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Laser-microprobe studies of rare gas isotopes in meteorites

Thesis/Dissertation ·
OSTI ID:6753337
A new rare gas mass spectrometer of high sensitivity coupled to a laser microprobe extraction system (constructed by the author) is described. The laser microprobe is applied to a long standing problem in cosmochemistry - determining the minerals which carry /sup 129/Xe from the decay of the extinct radioactive isotope /sup 129/I (this /sup 129/Xe is referred to as /sup 129/Xe/sub r/). The /sup 129/Xe/sub r//sup 127/I ratios and the inferred relative formation times of these minerals are also determined. In the Allende meteorite, sodalite (Na/sub 8/(Al/sub 6/Si/sub 6/O/sub 24/)Cl/sub 2/) has been verified to be the major carrier for /sup 129/Xe/sub r/ in fine-grained inclusions. Although the exact mineral phase responsible has not been identified a carrier other than sodalite is also present in matrix from Allende. The /sup 129/Xe/sub r/ of this carrier is physically correlated with trapped xenon in the matrix and has a chlorine/iodine ratio which is lower than the ratio in the fine-grained inclusions. The /sup 129/Xe/sub r///sup 127/I ratios for sodalite from the fine-grained inclusions, and matrix are similar - between 1.25 and 1.35 x 10/sup -4/. This implies an age for these samples within 2 million years of the Bjurbole meteorite (Bjurbole is commonly used as a standard for meteorite formation intervals). The /sup 129/Xe/sub r///sup 127/I ratio of the sample of the fine-grained inclusion in which sodalite was thermally decomposed by laboratory preheating, is 2.4 x 10/sup -4/ or 16 million years before Bjurbole. The alteration-product-free coarse-grained inclusion on the other hand showed a ratio of 3.15 x 10/sup -5/ or 35 million years after Bjurbole. These relative formation intervals are much longer than expected for nebular processes and hence are either due to parent body processes or heterogeneity of the /sup 129/I//sup 127/I ratio in the early solar system.
Research Organization:
California Univ., Berkeley (USA)
OSTI ID:
6753337
Country of Publication:
United States
Language:
English