Genesis of an exotic platinum-group-mineral-rich and Mg-poor chromitite in the Kevitsa Ni-Cu-platinum-group-elements deposit
This paper offers the first-ever study of a local chromitite stringer (~ 2 cm wide) enriched in platinum-group elements (PGE) from the Kevitsa Ni-Cu-PGE deposit. Chromite forming this chromitite is rich in Cr 2 O 3 (29.06 ̶ 37.17 wt%) and FeO (FeO total = 45.88 ̶ 56.06 wt%) and low in MgO (0.04 ̶ 0...
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Published in | Mineralogy and petrology Vol. 115; no. 5; pp. 535 - 555 |
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Main Authors | , , , |
Format | Journal Article |
Language | English |
Published |
Vienna
Springer Vienna
01.10.2021
Springer Nature B.V |
Subjects | |
Online Access | Get full text |
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Summary: | This paper offers the first-ever study of a local chromitite stringer (~ 2 cm wide) enriched in platinum-group elements (PGE) from the Kevitsa Ni-Cu-PGE deposit. Chromite forming this chromitite is rich in Cr
2
O
3
(29.06 ̶ 37.17 wt%) and FeO (FeO
total
= 45.88 ̶ 56.06 wt%) and low in MgO (0.04 ̶ 0.91 wt%). The chromitite host an unusual set of mineral inclusions including: (1) platinum-group minerals of the laurite-erlichmanite (RuS
2
-OsS
2
) solid solution series, irarsite (IrAsS), sperrylite (PtAs
2
), hollingworthite (RhAsS), anduoite [(Ru, Os)As
2
], kotulskite (PdTe) and As-, Te-, Os-, and Ru- bearing unidentified phases; (2) exsolution-lamellae of ilmenite and ulvöspinel along with chromite (111) and (100) planes, respectively; (3) silicates including crystallographically-oriented biotite, euhedral pyroxene and irregular-shaped amphiboles which tend to follow chromite growth planes, and (4) Fe-oxides, pyrrhotite, pentlandite, galena, barite, apatite, and native gold. Intercumulus minerals are microcrystalline Mg-rich biotite and minor amphibole. Pyroxenes (diopside) located immediately above the chromitite stringer exhibit higher CaO (23.02 ̶ 25.42 wt%) and Na
2
O (0.16 ̶ 0.55 wt%) than pyroxenes (augite) located below. We suggest that chromite saturation in the mafic melt was caused by local assimilation of a small pelitic xenolith. The xenolith also provided K and H
2
O explaining the occurrence of K-and volatile-rich intercumulus phases. Crystallization of chromite in this environment promoted preferential sequestering of Ir and Ru, and to a lesser extent Os, from the parental magma giving rise to an anomalous iridium-group-PGE (IPGE: Ir, Ru, and Os) enrichment. |
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ISSN: | 0930-0708 1438-1168 |
DOI: | 10.1007/s00710-021-00751-1 |