Literature DB >> 9836631

53Mn-53Cr dating of fayalite formation in the CV3 chondrite Mokoia: evidence for asteroidal alteration.

I D Hutcheon1, A N Krot, K Keil, D L Phinney, E R Scott.   

Abstract

Fayalite grains in chondrules in the oxidized, aqueously altered CV3 chondrite Mokoia have large excesses of radiogenic chromium-53. These excesses indicate the in situ decay of short-lived manganese-53 (half-life = 3.7 million years) and define an initial 53Mn/55Mn ratio of 2.32 (+/-0.18) x 10(-6). This ratio is comparable to values for carbonates in CI and CM chondrites and for several classes of differentiated meteorites. Mokoia fayalites formed 7 to 16 million years after Allende calcium-aluminum-rich inclusions, during hydrothermal activity on a geologically active asteroid after chondritic components had ceased forming in the solar nebula.

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Year:  1998        PMID: 9836631     DOI: 10.1126/science.282.5395.1865

Source DB:  PubMed          Journal:  Science        ISSN: 0036-8075            Impact factor:   47.728


  1 in total

1.  Early aqueous activity on the ordinary and carbonaceous chondrite parent bodies recorded by fayalite.

Authors:  Patricia M Doyle; Kaori Jogo; Kazuhide Nagashima; Alexander N Krot; Shigeru Wakita; Fred J Ciesla; Ian D Hutcheon
Journal:  Nat Commun       Date:  2015-06-23       Impact factor: 14.919

  1 in total

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