Preprints
https://doi.org/10.5194/egusphere-2022-987
https://doi.org/10.5194/egusphere-2022-987
 
10 Oct 2022
10 Oct 2022

Impact of permeability evolution in igneous sills on hydrothermal flow and hydrocarbon transport in volcanic sedimentary basins

Ole Rabbel1, Christophe Y. Galerne2, Jörg Hasenclever3, Olivier Galland1, Karen Mair1, and Octavio Palma4 Ole Rabbel et al.
  • 1NJORD, University of Oslo, P.O. 1048 Blindern, 0316 Oslo, Norway
  • 2Faculty of Geosciences, University of Bremen, Klagenfurter Straße 2–4, 28359 Bremen, Germany
  • 3Institute of Geophysics, Center for Earth System Research and Sustainability, University of Hamburg Bundesstrasse 55, 20146 Hamburg, Germany
  • 4Facultad de Ciencias Naturales y Museo, Universidad de La Plata, Paseo del Bosque s/no – B1900FWA – La Plata, Argentina

Abstract. Sill intrusions emplaced in organic-rich sedimentary rocks trigger the generation and migration of hydrocarbons in volcanic sedimentary basins. Based on seismic and geological observations, numerical modeling studies of hydrothermal flow around sills have shown that thermogenic methane is channeled towards the intrusion tip, where it rises to the surface in a hydrothermal vent. However, these models typically assume impermeable sills and ignore potential effects of permeability evolution in cooling sills, e.g., due to fracturing. To address this issue, we combine a geological field study of a volcanic basin (Neuquén Basin, Argentina) with hybrid FEM/FVM numerical modeling of hydrothermal flow around a sill, including hydrocarbon generation and transport. Our field observations show that graphitized bitumen veins and cooling joints filled with solid bitumen or fluidized shale are common within the studied sills. Raman spectroscopy indicates graphitization at temperatures between 350–500 °C, evidencing fluid flow within the intrusions shortly after solidification. This finding motivates our modeling study, which investigates flow patterns around intrusions that become porous and permeable upon solidification. The results show three distinct flow phases affecting the transport of hydrocarbons generated in the contact aureole: (1) Contact-parallel flow toward the sill tip before solidification, (2) upon complete solidification, sudden vertical “flushing” of overpressured hydrocarbon-rich fluids from the lower contact aureole through the hot sill, and (3) slow rise of hydrocarbon-rich fluids above the sill center, and backward-downward flow near the sill tip. We conclude that permeability creation within cooling sills may be an important factor for hydrothermal flow and hydrocarbon transport in volcanic basins, as it considerably alters the fluid pressure configuration and flow patterns by dissipating overpressure below the sills. This could, for instance, lead to a reduced potential for hydrothermal venting.

Ole Rabbel et al.

Status: final response (author comments only)

Comment types: AC – author | RC – referee | CC – community | EC – editor | CEC – chief editor | : Report abuse
  • RC1: 'Comment on egusphere-2022-987', Anonymous Referee #1, 04 Nov 2022
  • RC2: 'Comment on egusphere-2022-987', Anonymous Referee #2, 16 Nov 2022

Ole Rabbel et al.

Ole Rabbel et al.

Viewed

Total article views: 257 (including HTML, PDF, and XML)
HTML PDF XML Total BibTeX EndNote
181 65 11 257 3 2
  • HTML: 181
  • PDF: 65
  • XML: 11
  • Total: 257
  • BibTeX: 3
  • EndNote: 2
Views and downloads (calculated since 10 Oct 2022)
Cumulative views and downloads (calculated since 10 Oct 2022)

Viewed (geographical distribution)

Total article views: 253 (including HTML, PDF, and XML) Thereof 253 with geography defined and 0 with unknown origin.
Country # Views %
  • 1
1
 
 
 
 
Latest update: 06 Dec 2022
Download
Short summary
This work investigates the interaction between magma in the subsurface and the rocks and fluids that surrounds it. Specifically, the study investigates how fluids containing hydrocarbons such as methane are moving in the rocks surrounding the magma. This is important due to the possibility that methane is released to the atmosphere if the fluids reach the surface. The study shows that the generation of fluid pathways in the magma have a significant impact on the flow paths of the fluids.