JpGU-AGU Joint Meeting 2020

セッション情報

[E] ポスター発表

セッション記号 M (領域外・複数領域) » M-IS ジョイント

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

コンビーナ:多田 隆治(東京大学大学院理学系研究科地球惑星科学専攻)、Paul A Carling(University of Southampton)、Wickanet Songtham(Nakhon Ratchasima Rajabhat University, Thailand )、Kerry Sieh(Nanyang Technological University)

The impact of a small celestial body in Indochina Peninsula at 0.79 Ma, known as Australasia Tektite event (AATE), has been known for more than half a century due to the wide-spread distribution of tektite. Yet, the source crater of the tektite is not yet found inspite of the probable large size (>30 km in diameter) of crater, its relatively young age, and intensive search by many researchers. However, the situation is changing rapidly during the last several years and the area for the location of the crater is gradually narrowed down. Also, the evidence of environmental perturbation and possible relation with local extinction and migration of hominid and animals has been suggested recently.
In addition, because its timing is close to the Matsuyama/Brunhes paleomagnetic reversal event and in the middle of glacial lowstand during MIS 20, precise age of AATE and its relation with glacio-eustatic sea level changes should have a significant implication to Quaternary chronostratigraphy.
For these reasons, we propose a special interdisciplinary session on the location, mode, magnitude, and exact timing of the AATE impact and its possible effect on the environment and biota
The topic should be of major interest to geologists, sedimentologists, planetary scientists, paleontologists, paleoclimatologists, anthropologists, and so on, especially to those working in SE Asia. Thus adequate topic for JpGU-AGU joint meeting.

*Ryuji Tada1,2,3Toshihiro Tada3Jumpei Yoshioka4 (1.Geo-Cosmology Center, Chiba Institute of Technology、2.Research Center for Earth System Science, Yunnan University、3.Department of Earth and Planetary Science, the Univeristy of Tokyo、4.Atmospheric and Ocean Research Institute, the University of Tokyo)

*常 ユイ1鹿山 雅裕2田近 英一1関根 康人3関根 利守4西戸 裕嗣5小林 敬道6 (1.東京大学 大学院理学系研究科 地球惑星科学専攻、2.東京大学大学院総合文化研究科広域科学専攻広域システム科学系 、3.東京工業大学地球生命研究所、4.Center for High Pressure Science and Technology Advanced Research、5.Research Institute of Natural Science, Okayama University of Science、6.National Institute for Materials Science)

*多田 賢弘1鹿山 雅裕2常 ユイ1三宅 亮3伊神 洋平4多田 隆治1,5,6Carling Paul7Songtham Wickanet8田近 英一1 (1.東京大学大学院理学系研究科地球惑星科学専攻、2.東京大学大学院総合文化研究科広域科学専攻、3.京都大学大学院理学研究科地球惑星科学専攻、4.名古屋大学未来材料・システム研究所高度計測技術実践センター、5.千葉工業大学惑星探査センター、6.雲南大学地球系統科学中心、7.サウサンプトン大学、8.ナコンラチャシマラジャハト大学)

*Kerry Sieh1Jason Herrin1Dayana Schonwalder Angel1Vanpheng Sihavong2Brian Jicha3Brad Singer3Weerachat Wiwegwin4James Daniel Paul Moore1Paramesh Banerjee1Tawachai Chualaowanich4Punya Charusiri5 (1.Earth Observatory of Singapore, Nanyang Technological University, 639798 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, WI 53706、4.Department of Mineral Resources, Ministry of Natural Resources and Environment, Ratchatewi, 10400 Bangkok, Thailand、5.Department of Geology, Chulalongkorn University, Khet Pathumwan, 10330 Bangkok, Thailand)