Department of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125;
Department of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA 91125.
Proc Natl Acad Sci U S A. 2020 Feb 25;117(8):3989-3995. doi: 10.1073/pnas.1906507117. Epub 2020 Feb 11.
Natural gas is a key energy resource, and understanding how it forms is important for predicting where it forms in economically important volumes. However, the origin of dry thermogenic natural gas is one of the most controversial topics in petroleum geochemistry, with several differing hypotheses proposed, including kinetic processes (such as thermal cleavage, phase partitioning during migration, and demethylation of aromatic rings) and equilibrium processes (such as transition metal catalysis). The dominant paradigm is that it is a product of kinetically controlled cracking of long-chain hydrocarbons. Here we show that C-alkane gases (ethane, propane, butane, and pentane) are initially produced by irreversible cracking chemistry, but, as thermal maturity increases, the isotopic distribution of these species approaches thermodynamic equilibrium, either at the conditions of gas formation or during reservoir storage, becoming indistinguishable from equilibrium in the most thermally mature gases. We also find that the pair of CO and C (methane) exhibit a separate pattern of mutual isotopic equilibrium (generally at reservoir conditions), suggesting that they form a second, quasi-equilibrated population, separate from the C to C compounds. This conclusion implies that new approaches should be taken to predicting the compositions of natural gases as functions of time, temperature, and source substrate. Additionally, an isotopically equilibrated state can serve as a reference frame for recognizing many secondary processes that may modify natural gases after their formation, such as biodegradation.
天然气是一种关键的能源资源,了解其形成机制对于预测其在具有经济重要性的体积中形成的位置非常重要。然而,干热成因天然气的起源是石油地球化学中最具争议的话题之一,提出了几种不同的假说,包括动力学过程(如热裂解、迁移过程中的相分离和芳环脱甲基化)和平衡过程(如过渡金属催化)。占主导地位的范式是它是长链碳氢化合物动力学控制裂解的产物。在这里,我们表明 C-链烷烃气体(乙烷、丙烷、丁烷和戊烷)最初是通过不可逆裂解化学产生的,但随着热成熟度的增加,这些物质的同位素分布接近热力学平衡,无论是在气体形成条件下还是在储层储存过程中,在最热成熟的气体中与平衡状态没有区别。我们还发现 CO 和 C(甲烷)之间存在一对单独的同位素平衡模式(通常在储层条件下),这表明它们形成了第二个准平衡种群,与 C 到 C 化合物分开。这一结论意味着应该采取新的方法来预测天然气的组成作为时间、温度和源底物的函数。此外,同位素平衡状态可以作为识别许多可能在形成后改变天然气的次生过程的参考框架,例如生物降解。