Petrogenesis of Mediterranean lamproites and associated rocks: The role of overprinted metasomatic events in the post-collisional lithospheric upper mantle

M. Casalini, R. Avanzinelli, S. Tommasini, C. Natali, G. Bianchini, D. Prelević, M. Mattei, S. Conticelli
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引用次数: 11

Abstract

Abstract High-MgO lamproite and lamproite-like (i.e. lamprophyric) ultrapotassic rocks are recurrent in the Mediterranean and surrounding regions. They are associated in space and time with ultrapotassic shoshonites and high-K calc-alkaline rocks. This magmatism is linked with the geodynamic evolution of the westernmost sector of the Alpine–Himalayan collisional margin, which followed the closure of the Tethys Ocean. Subduction-related lamproites, lamprophyres, shoshonites and high-K calc-alkaline suites were emplaced in the Mediterranean region in the form of shallow level intrusions (e.g. plugs, dykes and laccoliths) and small volume lava flows, with very subordinate pyroclastic rocks, starting from the Oligocene, in the Western Alps (northern Italy), through the Late Miocene in Corsica (southern France) and in Murcia-Almeria (southeastern Spain), to the Plio-Pleistocene in Southern Tuscany and Northern Latium (central Italy), in the Balkan peninsula (Serbia and Macedonia) and in the Western Anatolia (Turkey). The ultrapotassic rocks are mostly lamprophyric, but olivine latitic lavas with a clear lamproitic affinity are also found, as well as dacitic to trachytic differentiated products. Lamproite-like rocks range from slightly silica under-saturated to silica over-saturated composition, have relatively low Al2O3, CaO and Na2O contents, resulting in plagioclase-free parageneses, and consist of abundant K-feldspar, phlogopite, diopsidic clinopyroxene and highly forsteritic olivine. Leucite is generally absent, and it is rarely found only in the groundmasses of Spanish lamproites. Mediterranean lamproites and associated rocks share an extreme enrichment in many incompatible trace elements and depletion in High Field Strength Elements and high, and positively correlated Th/La and Sm/La ratios. They have radiogenic Sr and unradiogenic Nd isotope compositions, high 207Pb over 206Pb and high time-integrated 232Th/238U. Their composition requires an originally depleted lithospheric mantle source metasomatized by at least two different agents: (1) a high Th/La and Sm/La (i.e. SALATHO) component deriving from lawsonite-bearing, ancient crustal domains likely hosted in mélanges formed during the diachronous collision of the northward drifting continental slivers from Gondwana; (2) a K-rich component derived from a recent subduction and recycling of siliciclastic sediments. These metasomatic melts produced a lithospheric mantle source characterized by network of felsic and phlogopite-rich veins, respectively. Geothermal readjustment during post-collisional events induced progressive melting of the different types of veins and the surrounding peridotite generating the entire compositional spectrum of the observed magmas. In this complex scenario, orogenic Mediterranean lamproites represent rocks that characterize areas that were affected by multiple Wilson cycles, as observed in the Alpine–Himalayan Realm.
地中海煌斑岩及伴生岩的岩石成因:叠印交代事件在碰撞后岩石圈上地幔中的作用
高镁煌斑岩和类煌斑岩(即煌斑岩)超古生代岩石在地中海及周边地区反复出现。它们在空间和时间上与超经典闪玄岩和高钾钙碱性岩相关。这种岩浆活动与阿尔卑斯-喜马拉雅碰撞边缘最西端的地球动力学演化有关,这是在特提斯洋关闭之后发生的。从渐新世开始,在西阿尔卑斯山(意大利北部),在科西嘉岛(法国南部)和穆尔西亚-阿尔梅里亚(西班牙东南部),在晚中新世,在地中海地区,与俯冲有关的煌斑岩、煌斑岩、闪玄岩和高钾钙碱性套岩以浅侵入体(如塞、脉岩和泥岩)和小体积熔岩流的形式,以非常次级的火山碎屑岩的形式嵌套在地中海地区。到托斯卡纳南部和北拉丁(意大利中部)、巴尔干半岛(塞尔维亚和马其顿)和安纳托利亚西部(土耳其)的普利奥-更新世。超古生代岩石以煌斑岩为主,但也有与煌斑岩有明显亲和关系的橄榄质-乳质熔岩,以及英质-粗质分异产物。类煌石岩成分由硅微欠饱和到硅过饱和,Al2O3、CaO和Na2O含量相对较低,无斜长石,由丰富的钾长石、辉云母、透辉斜辉石和高硅质橄榄石组成。白闪石一般不存在,很少只在西班牙煌斑岩的地块中发现。地中海煌斑岩及其伴生岩具有多种不相容微量元素的极度富集、高场强元素的极度富集、高Th/La和高Sm/La的正相关特征。它们具有放射性Sr和非放射性Nd同位素组成,207Pb高于206Pb, 232Th/238U时间积分高。它们的组成要求原始枯竭的岩石圈地幔源被至少两种不同的因素交代:(1)高Th/La和Sm/La(即SALATHO)成分来自含lawsonite的古老地壳域,可能是在冈瓦纳大陆向北漂移的大陆条状物的跨时碰撞期间形成的msamanlanges中;(2)富钾成分来源于近期的俯冲和硅屑沉积物的再循环。这些交代熔体分别形成了以长英质脉网和富辉云母脉网为特征的岩石圈地幔源。碰撞后的地热调整导致不同类型的脉体和周围的橄榄岩逐渐融化,形成了观测到的岩浆的整个成分谱。在这种复杂的情况下,造山带地中海煌斑岩代表了受多次威尔逊旋回影响的地区的岩石特征,正如在阿尔卑斯-喜马拉雅地区观察到的那样。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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