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AAPG Bulletin, Vol. 89 (2005). Program Abstracts (Digital).

AAPG Hedberg Conference
Vail, Colorado
April 24-29, 2005

ABSTRACT: Experimental Insights on Sources, Amounts, and Kinetics of Thermogenic Previous HitGasNext Hit

Michael D. Lewan
U. S. Geological Survey, Box 25046, MS 977, Denver Federal Center, Denver, CO 80225

The familiar paradigm for thermogenic Previous HitgasNext Hit generation suggests that, with increasing thermal maturity source rocks first generate Previous HitoilNext Hit and then generate thermogenic Previous HitgasNext Hit. This Previous HitgasNext Hit may be supplemented with additional thermogenic Previous HitgasNext Hit generated by the cracking of Previous HitoilNext Hit in deeply buried reservoirs. Various nuances of this sequence for thermogenic-Previous HitgasNext Hit generation and the required thermal-stress levels at which they occur have been proposed. However, this paradigm is based on intuitive interpretations of limited subsurface data. As a result, a quantitative understanding of sources, amounts, and kinetics of thermogenic Previous HitgasNext Hit in the subsurface has not fully developed into scientific concepts that can be applied to the assessment and exploration of conventional- and unconventional-Previous HitgasNext Hit resources. These limited subsurface data in the vastness of sedimentary basins, and the mobility of Previous HitgasNext Hit and Previous HitoilNext Hit to migrate through out a basin, makes laboratory pyrolysis experiments critical to developing a scientific understanding of thermogenic-Previous HitgasNext Hit generation. It is important that laboratory pyrolysis experiments be scrutinized in terms of how well their conditions and products simulate the natural process of thermogenic-Previous HitgasNext Hit generation. When unanticipated pyrolysis results present themselves, one must ask whether the results are revealing a new concept not previously considered in interpreting the limited subsurface data or are they simply an artifact of experimental conditions employed in the laboratory. This quandary can be minimized by conducting laboratory pyrolysis experiments as close to natural conditions as possible in order to understand reactions and mechanisms responsible for natural thermogenic-Previous HitgasNext Hit generation. With water being ubiquitous in the subsurface, pyrolysis experiments conducted in the presence of water at the lowest possible temperatures have proven to best simulate natural petroleum generation. These hydrous pyrolysis experiments provide insights on the sources, amounts, and kinetics of thermogenic Previous HitgasNext Hit that facilitate the development of scientifically sound concepts.

The two major sources of thermogenic Previous HitgasNext Hit typically considered in pyrolysis experiments are maturing source rocks and cracking of reservoir oils. Hydrous pyrolysis experiments on Previous HitoilNext Hit-prone source rocks indicate Previous HitgasNext Hit and Previous HitoilNext Hit generation is synchronous, which results in low ultimate Previous HitgasNext Hit:Previous HitoilNext Hit ratios (GORs<1,500 scf/bbl). These results indicate that basins with higher GORs (>1,500 scf/bbl) are sourced from Previous HitgasNext Hit-prone source rocks and (or) from cracking of Previous HitoilNext Hit in deeply buried reservoirs. Hydrous pyrolysis experiments also provide insights on the amount of thermogenic Previous HitgasNext Hit generated from source rocks containing different types of kerogen (i.e., Type-I, -II, -IIS, and III). Counter to our intuitive concepts, pyrolysis experiments indicate Previous HitoilNext Hit-prone kerogen (Type-I, II, and IIS) generates significantly more thermogenic Previous HitgasNext Hit than Previous HitgasNext Hit-prone kerogen (Type-III) on an organic-carbon basis. Type-IIS kerogen generates almost 2.5 times more thermogenic Previous HitgasNext Hit than Type-III kerogen, and Type-I and -II kerogen generates 1.8 times more thermogenic Previous HitgasNext Hit than Type-III kerogen. These results indicate that our designation of Previous HitoilNext Hit-prone and Previous HitgasNext Hit-prone source rocks are in reference to the proportions of Previous HitgasNext Hit to Previous HitoilNext Hit generated and not necessarily the amount of Previous HitgasNext Hit generated. The amounts of these different kerogen types needed to deem a rock, as a Previous HitgasNext Hit-prone source remains an issue that is currently being investigated by pyrolysis experiments. Results from hydrous pyrolysis experiments also show that on an organic-carbon basis the amount of thermogenic Previous HitgasNext Hit generated from thermal cracking of reservoir Previous HitoilNext Hit may be 3 to 4 times greater than thermogenic Previous HitgasNext Hit generation from source rocks. The significance of this Previous HitgasNext Hit source in a basin depends on Previous HitoilNext Hit remaining in coherent traps that are deeply buried in high thermal-maturity regimes.

Kinetics determines the timing and thermal maturity level of thermogenic Previous HitgasNext Hit generation from different sources. A consensus on appropriate kinetic parameters for thermogenic Previous HitgasNext Hit generation has not emerged, and a better scientific understanding of precursors, reactions, and mechanisms of Previous HitgasNext Hit generation under geological conditions is needed. Figure 1 shows generation curves based on published hydrous- and hydrothermal-pyrolysis kinetic parameters for generation of Previous HitoilNext Hit, source-rock Previous HitgasNext Hit, and Previous HitoilNext Hit-cracking Previous HitgasNext Hit at the base of the Mowry Shale at the Eagle Nest location in the Greater Green River Basin. Based on the vitrinite reflectance attained at the base of the Mowry Shale, 95% of Previous HitoilNext Hit generation is complete by 1.1 %Ro, 90% of source-rock Previous HitgasNext Hit generation is complete by 1.5 %Ro, and 10% of Previous HitgasNext Hit generation from Previous HitoilNext Hit cracking is complete by 2.1 %Ro. These results indicate that there is a significant gap (1.5 and 2.1 %Ro) in Previous HitgasNext Hit generation between maturing source rocks and Previous HitoilNext Hit cracking that current paradigms for Previous HitgasNext Hit generation have not considered. This maturity gap has been shown to have important implications in some areas and attests to the need for more experimental kinetic studies on Previous HitgasNext Hit generation.

 

Figure 1.Generation curves for Previous HitoilNext Hit (type-II), source-rock Previous HitgasNext Hit (C1+C2), and Previous HitoilNext Hit-cracking Previous HitgasNext Hit at the base of the Mowry Shale at the Eagle Nest location in the Greater Green River Basin. Curves are based on hydrous and hydrothermal pyrolysis kinetics, EASY%Ro, a 26.8°C thermal gradient, and a 4°C surface temperature.

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