| タイトル | Mineralogical Variation of Chelyabinsk with Depth from the Surface of the Parent Meteoroid |
| 本文（外部サイト） | http://hdl.handle.net/2060/20140006556 |
| 著者（英） | Haba, M. K.; Mikouchi, T.; Yoshida, S.; Nagao, K.; Hasegawa, H.; Zolensky, M. E.; Komatsu, M. |
| 発行日 | 2014-03-17 |
| 言語 | eng |
| 内容記述 | The Chelyabinsk meteorite, which passed over the Chelyabinsk Oblast, Russia on Feb. 15th, 2013, brought serious damage by the shock wave and airburst. The diameter of the parent meteoroid is estimated to be approximately 20 m in diameter [1]. It was reported that the impact by this meteorite shower was 4,000 times as large as the TNT explosive and this was the largest airburst on Earth since the asteroid impact in Tunguska, Russia in 1908. The mineralogy and geochemical study of the recovered samples shows that Chelyabinsk is an LL5 chondrite [1]. In this study we analyzed several fragments of Chelyabinsk whose noble gas compositions have been measured and depths from the surface of the parent meteoroid were estimated [2]. We examined how mineralogical characteristics change with depth from the surface. This kind of study has never been performed and thus may be able to offer significant information about the evolution of meteorite parent bodies. |
| NASA分類 | Lunar and Planetary Science and Exploration |
| レポートNO | JSC-CN-30302 |
| 権利 | Copyright, Distribution as joint owner in the copyright |
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