An Updated Reconstruction of Basaltic Crust Emplacement in Tyrrhenian Sea, Italy
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The Structure and Formation of the Tyrrhenian Basin in the Western Mediterranean Back-Arc Setting
Instituto de Ciencias del Mar Departament de Geodinàmica i Unidad deTecnología Marina Geofísica Barcelona Center for Consejo Superior de Subsurface Imaging Investigaciones Científicas The structure and formation of the Tyrrhenian basin in the Western Mediterranean back-arc setting Formación y estructura de la cuenca del Tirreno en el contexto de retrarco del Mediterraneo Occidental Memoria de Tesis Doctoral presentada por Manuel Prada Dacasa para optar al grado de Doctor en Geología por la Universidad de Barcelona Esta memoria se ha realizado dentro del programa de Doctorado de Ciencias de la Tierra de la Universidad de Barcelona bajo la dirección del Dr. Valentí Sallarès Casas y Dr. César Rodríguez Ranero, y bajo la tutela de Pilar Queralt Capdevila Barcelona, Enero de 2014 Para todo aquel que desee descubrir… Agradecimientos Para empezar, quiero agradecer a mis dos directores de Tesis, Valentí y César, el esfuerzo dedicado en mí durante estos cuatro años y medio de Doctorado. A Valentí, por su disposición a ayudar y la confianza depositada en mí, pero sobre todo por ser un buen consejero y maestro, gracias. A César, por enseñarme a ser un poco más exigente conmigo mismo, y por sus lecciones geológicas, su amplia visión me ha permitido “empezar” a comprender algunos de los procesos de formación de cuencas extensivas. Gracias a los dos por haber hecho que el camino sea un poco más llano. Quiero agradecer también a Nevio por haberme acogido en Bolonia y haber hecho que mi estancia allí sea provechosa. Sus conocimientos de la cuenca Tirrena son realmente extensos y han sido muy útiles para poder finalizar esta tesis. -
Holocene Evolution of the Burano Paleo-Lagoon (Southern Tuscany, Italy)
water Article Holocene Evolution of the Burano Paleo-Lagoon (Southern Tuscany, Italy) Maurizio D’Orefice 1, Piero Bellotti 2, Adele Bertini 3 , Gilberto Calderoni 4, Paolo Censi Neri 1, Letizia Di Bella 5,*, Domenico Fiorenza 1, Luca Maria Foresi 6,7, Markella Asimina Louvari 8, Letizia Rainone 3,Cécile Vittori 9 , Jean-Philippe Goiran 10, Laurent Schmitt 9 , Pierre Carbonel 10, Frank Preusser 11 , Christine Oberlin 12, Francesca Sangiorgi 13 and Lina Davoli 5 1 Italian Institute for Environmental Protection and Research, ISPRA, Department for the Geological Survey of Italy, 00144 Rome, Italy; maurizio.dorefi[email protected] (M.D.); [email protected] (P.C.N.); domenico.fi[email protected] (D.F.) 2 AIGeo, Italian Association of Physical Geography and Geomorphology, c/o Department of Earth Sciences, Sapienza, University of Rome, 00185 Rome, Italy; [email protected] 3 Department of Earth Sciences, University of Florence, 50121 Florence, Italy; adele.bertini@unifi.it (A.B.); [email protected]fi.it (L.R.) 4 Institute of Environmental Geology and Geoengineering, CNR, c/o Department of Earth Sciences, Sapienza, University of Rome, 00185 Rome, Italy; [email protected] 5 Department of Earth Sciences, Sapienza, University of Rome, 00185 Rome, Italy; [email protected] 6 Department of Physical sciences, Earth and environment University of Siena, 53100 Siena, Italy; [email protected] 7 Institute of Geosciences and Earth resources, CNR, c/o Research Area of Pisa, 1–56124 Pisa, Italy 8 Faculty of Geology -
Pontine Islands
