The primary mineral assemblages and initial Al-26/Al-27 ratios of rare calc
ium-aluminum-rich inclusions (CAIs) from enstatite (E) chondrites are simil
ar to those of CAIs from other chondrite classes. CAIs from all chondrite c
lasses formed under oxidizing conditions that are much different from the r
educing conditions under which the E chondrites formed. Either CAIs formed
at an earlier, more oxidizing epoch in the region where E chondrites ultima
tely formed, or they formed at a different place in the solar nebula and we
re transported into the E chondrite formation region.