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

Author:

Sun Vivian Z.1ORCID,Hand Kevin P.1ORCID,Stack Kathryn M.1,Farley Ken A.2,Simon Justin I.3ORCID,Newman Claire4ORCID,Sharma Sunanda1,Liu Yang1,Wiens Roger C.5ORCID,Williams Amy J.6,Tosca Nicholas7ORCID,Alwmark Sanna89ORCID,Beyssac Olivier10ORCID,Brown Adrian11ORCID,Calef Fred1ORCID,Cardarelli Emily L.1ORCID,Clavé Elise12ORCID,Cohen Barbara13ORCID,Corpolongo Andrea14ORCID,Czaja Andrew D.14ORCID,Del Sesto Tyler1,Fairen Alberto1516ORCID,Fornaro Teresa17ORCID,Fouchet Thierry18ORCID,Garczynski Brad5,Gupta Sanjeev19,Herd Chris D. K.20ORCID,Hickman‐Lewis Keyron2122,Horgan Briony5ORCID,Johnson Jeffrey23ORCID,Kinch Kjartan8ORCID,Kizovski Tanya24,Kronyak Rachel1ORCID,Lange Robert1,Mandon Lucia18ORCID,Milkovich Sarah1,Moeller Robert1,Núñez Jorge23ORCID,Paar Gerhard25ORCID,Pyrzak Guy1ORCID,Quantin‐Nataf Cathy26,Shuster David L.27,Siljestrom Sandra28,Steele Andrew1329ORCID,Tice Michael30,Toupet Olivier1ORCID,Udry Arya31ORCID,Vaughan Alicia32,Wogsland Brittan33ORCID

Affiliation:

1. Jet Propulsion Laboratory California Institute of Technology Pasadena CA USA

2. California Institute of Technology Pasadena CA USA

3. NASA Johnson Space Center Houston TX USA

4. Aeolis Research Chandler AZ USA

5. Purdue University West Lafayette IN USA

6. Department of Geological Sciences University of Florida Gainsville FL USA

7. University of Cambridge Cambridge UK

8. Niels Bohr Institute University of Copenhagen Copenhagen Denmark

9. Department of Geology Lund University Lund Sweden

10. CNRS Muséum National d'Histoire Naturelle Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie Sorbonne Université Paris France

11. Plancius Research Severna Park MD USA

12. Centre Lasers Intenses et Applications CNRS CEA Université de Bordeaux Bordeaux France

13. NASA Goddard Spaceflight Center Greenbelt MD USA

14. Department of Geology University of Cincinnati Cincinnati OH USA

15. Centro de Astrobiologia (CSIC‐INTA) Madrid Spain

16. Department Astronomy Cornell University Ithaca NY USA

17. INAF‐Astrophysical Observatory of Arcetri Florence Italy

18. LESIA, Observatoire de Paris CNRS Université PSL Sorbonne Université Université Paris Cité Meudon France

19. Imperial College London London UK

20. University of Alberta Edmonton AB Canada

21. Natural History Museum London UK

22. Dipartimento di Scienze Biologiche, Geologiche e Ambientali Università di Bologna Bologna Italy

23. Johns Hopkins University Applied Physics Laboratory Laurel MD USA

24. Brock University St. Catharines ON Canada

25. Joanneum Research, Graz Austria

26. Laboratoire de Géologie de Lyon Université Lyon Villeurbanne France

27. University of California, Berkeley Berkeley CA USA

28. RISE Research Institutes of Sweden Gothenburg Sweden

29. Carnegie Institute Washington Washington DC USA

30. Department of Geology and Geophysics Texas A&M University College Station TX USA

31. University of Nevada Las Vegas NV USA

32. United States Geological Survey Flagstaff AZ USA

33. University of Tennessee Knoxville TN USA

Abstract

AbstractThe 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 Máaz and Séítah 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 Máaz and Séítah formations are igneous in origin and composed of five and two geologic members, respectively. The Séítah formation represents the olivine‐rich cumulate formed from differentiation of a slowly cooling melt or magma body, and the Máaz formation likely represents a separate series of lava flows emplaced after Séítah. The Máaz and Séítah 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 Máaz‐Séítah 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.

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

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