Pontine islands Ponza Day One and Two: Ponza The Pontine islands have always been renowned for the beauty of their surrounding sea and sea-beds Ponza is the island's main settlement and requires a couple of days to be fully explored. It’s très chic, so be prepared to bump into football players and royals. It’s a labyrinth of orange-purple sea grottos, talcum powder- like beaches, white granite rocks and pirates caves where scuba divers still search for hidden treasures. Don’t miss the chance to take a trip to the wonderful ancient Roman sea caves commonly referred to as the Grotte di Pilato. The caves (four in all, connected by underwater tunnels) were hand-excavated by the Romans and used as a murenario (eel farm) in the 1st century A.D., when the emperor Augustus first built a villa on the hill above. Then, circumnavigate the island to discover all of its stunning bays, like Chiaia di Luna, Capo Bianco, Cala Feola etc. At sunset, pay a visit to the must-go aperitif at the Frontone, which is a rustic outdoor bar set up among the trees just behind the sand. In the evening, take a walk into town and stroll along the picturesque ancient Roman harbour made of colourful fishermen dwellings and prehistoric grottos turned into studios, and where evening drinks are served on rooftops. As for dinner, if you wish to get off your yacht, you can choose among many typical restaurants; we suggest you the Restaurants “Acquapazza” and “Chiaia di Luna” for a romantic poolside dinner. -
SPECIALE BORGHI Della CAMPANIA2
SPECIALE BORGHI della CAMPANIA2 COPIA OMAGGIO edizione speciale FIERE un parco di terra e di mare laboratorio di biodiversità a park of land and sea R laboratory of biodiversity www.cilentoediano.it GLI 80 COMUNI DEL PARCO NAZIONALE DEL CILENTO VALLO DI DIANO E ALBURNI Agropoli Gioi Roccagloriosa Aquara Giungano Rofrano Ascea Laureana Cilento Roscigno Auletta Laurino Sacco Bellosguardo Laurito Salento Buonabitacolo Lustra San Giovanni a Piro Camerota Magliano Vetere San Mauro Cilento Campora Moio della Civitella San Mauro la Bruca Cannalonga Montano Antilia San Pietro al Tanagro Capaccio Monte San Giacomo San Rufo Casal velino Montecorice Sant’Angelo a Fasanella Casalbuono Monteforte Cilento Sant’Arsenio Casaletto Spartano Montesano sulla Marcellana Santa Marina Caselle in Pittari Morigerati Sanza Castel San Lorenzo Novi Velia Sassano Castelcivita Omignano Serramezzana Castellabate Orria Sessa Cilento Castelnuovo Cilento Ottati Sicignano degli Alburni Celle di Bulgheria Perdifumo Stella Cilento Centola Perito Stio Ceraso Petina Teggiano Cicerale Piaggine Torre Orsaia Controne Pisciotta Tortorella Corleto Monforte Polla Trentinara Cuccaro Vetere Pollica Valle dell’Angelo Felitto Postiglione Vallo della Lucania Futani Roccadaspide I 15 COMUNI NELLE AREE CONTIGUE DEL PARCO NAZIONALE DEL CILENTO VALLO DI DIANO E ALBURNI Albanella Ogliastro Cilento Sala Consilina Alfano Padula Sapri Atena Lucana Pertosa Torchiara Caggiano Prignano Cilento Torraca Ispani Rutino Vibonati zona del parco Parco Nazionale del Cilento, Vallo di Diano e Alburni Ai Focei si deve, invece, la fondazione di Velia (VI secolo a.C.), patria della scuola Eleatica di Parmenide che ha fecon- dato e illuminato la storia della filosofia occidentale. La Certosa di San Lorenzo di Padula costituisce un vero e proprio gioiello dell’architettura monastica, principale esem- pio del Barocco del Mezzogiorno, inserita tra i Monumenti Internazionali già nel lontano 1882. -
2. the Tyrrhenian Sea Before Leg 1071
