Overview and Results From the Mars 2020 Perseverance Rover's First Science Campaign on the Jezero Crater Floor

被引:29
作者
Sun, Vivian Z. [1 ]
Hand, Kevin P. [1 ]
Stack, Kathryn M. [1 ]
Farley, Ken A. [2 ]
Simon, Justin I. [3 ]
Newman, Claire [4 ]
Sharma, Sunanda
Liu, Yang
Wiens, Roger C. [5 ]
Williams, Amy J. [6 ]
Tosca, Nicholas [7 ]
Alwmark, Sanna [8 ,9 ]
Beyssac, Olivier [10 ]
Brown, Adrian [11 ]
Calef, Fred
Cardarelli, Emily L. [1 ]
Clave, Elise [12 ]
Cohen, Barbara [13 ]
Corpolongo, Andrea [14 ]
Czaja, Andrew D. [14 ]
Del Sesto, Tyler [1 ]
Fairen, Alberto [15 ,16 ]
Fornaro, Teresa [17 ]
Fouchet, Thierry [18 ]
Garczynski, Brad [5 ]
Gupta, Sanjeev [19 ]
Herd, Chris D. K. [20 ]
Hickman-Lewis, Keyron [21 ,22 ]
Horgan, Briony [5 ]
Johnson, Jeffrey [23 ]
Kinch, Kjartan
Kizovski, Tanya [24 ]
Kronyak, Rachel [1 ]
Lange, Robert [1 ]
Mandon, Lucia
Milkovich, Sarah [1 ]
Moeller, Robert [1 ]
Nunez, Jorge [23 ]
Paar, Gerhard [25 ]
Pyrzak, Guy [1 ]
Quantin-Nataf, Cathy [26 ]
Shuster, David L. [27 ]
Siljestrom, Sandra [28 ]
Steele, Andrew [13 ,29 ]
Tice, Michael [30 ]
Toupet, Olivier [1 ]
Udry, Arya [31 ]
Vaughan, Alicia [32 ]
Wogsland, Brittan [33 ]
机构
[1] CALTECH, Jet Prop Lab, Pasadena, CA 91125 USA
[2] CALTECH, Pasadena, CA USA
[3] NASA Johnson Space Ctr, Houston, TX USA
[4] Aeolis Res, Chandler, AZ USA
[5] Purdue Univ, W Lafayette, IN USA
[6] Univ Florida, Dept Geol Sci, Gainesville, FL USA
[7] Univ Cambridge, Cambridge, England
[8] Univ Copenhagen, Niels Bohr Inst, Copenhagen, Denmark
[9] Lund Univ, Dept Geol, Lund, Sweden
[10] Sorbonne Univ, Inst Mineral Phys Mat & Cosmochimie, Museum Natl dHist Nat, CNRS, Paris, France
[11] Plancius Res, Severna Pk, MD USA
[12] Univ Bordeaux, Ctr Lasers Intenses & Applicat, CNRS, CEA, Bordeaux, France
[13] NASA Goddard Spaceflight Ctr, Greenbelt, MD USA
[14] Univ Cincinnati, Dept Geol, Cincinnati, OH USA
[15] Ctr Astrobiol CSIC INTA, Madrid, Spain
[16] Cornell Univ, Dept Astron, Ithaca, NY USA
[17] INAF Astrophys Observ Arcetri, Florence, Italy
[18] Univ Paris Cite, Univ PSL, Sorbonne Univ, LESIA,Observ Paris,CNRS, Meudon, France
[19] Imperial Coll London, London, England
[20] Univ Alberta, Edmonton, AB, Canada
[21] Nat Hist Museum, London, England
[22] Univ Bologna, Dipartimento Sci Biol Geolog & Ambientali, Bologna, Italy
[23] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD USA
[24] Brock Univ, St Catharines, ON, Canada
[25] Joanneum Res, Graz, Austria
[26] Univ Lyon, Lab Geol Lyon, Villeurbanne, France
[27] Univ Calif Berkeley, Berkeley, CA USA
[28] RISE Res Inst Sweden, Gothenburg, Sweden
[29] Carnegie Inst Washington, Washington, DC USA
[30] Texas A&M Univ, Dept Geol & Geophys, College Stn, TX USA
[31] Univ Nevada, Las Vegas, NV USA
[32] US Geol Survey, Flagstaff, AZ USA
[33] Univ Tennessee, Knoxville, TN USA
基金
瑞典研究理事会; 美国国家航空航天局;
关键词
Mars; Perseverance; rover; Jezero; RIDGE NETWORKS; NILI FOSSAE; FLUID-FLOW; HISTORY; MINERALOGY; VALLEYS; BEDROCK; SYRTIS; SYSTEM; ROCKS;
D O I
10.1029/2022JE007613
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The Mars 2020 Perseverance rover landed in Jezero crater on 18 February 2021. After a 100-sol period of commissioning and the Ingenuity Helicopter technology demonstration, Perseverance began its first science campaign to explore the enigmatic Jezero crater floor, whose igneous or sedimentary origins have been much debated in the scientific community. This paper describes the campaign plan developed to explore the crater floor's Maaz and Seitah formations and summarizes the results of the campaign between sols 100-379. By the end of the campaign, Perseverance had traversed more than 5 km, created seven abrasion patches, and sealed nine samples and a witness tube. Analysis of remote and proximity science observations show that the Maaz and Seitah formations are igneous in origin and composed of five and two geologic members, respectively. The Seitah formation represents the olivine-rich cumulate formed from differentiation of a slowly cooling melt or magma body, and the Maaz formation likely represents a separate series of lava flows emplaced after Seitah. The Maaz and Seitah rocks also preserve evidence of multiple episodes of aqueous alteration in secondary minerals like carbonate, Fe/Mg phyllosilicates, sulfates, and perchlorate, and surficial coatings. Post-emplacement processes tilted the rocks near the Maaz-Seitah contact and substantial erosion modified the crater floor rocks to their present-day expressions. Results from this crater floor campaign, including those obtained upon return of the collected samples, will help to build the geologic history of events that occurred in Jezero crater and provide time constraints on the formation of the Jezero delta. Plain Language Summary The Mars 2020 Perseverance rover, along with the Ingenuity Helicopter technology demonstration, landed in Jezero crater, Mars on 18 February 2021. Here, we detail results from the first science campaign of the mission, the purpose of which was to explore the enigmatic Jezero crater floor. By the end of the campaign, Perseverance traversed more than 5 km, created seven abrasion patches, and sealed a total of nine samples and a witness tube for return to Earth. Analysis of the rocks in the crater floor revealed two distinct geologic formations, named the Maaz and Seitah formations. Both formations were determined to be igneous in origin, the former likely from a series of lava flows and the latter formed from a slowly cooling melt or magma body. The composition of the Maaz and Seitah formation rocks also indicate that they experienced significant alteration from water in the past, consistent with Jezero crater having once been filled with water. Results from Perseverance's Jezero crater floor campaign, including those obtained upon return of the collected samples to Earth, will help build the geologic history of Jezero crater and reveal its past habitability.
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