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Overview and Results From the Mars 2020 Perseverance Rover's First Science Campaign on the Jezero Crater Floor
California Institute of Technology, USA.
RISE Research Institutes of Sweden, Materials and Production, Product Realisation Methodology.ORCID iD: 0000-0002-4975-6074
University of Tennessee, USA.
Number of Authors: 492023 (English)In: Journal of Geophysical Research - Planets, ISSN 2169-9097, E-ISSN 2169-9100, Vol. 128, no 6, article id e2022JE007613Article in journal (Refereed) Published
Abstract [en]

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 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.

Place, publisher, year, edition, pages
John Wiley and Sons Inc , 2023. Vol. 128, no 6, article id e2022JE007613
Keywords [en]
Jezero, Mars, Perseverance, rover, crater, emplacement, erosion, exploration
National Category
Natural Sciences
Identifiers
URN: urn:nbn:se:ri:diva-65699DOI: 10.1029/2022JE007613Scopus ID: 2-s2.0-85163299408OAI: oai:DiVA.org:ri-65699DiVA, id: diva2:1786664
Note

 This research was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration (80NM0018D0004). TF acknowledges the Italian Space Agency (ASI) grant agreement ASI/INAF n. 2017-48-H-0. SA acknowledges the Swedish Research Council (Grant 2017-06388). KK acknowledges the Carslberg Foundation Grant CF19-0023. SS acknowledges Swedish National Space Board (contracts 137/19 and 2021-00092).

Available from: 2023-08-09 Created: 2023-08-09 Last updated: 2023-08-09Bibliographically approved

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