Abstract
Chemical equilibrium calculations were performed to study the condensation
chemistry of the REE and actinides under the highly reducing conditions
which are necessary for the formation of the enstatite chondrites
1,2. Our calculations confirm that the REE and actinides condensed
into oldhamite (CaS), the major REE and actinide host phase in enstatite
chondrites, at a carbon-oxygen (C/O) ratio greater-than-or-equal-to
1 in an otherwise solar gas. Five basic types of REE abundance patterns,
several of which are analogous to REE abundance patterns observed
in the Ca, Al-rich inclusions (CAIs) in carbonaceous chondrites,
are predicted to occur in meteoritic oldhamites. All of the reported
REE patterns in oldhamites in enstatite chondrites can be interpreted
in terms of our condensation calculations. The observed patterns
fall into 3 of the 5 predicted categories. The reported Th and U
enrichments and ratios in meteoritic oldhamites are also consistent
with predictions of the condensation calculations. Finally, pure
REE sulfides are predicted to condense in the 10(-6) to 10(-9) bar
range and may be found in enstatite chondrites if they formed in
this pressure range.
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