Aqueous alteration processes in Jezero crater, Mars—implications for organic geochemistry-Reference-Cited by-同舟云学术

Aqueous alteration processes in Jezero crater, Mars—implications for organic geochemistry

Published:2022-12-09 Issue:6624 Volume:378 Page:1105-1110
ISSN:0036-8075
Container-title:Science
language:en
Short-container-title:Science

Author:

Scheller Eva L.¹²^ORCID,Razzell Hollis Joseph³⁴,Cardarelli Emily L.³^ORCID,Steele Andrew⁵^ORCID,Beegle Luther W.³^ORCID,Bhartia Rohit⁶^ORCID,Conrad Pamela⁵^ORCID,Uckert Kyle³^ORCID,Sharma Sunanda³^ORCID,Ehlmann Bethany L.¹³^ORCID,Abbey William J.³,Asher Sanford A.⁷^ORCID,Benison Kathleen C.⁸^ORCID,Berger Eve L.⁹¹⁰¹¹^ORCID,Beyssac Olivier¹²^ORCID,Bleefeld Benjamin L.¹³,Bosak Tanja²^ORCID,Brown Adrian J.¹⁴^ORCID,Burton Aaron S.¹¹^ORCID,Bykov Sergei V.⁷^ORCID,Cloutis Ed¹⁵^ORCID,Fairén Alberto G.¹⁶¹⁷^ORCID,DeFlores Lauren³,Farley Kenneth A.¹^ORCID,Fey Deidra M.¹³^ORCID,Fornaro Teresa¹⁸^ORCID,Fox Allison C.¹¹^ORCID,Fries Marc¹¹^ORCID,Hickman-Lewis Keyron¹⁹²⁰^ORCID,Hug William F.⁶^ORCID,Huggett Joshua E.¹³,Imbeah Samara¹³^ORCID,Jakubek Ryan S.¹¹^ORCID,Kah Linda C.²¹^ORCID,Kelemen Peter²²^ORCID,Kennedy Megan R.¹³^ORCID,Kizovski Tanya²³^ORCID,Lee Carina²⁴^ORCID,Liu Yang³^ORCID,Mandon Lucia²⁵^ORCID,McCubbin Francis M.¹¹^ORCID,Moore Kelsey R.³,Nixon Brian E.¹³^ORCID,Núñez Jorge I.²⁶^ORCID,Rodriguez Sanchez-Vahamonde Carolina¹³,Roppel Ryan D.⁷^ORCID,Schulte Mitchell²⁷^ORCID,Sephton Mark A.²⁸^ORCID,Sharma Shiv K.²⁹^ORCID,Siljeström Sandra³⁰^ORCID,Shkolyar Svetlana³¹³²^ORCID,Shuster David L.³³^ORCID,Simon Justin I.¹¹^ORCID,Smith Rebecca J.³⁴^ORCID,Stack Kathryn M.³^ORCID,Steadman Kim³^ORCID,Weiss Benjamin P.²^ORCID,Werynski Alyssa¹³^ORCID,Williams Amy J.³⁵^ORCID,Wiens Roger C.³⁶³⁷^ORCID,Williford Kenneth H.³³⁸,Winchell Kathrine¹³,Wogsland Brittan²¹^ORCID,Yanchilina Anastasia³⁹^ORCID,Yingling Rachel¹³^ORCID,Zorzano Maria-Paz¹⁶^ORCID

Affiliation:

1. Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA.

2. Department of Earth, Atmospheric, and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA, USA.

3. NASA Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA.

4. The Natural History Museum, London, UK.

5. Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA.

6. Photon Systems Incorporated, Covina, CA, USA.

7. Department of Chemistry, University of Pittsburgh, Pittsburgh, PA, USA.

8. Department of Geology and Geography, West Virginia University, Morgantown, WV, USA.

9. Texas State University, San Marcos, TX, USA.

10. Jacobs Johnson Space Center Engineering, Technology and Science Contract, Houston, TX, USA.

11. NASA Johnson Space Center, Houston, TX, USA.

12. Institut de Minéralogie, de Physique des Matériaux et de Cosmochimie, Centre National de la Recherche Scientifique, Sorbonne Université, Muséum National d’Histoire Naturelle, 75005 Paris, France.

