T169 Mass Extinctions: Volcanism, Impacts, and Catastrophic Environmental Change I
Monday, 20 October 2014
1:00 PM - 5:00 PM
223/224
ABRUPT SURFACE WATER REDUCTION DURING THE END-PERMIAN MASS EXTINCTION AND COMBUSTION OF OIL BY THE END-CRETACEOUS ASTEROID IMPACT
Paper number: T169-7
Program: Technical Sessions
Time: 2:20 PM – 2:35 PM
Authors
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Takashi MiyajiTohoku University, Sendai, N/A
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Kosuke ItoTohoku University, Sendai, N/A
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Takuya MizukamiTohoku University, Sendai, N/A
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Ryosuke SaitoTohoku University, Sendai, N/A
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Masahiro ObaTohoku University, Sendai
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Li TianChina University of Geosciences (Wuhan), Wuhan, N/A
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Jinnan TongChina University of Geosciences at Wuhan, Wuhan, N/A
Abstract
We also show that the asteroid impact at the end-Cretaceous resulted in the ejection of combusted and non-combusted fossil organic matter such as oil, most of which fell into the ocean and was transported by the impact-induced tsunami. The remaining combusted and non-combusted fossil organic matter remained in the stratosphere, along with atomic elements sourced from the asteroid, for a period of a year, during which devastation of land vegetation occurred. Combusted organic molecules (coronene) are now condensed in the tsunami deposits and the superjacent layer containing condensed iron and iridium sourced from the asteroid at Beloc, Haiti. The percentage of coronene in total combusted organic molecules is exceptionally high in the tsunami deposits and iridium layer, suggesting that the combusted organic molecules remained in the stratosphere for a year. Low carbon preference index (CPI) values of n-alkanes in the tsunami deposits and iridium layer relative to other strata, suggesting that the n-alkanes in the tsunami deposits and the iridium layer were sourced mainly from oil. Combusted oil molecules such as coronene suspended in the stratosphere may have contributed to the darkness.