Abstract
Cumulus titanomagnetite and subordinate ilmenite first appear in the Upper Zone of the Kiglapait intrusion. They arrive gradually and then reach abnormal abundances before falling to a sustained cotectic mode near seven volume per-cent. The most Ti-rich titanomagnetites (to Usp 66) are preserved in ore bands (layers) which solidified by adcumulus growth leading to the complete expulsion of interstitial silicate liquid. Analyses from three of these ore bands, applied to the solution model of Lindsley (1977), form a single linear array in fo2 versus 1/T °K, with log fo2 = (−28,283 ± 89)/T + 11.03 ± 0.25. This array implies log fo2 = −9.65 at 1094 °C, the model temperature of the Main Ore Band, consistent with primary mineral compositions Ilm89, Usp79 and a weight mode of 18 per cent ilmenite.

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