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Reconciling P–T–d evolution and structural architecture in the Dora-Maira Massif (Western Alps): insights from the Permo–Mesozoic cover sequences

Published online by Cambridge University Press:  12 October 2026

Davide Dana*
Affiliation:
Dipartimento di Scienze della Terra, Università di Torino, Italy
Francesco De Cesari
Affiliation:
Dipartimento di Scienze della Terra, Università di Torino, Italy
Salvatore Iaccarino
Affiliation:
Dipartimento di Scienze della Terra, Università di Torino, Italy
Chiara Montomoli
Affiliation:
Dipartimento di Scienze della Terra, Università di Torino, Italy
Alberto Corno
Affiliation:
Institute of Geosciences, CNR-GEO National Research Council of Italy, Italy
Daniela Rubatto
Affiliation:
Geological Sciences, University of Bern, Switzerland ISTE, University of Lausanne, Switzerland
Alessandro Borghi
Affiliation:
Dipartimento di Scienze della Terra, Università di Torino, Italy
Rodolfo Carosi
Affiliation:
Dipartimento di Scienze della Terra, Università di Torino, Italy
*
Corresponding author: Davide Dana; Email: davide.dana@unito.it
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Abstract

The structural and metamorphic architecture of the Dora-Maira Massif has traditionally been interpreted as a stack of multiple tectonic slices, distinguished primarily on P–T peak conditions. New structural, lithostratigraphic and petrological data from the Permo–Mesozoic cover sequences of the northern-central Dora-Maira Massif allow a reassessment of the tectonic slices. Detrital zircon U-Pb geochronology constrains the Permian depositional age of garnet-chloritoid micaschist within the cover sequence, allowing a more robust reconstruction of the original extent and stratigraphic continuity of the sequence. Structural and petrological analyses show that both the Permo–Mesozoic cover and the underlying basement share the same Alpine P–T–d evolution, reaching ultra-high-pressure (UHP) conditions in the coesite-chloritoid-facies (530–560°C and 2.6–2.9 GPa). Newly identified coesite relicts support peak conditions inferred from thermodynamic modelling. Consequently, any significant detachment of cover from basement occurred after the Alpine metamorphic peak. Field mapping and geochronological constraints document a discontinuous Permian–Upper Cretaceous succession occurring either as deformed slices folded with the basement rocks or as partially detached slivers along the tectonic contact with the oceanic units. These results support a reinterpretation of the Dora-Maira Massif architecture and allow the merging of several previously defined small units into a single tectono-metamorphic unit. More broadly, our data suggest that basement–cover associations represent a key criterion for reconstructing the tectonic architecture of the Dora-Maira Massif. On this basis, and through comparison with existing studies, we propose a revised structural framework for the entire massif that reconciles field relationships with the wider extent of Alpine UHP metamorphism.

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Original Article
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© The Author(s), 2026. Published by Cambridge University Press
Figure 0

Figure 1. Figure 1 long description.Tectonic sketch of the Western Alps, modified from Dana (2024). Abbreviations: DM = Dora-Maira, GP = Gran Paradiso, MR = Monte Rosa, PFT = Penninic Frontal Thrust, PFS = Periadriatic Fault System. Red box represents the study area of Figure 2.

Figure 1

Figure 2. (a) Simplified geological map of the study area (Western border of the Dora-Maira Massif between the Pellice and Chisone valleys), based on original field mapping for the Geological Map of Italy, Sheet “172 Pinerolo” and this work. The dashed lines indicate the tectonic contacts between the Serre, Muret and Chasteiran units as proposed by Nosenzo et al. (2024) and re-interpreted in this work. Note that previous authors did not map cover rocks (i.e. their Serre Unit) in the Salza di Pinerolo area, and their Serre Unit terminates at Villa di Prali. La Fracho Shear Zone (LFSZ) of Nosenzo et al. (2024) is drawn as a fault left of Col Clapier locality because, according to this study, this structure is a late fault (see main text). Red lines indicate nappe boundary as proposed in this study and partly in Nosenzo et al. (2024). (b) Tentative reconstruction of the Permo–Mesozoic cover sequence, integrating our new field observations with those of Caron (1977), Marthaler et al. (1986) and Nosenzo et al. (2024).

Figure 2

Table 1. Summary of representative samples selected for this studyTable 1 long description.

Figure 3

Figure 3. Figure 3 long description.(a) Fontane micaschist (sample DD20), characterized by sigmoidal lenses composed of chloritoid ± white mica and ankerite pods. (b) Detail of a Fontane micaschist with small orange ankerite pods. (c) Association between Fontane micaschist and Luserna orthogneiss; garnet-chloritoid-bearing micaschist are folded together with the orthogneiss in thin, centimetre-scale layers. (d) Typical meta-dolostone showing alternating whitish and bluish layers. (e) Grey-blue sandy marble containing deformed blue clasts (arrows) within a meta-calcarenitic matrix, wrapped by the main foliation. (f) Folded and deformed cover sequence in the Subiasco area (Pellice Valley area), preserved as a lens pinched within the core of a synformal structure. (g) Omission of Triassic–Jurassic carbonate-bearing rocks, with calcschist directly in contact with Fontane micaschist.

