Homogeneous Distribution of <SUP>26</SUP>Al in the Solar System from the Mg Isotopic Composition of Chondrules - Archive ouverte HAL Access content directly
Journal Articles Science Year : 2009

Homogeneous Distribution of 26Al in the Solar System from the Mg Isotopic Composition of Chondrules

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Abstract

The timing of the formation of the first solids in the solar system remains poorly constrained. Micrometer-scale, high-precision magnesium (Mg) isotopic analyses demonstrate that Earth, refractory inclusions, and chondrules from primitive meteorites formed from a reservoir in which short-lived aluminum-26 (26Al) and Mg isotopes were homogeneously distributed at ±10%. This level of homogeneity validates the use of 26Al as a precise chronometer for early solar system events. High-precision chondrule 26Al isochrons show that several distinct chondrule melting events took place from ~1.2 million years (My) to ~4 My after the first solids condensed from the solar nebula, with peaks between ~1.5 and ~3 My, and that chondrule precursors formed as early as 0.87-0.16+0.19 My after.

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insu-03619248 , version 1 (25-03-2022)

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Johan Villeneuve, Marc Chaussidon, Guy Libourel. Homogeneous Distribution of 26Al in the Solar System from the Mg Isotopic Composition of Chondrules. Science, 2009, 325, pp.985. ⟨10.1126/science.1173907⟩. ⟨insu-03619248⟩
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