Evolution of protoplanetary disk inferred from 26Al chronology of individual chondrules

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Abstract

We review the 26Al ages of chondrules in various type 3.0 chondrites. The 26Al ages of chondrules are 1-3Myr after calcium-aluminum-rich inclusion (CAI) for LL3.0, CO3.0, and Acfer 094 (Ungrouped C 3.0). Available data for chondrules in CR chondrites indicate that many chondrules are relatively younger (≥3Myr), although data from chondrules in CR3.0 are not yet available to confirm their younger ages. The total ranges for the 26Al ages of chondrules in a single chondrite group are more than 0.5-1Myr. However, most chondrules show relatively narrow range of ages in a single chondrite group (0.2-0.4Myr, 1 SD), which might be short enough to preserve the group-specific chemical and isotope signatures against radial diffusion of solid in the disk. Distinct oxygen isotope reservoirs might exist in the protoplanetary disk simultaneously, which could be spatially separated. © 2011 The Meteoritical Society.

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Kita, N. T., & Ushikubo, T. (2012). Evolution of protoplanetary disk inferred from 26Al chronology of individual chondrules. Meteoritics and Planetary Science, 47(7), 1108–1119. https://doi.org/10.1111/j.1945-5100.2011.01264.x

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