www.geologicacarpathica.com
GEOLOGICA CARPATHICA, AUGUST 2016, 67, 4, 371–389
doi: 10.1515/geoca-2016-0023
Pleistocene volcaniclastic units from North-Eastern
Sicily (Italy): new evidence for calc-alkaline explosive
volcanism in the Southern Tyrrhenian Sea
MARCELLA DI BELLA
1
, FRANCESCO ITALIANO
2
, GIUSEPPE SABATINO
1
, ALESSANDRO
TRIPODO
1
, ANGELA BALDANZA
3
, SERGIO CASELLA
1
, PAOLO PINO
1
,
RICCARDO RASA’
1
and SELMA RUSSO
1
1
Dipartimento di Scienze Matematiche e Informatiche, Scienze Fisiche e Scienze della Terra, Università di Messina,
Viale F. Stagno d’Alcontres 31, 98166 Messina, Italy; mdibella@unime.it
2
Istituto Nazionale di Geo sica e Vulcanologia, Palermo, Italy
3
Dipartimento di Fisica e Geologia, Università di Perugia, Via A. Pascoli, 06123 Perugia, Italy
(Manuscript received June 30, 2015; accepted in revised form June 7, 2016)
Abstract: A well-preserved volcaniclastic sequence crops out in Pleistocene marine sediments along the Tyrrhenian
coastline of the Calabrian-Peloritani arc (Sicily, Italy), testifying the occurrence of Lower-Middle Pleistocene volcanic
activity in Southern Tyrrhenian Sea. The presence of dominant highly vesicular and minor blocky glassy particles
indicates that the volcanic clasts were originated by explosive events related to the ascent and violent emission of
volatile-rich magmas accompanied by and/or alternated with hydromagmatic fragmentation due to magma-sea water
interaction. Field investigations and sedimentological features of the studied volcaniclastic units suggest a deposition
from sediment-water density ows. The chemical classi cation of the pumice clasts indicates prevalent rhyolitic and
dacitic compositions with calc-alkaline to high-K calc-alkaline af nity. The geochemical features of immobile trace
elements together with the presence of orthopyroxene are indicative of a provenance from an arc-type environment.
The age (from 980-910 to 589 ka), the chemical composition and the evidence of subaerial explosive volcanic activity
constrain the origin nature and temporal evolution of the arc-type volcanism in the Southern Tyrrhenian domain.
Finally, the new information here provided contribute to a better understanding of the temporal geodynamic evolution
of this sector of the Mediterranean domain.
Key words: volcaniclastic deposits, Pleistocene volcanism, N-E Sicily, stratigraphy, explosive volcanic activity, Arc
volcanism.
Introduction
The southern Tyrrhenian Sea is dotted with active volcanoes
and seamounts generated by the subduction of the Ionian
oceanic crust beneath the Calabrian-Peloritani Arc (e.g., Bar-
beri et al. 1974; Beccaluva et al. 1982, 1985). All of the struc-
tures were deeply studied during the past decades from the
geophysical (Barberi et al. 1973; Ventura et al. 1999; Marani
& Gamberi 2004), petrological (Selli et al. 1977; Savelli
1984; Trua et al. 2002), and geochemical (Caracausi et al.
2005; Heinicke et al. 2009, Lupton et al. 2011; Italiano et al.
2014) points of view. Despite the studies carried out so far,
the geodynamic setting and the evolution of the Mediterra-
nean basin is still a debated matter (e.g. Carminati et al. 2012,
and references therein).
The SE Tyrrhenian Sea is bordered to the East by the Cala-
brian-Peloritani Arc, which is laterally segmented by major
WNW-trending shear zones that have accommodated the
rotational movements (Malinverno & Ryan 1986; Knott &
Turco 1991) from the late Miocene (Van Dijk & Scheepers
1995) up to recent (Tansi
et al. 2007). The Calabrian-Pelori-
tani Arc has been affected by a rapid regional uplift since the
Quaternary (Westaway 1993; Cucci 2004; Ferranti et al.
2006), accommodated by a tectonic extensional regime
(Monaco & Tortorici 2000; Catalano et al. 2003) also con-
firmed by GPS measurements (Serpelloni et al. 2013). The
volcanic activity is located along the main regional faults and
apart from the volcanism of the Aeolian Islands no other
recent active volcanic centres were known. Loreto et al.
(2015) confirmed the existence of a buried volcano offshore
Capo Vaticano (Calabrian Arc). That seamount, which is still
venting volcanic volatiles, coincides with the volcanic edi-
fice responsible for the nearby Pleistocene volcaniclastic
units occurring inside the half-graben depressions of the
Mesima-Gioia Tauro and Reggio Calabria basins (De Rosa et
al. 2001, 2008).
A further well-exposed and well-preserved volcaniclastic
sequence included in marine sediments, crops out along the
Tyrrhenian coastline of the Calabrian-Peloritani Arc (Pelori-
tani Mountains), referred to the Lower-Middle Pleistocene
(Kézirian 1992a,b; Toussaint et al. 1999) and represents the
most complete outcrop of the area although other minor scat-
tered occurrences are reported nearby (Kézirian 1992a,b).
Within the Strait of Messina area, similar sequences are also
exposed along the Calabrian coast (Kézirian 1992a,b;
Calanchi 1988; Leyrit et al. 1998, 1999; Toussaint et al.
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1999) and in several sites of the Ionian and peri-Tyrrhenian
Calabria (Cello et al. 1983; Toussaint et al. 1999; De Rosa et
al. 2001, 2002; Bigazzi & Carobene 2004; Carobene et al.
2006; De Rosa et al. 2008). Since the Late Tortonian, exten-
sive explosive volcanic activity took place in the Mediterra-
nean area, with dispersion of pyroclastic products over
a large portion of the basin and of continental Europe
(Keller et al. 1978; Paterne et al. 1988; Pyle et al. 1998;
Narcisi & Vezzoli 1999; Pouclet et al. 1999; Schmidt et
al. 2002).
In the last years, some studies (De Rosa et al. 2008; Trua et
al. 2010) have been focused on volcaniclastic layers inter-
bedded in marine successions along the Italian peninsula.
In contrast, no information exists on the volcaniclastic hori-
zons cropping out over the north-eastern Sicilian coast,
located in front of the Aeolian Islands.
This paper accounts for the results of a multidisciplinary
study of the volcaniclastic deposits cropping out in the
north-eastern Sicilian coast (Fig. 1) and includes field inves-
tigations, stratigraphic, sedimentology, SEM-EDS and geo-
chemical analyses. The results help to constrain the type of
eruption, the deposition and transport mechanisms, and the
petrochemical features. The temporal range of the volcanic
events has been constrained by age data (Lentini et al. 2000,
2008; Pino et al. 2007a,b; Carbone et al. 2008) from
micro-fossil assemblages of the sedimentary clay succession
in which the volcaniclastic units are interbedded. The results
provide new information about the less studied Sicilian vol-
caniclastic deposits. Their identification and correlation are
adopted as tools for the reconstruction of the sedimentary
sequence and of the volcanic history in the area.
