Abstract

At Arvogno, Vigezzo valley in the Central Alps, Italy, pegmatite dikes are unique in the scenario of a tertiary alpine pegmatite field because they show marked geochemical and mineralogical niobium–yttrium–fluorine features. These pegmatites contain AB2O6 aeschynite group minerals and ABX2O8 euxenite group minerals as typical accessory minerals including aeschynite-(Y), polycrase-(Y), and samarskite-(Y). They are associated with additional typical minerals such as fluorite, Y-dominant silicates, and xenotime-(Y). The Y–Nb–Ti–Ta AB2O6 and ABX2O8 oxides at the Arvogno pegmatites did not exhibit any textural and compositional features of oxidation or weathering. They are characterized by low self-radiation-induced structural damage, leading to the acquisition of unit-cell data for aeschynite-(Y), polycrase-(Y), and samarskite-(Y) by single-crystal X-ray diffraction. Aeschynite-(Y) and polycrase-(Y) crystals allowed for both to provide space groups whereas samarskite-(Y) was the first crystal from pegmatites for which cell-data were obtained at room temperature but did not allow for the accurate determination of the space group. According to the chemical compositions defined by Ti-dominant content at the B-site, the cell parameters, respectively, corresponded to polycrase-(Y), aeschynite-(Y), and the monoclinic cell of samarskite-(Y). Emplacement of Alpine pegmatites can be related to the progressive regional metamorphic rejuvenation from east to west in the Central Alps, considering the progressive cooling of the thermal Lepontine Barrovian metamorphic dome. Previous studies considered magmatic pulses that led to emplace the pegmatite field in the Central Alps. As an example, the pegmatites that intruded the Bergell massif were aged at 28–25 millions of years or younger, around 20–22 m.y.

Highlights

  • Complex rare-earth elements (REEs)–Nb–Ta–Ti oxides are uncommon but locally important accessory phases occurring typically in the NYF family and REL–REE class

  • Aeschynite- and euxenite-group minerals have a general formula AB2 O6 where the eight-fold coordinated A-site, a square antiprism, is occupied by Y, REE, Ca, U, Th, Fe, while the six-fold coordinated B-site has a typical octahedra to form double chains in a zigzag pattern along the b-axis [2] occupied by Ti, Nb, Ta. and W

  • This study revealed that coexistent Y–Nb–Ti–Ta oxides from the Arvogno pegmatites are characterized by very low radiation damage [20,21,22] disregarding the rather high concentrations of U and Th, and it allowed to obtain the crystallographic determination by SCXRD at room temperature, as well as a Raman spectroscopy study for aeschynite-(Y), polycrase-(Y), and samarskite-(Y)

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Summary

Introduction

Complex REE–Nb–Ta–Ti oxides (aeschynite-, euxenite-, and samarskite-group minerals) are uncommon but locally important accessory phases occurring typically in the NYF (niobium, yttrium, fluorine) family and REL–REE (rare-element and rare earths) class (as per the listed pegmatites of allanite-, euxenite-, and gadolinite-type by Černý and Ercit [1]). Aeschynite- and euxenite-group minerals have a general formula AB2 O6 where the eight-fold coordinated A-site, a square antiprism, is occupied by Y, REE, Ca, U, Th, Fe, while the six-fold coordinated B-site has a typical octahedra to form double chains in a zigzag pattern along the b-axis [2] occupied by Ti, Nb, Ta. and W. Minerals 2019, 9, x FOR PEER REVIEW (AGMs) and in euxenite-group minerals are[2]orthorhombic, butNb, the Ta. BO6and stacking form double chains a zigzag pattern along (EGMs) the b-axis occupied by Ti, W. octahedra is different, leading to the. Pbcn space group in EGMs. Aeschynite-group minerals (AGMs) and euxenite-group minerals (EGMs) are orthorhombic, but the Historically, samarskite-group minerals have general formula antoα-PbO. BO6 stacking octahedra is different, leading to the Pbnm space group ABO in AGMs and the Pbcn space.

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