To cite this version:Xian-Hua Li, Michel Faure, Wei Lin, Gianreto Manatschal. New isotopic constraints on age and magma genesis of an embryonic oceanic crust: The Chenaillet Ophiolite in the Western Alps. Lithos, Elsevier, 2013, 160-161, pp.283-291
AbstractThe Chenaillet Ophiolite is one of the best-preserved remnants of the Piemont-Liguria oceanic basin, a branch of the Central Atlantic that opened during the separation of Adria/Africa from Europe. Despite numerous studies of structure, petrology, geochemistry and isotope geochronology, the timing and genesis of various magmatic rocks within the Chenaillet Ophiolite are still controversial. We provide in this study integrated in situ analyses of zircon U- Based on our new age results and compilation of the reliable literature U-Pb age data, the ophiolitic gabbros from Eastern, Central and, Western Alps, Liguria and Corsica crystallized nearly synchronously at 158-166 Ma, suggesting a short life span of < 11 m.y. for the formation of the Piemont-Liguria oceanic domain, rather than a ~ 30 m.y. life span as previously thought. The Chenaillet ophiolite is likely a remnant of embryonic oceanic crust, rather than a piece of "mature" oceanic crust. Provided the spreading velocities of < 3 cm/yr full rate for magma-poor MOR sequences, the maximum width to the Piemont-Liguria oceanic floor would have been in the order of 300 km.