GSA Connects 2024 Meeting in Anaheim, California

Paper No. 95-15
Presentation Time: 11:40 AM

RESOLVING CRUSTAL STRUCTURE IN THE SUPERDEEP BENGAL BASIN


SADLER, Benjamin1, PERSAUD, Patricia2, PULLIAM, Jay3, KUMAR, Sachin1, SANDVOL, Eric4, GAHERTY, James5, STECKLER, Michael S.6 and AKHTER, Syed Humayun7, (1)Baylor University, Waco, TX 76706, (2)Geosciences, University of Arizona, Tucson, AZ 85721, (3)Geosciences, Baylor University, One Bear Place #97354, Waco, TX 76798, (4)Department of Geological Sciences, University of Missouri, 101 Geology Building, Columbia, MO 65211, (5)Northern Arizona University, Flagstaff, AZ 86001, (6)Marine Geology and Geophysics, Columbia University, 61 Route 9W, Palisades, NY 10964, (7)Bangladesh Open University, Board Bazar, Gazipur, 1705, Bangladesh

The Bengal basin, with sediment thicknesses of up to 21 km, overlies the subduction of the India plate under the Burma microplate. The basin was formed by rifting in the Cretaceous and is now bounded by the Indian shield to the west, the Shillong plateau to the north, the Indo-Burma ranges to the east, and the Bay of Bengal to the south. The India-Asia collision, initiated during the Paleocene, resulted in the rise of the Himalayan Mountains. The Ganges and Brahmaputra Rivers have carried enormous volumes of sediment from the Himalayas, filling the basin from the Paleocene to the present.

Here we model crustal structure by waveform matching P receiver functions and teleseismic P autocorrelograms for 33 seismic stations across the Bengal basin. Our P receiver functions use teleseismic Ps conversions generated at local impedance contrasts (including the Moho, the sediment-basement interface, and several intrasedimentary contacts). Teleseismic P autocorrelograms recover P reverberations generated at these same impedance contrasts. Jointly, they constrain crustal structure that is parameterized in terms of interface depth, compressional wave velocity (VP), and the ratio of compressional to shear wave velocity (VP/VS).

Based on observable phases and solution stability, our models are comprised of either three sedimentary units overlying the crystalline crust, for 21 stations, or two sedimentary units overlying crystalline crust, for 12 stations (i.e., the two deeper sedimentary units from the 4-layer models are combined). The uppermost sedimentary unit is ~3 km thick with an average VP of 3.3 km/s. The second sedimentary unit averages ~8 km thick with an average VP of 5.9 km/s. In the deepest portion of the basin, we model a low velocity zone with an average VP of 4.4 km/s for the four-layer stations. We interpret this low velocity zone as an indication of fluids trapped in the deep basin. Potential origins of fluids include a) rapid sedimentation that led to incomplete dewatering of buried sediments, b) fluid release from diagenetic alteration of clay minerals at the pressures and temperatures present in the deep basin, or c) some combination of these factors. Below the sedimentary layers we observe a 14-25 km thick layer with an average VP of 6.9 km/s, which we interpret to be extended continental crust that was likely altered during the Cretaceous by intrusions from the Kerguelen plume.