J. V. Clark, B. Sutter, A. C. McAdam, J. M. T. Lewis, H. Franz, P. D. Archer, L. Chou, J. Eigenbrode, C. Knudson, J. Stern, D. Glavin, A. Steele, C. H. House, J. Schroeder, J. Berger, E. B. Rampe, S. Simpson, B. Tutolo, R. E. Milliken, C. Malespin, P. Mahaffy, A. Vasavada
{"title":"火星盖尔陨石坑粘土-硫酸盐过渡区沉积岩中记录的环境变化:火星科学实验室好奇号火星车上火星演化气体分析仪器样品分析的结果","authors":"J. V. Clark, B. Sutter, A. C. McAdam, J. M. T. Lewis, H. Franz, P. D. Archer, L. Chou, J. Eigenbrode, C. Knudson, J. Stern, D. Glavin, A. Steele, C. H. House, J. Schroeder, J. Berger, E. B. Rampe, S. Simpson, B. Tutolo, R. E. Milliken, C. Malespin, P. Mahaffy, A. Vasavada","doi":"10.1029/2024JE008587","DOIUrl":null,"url":null,"abstract":"<p>The <i>Curiosity</i> rover explored the region between the orbitally defined phyllosilicate-bearing Glen Torridon trough and the overlying layered sulfate-bearing unit, called the “clay-sulfate transition region.” Samples were drilled from the top of the fluviolacustrine Glasgow member of the Carolyn Shoemaker formation (CSf) to the eolian Contigo member of the Mirador formation (MIf) to assess in situ mineralogical changes with stratigraphic position. The Sample Analysis at Mars-Evolved Gas Analysis (SAM-EGA) instrument analyzed drilled samples within this region to constrain their volatile chemistry and mineralogy. Evolved H<sub>2</sub>O consistent with nontronite was present in samples drilled in the Glasgow and Mercou members of the CSf but was generally absent in stratigraphically higher samples. SO<sub>2</sub> peaks consistent with Fe sulfate were detected in all samples, and SO<sub>2</sub> evolutions consistent with Mg sulfate were observed in most samples. CO<sub>2</sub> and CO evolutions were variable between samples and suggest contributions from adsorbed CO<sub>2</sub>, carbonates, simple organic salts, and instrument background. The lack of NO and O<sub>2</sub> in the data suggest that oxychlorines and nitrates were absent or sparse, and evolved HCl was consistent with the presence of chlorides in all samples. The combined rover data sets suggest that sediments in the upper CSf and MIf may represent similar source material and were deposited in lacustrine and eolian environments, respectively. Rocks were subsequently altered in briny solutions with variable chemical compositions that resulted in the precipitation of sulfates, carbonates, and chlorides. The results suggest that the clay-sulfate transition records progressively drier surface depositional environments and saline diagenetic fluid, potentially impacting habitability.</p>","PeriodicalId":16101,"journal":{"name":"Journal of Geophysical Research: Planets","volume":"129 12","pages":""},"PeriodicalIF":3.9000,"publicationDate":"2024-11-28","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://onlinelibrary.wiley.com/doi/epdf/10.1029/2024JE008587","citationCount":"0","resultStr":"{\"title\":\"Environmental Changes Recorded in Sedimentary Rocks in the Clay-Sulfate Transition Region in Gale Crater, Mars: Results From the Sample Analysis at Mars-Evolved Gas Analysis Instrument Onboard the Mars Science Laboratory Curiosity Rover\",\"authors\":\"J. V. Clark, B. Sutter, A. C. McAdam, J. M. T. Lewis, H. Franz, P. D. Archer, L. Chou, J. Eigenbrode, C. Knudson, J. Stern, D. Glavin, A. Steele, C. H. House, J. Schroeder, J. Berger, E. B. Rampe, S. Simpson, B. Tutolo, R. E. Milliken, C. Malespin, P. Mahaffy, A. Vasavada\",\"doi\":\"10.1029/2024JE008587\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<p>The <i>Curiosity</i> rover explored the region between the orbitally defined phyllosilicate-bearing Glen Torridon trough and the overlying layered sulfate-bearing unit, called the “clay-sulfate transition region.” Samples were drilled from the top of the fluviolacustrine Glasgow member of the Carolyn Shoemaker formation (CSf) to the eolian Contigo member of the Mirador formation (MIf) to assess in situ mineralogical changes with stratigraphic position. The Sample Analysis at Mars-Evolved Gas Analysis (SAM-EGA) instrument analyzed drilled samples within this region to constrain their volatile chemistry and mineralogy. Evolved H<sub>2</sub>O consistent with nontronite was present in samples drilled in the Glasgow and Mercou members of the CSf but was generally absent in