Data di Pubblicazione:
2009
Abstract:
The present sheet of the 1:50,000 Carta Geologica d'Italia falls entirely in the
so called Piana del Sele (i.e. Sele River Plain). This alluvial-coastal plain lyes on
Quaternary sediments that were accumulated inside a coastal half-graben, which
continues in the off-shore with the deep Salerno Gulf. As shown in Fig. 1, this
tectonic depression cuts the -orogenically speaking- inner side of the Southern
Apennine chain, being interpreted as an effect of the opening and eastward migration
of the Tyrrhenian Sea back-arc basin. The present day bathimetry of the
Salerno Gulf is shown in Fig. 2, while Fig. 3 shows the thickness of the basin
fill by isopachs in milliseconds t.w.t.. The main tectonic features of the basin are
described in Fig. 5 and 6, according to Sacchi et alii (1994) for the off-shore and
according to the present authors for the faults running either near coast or on land.
The logs of Mina 1 and Sele 1 wells (Fig. 5 and 6) account for the deep stratigraphy
of the basin fill, but there are still doubts about the age of its lowest terms
and, consequently, the beginning of collapse. However, most authors agree that
the present day morphostructural setting is due to Quaternary extensional tectonics,
controlled by a NW-SE oriented ?3.
On land, the first phases of the collapse (and generation of strong relief) is
evidenced by the deposition of the so called Conglomerati di Eboli (i.e., the Eboli
Supersynthem; CE). This thick and widespread clastic unit of the Lower Pleistocene
is deeply buried in this Sheet (Fig 7) but it is largely exposed in the Sheets
467 and 468. It is mostly composed of fan-glomerates whose clasts came from
the dissection of the Mt. Picentini massif, where a thick succession of tectonized
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Mesozoic limestones and dolostones crops out. Around the beginning of Middle
Pleistocene, the geomorphology of the Plain was re-shaped by normal and
transtensional (transfer) faults (Fig. 8). Part of the area carrying the Lower Pleistocene
fanglomerates was uplifted, while another large part of the Plain continued
to subside and started accomodating the Battipaglia-Persano supersynthem (BP).
This unit, which is up to some hundreds meters thick, covers large part of the
present Sheet and associates with a wide depositional terrace that rests at 16-18
m a.s.l. closer to the modern coast and rises up to 100 m a.s.l. and more near the
mountain front (where alluvial fans increase locally its elevation; Fig. 9).
Even though never sampled and studied in detail, the lower part of the BP
supersynthem is lithostratigraphically described in the logs of numerous drillings
for water research. There it appears composed of decametrica alternations of
coarse grained intervals of probable fluvial origin, intervals dominated by grey
to blue clays (sometimes with peat and fossils) of probable lagoonal origin and
intervals of matrix free sands of probable beach and coastal dune environments.
Thickness and facies of the supersynthem's lower part prove that its deposition
was accompanied by subsidence and, maybe, NW-ward tilting (see Fig. 8).
The younger part of the supersynthem BP was investigated in detail with a
number of new drillings (see Appendice 1), palaeo-ecological analyses and correlations
with the logs of many pre-existing perforations. As shown in Fig. 14,
it is composed of coarse and fine grained alluvial deposits close to the hills of
Battipaglia (area of the ancient fan of the Tusciano River; see Fig. 9), while the
coeval, more distal part of it is composed of a number of coastal parasequences
that give evidence of several regressions and trasgressions. Based on pollen data
and relations with the Gromola Synthem (see below), those fluctuations are tentatively
framed between the OIS 9 and 5.5. As proved by the elevation of
Tipologia CRIS:
05.09 Cartografia
Keywords:
geological mapping; land-sea correlation; synthem; marine surveying
Elenco autori:
Bellonia, Antonello; D'Argenio, Bruno; Pelosi, Nicola; Budillon, Francesca; Ferraro, Luciana; Insinga, DONATELLA DOMENICA; Marsella, Ennio
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