Spinels of the C14 kimberlite have been divided into three distinct po
pulations: 1) spinels associated with garnet, 2) spinel macrocrysts, a
nd 3) groundmass microphenocrysts. Spinels associated with garnet may
occur within garnet or as a part of the kelyphitic rim surrounding gar
net. They are characterized by a high MG# (Mg/((Mg + Fe2+) = 0.7-0.9)
and moderate to low CR# (Cr/(Cr + Al) = 0.7). Spinel macrocrysts are C
r-rich (>50 wt. % Cr2O3) with moderate MG# (0.5-0.65). The composition
of these spinels and relatively large size (>80 mu m) are consistent
with a xenocrystic origin. The microphenocrysts are small ((40 mu m) g
rains displaying two distinct compositional trends. The first occurs i
n early crystallized chromites that are zoned to higher CR# (0.7-0.9)
and lower MG# (0.5) (the Cr-enrichment, CRE trend). The second trend o
ccurs in spinels zoned from high CR# (0.9) and moderate MG# (0.5) to l
ower values (0.05 and 0.25, respectively) with increasing Fe3+ and Ti.
This Fe-Ti-enrichment (FETIE) trend is very similar to the compositio
nal spinel trends identified in other group 1 kimberlites and is thoug
ht to be due to a late- stage oxidation event. Atoll spinels are a com
mon type of groundmass microphenocryst. A model is presented which int
erprets these grains as primary growth features from the melt.