TY - DATA T1 - Evidence of multi-phase Cretaceous to Quaternary alkaline magmatism on Tore–Madeira Rise and neighbouring seamounts from 40Ar/39Ar ages PY - 2016/06/21 AU - Renaud Merle AU - Fred Jourdan AU - Andrea Marzoli AU - Paul R. Renne AU - Marion Grange AU - Jacques Girardeau UR - https://geolsoc.figshare.com/articles/dataset/Evidence_of_multi-phase_Cretaceous_to_Quaternary_alkaline_magmatism_on_Tore_Madeira_Rise_and_neighbouring_seamounts_from_sup_40_sup_Ar_sup_39_sup_Ar_ages/3454679 DO - 10.6084/m9.figshare.3454679.v1 L4 - https://ndownloader.figshare.com/files/5426636 L4 - https://ndownloader.figshare.com/files/5426639 L4 - https://ndownloader.figshare.com/files/5426642 L4 - https://ndownloader.figshare.com/files/5426645 L4 - https://ndownloader.figshare.com/files/5426648 KW - 30 Ma KW - seamount KW - 68 Ma KW - Tore KW - Ar KW - Geology N2 - The Tore–Madeira Rise is a seamount chain located 300 km off the Portugal and Morocco coasts attributed to hotspot activity. U–Pb ages of lavas from the northern and central Tore–Madeira Rise range between 103 and 80.5 Ma whereas 40Ar/39Ar ages from the central and southern Tore–Madeira Rise yield ages ranging from 94.5 to 0.5 Ma. We performed new 40Ar/39Ar measurements to better understand the geodynamic history of the Tore–Madeira Rise. Plagioclase ages from the Bikini Bottom and Torillon seamounts suggest ages of >90 Ma and ≥60 Ma, respectively. Amphiboles from the Seine seamount yield an age of 24.0 ± 0.8 Ma. Biotites from lavas of the Ashton seamount give ages of 97.4 ± 1.1 Ma and 97.8 ± 1.1 Ma. The geochronological database available on the Tore–Madeira Rise has been filtered on statistical criteria to eliminate unreliable ages. The resulting database reveals three pulses of alkaline magmatism on the Tore–Madeira Rise at 103–80.5 Ma, at c. 68 Ma and between 30 Ma and the present. The magmatism was continuous from 103 Ma until c. 68 Ma and from c. 30 Ma until the present on the Tore–Madeira Rise, the surrounding seamounts and the Portugal coast. We suggest that the space–time distribution of this magmatism results from the interaction between a wide thermal anomaly emitting magmatic pulses and the complex motion of the Iberian plate. ER -