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首页> 外文期刊>Chemical geology >Noble gases in spinel peridotite xenoliths from Mt Quincan, North Queensland,Australia: Undisturbed MORB-type noble gases in the subcontinentallithospheric mantle
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Noble gases in spinel peridotite xenoliths from Mt Quincan, North Queensland,Australia: Undisturbed MORB-type noble gases in the subcontinentallithospheric mantle

机译:来自澳大利亚北昆士兰州昆坎山的尖晶石橄榄岩异质岩中的稀有气体:大陆下岩石圈地幔中不受干扰的MORB型稀有气体

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摘要

Noble gas elemental and isotopic compositions have been determined for a suit of fresh spinel peridotitexenoliths from Mt Quincan, North Queensland (Northeast Australia). The observed helium, argon and xenonisotopic compositions are very similar to those reported for mid-ocean ridge basalts (MORB) in that theyhave following features: (1) ~3He/ ~4He ratios covering a narrow range from 8 Ra to 10 Ra, (2) ~(40)Ar/~(36)Ar (300-4000) and the ~3He/~(36)Ar (0.0012-0.07; corrected for some recent elemental fractionation) values that plot onthe well-established MORB line, and (3) correlated excesses in ~(129)Xeand ~(136)Xewith regard to atmosphericxenon. MORB-like noble gas compositions suggest fluids ultimately derived from the asthenopshere are present inthe subcontinental lithospheric mantle beneath northeastern Australia. The absence of any subduction-related noble gas signature precludes the preservation of fluids in the xenoliths added during Paleozoicsubduction at the eastern margin of Australia. We also note that there is no mantle plume noble gas signaturefound in the Mt Quincan xenoliths, despite its location close to the suspected hotspot track across easternAustralia. These features are consistent with Sr and Nd isotopic characteristics of Mt Quincan xenoliths[Handler, M.R., Bennett, V.C., Carlson, R.W. 2005. Nd, Sr and Os isotope systematics in young, fertile peridotitexenoliths from northern Queensland, Australia: A unique view of depleted MORB mantle? Geochim.Cosmochim. Acta 69, 5747-5763.]. Thus, the fluid-entrapment is likely associated with subsequent riftingtectonic settings when asthenospheric fluid (and magma) could rise into the subcontinental lithosphericmantle and was able to overwrite any pre-existing signatures or even replace it with "MORB"-like mantle byphysical removal of previously metasomatised lithospheric mantle. Additionally, differing from noble gascompositions previously considered typical for the subcontinental lithospheric mantle, the north Queenslanddata highlight the existence of noble gas isotopic heterogeneity in the subcontinental lithospheric mantle ona global scale.
机译:已经确定了来自北昆士兰山(澳大利亚东北部)昆坎山的新鲜尖晶石橄榄石钛岩的一套稀有气体元素和同位素组成。观测到的氦,氩和氙同位素组成与中洋脊玄武岩(MORB)的报告非常相似,因为它们具有以下特征:(1)〜3He /〜4He比涵盖从8 Ra到10 Ra的狭窄范围,( 2)绘制在完善的MORB线上的〜(40)Ar /〜(36)Ar(300-4000)和〜3He /〜(36)Ar(0.0012-0.07;已针对某些最近的元素分馏进行校正)值, (3)将〜(129)Xe和〜(136)Xe与大气氙相关的过量相关联。 MORB状的稀有气体成分表明,最终来自软熔岩的流体存在于澳大利亚东北部以下的亚大陆岩石圈地幔中。没有任何与俯冲有关的稀有气体特征,排除了在澳大利亚东部边缘古生代俯冲过程中添加的异岩中流体的保留。我们还注意到,尽管昆卡山异岩中的地幔柱稀有气体没有发现,但其位置靠近整个澳大利亚东部的疑似热点。这些特征与金坎山异岩的Sr和Nd同位素特征一致[Handler,MR,Bennett,VC,Carlson,RW2005。来自澳大利亚昆士兰州北部的年轻肥沃的橄榄石钛岩中的Nd,Sr和Os同位素系统:耗尽的MORB地幔? Geochim.Cosmochim。 Acta 69,5747-5763。]。因此,当软流圈流体(和岩浆)可能上升到次大陆岩石圈地幔中并能够覆盖任何先前存在的特征,或者通过物理去除地幔中的“ MORB”状地幔时,流体包裹可能与随后的裂陷构造环境有关。先前已被交代的岩石圈地幔。此外,与先前认为的次大陆岩石圈地幔典型的稀有气体成分不同,昆士兰北部的数据突出显示了全球范围内次大陆岩石圈地幔中稀有气体同位素异质性的存在。

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