首页> 外文期刊>Indian Minerals >PETROGRAPHY AND PETMGCHEMISTEY OF IMPACT MELTS FROM LONAR CRATER, BULDANA DISTRICT, MAHARASHTRA, INDIA
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PETROGRAPHY AND PETMGCHEMISTEY OF IMPACT MELTS FROM LONAR CRATER, BULDANA DISTRICT, MAHARASHTRA, INDIA

机译:印度马哈拉施特拉邦布达纳地区隆纳尔克拉特的撞击熔体的岩石学和岩石化学

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The Lonar crater in Buldana district, Maharashtra has long been established as the largest hypervelocity impact crater of the world on Deccan basalt flows, although no extraterrestrial fragment could be located from geological, geophysical, geochemical and drilling approach. Considering the impact origin, the crater was revisited with an aim to throw light on the nature of target rocks and its impact melts. The country rock, prior to the extra-terrestrial impact, has been distinguished as a slightly oversaturated continental tboleiitic basalt with a distinct chemical signature. It is low in iroe and alkali and relatively high in magnesia compared to mean composition of Deccan basalt. Some amount of variation has been indicated by Cr, Ni, V, TH and Ta in relation to Mg No.. Petrogenetically, it has been identified as a secondary basaltic (less evolved) magma (Mg No. 54.7) of more subalkaline nature (alkalinity=1.39). Neither pyroxene-nor fractionation has fractionation has played any significant role in the magmatic evolution as indicated from texture and petrochemistry including the REE fractionation pattern. Petrochemistry of the glass ejecta (impact melt) and throw-out basaltic fragments do not reveal much significant change in their bulk composition from that of basalts of the area except some shock-induced optical features. Lonar impact melt exhibits flow banding and contortions along with vesicles of varying size, shape and proportions. Evidence recorded in the target rock as well as in glass indicates both equilibrium and non-equilibrium shock pressure upto more than 1000 kb. Available major minor- and trace-element chemistry of the impact melt when compared to that of target rock reveals that the release of high-magnitude volatile flux in plasma state from the projectile during the impact has caused heterogeneities in melt composition and dispersal of the plagioclase fraction-enriched component of the impact melt.
机译:长期以来,马哈拉施特拉邦博尔达纳地区的月球陨石坑一直被认为是世界上最大的对Deccan玄武岩流产生超高速撞击的陨石坑,尽管从地质,地球物理,地球化学和钻探方法中都无法找到外星碎片。考虑到撞击的起源,对陨石坑进行了重新研究,目的是阐明目标岩石的性质及其撞击融化。在受到地外冲击之前,该乡村岩石已被识别为略带饱和的陆生玄武质玄武岩,具有独特的化学特征。与Deccan玄武岩的平均组成相比,它的硫和碱含量较低,而镁的含量较高。 Cr,Ni,V,TH和Ta相对于Mg.No.指示出一定程度的变化。从岩石成因上,它被确定为次碱性的次生玄武岩(演化较少的)岩浆(Mg.No. 54.7)(碱度= 1.39)。如质地和石油化学(包括REE分级模式)所示,辉石-nor分级分离均未在岩浆演化中发挥任何重要作用。除了一些震动诱发的光学特征外,玻璃射出物(撞击熔体)和抛出的玄武岩碎片的石化与该地区的玄武岩相比,其本体组成没有显着变化。月球撞击熔体显示出流带和扭曲以及大小,形状和比例不同的囊泡。在目标岩石以及玻璃中记录的证据表明,平衡和非平衡冲击压力均超过1000 kb。与目标岩石相比,冲击熔体的可用主要微量元素和微量元素化学性质表明,在冲击过程中,从弹丸中释放出的等离子态高强度挥发性通量已引起熔体成分的异质性和斜长石的扩散冲击熔体中富含馏分的组分。

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