Huguenin R L, Miller K J, Harwood W S
J Mol Evol. 1979 Dec;14(1-3):103-32. doi: 10.1007/BF01732372.
A laboratory study of the interaction of H2O frost with samples of the minerals olivine (Mg,Fe)2SiO4 and pyroxene (Mg,Fe)SiO3 at -11 degrees C to -22 degrees C revealed that an acidic oxidant was produced. Exposure of the frost-treated minerals to liquie H2O produced a sudden drop in pH and resulted in the production of copious O2(g) (as much as approximately 10(20) molecules g-1). Exposure of frost-treated samples to 5 ml of 0.1M HCOONa solution resulted in the rapid oxidation of up to 43% of the formate to CO2(g). These reactions were qualitatively similar to the chemical activity observed during the active cycles of the Viking lander Gas Exchange and Labeled Release Biology experiments. Attempts to identify the oxidant by chemical indicators were inconclusive, but they tentatively suggested that chemisorbed hydrogen peroxide may have formed. The formation of chemisorbed peroxide could be explained as a byproduct of the chemical reduction of the mineral. The following model was proposed. H+ was incorporated into the mineral from surface frost. This would have left behind a residual of excess OH-(ads) (relative to surface H+). Electrons were then stripped from the surface OH-(ads) (due to the large repulsive potential between neighboring OH-(ads)) and incorporated into the crystal to restore charge balance and produce a chemical reduction of the mineral. The resultant surface hydroxyl radicals could then have combined to form the more stable chemisorbed hydrogen peroxide species. While the chemisorbed peroxide should be relatively stable at low temperatures, it should tend to decay to O(ads)+ H2O(g) at higher temperatures with an activation energy of greater than or approximately 34 kcal mole-1. This is consistent with the long-term storage and sterilization behavior of the Viking soil oxidants. It is possible that as little as 0.1--1% frost-weathered material in the martian soil could have produced the unusual chemical activity that occurred during the Viking Gas Exchange and Labeled Release experiments.
一项在-11摄氏度至-22摄氏度下对H2O霜与矿物橄榄石(Mg,Fe)2SiO4和辉石(Mg,Fe)SiO3样本相互作用的实验室研究表明,产生了一种酸性氧化剂。将经霜处理的矿物暴露于液态H2O中会导致pH值突然下降,并产生大量O2(g)(多达约10^20个分子g-1)。将经霜处理的样本暴露于5毫升0.1M HCOONa溶液中会导致高达43%的甲酸盐快速氧化为CO2(g)。这些反应在定性上与海盗号着陆器气体交换和标记释放生物学实验的活跃周期中观察到的化学活性相似。通过化学指示剂鉴定氧化剂的尝试没有得出结论,但初步表明可能形成了化学吸附的过氧化氢。化学吸附过氧化物的形成可以解释为矿物化学还原的副产物。提出了以下模型。H+从表面霜中掺入矿物中。这会留下过量的OH-(吸附)残余物(相对于表面H+)。然后电子从表面OH-(吸附)中剥离(由于相邻OH-(吸附)之间的大排斥电位)并掺入晶体中以恢复电荷平衡并产生矿物的化学还原。所得的表面羟基自由基然后可以结合形成更稳定的化学吸附过氧化氢物种。虽然化学吸附的过氧化物在低温下应该相对稳定,但在较高温度下它应该倾向于以大于或约34千卡摩尔-1的活化能分解为O(吸附)+ H2O(g)。这与海盗号土壤氧化剂的长期储存和灭菌行为一致。火星土壤中低至0.1--1%的霜蚀物质可能产生了海盗号气体交换和标记释放实验期间发生的异常化学活性。