Maity Surajit, Kaiser Ralf I, Jones Brant M
Department of Chemistry, W.M. Keck Research Laboratory in Astrochemistry, University of Hawai'i at Manoa, Honolulu, HI 96822, USA.
Phys Chem Chem Phys. 2015 Feb 7;17(5):3081-114. doi: 10.1039/c4cp04149f. Epub 2014 Dec 17.
The radiation induced chemical processing of methanol and methanol-carbon monoxide ices at 5.5 K exposed to ionizing radiation in the form of energetic electrons and subsequent temperature programmed desorption is reported in this study. The endogenous formation of complex organic molecules was monitored online and in situ via infrared spectroscopy in the solid state and post irradiation with temperature programmed desorption (TPD) using highly sensitive reflectron time-of-flight (ReTOF) mass spectrometry coupled with single photoionization at 10.49 eV. Infrared spectroscopic analysis of the processed ice systems resulted in the identification of simple molecules including the hydroxymethyl radical (CH2OH), formyl radical (HCO), methane (CH4), formaldehyde (H2CO), carbon dioxide (CO2), ethylene glycol (HOCH2CH2OH), glycolaldehyde (HOCH2CHO), methyl formate (HCOOCH3), and ketene (H2CCO). In addition, ReTOF mass spectrometry of subliming molecules following temperature programmed desorption definitely identified several closed shell C/H/O bearing organics including ketene (H2CCO), acetaldehyde (CH3COH), ethanol (C2H5OH), dimethyl ether (CH3OCH3), glyoxal (HCOCOH), glycolaldehyde (HOCH2CHO), ethene-1,2-diol (HOCHCHOH), ethylene glycol (HOCH2CH2OH), methoxy methanol (CH3OCH2OH) and glycerol (CH2OHCHOHCH2OH) in the processed ice systems. Additionally, an abundant amount of molecules yet to be specifically identified were observed sublimating from the irradiated ices including isomers with the formula C3H(x=4,6,8)O, C4H(x=8,10)O, C3H(x=4,6,8)O2, C4H(x=6,8)O2, C3H(x=4,6)O3, C4H8O3, C4H(x=4,6,8)O4, C5H(x=6,8)O4 and C5H(x=6,8)O5. The last group of molecules containing four to five oxygen atoms observed sublimating from the processed ice samples include an astrobiologically important class of sugars relevant to RNA, phospholipids and energy storage. Experiments are currently being designed to elucidate their chemical structure. In addition, several reaction pathways were identified in the irradiated ices of mixed isotopes based upon the results of both in situ FTIR analysis and TPD ReTOF gas phase analysis. In general, the results of this study provide crucial information on the formation of a variety of classes of organics including alcohols, ketones, aldehydes, esters, ethers, and sugars within the bulk ices upon exposure to ionizing radiation that are relevant to the molecular clouds within the interstellar medium.
本研究报道了在5.5 K下,以高能电子形式的电离辐射对甲醇和甲醇 - 一氧化碳冰进行辐射诱导化学处理,随后进行程序升温脱附的过程。通过固态红外光谱在线原位监测复杂有机分子的内源性形成,并在辐照后使用高灵敏度反射式飞行时间(ReTOF)质谱结合10.49 eV的单光子电离进行程序升温脱附(TPD)。对处理后的冰体系进行红外光谱分析,鉴定出了包括羟甲基自由基(CH2OH)、甲酰基自由基(HCO)、甲烷(CH4)、甲醛(H2CO)、二氧化碳(CO2)、乙二醇(HOCH2CH2OH)、乙醇醛(HOCH2CHO)、甲酸甲酯(HCOOCH3)和乙烯酮(H2CCO)在内的简单分子。此外,程序升温脱附后升华分子的ReTOF质谱明确鉴定出处理后的冰体系中几种含闭壳C/H/O的有机物,包括乙烯酮(H2CCO)、乙醛(CH3COH)、乙醇(C2H5OH)、二甲醚(CH3OCH3)、乙二醛(HCOCOH)、乙醇醛(HOCH2CHO)、1,2 - 乙二醇(HOCHCHOH)、乙二醇(HOCH2CH2OH)、甲氧基甲醇(CH3OCH2OH)和甘油(CH2OHCHOHCH2OH)。此外,还观察到大量尚未明确鉴定的分子从辐照冰中升华,包括分子式为C3H(x = 4,6,8)O、C4H(x = 8,10)O、C3H(x = 4,6,8)O2、C4H(x = 6,8)O2、C3H(x = 4,6)O3、C4H8O3、C4H(x = 4,6,8)O4、C5H(x = 6,8)O4和C5H(x = 6,8)O5的异构体。从处理后的冰样品中升华出来的最后一组含有四到五个氧原子的分子包括一类与RNA、磷脂和能量储存相关的对天体生物学很重要的糖类。目前正在设计实验以阐明它们的化学结构。此外,根据原位傅里叶变换红外光谱分析和TPD ReTOF气相分析的结果,在混合同位素的辐照冰中确定了几种反应途径。总的来说,本研究结果为星际介质中与分子云相关的大块冰在暴露于电离辐射时形成各种有机化合物(包括醇、酮、醛、酯、醚和糖)提供了关键信息。