首页> 外文期刊>Journal of geophysical research. Solid earth: JGR >Magnetic petrology of variably retrogressed eclogites and amphibolites: A case study from the Hercynian basement of northern Sardinia (Italy)
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Magnetic petrology of variably retrogressed eclogites and amphibolites: A case study from the Hercynian basement of northern Sardinia (Italy)

机译:易退变的榴辉岩和角闪石的磁性岩石学:以撒丁岛(意大利)北部海西基底为例

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This study constitutes the first attempt to integrate rock magnetism and metamorphic petrology in the Hercynian basement of northern Sardinia. The investigation focused on the magnetic petrology of variably retrogressed eclogites and amphibolites from two suites of basic meta-igneous rocks, which occur along a major tectonic line (Posada-Asinara Line), within a medium-grade (MG) and a high-grade (HG) metamorphic complex. Consistent with petromagnetic results, HG metabasites contain variable amounts of monoclinic pyrrhotite (intergrown with rutile) and titanomagnetite (occurring as inclusions in garnet), abundant ilmenite (associated to secondary hornblende and with sphene ± low-Ti-magnetite rims), and rutile both as inclusions in ilmenite and as discrete grains. In MG metabasites, pyrrhotite is restricted to amphibolites of the Posada Valley area where it occurs as rare inclusions in garnet. All samples are characterized by variable amounts of ilmenite, rutile, and sphene which show the same microstructural features described in HG rocks. Microstructural evidence and geothermobarometric data indicate that (1) pyrrhotite and titanomagnetite likely formed prior to and remained stable during the eclogite facies metamorphic peak and (2) the growth of ilmenite and sphene can be attributed to the amphibolite facies retrogression, mainly due to model reactions such as garnet + omphacite + rutile + H2O → hornblende + plagioclase + ilmenite and amphibole + ilmenite + O2 → sphene + magnetite + quartz + H2O. The results from our combined petrological and petromagnetic study corroborate the hypothesis that significant volumes of mafic/ultramafic rocks, similar to some of the investigated outcrops, may account for the magnetic anomalies flanking the northeastern part of the Posada-Asinara Line.
机译:这项研究是在撒丁岛北部海西基底中整合岩石磁性和变质岩石学的首次尝试。研究的重点是来自两套基本的亚火成岩的可变退变的榴辉岩和角闪岩的磁岩石学,这些岩屑沿着中构造(MG)和高构造的主要构造线(波萨达-阿西纳拉线)发生。 (HG)变质复合物。与铁磁结果一致,HG变质岩中含有不同数量的单斜晶黄铁矿(与金红石共生)和钛磁铁矿(石榴石中的夹杂物),丰富的钛铁矿(与次生角闪石有关,并具有镜面±低Ti-磁铁矿边缘),并且都金红石作为钛铁矿中的夹杂物和不连续的晶粒。在MG阶地中,黄铁矿仅限于Posada谷地区的闪石,在石榴石中以稀有夹杂物的形式出现。所有样品的特征都在于可变数量的钛铁矿,金红石和蝶粉,它们显示出与HG岩石中描述的相同的微观结构特征。微观结构证据和地热气压数据表明,(1)黄铁矿和钛磁铁矿可能在榴辉岩相变质峰形成之前形成并保持稳定;(2)钛铁矿和蝶粉的生长可归因于闪石相的倒退,这主要是由于模型反应引起的例如石榴石+绿沸石+金红石+ H2O→角闪石+斜长石+钛铁矿和闪石+钛铁矿+氧气→+磁铁矿+石英+ H2O我们的岩石学和岩磁研究相结合的结果证实了以下假说:大量的镁铁质/超镁铁质岩石(与某些已调查的露头相似)可能解释了Posada-Asinara线东北侧的磁异常。

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