Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Université Grenoble Alpes/CNRS-INSU, UMR 5274, Grenoble F-38041, France.
Institut de Planétologie et d'Astrophysique de Grenoble (IPAG), Université Grenoble Alpes/CNRS-INSU, UMR 5274, Grenoble F-38041, France.
Spectrochim Acta A Mol Biomol Spectrosc. 2021 Oct 5;259:119853. doi: 10.1016/j.saa.2021.119853. Epub 2021 Apr 24.
The determination of the abundances of the CH, C = O and aromatic groups in chondritic Insoluble Organic Matter (IOM) and coals by Infrared (IR) spectroscopy is a challenging issue due to insufficient knowledge on the absorption cross-sections and their sensitivity to the molecular environment. Here, we report a calibration approach based on a C synthetic model material whose composition was unambiguously determined by Direct-Pulse/Magic Angle Spinning Nuclear Magnetic Resonance (DP/MAS NMR). Ratios of the cross-sections of the CH, C = O and aromatic groups have been determined, and the method has been applied to IOM samples extracted from four chondrites as Orgueil (CI), Murchison (CM), Tagish Lake (C2-ungrouped) and EET 92042 (CR2), and to a series of coals. The estimate of the aliphatic to aromatic carbon ratio (n/n) in IOM samples from Orgueil, Murchison and Tagish Lake chondrites is in good agreement with Single-Pulse/NMR estimates earlier published, and is lower by a factor of 1.3 in the case of the CR chondrite EET 92042 (but the error bars overlap). In contrast, the aliphatic to carbonyl ratio (n/n) is overestimated for the four chondrites. These discrepancies are likely due to the control of the absorption cross-section of the C = O and C = C bonds by the local molecular environment. Regarding coals, the use of published NMR analyses has brought to light that the integrated cross-section ratio A/A varies with the vitrinite reflectance over an order of magnitude. Here as well, the local oxygen speciation plays a critical control in A, which decreases with increasing the vitrinite reflectance. We provide an analytical law that links A/A and vitrinite reflectance, which will allow the determination of n/n for any coal sample, provided its vitrinite reflectance is known.
由于对吸收截面及其对分子环境的敏感性了解不足,用红外(IR)光谱法测定球粒陨石不溶性有机质(IOM)和煤中 CH、C=O 和芳族基团的丰度是一个具有挑战性的问题。在这里,我们报告了一种基于 C 合成模型材料的校准方法,该模型材料的组成通过直接脉冲/魔角旋转核磁共振(DP/MAS NMR)明确确定。确定了 CH、C=O 和芳族基团的截面比,并将该方法应用于从 4 颗陨石中提取的 IOM 样品,包括 Orgueil(CI)、Murchison(CM)、Tagish Lake(C2-未分组)和 EET 92042(CR2),以及一系列煤。Orgueil、Murchison 和 Tagish Lake 陨石 IOM 样品中脂肪族与芳族碳比(n/n)的估计与早先发表的单脉冲/NMR 估计值非常吻合,而 CR 陨石 EET 92042 的估计值低 1.3 倍(但误差幅度重叠)。相比之下,四种陨石的脂肪族与羰基比(n/n)被高估。这些差异可能是由于 C=O 和 C=C 键的吸收截面受局部分子环境的控制。关于煤,使用已发表的 NMR 分析表明,积分截面比 A/A 随镜质体反射率变化一个数量级。同样,局部氧态也对 A 起着关键的控制作用,随着镜质体反射率的增加,A 减小。我们提供了一个分析定律,将 A/A 和镜质体反射率联系起来,只要知道煤样的镜质体反射率,就可以确定任何煤样的 n/n。