Geological setting
The investigated area is located along the Sicilian sector of
the Calabrian-Peloritani arc close to the Tyrrhenian coastline,
about 25 km south of the Aeolian Arc (Fig. 1). It is characte-
rized by a prevalent homogeneous and continuous lithologi-
cal sequence of poorly fossiliferous marly clays, with
inter-layered volcaniclastic units.
This clayey sequence, reported as “Argille di Spadafora
Auctt.” (Lentini et al. 2008; Carbone et al. 2008), was origi-
nally assigned to the Pleistocene on the basis of foraminifera
content (Lombardo 1980; Violanti 1989; Kézirian 1992a,b).
The calcareous nannofossil associations with Pseudoemi-
liania lacunosa, Gephyrocapsa oceanica and Gephyrocapsa
sp.3 (MNN19f biozone sensu Rio et al. 1990) allowed us to
ascribe the clayey formation to the Middle Pleistocene (Di
Stefano & Lentini, 1995; Lentini et al. 2000, 2008; Pino et
Fig. 1. Bathymetric map of the Southern Tyrrhenian Sea (following Kamenov et al. 2009, modi ed) on the left and geological sketch map
of the study area showing the main outcropping formations and the volcaniclastic units (right). Black star — hypothetic volcanic edi ce
(Kezirian 1992a,b); black triangle — hypothesized volcanic edi ce of Capo Vaticano (Loreto et al., 2015); 1 — beach deposits (Holocene);
2 — alluvial deposits (Holocene); 3 — gray-blue marly clay (Middle Pleistocene); 4 — volcaniclastic units; 5 — pre-Pleistocene substra-
tum; 6 — traces of the stratigraphic sections; 7 — faults.
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al. 2007a,b; Di Stefano in Carbone et al. 2008). The emplace-
ment age of the marly-clayey sequence is constrained by the
distribution of Gephyrocapsa sp.3 (sensu Rio et al. 1990;
Pino et al. 2007a,b; Di Stefano in Carbone et al. 2008) that,
in the Mediterranean Sea, covers a time interval from
980–910 to 589 ka (Castradori 1993; Sprovieri et al. 1998;
Cita et al. 1998; Pino et al. 2007a,b). Based on published
magnetostratigraphic data (criterion guide of Matuyama/
Brunhes boun dary: 0.78 Ma), the studied sequence has been
attributed to the uppermost part of the Lower Pleistocene
(Calabrian stage), corresponding to the top of the Jamarillo
magnetic event, up to the lower part of the Middle Pleisto-
cene (ex-Ionian stage sensu Cita et al. 2006). The estimated
age fits that obtained by Cornette et al. (1987; from 1 to
0.72 Ma) for similar volcaniclastic units cropping out in the
Reggio Calabria basin.
During this time interval, the deposition of deep-sea pelites
in the deeper circalittoral to upper epi-bathyal zone (Kèzirian
1992a,b; Leyrit et al. 1998; Toussaint et al. 1999), up to
500–700 m below sea level, is testified by the foraminiferal
benthonic assemblages recognized in similar clay marls
cropping out in neighbouring localities (Violanti et al. 1987;
Violanti 1988, 1989). These sedimentary deposits are pre-
served within a structural depression in areas adjacent to the
present coastline. The substrate shows a siliciclastic (con-
glomeratic-arenaceous-clay) sequence (Gargano 1994;
Lentini et al. 1995, 1997), Serravallian–Lower Messinian in
age (Lentini et al. 2000), which was covered during Messi-
nian times by discontinuous evaporitic carbonates (Gargano
1994; Lentini et al. 2000). Lower Pliocene marls and marly
limestones (Trubi Formation) follow in the sequence. They
are covered by limestone, sandy marls, organogenic sands
and deep-water coral facies limestones attributed to the upper
part of the Lower Pliocene up to Upper Pliocene (Gaetani &
Saccà 1984; Barrier et al. 1987; Violanti et al. 1987; Violanti
1988; Di Stefano & Lentini 1995; Lentini et al. 2000; Pino et
al. 2007a,b). The persistent tectonic activity caused, before
clay sedimentation, a general uplift of the area up to the
emersion and marine terrace formation (Lentini et al. 1996,
Catalano & Cinque 1995).
During these latest phases, the marly clays pass into an
alternating clay and sand sequence of circalittoral environ-
ment s.l. (Kézirian 1992a,b), and later to a 3
rd
and 4
rd
order of
fluvial and marine terraces (altitude of 90–220 m a.s.l.).
They are related to the uppermost part of the Middle Pleisto-
cene (isotopic stage 7) (Catalano & Cinque 1995, Catalano &
Di Stefano 1997) and to the Tyrrhenian (isotopic stage 5)
(Bonfiglio & Violanti 1984).
Multidisciplinary approach and analytical techniques
Field work
Eight volcaniclastic units (hereafter referred to as VU)
were identified by field investigations. Thirteen stratigraphic
sections have been reconstructed and correlated each other
using the most widespread unit VU7 as a marker horizon
(Fig. 2). Despite the fact that the volcaniclastic units are not
exposed in all the sections, it was possible to establish cor-
relations based on their lithological characteristics and strati-
graphic position. A suite of fifty samples of volcanic sedi-
ments were collected and among all the pumice-rich units,
the least altered samples were selected for laboratory work.
Detailed information on each volcaniclastic unit (VU) is
reported in the result section.
Laboratory work
In the laboratory, the grain-size characteristics were deter-
mined by dry sieving at ½ intervals, in the –5< <4 size
range. Sieving was carried out by hand to avoid excessive
breakage of juvenile vesicular fragments. Statistical parame-
ters, such as median diameter (Md ), mean (M ), graphical
standard deviation (
) and first-order skewness (
), have
been obtained by construction of cumulative curves as pro-
posed by Inmann (1952).
In order to constrain the provenance and the processes
involved in the fragmentation and alteration mechanisms,
morphological investigations and mineral chemistry of the
main representative phases and pumice particles (size ran-
ging from 250 to 1100 μm) were performed by SEM-EDS
(Sheridan & Wohletz 1983) focussed on the characterization
of surface and vesicle structures. After selection, the pumice
clasts were cleaned for a few seconds in ultrasonic bath and
then mounted individually on a metal stub. Afterwards,
a petrographic study was carried out to better define structure
and composition of both pumice clasts and blackish lithics.
Bulk rock analyses of twenty-one selected pumices were car-
ried out by X-Ray Fluorescence to obtain geochemical infor-
mation on the parental magma of the volcaniclastic sequence.
Analytical techniques
The chemical composition of minerals in selected pumice
clasts was determined at the Physics and Earth Sciences
SEM-EDS Laboratory of the Messina University. Analyses
of Si, Al, Ti, Mn, Mg, Fe, Ca, Na, K, Cr and P contents were
carried out using a LEO-S420 Electron Microscope coupled
to an Oxford link ISIS series 3000 EDX spectrometer and
Si(Li) detector with resolution of 156 eV at MnK . Working
distance 19mm at acceleration voltage of 20 kV and 550 pA
(PROBE). The spectral data were acquired at 1500 to 2000
counts/s with dead time below 25 %, using the ZAF correction.
