Japan Geoscience Union Meeting 2023

Presentation information

[J] Online Poster

S (Solid Earth Sciences ) » S-GL Geology

[S-GL22] Frontier research on chronostratigraphic unit boundaries

Fri. May 26, 2023 1:45 PM - 3:15 PM Online Poster Zoom Room (4) (Online Poster)

convener:Hiroyuki Hoshi(Department of Earth Sciences, Aichi University of Education), Reishi Takashima(Tohoku University Museum, Tohoku University), Junichiro Kuroda(Department of Ocean Floor Geoscience, Atmosphere and Ocean Research Institute, the University of Tokyo), Makoto Okada(Department of Earth Sciences, College of Science, Ibaraki University)

On-site poster schedule(2023/5/26 17:15-18:45)

1:45 PM - 3:15 PM

[SGL22-P09] Magnetostratigraphy of the Nemuro Group in the Shiranuka Hill area in eastern Hokkaido

*Hiroyuki Hoshi1, Yota Kitano1, Ichiha Mita1, Reishi Takashima2, Keiichi Hayashi3 (1.Aichi University of Education, 2.Tohoku University, 3.Hokkaido Research Organization)

Keywords:K–Pg boundary, Shiranuka Hill, Nemuro Group, Magnetostratigraphy


Previous and ongoing studies have suggested that a Cretaceous–Paleogene (K–Pg) boundary is present in a muddy sequence of the Nemuro Group in the Shiranuka Hill area in eastern Hokkaido. An interdisciplinary approach, including detailed mapping, radiometric dating, geochemical analyses, and biostratigraphic and magnetostratigraphic investigations, is needed to locate a K–Pg horizon in the group. For this purpose, we are currently investigating the magnetic polarity stratigraphy of the Kawaruppu and Tomikawa Formations of the group. Mudstones and fine tuffs were sampled along two sections for magnetic measurements; one section is along the Kawaruppu River, where a sedimentary sequence of the two formations is well exposed, and the other section is along a tributary of the Kawaruppu River, where a probable K–Pg horizon exists in the Kawaruppu Formation. Demagnetization experiments yielded preliminary results showing a reverse–normal–reverse polarity sequence in the Kawaruppu River section and a reverse polarity sequence in the tributary section. The probable K–Pg horizon is within a reverse polarity sequence, which is compatible with the fact that the K–Pg boundary is located within reverse polarity chron C29r. The normal polarity portion is in the Tomikawa Formation and is probably correlated to a normal polarity chronozone in the Danian stage.