13. Malin Space Science Systems, San Diego, CA, USA.

14. Plancus Research, Severna Park, MD, USA.

15. Geography, The University of Winnipeg, Winnipeg, MB, Canada.

16. Centro de Astrobiología, Consejo Superior de Investigaciones Cientificas–Instituto Nacional de Tecnica Aeroespacial, Madrid, Spain.

17. Department of Astronomy, Cornell University, Ithaca, NY, USA.

18. Astrophysical Observatory of Arcetri, Istituto Nazionale di Astrofisica, Florence, Italy.

19. Department of Earth Sciences, The Natural History Museum, London, UK.

20. Dipartimento di Scienze Biologiche, Geologiche e Ambientali, Università di Bologna, Bologna, Italy.

21. Department of Earth and Planetary Sciences, University of Tennessee, Knoxville, TN, USA.

22. Lamont Doherty Earth Observatory, Columbia University, Palisades, NY, USA.

23. Department of Earth Sciences, Brock University, St. Catharines, ON L2S 3A1, Canada.

24. Lunar and Planetary Institute, Universities Space Research Association, Houston, TX, USA.

25. Laboratoire d’Etudes Spatiales et d’Instrumentation en Astrophysique, Observatoire de Paris, Centre National de la Recherche Scientifique, Sorbonne Université, Université Paris Diderot, 92195 Meudon, France.

26. Johns Hopkins University Applied Physics Laboratory, Laurel, MD, USA.

27. Mars Exploration Program, NASA Headquarters, Washington, DC, USA.

28. Earth Science and Engineering, South Kensington Campus, Imperial College London, SW7 2AZ London, UK.

29. Hawaii Institute of Geophysics and Planetology, University of Hawaii at Manoa, Honolulu, HI, USA.

30. Research Institutes of Sweden, Stockholm, Sweden.

31. Department of Astronomy, University of Maryland, College Park, MD, USA.

32. NASA Goddard Space Flight Center, Greenbelt, MD, USA.

33. Earth and Planetary Science, University of California Berkeley, Berkeley, CA, USA.

34. Department of Geosciences, Stony Brook University, Stony Brook, NY, USA.

35. Department of Geological Sciences, University of Florida, Gainesville, FL, USA.

36. Los Alamos National Laboratory, Los Alamos, NM, USA.

37. Earth, Atmospheric, and Planetary Sciences, Purdue University, West Lafayette, IN, USA.

38. Blue Marble Space Institute of Science, Seattle, WA, USA.

39. Impossible Sensing, St. Louis, MO, USA.

Abstract

The Perseverance rover landed in Jezero crater, Mars, in February 2021. We used the Scanning Habitable Environments with Raman and Luminescence for Organics and Chemicals (SHERLOC) instrument to perform deep-ultraviolet Raman and fluorescence spectroscopy of three rocks within the crater. We identify evidence for two distinct ancient aqueous environments at different times. Reactions with liquid water formed carbonates in an olivine-rich igneous rock. A sulfate-perchlorate mixture is present in the rocks, which probably formed by later modifications of the rocks by brine. Fluorescence signatures consistent with aromatic organic compounds occur throughout these rocks and are preserved in minerals related to both aqueous environments.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference64 articles.

1. Mars 2020 Mission Overview

2. Assessing the mineralogy of the watershed and fan deposits of the Jezero crater paleolake system, Mars

3. Orbital Identification of Carbonate-Bearing Rocks on Mars

4. The mineral diversity of Jezero crater: Evidence for possible lacustrine carbonates on Mars

5. Reanalysis of the Viking results suggests perchlorate and organics at midlatitudes on Mars

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