Department of Chemistry, University of Hawaii at Manoa, Honolulu, HI 96822, USA.
W. M. Keck Research Laboratory in Astrochemistry, University of Hawaii at Manoa, Honolulu, HI 96822, USA.
Phys Chem Chem Phys. 2023 Jul 5;25(26):17460-17469. doi: 10.1039/d3cp02307a.
Enols - tautomers of ketones or aldehydes - are anticipated to be ubiquitous in the interstellar medium and play a key role in the formation of complex organic molecules in deep space, but their fundamental formation mechanisms have remained largely elusive as of now. Here we present a combined experimental and computational study demonstrating the first preparation of propen-2-ol (CHC(OH)CH) and its isomer methyl vinyl ether (CHOCHCH) in low-temperature acetone (CHCOCH) ices upon exposure to energetic electrons. Propen-2-ol is the simplest enol tautomer of a ketone. Exploiting tunable vacuum ultraviolet photoionization in conjunction with reflectron time-of-flight mass spectrometry, propen-2-ol and methyl vinyl ether were monitored in the gas phase upon sublimation during the temperature-programmed desorption process suggesting that both isomers are promising candidates for future astronomical searches such as the James Webb Space Telescope. Electronic structure calculations reveal that the barrier of keto-enol tautomerization can be reduced by more than a factor of two (162 kJ mol) through the involvement of solvating water molecules under realistic conditions on interstellar grains. The implicit solvent effects, , the influences of the solvent dipole field on the barrier height are found to be minimal and do not exceed 10 kJ mol. Our findings signify a crucial step toward a better understanding of the enolization of ketones in the interstellar medium thus constraining the molecular structures and complexity of molecules that form in extraterrestrial ices - ketones - through non-equilibrium chemistry.
烯醇-酮或醛的互变异构体-预计在星际介质中无处不在,并在深空形成复杂有机分子中发挥关键作用,但迄今为止,其基本形成机制仍很大程度上难以捉摸。在这里,我们进行了一项组合实验和计算研究,证明了在低温丙酮(CHCOCH)冰中首次制备丙烯-2-醇(CHC(OH)CH)及其异构体甲基乙烯基醚(CHOCHCH),方法是暴露于高能电子。丙烯-2-醇是酮的最简单烯醇互变异构体。利用可调谐真空紫外光电离结合反射飞行时间质谱,在程序升温脱附过程中监测升华过程中的气相中的丙烯-2-醇和甲基乙烯基醚,表明这两种异构体都是未来天文搜索的有希望的候选者,例如詹姆斯·韦伯太空望远镜。电子结构计算表明,通过在星际尘埃上的实际条件下涉及溶剂水分子,可以将酮烯醇互变异构化的势垒降低两倍以上(162 kJ mol)。溶剂的隐式效应,即溶剂偶极场对势垒高度的影响可忽略不计,不超过 10 kJ mol。我们的发现标志着朝着更好地理解星际介质中酮的烯醇化迈出了关键一步,从而通过非平衡化学限制了在天外冰中形成的分子的分子结构和复杂性-酮。