We report the petrology, O isotopic composition, and Al-Mg isotope systematics of a chondrule fragment from the Jupiter-family comet Wild 2, returned to Earth by NASA's Stardust mission. This object shows characteristics of a typeII chondrule that formed from an evolved oxygen isotopic reservoir. No evidence for extinct 26Al was found, with (26Al/ 27Al)0 < 3.0 × 10-6. Assuming homogenous distribution of 26Al in the solar nebula, this particle crystallized at least 3Myr after the earliest solar system objects - relatively late compared to most chondrules in meteorites. We interpret the presence of this object in a Kuiper Belt body as evidence of late, large-scale transport of small objects between the inner and outer solar nebula. Our observations constrain the formation of Jupiter (a barrier to outward transport if it formed further from the Sun than this cometary chondrule) to be more than 3Myr after calcium-aluminum-rich inclusions. © 2012. The American Astronomical Society. All rights reserved..
CITATION STYLE
Ogliore, R. C., Huss, G. R., Nagashima, K., Butterworth, A. L., Gainsforth, Z., Stodolna, J., … Tyliszczak, T. (2012). Incorporation of A late-forming chondrule into comet Wild 2. Astrophysical Journal Letters, 745(2). https://doi.org/10.1088/2041-8205/745/2/L19
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