Li Feiyang, Wan Ye, Sun Dongquan, Wang Xiaolin, Hu Wenxuan
State Key Laboratory for Mineral Deposits Research, School of Earth Sciences and Engineering, Nanjing University, Nanjing, Jiangsu 210023, China.
Institute of Deep-sea Science and Engineering, Chinese Academy of Sciences, Sanya, Hainan 572000, China.
Spectrochim Acta A Mol Biomol Spectrosc. 2024 Mar 5;308:123774. doi: 10.1016/j.saa.2023.123774. Epub 2023 Dec 18.
Carbonaceous fluid within mineral-hosted inclusions provides important information for carbon cycle in deep Earth. In addition to CH and CO, heavy hydrocarbons (e.g., CH and CH) are frequently observed in carbonaceous fluid inclusions (i.e, wet gas inclusions with C/∑C < 0.95). However, determination of the composition of such complex volatiles is difficult based on traditional microthermometric measurements. Here we carried out experimental calibrations on Raman spectroscopic measurements of the pressure (P) and composition of the CH ± CH ± CH ± HS system at room temperature and 0.1-130 MPa. We confirmed that the C-H symmetric stretching vibration band of CH [ν(CH), ∼2917 cm] shifted to lower wavenumber with rising pressure, thus the P-ν(CH) relationship could be applied to calculate the pressure of wet gas. It should be noted that the presence of C+ and/or HS will shift the [ν(CH)] to lower wavenumber at constant pressure (with the order of CH ≥ HS > CH). Obviously, the P-ν(CH) relationship derived from pure CH system could not be simply applied to wet gas inclusion, otherwise the pressure would be overestimated. To avoid the overlap of the C-H vibrations of CH, CH and CH, the peak areas and peak heights of the overtone vibration of CH [2ν(CH), ∼2580 cm], C-C symmetric stretching vibrations of CH [ν(CH), ∼995 cm] and CH [ν(CH), ∼868 cm], and S-H symmetric stretching vibration of HS [ν(HS), ∼2612 cm] were fitted using Gaussian + Lorentz functions. The obtained peak areas and peak heights were then used to calculate the Raman quantification factors (F factor and G factor, respectively) of CH, CH and HS relative to CH, respectively. Both the F factor and G factor increased with rising pressure, whereas the FCH, FCH and GHS kept nearly constant at ∼5.69, 6.39 and 153.8, respectively in high pressure gas mixtures (e.g., >30 MPa). Therefore, for inclusions with higher internal pressure, the molar ratio of CH, CH, CH and HS could be determined by the aforementioned F and G factors. This method was applied to the calcite-hosted single-phase gas inclusions in the Upper Permian Changxing Formation carbonate reservoir from the eastern Sichuan Basin (South China). Our results indicated that the trapping pressure would be obviously overestimated if the presence of heavy hydrocarbons was not taken into account.
矿物包裹体中的含碳流体为地球深部碳循环提供了重要信息。除了CH₄和CO₂外,重烃(如C₂H₆和C₃H₈)也经常在含碳流体包裹体中被观察到(即C₁/∑C₁<0.95的湿气包裹体)。然而,基于传统的显微测温测量来确定这种复杂挥发物的成分是困难的。在此,我们对室温及0.1 - 130MPa条件下CH₄±C₂H₆±C₃H₈±H₂S体系的压力(P)和成分进行了拉曼光谱测量的实验校准。我们证实,CH₄的C - H对称伸缩振动带[ν(C - H),2917cm⁻¹]随压力升高向低波数移动,因此P - ν(C - H)关系可用于计算湿气的压力。需要注意的是,C₂H₄和/或H₂S的存在会在恒定压力下使[ν(C - H)]向低波数移动(顺序为C₂H₄≥H₂S>C₂H₆)。显然,从纯CH₄体系得出的P - ν(C - H)关系不能简单地应用于湿气包裹体,否则压力会被高估。为避免CH₄、C₂H₆和C₃H₈的C - H振动重叠,使用高斯 + 洛伦兹函数拟合了CH₄的倍频振动[2ν(C - H),2580cm⁻¹]、C₂H₄的C - C对称伸缩振动[ν(C - C),995cm⁻¹]和C₃H₈的[ν(C - C),868cm⁻¹]以及H₂S的S - H对称伸缩振动[ν(S - H),2612cm⁻¹]的峰面积和峰高。然后将得到的峰面积和峰高分别用于计算C₂H₆、C₃H₈和H₂S相对于CH₄的拉曼定量因子(分别为F因子和G因子)。F因子和G因子均随压力升高而增加,而在高压气体混合物(如>30MPa)中,FCH₄、FCH₃、GHS分别在5.69、6.39和153.8左右保持近恒定。因此,对于内部压力较高的包裹体,CH₄、C₂H₆、C₃H₈和H₂S的摩尔比可通过上述F和G因子确定。该方法应用于四川盆地东部(中国南方)上二叠统长兴组碳酸盐岩储层中方解石寄主的单相气体包裹体。我们的结果表明,如果不考虑重烃的存在,捕获压力将被明显高估。