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首页> 外文期刊>Geochimica et Cosmochimica Acta: Journal of the Geochemical Society and the Meteoritical Society >Source, genesis, and timing of giant ignimbrite deposits associated with Ethiopian continental flood basalts [Review]
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Source, genesis, and timing of giant ignimbrite deposits associated with Ethiopian continental flood basalts [Review]

机译:与埃塞俄比亚大陆性洪水玄武岩有关的巨大火成岩沉积物的来源,成因和时间[综述]

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摘要

The Ethiopian continental flood basalt (CFB) province (similar to30 Ma, > 3 x 10(5) km(3)) was formed as the result of the impingement of the Afar mantle plume beneath the Ethiopian lithosphere. This province includes major sequences of rhyolitic ignimbrites generally found on top of the flood basalt sequence. Their volume is estimated to be at least 6 x 10(4) km(3), which represents 20% of that of the trap basalts. Their phenocryst assemblage (alkali feldspar, quartz, aegyrine-augite, ilmenite +/- Ti-magnetitc, richterite, and eckermanite) suggests temperatures in the range of 740 to 900degreesC. Four units were recognized in the field (Wegel Tena, Jima, Lima Limo, and Debre Birhan areas), each with its own geochemical specificity. Zr/Nb ratios remain constant between basalt and rhyolite in each area, and rhyolites associated with high-Ti or low-Ti basalts are, respectively, enriched or depleted in titanium. Their trace element and isotope (Sr, Nd, O) signatures (high Nd-143/Nd-144 and low Sr-87/Sr-86 ratios, compared to those of rhyolites from other CFB provinces) are clearly different from those of typical crustal melts and indicate that the Ethiopian rhyolites are among the most isotopically primitive rhyolites. Their major and trace element patterns suggest that they are likely to be derived from fractional crystallization of basaltic magmas similar in composition to the exposed flood basalts with only limited crustal contribution. Since Ethiopian high-Ti basalts have been shown to form from melting of a mantle plume, it is likely that Ethiopian ignimbrites, at least those that are Ti-rich, also incorporated material from the deep mantle. Rb-Sr isochrons on whole rocks and mineral separates (30.1 +/- 0.4 Ma for Wegel Tena and 30.5 +/- 0.4 Ma for Jima ignimbrites) show that most of the silicic volcanism occurred within < 2 Ma during the Oligocene. Ignimbritic eruptions resumed in the Miocene during two episodes dated at 15.4 +/- 0.2 Ma and 8.0 +/- 0.2 Ma for the Debre Birhan area. The Rb-Sr isochron ages of ignimbrites (both Oligocene and Miocene rhyolites) are indistinguishable within uncertainties from the Ar-40/Ar-39 ages of the underlying flood basalts. The Oligocene ignimbrites and the underlying trap basalts are synchronous with a shift in the oxygen composition of foraminifera recorded in Indian and Atlantic Ocean cores. The temporal coincidence of Ethiopian Oligocene volcanism, which released immense volumes of S (> 1.4 x 10(15) mol) and Cl (6.4 x 10(15) mol) into the atmosphere over a short time span, with the global cooling event at 30.3 Ma suggests that this volcanism might have accelerated the climate change that was already underway. Copyright (C) 2002 Elsevier Science Ltd. [References: 114]
机译:埃塞俄比亚大陆洪水玄武岩(CFB)省(类似于30 Ma,> 3 x 10(5)km(3))是由于埃塞俄比亚岩石圈下方的Afar地幔柱撞击而形成的。该省包括流纹玄武岩的主要层系,通常在洪水玄武岩层系之上。它们的体积估计至少为6 x 10(4)km(3),占圈闭玄武岩体积的20%。他们的隐晶石组合(碱金属长石,石英,aegyrine-augite,钛铁矿+/- Ti-磁铁矿,富钛矿和埃克锰矿)的温度范围为740至900℃。该领域共有四个单位(韦格尔·泰纳(Wegel Tena),吉马(Jima),利马·利莫(Lima Limo)和德布勒·伯罕(Debre Birhan)地区),每个单位都有其自身的地球化学特异性。 Zr / Nb比在每个区域的玄武岩和流纹岩之间保持恒定,并且与高Ti或低Ti玄武岩相关的流纹岩分别富含钛或贫钛。它们的痕量元素和同位素(Sr,Nd,O)特征(与来自其他CFB省的流纹岩相比,高Nd-143 / Nd-144和低Sr-87 / Sr-86比率)明显不同于典型地壳融化,表明埃塞俄比亚流纹岩属于同位素最原始的流纹岩。它们的主要元素和痕量元素模式表明,它们很可能源自玄武岩浆的分步结晶,其组成与裸露的玄武岩相似,地壳贡献有限。由于已显示埃塞俄比亚的高Ti玄武岩是由地幔柱的融化形成的,因此埃塞俄比亚的火成岩(至少是富含Ti的那些)也可能结合了深地幔的物质。整个岩石和矿物分离层上的Rb-Sr等时线(Wegel Tena为30.1 +/- 0.4 Ma,Jima火山岩为30.5 +/- 0.4 Ma)表明,大多数硅质火山岩发生在渐新世<2 Ma内。在中新世期间,在德布瑞米尔伯罕地区的两次发作分别在15.4 +/- 0.2 Ma和8.0 +/- 0.2 Ma期间恢复了火成岩喷发。火成岩(渐新世和中新世流纹岩)的Rb-Sr等时年龄与潜在洪泛玄武岩的Ar-40 / Ar-39年龄在不确定性上是无法区分的。渐新世的火成岩和下伏的捕集玄武岩与印度和大西洋中心有孔虫的氧气组成变化同步。埃塞俄比亚渐新世火山的时间重合,在短时间内向大气释放了大量S(> 1.4 x 10(15)mol)和Cl(6.4 x 10(15)mol)的气体,全球降温事件为30.3 Ma认为,这种火山作用可能加速了已经在发生的气候变化。版权所有(C)2002 Elsevier ScienceLtd。[参考:114]

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