Newly discovered mud volcanoes in the Coastal Belt of Makran, Pakistan—tectonic implications

• Published in: Arabian journal of geosciences Vol. 7; no. 11; pp. 4899 - 4909
• Main Authors: Kassi, Akhtar M., Khan, Shuhab D., Bayraktar, Huseyin, Kasi, Aimal K.
• Format: Journal Article
• Language: English
• Published: Berlin/Heidelberg Springer Berlin Heidelberg 01-11-2014
• Subjects: Earth and Environmental Science; Earth Sciences; Original Paper; ISW, Pakistan, Balochistan, Makran; Cluster; Mud volcano; Makran; Accretionary wedge
• ISSN: 1866-7511; 1866-7538
• DOI: 10.1007/s12517-013-1135-7

The Makran accretionary wedge has a much larger number of mud volcanoes then those reported earlier. Using high-resolution satellite images, over 70 active mud volcanoes were identified. These mud volcanoes occur within a well-defined zone; we call it the Makran zone of active mud volcanoes (MZAMV), which is parallel to the regional trend of the accretionary wedge. Mud volcanoes within the zone occur as clusters, which form linear belts parallel to the regional thrusts associated with anticlines. The MZAMV zone also includes the offshore mud volcanoes occurring in the shallow shelf area, including the recurrently emerging mud islands. Several occurrences of thick deposits of old mud volcanoes (Pleistocene or even older) are also present within this zone, which also display recognizable features that are characteristic of the fossil mud volcanoes. We propose that the MZAMV developed and evolved in response to the continued compression within the Makran accretionary wedge, which in turn, is a response of the subduction process. Mud diapirism has been an ongoing phenomena since Pleistocene or even earlier. The events of enhanced mud extrusion in mud volcanoes and/or emergence of island(s) have relevance with seismic phenomena and, therefore, may be closely monitored.