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Sampling the Margin Unit of Jezero Crater, Mars for Future Mars Sample ReturnMars 2020 Perseverance rover is currently exploring Jezero crater, which contains an ancient lake-delta system with a high potential for past habitability. One of Perseverance’s primary science goals is to collect a set of scientifically return-worthy samples for return to Earth (Mars Sample Return; MSR). Between February 2021 and December 2023, Perseverance has sealed 23 tubes containing 20 rock cores, 2 regolith samples and one atmosphere sample. All rock and regolith samples are accompanied by a set of observations (Sample Threshold Observation Protocol, the STOP List) performed on abrasion patches or regolith near each sample collection site. These observations are documented in the Initial Reports and the Sample Dossier (https://pds-geosciences.wustl.edu/missions/mars2020/returned_sample_science.htm). Here we provide an overview of the samples collected during the Margin campaign.

The Margin unit is situated interior and adjacent to the western crater rim and exhibits a strong carbonate signal from orbital reflectance spectroscopy. Stratigraphically the unit lies beneath the previously explored curvilinear and blocky units of the fan top and is therefore older than those units. Based on its position near the crater rim and the strong carbonate detections it has been proposed to be a shoreline deposit with possible lacustrine carbonates. Alternative hypotheses include pyroclastic, fluviolacustrine and aeolian deposits. Based on rover observations a lacustrine shoreline deposit seems most likely. The planning of the Margin campaign took place during the summer of 2023, and 3-5 samples were baselined to be collected.

Exploration of the Margin unit began in September 2023 and so far, two samples have been collected: the Pelican Point core at the Hans Amundsen Memorial Workspace in the Mandu Wall region, and the Lefroy Bay core at Lake Newell in the Turquoise Bay region (Fig. 1). The associated abrasion patches are Amherst Point (Pelican Point) and Bills Bay (Lefroy Bay). Mandu Wall is interpreted to be stratigraphically lower than Turquoise Bay based on topography.
Document ID
20240000403
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
S Siljeström ORCID
(RISE Research Institutes of Sweden Gothenburg, Sweden)
K A Farley ORCID
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
T Bosak ORCID
(Massachusetts Institute of Technology Cambridge, United States)
F J Calef, III ORCID
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
A D Czaja ORCID
(University of Cincinnati Cincinnati, Ohio, United States)
B Garcynski
(Western Washington University Bellingham, United States)
E M Hausrath ORCID
(University of Nevada, Las Vegas Las Vegas, Nevada, United States)
C D K Herd ORCID
(University of Alberta Edmonton, Canada)
B Horgan ORCID
(Purdue University West Lafayette West Lafayette, United States)
L E Mayhew ORCID
(University of Colorado Boulder Boulder, United States)
N Randazzo ORCID
(University of Alberta Edmonton, Canada)
S Sholes ORCID
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
D L Shuster ORCID
(University of California, Berkeley Berkeley, United States)
J I Simon ORCID
(Johnson Space Center Houston, United States)
K M Stack ORCID
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
B P Weiss
(Massachusetts Institute of Technology Cambridge, United States)
M -P Zorzano ORCID
(Centro de Astrobiología Torrejón de Ardoz, Spain)
A C Allwood ORCID
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
J Bell
(Arizona State University Tempe, United States)
R Bhartia ORCID
(Photon Systems (United States) Covina, California, United States)
E Clavé ORCID
(German Aerospace Center Cologne, Germany)
J Hurowitz
(Stony Brook University Stony Brook, New York, United States)
J Johnson
(Johns Hopkins University Applied Physics Laboratory North Laurel, United States)
Y Liu
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
G Lopez-Reyes ORCID
(University of Valladolid Valladolid, Spain)
J Maki ORCID
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
L Mandon ORCID
(California Institute of Technology Pasadena, United States)
E N Mansbach ORCID
(Massachusetts Institute of Technology Cambridge, United States)
E Moreland ORCID
(Rice University Houston, United States)
L P O'Neil ORCID
(Texas A&M University College Station, Texas, United States)
A C Pascuzzo ORCID
(Malin Space Science Systems (United States) San Diego, California, United States)
E Ravanis ORCID
(University of Hawaiʻi at Mānoa Honolulu, United States)
P Russell ORCID
(University of California, Los Angeles Los Angeles, United States)
S Sharma ORCID
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
K Siebach ORCID
(Rice University Houston, United States)
A Steele ORCID
(Carnegie Institution for Science Washington, United States)
M M Tice ORCID
(Texas A&M University College Station, Texas, United States)
K H Williford ORCID
(Blue Marble Space Institute of Science Seattle, Washington, United States)
R C Wiens ORCID
(Purdue University West Lafayette West Lafayette, United States)
A Udry ORCID
(University of Nevada, Las Vegas Las Vegas, Nevada, 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
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