Raman spectroscopic documentation of Mars analog basalt alteration by brines
Raman spectroscopic documentation of Mars analog basalt alteration by brines
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DOI:
10.1016/j.icarus.2022.115111
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发表时间:
2022-05
期刊:
影响因子:
3.2
通讯作者:
Andrew Rodriguez;L. Hunt;C. Phillips‐Lander;D. Mason;M. Madden
中科院分区:
文献类型:
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作者:
Andrew Rodriguez;L. Hunt;C. Phillips‐Lander;D. Mason;M. Madden
Salts and basalt are widespread on the surface of Mars. Therefore, basalt-brine interactions may have significant effects on both the aqueous history of the planet, and near-surface alteration assemblages. Raman spectra were collected from McKinney Basalt samples that were immersed in eight near-saturated brines composed of Na-Cl-H2O, Na-SO4-H2O, Na-ClO4-H2O, Mg-Cl-H2O, Mg-SO4-H2O, and two salt mixtures (Mg-Cl-SO4-H2O and Na-ClO4-SO4-H2O), as well as ultra-pure water for up to one year. Secondary minerals were observed in the Raman specta, including iron oxides, hydrated sulfates, amorphous silica, phosphates, and carbonates. Detection of these secondary minerals demonstrates the utility of Raman spectroscopy to identify basalt-brine alteration assemblages on Mars. This work also demonstrates that major classes of alteration phases can be distinguished using Raman spectra with resolution similar to those expected from the Raman instruments aboard the Perseverance and Rosalind Franklin Mars rovers. In addition, observations of carbonate minerals within alteration assemblages suggest CO2from the atmosphere readily reacted with ions released from the basalt during alteration in near-saturated brines.