2. THE TYRRHENIAN SEA BEFORE LEG 1071 J. P. Rehault2, J. Mascle2, A. Fabbri3, E. Moussat4, and M. Thommeret2 The Tyrrhenian Sea (Fig. 1) is a small triangular marine ba• is bisected by the Marsili Seamount, the largest volcano within sin surrounded by Corsica, Sardinia, Sicily, and peninsular It• the Tyrrhenian Sea, culminating at 505 m. The Magnaghi, Vav• aly, lying between the Neogene Western Mediterranean Basin ilov, and Marsili volcanoes are tens of kilometers (30-50) in and the Mesozoic Ionian and Levantine Basins (Biju Duval et length. They are similarly elongated and subparallel with their al., 1978). The Tyrrhenian Sea has been, for more than a dec• long axis trending N10°-20°E. ade, the subject of many geophysical and geological explorations summarized by Morelli (1970), Boccaletti and Manetti (1978), Continental Margins Lort (1978), Moussat (1983), Duchesnes et al. (1986), and Re• The northern Sicily and western Calabria continental mar• hault et al. (1984, 1987). The evolution of the Tyrrhenian Sea is gins average 100-120 km in width. They are characterized by a unusual and intriguing in that the basin has developed both system of close-spaced sediment-filled upper slope basins, the back of a subduction-volcanic-arc system (the Calabrian arc) Cefalu, Gioia, and Paola Basins (Perityrrhenian Basins, Selli, and inside of successive collision zones (Alpine and Apennines 1970; Basin and Range System, Hsu, 1978). An arcuate belt of s.l.). Collision is still active both east and south of the Tyrrhe• volcanoes known as the Eolian Islands follows the curve of the nian in the peninsular Apennines and Sicily. -
The Historical Geothermal Investigations of Campanian Volcanoes: Constrains for Magma Source Location and Geothermal Potential Assessment S
GNGTS 2011 SESSIONE 1.3 THE HISTORICAL GEOTHERMAL INVESTIGATIONS OF CAMPANIAN VOLCANOES: CONSTRAINS FOR MAGMA SOURCE LOCATION AND GEOTHERMAL POTENTIAL ASSESSMENT S. Carlino, G. De Natale, C. Troise, R. Somma Istituto Nazionale di Geofisica e Vulcanologia, sezione di Napoli “Osservatorio Vesuviano”, Napoli, Italy The Campania region is characterized by the presence of the active volcanoes of Phlegrean dis- trict (Campi Flegrei and Ischia calderas), west to the city of Naples, and Somma-Vesuvius to the east. Most of this area is marked by the occurrence of anomalous high heat flow and temperature at very shallow depth (Geothermal gradient: 150-200°C at Campi Flegrei and Ischia respectively; 30°C/km at Vesuvius. Heat flow: Mofete, 160mWm-2; S.Vito and Mt.Nuovo, 160mWm-2; Agnano:120 mWm-2; Ischia western and southern sector, 560-580mWm-2). These features are relat- ed to different causes: the rising of the Moho (~ 20 km of depth) and the thinning of the crust in the central part of the Tyrrhenian Basin, due to the spreading of the sea floor; the migration of magma at a minimum depth of 8-10 km due to the buoyancy forces; the geothermal fluids circulation above the magmatic sources. The study of the geothermal systems of Campanian volcanoes represents an important tool for the understanding of volcano dynamic and associated risk, and also for the quan- tification of the geothermal potential for thermal and electric energy production. Pioneering researches of geothermal resources were carried out in Campanian region since 1930. Such researches were part of the Energy National Plan, aimed to better constrain the geother- mal potential in the volcanic district of Campania (Vesuvius, Campi Flegrei caldera and Ischia Island), and were supported by a Joint Venture between ENEL and AGIP Companies. -
