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/sup 129/I//sup 127/I variations among enstatite chondrites

Journal Article · · Geochim. Cosmochim. Acta; (United States)

This paper presents the /sup 129/I//sup 127/I composition for 11 different enstatite chondrites. There is a well-defined hiatus in iodine isotopic compositions separating the enstatite chondrites. The hiatus correlates with a similar hiatus defined by variations in chemical composition (both major and minor elements). EH(4,5) chondrites have /sup 129/I//sup 127/I ratios approx. 20% higher (approx. 4 m.y. older) than EL(6) chondrites. The enstatite chondrites are the third meteorite group, joining silicates in IAB irons and C3V carbonaceous chondrites, in which /sup 129/I//sup 127/I correlates with chemical composition. Within each enstatite chondrite group, the variations in initial iodine isotopic composition is less than approx. +/- 4%, comparable to the experimental resolution. The approx. 20% difference between EH and EL may indicate a maximum iodine isotopic heterogeneity between the EH and EL nebular reservoirs. Alternatively, if EH and EL chondrites evolved from a homogeneous iodine isotopic reservoir, then the EL group must have evolved approx. 4.0 m.y. longer than the EH group and either in an environment with a much lower I/Xe ratio than presently observed or one which was open to the loss of radiogenic /sup 129/Xe. The latter case may imply a nebular environment and would therefore be consistent with the open system evolution required to produce the chemical hiatus. The duration of subsequent evolution in the high I/Xe environment must have been less than or equal to 1 m.y. and probably represents thermal metamorphism in two different parent bodies.

Research Organization:
Washington Univ., St. Louis, MO (USA)
OSTI ID:
6996766
Journal Information:
Geochim. Cosmochim. Acta; (United States), Journal Name: Geochim. Cosmochim. Acta; (United States) Vol. 52:1; ISSN GCACA
Country of Publication:
United States
Language:
English