Ultraviolet Laser microprobe analyses of a calcium-aluminum-rich inclu
sion (CAI) from the Allende meteorite suggest that a Line with a slope
of exactly 1.00 on a plot of delta(17)O against delta(18)O represents
the primitive oxygen isotope reservoir of the early solar nebula. Mos
t meteorites are enriched in O-17 and O-18 relative to this Line, and
their oxygen isotope ratios can be explained by mass fractionation or
isotope exchange initiating from the primitive reservoir. These data e
stablish a Link between the oxygen isotopic composition of the abundan
t ordinary chondrites and the primitive O-16-rich component of CAIs.