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Neutron capture records of mesosiderites and an iron meteorite

机译:中子捕获中铁菱铁矿和铁陨石的记录

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摘要

The Sm and Gd isotopic compositions of silicates from six mesosiderites (Dalgaranga, Estherville, Morristown, Northwest Africa (NWA) 1242, NWA 2932, and Vaca Muerta) and one iron meteorite (Udei Station) were determined to elucidate the cosmic-ray exposure records. All seven samples showed significant ~(150)Sm/~(149)Sm and ~(158)Gd/~(157)Gd isotopic shifts from neutron capture reactions corresponding to neutron fluences of (1.3-21.8)×10~(15)ncm~(-2). In particular, Vaca Muerta showed a significantly higher neutron fluences than the other six samples. The parameter for the degree of neutron thermalization (ε_(Sm)/ε_(Gd)) also showed a significant difference between Vaca Muerta (0.76) and the other samples (0.93-1.20). These results suggest a two-stage irradiation of the Vaca Muerta silicates in the parent body (>50Ma) before formation of the mesosiderite and during its transit to Earth (138Ma). This is consistent with the ~(81)Kr-Kr cosmic-ray exposure age data of a Vaca Muerta pebble from a previous noble gas isotopic study.
机译:确定了六种中观菱铁矿(Dalgaranga,Estherville,Morristown,西北非洲(NWA)1242,NWA 2932和Vaca Muerta)和一种铁陨石(Udei站)的硅酸盐的Sm和Gd同位素组成,以阐明宇宙射线的暴露记录。 。所有七个样品均显示出来自中子俘获反应的〜(150)Sm /〜(149)Sm和〜(158)Gd /〜(157)Gd同位素位移,对应于中子注量为(1.3-21.8)×10〜(15) ncm〜(-2)。特别是,瓦卡·穆尔塔(Vaca Muerta)的中子注量明显高于其他六个样品。中子热化程度的参数(ε_(Sm)/ε_(Gd))在Vaca Muerta(0.76)和其他样品(0.93-1.20)之间也显示出显着差异。这些结果表明,在中速菱铁矿形成之前和过渡到地球(138Ma)期间,母体中的Vaca Muerta硅酸盐(> 50Ma)经历了两阶段照射。这与来自先前稀有气体同位素研究的Vaca Muerta卵石的〜(81)Kr-Kr宇宙射线暴露年龄数据一致。

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