In situ ion microprobe analyses of spinel in refractory calcium-aluminium-r
ich inclusions (CAIs) from type 3 EH chondrites yield O-16-rich composition
s (delta O-18 and delta O-17 about -40 parts per thousand). Spinel and feld
spar in a CAI from an EL3 chondrite have significantly heavier isotopic com
positions (delta O-18 and delta O-17 about -5 parts per thousand). A regres
sion through the data results in a line with slope 1.0 on a three-isotope p
lot, similar to isotopic results from unaltered minerals in CAIs from carbo
naceous chondrites. The existence of CAIs with O-16-rich and O-16-poor comp
ositions in carbonaceous as well as enstatite chondrites indicates that CAI
s formed in at least two temporally or spatially distinct oxygen reservoirs
. General similarities in oxygen isotopic compositions of CAIs from enstati
te, carbonaceous, and ordinary chondrites indicate a common nebular mechani
sm or locale for the production of most CAIs.