Tl. Dickinson et Tj. Mccoy, EXPERIMENTAL RARE-EARTH-ELEMENT PARTITIONING IN OLDHAMITE - IMPLICATIONS FOR THE IGNEOUS ORIGIN OF AUBRITIC OLDHAMITE, Meteoritics & planetary science, 32(3), 1997, pp. 395-412
Aubritic oldhamite (CaS) has been the subject of intense study recentl
y because it is the major rare-earth-element (REE) carrier in aubrites
, has a variety of REE patterns comparable to those in unequilibrated
enstatite chondrites and has an extraordinarily high melting point as
a pure substance (2525 degrees C). These latter two facts have caused
some authors to assert that much of the aubritic oldhamite is an unmel
ted nebular relict, rather than of igneous origin. We have conducted R
EE partitioning experiments between oldhamite and silicate melt using
an aubritic bulk composition at 1200 degrees C and 1300 degrees C and
subsolidus annealing experiments. All experiments produced crystalline
oldhamite, with a range of compositions, glass and Fe metal, as well
as enstatite, SiO2, diopside and troilite in some charges. Rare-earth-
element partitioning is strongly dependent on oldhamite composition an
d temperature. Subsolidus annealing results in larger partition coeffi
cients for some oldhamite grains, particularly those in contact with t
roilite. All experimental oldhamite/silicate melt partition coefficien
ts are <20 and the vast majority are <5, which is similar to those rep
orted in the literature and is two orders of magnitude less than those
inferred for natural aubritic oldhamite. These partition coefficients
preclude a simple igneous model, since REE abundances in aubritic old
hamite are greater than would be predicted on the basis of the experim
ental partition coefficients. Our experimental partition coefficients
are consistent with a relict nebular origin for aubritic oldhamite, al
though experimental evidence that suggests melting of oldhamite at tem
peratures lower than that reached on the aubrite parent body are clear
ly inconsistent with the nebular model. Our experiments are consistent
also with a complex igneous history. Oldhamite REE patterns may refle
ct a complex process of partial melting, melt removal, fractional crys
tallization and subsolidus annealing and exsolution. These mechanisms
(primarily fractional crystallization and subsolidus annealing) can pr
oduce a wide range of REE patterns in aubritic oldhamite, as well as e
levated (100-1000 x CI) REE abundances observed in aubritic oldhamite.