NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Mapping Organic-Mineral Associations in Jezero craterThe search for potential signs of life on Mars, a primary aim of the Mars 2020 mission, is greatly informed by the detection of organic matter1. The presence of organic matter also provides key information about the habitability and biological potential of the planet throughout its history. The Perseverance rover was designed for in situ science with the ability to collect a suite of promising samples for eventual return to Earth. One of its instruments, Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals (SHERLOC), is a deep ultraviolet (DUV) Raman and fluorescence spectrometer designed to map the distribution of organic molecules and minerals on rock surfaces at a resolution of 100 μm2. With its unique spectral mapping capabilities, SHERLOC enables a novel understanding of organic-mineral relationships on Mars to better determine their formation, deposition, and preservation mechanisms.
The rover’s landing site within Jezero crater combines a high potential for past habitability as the site of an ancient lake basin with a diverse set of minerals, including carbonates and clays, that may preserve organic materials and potential biosignatures. The Jezero crater floor includes three formations (fm); two of these, Máaz and Séítah, were explored as part of the mission’s first campaign. Here, we report the detection of multiple species of aromatic organic molecules using Raman and fluorescence spectroscopy across ten targets in the two formations. This is the first evidence of organic molecules in Martian materials obtained using Raman spectroscopy, and among the first using fluorescence spectroscopy, beyond Earth3. We report specific spatial patterns and classes of organic molecules in these compositionally distinct formations, potentially indicating different fates of carbon in these environments. Our findings indicate that there is a diversity of aromatic molecules prevalent on the Martian surface and these materials persist despite exposure to surface conditions. These organic molecules are largely found within minerals linked to aqueous processes, suggesting that these processes may have had a key role in organic synthesis, transport from their point of origin, or preservation.
Document ID
20220011715
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Sunanda Sharma
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Ashley Murphy
(Planetary Science Institute Tucson, Arizona, United States)
Luther W. Beegle
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Rohit Bhartia
(Photon Systems (United States) Covina, California, United States)
Andrew Steele
(Carnegie Institution for Science Washington D.C., District of Columbia, United States)
Joseph Razzell Hollis
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Sandra Siljestroem
(RISE Research Institutes of Sweden Gothenburg, Sweden)
Francis M. Mccubbin
(Johnson Space Center Houston, Texas, United States)
Sanford A. Asher
(University of Pittsburgh Pittsburgh, Pennsylvania, United States)
William J. Abbey
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Abigail C. Allwood
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Eve L. Berger
(Jacobs Technology Houston, Texas, United States)
Benjamin L. Bleefeld
(Malin Space Science Systems (United States) San Diego, California, United States)
Aaron S. Burton
(Johnson Space Center Houston, Texas, United States)
Sergei V. Bykov
(University of Pittsburgh Pittsburgh, Pennsylvania, United States)
Emily L. Cardarelli
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Pamela G. Conrad
(Carnegie Institution for Science Washington D.C., District of Columbia, United States)
Andrea Corpolongo
(University of Cincinnati Cincinnati, Ohio, United States)
Andrew D. Czaja
(University of Cincinnati Cincinnati, Ohio, United States)
Lauren P. DeFlores
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Kenneth Edgett
(Malin Space Science Systems (United States) San Diego, California, United States)
Kenneth A. Farley
(California Institute of Technology Pasadena, California, United States)
Teresa Fornaro
(INAF - Osservatorio Astronomico di Cagliari Selargius, Italy)
Allison C. Fox
(Universities Space Research Association Columbia, Maryland, United States)
Marc D. Fries
(Johnson Space Center Houston, Texas, United States)
David Harker
(Malin Space Science Systems (United States) San Diego, California, United States)
Keyron Hickman-lewis
(Natural History Museum London, United Kingdom)
Joshua Huggett
(Malin Space Science Systems (United States) San Diego, California, United States)
Samara Imbeah
(Malin Space Science Systems (United States) San Diego, California, United States)
Ryan S. Jakubek
(Jacobs Technology Dallas, Texas, United States)
Linda C. Kah
(University of Tennessee at Knoxville Knoxville, Tennessee, United States)
Carina Lee
(Universities Space Research Association Columbia, Maryland, United States)
Yang Liu
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Angela Magee
(Malin Space Science Systems (United States) San Diego, California, United States)
Michelle Minitti
(Arizona State University Tempe, Arizona, United States)
Kelsey R. Moore
(California Institute of Technology Pasadena, California, United States)
Alyssa Pascuzzo
(Malin Space Science Systems (United States) San Diego, California, United States)
Carolina Rodiguez
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Eva L. Scheller
(Massachusetts Institute of Technology Cambridge, Massachusetts, United States)
Svetlana Shkolyar
(University of Maryland, College Park College Park, Maryland, United States)
Kathryn M. Stack
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Kimberly Steadman
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Michael Tuite
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Kyle Uckert
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Alyssa Werynski
(Malin Space Science Systems (United States) San Diego, California, United States)
Roger C. Wiens
(Los Alamos National Laboratory Los Alamos, New Mexico, United States)
Amy J. Williams
(Towson University Towson, Maryland, United States)
Katherine Winchell
(Malin Space Science Systems (United States) San Diego, California, United States)
Megan Wu
(Malin Space Science Systems (United States) San Diego, California, United States)
Ryan D. Roppel
(University of Pittsburgh Pittsburgh, Pennsylvania, United States)
Anastasia Yanchilina
(Jet Propulsion Lab La Cañada Flintridge, California, United States)
Alberto G Fairen
(Cornell University Ithaca, New York, United States)
Date Acquired
August 2, 2022
Subject Category
Inorganic, Organic And Physical Chemistry
Meeting Information
Meeting: AGU Fall Conference
Location: Chicago, IL
Country: US
Start Date: December 12, 2022
End Date: December 16, 2022
Sponsors: American Geophysical Union
Funding Number(s)
WBS: 971200.05.11.01.04
PROJECT: Mars 2020-SHERLOC
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
Single Expert
No Preview Available