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Jadeite in Chelyabinsk meteorite and the nature of an impact event on its parent body.
Ozawa, Shin; Miyahara, Masaaki; Ohtani, Eiji; Koroleva, Olga N; Ito, Yoshinori; Litasov, Konstantin D; Pokhilenko, Nikolay P.
Afiliación
  • Ozawa S; Department of Earth Science, Graduate School of Science, Tohoku University, Sendai 980-8578, Japan.
  • Miyahara M; 1] Department of Earth Science, Graduate School of Science, Tohoku University, Sendai 980-8578, Japan [2] Department of Earth and Planetary Systems Science, Graduate School of Science, Hiroshima University, Higashi-Hiroshima 739-8526, Japan.
  • Ohtani E; 1] Department of Earth Science, Graduate School of Science, Tohoku University, Sendai 980-8578, Japan [2] V. S. Sobolev Institute of Geology and Mineralogy, SB RAS, Novosibirsk, 630090, Russia.
  • Koroleva ON; Institute of Mineralogy, UB RAS, Miass, 456317, Russia.
  • Ito Y; Department of Earth Science, Graduate School of Science, Tohoku University, Sendai 980-8578, Japan.
  • Litasov KD; 1] V. S. Sobolev Institute of Geology and Mineralogy, SB RAS, Novosibirsk, 630090, Russia [2] Novosibirsk State University, Novosibirsk, 630090, Russia.
  • Pokhilenko NP; V. S. Sobolev Institute of Geology and Mineralogy, SB RAS, Novosibirsk, 630090, Russia.
Sci Rep ; 4: 5033, 2014 May 22.
Article en En | MEDLINE | ID: mdl-24852082
ABSTRACT
The Chelyabinsk asteroid impact is the second largest asteroid airburst in our recorded history. To prepare for a potential threat from asteroid impacts, it is important to understand the nature and formational history of Near-Earth Objects (NEOs) like Chelyabinsk asteroid. In orbital evolution of an asteroid, collision with other asteroids is a key process. Here, we show the existence of a high-pressure mineral jadeite in shock-melt veins of Chelyabinsk meteorite. Based on the mineral assemblage and calculated solidification time of the shock-melt veins, the equilibrium shock pressure and its duration were estimated to be at least 3-12 GPa and longer than 70 ms, respectively. This suggests that an impactor larger than 0.15-0.19 km in diameter collided with the Chelyabinsk parent body at a speed of at least 0.4-1.5 km/s. This impact might have separated the Chelyabinsk asteroid from its parent body and delivered it to the Earth.

Texto completo: 1 Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Sci Rep Año: 2014 Tipo del documento: Article País de afiliación: Japón

Texto completo: 1 Colección: 01-internacional Banco de datos: MEDLINE Idioma: En Revista: Sci Rep Año: 2014 Tipo del documento: Article País de afiliación: Japón