We processed and interpreted a newly acquired geophysical dataset (WS10 project) integrated with vintage
seismic profiles to study the evolution of the Sardinian passive margin of the Sardo-Provençal basin. The most
prominent features of the area of study are a consequence of the Messinian Salinity Crisis (MSC)which produced
a thick salt layer in the deep basin. Complex halokinetic tectonics deformed the overlying Messinian Upper Unit
(UU) and the Pliocene–Quaternary (PQ) sediments, sometimes also bending the sea bottom. A thinner autochthonous
salt in the UU suggests at least one further low stand during the late MSC.
The Messinian Erosional Surface (MES) separates the erosional truncation of the pre-Messinian sedimentary sequence
fromthe overlaying Plio-Pleistocene sequencewith a clear angular discordance,which almost completely
masks possible earlier erosional events. The MES is present across the middle and upper slopes of the Sardinian
margin and can be easily recognized downto the lower slope,where it interfingerswith the Messinian evaporites
which gradually thicken basinward.
We propose a correlation between the main erosional surface of the lower slope and the salt layer recognized in
the UU as a consequence of a falling stage during the last part of the MSC.
The seismic profiles now available along theWest Sardinian margin provide novel and crucial information to correlate
theMessinian depositional units in the deep basinwith those present in the lower continental slope and with
the erosional surface of the middle and upper slopes. Our data and interpretation highlight the main units of the
Messinian trilogy and further internal sequences that are probable related to cyclic fluctuations during their
deposition.
