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Microstructures, mineral chemistry, noble gases and nitrogen in the recent fall, Bhuka iron (IAB) meteorite

机译:最近秋天的微结构,矿物化学,稀有气体和氮气Bhuka铁(IAB)陨石

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We report some chemical, petrological and isotopic studies of the Bhuka iron meteorite that fell in Rajasthan, India in 2005. Numerous silicate and graphite inclusions are visible on the surface of the hand specimen. In the polished and etched surface studied, irregular patches of graphite are found as the most dominant inclusion and commonly associated with pure corundum (95 wt% Al2O3), spinet, feldspar and Si-rich phases. Apart from typical lamellar intergrowth with kamacite (i.e. the Widmanstatten pattern), taenites are also commonly found to occur as a rim of the graphite inclusions. P-rich (up to 10 wt%) taenites are also found locally within the recrystallised kamacite matrix. Based on mineralogy, texture and bulk composition, Bhuka resembles the low-Ni IAB subgroup (ungrouped). Noble gas isotope studies suggest He, Ne and Ar are mostly of cosmogenic origin, while Kr and Xe are a mixture of cosmogenic, radiogenic and trapped components. A pre-atmospheric radius of 10 +/- 1 cm and a cosmic ray exposure age of 346 +/- 52 Ma are derived based on depth dependant (He-3/He-4)(c) and Ar-38(c) respectively, as per the production systematics of cosmogenic noble gas isotopes (Ammon et al., 2009). Cosmogenic Kr-83 and Xe-126 yield production rates of 12 and 0.335 (in 10(-15)ccSTP/g Ma) for Kr-83 and Xe-126 respectively. Presence of trapped Kr and Xe, with (Kr-84/Xe-132)(t)=2 and radiogenic Xe-129=120 x 10(-12) ccSTP/g are due to presence of graphite/silicate inclusions in the analysed sample. Over similar to 150% excess Xe-131(c), than expected from spallation suggests contribution from (n,gamma) reactions from Ba from inclusions and suggests irradiation of pre-atmospheric object in a larger body, indicative of complex irradiation. Trapped N of 24 ppm, with delta N-15= -10.7 +/- 0.8 parts per thousand observed in Bhuka, is heavier than the range observed hither to in IAB irons. (C) 2016 Elsevier Ltd. All rights reserved.
机译:我们报告了2005年在印度拉贾斯坦邦落下的布卡铁陨石的一些化学,岩石学和同位素研究。手部标本的表面可见大量硅酸盐和石墨夹杂物。在研究的抛光和蚀刻表面中,发现不规则的石墨斑是最主要的夹杂物,通常与纯刚玉(95 wt%Al2O3),尖晶石,长石和富硅相有关。除了典型的层状共生体与滑石矿共生(即Widmanstatten模式)以外,还经常发现石是石墨夹杂物的边缘。在重结晶的kamacite基质中还局部发现了富磷(最高10 wt%)的钛矿。基于矿物学,质地和整体组成,布卡(Bhuka)类似于低Ni IAB亚组(未分组)。稀有气体同位素研究表明,He,Ne和Ar主要是宇宙成因的,而Kr和Xe是宇宙成因,放射成因和被困成分的混合物。根据与深度有关的(He-3 / He-4)(c)和Ar-38(c)得出大气前半径为10 +/- 1 cm和宇宙射线暴露年龄为346 +/- 52 Ma分别根据宇宙成因稀有气体同位素的生产系统(Ammon等,2009)。宇宙成因的Kr-83和Xe-126的生产率分别为Kr-83和Xe-126,分别为12和0.335(在10(-15)ccSTP / g Ma中)。 (Kr-84 / Xe-132)(t)= 2和放射源Xe-129 = 120 x 10(-12)ccSTP / g的捕获Kr和Xe的存在是由于分析中存在石墨/硅酸盐夹杂物样品。超过150%的过量Xe-131(c),比剥落所预期的多,暗示了来自夹杂物Ba的(n,γ)反应的贡献,并暗示了较大物体中对大气前物体的辐照,表明存在复杂的辐照。捕获的N为24 ppm,在Bhuka中观察到的δN-15 = -10.7 +/- 0.8千分之一,比迄今在IAB铁中观察到的范围重。 (C)2016 Elsevier Ltd.保留所有权利。

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