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Underground Coal Gasification transforms coal into energy underground, but doing so safely and efficiently requires understanding one of the most complex coupled subsurface processes in energy engineering.
It is an in-situ process that converts coal into syngas by injecting oxidants into a coal seam and producing combustible gases through a network of high-temperature chemical reactions.
In this study, CMG STARS was used to develop a fully coupled thermal-hydro-mechanical-chemical (THMC) model of UCG, capturing the evolution of the gasification cavity, chemical reactions, composition of produced syngas, production behavior, and subsidence.
Outcome: The model demonstrates how coupled simulation can predict cavity growth, gas production, and geomechanical deformation, providing critical insights for safe and efficient UCG operations.
UCG is a process where coal is converted into gas underground, rather than being mined and processed at the surface.
The process involves:
Unlike oil & gas production:
This makes UCG not just a flow problem, but a reactive, deforming system.
UCG is one of the most complex subsurface processes to simulate because it requires simultaneous coupling of multiple physical domains.
UCG involves multiple reactions, including:
Example (Pyrolysis: from the model below):
Coal 🡪 Char + CO + CO₂ + H₂ + CH₄
Despite the interdependencies among the reactions, each reaction has:
This implies that the treatment of coal seams in the UCG process is fundamentally different from that of conventional oil and gas reservoirs, where the available pore volume for fluids changes far less significantly.
As the cavity grows:
This directly impacts:
CMG STARS enables:
This makes it uniquely suited for UCG modeling.
From the simulation setup:
The simulation includes:
With full kinetic parameters:
This enables realistic gas composition prediction. The key step in modeling UCG reactions in STARS is representing the pyrolysis process as accurately as possible, in which coal is consumed to produce char that subsequently combusts and generates the required in-situ heat. In addition, this process produces significant quantities of gaseous species that serve as reactants in subsequent gasification and combustion reactions. Leveraging coal elemental analysis to derive realistic stoichiometric coefficients for the pyrolysis reaction is therefore of critical importance.
The simulation shows:

Gas production is directly linked to:
Gas production strategies must account for reaction front progression and cavity evolution to avoid premature decline.
After ~90 days:

The cavity is not uniform. It evolves based on:
Pyrolysis and char combustion reactions occur mainly along the cavity boundaries. However, due to the tendency of gas flow toward the production perforation, the high-temperature front is typically oriented in that direction and gradually advances toward the producer over time.

Results show:

Reaction zones migrate dynamically, altering:
Simulation shows:



Geomechanics directly affects:
Subsidence prediction is critical for ensuring well integrity and minimizing surface impact.
This case demonstrates that UCG is not just about maximizing gas production.
It requires understanding:
Underground Coal Gasification is one of the most complex subsurface processes to model, requiring the integration of chemical reactions, fluid flow, heat transfer, and geomechanics.
This study demonstrates that CMG STARS provides a unified framework to simulate these coupled processes, enabling accurate prediction of gas production, cavity evolution, and subsurface deformation.
By capturing the full system behavior, engineers can move beyond simplified assumptions and make more informed decisions about UCG design, operation, and safety.