The abundance of FeTiO3 and chromite precipitates in olivine of the Al
pe Arami peridotite massif, Switzerland, requires a much higher solubi
lity for highly charged cations than is found in mantle xenoliths from
depths of 250 kilometers. Three previously unknown crystal structures
of FeTiO3 were identified that indicate that the originally exsolved
phase was the high-pressure perovskite polymorph of ilmenite, implying
a minimum depth of origin of 300 kilometers. These observations, coup
led with the unique lattice preferred orientation of olivine, further
suggest that the original composition of olivine may reflect that of a
precursor phase, perhaps wadsleyite, that is stable only at depths gr
eater than 400 kilometers.