
Flash Media
Update: 20/02/2007
The Island, together with a limited strip of the Sicilian coast,
is shown in Sheet no. 585 “Mondello – Ustica
Island” of the Geological Map of Italy on scale 1:50,000. The
Ustica Island survey was based on an agreement between the National
Geological Survey (which was later merged with ISPRA) and the
University of Milan and was realized in 2002 thanks to the
collaboration of geologists from the two organizations. G.
Pasquarè was in charge of the project’s scientific
coordination and L. B. Marinoni, of the University of Milan,
directed the survey. The following geologists also worked on the
project for the National Geological Survey: R. Bonomo, V. Ricci, L.
Vita, L. Vezzoli (University of Insubria). M. D’Orazio
(University of Pisa) directed the chemical analyses of collected
volcanic samples. The map was a result of the agreement and was
prepared by P. Moneta.
Following guidelines of the new Geological Map of Italy, the survey
(carried out on a scale of 1:10,000) tried a different approach for
the stratigraphic reconstruction of the area. It did this through
the application of unconformity-bounded stratigraphic units (UBSUs)
and morpho-stratigraphic units (lithosomes) combined with
traditional lithostratigraphic units. UBSUs, which can also include
other types of stratigraphic units, enable a synthesis of space and
time relations that take place between mapped units and their
eventual connection with morphogenetic and tectonic or
volcanic-tectonic stages. This can be deduced by considering the
important discontinuities (such as paleosoils, unconformity,
erosive surfaces, etc.) that mark the area’s history and the
evolution of its eruptive system. The volcanic island of Ustica is
the remaining part of a seamount’s peak that emerged from the
waters of the Tyrrhenian Sea. Its geological history includes an
emersion stage with a subsequent evolution as coastal and subaerial
environment. It shows pillow-lavas, hyaloclasta and volcanoclastic
facies (which are typical of the interaction between magma and
water) as well as subaerial lava flows. The numerous lava flows
with a basic composition (after a long quiescence interval) were
associated to trachytic products (even pumice blocks) of explosive
eruptions, which caused the destruction of the Northern part of the
island. This depression was later filled in by several lava flows.
Furthermore, several dike systems created further volcanic
activities in various parts of the island, where tectonic tension
features are found. The volcanic activity continued for about
600,000 years in the Middle and Upper Pleistocene with different
emission points and changes in the geometry of the superficial
eruptive system. When euptive events ended, marine erosion
processes became predominant over the island’s constructive
ones. The current morphology shows an intense marine abrasion,
which has contributed to cancelling the original volcanic forms but
has, at the same time, exposed magnificent sections of great beauty
and interest.