首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >Pd-Ag chronometry of IVA iron meteorites and the crystallization and cooling of a protoplanetary core
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Pd-Ag chronometry of IVA iron meteorites and the crystallization and cooling of a protoplanetary core

机译:IVA铁陨石的PD-AG编程和原始核心的结晶和冷却

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摘要

To constrain the timescales and processes involved in the crystallization and cooling of protoplanetary cores, we examined the Pd-Ag isotope systematics of the IVA iron meteorites Muonionalusta and Gibeon. A Pd-Ag isochron for Muonionalusta provides an initial Pd-107/(108) Pd = (2.57 +/- 0.07) x 10(-5). The three metal samples analyzed from Gibeon plot below the Muonionalusta isochron, but these samples also show significant effects of cosmic ray-induced neutron capture reactions, as is evident from 196 Pt excesses in the Gibeon samples. After correction for neutron capture effects on Ag isotopes, the Gibeon samples plot on the Muonionalusta isochron, indicating that these two IVA irons have indistinguishable initial Pd-107/(108) Pd. Collectively, the Pd-Ag data indicate cooling of the IVA core below Pd-Ag closure between 2.9 +/- 0.4 Ma and 8.9 +/- 0.6 Ma after CAI formation, where this age range reflects uncertainties in the initial Pd-107/(108) Pd ratios of the solar system, which in turn result from uncertainties in the Pb-Pb age of Muonionalusta. The Ag isotopic data indicate that the IVA core initially evolved with a modestly elevated Pd/Ag, but the low Ag concentrations measured for some metal samples indicate derivation from a source with much lower Ag contents and, hence, higher Pd/Ag. These contrasting observations can be reconciled if the IVA irons crystallized from an initially more Ag-rich core, followed by extraction of Fe-S melts during compaction of the nearly solidified core. Owing to its strong tendency to partition into Fe-S melts, Ag was removed from the IVA core during compaction, leading to the very low Ag concentration observed in metal samples of IVA irons. Alternatively, Ag was lost by evaporation from a still molten metallic body just prior to the onset of crystallization. The Pd-Ag isotopic data indicate that Muonionalusta cooled at >500 K/Ma through the Pd-Ag closure temperature of similar to 900 K, consistent with the rapid cooling inferr
机译:为了限制涉及原型核心结晶和冷却的时间尺度和过程,我们研究了IVA铁陨石Muonionalusta和Gibon的PD-Ag同位素系统。 MuonIonalusta的PD-AG等色提供初始PD-107 /(108)PD =(2.57 +/- 0.07)×10(-5)。从muonionalusta等中的Gibeon Plot分析的三种金属样品,但这些样品也显示出宇宙射线诱导的中子捕获反应的显着影响,从GIBEON样品中的196pt过量的显而易见。在对Ag同位素上的中子捕获作用校正后,GIBEON样品在muonionalusta等中的图案,表明这两个IVA铁杆具有难以区分的初始PD-107 /(108)PD。统称,PD-AG数据表示CAI形成后PD-AG闭合低于PD-AG闭合的IVA核心的冷却,在CAI形成后,该年龄范围反映了初始PD-107 /( 108)太阳系的PD比率,这反过来导致Muonionalusta的PB-PB年龄的不确定性。 AG同位素数据表明,IVA核最初用适度升高的Pd / Ag演变,但是对于一些金属样品测量的低Ag浓度表明来自具有大得多的Ag含量的源极,因此,更高的Pd / Ag。如果IVA铁磁从最初更富含Ag的核心结晶,然后在几乎固化的核心的压实期间提取Fe-S熔体,则可以和解这些对比观察。由于其强烈分配进入Fe-S熔体的趋势,在压实过程中从IVA核中取出Ag,导致IVA铁杆的金属样品中观察到的非常低的AG浓度。或者,在结晶开始之前,通过从仍然熔融金属体蒸发蒸发Ag。 PD-AG同位素数据表明,通过PD-AG闭合温度与900 k相似的PD-AG闭合温度,MuonIongusta通过快速冷却下骤下的符合

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