日本地球惑星科学連合2014年大会

講演情報

インターナショナルセッション(口頭発表)

セッション記号 P (宇宙惑星科学) » P-EM 太陽地球系科学・宇宙電磁気学・宇宙環境

[P-EM08_1PM2] Space Weather and Space Climate

2014年5月1日(木) 16:15 〜 18:00 411 (4F)

コンビーナ:*片岡 龍峰(国立極地研究所)、海老原 祐輔(京都大学生存圏研究所)、草野 完也(名古屋大学太陽地球環境研究所)、清水 敏文(宇宙航空研究開発機構宇宙科学研究所)、三好 由純(名古屋大学太陽地球環境研究所)、浅井 歩(京都大学宇宙総合学研究ユニット)、佐藤 達彦(日本原子力研究開発機構)、陣 英克(情報通信研究機構)、伊藤 公紀(横浜国立大学大学院工学研究院)、宮原 ひろ子(武蔵野美術大学造形学部)、座長:片岡 龍峰(国立極地研究所)、佐藤 達彦(日本原子力研究開発機構)

17:45 〜 18:00

[PEM08-07] 星雲遭遇による白亜紀末の大量絶滅

*二村 徳宏1戎崎 俊一2丸山 茂徳3 (1.岡山天文博物館、2.理化学研究所、3.東京工業大学 地球生命研究所)

キーワード:星雲の冬, 暗黒星雲, 大量絶滅, 白亜紀末, K-Pg境界, 国際深海掘削計画

We found that a significant positive broad component of iridium in a pelagic deep sea sediment core (886C) around an iridium peak by asteroid impact corresponds at the K-Pg boundary. The 886C is core sample was taken by the Ocean Drilling Program (ODP) in the central portion of the North Pacific. This site has been in Pelagic from the End-Cretaceous periods. The accumulation rate is 0.5 m Myr-1. Kyte et al., (1995) measured iridium density in the 886C core of 0.75-72.2 m which corresponds of 〜80 Ma from the present. In this data, there is one sharp peak around 65.5 m correspond at K-Pg boundary. In addition, we found that there are broad components across 〜20 m above the back ground which have some sharp peak component. The Ir value of the broad component which is about dozen times of back ground. This broad component is difficult to be explained by the materials on the surface of the Earth, and requires the contribution from the iridium-rich extraterrestrial materials, such as CI chondrite. And it is difficult to explain the broad component by diffusion and bioturbation of an iridium peak by asteroid impact. Platinum-group-element such as Pt, Re and Ir are redistributed by changes in sedimentary redox condition. However such change can probably account for many of small < 10 cm (Colodner et al., 1992) and the mean global depth of marine bioturbation was calculated to be 9.8±4.5 cm (Boudreau, 1994). And also an evidence of bioturbation was not found from lithofacies (Proc. ODP, Init. Repts., 145).We consider that the broad component can be caused by an encounter of the solar system with a dark cloud with a size of 〜100 pc and the central density of over 2000 protons/cc in the galactic disk and estimated that the flux of exosolar material began 〜73 Ma and has run through 〜8 Myr. By the Kataoka's "Nebula Winter model" (Kataoka 2013), dark cloud can lead to an environmental catastrophe to the Earth from a few kiloannum to megaannum. The dark cloud encounter enhances a flux of cosmic dust particles and cosmic rays which lead to global cooling and destruction of the ozone layer.The solid particles from the dark cloud accrete on the Earth and in the stratosphere, stay for a several months; their sunshield effect is as large as -9.3 W m-2. The climate cooling in the End-Cretaceous period is also suggested by the variations of stable isotope rations in oxygen and strontium (Brian and Huber, 1990; Barrera and Savin, 1999; Li and Keller, 1998). Any photosynthetic plants had heavy damaged, and loss of biodiversity began to the top of food chain.The mass extinction at K-Pg boundary, which is widely thought to be caused by an impact of an asteroid (e. g., Schulte et al., 2010). However, a complete extinction of level of family by asteroid impact seems rather difficult. First, a severe environment turn-over would finish few years after impact, the solid particles and sulphate launched by the asteroid impact was settled down for only few month (troposphere) to few years (stratosphere) and negative radiative forcing became negligible after a few years from the impact (Pierazzo, 2001).The number of individuals would recover completely after the environmental catastrophe was over, if a few percent of individuals of one species survived.Second, in spite of there were similar impacts without catastrophic on the Earth, for example, Alamo, Woodleigh, and Popigai crater, there are no evidences of association for extinction. However, because the encounter with the dark cloud perturbs the orbit of asteroid or comet by its gravitational potential and may lead an asteroid or comet shower, the asteroid impact at K-Pg may be one of the consequences of the dark cloud. For a certainly, only an asteroid impact cannot involve mass extinction, however may be role cruncher. The multiple impact and volcanism in a short period of time (Keller, 2005) may have been caused by encounter the dark nebula and atte