The chemical analyses of pumice clasts were carried out at
the Earth Sciences XRF laboratory at Perugia University.
The samples were crushed in a steel jaw crusher and reduced
to a fine powder in agate mortars. The concentrations of
SiO
2
, TiO
2
, Al
2
O
3
, Fe
2
O
3
, MnO, CaO, K
2
O, P
2
O
5
, Nb, Zr, Y,
Sr, Rb, Ba, Cr, V, and Ni were measured by X-ray fluores-
cence on powder pellets using a wavelength-dispersive auto-
mated Philips PW1400 spectrometer. MgO and Na
2
O
DI BELLA, ITALIANO, SABATINO, TRIPODO, BALDANZA, CASELLA, PINO, RASA’ and RUSSO
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Fig. 2.
Key stratigraphic sections of Middle Pleistocene clayey sequence with volcaniclastic deposits located in the geological map of
Figure 1.
Inset:
generalized stratigraphic log showing
the position of the studied volcaniclastic units.
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concentrations were respectively determined by atomic
absorption spectrophotometry and flame emission on sample
solution after perchloric and hydrofluoric acid attack. FeO
was determined by titration after rapid HF-H
2
SO
4
attack.
LOI (Loss on Ignition) is the weight loss after heating
at 950
°C. Precision is better than 10
% for all trace
elements.
Results
Detailed information on the volcaniclastic units
VU1, VU2 and VU3 crop out in the Scarano Locality
(section L of Fig. 2) and nearby Venetico Village (section B
of Fig. 2), where the lowest portion of the entire sequence is
exposed. VU4, VU5, VU6 crop out in the Venetico Marina
quarries (sections B and C of Fig. 1), east of the Torregrotta
cemetery (Section E of Fig. 2) and between Acquasanta
and Scarano localities (sections I and L of Fig. 2). Further-
more, VU5 also occurs on the eastern side of the hill, where
the Tracoccìa Village is located (section D of Fig. 2).
VU6 is also exposed in the northern boundary of the studied
area (section A of Fig. 2), near the margin of the Venetico
Marina coastal plain. VU7 is the most widespread among the
analysed layers and is found throughout the investigated
area, with the exception of Scarano Locality (section L of
Fig. 2), where the uppermost portion of the series is truncated
by erosion and subsequent deposition of a Tyrrhenian
Terrace. VU8 is at the top of the sequence, and crops out
sparsely in the northern (sections B, C, E of Fig. 2), central
and southern (sections H and I of Fig. 2) sector zones of the
investi gated area.
The field characteristics, such as thickness, lateral varia-
tions, juvenile and lithic component fractions, of the volcani-
clastic units are briefly described below, from bottom to top
of the stratigraphic sequence. The standard granulometric
classification scheme of Fisher (1961, 1966) for pyroclastic
rocks associated with explosive and non-explosive fragmen-
tation processes is used in this study. The term “volcaniclas-
tic” was defined by Fisher (1961, 1966) to denominate all
clastic sediments and rocks, regardless of depositional pro-
cess, composed of particles predominantly of volcanic
origin.
VU1 (Fig. 3a and b) is lentiform, variably thick (3÷10 cm)
and discontinuously outcrops. The basal contact with clays is
sharp, from planar to gently undulated. The upper contact is
less defined, variously corrugated and sometimes marked by
an orange alteration aureole. The textural features allow us to
recognize two lithofacies (VU1-1 and VU1-2). The lower
one (VU1-1; 1÷2 cm thick; Fig. 3b) is characterized by
mm-sized laminae of coarse ash black lithic clasts with
massive structure. Some interfingered plane-parallel lami-
nated layers of poorly cemented, well sorted and rounded
grey lapilli pumices, are also observed. This lithofacies is
characterized by lateral pinch-out closures showing sharp
contacts with the upper lithofacies VU1-2. This last lithofa-
cies (
VU1-2; Fig. 3b) is composed of clast-supported
normal graded slightly cemented grey, mainly sub-rounded
pumice lapilli clasts (up to 2–3 cm in diameter), sometimes
altered.
VU2 (Fig. 3c and d) shows variable thickness (2.5÷6 cm)
with spatial extent up to twenty metres in length, strongly
discontinuous and with pocket-like geometry. Generally, it
occurs as boudins laterally tapered due to load pressure. Its
basal and upper contacts are sharp and irregular and marked
by a yellow-orange alteration crust (2÷3 mm thick; Fig. 3d).
Evident fluidification structures are observed along the basal
surface (Fig. 3d). Generally, this volcaniclastic unit is charac-
terized by a massive appearance (2.5÷4.5 cm thick) com-
posed of prevailing whitish well sorted rounded pumices
with subordinate black lithic fragments (1÷3 mm) (Fig. 3d).
Locally, especially in the section L (Fig. 1), this volcaniclas-
tic unit is overlain by a layer of clast-supported fine
lapilli-sized rounded pumices (2-3 cm thick), through a sharp
and gently undulated contact (Fig. 3c).
VU3 is strongly discontinuous, up to 3 cm in thickness,
with laminated structure composed of a loose grey fine to
medium ash mixed with abundant fine terrigenous sand
(mica and quartz), foraminiferal microfauna and minute bio-
clasts. The basal contact is sharp and slightly undulated; the
upper contact is erosive and irregular.
VU4 (Fig. 3e and f) is 5÷18 cm thick and shows a lateral
continuity at the scale of outcrop (about 40 m) with general
lenticular geometry. Its basal contact with clays is erosive
and rather wavy ( 25 cm wavelength), the upper contact is
sharp, from planar to slightly wavy sometimes showing load
structures (Fig. 3e). This volcaniclastic unit is well exposed
in sections L and B (Fig. 1), where two lithofacies have been
recognized (VU4-1 and VU4-2; Fig. 3f). The lower VU4-1
subunit is massive, up to 5.5 cm in thickness (section L) and
composed of sub-angular and sub-rounded loose black lapilli
scoria (2÷3 mm in diameter), sometimes altered and charac-
terized by pinch-out closures (Fig. 3e). The upper subunit
(VU4-2) consists of medium-coarse grained ashes, up to
8÷10 cm thick, with distinctive plane-parallel or slightly
undulated lamination structures, a few mm in thickness.
These structures are marked by alternating light non-volca-
nic fraction (terrigenous clasts, foraminiferal microfauna and
minute bio-clasts) and dark scoria fragments. It is to be
emphasized that in the north (Section B) the VU4-1 lithofa-
cies is poorly represented.
VU5 (Fig. 3g) is generally continuous, variably thick
(3÷20 cm in the different sections), and shows evident lenti-
cular and pocket-like geometry, on the metre scale (sec-
tion E). The basal contact with clays is erosive and sharp,
showing from slightly to densely wavy channel-like struc-
tures, whereas the upper contact is irregular with small steps.
