2012
DOI: 10.3809/jvirtex.2011.00287
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Multiscale structural analysis in the subducted continental crust of the internal Sesia-Lanzo Zone (Monte Mucrone, Western Alps)

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Cited by 10 publications
(26 citation statements)
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“…In all rock types, blueschist-facies mineral assemblages (Table 3) define S2. This finding is in contrast with the nearby metaintrusive of M. Mucrone, where eclogitic mineral assemblages mark the pervasive fabric (Delleani et al, 2012;Delleani et al, 2013;Zucali et al, 2002). Thus, different FE and MT would have affected the retrograde blueschist re-equilibration and potentially generated km-scale heterogeneities within the EMC.…”
Section: Resultscontrasting
confidence: 53%
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“…In all rock types, blueschist-facies mineral assemblages (Table 3) define S2. This finding is in contrast with the nearby metaintrusive of M. Mucrone, where eclogitic mineral assemblages mark the pervasive fabric (Delleani et al, 2012;Delleani et al, 2013;Zucali et al, 2002). Thus, different FE and MT would have affected the retrograde blueschist re-equilibration and potentially generated km-scale heterogeneities within the EMC.…”
Section: Resultscontrasting
confidence: 53%
“…For instance, in the nearby area of M. Mucrone the correlation between FE and MT shows that the dominant tectono-metamorphic imprint is related to high degree of FE and MT (Delleani et al, 2012;Delleani et al, 2013;Zucali et al, 2002). Similar results have been also obtained in the Mont Morion complex of the Dent Blanche nappe (Roda & Zucali, 2008) and in the LanguardTonale unit in the central Austroalpine domain .…”
Section: Resultsmentioning
confidence: 99%
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“…The Biella pluton, which is also known as the Valle del Cervo pluton, shows a concentric zoning in which the outer part consists of monzonite grading to syenite and the inner part consists of granite (Bigioggero et al, 1994 and references therein). The Biella and Traversella plutons are 30 Ma Bigioggero et al, 1994;Krummenacher & Evernden, 1960;Romer et al, 1996) and are emplaced in the internal Sesia-Lanzo Zone of the western Austroalpine domain (Figure 1(b)), which shows a pervasive structural imprint under eclogite facies conditions (Delleani, Spalla, Castelli, & Gosso, 2012, 2013Giorgetti, Tropper, Essene, & Peacor, 2000;Koons, 1986;Rubbo, Borghi, & Compagnoni, 1999;Tropper & Essene, 2002;Tropper, Essene, Sharp, & Hunziker, 1999;Zucali, 2002;Zucali & Spalla, 2011;Zucali, Spalla, & Gosso, 2002) dated 60 -80 Ma (Bussy, Venturini, Hunziker, & Martinotti, 1998;Cenki-Tok et al, 2011;Roda, Spalla, & Marotta, 2012;Rubatto, Gebauer, & Compagnoni, 1999;Rubatto et al, 2011) and related to the Alpine subduction. The Sesia-Lanzo Zone preserves scattered granulite to amphibolite facies relicts, which are related to Permian-Triassic lithospheric thinning that predates the Alpine convergence (Cenki-Tok et al, 2011;Lardeaux & Spalla, 1991;Rebay & Spalla, 2001;Spalla et al, 2014).…”
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confidence: 99%