Fort À La Corne Kimberlite Model
Unlike the idealized South African kimberlite model (Hawthorne, 1975), the majority of the FalC kimberlites are mainly shallow bowl-shaped kimberlites which have kimberlite footprints ranging up to 2,000 m wide and extending to depths ranging from approximately 100 m to greater than 700 m.
The limited deep drilling, however, precludes any interpretation of the shape of the kimberlites below about 450 m. Therefore, at depth, the FalC kimberlites may, in fact, resemble the idealized South African model.
FalC kimberlites were emplaced into poorly consolidated Cretaceous-aged clastic and marine sedimentary rocks. They are generally interpreted to be in the form of stacked, sub-horizontal lenses or shallow zones of crater facies material with associated pyroclastic flow and fall deposits of large lateral extent. The kimberlite phases are classified entirely as crater-facies pyroclastic kimberlite, although a number of kimberlite units may be distinguished according to their grain size, style of emplacement, primary and chemical alteration and the abundance and presence of olivine macrocrysts.
Star Kimberlite Geology And Mineralization
The Star Kimberlite was deposited within the Cretaceous sedimentary rocks of the lower Colorado and Mannville groups, which unconformably overlie Paleozoic limestones and dolomites. The glacial overburden thickness ranges from 90 to 130 m with an average of 92 m. Portions o ........
