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An Orbital Photogeologic Map of the Jezero Crater Rim: Diverse Targets for Mars 2020 Future Exploration. The Perseverance rover on the Mars 2020 mission is currently collecting samples in Jezero crater for potential future return to Earth by the Mars Sample Return (MSR) mission. Jezero is a 45 km diameter mid- to late-Noachian-aged crater selected for its diverse geology and potential for preserving evidence of ancient life. The rover is approaching the crater rim, an area of interest for its potential to preserve diverse lithologies representative of a large period of geologic history. It has significant astrobiological potential, as it may preserve evidence of uplifted deep crust and ancient hydrothermal environments. Impact megabreccia in the crater rim may be exhumed pre-Noachian crust from the Isidis impact, which would likely be the oldest materials ever investigated by a rover on Mars. Additionally, the rim hosts outcrops of the regionally extensive and potentially volcanic olivine/carbonate unit and mafic capping unit, which could have implications for the evolution of Mars volcanism. Regional maps have delineated the lithologies present in and around Jezero as a whole. The largest scale that the crater rim geology has been mapped is 1:5000.
Document ID
20240000473
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
M C Deahn
(Purdue University West Lafayette West Lafayette, United States)
B Horgan
(Purdue University West Lafayette West Lafayette, United States)
F Calef III
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
J Schroeder
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
K M Stack
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
N R Williams
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
S Alwmark
(Lund University Lund, Sweden)
C C Bedford
(Purdue University West Lafayette West Lafayette, United States)
M Bramble
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
L Crumpler
(New Mexico Museum of Natural History and Science Albuquerque, New Mexico, United States)
D Flannery
(Queensland University of Technology Brisbane, Australia)
B Garczynski
(Western Washington University Bellingham, United States)
S Gwizd
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
L Ives
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
A Klidaras
(Purdue University West Lafayette West Lafayette, United States)
C Lesh
(University of California, Los Angeles Los Angeles, United States)
H Manelski
(Purdue University West Lafayette West Lafayette, United States)
C Miller
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
M Nachon
(Texas A&M University System College Station, Texas, United States)
C Quantin-Nataf
(Université de Lyon Lyon, France)
N Randazzo
(University of Alberta Edmonton, Canada)
E Ravanis
(University of Hawaiʻi at Mānoa Honolulu, United States)
P Russell
(University of California, Los Angeles Los Angeles, United States)
T Del Sesto
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
J Simon
(Johnson Space Center Houston, United States)
J R C Voigt
(Jet Propulsion Laboratory La Cañada Flintridge, United States)
Date Acquired
January 11, 2024
Subject Category
Lunar and Planetary Science and Exploration
Meeting Information
Meeting: 55th Lunar and Planetary Science Conference
Location: Woodlands, TX
Country: US
Start Date: March 11, 2024
End Date: March 15, 2024
Sponsors: National Aeronautics and Space Administration
Funding Number(s)
WBS: 203959
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
NASA Peer Committee
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