Both contacts are often highlighted by an about 1 cm thick
orange alteration level (Fig. 3g). The volcaniclastic unit is
generally characterized by cm-thick layers (up to three) of
structureless to normally graded whitish fine lapilli pumices
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Fig. 3. Outcrop and/or detail photographs of the most representative studied volcaniclastic units: a, b — VU1, section B; c, d — VU2,
section L; e, f — VU4, section B; g — VU5, section E; h — VU6, section I. The white continuous lines indicate the entire volcaniclastic
units, the white dashed lines indicate the subunits. See text for details of descriptions.
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(up to 1 cm) with rare dark lithic fragments, separated by thin
(few mm to 1 cm) intercalations (usually two) of fine grained
greyish ash showing erosive contacts (Fig. 3g). The pumice
lapilli layers are well sorted and consist of sub-angular and
sub-rounded frequently altered clasts. The lowest pumice
layer is the coarsest with low matrix fraction and grainy
appearance. This layered sequence sometimes starts with
lenses (up to 1 cm thick) consisting of prevalent structureless
coarse ash (1–2 mm) to whitish pumiceous lapilli.
VU6 (Fig. 3h) shows variable thickness with an average
value of 25÷30 cm ( 5 cm in section L, 40 cm in section I)
and is laterally continuous with ribbon-like geometry (Hor-
nung et al. 2002). The contact with marly clays is clear and
defined by narrow undulations, barely defined at the base and
more prominent at the top. In general, the volcaniclastic unit
is characterized by an abundant non-volcaniclastic fraction
consisting of terrigenous component, Foraminifera (Orbuli-
nidae) and minute bio-clastic fragments mixed with the vol-
canic fraction mainly consisting of scoria (2÷5 mm). The two
fractions are organized in structureless cm-thick layers some-
times with slightly undulated plane-parallel and subordinate
low-angle cross lamination. In section L the two layers are
distinctively separated by a sharp surface, planar to gently
undulated. The latter is composed of terrigenous sediments
plus minor scoriae whereas the upper layer is mainly com-
posed of altered yellowish-white pumices (2÷7 mm) with
subordinate scoriae (Fig. 3h).
VU7 is the most widely occurring volcaniclastic unit. It is
continuous and shows a thickness from a few dm (sections D,
E and H) to over 2 m ( 2.30 m in section G). Its geometrics
generally range from ribbon-like, to channel-shape or gently
bell-shaped on the outcrop scale.
In Section O thickness
varia tions with reduction up to pinch-out closures have been
observed. The basal contact with clays is sharp and slightly
wavy to planar; the upper contact is also sharp (Fig. 4a and b).
Abruptly truncated erosive lateral closures are observed
between sections E and G. In the most complete sequence
(sections A, G and N) the VU7 unit shows peculiar lithologi-
cal and sedimentological features that clearly allow us to
define three lithofacies (section G). The lowest lithofacies
(VU7-1, Fig. 4c) is informally called the “lithic rich lithofa-
cies” (from 2÷4 cm to >10 cm thick in sections N, A; 30 cm
in section G). It contains abundant black angular lithic clasts
(up to 5 cm) mixed with sub-angular/sub-rounded pumices
(0.5 cm up to 6 cm), lithified, clast-supported massive struc-
ture which locally shows lateral transitions to reverse grading
of coarser lapilli (up to 6 cm in section G) (Fig. 4c) with lami-
nated lithic-rich beds (up to 1 cm in section A). Near sec-
tion E, at the contact surface with the marl-clay substrate,
flute-cast structures (N200W–N20E preferential direction)
have been identified. The VU7-2 is a planar to cross bedded
ash-lapilli tuff lithofacies showing a thickness of 10÷15 cm
reaching 35 cm in section G. Two sub-lithofacies have been
recognized (Fig. 4c). Both are well sorted. The lower VU7-2a
is more continuous (over 30–50 m) showing prevalent struc-
tureless plane-parallel laminae sometimes slightly wavy,
with generally regular contacts; the upper sub-lithofacies
(VU7-2b) is characterized by mm to cm thick gently wavy
with low- to medium-angle cross beds, variously interfin-
gered with very fine-grained whitish pumices and dark
lithics. Only in section N, along strata interfaces, the pre-
sence of several flute casts with ESE–WNW preferential
orientation (N285E) from East-Southeastern to West-North-
western, marked by orange aureoles (Fig. 4d), was observed.
“Tool marks” have also been found. The chromatic variabi-
lity led us to informally call this sub-lithofacies “Zebra layer”
(Fig. 4c).
The third lithofacies (VU7-3, 25–30 cm thick; Fig. 4e) is
characterized by the presence of abundant sub-angular to
sub-rounded white lapilli pumices, with subordinate ran-
domly dispersed coarse angular lithics (1–2 cm up to 10 cm;
Fig. 4f). This lithofacies, informally called “White lapilli
pumices”, crops out in all the recognized sections represen-
ting 60–100 % of the whole VU7. The common presence of
at least three erosive contacts, usually marked by cm-thick
beds (2–3 cm thick) enriched in mm-sized angular lithics,
allow subdivision of the VU7-3 into four sub-lithofacies
(Fig. 4e). The lowermost one (VU7-3a) is incised into the
underlying VU7-2 with sharp and wavy erosive contact. It is
characterized by medium to coarse lapilli with rare dark ran-
dom lithics, showing the coarser fraction (1–2 cm in size)
concentrated in the median portion. VU7-3b (15–100 cm
thick), VU7-3c (15–40 cm thick) and VU7-3d (dm–cm thick)
show similar compositions to the previous sub-lithofacies
but different structures. In particular, VU7-3b is massive
(e.g. in section M) with some plane parallel lamination (e.g.
in section N, Fig. 4e); VU7-3c is massive and composed of
very coarse lapilli (3–6 cm sized) and randomly dispersed
sub-rounded to rounded pumiceous clasts (8–12 cm-sized);
VU7-3d is normally graded with pumice lapilli (mm-sized)
grading upward to whitish fine ash beds (1–8 cm thick) which
sometimes display convoluted structures (Fig. 4e).
The sequence described above is frequently incomplete
showing stratigraphic gaps and lateral variations, which are
continuous on metre-scale but discontinuous over 10’s of m
(20–30 m). For these reasons, in Fig. 5 a synthetic lithologi-
cal column is reported relative to the complete sequence of
VU7.
The average thickness of VU8 ranges between 10÷15 cm,
with a maximum thickness of 40 cm in section C, and it
is widely distributed. Sideways, it is rather continuous with
plane-concave lentiform geometry and pinch-out closures.
Its basal contact with clays is slightly undulated, the upper
erosive contact is markedly undulated and articulated, with
small steps. Both contacts are sharp and frequently marked
by an orange alteration level (up to 1 cm in size). The unit
shows abundant pumices mainly fine-grained (<1 cm in
size), loose and sub-rounded and rarely coarse-grained
(3–5 cm in size), which are arranged in cm-thick laminae
(1–3 cm). The latter are plane-parallel and marked by grey to
yellow-orange chromatic variations. Rare dispersed dark
lithics have also been found. The pumiceous beds are
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Fig. 4. Representative pictures of structures and detailed features of the VU7 unit: a, b — outcrop views, section G; c — basal portion,
section G; d — ngerprints of ute casts with orientation, section N; e — middle part, section G; f — detail with a sub-angular lithic clast.
