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根据球粒陨石的镁同位素组成推断太阳系中26Al的均匀分布。

Homogeneous distribution of 26Al in the solar system from the Mg isotopic composition of chondrules.

作者信息

Villeneuve Johan, Chaussidon Marc, Libourel Guy

机构信息

Centre de Recherches Petrographiques et Geochimiques (CRPG)-Nancy Université-CNRS, UPR 2300, 15 Rue Notre-Dame des Pauvres, Boite Postale 20, 54501 Vandoeuvre-lès-Nancy, France.

出版信息

Science. 2009 Aug 21;325(5943):985-8. doi: 10.1126/science.1173907.

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 approximately 1.2 million years (My) to approximately 4 My after the first solids condensed from the solar nebula, with peaks between approximately 1.5 and approximately 3 My, and that chondrule precursors formed as early as 0.87(-0.16)(+0.19) My after.

摘要

太阳系中第一批固体物质形成的时间仍然受到很大限制。微米级的高精度镁(Mg)同位素分析表明,地球、难熔包体以及原始陨石中的球粒是由一个储库形成的,在这个储库中,短寿命的铝-26(26Al)和镁同位素以±10%的比例均匀分布。这种均匀程度验证了将26Al用作早期太阳系事件精确计时工具的可行性。高精度的球粒26Al等时线表明,在第一批固体物质从太阳星云凝聚出来后的大约120万年(My)到大约400万年之间,发生了几次不同的球粒熔化事件,峰值出现在大约150万年到大约300万年之间,并且球粒前体早在0.87(-0.16)(+0.19)百万年后就已形成。

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