shannon hay msc thesis abstract
a representative collection of minerals from two niobium deposits found within the oka carbonatite complex: thebondzonedeposit; and the niocan deposit, were analysed using an electron microprobe, and compared with existing data from the st. lawrence columbium deposit. these minerals are good indicators of the petrological evolution of alkaline rocks, and can be used to re-evaluate the paragenesis of niobium mineralization, and the relationships between nb-bearing minerals. in addition, this study has revealed the presence of zirconolite as an accessory mineral in calciocarbonatite.
at oka , pyrochlore typically occurs as euhedra -to -subhedral crystals, rarely as aggregates and clusters. back-scattered images, coupled with microprobe analyses, reveal complex compositional zoning in pyrochlore, which undoubtedly reflects changes in the fluid composition during the growth of the mineral. large compositional variations were observed for the major oxides of the pyrochlores: cao (ranging from 4.1-34.8 wt. % oxide), tio2 (2.3-40.4 wt. %), nb2o5 (20.1-58.1 wt. %), tho2 (0.3-18.2 wt. %), and uo2 (0.1-28.0 wt. %). ceriopyrochlore, cerium pyrochlore, and uranpyrochlore exhibit the greatest a-site vacancies, ranging from 8.1-62.5 %. of the rees, only ce is present at high concentration levels (ranging from 2.1-15.8 wt. %). of note is the significant content of zro2, which ranges from 0.9-16.3 wt. %. an a-site substitution in the pyrochlore-group minerals has been identified between (ree+u+th) and (na+ca), as well as a b-site substitution between (nb+ti) and zr.
latrappite and nb-rich members of the perovskite-group are found occurring as euhedral - to -subhedral crystals. both oscillatory and patchy zonation in theokaperovskites has been identified using back-scattered imaging. small compositional variations are observed in the major oxides of both the latrappite- and -perovskite end-members. okaperovskites are slightly enriched in the lree's, ce being the dominant lree (averaging 3.5 wt. % oxide).