首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >Chemical studies of L chondrites. V: Compositional patterns for 49 trace elements in 14 L4-6 and 7 LL4-6 falls
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Chemical studies of L chondrites. V: Compositional patterns for 49 trace elements in 14 L4-6 and 7 LL4-6 falls

机译:L球粒陨石的化学研究。 V:14个L4-6和7个LL4-6跌落中49个微量元素的组成模式

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To study compositional trends associated with open-system thermal metamorphism and shock-induced collisional breakup of L4-6 chondrite parent(s), we used inductively coupled plasma mass spectrometry and radiochemical neutron activation analysis to determine 49 trace elements in 62 falls. Trends for the 49 elements, especially of the 14 rare earth elements in 5 members of a putative L/LL group (Bjurbole, Cynthiana, Holbrook, Knyahinya, Sultanpur) and 9 additional L chondrites (Air, Aumieres, Bachmut, Forksville, Kandahar, Kiel, Milean, Narellan, Santa Isabel) differed markedly from those in the remaining normal 46 samples. Here, we report the data for the 14 L and putative L/LL chondrites and 7 LL (Appley Bridge, Athens, Bandong, Ensisheim, Mangwendi, Olivenza, Soko-Banja), analyzed to test the affinity of the putative L/LL suite to well-characterized LL chondrites. Compositional trends of the 14 atypical L chondrites (including Air's unique and possibly contaminated signature) and Mangwendi, an LL6 chondrite, indicate that each is compositionally unrepresentative of well-sampled, whole-rock chondrites. Indeed, half of the unrepresentative chondrites were less than or equal to 2-g samples. Compositionally, members of the putative L/LL chondrites demonstrate no affinities to normal LL chondrite falls. To establish compositional trends accompanying open-system, thermal episodes involving the L chondrite parent(s), we should ignore data for the 14 unrepresentative L chondrites reported here. Copyright (C) 2003 Elsevier Science Ltd. [References: 40]
机译:为了研究与开放系统热变质和L4-6球粒陨石母体撞击引起的碰撞破裂相关的成分趋势,我们使用电感耦合等离子体质谱法和放射化学中子活化分析来确定62个落差中的49个微量元素。推测的L / LL族(Bjurbole,Cynthiana,Holbrook,Knyahinya,Sultanpur)的5个成员中的49种元素,尤其是14种稀土元素的趋势以及另外9种L球粒陨石(空气,Aumieres,Bachmut,Forksville,Kandahar,基尔(Kiel),米兰(Milan),纳雷兰(Narellan),圣伊莎贝尔(Santa Isabel)与其余正常46个样本中的样本有显着差异。在这里,我们报告14 L和假定的L / LL球粒陨石和7 LL(Appley Bridge,雅典,万隆,恩西斯海姆,Mangwendi,Olivenza,Soko-Banja)的数据,以测试假定的L / LL套件的亲和力特有的LL球粒陨石。 14种非典型L球粒陨石(包括Air的独特且可能受到污染的特征)和LL6球粒陨石Mangwendi的成分趋势表明,每种成分在取样充分的全岩石球粒陨石上均不具有代表性。实际上,一半的代表性球粒陨石都小于或等于2克样品。从组成上看,假定的L / LL球粒陨石成员没有表现出对正常LL球粒陨石坠落的亲和力。要建立涉及L球粒陨石父体的开放系统热事件的成分趋势,我们应该忽略此处报告的14种无代表性L球粒陨石的数据。版权所有(C)2003 Elsevier Science Ltd. [引用:40]

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