Evolved gas analyses of sedimentary rocks and eolian sediment in Gale Crater, Mars: Results of the Curiosity rover's sample analysis at Mars instrument from Yellowknife Bay to the Namib Dune

Brad Sutter (1, 2) , Amy C. Mcadam (3) , Paul R. Mahaffy (3) , Doug W. Ming (2) , Ken S. Edgett (4) , Elizabeth B. Rampe (5) , Jennifer L. Eigenbrode (3) , Heather B. Franz (6) , Caroline Freissinet (7) , John P. Grotzinger (8) , Andrew Steele (9) , Christopher H. House (10) , P. Douglas Archer (2, 1) , Charles A. Malespin (3) , Rafael Navarro-González (11) , Jennifer C. Stern (3) , James F. Bell (12) , Fred J. Calef (13) , Ralf Gellert (14) , Daniel P. Glavin (3) , Lucy M. Thompson (15) , Albert S. Yen (13)

1 Jacobs Technology ESCG
2 JSC - NASA Johnson Space Center
3 GSFC - NASA Goddard Space Flight Center
4 MSSS - Malin Space Science Systems
5 ARES - Astromaterials Research and Exploration Science
6 CRESST - Center for Research and Exploration in Space Science and Technology [GSFC]
7 PLANETO - LATMOS
8 Division of Geological and Planetary Sciences [Pasadena]
9 Geophysical Laboratory [Carnegie Institution]
10 Department of Geosciences [PennState]
11 Instituto de Ciencias Nucleares [Mexico]
12 SESE - School of Earth and Space Exploration [Tempe]
13 JPL - Jet Propulsion Laboratory
14 Guelph-Waterloo Physics Institute
15 PASSC - Planetary and Space Science Centre

The Sample Analysis at Mars instrument evolved gas analyzer (SAM-EGA) has detected evolved water, H₂, SO₂, H₂S, NO, CO₂, CO, O₂ and HCl from two eolian sediments and nine sedimentary rocks from Gale Crater, Mars. These evolved gas detections indicate nitrates, organics, oxychlorine phase, and sulfates are widespread with phyllosilicates and carbonates occurring in select Gale Crater materials. Coevolved CO₂ (160 ± 248 - 2373 ± 820 μgC_(CO2)/g), and CO (11 ± 3 - 320 ± 130 μgC_(CO)/g) suggest organic-C is present in Gale Crater materials. Five samples evolved CO₂ at temperatures consistent with carbonate (0.32± 0.05 - 0.70± 0.1 wt.% CO₃). Evolved NO amounts to 0.002 ± 0.007 - 0.06 ± 0.03 wt.% NO₃. Evolution of O₂ suggests oxychlorine phases (chlorate/perchlorate) (0.05 ± 0.025 - 1.05 ± 0.44wt. % ClO₄) are present while SO₂ evolution indicates the presence of crystalline and/or poorly crystalline Fe- and Mg-sulfate and possibly sulfide. Evolved H₂O (0.9 ± 0.3 - 2.5 ± 1.6 wt.% H₂O) is consistent with the presence of adsorbed water, hydrated salts, interlayer/structural water from phyllosilicates, and possible inclusion water in mineral/amorphous phases. Evolved H₂ and H₂S suggest reduced phases occur despite the presence of oxidized phases (nitrate, oxychlorine, sulfate, carbonate). SAM results coupled with CheMin mineralogical and APXS elemental analyses indicate that Gale Crater sedimentary rocks have experienced a complex authigenetic/diagenetic history involving fluids with varying pH, redox, and salt composition. The inferred geochemical conditions were favorable for microbial habitability and if life ever existed, there was likely sufficient organic-C to support a small microbial population.

Domaines: Géophysique [physics.geo-ph]

Brad Sutter, Amy C. Mcadam, Paul R. Mahaffy, Doug W. Ming, Ken S. Edgett, et al.. Evolved gas analyses of sedimentary rocks and eolian sediment in Gale Crater, Mars: Results of the Curiosity rover's sample analysis at Mars instrument from Yellowknife Bay to the Namib Dune. Journal of Geophysical Research. Planets, 2017, 122 (12), pp.2574-2609. ⟨10.1002/2016JE005225⟩. ⟨insu-01562821⟩