Iodine-xenon analyses of chondrules from the Bjurbole L4 and Parnallee
LL3.5 meteorites have been made using a continuous wave laser micropr
obe and the resonance ionisation mass spectrometer RELAX. The excess X
e-129 content released from the Bjurbole chondrule is lower than previ
ous stepped-heating studies have found, suggesting that the technique
does not completely degas the samples. Nonetheless, clear isochrons we
re produced, and data for initial Xe-129/Xe-130 are consistent with ea
rlier work. A correlation is evident in each chondrule between Xe-131
and Xe-128, perhaps indicating a common host-phase for their parent
nuclides, a condition possibly fulfilled by a Te- and I-bearing sulfid
e. The I-Xe system of a Parnallee macrochondrule exhibits no excess Xe
-129, possibly as a result of thermal alteration or deformation before
accumulation of the meteorite. A cristobalite-bearing chondrule deple
ted in O-16 yields an I-Xe age of 4.5 +/- 0.5 Ma after the mean Bjurbo
le age.