19] MIT, Dept Earth Atmospher & Planetary Sci, Cambridge, MA 02139 USA

[20] Plancius Res, Severna Pk, Severna Park, MD 21146 USA

[21] Space Sci Inst, Boulder, CO 80301 USA

[22] Univ Toulouse 3 Paul Sabatier, Ctr Natl Rech Sci, Ctr Natl Etude Spatiale, Inst Rech Astrophys & Planetol, F-31400 Toulouse, France

[23] US Geol Survey, Astrogeol Sci Ctr, Flagstaff, AZ 86001 USA

[24] Imperial Coll London, Dept Earth Sci & Engn, London SW7 2AZ, England

[25] Univ Alberta, Dept Earth & Atmospher Sci, Edmonton, AB T6G 2E3, Canada

[26] Nat Hist Museum, Department Earth Sci, London SW7 5BD, England

[27] Univ Bologna, Dipartimento Sci Biol Geol & Ambientali, I-40126 Bologna, Italy

[28] Johns Hopkins Univ Appl Phys Lab, Laurel, MD 20723 USA

[29] Univ Tennessee, Dept Earth & Planetary Sci, Knoxville, TN 37996 USA

[30] Columbia Univ, Dept Earth & Environm Sci, Lamont Doherty Earth Observ, Palisades, NY 10964 USA

[31] Univ Copenhagen, Niels Bohr Inst, DK-1350 Copenhagen, Denmark

[32] Sorbonne Univ, Univ Paris Diderot, Ctr Natl Rech Sci, Lab Etudes Spati & Instrumentat Astro,Observ Pari, F-92195 Meudon, France

[33] Nantes Univ, Univ Angers, Ctr Natl Rech Sci, Laboratoire Planetol & Geosci, F-44000 Nantes, France

[34] Univ Lyon, Univ Claude Bernard Lyon1, Univ Jean Monnet St Etienne, Lab Geol Lyon,Ecole Normale Superieure Lyon,Ctr N, F-69622 Villeurbanne, France

[35] Western Washington Univ, Dept Geol, Bellingham, WA 98225 USA

[36] Univ Calif Los Angeles, Dept Earth Planetary & Space Sci, Los Angeles, CA 90095 USA

[37] Res Inst Sweden, Dept Metrol Text & Med Technol, S-11486 Stockholm, Sweden

[38] Earth & Planetary Lab, Carnegie Sci, Washington, DC 20015 USA

[39] Cornell Univ, Cornell Ctr Astrophys & Planetary Sci, Ithaca, NY 14853 USA

[40] Univ Florida, Det Geol Sci, Gainesville, FL 32611 USA

[41] Univ Hawai Manoa, Hawai Inst Geophys & Planetol, Honolulu, HI 96822 USA

[42] Univ Grenoble Alpes, Ctr Natl Rech Sci, Inst Planetol & Astrophys Grenoble, F-38000 Grenoble, France

[43] NASA Johnson Space Ctr, Houston, TX 77058 USA

[44] Univ Bordeaux, Ctr Natl Rech Sci, Ctr Lasers Intenses & Applicat, Commissariat Ienergie Atom, F-33400 Bordeaux, France

[45] Univ Winnipeg, Ctr Terr & Planetary Explorat, Winnipeg, MB R3B 2E9, Canada

[46] NASA Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

[47] Univ Cincinnati, Dept Geol, Cincinnati, OH 45221 USA

[48] Univ Libre Bruxelles, Lab G Time, B-1050 Brussels, Belgium

[49] Consejo Super Investigaciones Cient Inst Nacl Tec, Ctr Astrobiol, Madrid 28850, Spain

[50] Cornell Univ, Dept Astron, Ithaca, NY 14853 USA

来源：

SCIENCE | 2022年 / 377卷 / 6614期

基金：

欧洲研究理事会; 澳大利亚研究理事会; 加拿大自然科学与工程研究理事会;

关键词：

LITHOAUTOTROPHIC MICROBIAL ECOSYSTEMS; MINERAL CARBONATION; BASIN LAKES; OLIVINE; SYSTEM; DEPOSITS; BEDROCK; SURFACE; VALLEY; HALITE;

D O I：

10.1126/science.abo2196

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

The Perseverance rover landed in Jezero crater, Mars, to investigate ancient lake and river deposits. We report observations of the crater floor, below the crater's sedimentary delta, finding that the floor consists of igneous rocks altered by water. The lowest exposed unit, informally named Seitah, is a coarsely crystalline olivine-rich rock, which accumulated at the base of a magma body. Magnesium-iron carbonates along grain boundaries indicate reactions with carbon dioxide-rich water under water-poor conditions. Overlying Seitah is a unit informally named Maaz, which we interpret as lava flows or the chemical complement to Seitah in a layered igneous body. Voids in these rocks contain sulfates and perchlorates, likely introduced by later near-surface brine evaporation. Core samples of these rocks have been stored aboard Perseverance for potential return to Earth.

引用

页码：1512 / +

页数：12

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