HOTTER THAN YOU THOUGHT--KOMATIITES FROM THE BARBERTON GREENSTONE BELT
Previous studies have demonstrated that random spinifex zones are nearest to primary liquid compositions in texturally complex komatiitic flows. Apparent Kds found from the olivine accumulation trend or from microprobe analyses of the most magnesian olivines found in the flows are: Ni - 2.0, Co - 1.3, Mn - 0.50, Cr - 0.45, Sc - 0.10, Y - 0.03, V - 0.01, and Zr , Ti, and Al all less than 0.01. These values are very consistent with recent studies of very high temperature and/or highly oxidized magmas. V, Cr, and Fe are all at appropriate values for conditions as oxidizing as NNO+2.
The olivine-melt Fe-Mg Kd observed in this highly oxidized liquid, at 0.37, is higher than often reported, but consistent with other relatively fresh Barberton flows and consistent with some theoretical and experimental results. The temperature of eruption for such a liquid would be 1700 degrees Celsius, and even the much more conservative use of the oriented spinifex samples (MgO 30.6%) would yield a temperature of 1600 degrees. These high temperatures and oxidation states should have important implications for both Archean tectonism and mantle evolution. However, these komatiites are not boninites or kimberlites. Petrographic and field studies confirm that they represent aphyric liquids, erupted and transported long distances at the Earth's surface prior to the onset of any crystallization.