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


Дәйексөз келтіру

Толық мәтін

Ашық рұқсат Ашық рұқсат
Рұқсат жабық Рұқсат берілді
Рұқсат жабық Тек жазылушылар үшін

Аннотация

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.

Авторлар туралы

K. Litasov

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

Хат алмасуға жауапты Автор.
Email: klitasov@igm.nsc.ru
Ресей, Novosibirsk, 630090; Novosibirsk, 630090

A. Ishikawa

Tokyo Institute of Technology

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

A. Kopylova

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

Email: klitasov@igm.nsc.ru
Ресей, Yakutsk, 677000

N. Podgornykh

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

Email: klitasov@igm.nsc.ru
Ресей, Novosibirsk, 630090

N. Pokhilenko

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

Email: klitasov@igm.nsc.ru
Ресей, Novosibirsk, 630090

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