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      A model for planetesimal meltdown by26Al and its implications for meteorite parent bodies

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      Meteoritics & Planetary Science
      Wiley-Blackwell

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          Lead isotopic ages of chondrules and calcium-aluminum-rich inclusions.

          The lead-lead isochron age of chondrules in the CR chondrite Acfer 059 is 4564.7 +/- 0.6 million years ago (Ma), whereas the lead isotopic age of calcium-aluminum-rich inclusions (CAIs) in the CV chondrite Efremovka is 4567.2 +/- 0.6 Ma. This gives an interval of 2.5 +/- 1.2 million years (My) between formation of the CV CAIs and the CR chondrules and indicates that CAI- and chondrule-forming events lasted for at least 1.3 My. This time interval is consistent with a 2- to 3-My age difference between CR CAIs and chondrules inferred from the differences in their initial 26Al/27Al ratios and supports the chronological significance of the 26Al-26Mg systematics.
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            Aluminum-26 in the early solar system - Fossil or fuel

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              The Record in the Meteorites. III. on the Development of Meteorites in Asteroidal Bodies.

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                Author and article information

                Journal
                Meteoritics & Planetary Science
                Wiley-Blackwell
                10869379
                January 2006
                January 2006
                : 41
                : 1
                : 95-106
                Article
                10.1111/j.1945-5100.2006.tb00195.x
                cc56b422-372b-491d-a693-8d40cd1ae784
                © 2006

                http://doi.wiley.com/10.1002/tdm_license_1

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