1986
DOI: 10.2113/gsecongeo.81.5.1226
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Platinum-group elements and gold in the komatiite-hosted Fe-Ni-Cu sulfide deposits at Kambalda, Western Australia

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Cited by 35 publications
(19 citation statements)
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“…It is possible that the experimental conditions are not applicable to Kambalda and that Zn partitioned more strongly into sulfide magma than the silicate magma, but it is not clear that a partition coefficient as high as 6 is justified. We obviously need better constraints on D Zn Sul/Sil , but if it is less than 6, the relatively high Zn contents of Kambalda ores (200-400 ppm: Cowden et al 1986) require an external source. A value of 2.5 produces results that are compatible with the other elements.…”
Section: Metal Variations At Kambaldamentioning
confidence: 99%
“…It is possible that the experimental conditions are not applicable to Kambalda and that Zn partitioned more strongly into sulfide magma than the silicate magma, but it is not clear that a partition coefficient as high as 6 is justified. We obviously need better constraints on D Zn Sul/Sil , but if it is less than 6, the relatively high Zn contents of Kambalda ores (200-400 ppm: Cowden et al 1986) require an external source. A value of 2.5 produces results that are compatible with the other elements.…”
Section: Metal Variations At Kambaldamentioning
confidence: 99%
“…22) to explain the presence of chromites on the komatiite-ore interface of the Silver Swan ore body (Black Swan area,Western Australia). Kambalda's massive sulphides are Ni-rich, with Ni/Fe $ 0.30, and relatively Cu-poor with only $1 wt% Cu (Cowden et al, 1986). Murck and Fig.…”
Section: Kambalda (Western Australia)mentioning
confidence: 98%
“…Eruption temperatures of komatiite lavas ranged from 1400 to 1700°C, the lavas were of very low viscosity (~0.1–1 Pa s), and it is widely assumed that they flowed turbulently ( Huppert et al 1984 ; Huppert & Sparks 1985; Hill et al 1995 ; Williams et al 1998 ). The lava is considered to have been focused into ‘channels’, (either open lava rivers, tubes or constructional lava complexes) forming thick, high‐Mg flows ( Gresham & Loftus‐Hills 1981; Lesher et al 1984 ; Cowden 1988; Cowden & Roberts 1990; Hill et al 1995 ), and laminar flowing overspills of lava from the ‘channels’ formed thin sheet flows in ‘flank’ settings.…”
Section: Komatiites and The Kambalda Modelmentioning
confidence: 99%
“…At Kambalda this sulfide mineralisation is now often preserved in trough structures, the origin of which has been widely debated. The troughs have been variably interpreted as: (i) thermal erosion channels, formed by melting and assimilation of the substrate by turbulent komatiite lava ( Huppert et al 1984 ; Huppert & Sparks 1985); (ii) pre‐existing topographic depressions deepened by thermal erosion ± structural modification ( Lesher et al 1984 ; Groves et al 1986 ); or (iii) purely structural features, with sulfide bodies in the channel facies being the focus for subsequent deformation ( Cowden 1988; Cowden & Roberts 1990). The thin flanking flows are observed to conformably overlie either the footwall metabasalt or sulfidic metasedimentary rocks at Kambalda.…”
Section: Komatiites and The Kambalda Modelmentioning
confidence: 99%