Figure 4

Figure 4. Figure 4 long description.Meso-scale structures in the study area. (a) F2 fold affecting the contact between Fontane micaschist and dolomitic marble (S1), with S2 as axial planar foliation. (b) Top-to-the-SW, σ-type rotated porphyroclast associated with the S2 main foliation in a mylonitic sandy marble of the cover sequence. (c) F3 folds in impure marble; a local S3 crenulation cleavage is visible. (d) Decameter-scale F3 folds affecting the Luserna orthogneiss and adjacent calcschists in the Subiasco area (Pellice valley in Figure 2a). (e) Cargneules/tectonic breccia layer underlying the Triassic marble sequence. (f) Basement–cover (represented by Luserna orthogneiss and calcschist) interface in the Subiasco Valley, a tributary of the Pellice river, transposed towards parallelism to S2/S3.

Figure 5

Figure 5. Figure 5 long description.Mineral phases and petrography of sample 23PIN43. (a) Processed X-ray map showing the mineral assemblage (h/G = hole/graphite). (b) Relict of S1 foliation in a microlithon of the S2 foliation defined by white mica (Wm 1) (XPL = Crossed Polarized Light). (c) Aggregate of chloritoid (Cld 2) and white mica (Wm 2) defining the main S2 foliation, wrapping around S1 chloritoid (Cld 1) (PPL= Plane Polarized Light). (d) Particular growth zoning in garnet highlighted by inclusions. (e) Aggregates of chlorite and albite, interpreted as pseudomorph after sodic-amphibole (PPL).

Figure 6

Figure 6. Mineral phases and petrography of sample DD20A. (a) Processed X-ray map showing the mineral assemblage (h/G = hole or graphite). (b) Relict of S1 foliation within a microlithon of the S2 foliation (XPL). (c) Relicts of chloritoid (Cld 1) and white mica (Wm 1) defining the S1 foliation, in a microlithon of the S2 foliation (PPL). (d) Aggregates of chloritoid (Cld 2) and white mica (Wm 2), defining the main S2 foliation in a quartz-rich domain (PPL). (e) Garnet wrapped by the S2 main foliation, with strain shadows mainly made of quartz (PPL).

Figure 7

Figure 7. Figure 7 long description.X-ray map (WDS = Wavelength-Dispersive Spectroscopy) of garnet grains from samples 23PIN43, DD20 and FONT2, showing zoning for Fe, Ca, Mn and Mg. The interface between garnet core and rim is regular, suggesting limited or no dissolution of garnet core before the growth of garnet rim. Mineral inclusions are shown with different symbols in the Mg map. Abbreviations: R = Rim (Grt 2), M = Mantle (Grt 1b), C = Core (Grt 1a). Electron Probe Micro-Analyzer (EPMA) spot analyses are reported in Supplementary Material 2.

Figure 8

Figure 8. Mineral chemistry and zoning for white mica in samples 23PIN43, DD20 and FONT2. X-ray map (WDS) showing zoning in white mica for Mg and Na in samples 23PIN43 (a, b), DD20 (d, e) and FONT2 (g, h). White mica compositions for samples 23PIN43 (c), DD20 (f) and FONT2 (i). EPMA spot analyses are reported in Supplementary Material 2.

Figure 9

Figure 9. Figure 9 long description.Raman characterization of coesite. (a–d) Microphotographs of garnets with pristine coesite inclusions located in the garnet mantle in samples 23PIN43 (a–b) and FONT2 (c–d). (e) Raman spectra of two coesite inclusions. Garnet peak values at 346 and 916 cm−1 are marked with an asterisk. The garnet peak near 1040 cm–1 is shared with coesite.

Figure 10

Figure 10. (a) Equilibrium assemblage diagram calculated using Bulk I (garnet core composition) for sample 23PIN43. (b) Overlap of selected garnet compositional isopleths (XPrp = 0.06, XSps = 0.06, XAlm = 0.79, XGrs = 0.09), together with XMg in chloritoid and Si4+ (a.p.f.u.) in white mica; the intersection is highlighted by the black ellipse. (c) Overlap of garnet compositional isopleths for the garnet mantle (Bulk II; XPrp = 0.08, XSps = 0.02, XAlm = 0.82, XGrs = 0.08), combined with XMg in chloritoid and Si (a.p.f.u.) in white mica. (d) Overlap of garnet compositional isopleths for the garnet rim (Bulk III; XPrp = 0.03, XSps = 0.02, XAlm = 0.70, XGrs = 0.25) and Si (a.p.f.u.) in white mica. Equilibrium assemblage diagrams calculated using Bulk II and Bulk III are provided in Supplementary Material 1 (Figure S5).

