Evolution of ultrapotassic volcanism on the Kaapvaal craton: deepening the orangeite versus lamproite debate

S. Tappe, Azhar M. Shaikh, Allan H Wilson, A. Stracke
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引用次数: 12

Abstract

Abstract Orangeites are a significant source of diamonds, yet ambiguity surrounds their status among groups of mantle-derived potassic rocks. This study reports mineralogical and geochemical data for a c. 140 Ma orangeite dyke swarm that intersects the Bushveld Complex on the Kaapvaal craton in South Africa. The dykes comprise distinctive petrographic varieties that are linked principally by olivine fractionation, with the most evolved members containing minor amounts of primary carbonate, sanidine and andradite garnet in the groundmass. Although abundant groundmass phlogopite and clinopyroxene have compositions that are similar to those of cratonic lamproites, these phases show notable Ti-depletion, which we consider a hallmark feature of type orangeites from the Kaapvaal craton. Ti-depletion is also characteristic of bulk rock compositions and is associated with strongly depleted Th–U–Nb–Ta contents at high Cs–Rb–Ba–K concentrations. The resultant high large ion lithophile element/high field strength element ratios of orangeites suggest that mantle source enrichment occurred by metasomatic processes in the proximity of ancient subduction zones. The Bushveld-intersecting orangeite dykes have strongly enriched Sr–Nd–Hf isotopic compositions (initial 87Sr/86Sr = 0.70701–0.70741; εNd = −10.6 to −5.8; εHf = −14.4 to −2.5), similar to those of other orangeites from across South Africa. Combined with the strong Ti–Nb–Ta depletion, this ubiquitous isotopic feature points to the involvement of ancient metasomatized mantle lithosphere in the origin of Kaapvaal craton orangeites, where K-rich metasomes imparted a ‘fossil’ subduction geochemical signature. Previous geochronology studies identified ancient K-enrichment events within the Kaapvaal cratonic mantle lithosphere, possibly associated with collisional tectonics during the 1.2–1.1 Ga Namaqua–Natal orogeny of the Rodinia supercontinent cycle. It therefore seems permissible that the cratonic mantle root was preconditioned for ultrapotassic magma production by tectonomagmatic events that occurred along convergent plate margins during the Proterozoic. However, reactivation of the K-rich metasomes had to await establishment of an extensional tectonic regime, such as that during the Mesozoic breakup of Gondwana, which was accompanied by widespread (1000 × 750 km) small-volume orangeite volcanism between 200 and 110 Ma. Although similarities exist between orangeites and lamproites, these and other potassic rocks are sufficiently distinct in their compositions such that different magma formation processes must be considered. In addition to new investigations of the geodynamic triggers of K-rich ultramafic magmatism, future research should more stringently evaluate the relative roles of redox effects and volatile components such as H2O–CO2–F in the petrogeneses of these potentially diamondiferous alkaline rocks.
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卡普瓦尔克拉通的超古典纪火山活动演化:加深了橘岩与煌斑岩之争
橙岩是钻石的重要来源,但其在地幔钾质岩石群中的地位尚不明确。本研究报告了在南非Kaapvaal克拉通上与Bushveld杂岩相交的约140 Ma的橙色岩脉群的矿物学和地球化学数据。这些岩脉由不同的岩相组成,主要由橄榄石分馏作用联系在一起,最演化的岩脉在地质体中含有少量的原生碳酸盐、生辉石和角闪石石榴石。虽然丰富的陆块辉云母和斜辉石的组成与克拉通煌斑岩相似,但这些相均表现出明显的ti亏缺,这是卡普瓦尔克拉通型橙色岩的标志特征。ti亏缺也是大块岩石组成的特征,并与高Cs-Rb-Ba-K浓度下Th-U-Nb-Ta含量的强烈亏缺有关。由此产生的大离子亲石元素/高场强元素比值表明,在古俯冲带附近,地幔源富集是通过交代作用发生的。与bushveld相交的橙长岩岩脉具有强烈富集的Sr-Nd-Hf同位素组成(初始87Sr/86Sr = 0.70701-0.70741;εNd =−10.6 ~−5.8;εHf = - 14.4 ~ - 2.5),与来自南非各地的其他橙猿相似。结合强烈的Ti-Nb-Ta枯竭,这种普遍存在的同位素特征表明,古代交代地幔岩石圈参与了Kaapvaal克拉通橙色岩的起源,其中富含k的交代体赋予了“化石”俯冲的地球化学特征。先前的地质年代学研究确定了Kaapvaal克拉通地幔岩石圈内的古代k富集事件,可能与Rodinia超大陆旋回的1.2-1.1 Ga Namaqua-Natal造山运动期间的碰撞构造有关。因此,元古代沿收敛的板块边缘发生的构造岩浆事件似乎为克拉通地幔根的超古典岩浆的产生提供了先决条件。然而,富钾变质体的重新激活必须等待伸展构造制度的建立,例如在中生代冈瓦纳破裂期间,伴随着200至110 Ma之间广泛的(1000 × 750 km)小体积的橙色火山活动。虽然在橙辉岩和煌斑岩之间存在相似之处,但这些和其他钾质岩石在成分上有足够的区别,因此必须考虑不同的岩浆形成过程。除了对富钾超镁铁质岩浆活动的地球动力学成因进行新的研究外,未来的研究还应更严格地评估氧化还原效应和挥发性组分(如H2O-CO2-F)在这些潜在含金刚石碱性岩石成岩作用中的相对作用。
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