The carbonatite occurrences in the State of Rajasthan, Western India,
comprise two age groups: the Newania Complex relates to the Aravalli o
rogeny (Proterozoic), while the remaining three: Mundwara, Sarnu-Danda
li-Kamathi, and Bhamni, represent the pre-Deccan Flood Basalt carbonat
ite-alkalic activity at ca 68.5 Ma. Geochemical, Sr isotope (varying f
rom 0.7021 to 0.7034), and C and O isotopic data (between -5 and +8 pa
rts per thousand respectively), for the Newania carbonatite indicate t
hat it is a mantle-derived primary melt that has preserved its initial
composition. Low Sr isotopic composition and negative epsilon(Nd) val
ue indicate that the Newania rauhaugite is derived from an old, LREE-e
nriched lithospheric mantle source. The younger carbonatite occurrence
s are closely associated with nephelinites and phonolites into which t
hey penetrate as dikes. The significant feature of the Newania carbona
tites is their varied mineral assemblages from cumulate apatite, magne
tite, pyrochlore, Nb-silicate in rauhaugite to pyrite, chalcopyrite, m
alachite, monazite in the late-phase ankeritic carbonatite. Pyrochlore
is exceptionally rich in UO2, varying between 18.68 to 22.92%. There
are mainly two types of pyrochlores; one rich in BaO (2.41% to 9.68%)
and the other very poor in BaO (0.20 to 0.31%), Chalcopyrite does not
show much variation (S = 35.07%, Fe = 30.18% and Cu = 35.09%), while m
alachite shows small variation in Cu content (average CuO = 72%). The
alvikite dikes in Kamathi are highly enriched in REE (total REE at tim
es exceeds 15%), while in the Bhamni area carbonatite contains appreci
able amounts of fluorite and lead-zinc ore (PbO = 22.12%, ZnO = 32.50%
, Fe2O3 = 16.02%, CdO = 0.25%, Sb2O3 = 0.03%, SiO2 = 9.05%, Zr = 814 p
pm, Cu = 160 ppm, Cr = 70 ppm, Co = 23 ppm, and Ni = 23 ppm).