The Late Carboniferous-Early Permian gabbroic complexes of the Alpine belt are commonly ascribed to the extensional tectonics which postdate the Variscan orogeny (Dal Piaz, 1993). The best examples are provided by the Main Gabbro from the Ivrea-Verbano Zone (Quick et al., 1994) and by the Malenco Gabbro (Hermann et al., 1997). However, both Main and Malenco Gabbro have a widespread granulite-facies metamorphic overprint, which does not allow a complete petrological characterization of their igneous features. Very little is known about the Sondalo gabbroic complex of the Languard-Campo nappe (Austroalpine nappe system of Central Alps), although it is volumetrically important (it occupies an area of about 40 km 2) and almost devoid of metamorphic recrystallization. There are no recent studies on its petrogenesis and a determination of the intrusion age is lacking, despite geochronological determinations on adjacent granitoid masses suggesting that the Sondalo gabbroic complex was emplaced in Permian times (Del Moro and Notarpietro, 1987). The Sondalo gabbroic complex is a stock intrusive into high-grade metapelites of the Languard-Campo nappe (Austroalpine nappe system of the Central Alps). The pluton broadly consists of norites and minor troctolites at the core, and diorites and subordinate granodiorites at the rim. The pluton frequently contains xenoliths of granulite-facies restitic rocks and is crosscut by muscovite-bearing pegmatitic to aplitic dykes. This work aims to verify whether the Sondalo gabbroic complex is related to the Alpine gabbroic complexes which postdate the Variscan orogeny. For this purpose, we carried out a petrological study (petrography, major and trace element mineral chemistry, and Nd-Sr-O isotopic compositions) of the troctolite/norite association, thus unraveling the intrusion age, the affinity of the parental liquids and the role of crustal contamination. Combining the data presented with the literature information on the Late Carboniferous-Early Permian gabbroic complexes from the Alpine belt, we give some insights into the origin of the postVariscan magmatism. Troctolitic rocks commonly consist of euhedral to subhedral plagioclase and olivine (Fo = 73-78 mol %), and minor poikilitic clinopyroxene. The variation trend of anorthite content of plagioclase versus the forsterite content of olivine differs from that of arcrelated troctolitic rocks (Beard, 1986) and is similar to that of troctolitic rocks from slow spreadingridges. Noritic rocks are usually composed of euhedral to subhedral plagioclase and orthopyroxene, and minor poikilitic clinopyroxene. Moreover, noritic rocks may contain relatively high percentages of interstial ilmenite and biotite. Both troctolitic and noritic rocks have up to 15 % of titanian pargasite, which occurs as discontinuous rims around mafic minerals or as poikilitic grains. Pyroxenes and Tipargasite from troctolitic rocks have higher Mg, A1 and Cr than those from noritic rocks, whereas plagioclase does not show systematic compositional variations (An about 65 mol %). Plagioclase, pyroxene and Ti-pargasite were analysed for REE and selected trace elements by ion microprobe. Plagioclase shows a regular decrease from LREE to HREE and a marked positive Eu anomaly. Orthopyroxene contains low REE, with a steady increase from LREE to HREE. Clinopyroxene has depleted LREE, negative Eu anomaly and slightly depleted to almost fiat HREE. The REE pattern of titanian pargasite mimics that of the associated clinopyroxene, but at higher abundance levels. Chondrite normalization of incompatible trace elements in Ti-pargasite reveals that K, Ba and Sr (LILE) are slightly depleted relative to LREE, and Nb is commonly enriched relative to K and Ba. The trace element compositions of parental liquids,
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