West Mediterranean) (Peracarida: Isopoda
Fragmenta entomologica, 51 (2): 217–223 (2019) eISSN: 2284-4880 (online version) pISSN: 0429-288X (print version) Research article Submitted: August 25th, 2019 - Accepted: October 8th, 2019 - Published: November 15th, 2019 Insights into the late-Sixties taxocenosis of Oniscidea from the Pontine islands (West Mediterranean) (Peracarida: Isopoda) Gabriele GENTILE1 ,*, Roberto ARGANO 2, Stefano TAITI 3,4 1 Dipartimento di Biologia, Università di Roma Tor Vergata - Via della Ricerca Sientifica 1, 00133 Rome, Italy [email protected] 2 Dipartimento di Biologia e Biotecnologie “Charles Darwin”, Università degli Studi “La Sapienza” - Viale dell’Università 32 00185 Rome, Italy 3 Istituto di Ricerca sugli Ecosistemi Terrestri, Consiglio Nazionale delle Ricerche - Via Madonna del Piano 10, 50019 Sesto Fiorentino (Florence), Italy 4 Museo di Storia Naturale dell’Università di Firenze, Sezione di Zoologia “La Specola” - Via Romana 17, 50125 Florence, Italy * Corresponding author Abstract We report and discuss faunistic data of Oniscidea inhabiting the Pontine islands, a group of five small volcanic islands and several islets in the Tyrrhenian Sea, located about 60 km from the Italian mainland. Data here presented were primarily obtained from the examina- tion of the material collected during a three-year (1965-1968) research program supported by the Italian National Council of Research and aimed at investigating Mediterranean small island faunas, including Oniscidea. Despite the sampling was not specifically directed at Oniscidea, these data may provide insights into the structure of the Oniscidean taxocenosis of the islands as it existed fifty years ago. Thirty-five species belonging to 11 families, 8 ecological and 7 biogeographical classes were found on these islands. -
Ocean Drilling Program Initial Reports Volume
1. INTRODUCTION1 Shipboard Scientific Party2 The Tyrrhenian Sea is the small triangular sea surrounded by and Ryan, 1986). Furthermore, because the Tyrrhenian is peninsular Italy, Sicily, Sardinia, and Corsica (Fig. 1). Drilling bounded to the northeast and southeast by orogenic belts (see objectives for Leg 107 of the Ocean Drilling Program consid• "A Review of Circum-Tyrrhenian Regional Geology" chapter, ered the Tyrrhenian Sea from three different perspectives: (1) as this volume), interactions between extension and collision could a landlocked back-arc basin, (2) as a young passive margin, and be explored and the basin could be regarded as a model for (3) as a stratigraphic type locality. landlocked back-arc basin evolution. In common with other back-arc basins, the Tyrrhenian Sea In common with other passive margins, the western Tyrrhe• exhibits a Benioff zone (Gasparini et al., 1982), a calc-alkaline nian Sea is floored by continental crust which has been stretched volcanic belt (Barberi et al., 1974; Selli et al., 1977), thinned and thinned by listric faulting (Fabbri et al., 1981; Malinverno crust on the margins (Panza et al., 1980), tholeiitic (mid-ocean et al., 1981; Rehault et al., 1985). A principal goal of drilling on ridge basalt) volcanism (Barberi et al., 1978; Dietrich et al., the Tyrrhenian margin was to determine the timing and rate of 1978) high heat flow (Delia Vedova et al., 1984; Hutchinson et extension and subsidence during the stretching phase as well as al., 1985), and high-amplitude magnetic anomalies (Bolis -
