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首页> 外文期刊>Journal of geophysical research. Planets >The formation and stability of the superoxide radical (O2?) on rock-forming minerals: Band gaps, hydroxylation state, and implications for Mars oxidant chemistry
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The formation and stability of the superoxide radical (O2?) on rock-forming minerals: Band gaps, hydroxylation state, and implications for Mars oxidant chemistry

机译:过氧化物的形成和稳定自由基(O2)矿物:乐队差距,羟基化状态,和影响火星化学氧化剂

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摘要

We have examined the generation and stability of O2 ? on TiO2 and albite, a common Na feldspar. We were not able to produce thermally stable superoxide on albite, in contrast to the results of Yen et al., who reported the generation of O2 ? that was stable up to 200°C on labradorite, another common feldspar. The superoxide radical did form under UV irradiation at 77 K on albite that was not dehydrated but decayed rapidly at room temperature. On dehydrated albite, no superoxide signal was observed. We studied the kinetics of O2 ? decomposition on hydrated albite and derived an activation energy, E a = 15.2 kJ/mol. Assuming pseudo first-order kinetics, a simple thermal model of Mars' regolith demonstrates that the surface O2 ? population does not go to zero overnight; superoxide extinction at the surface is only complete when the seasonal CO2 cap covers the surface and surface photolysis is inhibited. Depending on the specific quantum efficiency of the e?/h+ generation process, a finite, non-equilibrium population of O2 ? should be observable on Martian surface materials throughout the Martian year. However, on the basis of our inability to generate stable O2 ? on hydrated albite via direct UV irradiation, we do not believe that this mechanism is capable of explaining the O2 release in the Viking Gas Exchange (GEx) results, since O2 release in that case was observed even after samples had been stored for 143 sols in the dark at 10°C, then heated to 145°C for 3 hours. At least two other potential pathways to the generation of O2 ? are identified in this article. The first possibility is that metal oxides common on the Martian surface, particularly hematite, may be photoactive on Mars and play a role analogous to TiO2 in surface catalysis. Secondly, we found that superoxide that formed during the sorption or drying of a 1% H2O2 solution on TiO2, and potentially other oxides seems to be stable indefinitely.
机译:我们已经检查了的一代和稳定性O2 ?无法产生热稳定过氧化钠长石,对比结果日元的et al .,报告的生成氧气? 另一个常见的长石。在紫外光照射下形成了在77 K钠长石吗这不是脱水但迅速衰退室温。超氧化物观察信号。O2动力学?和派生的活化能E = 15.2焦每摩尔。简单的火星表层热模型表明表面氧气吗?不会在一夜之间趋于零;灭绝的表面只是完成时季节性二氧化碳帽覆盖表面表面光解作用受到抑制。具体的量子效率e ?生成过程,一个有限的、非平衡人口的O2 ?整个火星的火星表面材料的一年。生成稳定的O2 ?紫外线直接照射,我们不相信这种机制能够解释O2在维京气体交换(GEx)结果,自氧气释放甚至在这种情况下被观察到后样品存储了143溶胶黑暗在10°C,然后加热到145°C 3小时。至少有两个其他的潜在途径代的O2 ?篇文章。在火星表面氧化物共同,尤其是赤铁矿,可能是火星上的感光性的和类似于表面二氧化钛中发挥作用催化。形成在吸附或干燥的1%过氧化氢溶液在二氧化钛,和潜在的其他氧化物似乎稳定下去。

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