The white continuous lines indicate the entire volcaniclastic units, the white dashed lines indicate the subunits. See text for
details of descriptions.
VU6 and VU8 are well-sorted, VU2, VU3 and VU4 are dis-
tinctively uni-modal and better sorted, whereas only VU7-1
and VU7-3 are poorly sorted and show low Md typical of
pyroclastic flow deposits (Table 1).
Representative SEM images of clast morphologies are
displayed in Fig. 6. The studied juvenile material shows two
main morphologies (Table 2). Some pumice clasts have
a fluidal texture with thin, commonly tubular, frequently
coalescing vesicles, related to high energy magmatic erup-
tions (Fig. 6A, C, F, G, H). Other fragments are blocky
usually interbedded with mm-sized light grey fine-
ashes, which are characterized by slightly wavy erosional
surfaces.
Grain size distribution and morphological features of
volcanic clasts
The parameters of grain size distribution and summary of
volcaniclastic component sorting (Cas and Wright, 1987) are
reported in Table 1. The results highlight that VU1, VU5,
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and dense poorly vesiculated to massive glassy with con-
choidal fracture (Fig. 6D) In both cases, the clasts frequently
show surfaces coated with adhering particles
(Fig. 6A, C, D, G, H).
Petrography and mineral chemistry
The studied volcaniclastic units are composed of predomi-
nant pumices (vesiculated juvenile materials) associated with
rare volcanogenic minerals (loose pyroxene and plagioclase
crystals) and a basaltic lithic fraction. The results of
petrographic and mineral chemistry investigations indicate
homogeneous features of the pumice clasts among the
various volcaniclastic units in terms of both texture and com-
position. In general, the various units are characterized by
different amounts of non-volcanic extra-basinal and intra-
basinal clastic components. Commonly, the extra-basinal
fraction, derived from inland, is represented by non-volcanic
mineral clasts of quartz, feldspar, chlorite, mica flakes
(biotite, muscovite), and fragments of metamorphic, intru-
sive and sedimentary rocks. The intra-basinal component is
represented by clay containing fossils and diffuse pyrite
grains.
Juvenile volcanic clasts in all units consist of predomi-
nantly white and minor brown pumices, marked by fluidal,
spongy and minor blocky texture. The lithic volcanic fraction
is mainly represented by rock fragments. Some mafic lithics
contain phenocrysts of plagioclase and pyroxene in a ground-
mass consisting of the same phases plus magnetite and brown
glass. Under the microscope most of the lithic clasts show the
same mineral assemblage occurring as phenocrysts in pumi-
ces, suggesting that they should be consi dered genetically
related to pumices, at least for those contained in the VU7.
Igneous minerals, include plagioclase, clino- and orthopy-
roxene (Fig. 7A and B). They occur as loose crystals and as
phenocrysts in pumices and in lithic clasts of all the volcani-
clastic units. Plagioclase appears as the dominant and ubiqui-
tous phenocryst phase as sub-euhedral slightly zoned crystals
Volcaniclastic
Units
Skewness
Sorting*
VU1
0.50
1.40
0.64
Well sorted
VU2
1.60
0.85
0.06
Very well sorted
VU4
-0.65
0.45
0.22
Very well sorted
VU5
1.50
1.55
-0.61
Well sorted
VU7-1
1.60
1.30
0.076
Well sorted
VU7-2
1.00
2.82
0.061
Poorly sorted
VU7-3.1
2.80
1.40
0.14
Well sorted
VU7-3.2
0.20
2.00
0.90
Poorly sorted
VU7-3.3
1.60
1.82
0.31
Well sorted
VU7-3.4
1.55
1.70
0.60
Well sorted
VU8
1.20
1.65
-0.090
Well sorted
(* from Cas & Wright 1987)
Table 1: Grain size distribution of representative volcanic compo-
nent of the studied volcaniclastic units.
Fig. 5. Reconstructed schematic depositional features of volcaniclastic unit VU7. See text for explanation of emplacement mechanisms.
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Fig. 6. Secondary electron images of selected pumice grains: A — uidal pumice shards of VU1; B — spiny shape of a pumice from VU2;
C — uidal and angular shape of a VU3 fragments; D — blocky glass grains from VU4; E — spiny shape of a VU5 pumice clast;
F — uidal pumice fragments from VU6; G and H — uidal pumice shards from VU7 and VU8, respectively.
381
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with marked resorption phenomena and frequent inclusions
of brown glass. The composition of the analysed plagio clase
crystals ranges from andesite to labradorite from rim to
core, with average values of An 38÷57 (Fig. 7A). Pyroxene
is present as euhedral to subhedral colourless to light-green
crystals in all the investigated pumices. Compositions
are pigeonite-augite with an average composition of
En
43
Fe
18
Wo
39
(Fig.
7B). The orthopyroxene is enstatite
(Fig. 7B).
Bulk rock chemistry
Pumice clasts, mainly belonging to the most representa-
tive volcaniclastic unit (VU7), have been analysed for major
and trace elements. The analytical results are reported in
Table 3 (major elements) and Table 4 (trace elements). Most
of the samples show high LOI values (> 2.5 %, Table 3),
probably due either to primary water and alteration. As alte-
ration may have changed the pristine compositions, espe-
cially in terms of alkali contents, the discussion is mainly
based on Zr, Y, Nb and Ti considered as immobile trace ele-
ments during secondary processes.
The total alkali versus silica (TAS) diagram recalculated
on a water-free basis (Le Bas et al. 1986; Fig. 8A) shows
subalkaline dacitic and rhyolitic compositions (Fig. 8A)
with two samples (VU7.4, VU8) characterized by
a slight alkali enrichment, falling in the trachyte field
(Fig. 8A). Fig. 8B shows how most of the samples plot
in the high potassic calc-alkaline field (Peccerillo &
Taylor 1976).
The incompatible trace-element abundances are displayed
on the multi-element mantle-normalized diagram (Sun &
McDonough 1989; Fig. 8C), in which
the negative Nb ano maly and the posi-
tive Pb spike are evident. On the Ti-Zr-Y
tectonic discrimination diagram (Pearce
& Cann 1973) all the samples fall in the
field of volcanic arc products
(Fig. 8D).
Discussion
Emplacement mechanisms
The eight volcaniclastic units besides
other ten minor lens-shaped disconti-
nuous volcaniclastic horizons (up to
3 cm thick) generally composed of ash to
very-fine whitish pumiceous lapilli and
ranging in age from 980–910
ka to
589 ka (Castradori 1993; Sprovieri et al.
1998, Cita et al. 1998), provide compel-
ling evidence for an intense long-lasting
volcanic activity with variable composi-
tion of the erupted products. Clasts have
Fig. 7. Composition domains (grey) of plagioclase (A) and pyroxene (B) of the samples
from the studied volcaniclastic units.
settled in a subaqueous environment to a depth of about 500–
700 metres, in an upper epi-bathyal zone, as suggested by the
constant presence of a benthic fossil association (Violanti,
1989).
