Mineralogy, Trace Element Composition, and Classification of Onello High-Ni Ataxite


如何引用文章

全文:

开放存取 开放存取
受限制的访问 ##reader.subscriptionAccessGranted##
受限制的访问 订阅存取

详细

The trace element composition of the Onello meteorite is analyzed in detail using SEM and LA-ICP-MS. The following Ni contents of minerals are determined (wt %): 23.0–25.4 in taenite, 5.8–8.8 in kamacite, 22–26 in schreibersite, 44–52 in nickelphosphide, 20.6–21.8 in allabogdanite, and 75–81 in awaruite. In the trace element content, the Onello meteorite corresponds to the IAB group of iron meteorites. Inside this group, it mostly matches the sHH subgroup (with high Au and Ni contents). The presence of allabogdanite in the meteorite indicates the high PT parameters of its formation: >8 GPa and 1000–1400°C. Thus, the formation of the Onello meteorite is related to impact metamorphism of a parental body of iron meteorites of the IAB group and vinonaites, in which a P- and Ni-rich area underwent melting and further crystallization.

作者简介

K. Litasov

Sobolev Institute of Geology and Mineralogy,
Siberian Branch, Russian Academy of Sciences; Novosibirsk State University

编辑信件的主要联系方式.
Email: klitasov@igm.nsc.ru
俄罗斯联邦, Novosibirsk, 630090; Novosibirsk, 630090

A. Ishikawa

Tokyo Institute of Technology

Email: klitasov@igm.nsc.ru
日本, Tokyo, 152-8550

A. Kopylova

Institute of Geology of Diamond and Precious Metals, Siberian Branch, Russian Academy of Sciences

Email: klitasov@igm.nsc.ru
俄罗斯联邦, Yakutsk, 677000

N. Podgornykh

Sobolev Institute of Geology and Mineralogy,
Siberian Branch, Russian Academy of Sciences

Email: klitasov@igm.nsc.ru
俄罗斯联邦, Novosibirsk, 630090

N. Pokhilenko

Sobolev Institute of Geology and Mineralogy,
Siberian Branch, Russian Academy of Sciences

Email: klitasov@igm.nsc.ru
俄罗斯联邦, Novosibirsk, 630090

补充文件

附件文件
动作
1. JATS XML

版权所有 © Pleiades Publishing, Ltd., 2019