...
首页> 外文期刊>Meteoritics & planetary science >QUE 94204: A primitive enstatite achondrite produced by the partial melting of an E chondrite-like protolith
【24h】

QUE 94204: A primitive enstatite achondrite produced by the partial melting of an E chondrite-like protolith

机译:QUE 94204:一种原始的顽辉石陨石,是通过部分熔化类似E球粒陨石的原石而产生的

获取原文
获取原文并翻译 | 示例

摘要

Queen Alexandra Range (QUE) 94204, an enstatite achondrite, is a coarse-grained, highly recrystallized, chondrule-free and unbrecciated rock dominated (about 70vol%) by anhedral, equigranular crystals of orthoenstatite of nearly endmember composition (Fs_(0.1-0.4), Wo_(0.3-0.4)) with interstitial plagioclase, kamacite, and troilite. Abundance of approximately 120° triple junctions and the close association of metal-sulfide and plagioclase-rich melts indicate that QUE 94204 has undergone limited partial melting with inefficient melt extraction. Mineral chemistry indicates a high degree of thermal metamorphism. Kamacite in QUE 94204 contains between 2.09 and 2.55wt% Si, similar to highly metamorphosed EL chondrites. Plagioclase has between 4.31 and 6.66wt% CaO, higher than other E chondrites but closer in composition to plagioclase from metamorphosed EL chondrites. QUE 94204 troilite contains up to 2.55wt% Ti, consistent with extensive thermal metamorphism of an E chondrite-like precursor. Results presented in this study indicate that QUE 94204 is the result of low degree, (about 5-20vol%, probably toward the lower end of this range) partial melting of an E chondrite protolith. Textural and chemical evidence suggests that during the metamorphism of QUE 94204, melts formed first at the Fe,Ni-FeS cotectic near approximately 900°C, followed by plagioclase-pyroxene silicate partial melts near approximately 1100°C. Neither the Fe,Ni-FeS nor the plagioclase-pyroxene melts were efficiently segregated or extracted. QUE 94204 belongs to a grouplet of similar "primitive enstatite achondrites" that are analogous to the acapulcoites-lodranites, but that have resulted from the partial melting of an E chondrite-like protolith.
机译:亚历山德拉皇后山脉(QUE)94204,一种顽辉长晶陨石,是一种粗晶,高度重结晶,无球粒且未结块的岩石,主要成分为(约70vol%)角正石的近端成员组成的正钙长石的反面,等粒晶体(Fs_(0.1-0.4 ),Wo_(0.3-0.4))以及间质斜长石,高岭石和三叶草。大约120°的三重结的丰度以及金属硫化物和富含斜长石酶的熔体的紧密结合表明QUE 94204已经历了有限的部分熔解,熔体提取效率低下。矿物化学表明高度的热变质作用。 QUE 94204中的Kamacite含有2.09至2.55wt%的Si,类似于高度变质的EL球粒陨石。斜长石具有的CaO在4.31至6.66wt%之间,高于其他E球粒陨石,但其组成更接近于由变质的EL球粒石形成的斜长石。 QUE 94204闪锌矿包含高达2.55wt%的Ti,这与E球粒状前体的广泛热变质相一致。这项研究给出的结果表明,QUE 94204是E球粒陨石原石低度熔融(约5-20vol%,可能接近该范围的下限)的结果。组织和化学证据表明,在QUE 94204的变质过程中,首先在大约900°C附近的Fe,Ni-FeS共晶处形成熔体,然后在大约1100°C附近形成斜长石-py-硅酸盐硅酸盐。 Fe,Ni-FeS或斜长石-辉石熔体均无法有效地分离或萃取。 QUE 94204属于一组相似的“原始顽辉石陨石”,类似于链长石-菱锰矿,但是由于E球粒陨石样原石的部分熔化而导致的。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
获取原文

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号