R. Schoenberg et al., PGE enrichment in chromitite layers and the Merensky Reef of the western Bushveld Complex; a Re-Os and Rb-Sr isotope study, EARTH PLAN, 172(1-2), 1999, pp. 49-64
Four poikilitic pyroxenites of the Bastard Unit, all being relatively low i
n osmium concentrations, define a Re-Os isochron age of 2043 +/- 11 Ma (wit
h initial Os-187/Os-188 = 0.151), which is in accordance with the normally
cited crystallization age of the Bushveld Complex. The isochron fit demonst
rates an excellent radiogenic Os isotopic homogeneity of this portion of th
e complex at the time of crystallization and excludes any later disturbance
of the Re-Os isotope system, Initial Os-187/Os-188 ratios of platinum-grou
p element (PGE) enriched sulfides and whole rocks of the directly underlyin
g Merensky Reef are highly radiogenic and variable (with values between 0.1
68 and 0.181). Separates of chromite grains and interstitial phases of Crit
ical Zone chromitite layers show initial Os-187/Os-188 signatures ranging f
rom the near-chondritic mantle values of lower group chromitites (i.e. simi
lar to 0.120) to 0.137 for middle group chromitites and to 0.150 for the up
per group 2 chromitite layer. Osmium concentrations of interstitial phases
exceed those of the associated chromite in all layers by up to 30 fold, sho
wing the presence of highly PGE-enriched interstitial sulfides. Equal or ve
ry similar initial Os-187/Os-188 signatures of the interstitial minerals an
d the cumulus chromite grains together with their coupled increasing and de
creasing trends in this ratio clearly demonstrate that interstitial sulfide
s and associated cumulus chromite of the different chromitite layers scaven
ged their osmium from the same or similar sources. Therefore, a PGE enrichm
ent of the interstitial sulfides by a primary magmatic process, such as pre
cipitation of immiscible sulfide droplets during magma mixing appears more
likely than a scenario involving fluid or melt transport of PGE into these
layers. Such a primary magmatic PGE enrichment process is also preferred fo
r the formation of the Merensky Reef. (C) 1999 Elsevier Science B.V. All ri
ghts reserved.