2. the Miocene/Pliocene Boundary in the Eastern Mediterranean: Results from Sites 967 and 9691
Robertson, A.H.F., Emeis, K.-C., Richter, C., and Camerlenghi, A. (Eds.), 1998 Proceedings of the Ocean Drilling Program, Scientific Results, Vol. 160 2. THE MIOCENE/PLIOCENE BOUNDARY IN THE EASTERN MEDITERRANEAN: RESULTS FROM SITES 967 AND 9691 Silvia Spezzaferri,2 Maria B. Cita,3 and Judith A. McKenzie2 ABSTRACT Continuous sequences developed across the Miocene/Pliocene boundary were cored during Ocean Drilling Project (ODP) Leg 160 at Hole 967A, located on the base of the northern slope of the Eratosthenes Seamount, and at Hole 969B, some 700 km to the west of the previous location, on the inner plateau of the Mediterranean Ridge south of Crete. Multidisciplinary investiga- tions, including quantitative and/or qualitative study of planktonic and benthic foraminifers and ostracodes and oxygen and car- bon isotope analyses of these microfossils, provide new information on the paleoceanographic conditions during the latest Miocene (Messinian) and the re-establishment of deep marine conditions after the Messinian Salinity Crisis with the re-coloni- zation of the Eastern Mediterranean Sea in the earliest Pliocene (Zanclean). At Hole 967A, Zanclean pelagic oozes and/or hemipelagic marls overlie an upper Messinian brecciated carbonate sequence. At this site, the identification of the Miocene/Pliocene boundary between 119.1 and 119.4 mbsf, coincides with the lower boundary of the lithostratigraphic Unit II, where there is a shift from a high content of inorganic and non-marine calcite to a high content of biogenic calcite typical of a marine pelagic ooze. The presence of Cyprideis pannonica associated upward with Paratethyan ostracodes reveals that the upper Messinian sequence is complete. -
Mass Failures Scenarios from the Flanks of the Marsili Submarine
Geophysical Research Abstracts Vol. 21, EGU2019-10621, 2019 EGU General Assembly 2019 © Author(s) 2019. CC Attribution 4.0 license. Mass failures scenarios from the flanks of the Marsili submarine volcano, Tyrrhenian sea, and consequent tsunami hazard Glauco Gallotti (1), Stefano Tinti (1), Filippo Zaniboni (1), Gianluca Pagnoni (1), and Claudia Romagnoli (2) (1) University of Bologna, DIFA, Geophysics, Bologna, Italy ([email protected]), (2) University of Bologna, BIGEA, Geology, Bologna, Italy The Marsili Seamount (MS) is the biggest volcanic structure in Europe, located in the axial portion of the Marsili Basin, in the southern part of the Tyrrhenian sea. The MS is 70 km long, 30 km wide and about 3000 m high, arising from a depth of - 3500 m to - 500 m. In this work, we present a number of scenarios of possible mass failures occurring on the eastern flank of this structure, covering a broad range of volumes. The landslides are simulated by means of two different numerical models. In one model, that is a new original mechanical model and is implemented in the numerical code UBO-Inter, the moving body is represented by a number of point masses that can be seen as the projection on the sliding surface of the center of mass of the elements the system is discretized into. The other (implemented in the code UBO-Block) is based on the partition of the landslide into a matrix of blocks whose dynamics is computed through a Lagrangian approach. The mass failures modelled for the Marsili have the potential to be tsunamigenic and hence our study may be also seen as a significant contribution to tsunami hazard assessment in the pery-Tyrrhenian region. -
