Meteorite Seymchan Structure / Hontsova S. S.,Petrova E. V.,Muftahetdinova R. F.,Chulanova V. N.,Grokhovsky V. I. // . - 2016. - V. 1767, l. .

ISSN/EISSN:

0094-243X / нет данных

Type:

Proceedings Paper

Abstract:

The meteorite Seymchan specimen was studied using optical microscopy and scanning electron microscopy. Olivine grains have roundish shapes, which was formed during matter cooling. Different features of the metal structure such as plessite structure and Neimann bands were observed. The oxide edges were observed in the boundaries between phases. The oxides were formed in the terrestrial conditions. The boundary regions between metal and olivine in the meteorite contain grains of troilite, schreibersite, and chromite.

Author keywords:

PALLASITE METEORITES

DOI:

10.1063/1.4962611

Web of Science ID:

ISI:000392693900027

Соавторы в МНС:

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Другие поля

Поле	Значение
Editor	Rempel, AA and Volkovich, VA
Booktitle	PHYSICS, TECHNOLOGIES AND INNOVATION (PTI-2016)
Series	AIP Conference Proceedings
Note	3rd International Young Researchers Conference - Physics, Technologies and Innovation (PTI), Ekaterinburg, RUSSIA, MAY 16-20, 2016
Organization	Ural Fed Univ, Inst Phys \& Technol
Publisher	AMER INST PHYSICS
Address	2 HUNTINGTON QUADRANGLE, STE 1NO1, MELVILLE, NY 11747-4501 USA
Language	English
Article-Number	020027
ISBN	978-0-7354-1425-9
Keywords-Plus	PALLASITE METEORITES
Research-Areas	Physics
Web-of-Science-Categories	Physics, Applied; Physics, Multidisciplinary
Author-Email	sgoncova@gmail.com evgeniya.petrova@urfu.ru
Funding-Acknowledgement	Russian Foundation for Basic Research {[}16-35-50029 mol\_nr, 15-35-21164 mol\_a\_ved]
Funding-Text	This work was supported by Russian Foundation for Basic Research grant No. 16-35-50029 mol\_nr and partial support of the Russian Foundation for Basic Research grant No. 15-35-21164 mol\_a\_ved.
Number-of-Cited-References	7
Doc-Delivery-Number	BG8SP