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Production of Phyllosilicates and Sulfates on Mars Through Acidic Weathering: The Rio Tinto Mars Analog Model

机译:通过酸性耐候生产MARS的Phyllosilicates和硫酸盐:Rio Tinto Mars模拟模型

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Understanding the paleoclimate of Mars and the nature and ex-tent of the interaction of water with crustal materials is essential to evaluate if life emerged once on Mars. Using recent results obtained by orbiters and surface rovers we propose that mildly acidic aqueous conditions produced phyl-losilicate minerals during the Noachian period on Mars related to a CO_2 -rich atmosphere and an active hydrosphere. Underground neutralization of these mild acidic meteoric solutions with crustal materials would produce subsurface carbonates inside the crust after. Moreover, hydrothermalism provides miner-alization to favor subsurface sulfide orebodies, but also secondary geochemical processes would also favor its formation. After cessation of the internal magnetic dynamo, the CO_2 -rich atmosphere was eroded and decreased by interactions with the solar wind and the hydrologic cycle that induced a climatic change to dry conditions where hydrological processes had subsurface dominance. Un-der this thin atmospheric aridic conditions photochemistry played an essential role in generating oxidizing and acidifying compounds that after entering the Mars crust promoted carbonate dissolution and sulfide oxidation. As a conse-quence, acid-sulfate evaporite deposits were precipitated in areas where acidic subsurface solutions emerged. Analogous processes have been observed in the underground fluids that feed the Rio Tinto Mars analog. Seasonal subsurface of sulfur continued by a rapid oxidation induced by rainwaters, which induces a strong acidification through proton releasing (FeS_2 + 3. O_2 + 2 H_2O→2. 50_4~(2-)+ Fe~(2+) + 4 H~+). This stage is followed by a neutralization and reduction of the ferric and sulfate rich acidified waters, which favors the subsurface carbonate precipitation. In addition, phyllosillicate sedimentation under the strong acidic conditions of Rio Tinto, supports preservation of same minerals under early Noachian mildly acidic conditions.
机译:了解火星的古平衡和水与地壳材料相互作用的性质和例子是必不可少的,以评估生命在火星上出现一次。使用轨道和表面缺失获得的最近结果我们提出了温和的酸性水性条件在与CO_2-RICH气氛和活性水层相关的马氏上的马氏期间产生的乳硅酸盐矿物质。地下中和与地壳材料的这种温和的酸性溶液溶液将在外壳内部产生地下碳酸盐。此外,水热量提供矿工化以利用地下硫化物矿体,而且还有二次地球化学方法也将有利于其形成。在停止内部磁发电机之后,通过与太阳风的相互作用和水文循环的相互作用侵蚀并降低了CO_2-rich气氛,该水文循环对水文过程具有地下优势的干燥条件。这种薄的大气暴风条件光化学在产生氧化和酸化化合物方面发挥了重要作用,即进入火星地壳促进碳酸盐溶解和硫化物氧化。作为灭绝,酸 - 硫酸盐蒸发矿沉淀在酸性地下溶液出现的区域中沉淀出来。在地下流体中观察到类似方法,其饲喂RIO TINO MARS模拟。雨水诱导的汽油诱导的季节性地下持续,这促使通过质子释放强烈酸化(FES_2 + 3. O_2 + 2 H_2O→2。50_4〜(2 - )+ Fe〜(2+)+ 4 H〜 +)。然后,该阶段之后是富含铁和硫酸盐的酸化水的中和,其利用地下碳酸盐沉淀。此外,在Rio Tinto的强酸性条件下的Phyllosillate沉降,在早期Noachian轻度酸性条件下支持保持相同的矿物质。

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