David R. Frank^a, Michael E. Zolensky^b and Loan Le^a

^aESCG, NASA Johnson Space Center, Houston, TX 77058, USA
^bAstromaterials Research and Exploration Science, NASA Johnson Space Center, Houston, TX 77058, USA

The dearth of both major and minor element analyses of anhydrous silicate phases in chondrite matrix has thus far hindered their comparison to the Wild 2 samples. We present 68 analyses of olivine (Fa_0-97) in the coarse-grained terminal particles of Stardust aerogel tracks and a comprehensive dataset (> 10³ analyses) of analogous olivine grains (5-30μm) isolated in CI, CM, CR, CH, CO, CV3-oxidized, CV3-reduced, C3-ungrouped (Acfer 094 and Ningqiang), L/LL 3.0-4, EH3, and Kakangari chondrite matrix. These compositions reveal that Wild 2 likely accreted a diverse assortment of material that was radially transported from various carbonaceous and ordinary chondrite-forming regions. The Wild 2 olivine includes ameoboid olivine aggregates (AOAs), refractory forsterite, type I and type II chondrule fragments and/or microchondrules, and rare relict grain compositions. In addition, we have identified one terminal particle that has no known compositional analog in the meteorite record and may be a signature of low-temperature, aqueous processing in the Kuiper Belt. The generally low Cr content of FeO-rich olivine in the Stardust samples indicates that they underwent mild thermal metamorphism, akin to a petrologic grade of 3.05-3.15.

Reference
Frank DR, Zolensky ME and Le L (in press) Olivine in terminal particles of Stardust aerogel tracks and analogous grains in chondrite matrix. Geochimica et Cosmochimica Acta
[doi:10.1016/j.gca.2014.05.037]
Copyright Elsevier

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