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

Authors :
Vivian Z. Sun
Kevin P. Hand
Kathryn M. Stack
Ken A. Farley
Justin I. Simon
Claire Newman
Sunanda Sharma
Yang Liu
Roger C. Wiens
Amy J. Williams
Nicholas Tosca
Sanna Alwmark
Olivier Beyssac
Adrian Brown
Fred Calef
Emily L. Cardarelli
Elise Clavé
Barbara Cohen
Andrea Corpolongo
Andrew D. Czaja
Tyler Del Sesto
Alberto Fairen
Teresa Fornaro
Thierry Fouchet
Brad Garczynski
Sanjeev Gupta
Chris D. K. Herd
Keyron Hickman-Lewis
Briony Horgan
Jeffrey Johnson
Kjartan Kinch
Tanya Kizovski
Rachel Kronyak
Robert Lange
Lucia Mandon
Sarah Milkovich
Robert Moeller
Jorge Núñez
Gerhard Paar
Guy Pyrzak
Cathy Quantin-Nataf
David L. Shuster
Sandra Siljestroem
Andrew Steele
Michael Tice
Olivier Toupet
Arya Udry
Alicia Vaughan
Brittan Wogsland
Source :
Journal of Geophysical Research: Planets. 128(6)
Publication Year :
2023
Publisher :
United States: NASA Center for Aerospace Information (CASI), 2023.

Abstract

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.

Details

Language :
English
ISSN :
21699100 and 21699097
Volume :
128
Issue :
6
Database :
NASA Technical Reports
Journal :
Journal of Geophysical Research: Planets
Notes :
203959, , 80NM0018D0004, , ASI/ INAF 2017-48-H-0, , SRC 2017-06388, , CF19-0023, , Swedish National Space Board 137/19, , Swedish National Space Board 2021-00092
Publication Type :
Report
Accession number :
edsnas.20230016431
Document Type :
Report
Full Text :
https://doi.org/10.1029/2022JE007613