FeC4H2: A Potential Astrophysical Molecule Featuring Planar Tetracoordinate Iron to Unveil the Mystery of Missing Iron in Interstellar Medium

IF 2.9 3区 化学 Q2 CHEMISTRY, MULTIDISCIPLINARY ACS Earth and Space Chemistry Pub Date : 2024-09-25 DOI:10.1021/acsearthspacechem.4c0017810.1021/acsearthspacechem.4c00178
Shilpa Shajan,  and , Krishnan Thirumoorthy*, 
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Abstract

The exploration of iron-containing species represents a prominent area in contemporary astrochemical investigations. Iron in the interstellar medium exhibits predominantly low concentrations, hinting at the potential presence of missing iron in either a condensed or molecular state. The FeC4H2 neutral system has been investigated using computational calculations, emphasizing the hypothesis that missing iron may exist as iron–carbon hydride compounds or their higher order. A total of 61, 46, and 36 stationary points have been identified on the potential energy surface (PES) of the FeC4H2 in the singlet, triplet, and quintet electronic states, respectively, showcasing the existence of a planar tetracoordinate iron (ptFe). A linear geometry represents the global minimum on the PES of FeC4H2 as observed in the quintet ground electronic state. Meanwhile, the ptFe geometry is identified as the second most stable isomer in the quintet electronic state, which is the lowest energy solely in the singlet electronic state. Further, the observed ptFe geometry closely resembles the experimentally detected FeC4 molecule in the gas phase. In light of its similarity to FeC4 and the recent detection of FeC in the interstellar medium, the ptFe would be a potential astrophysical molecule that will also be identified in the gas phase. From that point of view, a comprehensive examination of the nature of chemical bonding of the ptFe geometry in the singlet, triplet, and quintet electronic states has been characterized, which dictates the stabilization of ptFe through multicenter bonding with surrounding carbon atoms. Ab initio molecular dynamics simulations revealed the dynamic stability of the system. Understanding the interstellar species with its structure and chemical bonding is an important aspect that would shed light on new insights into the experimental observations in the future.

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FeC4H2:以平面四配位铁为特征的潜在天体物理分子,揭开星际介质中铁缺失之谜
对含铁物种的探索是当代天体化学研究的一个重要领域。星际介质中的铁主要表现为低浓度,这暗示着可能存在凝结态或分子态的缺失铁。通过计算研究了 FeC4H2 中性体系,强调了缺失的铁可能以铁碳氢化物或其高阶化合物的形式存在的假设。在 FeC4H2 的单电子态、三电子态和五电子态的势能面(PES)上分别发现了 61、46 和 36 个静止点,显示了平面四配位铁(ptFe)的存在。在五重基态电子态观察到的线性几何形状代表了 FeC4H2 PES 的全局最小值。同时,ptFe 几何形状被确定为五元电子态中第二稳定的异构体,它是单电子态中能量最低的异构体。此外,观测到的 ptFe 几何形状与气相中实验检测到的 FeC4 分子非常相似。鉴于ptFe与FeC4的相似性以及最近在星际介质中探测到的FeC,ptFe将是一种潜在的天体物理分子,也将在气相中被识别出来。从这个角度出发,我们对ptFe几何形状在单电子态、三电子态和五电子态的化学键性质进行了全面研究,发现ptFe通过与周围碳原子的多中心键而稳定。Ab initio 分子动力学模拟揭示了该系统的动态稳定性。了解星际物种的结构和化学键是一个重要方面,将为今后的实验观测提供新的启示。
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来源期刊
ACS Earth and Space Chemistry
ACS Earth and Space Chemistry Earth and Planetary Sciences-Geochemistry and Petrology
CiteScore
5.30
自引率
11.80%
发文量
249
期刊介绍: The scope of ACS Earth and Space Chemistry includes the application of analytical, experimental and theoretical chemistry to investigate research questions relevant to the Earth and Space. The journal encompasses the highly interdisciplinary nature of research in this area, while emphasizing chemistry and chemical research tools as the unifying theme. The journal publishes broadly in the domains of high- and low-temperature geochemistry, atmospheric chemistry, marine chemistry, planetary chemistry, astrochemistry, and analytical geochemistry. ACS Earth and Space Chemistry publishes Articles, Letters, Reviews, and Features to provide flexible formats to readily communicate all aspects of research in these fields.
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Issue Publication Information Issue Editorial Masthead Structural Investigation of Diprotonated Glycine, Diprotonated Glycine Methyl Ester, and Monoprotonated Glycinoyl Fluoride FeC4H2: A Potential Astrophysical Molecule Featuring Planar Tetracoordinate Iron to Unveil the Mystery of Missing Iron in Interstellar Medium A CAPRAM Modeling Study on the Role of Heterogeneous Reactions on Dust in Tropospheric Chemistry
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