Japan Geoscience Union Meeting 2025

Presentation information

[J] Oral

B (Biogeosciences ) » B-CG Complex & General

[B-CG06] Decoding the history of Earth: From Hadean to the present

Wed. May 28, 2025 3:30 PM - 5:00 PM 301A (International Conference Hall, Makuhari Messe)

convener:Tsuyoshi Komiya(Department of Earth Science & Astronomy Graduate School of Arts and Sciences The University of Tokyo), Fumito Shiraishi(Earth and Planetary Systems Science Program, Graduate School of Advanced Science and Engineering, Hiroshima University), Yusuke Sawaki(The University of Tokyo), Teruhiko Kashiwabara(Japan Agency for Marine-Earth Science and Technology), Chairperson:Satoshi Yoshida(Center for Northeast Asian Studies, Tohoku University), Tsuyoshi Komiya(Department of Earth Science & Astronomy Graduate School of Arts and Sciences The University of Tokyo)

4:30 PM - 4:45 PM

[BCG06-23] Drivers of the K-Pg mass extinction: impact and volcanism interaction

*Kunio Kaiho1, Jeroen E. Sonke2, Akane Yamakawa3, David Jones4, Satoshi Takahashi5, Masanobu Yamamoto6, Naga Oshima7, Laure Laffont2, Stephen E. Grasbyi8 (1.Tohoku University, 2.Université Paul Sabatier Toulouse 3, 3.National Institute for Environmental Studies, 4.Amherst College, 5.Nagoya University, 6.Hokkaido University, 7.Meteorological Research Institute, 8.University of Calgary)

Keywords:Cretaceous-Paleogene boundary mass extinction, Climate change, mercury isotopes, meteorite impact, volcanism, organic molecule indicators

This study provides novel insights into the mechanisms driving the Cretaceous-Paleogene (K-Pg) mass extinction. Key findings include: (i) Spikes in iridium (Ir) and mercury (Hg) within K-Pg layers, with elevated Hg/Ir ratios compared to chondritic values at both proximal (near the impact site) and distal locations, suggest a simultaneous bolide impact and Deccan Trap volcanism. (ii) Strong correlations between δ202Hg, the coronene index, and Δ199Hg in proximal samples introduce a new method for distinguishing volcanic emissions from impact-related sources. (iii) Similarities in volcanic δ202Hg and Δ199Hg in high-Hg pre- and post-impact sediments, alongside medium to high coronene levels, indicate that Hg originated primarily from Deccan Traps eruptions rather than background volcanic activity. (iv) Near-zero Δ199Hg values at the top of impact turbidites at the proximal site suggest local darkness caused by the ejecta cloud. (v) The largest volcanic plume eruptions, likely from the Deccan Traps, occurred approximately one year after the Chicxulub impact. (vi) These dual events coincided with terrestrial plant devastation, severe soil erosion, and the extinction of surface-dwelling planktonic foraminifera. (vii) Climate models incorporating target rock soot followed by volcanic SO2 emissions predict prolonged sunlight reduction and global cooling. (viii) TEX86H data indicate post-impact warming, correlating with the extinction of deep-sea planktonic foraminifera. These findings suggest that the Chicxulub asteroid impact, combined with Deccan Trap SO2 emissions, triggered an initial phase of cooling and environmental collapse, leading to the extinction of surface-dwelling planktonic foraminifera, followed by deep-sea foraminiferal extinction due to subsequent global warming.