65 D30. Recent Advances in Sediments, Carbonates (Posters)
Sunday, 9 October 2022
2:00 PM - 6:00 PM
Exhibit Hall F
POSSIBLE MASS TRANSPORT DEPOSITS AND FLUID ESCAPE PIPES IN EOCENE LIMESTONES OF THE DUNGUL FORMATION, SOUTHEAST WESTERN DESERT, EGYPT
Paper number: 65-2
Program: Technical Sessions
Time: 2:00 PM – 6:00 PM
Authors
-
Erin PimentelCalifornia Institute of Technology, Pasadena, CA
-
William BresnahanHamilton College, Clinton, NY
Abstract
The bands consist of lighter-colored stripes a few meters to 10s of meters wide separated by topographically lower, darker-colored stripes 1-5 m wide. Sets of bands display parallel, sinuous, lobate, plumose, and arcuate patterns. Patterns extend beneath the next younger limestone layer, and immediately overlying and underlying layers are unpatterned, indicating that the patterning is part of the limestone layer in the stratigraphic sequence. Individual bedding plane exposures of the patterning range up to ~4.5 km2 in area, with pattern-parallel lengths ranging up to ~2.5 km. Pits occur on bedding surfaces as small, quasi-circular, low-relief depressions that commonly display a concentric pattern of more and less resistant layers. Some pits show clear inward dips in bedding. Prominent regional WNW-ESE joints cut the limestone inside the pits, indicating that pits are not young sinkholes. Most pits are randomly distributed, although some occur as aligned sets.
The layer-confined patterning is strikingly similar to patterns typical of marine mass transport deposits, and we propose that these patterns resulted from mobilization on a shallowly sloping carbonate shelf, although the triggering mechanism is unclear. The southeast Western Desert is cut by a major set of E-W faults that have been repeatedly active since the late Mesozoic, so seismicity may have played a role. Because the pits resemble fluid escape pipes, episodic fluid escape may have been a trigger. The patterned layer is also co-located with several large, low amplitude domes in bedding across an area of ~4000 km2, and diapirism in underlying shales may have been a factor.
Geological Society of America Abstracts with Programs. Vol. 54, No. 6
doi: 10.1130/abs/2022AM-379763
© Copyright 2022 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.