Collision processes between the African and European plates in the Ion
ian Sea offshore Calabria and in Sicily take place in several ways. To
the east, normal subduction of oceanic crust (underlying the Ionian S
ea) occurs underneath the Calabrian are, whereas to the west, continen
tal collision between the Pelagian block and the Calabrian are (which
extends from Calabria to the northeastern tip of Sicily and offshore o
f the island to the north) gives rise to the Maghrebian thrust belt on
mainland Sicily. This belt consists mostly of stacked basinal and pla
tform carbonates of Mesozoic-early Tertiary age deposited along the Af
rica passive margin. No clear subduction characterizes the area north
of the Hyblean-Malta plateau where it collides with the Maghrebian cha
in. The origin of the Hyblean-Malta plateau is unclear. Geophysical da
ta indicate, however, that its crustal structure is different from tha
t of the surrounding Pelagian foreland. Crustal structure variations a
t the edge of the subducted African plate may thus cause the observed
segmentation of the collisional are system. A computer model of the re
gion was created to learn about the deformation and faulting processes
in the region. The simulation starts prior to the collision of the Pe
lagian block with the Calabrian are. With time the Hyblean-Malta plate
au collides with the northern crustal block and, as a result, a new si
mulated topography, a new distribution of velocities and, most importa
nt, a new distribution of fracture zones are created. A shear fracture
zone is formed east of the Hyblean-Malta plateau (Malta escarpment) e
xtending to the subduction zone at the Calabrian are. A less active st
rike-slip fracture zone is created west of the Hyblean-Malta plateau.
An additional E-W trending active fracture zone is creating in the sou
thern part of the simulated area. This feature may correspond to a fau
lt zone which runs from the Strait of Sicily to the Ionian Sea.