首页> 外文会议>International Zeolite Conference; 20070812-17; Beijing(CN) >Water and carbon dioxide sorption properties of natural zeolites and clay minerals at martian surface temperature and pressure conditions
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Water and carbon dioxide sorption properties of natural zeolites and clay minerals at martian surface temperature and pressure conditions

机译:火星表面温度和压力条件下天然沸石和粘土矿物对水和二氧化碳的吸附特性

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摘要

The verified presence of smectites, natural zeolites, sulfates and other water-bearing minerals on the martian surface have encouraged us to study their water and CO_2 adsorption behaviour under conditions close to martian equatorial surface temperature and pressure. The results for smectites and zeolites show about 2.5-25 wt% of (partially mobile) water at low temperatures and a very low partial pressure of 0.001 mbar. Mars relevant minerals such as nontronite, montmorillonite, clinoptilolite and chabazite can adsorb water even in a more than thousandfold surplus (6 mbar) of carbon dioxide. The presence of water in equatorial latitudes might be of importance for water involved chemistry and hypothetical exobiological activity on Mars.
机译:在火星表面证实存在蒙脱石,天然沸石,硫酸盐和其他含水矿物,这促使我们研究在接近火星赤道表面温度和压力的条件下它们对水和CO_2的吸附行为。蒙脱石和沸石的结果表明,在低温和0.001 mbar的极低分压下,约2.5-25 wt%的(部分移动的)水。火星相关的矿物,如绿脱石,蒙脱石,斜发沸石和菱沸石可以吸收水,即使是在二氧化碳的千余倍(6毫巴)中也是如此。赤道纬度中水的存在可能对涉及火星的化学和假想生物活动具有重要意义。

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