GEOLOGIC TIME SCALE V
GSA GEOLOGIC TIME SCALE v. 4.0 CENOZOIC MESOZOIC PALEOZOIC PRECAMBRIAN MAGNETIC MAGNETIC BDY. AGE POLARITY PICKS AGE POLARITY PICKS AGE PICKS AGE . N PERIOD EPOCH AGE PERIOD EPOCH AGE PERIOD EPOCH AGE EON ERA PERIOD AGES (Ma) (Ma) (Ma) (Ma) (Ma) (Ma) (Ma) HIST HIST. ANOM. (Ma) ANOM. CHRON. CHRO HOLOCENE 1 C1 QUATER- 0.01 30 C30 66.0 541 CALABRIAN NARY PLEISTOCENE* 1.8 31 C31 MAASTRICHTIAN 252 2 C2 GELASIAN 70 CHANGHSINGIAN EDIACARAN 2.6 Lopin- 254 32 C32 72.1 635 2A C2A PIACENZIAN WUCHIAPINGIAN PLIOCENE 3.6 gian 33 260 260 3 ZANCLEAN CAPITANIAN NEOPRO- 5 C3 CAMPANIAN Guada- 265 750 CRYOGENIAN 5.3 80 C33 WORDIAN TEROZOIC 3A MESSINIAN LATE lupian 269 C3A 83.6 ROADIAN 272 850 7.2 SANTONIAN 4 KUNGURIAN C4 86.3 279 TONIAN CONIACIAN 280 4A Cisura- C4A TORTONIAN 90 89.8 1000 1000 PERMIAN ARTINSKIAN 10 5 TURONIAN lian C5 93.9 290 SAKMARIAN STENIAN 11.6 CENOMANIAN 296 SERRAVALLIAN 34 C34 ASSELIAN 299 5A 100 100 300 GZHELIAN 1200 C5A 13.8 LATE 304 KASIMOVIAN 307 1250 MESOPRO- 15 LANGHIAN ECTASIAN 5B C5B ALBIAN MIDDLE MOSCOVIAN 16.0 TEROZOIC 5C C5C 110 VANIAN 315 PENNSYL- 1400 EARLY 5D C5D MIOCENE 113 320 BASHKIRIAN 323 5E C5E NEOGENE BURDIGALIAN SERPUKHOVIAN 1500 CALYMMIAN 6 C6 APTIAN LATE 20 120 331 6A C6A 20.4 EARLY 1600 M0r 126 6B C6B AQUITANIAN M1 340 MIDDLE VISEAN MISSIS- M3 BARREMIAN SIPPIAN STATHERIAN C6C 23.0 6C 130 M5 CRETACEOUS 131 347 1750 HAUTERIVIAN 7 C7 CARBONIFEROUS EARLY TOURNAISIAN 1800 M10 134 25 7A C7A 359 8 C8 CHATTIAN VALANGINIAN M12 360 140 M14 139 FAMENNIAN OROSIRIAN 9 C9 M16 28.1 M18 BERRIASIAN 2000 PROTEROZOIC 10 C10 LATE -
Istock - Getty Images LATIUM
82 Rome, Colosseum, © belenox - iStock - Getty Images LATIUM Latium is an area worth getting to know, beaches, the lovely cli's, all along the a land rich in blends of art, culture and coastline, from Tarquinia beach to the nature, the crossroads of Mediterranean white sand of Sabaudia with its famous civilization and of Etruscan, Sabine, Sam- dunes, to the clear waters of San Felice al nite, Campanian and Latin peoples. The Circeo and Sperlonga, an authentic region probably got its name from the Tyrrhenian fishing village, down to Gae- Latins, whose most recent history min- ta, with its split mountain overhanging gles with that of Rome and the Pontifical the sea. There are very charming under- State, the Terra del Lavoro and the King- water itineraries along the lovely seabeds dom of the Two Sicilies. A compound of the Pontine islands, to underwater memory that only a few dozen years ago caves, fields of posidonia, lobsters and recovered its role as a unique tourist at- even submerged shipwrecks. traction, together with that of the capital The counterpoint to the sea are the city. Nowadays the region stands out beautiful mountains, rich in avifauna and with its many charms, from spas to spec- biodiversity, which mark out the region’s tacular lakes, from gentle hilly scenery to ridge and follow its outline from the bor- charming beaches, from archaeology ders of Tuscany to Campania, from the and art to the great wealth of traditions. Rieti salt road to the Abruzzo National Latium is a wonderland, the essence of Park. Then there are the Monti della Laga natural beauty, historic remains and a and della Duchessa, the magical Simbru- variety of food and wine related to the ini mountains, the heart of Latium, the soil and the simplicity and wholesome- Ausoni mountains and the Aurunci, ness of the crops.