Manganese Mobility in Gale Crater, Mars: Leached Bedrock and Localized Enrichments

被引:8
|
作者
Berger, J. A. [1 ]
King, P. L. [2 ]
Gellert, R. [3 ]
Clark, B. C. [4 ]
Flood, V. A. [5 ]
McCraig, M. A. [3 ]
Ming, D. W. [1 ]
O'Connell-Cooper, C. D. [6 ]
Schmidt, M. E. [7 ]
Thompson, L. M. [6 ]
VanBommel, S. J. V. [8 ]
Wilhelm, B. [3 ]
Yen, A. S. [9 ]
机构
[1] NASA, Jacobs JETS, Johnson Space Ctr, Houston, TX 77058 USA
[2] Australian Natl Univ, Res Sch Earth Sci, Canberra, ACT, Australia
[3] Univ Guelph, Dept Phys, Guelph, ON, Canada
[4] Space Sci Inst, Boulder, CO USA
[5] Univ Toronto, Dept Phys, Toronto, ON, Canada
[6] Univ New Brunswick, Earth Sci Dept, Fredericton, NB, Canada
[7] Brock Univ, Dept Earth Sci, St Catharines, ON, Canada
[8] Washington Univ, Dept Earth & Planetary Sci, St Louis, MO 63130 USA
[9] CALTECH, Jet Prop Lab, Pasadena, CA USA
基金
澳大利亚研究理事会;
关键词
manganese on Mars; APXS manganese results; APXS in Gale crater; martian geochemistry; X-RAY SPECTROMETER; ROCKS; CHEMISTRY; EVOLUTION; OXIDATION; MUDSTONE; IDENTIFICATION; MINERALOGY; CHEMCAM; SULFUR;
D O I
10.1029/2021JE007171
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
In Gale crater on Mars, the rover Curiosity has discovered evidence of fluid mobilization of the redox-sensitive element manganese. We present results for Mn from Curiosity's Alpha Particle X-ray Spectrometer (APXS), which show that the average MnO concentration in mudstone-dominated sedimentary units (0.22 wt%) is about one-half of the concentration in the average Mars crust (0.44 wt%). Geochemical trends indicate that Mn in the sedimentary bedrock, most of which has a basaltic provenance, was leached by chemical alteration and dissolution. In >350 vertical meters of mudstone-dominated strata, the apparent leaching of Mn and retention of Fe in Fe-O-H phase(s) resulted in the fractionation of Fe and Mn, indicating relatively moderate Eh-pH fluid conditions that were not highly alkaline, reducing, or oxidizing. Exceptions are fracture-associated, silica-rich haloes where both Mn and Fe were leached by low pH fluids. The rover also discovered Mn-rich veins, nodules, and patchy, dark coatings on rock surfaces, which are variably associated with enrichments in Fe, P, Cl, and/or Zn. These Mn-rich features represent similar to 1% of the 1029 APXS measurements acquired over similar to 25 km of rover traverse. A thermochemical model shows that dissolved Mn2+ could have been concentrated via evaporation, sublimation, and/or freezing. Manganese was then likely precipitated in localized features when >99.99% of the Mn2+-bearing water was removed from the system. These findings indicate that Mn was mobile in Gale crater and therefore bioavailable as a potential energy source for life.
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页数:21
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