嵌入星际冰中的甘氨酸分子的温度驱动的转变
Maysa Yusef-Buey1, Tzonka Mineva2, Dahbia Talbi3
1Laboratoire de Chimie et Physique Quantique (LCPQ/FERMI), UMR5626, Université de Toulouse (UPS) and CNRS, 118 Route de Narbonne, F-31062 Toulouse, France.
Physical chemistry chemical physics : PCCP
|January 3, 2024
概括
星际冰粒上的氨基酸甘氨酸保持其中性形式. 淘米化取决于水分子和同位体结构,这对于理解太空中的 prebiot 化学是至关重要的.
科学领域:
- 天体化学是天体化学.
- 计算化学的计算化学
- 生物化学 生物化学
背景情况:
- 甘氨酸是一种关键的氨基酸,在星际冰粒中发现.
- 它在太空中的形成和稳定性对于理解生命起源至关重要.
- 星际甘氨酸化学需要了解其在冰冷环境中的行为.
研究的目的:
- 调查甘氨酸的构造空间和分体化机制.
- 在星际冰和类似水的环境中模拟糖氨酸.
- 在太空条件下确定甘氨酸的稳定性和潜在的转变.
主要方法:
- 量子力学/分子力学 (QM/MM) 分子动力学模拟.
- 研究了四种甘氨酸异构体 (cc,ct,tc,tt).
- 模拟条件包括20K的星际低密度无形 (LDA) 冰,以及更高的温度 (250K,450K) 来模拟升温事件. 在水集群中也模拟了甘氨酸 (4,17,27 H2O分子).
主要成果:
- 甘氨酸异构体在星际冰 (20K) 中大部分保留它们的中性构造.
- 陶氏化受到水分子数量和特定的甘氨酸异构体的显著影响.
- 在水集群中的模拟显示了根据水集群大小的不同分体化行为.
结论:
- 甘氨酸的规范中性构造在典型的星际冰条件下是稳定的.
- 水分子在调解甘氨酸的分体化中起着至关重要的作用.
- 了解这些过程对于天体生物学和寻找外星生命至关重要.
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