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The Scientific Value of Collecting Samples From the Jezero Crater RimThe Mars 2020 mission has been conducting ground-based investigation of the geology, habitability, and biosignature preservation potential and collecting samples for return to Earth in Jezero crater, Mars for nearly 3 years. Analysis of these samples will address outstanding questions in Mars science including potential habitability and how and why the climate the interior of the planet evolved through time. As of December 2023, samples of 4 igneous rocks of the Jezero crater floor and 9 sedimentary rocks of the Jezero fan and inner margin, remain on the rover. 15 tubes remain to be filled to enhance the diversity of the cache and broaden the scope of the science questions that can be addressed with returned sample studies.

The next step in the mission is to explore the Jezero crater rim. It will be imperative to investigate and sample the diversity of crater rim rocks because they represent materials from Mars’ most ancient crust older than those sampled in Jezero crater, a diversity of geologic processes, and potential ancient habitable environments that have not yet been investigated or sampled. Ongoing mapping efforts are using orbiter data and long-distance images from Perseverance to identify and interpret the geologic context of the crater rim. Building on this effort and the broader geologic context for the crater rim put forward by previous studies, we identify diverse targets for in situ investigation and potential sampling by Mars 2020.
Document ID
20240000398
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
L. E. Mayhew ORCID
(University of Colorado Boulder Boulder, United States)
C. Quantin-Nataf
(Université de Lyon Lyon, France)
E. Scheller ORCID
(Massachusetts Institute of Technology Cambridge, United States)
J. I. Simon ORCID
(Johnson Space Center Houston, United States)
B. P. Weiss
(Massachusetts Institute of Technology Cambridge, United States)
B. Horgan ORCID
(Purdue University West Lafayette West Lafayette, United States)
M. Deahn ORCID
(Purdue University West Lafayette West Lafayette, United States)
S. Alwmark ORCID
(Lund University Lund, Sweden)
C. C. Bedford ORCID
(Purdue University West Lafayette West Lafayette, United States)
E. M. Hausrath ORCID
(University of Nevada, Las Vegas Las Vegas, Nevada, United States)
A. Klidaras
(Purdue University West Lafayette West Lafayette, United States)
K. M. Stack ORCID
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
K. Farley ORCID
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
C. D. K. Herd ORCID
(University of Alberta Edmonton, Canada)
S. Siljeström ORCID
(RISE Research Institutes of Sweden Gothenburg, Sweden)
M. Wadhwa ORCID
(Arizona State University Tempe, United States)
Date Acquired
January 10, 2024
Publication Date
March 11, 2024
Publication Information
Publisher: Lunar and Planetary Institute
Subject Category
Lunar and Planetary Science and Exploration
Meeting Information
Meeting: 55th Lunar and Planetary Science Conference (LPSC)
Location: The Woodlands, TX
Country: US
Start Date: March 11, 2024
End Date: March 15, 2024
Sponsors: Lunar and Planetary Institute, National Aeronautics and Space Administration
Funding Number(s)
CONTRACT_GRANT: Mars Exploration Program
WBS: 203959
CONTRACT_GRANT: 80NM0018D0004
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
NASA Peer Committee
Keywords
Mars sample return
Mars 2020
Jezero Crater rim
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