Figure 11

Figure 11. Figure 11 long description.(a) Equilibrium assemblage diagram calculated using Bulk I for sample DD20. (b) Overlap of selected garnet core compositional isopleths (XPrp = 0.08, XSps = 0.12, XAlm = 0.75, XGrs = 0.05), together with XMg in chloritoid and Si (a.p.f.u.) in white mica; the intersection is highlighted by the black ellipse. (c) Overlap of garnet compositional isopleths for the garnet mantle (Bulk II; XPrp = 0.09, XSps = 0.09, XAlm = 0.75, XGrs = 0.06), combined with XMg in chloritoid and Si (a.p.f.u.) in white mica. (d) Overlap of garnet compositional isopleths for the garnet rim (Bulk III; XPrp = 0.10, XSps = 0.05, XAlm = 0.72, XGrs = 0.13) and Si4+ (a.p.f.u.) in white mica. Equilibrium assemblage diagrams calculated using Bulk II and Bulk III are provided in Supplementary Material 1 (Figure S8).

Figure 12

Figure 12. Detrital zircon geochronology. Cathodoluminescence images of representative zircon crystals and kernel density plots of 206Pb/238U ages (<1 Ga) and 207Pb/206Pb ages (>1 Ga) for metasediments 23PIN43 (a, b), FONT2 (c, d) and DD97 (e, g). In the cathodoluminescence images (a, c and e) circles indicate the location of the analyses and numbers are dates with absolute uncertainty (Ma ± 2 sigma). Diagrams show data filtered at ≥90% concordance. (f) Concordia plot of youngest zircon analyses from samples 23PIN43 and FONT2. The detrital zircon age populations from the northern Dora-Maira basement (Nosenzo et al.2024), Pinerolo-Sanfront and Zone Houillère (Manzotti et al.2016) and the northern Gondwana mainland (Siegesmund et al.2021) are shown for comparison in the lowest part of the figure.

Figure 13

Figure 13. Figure 13 long description.Palaeogeographic and tectonic evolution of the Dora-Maira Massif. (a) Late Cretaceous configuration of the Briançonnais microcontinent, with the Dora-Maira forming a distal crustal high located beyond the pre-Piemonte palaeogeographic domain (based on Pantet et al.2020; Michard et al.2022 and Agard, 2021). Syn-rift oceanic sediments have been omitted for clarity. (b) Continental subduction during the Middle–Late Eocene, slicing and incorporation of basement–cover successions into the subduction channel, and burial to UHP conditions in the Dora-Maira units (modified from Dana et al.2023 and Agard, 2021). (c) Latest Eocene to Early Oligocene crustal stacking and beginning of exhumation, with pinching of subduction channel slices (modified from Michard et al.2004; Dana et al.2023; Agard, 2021). Upper plate oceanic units represent fragments of the Piemonte-Ligurian Ocean that escaped deep subduction and during the convergence remained at shallow crustal levels or within the overriding upper plate (see Schmid et al.2004, 2017). (d) From c. 35 Ma to the present, continued plate convergence and the westward indentation of the Ivrea mantle wedge (Schmid et al.2017) induced large-scale retro-vergent deformation throughout the Western Alps. The internal portion of the nappe stack, including the Dora-Maira Massif, was progressively transported eastwards, leading to the development of the large regional backfolds and backthrusts. The Piemonte–Ligurian oceanic units, originally located structurally above and east of the Briançonnais continental units during subduction, were subsequently carried over and folded around the Dora-Maira, reaching their present-day position. Units that formed part of the upper plate during subduction are no longer exposed in this portion of the Western Alps and were probably largely eroded, with the exception of the Chenaillet klippe. Modified after Molli et al. (2010), Schwartz et al. (2009), Lardeaux et al. (2006) and Schmid et al. (2017).

Figure 14

Figure 14. P–T–d path and related microstructures for the studied samples compared with those path proposed by Manzotti et al. (2022, 2025b).

Figure 15

Figure 15. Tectonic map of the Dora-Maira Massif showing the newly proposed structural subdivisions and compiled peak P–T conditions from this and previous study. The map was compiled after Dana et al. (2025), incorporating data from Henry (1990), Servizio Geologico d’Italia (2002) and Michard et al. (2022). P–T data derive from Pognante and Sandrone (1989), Hermann (2003), Gasco et al. (2011), Groppo et al. (2019, 2025), Manzotti et al. (2022, 2025b, 2026), Nosenzo et al. (2023), Nerone et al. (2024) and Petroccia et al. (2025). The small San Chiaffredo Unit of Compagnoni et al. (2012) is here mapped as part of the Brossasco-Isasca Unit following Michard et al. (2022). Abbreviations (uppercase bold for tectonic nappes, lowercase bold for units defined solely on the basis of P–T estimates but not constrained by nappe boundaries): MV = Monviso, SOR = Susa-Orsiera-Rocciavrè Unit, LA = Lanzo, CLSZ = Cima Lubin Shear Zone, VG = Valle Grana Unit, VMS = Val Maira-Sampeyre Unit, DU = Dronero Unit, VSZ = Valmala Shear Zone, VS = Varaita-Susa Unit (se = Serre Unit, mru = Muret-Ricordone Unit, cu = Chasteiran Unit), RS = Rocca Solei Unit (gu = Grimbassa Unit; rs = Rocca Solei Unit), BIU = Brossasco-Isasca Unit (sc = San Chiaffredo Unit), PSU = Pinerolo-Sanfront Unit.

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