A petrographic and Ar-40/Ar-39 geochronological study of the Voorspoed kimberlite, South Africa: Implications for the origin of Group II kimberlite magmatism
D. Phillips et al., A petrographic and Ar-40/Ar-39 geochronological study of the Voorspoed kimberlite, South Africa: Implications for the origin of Group II kimberlite magmatism, S AFR J GEO, 101(4), 1998, pp. 299-306
The Voorspoed kimberlite pipe is one of a cluster of eleven kimberlite and
related rock intrusives, located north of Kroonstad in the Free State. The
pipe comprises tuffisitic kimberlite plus tuffisitic kimberlite breccia and
is associated with several hypabyssal sills and dykes. A large down-rafted
block of Karoo lava occupies about six hectares of the pipe to a depth of
at least 300 m. A recent drilling programme has enabled the recognition of
two types of tuffisitic kimberlite breccia, as well as seven varieties of h
ypabyssal facies kimberlite. As the Voorspoed kimberlite is located between
the similar to 120 Ma Barkly West and the similar to 145 Ma Swartruggens k
imberlites, accurate determination of an intrusion age is crucial to the ev
aluation of the Group II age progression across southern Africa and models
proposed for the origin of Group II magmatism. Ar-40/Ar-39 laser probe anal
yses were carried out on six individual groundmass phlogopite grains from a
hypabyssal kimberlite autolith. All grains yielded reproducible plateau ag
es averaging 131.8 +/- 1.7 Ma (2 sigma). The intra- and inter-grain reprodu
cibility of the current data indicates that this age represents a reliable
estimate for the time of pipe emplacement. The age is also in agreement wit
h recent data obtained for the nearby Lace and Besterskraal kimberlites. In
combination, these results confirm the regular northeasterly age progressi
on of Group II kimberlites across the Kaapvaal Craton. Postulated models to
account for the distribution of Group II kimberlites have invoked hot spot
tracks, subduction of oceanic crust, and rafting of the subcontinent over
an oceanic lithosphere megalith. As an alternative, a model involving exten
sional tectonics in relation to the disaggregation of Gondwanaland is consi
dered.