We report the results of oxygen isotopic analyses made on mineral separates
prepared from chondrules and whole meteorites (UOCs), Feldspar/glass (main
ly chondrule mesostasis) is more O-16-poor than the olivine/low Ca pyroxene
from which it was separated. This relationship is true both for chondrules
and whole meteorites from the three UOC groups. Feldspar and glass have ex
changed to a higher degree with O-16-poor gases than ferromagnesian mineral
s because of the susceptibility of framework silicates and glass to gas-sol
id diffusion. Olivine and low Ca pyroxene have preserved primitive isotopic
compositions. In this way, mineralogy is the dominant control on the oxyge
n isotopic compositions of UOCs. The similarity of chondrule and whole mete
orite isotope compositions suggests that for many UOCs, matrix and chondrul
es have undergone exchange with the same isotope reservoirs. This exchange
postdates chondrule formation and is believed to have occurred after consol
idation with the surrounding chondrite matrix in a parent body regolith. Af
ter this gas-solid exchange. some isotopic equilibration took place between
feldspar and the other relatively O-16-rich solids, as a result of metamor
phism. A progressive decrease in the values of delta(18)O(feldspar/glass)-
delta(18)O(olivine/pyroxene) for bulk meteorites occurs with increasing pet
rologic subtype, from 8 parts per thousand for a type 3.2 to 2.5%, for a ty
pe 3.9. A chemical origin for the initial O-16-poor gas reservoirs in the H
, L, and LL parent bodies by processes of mass independent fractionation is
considered more likely than nucleosynthesis. Feldspar/glass separated from
Adrar 003 (L/LL3.2) may be in, or close to having, isotopic equilibrium wi
th the O-16-poor gases for L or LL chondrites, On this basis and assuming t
hat the gas was dominated by H2O and its isotopic composition lay along a l
ine of slope 1 (corresponding to what has been called the equilibrated chon
drite line), a tentative upper limit for gas-solid isotopic exchange in UOC
s can be calculated, which gives 370 degrees C. Copyright (C) 1999 Elsevier
Science Ltd.