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We report the petrology, O isotopic composition, and Al-Mg isotope system-atics 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 type II 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 3 Myr after the earliest solar system objects—relatively late compared to most chon-drules 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 3 Myr after calcium-aluminum-rich inclusions. Subject headings: comets: individual (Wild 2) — Kuiper belt — solar system: formation — planets and satellites: individual (Jupiter) ar X i