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Going With the Flow: Sedimentary Evolution of the Jezero Western Fan, MarsSedimentary fans developed at the mouths of Martian valleys have been interpreted as the deposits of sustained surface water flow on early Mars building either fluvial fan systems or deltas into standing bodies of water. Whilst much insight has been gleaned from orbital observations, it is only possible to constrain the character, relative timing and persistence of ancient aqueous activity on Mars through detailed on-the-ground interrogation of sedimentary successions built during fan growth. A prominent sedimentary fan deposit at the western margin of Jezero crater – the Western fan – has been interpreted from orbital data/observations to be a river delta that prograded into an ancient lake basin during the Late Noachian-Early Hesperian epochs on Mars (~3.6-3.8 Ga). The Western fan deposit forms a point-sourced depositional system developed at the mouth of Neretva Vallis, a valley system that is incised across the crater rim and has an extensive extra-crater catchment draining over diverse ancient geological units in Nili Planum. The mechanism of crater rim breaching remains unconstrained. Between 2022 and 2023, the Mars 2020 Perseverance rover explored the Western fan, with the objective of characterizing its paleoenvironmental context and collecting a diverse suite of sedimentary rock samples for return to Earth via the Mars Sample Return mission. Perseverance has now completed her traverse across the Western fan having commenced in the distal downstream sectors exposed at the erosional front of the fan and then crossing across its upper exposed surface toward the fan apex region near the mouth of Neretva Vallis. This transect provides a unique window into a Martian sediment routing system at a time when climate conditions permitted the flow of surface water. In this contribution, we review the overall sedimentary architecture of the fan and develop a model for its evolution based on detailed mapping of lithofacies changes across the fan. A first-order synoptic overview is presented.
Document ID
20240000500
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
S Gupta
(Imperial College London London, United Kingdom)
K Stack Morgan ORCID
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
N Mangold ORCID
(Laboratoire de Planétologie et Géosciences Nantes, France)
L R W Ives ORCID
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
S Gwizd ORCID
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
R M E Williams ORCID
(Planetary Science Institute Tucson, Arizona, United States)
N Randazzo ORCID
(University of Alberta Edmonton, Canada)
A J Williams ORCID
(University of Florida Gainesville, United States)
P Russell ORCID
(University of California, Los Angeles Los Angeles, United States)
B H N Horgan ORCID
(Purdue University West Lafayette West Lafayette, United States)
K L Siebach ORCID
(Rice University Houston, United States)
M M Tice ORCID
(Texas A&M University College Station, Texas, United States)
J Hurowitz
(Stony Brook University Stony Brook, New York, United States)
R Barnes
(Imperial College London London, United Kingdom)
C Tate ORCID
(Cornell University Ithaca, United States)
J I Núñez
(Johns Hopkins University Applied Physics Laboratory North Laurel, United States)
S Sholes ORCID
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
L C Kah ORCID
(University of Tennessee at Knoxville Knoxville, United States)
M E Minitti ORCID
(Framework (United States) Silver Spring, Maryland, United States)
G Dromart
(Laboratoire de Géologie de Lyon : Terre, Planètes et Environnement Villeurbanne, France)
J F Bell, III
(Arizona State University Tempe, United States)
J Maki ORCID
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
G Paar ORCID
(Joanneum Research Graz, Austria)
A Annex ORCID
(California Institute of Technology Pasadena, United States)
B P Weiss
(Massachusetts Institute of Technology Cambridge, United States)
O Beyssac
(Institute of Mineralogy, Materials Physics and Cosmochemistry Paris, France)
J Frydenvang ORCID
(University of Copenhagen Copenhagen, Denmark)
M Nachon ORCID
(Texas A&M University College Station, Texas, United States)
R Kronyak
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
V Sun ORCID
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
A J Jones
(Imperial College London London, United Kingdom)
D L Shuster ORCID
(University of California, Berkeley Berkeley, United States)
J I Simon ORCID
(Johnson Space Center Houston, United States)
M P Lamb ORCID
(California Institute of Technology Pasadena, United States)
J P Grotzinger
(California Institute of Technology Pasadena, United States)
S Le Mouélic ORCID
(Laboratoire de Planétologie et Géosciences Nantes, France)
O Gasnault ORCID
(Research Institute in Astrophysics and Planetology Toulouse, France)
R C Wiens ORCID
(Purdue University West Lafayette West Lafayette, United States)
S Maurice
(Research Institute in Astrophysics and Planetology Toulouse, France)
K A Farley ORCID
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
Date Acquired
January 11, 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)
WBS: 203959
CONTRACT_GRANT: 80NM0018D0004
CONTRACT_GRANT: 80NSSC22M0277
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
NASA Peer Committee
Keywords
Mars 2020
Jezero Western Fan
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