The Okhansk Meteorite: Specifics of Composition, Structure, and Genesis

被引:0
|
作者
Bakhtin, A. I. [1 ]
Sonin, G. V. [1 ]
Sungatullin, R. Kh. [1 ]
Petrova, R. D. [1 ]
机构
[1] Kazan Fed Univ, Kazan 420008, Russia
关键词
Okhansk meteorite; chondrites; protosolar nebula; genesis;
D O I
暂无
中图分类号
O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];
学科分类号
07 ; 0710 ; 09 ;
摘要
The Okhansk meteorite fell on August 18, 1887 near the village of Tabor, about 15 km away from the town of Okhansk in Perm province and weighed 186.5 kg (the total weight of collected fragments, according to P. I. Krotov, was more than 245 kg). The shock wave from the meteorite entry knocked down animals and riders on horses. Despite the fact that it was significantly stronger than that caused by the Chelyabinsk meteorite of 2013, all information about this meteorite has completely erased from people's memory. It has been shown that the meteorite is an ordinary olivine-bronzite chondrite. Its main silicate minerals are olivine, bronzite, plagioclase, and diopside. The main ore minerals are kamacite and troilite. The meteorite contains silicate glass in large amounts. The analysis of the composition and structure of the Okhansk meteorite has demonstrated that it was formed at the early stages of accretion of the melted substance of the protosolar nebula without undergoing endogenous, temperature, or pressure changes.
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页码:569 / 582
页数:14
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