JpGU-AGU Joint Meeting 2020

Presentation information

[E] Oral

M (Multidisciplinary and Interdisciplinary) » M-IS Intersection

[M-IS04] An asteroid impact in SE Asia at 0.8 Ma and its effect on the environment and biota

convener:Ryuji Tada(Department of Earth and Planetary Science, Graduate School of Science, The Univeristy of Tokyo), Paul A Carling(University of Southampton), Wickanet Songtham(Nakhon Ratchasima Rajabhat University, Thailand ), Kerry Sieh(Nanyang Technological University)

[MIS04-01] Converging lines of evidence for burial of the Australasian impact crater within the Bolaven volcanic field, Southern Laos

★Invited Papers

Kerry Sieh1, *Jason S Herrin1, Dayana Angel Schonwalder1, Vanpheng Sihavong2, Brian Jicha3, Brad Singer3, Weerachat Wewegwin4, Paramesh Banerjee1, Tawachai Chualaowanich4, Punya Charusiri5 (1.Earth Observatory of Singapore, Nanyang Technological University, Singapore, 2.Department of Geology and Mines, Ministry of Energy and Mines, Vientiane, Lao People’s Democratic Republic, 3.Department of Geoscience, University of Wisconsin–Madison, Madison, Wisconsin, USA, 4.Department of Mineral Resources, Ministry of Natural Resources and Environment, Ratchatewi, Bangkok, Thailand, 5.Department of Geology, Chulalongkorn University, Khet Pathumwan, Bangkok, Thailand)

Keywords:Australasian, tektite, Bolaven, impact, Laos

Physical and chemical characteristics of the Australasian tektites suggest that they originated within the Thai-Lao Khorat Plateau, and more specifically within the 100,000 km2 inner strewnfield of Muong Nong-type tektites. The lack of an obvious crater and very low rates of erosion in this region imply that the crater must lay buried. Several converging lines of evidence imply that indeed the 0.8-Ma impact crater is buried beneath the 350-m thick summit flows of the 5,000-km2 Bolaven volcanic field in southern Laos. Chemical compositions of the tektites indicate the presence of a weathered basaltic component that had accumulated mostly during the few million years before the impact. Accordingly, 40Ar-39Ar dates from distal lava flows can be traced uphill to weathered pre-impact basalts now buried beneath younger flows of the summit impact region. Also as predicted by the hypothesis, all 40Ar-39Ar dates from exposed flows at and near the impact region post-date the impact. Moreover, a gravity anomaly there may reflect the presence of a buried ~15 km wide elliptical crater with low-density fill. We interpret a thick deposit of crudely layered, bouldery sandstone and mudstone breccia in two outcrops 10–20 km from the center of the impact crater to be part of the proximal ejecta blanket. Fractured quartz grains within these boulder clasts lend support to this interpretation of an impact origin of these peculiar deposits. A pebbly, cobbly layer that extends and thins for more than 100 km from the impact site, almost everywhere containing angular muong nong tektites, comprises the more distal part of the ejecta blanket. Commonly, atop this layer is a massive, meters-thick coarse-silty to fine-sandy layer that we interpret to be partially or largely comprised of fallout of fine debris driven and convected into the atmosphere during and immediately following the impact. In this talk, we will present available physical and geochronologic evidence for the Bolaven impact as the source for the Australasian tektite strewnfield. In an accompanying contribution, we will present correlative geochemical evidence.