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Carbon isotopic evidence for the catalytic origin of light hydrocarbons
Geochemical Transactions volume 1, Article number: 38 (2000)
The molecular proportionality between C6 and C7 isomers reported recently (F. D. Mango, Geochim. Cosmochim. Acta, 2000, 64, 1265; ref. 1) is probably the strongest evidence for catalysis yet published. It implicates two cyclopropane-like precursors, [S6] and [S7] (where S denotes any substrate), of similar structures, each yielding three isomers along similar kinetic pathways:
[S6] → n-hexane + 2-methylpentane + 3-methylpentane
[S7] → n-hexane + 2-methylhexane + 3-methylhexane
This view is supported here by the carbon isotope ratios of these isomers in 36 oils from Western Canada (M. J. Whiticar and L. R. Snowdon, Org. Geochem., 1999, 30, 1127; ref. 2). They exhibit strong correlations in δ13C, consistent with their being formed in triads through isotopically indistinguishable precursors. These results add significantly to the growing body of evidence supporting catalysis.
There can be little doubt that light hydrocarbons (C1–C9) can be produced thermally from decomposing hydrocarbons in sedimentary rocks. Although other pathways have always seemed possible (e.g., catalysis[4, 5]), they were rarely given serious consideration until it became clear that (a) ordinary hydrocarbons should remain stable under the time–temperature conditions typically seen in sedimentary rocks, [6–9] and (b) thermal cracking in the laboratory does not produce a gas resembling natural gas. [8, 10–16] Catalysis gained additional recognition in 1987 when an invariance in isoheptanes was disclosed. That work introduced steady-state kinetics as a critical, if not necessary, element to light hydrocarbons (LH) genesis, thereby undermining thermal cracking as the sole explanation.
Catalysis by acidic clay minerals [18–20] and reduced transition metals were offered as alternative sources of LHs. However, only the latter has reproduced the composition of natural gas in the laboratory. [22–25] LHs exhibit a striking molecular proportionality consistent with a catalytic origin through cyclopropane-like intermediates, a mechanism independently supported elsewhere.[26, 27] An isotopic analysis of these same hydrocarbons is reported here. The data used are from Whiticar and Snowdon who reported the molecular and isotopic compositions for 26 LHs in 42 oils and condensates from Western Canada.
Results and discussion
If the kinetic pathways [S6] → [n-C6 + 2-MP + 3-MP] and [S7] → [n-C7 + 2-MH + 3-MH] are energetically similar, as would be the case in Fig. 1 for example, then the following proportionality obtains:
[(n-C6)(MHs)]/[(MPs)(n-C7)] = α (1)
(where MHs = 2-methylhexane + 3-methylhexane; MPs = 2-methylpentane + 3-methylpentane).
The LH in crude oils obey eqn. (1) to a remarkable degree. Fig. 2 shows the correlation between [(n-C6)(MHs)] and [(MPs)(n-C7)] in concentrations of wt.% total oil (r2 = 0.99; ref. 1). α is tightly constrained to a mean of 0.75 with a standard deviation (s) of 0.20 (mean centered), significantly below those of the ratios composing α: s = 0.42 for (n-C6/n-C7), 0.46 for (n-C6/MPs), 0.51 for (n-C6/MHs), and 0.41 for (MPs/MHs).
Moreover, the variability of α is unique to its particular combination of product functions. Its s of 0.20 increases by a factor of four in [(MPs)(MHs)]/[(n-C6)(n-C7)] and by a factor of almost five in [(n-C7)(MHs)]/[(n-C6)(MPs)] (ref. 1). Thus, at all concentrations, [(n-C6)(MHs)] and [(MPs)(n-C7)] express a strong and significant correlation in crude oils, perhaps the strongest yet disclosed among LHs, while a remains nearly constant.
This relationship establishes a genetic link between [n-C6 + 2-MP + 3-MP] and [n-C7 + 2-MH + 3-MH] pointing to structurally similar precursors. It would be reinforced if it could also be shown that the six LH reflect isotopically similar precursors. Although δ13C for [S6] and [S7] cannot be measured directly, they can be calculated from the weighted sums:
δ13C([S6]) = a δ13C(2-MP) + b δ13C(3-MP)+ c δ13C(n-C6) (2)
δ13C([S7]) = d δ13C(2-MP) + e δ13C(3-MP) + f δ13C(n-C6) (3)
(where a, b and c (d, e, and f) are the molecular fractions of the respective isomers; a + b + c = 1, and d + e + f = 1). Thus, δ13C's for [S6] and [S7] can be calculated from the δ13C's and molecular fractions of the six isomers.
Whiticar and Snowdon published this data for the LH in 42 oils from Western Canada. Table 1 was constructed from their data. It contains 36 of their oils, including all with sufficient data to calculate δ13C ([S6]) and δ13C ([S7]) except for two, possibly altered oils. Fig. 3 shows [S6] to be isotopically indistinguishable from [S7]. The mean for δ13C ([S6])/δ13C ([S7]) = 1.00 ± 0.024s, which is within the experimental error reported for this data (± 0.5s).
Fig. 2 (ref. 1) provides molecular evidence for structurally similar precursors, like the hypothetical intermediates [S6] and [S7] in Fig. 1. Fig. 3 is consistent with this, implicating isotopically indistinguishable precursors. Whiticar and Snowdon came to a similar conclusion: "these isotopic distributions among isomers are strong evidence suggesting that the formation of these gasoline-range hydrocarbons is intricately linked to the isotopic signature of the precursor molecules from which they are derived".
Fig. 3 does not exclude the conventional view that LH are thermal descendents of higher isoprenoids and n-alkanes (ref. 28). But it is difficult to explain the two correlations (Fig. 2 and 3) by this mechanism. They suggest a catalytic agent guiding the course of reaction through structurally similar intermediates. Irrespective of how these six LH might originate (catalytically or thermally), however, their molecular and isotopic correlations establish a genetic link (↔) between n-alkanes and isoalkanes that traverses carbon number and is fundamental to the origin of LH:
[n-C6 ↔ 2-MP ↔ 3-MP] ↔ [n-C7 ↔ 2-MH ↔ 3-MH]
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I am grateful to the US Department of Energy for Grant DE-FG05-92ER14295. I thank Alan Young for his review of the manuscript and helpful comments.
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Mango, F.D. Carbon isotopic evidence for the catalytic origin of light hydrocarbons. Geochem Trans 1, 38 (2000). https://doi.org/10.1186/1467-4866-1-38
- Carbon Isotope
- Light Hydrocarbon
- Carbon Isotope Ratio
- Molecular Fraction