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The survival of glycine in interstellar ices: A coupled investigation using NEXAFS experiments and theoretical calculations

机译:甘氨酸在星际冰中的存活:使用NEXAFS实验和理论计算的耦合研究

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Complex organic molecules have been observed in the interstellar medium in comets and meteorites. Among these compounds are the building blocks that may have led to prebiotic systems and ultimately to the origin of life. In the panspermia hypothesis, the survival and the transfer of the amino acids from space to planets is a necessary condition for the appearance of life, and, especially, their resistance to the solar UV radiation in ice is a key issue. The case of glycine, which is the smallest molecule in the amino acid family, is presented here. To improve our knowledge on the decomposition mechanisms of glycine, we have undertaken a coupled experimental and computational study. On the one hand, it has been performed a near-edge X-ray absorption spectroscopy (NEXAFS) study at the oxygen K-edge of solid glycine and of glycine diluted into H_2O ice, and irradiated at 30 K with soft X-rays. However, extensive quantum chemical simulations using density functional theory have been realized at the B3LYP/cc-pVQZ level. A systematic investigation of the most plausible fragmentations has been performed for neutral glycine itself, ionized glycine, doubly ionized glycine, protonated glycine, and zwitterionic glycine, the well known stable form of glycine trapped in ices. We show that glycine easily decomposes under irradiation. Water does not enhance or protect glycine from photodecomposition, but it increases the production of CO_2 in the secondary photoreactions. The concentration of glycine tends to a limit of ~30% of the initial load in the ice. The role of water ice appears to be that of a containment environment allowing the fragments to remain close, thus leading to reformation of glycine in situ. Under these conditions, it can be concluded that glycine is partially, but not entirely, protected by ice during its journey to the Earth. It is a strong point to be credited to the panspermia hypothesis.
机译:在星际介质中的彗星和陨石中观察到了复杂的有机分子。在这些化合物中,可能是导致益生元系统并最终导致生命起源的基础。在全精子假说中,氨基酸的生存和从太空到行星的转移是生命出现的必要条件,尤其是其对冰中太阳紫外线辐射的抵抗力是一个关键问题。甘氨酸是氨基酸家族中最小的分子,在此介绍。为了提高我们对甘氨酸分解机理的认识,我们进行了实验和计算的耦合研究。一方面,已经在固体甘氨酸和稀释到H_2O冰中的甘氨酸的氧K边缘进行了近边缘X射线吸收光谱(NEXAFS)研究,并在30 K下用软X射线照射。但是,已经在B3LYP / cc-pVQZ级别实现了使用密度泛函理论的大量量子化学模拟。对中性甘氨酸本身,离子化甘氨酸,双离子化甘氨酸,质子化甘氨酸和两性离子甘氨酸(被困在冰中的众所周知的稳定形式)进行了最合理的裂解的系统研究。我们表明,甘氨酸在辐射下容易分解。水不能增强或保护甘氨酸免于光分解,但会增加次级光反应中CO_2的产生。甘氨酸的浓度趋向于在冰中初始负荷的约30%的极限。水冰的作用似乎是封闭环境,其允许碎片保持紧密,从而导致甘氨酸原位重整。在这些条件下,可以得出结论,在冰到达地球的过程中,甘氨酸部分但不是全部受到冰的保护。值得一提的是,它可以归因于泛精子症的假设。

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