FWGS March 2020 Luncheon
Time & Location
Time: 11:30 am Buffet, Noon Speaker Presentation
RSVP online by Thursday, March 12th at Midnight
Cost: $30 with RSVP, $35 with no RSVP, student members eat free with RSVP (Student Members please directly email the FWGS Secretary to RSVP).
Reminder: FWGS is charged for all RSVP's, so if you RSVP and do not attend you will be contacted concerning payment.
Speaker: Richard Denne and Samantha Patterson
Title: Relationship between East Texas deltas and Eagle Ford production
Abstract: Production studies performed during development of the Eagle Ford unconventional resource have found that the zones containing less than 35% clay that have a high frequency of thin limestones were among the highest producers. Near the San Marcos Arch, two clay-rich, non-productive mudstones have been identified, a lower clay-rich unit between the primary Eagle Ford producing zone and the underlying Buda Limestone, and an upper clay-rich unit at the top of the Lower Eagle Ford. Biostratigraphic analysis of the lower unit in multiple cores identified Early Cenomanian ammonites and nannofossils that were also found in cores taken from the East Texas field within the Maness Shale, a clay-rich mudstone that lies between the Woodbine Sandstone and the Buda Limestone. A study of the Maness in cores from Lavaca and Fayette counties found that it is significantly weaker than the overlying Eagle Ford, averaging 32% to 36% lower calculated unconfined compressive strength (UCS) values than the Eagle Ford. Higher clay and lower calcite abundances within the mudstone are responsible for its lower strength; XRD analyses found that the shale samples from the Maness contained an average of 50% clay. Petrographic analyses found that the clay in the Maness is concentrated within structureless layers that are interpreted to represent fluid-mud deposits associated with hypopycnal plumes. Comparison of Maness thicknesses with cumulative first year oil and water production data found a significant correlation between Maness thickness and oil/water ratios. In particular, there was a 50% decrease in oil/water ratios between Maness thicknesses of 5 to 10 ft, suggesting that the Maness may be acting as a fracture barrier where it is >10 ft thick. The upper clay-rich unit has been dated as Late Cenomanian and tied to the sands within the Kurten field of the Brazos Basin. These sands were derived from the Harris Delta, which was produced by erosion and re-deposition of older Woodbine sands on the southern portion of the Sabine Uplift. Based on their similar depositional patterns, the Maness and Harris are thought to have been sourced from the same area.
Bio: Richard Denne is the Director of the TCU Energy Institute and the founding chairholder of the Hunter Enis Endowed Chair in Petroleum Geology at Texas Christian University. Richard worked as a geologist in the oil and gas industry for over 25 years, working with integrated teams at Exxon and Marathon Oil and as a consultant in the exploration and production of hydrocarbons from deep-water basins across the globe, including the Gulf of Mexico, West Africa, Brazil, Trinidad, and the North Sea. He has also been heavily involved in unconventional shale plays, particularly the Haynesville and Eagle Ford of Texas. He has been at TCU since 2016, where his current research is focused on depositional systems of organic-rich rocks, especially those from the Cretaceous of Texas and the Eagle Ford / Woodbine systems in particular. Richard is a graduate of the University of Iowa (B.S.) and Louisiana State University (Ph.D).