日本地球惑星科学連合2018年大会

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[JJ] 口頭発表

セッション記号 S (固体地球科学) » S-GC 固体地球化学

[S-GC46] 固体地球化学・惑星化学

2018年5月22日(火) 10:45 〜 12:15 202 (幕張メッセ国際会議場 2F)

コンビーナ:下田 玄(産業技術総合研究所地質調査総合センター)、鈴木 勝彦(国立研究開発法人海洋研究開発機構・海底資源研究開発センター)、山下 勝行(岡山大学大学院自然科学研究科、共同)、石川 晃(東京大学大学院総合文化研究科)、座長:若木 重行(国立研究開発法人海洋研究開発機構)、石川 晃(東京工業大学)、下田 玄(産業操業技術研究所)

11:30 〜 11:45

[SGC46-04] Platinum group elements and Re-Os isotopes in the K-Pg transition of the Chicxulub peak-ring rocks

*佐藤 峰南1石川 晃2Ferrière Ludovic3Morgan Joanna4Gulick Sean5IODP-ICDP Expedition 364 Scientists (1.千葉工業大学、2.東京大学、3.Natural History Museum Vienna、4.Imperial College London、5.University of Texas at Austin)

キーワード:Platinum group elements、Re-Os isotopes、Cretaceous-Paleogene boundary、Chicxulub crater

The presence of extraterrestrial material in terrestrial sediments is usually indicated by an enrichment of platinum group elements (PGEs: Os, Ir, Ru, Pt, Pd) due the PGE concentrations in chondrite are about three orders higher than those of the upper continental crust. The K-Pg boundary clay layer exhibiting PGE anomalies, containing Ni-rich spinels and spherules, has been found in sites worldwide and interpreted as the ejecta layer produced by large impact that formed the Chicxulub crater and marks the end of the Cretaceous. However, the spatial distribution and amount of projectile materials within the crater is still poorly constrained. In order to determine the distribution and abundance of the projectile component within the impact site, we examined PGE concentrations and Re–Os isotope (187Os/188Os) compositions in the Cretaceous–Paleogene transitional layer of the Chicxulub peak ring rocks obtained from IODP–ICDP expedition 364 cores.

Platinum group element (PGE) concentrations and 187Os/188Os compositions show systematic variations across the transitional layer. The upper part (616.59–616.63 mbsf) is characterized by about one order of magnitude higher Os, Ir, and Ru contents compared to the average continental crust abundances, but much lower than for the typical Ir-enriched Cretaceous–Paleogene boundary distal sites (e.g., Gubbio and Caravaca: Alvarez et al., 1980; Smit and Hertogen, 1980). Relatively flat CI chondrite–normalized PGE patterns are observed in the upper part of the layer. Meanwhile, the PGE concentrations in the lower part of the transitional layer (617.315–617.34 mbsf) are almost equivalent to those of upper continental crust showing pronounced step CI chondrite-normalized PGE patterns (0.8–1.2 × 10-4 for Ir, and 1.2–2.7 × 10-3 for Pt and Pd). 187Os/188Os and Re/Os ratios in the transitional layer gradually decrease from 0.33 to 0.25 and 35.45 to 1.14, respectively, from bottom to top. These results suggest that the projectile component, with chondritic composition, is enriched in the uppermost part of the transitional layer just below carbonate rocks that are early Paleogene in age, but could be distributed over a thicker interval than for the Ir-enriched sites. Further detailed studies of PGE and 187Os/188Os compositions through the stratigraphic sequence will reveal the distribution and dilution effect of the projectile component.