T146 Presentaciones de Geociencias en Español II: Una Nueva Experiencia en una Reunión de la Sociedad Geológica Americana (GSA)//Spanish Presentations about Geosciences in the America II: A new GSA Experience
Monday, 23 September 2024
1:30 PM - 5:30 PM
304C
DIAGENETIC STUDIES IN THE SABINAS BASIN: IMPLICATIONS FOR SOURCE ROCK MATURATION
Paper number: T146-6
Program: Technical Sessions
Time: 2:55 PM – 3:10 PM
Authors
-
Eduardo González-PartidaUniversidad Nacional Autónoma de México, Juriquilla, QA
-
Alejandro Carrillo-ChávezUniversidad Nacional Autónoma de México, Juriquilla, QA
-
Juan Josue EncisoUniversidad Autónoma de Coahuila, Nueva Rosita, CU
Abstract
Three distinct thermal episodes related to diagenetic cement formation were identified. Among these, only one-episode correlates directly with gas production, characterized by temperatures ranging between 99°C and 168°C. Isotopic analyses of the cements and calcite segregations revealed that the genesis of these minerals is closely tied to CO2 production derived from organic matter decomposition. This indicates that their formation occurred during the interaction of hot fluids, organic acids, and meteoric waters.
As the geological succession experienced increased compaction and deepening, these fluids migrated through zones of dissolution, recrystallization, and fractures. The migration predominantly followed a lateral trajectory until reaching major fault systems. This migration pattern underscores how the hottest fluids are expelled near the basin boundaries. Furthermore, the presence of light and intermediate hydrocarbons in permeable zones suggests that the Eagle Ford and Indidura Formations function as reservoir rocks. This is facilitated by a fracture system that enabled extensive fluid circulation.
To better understand these processes, a thermal convection model for the Sabinas Basin was developed using microthermometric data from fluid inclusions. This model delineates the zones of wet gas and dry gas production within the stratigraphic framework. The insights gained from this model highlight the critical role of thermal convection in hydrocarbon generation and migration.
Overall, this study provides a detailed understanding of the diagenetic processes, fluid interactions, and thermal history within Cenomanian-Turonian source rocks. These findings are essential for improving hydrocarbon exploration strategies and enhancing our knowledge of subsurface fluid dynamics.
Geological Society of America Abstracts with Programs. Vol. 56, No. 5
doi: 10.1130/abs/2024AM-405636
© Copyright 2024 The Geological Society of America (GSA), all rights reserved. Permission is hereby granted to the author(s) of this abstract to reproduce and distribute it freely, for noncommercial purposes. Permission is hereby granted to any individual scientist to download a single copy of this electronic file and reproduce up to 20 paper copies for noncommercial purposes advancing science and education, including classroom use, providing all reproductions include the complete content shown here, including the author information. All other forms of reproduction and/or transmittal are prohibited without written permission from GSA Copyright Permissions.