Field investigations suggest that all the studied volcani-
clastic units are well correlated for all the thirteen examined
stratigraphic sections (Figs. 1 and 2) as indicated by the same
mutual stratigraphic position, by the comparable thicknesses
Samples
Clast morphologies
Description
VU1
Fluidal pumice
Well vesiculated, surfaces coated with ne
adhering particles.
VU2
Blocky
Higly vesiculated, elongated to sub-
spherical bubbles, conchoidal surfaces
coated with ne adhering particles, trace of
mechanical modi cations due to transport.
VU3
Fluidal angular shape
pumice
Strongly stretched vesicles, slight coated
with ne adhering particles.
VU4
Blocky
Moderately vesiculated, sub-spherical and
elongated vesicles with thick walls, trace
of modi cations by mechanical abrasion.
VU5
Blocky glass
Highly vesiculated, sub-spherical to
elongated vesicles with thin walls, surfaces
coated with ne adhering particles.
VU6
Fluidal pumice
Spiny shaped with sub-spherical to
elongated vesicles.
VU7
Fluidal pumice and
blocky
Fluidal shaped with tubular large and small
vesicles, evidence of stretching effects
- blocky shaped, pits due to chemical
etching – on both types surfaces coated
with ne adhering particles and no signs
of surface modi cations due to transport
processes.
VU8
Fluidal pumice
Parallel elongated vesicles with tiny
walls, surfaces coated with ne adhering
particles.
Table 2: Morphologies of the analyzed juvenile clasts.
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of the neighbouring clays, by the uniformity of their sedi-
mentological and petrographic features. Each volcaniclastic
unit, correlated in various sites, belongs to the same deposi-
tional event and therefore to the same eruptive or post-erup-
tive phase.
In most cases the units are composed of whitish pumiceous
lapilli with variable amounts of admixed lithic clasts, except
for the VU4 which is composed of prevailing black lapilli to
ash-sized scoriae. Among the units, VU7 is the most promi-
nent for its thickness of about 1 to 2.3 metres, the lateral
extension and also for its occurrence over a wide area.
Sedimentological features allow us to subdivide some volca-
niclastic units into distinct lithofacies. The VU3, VU4 and
VU6 units contain abundant exotic terrigenous clasts, fora-
miniferal microfauna and minute bio-clasts mixed with vol-
caniclastic materials. Because of the presence of basal
scouring and their internal structures indicative of water-sup-
ported gravitational flows, these are interpreted as epiclastic
units. They were generated by re-depositional processes and
are defined as secondary volcaniclastic products related to
post-eruptive processes. Contrastingly, the non-contaminated
volcaniclastic units (VU1, VU2, VU5, VU7, VU8),
SAMPLES
SiO
2
TiO
2
Al
2
O
3
Fe
2
O
3
FeO
MnO
MgO
CaO
Na
2
O
K
2
O
P
2
O
5
LOI
weight %
VU1
white pumice
62.11
0.85
13.96
3.29
3.48
0.16
1.25
3.47
3.78
2.73
0.18
4.72
VU2
white pumice
67.36
0.57
12.36
1.96
2.53
0.13
0.53
1.82
4.06
3.29
0.06
5.33
VU4-1
dark pumice
58.19
1.09
13.97
5.19
5.46
0.18
2.52
5.48
3.31
2.13
0.19
2.29
VU4-2
dark pumice
58.26
1.15
14.13
4.46
5.98
0.18
2.55
5.65
3.31
2.22
0.18
1.92
VU5-1
white pumice
65.29
0.58
12.35
3.41
2.90
0.16
0.65
2.53
3.85
3.51
0.12
4.65
VU5-2
white pumice
63.84
0.54
13.37
4.69
1.96
0.14
0.69
2.39
3.84
3.07
0.10
5.38
VU7-1
white pumice
68.39
0.67
14.48
2.70
1.79
0.15
0.94
2.72
4.47
2.98
0.14
0.55
VU7-2
white pumice
66.42
0.69
13.77
2.26
1.82
0.15
0.90
2.63
4.12
3.15
0.12
3.98
VU7-3
dark pumice
62.05
0.92
13.95
4.10
3.95
0.18
1.78
4.71
3.86
2.42
0.21
1.87
VU7-4
white pumice
61.11
1.25
9.70
7.14
2.07
0.30
0.83
4.42
3.97
4.62
0.14
4.44
VU7-5
white pumice
66.30
0.71
13.73
1.99
2.31
0.15
0.88
2.32
3.96
2.70
0.10
4.86
VU7-6
white pumice
68.96
0.81
12.10
2.80
2.38
0.16
0.90
2.88
4.25
3.05
0.09
1.61
VU7-7
white pumice
66.80
0.69
13.38
1.75
2.48
0.15
0.83
2.42
4.00
2.91
0.11
4.48
VU7-8
white pumice
65.89
0.69
13.32
1.88
2.30
0.14
1.07
2.53
3.98
2.93
0.11
5.18
VU7-9
white pumice
66.28
0.72
13.46
2.30
2.19
0.17
0.79
2.29
3.92
2.97
0.11
4.80
VU7-10
dark pumice
67.17
0.70
13.38
1.74
2.26
0.14
0.82
2.38
3.93
3.16
0.11
4.21
VU7-11
white pumice
67.83
0.74
14.44
2.59
2.12
0.16
0.88
2.79
4.33
3.02
0.15
0.97
VU7-12
white pumice
67.62
0.67
13.24
1.67
2.26
0.14
0.83
2.23
3.80
2.85
0.10
4.60
VU7-13
white pumice
68.23
0.67
12.66
2.10
1.86
0.13
0.90
2.34
3.79
2.74
0.11
4.47
VU7-14
white pumice
64.11
0.74
13.54
4.42
1.93
0.13
1.03
3.41
3.61
2.38
0.14
4.57
VU8-1
white pumice
63.21
0.97
9.81
5.79
2.11
0.23
0.69
3.55
3.88
4.39
0.10
5.28
SAMPLES
V
Cr
Co
Ni
Cu
Zn
Ga
Rb
Sr
Y
Zr
Nb
Ba
La
Pb
Ce
Th
ppm
VU1
white pumice
44
7
9
6
10
99
22
80
384
36
170
10
572
32
21
73
9
VU2
white pumice
13
7
1
10
9
76
20
97
280
36
197
11
670
31
24
62
17
VU4-1
dark pumice
272
20
24
19
42
107
24
71
429
29
146
12
473
27
19
65
8
VU4-2
dark pumice
322
24
22
11
39
100
24
70
447
31
150
11
494
29
14
47
6
VU5-1
white pumice
6
7
3
11
13
101
32
106
293
33
198
10
644
40
41
86
27
VU5-2
white pumice
10
3
1
15
17
90
20
96
315
38
189
11
624
33
20
131
19
VU7-1
white pumice
24
7
5
12
7
79
19
88
383
31
186
13
660
42
17
66
10
VU7-2
white pumice
21
6
5
11
7
81
17
92
361
31
184
12
646
42
17
70
10
VU7-3
dark pumice
125
16
8
12
16
96
22
73
466
27
154
11
521
38
17
104
6
VU7-4
white pumice
15
7
5
11
26
127
41
114
447
46
226
14
606
40
52
70
37
VU7-5
white pumice
15
4
6
8
11
95
20
85
364
32
182
11
718
36
27
69
16
VU7-6
white pumice
24
6
4
13
11
97
23
92
379
35
181
10
610
33
25
58
22
VU7-7
white pumice
19
5
3
10
10
79
17
83
350
37
182
11
635
40
22
60
16
VU7-8
white pumice
18
5
3
8
8
79
17
82
362
36
183
11
634
37
21
69
15
VU7-9
white pumice
15
3
4
10
12
86
24
90
332
35
178
10
623
35
31
68
24
VU7-10
dark pumice
15
6
2
10
10
85
21
89
346
33
173
10
641
36
25
64
25
VU7-11
white pumice
21
6
3
12
10
85
20
90
379
33
183
11
662
39
20
61
15
VU7-12
white pumice
16
5
1
9
8
83
17
81
347
36
182
11
662
38
23
71
14
VU7-13
white pumice
24
9
1
6
9
83
24
80
341
34
163
9
633
40
33
65
21
VU7-14
white pumice
52
6
9
17
14
74
23
74
320
27
161
9
519
21
26
90
15
VU8-1
white pumice
16
6
7
18
348
100
34
116
371
36
217
12
593
37
41
87
23
Table 3: XRF major elements data of the analyzed pumice clasts from the volcaniclastic units.
