Vitrinite particle with pitted surface (tiny black spots) and iron oxides with reddish internal reflections. Source: Fernández et al. (2025) - International Journal of Coal Geology
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Geology & Geophysics

A cool vitrinite reflectance model

Following decades of refinement, the current VRo model seems well-versed to reconstruct the timing of source rock maturation

A basin model de­scribes the ther­mal evolution of a basin to esti­mate when its source rocks expel hydrocarbons and of what type. Basin models do so by evaluating a num­ber of relationships, such as heat flow from beneath the basin, heat generation, heat transfer through the sedi­ments and the loss of heat at surface.

These relationships need to be anchored to provide somewhat accurate results for the unknown past. One obvious anchor is the pres­ent-day temperature meas­ured at the surface and in wells. This fairly reliably anchors one end of the mod­elled history but leaves large uncertainty for the entire modelled history. We need other indirect thermal indi­cators informing us about the thermal conditions in the past. The most widely used one is the reflectance of light off the surface of woody particles, called vit­rinite.

Vitrinite is the prin­cipal component of coal but is also present in trace amounts in other hydrocar­bon source rocks. As vitrin­ite thermally matures, its in­ternal structure rearranges, leading to an increase in its ability to reflect light. Pio­neered by the coal industry, vitrinite reflectance (VRo) was eventually tied to time and temperature through lab heating experiments and field investigations. Initial VRo models relied on statistical correlations between VR and tempera­ture-time exposure. By the 1980s and 1990s, models such as Sweeney & Burn­ham’s VITRIMAT intro­duced kinetic reaction prin­ciples. These models treated vitrinite transformation as a series of temperature-de­pendent reactions, signif­icantly improving predic­tions over simple empirical relationships. EASY%Ro, a simplified version of VIT­RIMAT, in particular, be­came widely adopted due to its ease of implementation and broad applicability.

The 2000s saw further refinements with mod­els incorporating variable activation energies and detailed kinetic reaction schemes. These refinements were driven by growing computational speed, bet­ter calibration sample sets and the need to explain the mismatch of VRo mod­els with some VRo data. More extensive calibration data proved an older idea that VRo evolution during burial is affected by the presence of liptinite organ­ic matter. Vitrinite from woody coals increases its reflectance gradually with increasing temperature and time. Vitrinite from liptinite-rich samples (i.e. with high hydrogen index) display delayed reflectance at lower temperatures and faster reflectance increase at higher temperatures. This caused two phenom­ena observed in common VRo data: 1) the “dog leg” kink in the VRo trend at depth and 2) appar­ent “VRo suppression” in high-quality source rock samples (with high HI) rel­ative to EASY%Ro model. This also means that basin models calibrated to the EASY%Ro model tend to overestimate the thermal history of a basin in order to fit the “suppressed” VRo calibration data.

An updated model, EASY%Ro-DL, solved this problem by calibrating its parameters to higher-HI samples and by adjusting the frequency factor of the reaction equations to yield more consistent results over a range of heating rates. Various uncertainties re­main in VRo application for basin modelling, but I think that, at the very least, we now have a suffi­ciently accurate VRo mod­el to interpret available VRo data.

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