TY - JOUR
T1 - Evolved gas analyses of sedimentary rocks and eolian sediment in Gale Crater, Mars
T2 - Results of the Curiosity rover's sample analysis at Mars instrument from Yellowknife Bay to the Namib Dune
AU - Sutter, B.
AU - McAdam, A. C.
AU - Mahaffy, P. R.
AU - Ming, D. W.
AU - Edgett, K. S.
AU - Rampe, E. B.
AU - Eigenbrode, J. L.
AU - Franz, H. B.
AU - Freissinet, C.
AU - Grotzinger, J. P.
AU - Steele, A.
AU - House, C. H.
AU - Archer, P. D.
AU - Malespin, C. A.
AU - Navarro-González, R.
AU - Stern, J. C.
AU - Bell, J. F.
AU - Calef, F. J.
AU - Gellert, R.
AU - Glavin, D. P.
AU - Thompson, L. M.
AU - Yen, A. S.
N1 - Funding Information:
The authors are grateful to the engineers and scientists of the MSL Curiosity team, who have made the mission possible and the reported data available. SAM data are publically available through the NASA Planetary Data System at: http://pds-geosciences. wustl.edu/missions/msl/sam.htm. This work was funded by support from NASA to the SAM and MSL teams. D.P.G., J.L.E., A.C.M, and C.H.H. acknowledge funding support from the NASA ROSES MSL Participating Scientist Program. C.F. acknowledges support from the NASA Postdoctoral Program, administered by Oak Ridge Associated Universities through a contract with NASA. R.N.G. acknowledges funding from Universidad Nacional Autónoma de México (DGAPA-IN109416) and Consejo Nacional de Ciencia y Tecnología de México (CONACyT 220626). The authors acknowledge the Mastcam and MAHLI operations team at Malin Space Science Systems (MSSS) for producing and providing all Mastcam mosaic and MAHLI images used in this manuscript. The authors are grateful for assistance from Deirdra M. Fey, Marie J. McBride, and Michael A. Ravine who produced the MAHLI images and MAHLI mosaics used in this manuscript. We are grateful to Steven D’hondt and Jens Kallmeyer for useful discussions regarding organic carbon data generated by the shipboard party of Integrated Ocean Drilling Program (IODP) Expedition 329 and the use of those data for comparison to Mars. We would like to thank Tanya Peretyazhko, the JGR Editor David Baratoux, the Associate Editor, and two anonymous reviewers for useful comments and edits that significantly improved this manuscript.
PY - 2017/12
Y1 - 2017/12
N2 - 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 that 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 that oxychlorine phases (chlorate/perchlorate) (0.05 ± 0.025–1.05 ± 0.44 wt % 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 that reduced phases occur despite the presence of oxidized phases (nitrate, oxychlorine, sulfate, and carbonate). SAM results coupled with CheMin mineralogical and Alpha-Particle X-ray Spectrometer 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.
AB - 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 that 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 that oxychlorine phases (chlorate/perchlorate) (0.05 ± 0.025–1.05 ± 0.44 wt % 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 that reduced phases occur despite the presence of oxidized phases (nitrate, oxychlorine, sulfate, and carbonate). SAM results coupled with CheMin mineralogical and Alpha-Particle X-ray Spectrometer 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.
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U2 - 10.1002/2016JE005225
DO - 10.1002/2016JE005225
M3 - Article
AN - SCOPUS:85040676900
VL - 122
SP - 2574
EP - 2609
JO - Journal of Geophysical Research: Atmospheres
JF - Journal of Geophysical Research: Atmospheres
SN - 2169-897X
IS - 12
ER -