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The AAPG/Datapages Combined Publications Database

Houston Geological Society Bulletin

Abstract


Houston Geological Society Bulletin, Volume 52, No. 7, March 29, 2010. Pages 24 and 27.

Abstract: Hydrocarbons Associated with Previous HitIgneousNext Hit Rocks (North America and Worldwide)

Steve Schutter

Explorationists generally disregard Previous HitigneousNext Hit rocks and their immediate surroundings, condemning the surrounding sediments as overmature and the Previous HitigneousNext Hit rocks themselves as nonporous crystalline masses. However, these are misconceptions, and there is opportunity in moving beyond them. The maturation effect of the Previous HitigneousNext Hit activity is often overrated. Most shallow Previous HitigneousNext Hit intrusions are volumetrically too small to affect a large volume of rock and even flood basalts cool too quickly to have a marked effect.Most thermal effects are due to regional heating or hydrothermal circulation.

Porosity in Previous HitigneousNext Hit rocks may be due to fracturing, particularly fracturing developed during cooling. Some extrusive rocks are also vesicular or may have a clastic texture. However, retrograde metamorphism can also provide significant porosity by creating what is essentially a vuggy texture. Combinations of these can produce effective reservoir rock.

Previous HitIgneousNext Hit rocks can also provide their own traps. Variations in porosity can produce a pseudo-stratigraphic trap. However, thick intrusive bodies (such as laccoliths and plugs) and volcanic cones can also provide trapping structures. Dikes can block migration pathways. Syndepositional sedimentary and Previous HitigneousNext Hit facies may also provide traps, as well as post-emplacement draping over non-compacting Previous HitigneousNext Hit bodies.

While generally not considered to be source rocks, extrusive Previous HitigneousNext Hit terrains are often lake-prone, and thus may provide source rocks for subsequent Previous HitigneousNext Hit rocks. Migration in Previous HitigneousNext Hit areas is predominantly normal. But, CO2-dominated systems and those subject to supercritical steam may both be present and they may have distinctive favorable peculiarities. Since they are nonpolar fluids, they are considerably more effective than water-dominated systems at mobilizing hydrocarbons, and the conventional “rules of thumb” for organic matter type, richness, and maturity may not apply.

Exploration methods need to be as variable as the Previous HitigneousNext Hit Previous HitreservoirsNext Hit. Some Previous HitigneousNext Hit rocks contain abundant iron, and have a strong magnetic signature. Others do not. Some Previous HitigneousNext Hit rocks are much denser than the surrounding rock; others are not. Notably, one of the earliest plays in Texas, the “serpentine” trend, was instrumental in developing many of the early geophysical techniques. Likewise, log results may be so variable as to be ambiguous. Some characteristics may be recognizable, but the nature of the Previous HitigneousNext Hit rocks and their relationships must be considered.

Due to the lack of “rules” and systematic study, currently the best approach to exploration in and around Previous HitigneousNext Hit rocks is to look for analogs. The search for analogs cannot be limited to one area or continent, but a global view is needed. Analogs from around the world have applicability to possible plays in North America. Thus, an extensive reference list of possible analogs should be considered.

More broadly, the presence of hydrocarbons in or around Previous HitigneousNext Hit rocks in a basin may indicate the presence of an effective hydrocarbon system in that basin. There are still basins in the world where leaking hydrocarbons may indicate the potential of the basin. Also, large areas of productive sedimentary basins are covered by volcanics, both flood basalts and ash-flow tuffs. Exploration models can complement and enhance geophysical methods in such areas.

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