Table 4: XRF trace elements data of the analyzed pumice clasts from the volcaniclastic units.
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consis ting entirely of fresh volcanic fragments, are regarded
as primary deposits originated by subaqueous concentrated
density flows (Mulder and Alexander, 2001).
Density currents bearing unmodified eruption-formed
fragments originate either directly from volcanic eruptions
(pyroclastic flows) or indirectly by remobilization and rede-
position of material initially emplaced by a different process
(Fisher & Schmincke 1984; Cas & Wright 1987; McPhie et
al. 1993). For submarine settings, even deposits formed by
pyroclastic fragmentation followed by uninterrupted trans-
port through the ambient water column have been commonly
termed as reworked or redeposited (Cas & Wright 1987;
McPhie et al. 1993). Consequently, remobilized unconsoli-
dated pyroclastic debris transported downstream via density
current processes in a submarine setting with preserved pyro-
clastic components may be referred to as pyroclastic in ori-
gin. Pumice shreds, vitric shards, broken or euhedral crystals,
and vesicular to non-vesicular, angular lithic fragments
(Fisher & Schmincke 1984; Stix 1991) are consistent
with a pyroclastic origin as a direct result of volcanic
activity.
The compositional homogeneity of the volcanic products
and the absence of interbedded clayey layers suggest that
deposition occurred almost contemporary with the eruption
phases, quickly enough to inhibit the resumption of normal
marine sedimentation before volcanic activity ceased. There-
fore, the VU1÷VU8 volcaniclastic units are considered cold
mass flow deposits as the direct result of an eruption, with
transport and deposition mechanism controlled by aqueous
processes. VU7 best illustrates the primary pyroclastic origin
of these deposits. The flute casts in the plane-parallel lami-
nated facies (VU7-2b), channel scours bedforms, chan-
nel-shape geometry of deposits outcrops (Fig. 4) and dip
directions of slumpings of VU7 indicates a remobilization of
primary pyroclastic material in a near-shore environment,
probably outer muddy continental shelf, located to the
south-southeast, during or immediately after their primary
submarine deposition.
The interaction between volcanism and sedimentation, and
the development of concurrent facies are largely governed by
two factors: 1) the active volcanism producing abundant
material which is rapidly delivered to the deposition sites,
and 2) the lateral changes which are the result of flow trans-
formations. During eruptions large volumes of pyroclastic
materials are released far more rapidly than any production
process of epiclastic particles.
Fig. 8. Major and trace elements composition diagrams of the analyzed pumice clasts [VU7 has also lithic clasts, not only pumice!] from
the studied volcaniclastic units. A — TAS classi cation diagram of Le Bas et al. (1986); B — SiO
2
vs K
2
O classi cation diagram of
Peccerillo & Taylor (1976); C — Spider diagram of incompatible elements normalized to primordial mantle composition (McDonough et
al. 1992); D — Tectonic classi cation diagram based on HFS elements (after Pearce & Cann 1973).
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Type of eruptions
The investigated submarine volcaniclastic deposits are
diagnostic of different types of eruption. The analysis of the
morphological features of juvenile clasts is a valid tool for
reconstructing the modalities of magma vesiculation and
fragmentation during explosive eruptions (Heiken & Wohletz
1985). In particular, morphological analyses have been per-
formed to infer the style of fragmentation and especially the
active involvement of external fluids (phreatic or surface
water, steam) in the eruption dynamics (Wohletz 1983;
Dellino & La Volpe 1996). Volcanic ash particles from diffe-
rent fragmentation mechanisms have different surface tex-
tures and morphologies. The particles forming the analysed
volcaniclastic units show mainly pyroclasts with fluidal tex-
tures. The predominance of fluidal and highly vesicular frag-
ments over the blocky, dense clasts in the lapilli layers is
evidence of pure magmatic fragmentation. The blocky type
clasts, are dense fragments frequently marked by conchoidal
external surfaces with the presence of adhering particles
(Heiken & Wohletz 1985). This is a typical morphology of
hydroclastic tephra formation from a system associated with
shallow-water phreatomagmatic explosions, in which the
explosive vaporization of external water results in the frag-
mentation and quenching of magma (Heiken & Wohletz
1985, 1991; Wholetz 1987; Houghton & Wilson 1989;
Buttner et al. 1999). The angular blocky glassy shards, the
presence of glass alteration and the presence of adhering par-
ticles on the external surface of the clasts, indicate
the important role of magma-water
inte raction (Wohletz
1983; Sheridan & Wohletz 1983; Kokelaar 1986;
Wohletz 1987).
Abundant angular lithic fragments and sub-angular to
rounded pumices, both coarser in size, low vesicular to high
vesicular pumices, suggest depositional mechanisms as
a result of either fallout and pyroclastic flows during mode-
rate Vulcanian to large magnitude Plinian subaerial and/or
shallow-water phreatomagmatic eruptions.
The presence of (rare) lithic fragments combined with the
estimated volume of VU7 unit exceeding 2 10
6
m
3
( assuming
a conservative average thickness of 0.5 m over the whole dis-
tribution area) are consistent with partial volcanic conduit
collapse and/or vent clearing events during the volcanic
eruption.
Provenance of the volcaniclastic deposits
The analysed volcaniclastic-sequence represents the pro-
duct of explosive volcanic events from one or more volcanic
centres located in the Southern Tyrrhenian area. The mineral
assemblage, including orthopyroxene phenocrysts, and the
geochemical data (especially high ratios of LILE/HFSE)
highlight that the studied tephra originated in a volcanic arc
environment.
