Oxygen isotope composition of phenocrysts from Tristan da Cunha and Gough Island lavas: variation with fractional crystallization and evidence for assimilation
C. Harris et al., Oxygen isotope composition of phenocrysts from Tristan da Cunha and Gough Island lavas: variation with fractional crystallization and evidence for assimilation, CONTR MIN P, 138(2), 2000, pp. 164-175
We have measured the delta(18)O values of the major phenocrysts (olivine, c
linopyroxene and plagioclase) present in lavas from Tristan da Cunha and Go
ugh Island. These islands, which result from the same mantle plume, have en
riched radiogenic isotope ratios and are, therefore, prime candidates for a
n oxygen isotope signature that is distinct from that of MORB. Consistent d
ifferences between the delta(18)O values of olivine, pyroxene and feldspar
in the cough lavas show that the phenocrysts in the mafic Gough Island lava
s are in oxygen isotope equilibrium. The olivines in lavas with SiO2 <50 wt
% have a mean delta(18)O value of 5.19 parts per thousand, consistent with
crystallization from a magma having the same oxygen isotope composition as
MORB. Phenocrysts in all the cough lavas show a systematic increase in delt
a(18)O value as silica content increases, which is consistent with closed-s
ystem fractional crystallization. The lack of enrichment in delta(18)O of t
he Gough magmas suggests that the mantle source contained <2% recycled sedi
ment. In contrast, the Tristan lavas with SiO2 >48 wt% contain phenocrysts
which have delta(18)O values that are systematically similar to 0.3 parts p
er thousand lower than their counterparts from Cough. We suggest that the p
arental mafic Tristan magmas were contaminated by material from the volcani
c edifice that acquired low delta(18)O Values by interaction with water at
high temperatures. The highly porphyritic SiO2-poor lavas show a negative c
orrelation between olivine delta(18)O value and whole-rock silica content r
ather than the expected positive correlation. The minimum delta(18)O value
occurs at an SiO2 content of about 45 wt%. Below 45 wt% SiO2, magmas evolve
d via a combination of assimilation, fractionational crystallization and cr
ystal accumulation; above 45 wt% SiO2, magmas appeared to have evolved via
closed-system fractional crystallization.