Please use this identifier to cite or link to this item: http://hdl.handle.net/2122/6189
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dc.contributor.authorallEtiope, G.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallSavini, A.; ULR CoNISMa-Department of Geological Sciences and Geotechnologies–University of Milano-Bicocca, Piazza della Scienza 4, 20126 Milano, Italyen
dc.contributor.authorallLo Bue, N.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallFavali, P.; Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.authorallCorselli, C.; ULR CoNISMa-Department of Geological Sciences and Geotechnologies–University of Milano-Bicocca, Piazza della Scienza 4, 20126 Milano, Italyen
dc.date.accessioned2010-11-08T07:01:18Zen
dc.date.available2010-11-08T07:01:18Zen
dc.date.issued2010en
dc.identifier.urihttp://hdl.handle.net/2122/6189en
dc.description.abstractThe “Santa Maria di Leuca” Cold-Water Coral (CWC) province (northern Ionian Sea) was investigated for the first time to detect eventual occurrence of methane anomalies as a possible indication of hydrocarbon seepage stimulating the coral growth. Most coral mounds have developed in correspondence with tectonic scarps and faults, orthogonal to the southern margin and trending NW-SE, which could be potential sites of gas escape. A visual and instrumental inspection was performed by using a new deep-sea probe equipped with video-cameras, sonar, CTD, methane sensors, and a water sampler. Eight areas were explored by 10 surveys, depths ranging from 380 to 1100 m, for a total of more than 26 h of continuous video and instrumental recording. Sediments were also sampled by gravity corers and analysed in laboratory. The images allowed to assess distribution, abundance and geometry of the colonies, most of which are developed on morphological highs often characterised by tectonic scarps. All data indicate however the lack of a significant occurrence of methane, both in seawater and sediments. No direct or indirect expressions of gas seepage were recognised on the seabed. Weak methane anomalies were detected only in seawater at the base of some fault-linked scarps, where more reducing conditions and bacterial methanogenesis are possibly enhanced by less water circulation. The faults are not fluid-bearing as previously suggested by high-resolution geophysical signatures. The development of the coral colonies thus cannot be attributed to seeping fluids, but to a favourable physiographic position with exposure to nutrient-rich currents.en
dc.language.isoEnglishen
dc.publisher.nameElsevieren
dc.relation.ispartofDeep-SeaResearch IIen
dc.relation.ispartofseries/ 57 (2010)en
dc.relation.isversionofhttp://hdl.handle.net/2122/5540en
dc.subjectMethaneen
dc.subjectCoralsen
dc.subjectSeepageen
dc.subjectMarine geologyen
dc.titleDeep-sea survey for the detection of methane at the “Santa Maria di Leuca” cold-water coral mounds (Ionian Sea, South Italy)en
dc.typearticleen
dc.description.statusPublisheden
dc.type.QualityControlPeer-revieweden
dc.description.pagenumber431-440en
dc.subject.INGV04. Solid Earth::04.04. Geology::04.04.12. Fluid Geochemistryen
dc.identifier.doi10.1016/j.dsr2.2009.08.020en
dc.description.obiettivoSpecifico4.5. Studi sul degassamento naturale e sui gas petroliferien
dc.description.journalTypeJCR Journalen
dc.description.fulltextrestricteden
dc.contributor.authorEtiope, G.en
dc.contributor.authorSavini, A.en
dc.contributor.authorLo Bue, N.en
dc.contributor.authorFavali, P.en
dc.contributor.authorCorselli, C.en
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentULR CoNISMa-Department of Geological Sciences and Geotechnologies–University of Milano-Bicocca, Piazza della Scienza 4, 20126 Milano, Italyen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentIstituto Nazionale di Geofisica e Vulcanologia, Sezione Roma2, Roma, Italiaen
dc.contributor.departmentULR CoNISMa-Department of Geological Sciences and Geotechnologies–University of Milano-Bicocca, Piazza della Scienza 4, 20126 Milano, Italyen
item.openairetypearticle-
item.cerifentitytypePublications-
item.languageiso639-1en-
item.grantfulltextrestricted-
item.openairecristypehttp://purl.org/coar/resource_type/c_18cf-
item.fulltextWith Fulltext-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptDip. Scienze Geologiche e Geotecnologie, Universita` di Milano-Bicocca, P.za della Scienza 4, 20126 Milano, Italy-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptIstituto Nazionale di Geofisica e Vulcanologia (INGV), Sezione Roma2, Roma, Italia-
crisitem.author.deptUniversita` di Milano-Bicocca Dipartimento di Scienze Geologiche e Geotecnologiche, Piazza dell’Ateneo Nuovo 1, 20126 Milan, Italy-
crisitem.author.orcid0000-0001-8614-4221-
crisitem.author.orcid0000-0002-5818-5947-
crisitem.author.orcid0000-0002-5160-941X-
crisitem.author.orcid0000-0002-0810-0263-
crisitem.author.orcid0000-0002-0319-0191-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.author.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.classification.parent04. Solid Earth-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
crisitem.department.parentorgIstituto Nazionale di Geofisica e Vulcanologia-
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