Depositional and Diagenetic Sulfates of Hogwallow Flats and Yori Pass, Jezero Crater: Evaluating Preservation Potential of Environmental Indicators and Possible Biosignatures From Past Martian Surface Waters and Groundwaters

Author:

Benison Kathleen C.1ORCID,Gill Karena K.12,Sharma Sunanda3,Siljeström Sandra4ORCID,Zawaski Mike5ORCID,Bosak Tanja6ORCID,Broz Adrian7ORCID,Clark Benton C.8ORCID,Cloutis Edward9ORCID,Czaja Andrew D.10,Flannery David11ORCID,Fornaro Teresa12ORCID,Gómez Felipe13ORCID,Hand Kevin3ORCID,Herd Chris D. K.14ORCID,Johnson Jeffrey R.15ORCID,Madariaga Juan Manuel16ORCID,Madsen Morten B.17ORCID,Martinez‐Frías Jesús18ORCID,Nachon Marion5,Núñez Jorge I.15ORCID,Pedersen David A. K.19ORCID,Randazzo Nicholas14,Shuster David L.20,Simon Justin21ORCID,Steele Andrew22ORCID,Tate Christian23ORCID,Treiman Allan24ORCID,Uckert Kyle3ORCID,Williams Amy J.25ORCID,Yanchilina Anastasia3

Affiliation:

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

2. Now at Department of Earth and Environmental Sciences Washington and Lee University Lexington VA USA

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

4. RISE Research Institutes of Sweden Stockholm Sweden

5. Department of Geology and Geophysics Texas A & M University College Station TX USA

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

7. Department of Earth Sciences University of Oregon Eugene OR USA

8. Space Science Institute Boulder CO USA

9. Department of Geography University of Winnipeg Winnipeg MB Canada

10. Department of Geology University of Cincinnati Cincinnati OH USA

11. School of Earth and Atmospheric Sciences Queensland University of Technology Brisbane QLD Australia

12. INAF‐Astrophysical Observatory of Arcetri Florence Italy

13. Centro de Astrobiologia—CAB (INTA‐CSIC) Madrid Spain

14. Department of Earth and Atmospheric Sciences University of Alberta Edmonton AB Canada

15. Johns Hopkins University Applied Physics Laboratory (JHU/APL) Laurel MD USA

16. Department of Analytical Chemistry University of the Basque Country UPV/EHU Leioa Spain

17. Niels Bohr Institute University of Copenhagen Copenhagen Denmark

18. Institute of Geosciences (CSIC‐UCM) Madrid Spain

19. Department of Space Research and Technology Technical University of Denmark Kongens Lyngby Denmark

20. Department of Earth and Planetary Science University of California Berkeley CA USA

21. NASA Johnson Space Center Houston TX USA

22. Carnegie Institute for Science Washington DC USA

23. Department of Astronomy Cornell University Ithaca NY USA

24. Lunar and Planetary Institute Houston TX USA

25. Department of Geological Sciences University of Florida Gainesville FL USA

Abstract

AbstractThe Mars 2020 Perseverance rover has examined and sampled sulfate‐rich clastic rocks from the Hogwallow Flats member at Hawksbill Gap and the Yori Pass member at Cape Nukshak. Both strata are located on the Jezero crater western fan front, are lithologically and stratigraphically similar, and have been assigned to the Shenandoah formation. In situ analyses demonstrate that these are fine‐grained sandstones composed of phyllosilicates, hematite, Ca‐sulfates, Fe‐Mg‐sulfates, ferric sulfates, and possibly chloride salts. Sulfate minerals are found both as depositional grains and diagenetic features, including intergranular cement and vein‐ and vug‐cements. Here, we describe the possibility of various sulfate phases to preserve potential biosignatures and the record of paleoenvironmental conditions in fluid and solid inclusions, based on findings from analog sulfate‐rich rocks on Earth. The samples collected from these outcrops, Hazeltop and Bearwallow from Hogwallow Flats, and Kukaklek from Yori Pass, should be examined for such potential biosignatures and environmental indicators upon return to Earth.

Funder

Swedish National Space Agency

Publisher

American Geophysical Union (AGU)

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