stratigraphically higher samples. SO<sub>2</sub> peaks consistent with Fe sulfate were detected in all samples, and SO<sub>2</sub> evolutions consistent with Mg sulfate were observed in most samples. CO<sub>2</sub> and CO evolutions were variable between samples and suggest contributions from adsorbed CO<sub>2</sub>, carbonates, simple organic salts, and instrument background. The lack of NO and O<sub>2</sub> in the data suggest that oxychlorines and nitrates were absent or sparse, and evolved HCl was consistent with the presence of chlorides in all samples. The combined rover data sets suggest that sediments in the upper CSf and MIf may represent similar source material and were deposited in lacustrine and eolian environments, respectively. Rocks were subsequently altered in briny solutions with variable chemical compositions that resulted in the precipitation of sulfates, carbonates, and chlorides. 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Environmental Changes Recorded in Sedimentary Rocks in the Clay-Sulfate Transition Region in Gale Crater, Mars: Results From the Sample Analysis at Mars-Evolved Gas Analysis Instrument Onboard the Mars Science Laboratory Curiosity Rover
The Curiosity rover explored the region between the orbitally defined phyllosilicate-bearing Glen Torridon trough and the overlying layered sulfate-bearing unit, called the “clay-sulfate transition region.” Samples were drilled from the top of the fluviolacustrine Glasgow member of the Carolyn Shoemaker formation (CSf) to the eolian Contigo member of the Mirador formation (MIf) to assess in situ mineralogical changes with stratigraphic position. The Sample Analysis at Mars-Evolved Gas Analysis (SAM-EGA) instrument analyzed drilled samples within this region to constrain their volatile chemistry and mineralogy. Evolved H2O consistent with nontronite was present in samples drilled in the Glasgow and Mercou members of the CSf but was generally absent in stratigraphically higher samples. SO2 peaks consistent with Fe sulfate were detected in all samples, and SO2 evolutions consistent with Mg sulfate were observed in most samples. CO2 and CO evolutions were variable between samples and suggest contributions from adsorbed CO2, carbonates, simple organic salts, and instrument background. The lack of NO and O2 in the data suggest that oxychlorines and nitrates were absent or sparse, and evolved HCl was consistent with the presence of chlorides in all samples. The combined rover data sets suggest that sediments in the upper CSf and MIf may represent similar source material and were deposited in lacustrine and eolian environments, respectively. Rocks were subsequently altered in briny solutions with variable chemical compositions that resulted in the precipitation of sulfates, carbonates, and chlorides. The results suggest that the clay-sulfate transition records progressively drier surface depositional environments and saline diagenetic fluid, potentially impacting habitability.
期刊介绍:
The Journal of Geophysical Research Planets is dedicated to the publication of new and original research in the broad field of planetary science. Manuscripts concerning planetary geology, geophysics, geochemistry, atmospheres, and dynamics are appropriate for the journal when they increase knowledge about the processes that affect Solar System objects. Manuscripts concerning other planetary systems, exoplanets or Earth are welcome when presented in a comparative planetology perspective. Studies in the field of astrobiology will be considered when they have immediate consequences for the interpretation of planetary data. JGR: Planets does not publish manuscripts that deal with future missions and instrumentation, nor those that are primarily of an engineering interest. Instrument, calibration or data processing papers may be appropriate for the journal, but only when accompanied by scientific analysis and interpretation that increases understanding of the studied object. A manuscript that describes a new method or technique would be acceptable for JGR: Planets if it contained new and relevant scientific results obtained using the method. Review articles are generally not appropriate for JGR: Planets, but they may be considered if they form an integral part of a special issue.