The volcanic centres in the Southern Tyrrhenian Sea cha-
racterized by arc signature are the seven subaerial volcanic
edifices of the Aeolian islands and the seamounts roughly
distributed around the Marsili Basin (Romagnoli 2013;
Romagnoli et al. 2013) (Fig. 1). The age of the subaerial Aeo-
lian volcanism ranges from 219 ka (Filicudi) to Present
(Stromboli) (De Astis et al. 2003; De Rosa et al. 2003, Pec-
cerillo 2005), younger than the studied volcaniclastic depo-
sits (Lucchi et al. 2013). The oldest documented volcanic
activity is represented by the 1.3 Ma age of dredged samples
coming from the Sisifo seamount (in the western submarine
portion of the arc).
Structural and magmatic variations recognized along the
arc depending on the variable composition of the subducted
slab (oceanic in the west and oceanic plus sediments in the
east), as well as on the local structural setting (e.g. Peccerillo
& Frezzotti 2015). On the basis of geochemical and isotopic
features, three distinct sectors have been identified in the arc
(Calanchi et al. 2002; Peccerillo 2005): 1) the western sector
includes the Alicudi and Filicudi islands and consists of
calc-alkaline basalt to andesite and minor dacites, characte-
rized by typical island arc signature; 2) the central sector,
including Salina, Vulcano, Lipari and Panarea islands, which
consists of calc-alkaline to shoshonitic mafic to silicic rocks,
with abundant rhyolites mainly erupted during the latest vol-
canic phases; 3) the eastern sector formed by the Island of
Stromboli characterized by calc-alkaline to potassic-alkaline
mafic-intermediate rocks showing isotopic incompatible
trace element ratios and radiogenic isotope signatures diffe-
rent from those of the western and central islands (Peccerillo
et al. 2013).
From the geochemical point of view, the studied volcani-
clastic sequence is characterized by arc signature, mostly fel-
sic with subordinate mafic compositions represented by two
andesites samples from VU4. Most of the pumices show
mainly dacitic and rhyolitic compositions, characterized by
CA and HKCA affinity (Fig. 8B), without significant varia-
bility inside each unit and among the different units. The vol-
canic arc signature is indicated by negative anomalies of Nb
and Zr and by the positive spike of Pb (Fig. 8C). Trace ele-
ments ratios of the most evolved pumices, such as Zr/Nb
(17÷21), Rb/Nb (5÷8) and Ba/Rb (5÷8) are slightly
variable.
The age of the volcaniclastic sequence and the chemical
composition of the studied products suggest that they could
be related to the oldest phases of the Aeolian Arc volcanism,
effectively excluding an origin from the younger volcanic
systems currently exposed above sea-level (De Rosa et al.
2003; Dolfi et al. 2007). Affinity with dacites found within
the oldest part of the Panarea volcanic complex dated 800 Ky
(Savelli 2002; Lucchi et al. 2013 and references therein) can
be considered.
The geochemical data we recorded are compared with
those of subaerial volcanic rocks from the Aeolian archi-
pelago (Peccerillo 2005) as well as with the coeval volcani-
clastic deposits outcropping along the Calabrian coast
(De Rosa et al. 2008). The comparison does not highlight any
clear correlation with the CA and HKCA rocks from the
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Aeolian islands (Fig. 9) especially regarding the trace ele-
ments and their ratios. In contrast, the comparison with data
of the coeval Pleistocene tephra outcropping along the Cala-
brian coast reveals similar Zr/Nb and Ba/Rb ratios. Accor-
ding to De Rosa et al. (2008) it could represent the product of
explosive activity from one or more volcanic centres active
in the Southern Tyrrhenian domain during the last one mil-
lion years. Such an eruption centre has been identified in the
seamount located 6 miles off the western coast of the Calabria
region (Loreto et al. 2015), (Fig. 9).
Combining all the recovered information, it seems very
unlikely that the Aeolian Islands are the origin of the studied
deposits (VU7, in particular), and difficult to explain the
presence of the deposits over the northern Sicilian coast
taking into account their distance (> 30 km) and their coarse
grain size. The seamount located offshore from the Capo
Vaticano promontory (Loreto et al. 2015) looks to be very far
away, (about 80 km to the North although compatible in age
and chemistry (De Rosa et al. 2008; De Ritis et al. 2010) with
the top located at shallow depth (about 70 m b.s.l.). The grain
size characteristics of the pyroclastic material of VU7 and
also of VU1, VU2, VU5, VU8 indicate a primary emplace-
ment at a distance of less than 5 km from the vent, on a deep
shore environment of the Sicilian continental margin,
and subsequently remobilization and final redeposition
away towards the northwest and north by means of sea
currents.
The existence of a subaerial or shallow-water volcanic edi-
fice located somewhere between the northern coast of Sicily,
the western coast of Calabria and the Aeolian Islands
(Fig. 10) would also be able to explain the abundance of
coarse angular lithic and pumiceous clasts (both up to
10–12 cm). This possibility cannot be rejected.
Conclusions
The results of this study highlight for the first time that
volcaniclastic deposits outcropping along the Tyrrhenian
coastline of the Peloritani Mountains (Sicily) are related to
recent (Lower-Middle Pleistocene) explosive activity in the
Southern Tyrrhenian sea. The results match those of similar
deposits spread over the Mesima-Gioia Tauro and Reggio
Calabria basins (De Rosa et al. 2008) for which a possible
explosive centre has been identified offshore from the Capo
Vaticano promontory (Loreto et al. 2015) while there is no
clear correlation with rocks from the subaerial portion of the
Aeolian archipelago.
The field investigations besides the sedimentological fea-
tures of the widespread volcaniclastic deposits suggest that
they underwent reworking by sea currents after the primary
emplacement. The volcaniclastic units can be identified as
the results of deposition of pyroclastic fall and/or flow related
to Vulcanian to Plinian type eruptions. Clasts underwent
Fig. 9. Rb, Zr/Nb, Ba/Rb and Rb/Nb versus Zr diagrams of analyzed pumice clasts compared with literature data of Aeolian Islands
(Peccerillo 2005) and Calabrian volcanic products of similar in age (De Rosa et al. 2008). Symbols are the same as in Fig. 8.
DI BELLA, ITALIANO, SABATINO, TRIPODO, BALDANZA, CASELLA, PINO, RASA’ and RUSSO
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syn- to post-eruptive remobilization onto the seafloor by den-
sity currents. Alternatively, they may represent the extension
of subaerial pyroclastic flows entering into the sea and trig-
gering subaqueous dense currents.
The volcaniclastic units probably derive from a common
source as testified by a single trend of magmatic differentia-
tion. The presence of the volcaniclastic deposits included in
deep water marine clayey sediments allow us to conclude
that intense and prolonged explosive mafic to felsic calc-
alkaline and high-K calc-alkaline activity occurred at a vol-
canic centre or centres located in the Southern Tyrrhenian Sea.
Acknowledgements: This paper is dedicated to the memory
of our friend, Prof. Riccardo Rasà. The authors are grateful to
the 2 anonymous reviewers for their constructive reviews
that improved the quality of the paper. They also thank Mauro
Coltelli (INGV Catania) for his useful suggestions. The XRF
Laboratory of the University of Modena and Reggio Emilia
is acknowledged for the technical support during the chemi-
cal analyses.
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