georefid:2013-007323SEDIS Publication Catalogue
ana.macario@awi.de
http://sedis.iodp.org/pub-catalogue/informationpointOfContact2013-07-08T00:00:00Zhttp://sedis.iodp.org/pub-catalogue/index.php?id=10.1016/j.margeo.2012.08.008<gco:CharacterString>Mass wasting processes along the Owen Ridge (northwest Indian Ocean)</gco:CharacterString>2012-01-01publicationgeorefid:2013-007323doi:10.1016/j.margeo.2012.08.008Rodriguez, MathieuUniversite Pierre and Marie Curie, Institut des Sciences de la Terre de Paris, Paris, FranceauthorFournier, MarcEcole Normale Superieure de Paris, FranceauthorChamot-Rooke, NicolasUniversite Bordeaux 1, FranceauthorHuchon, PhilippeauthorZaragosi, SebastienauthorRabaute, AlainauthorElsevier, Amsterdam, NetherlandspublisherdocumentHardcopyMarine Geology326-32880-100The Owen Ridge is a prominent relief that runs parallel to the coast of Oman in the NW Indian Ocean and is closely linked to the Owen Fracture Zone, an 800-km-long active fault system that accommodates today the Arabia-India strike-slip motion. Several types of mass failures mobilizing the pelagic cover have been mapped in details along the ridge using multibeam bathymetry and sediment echosounder. Here we present a synthetic map of the different types of mass wasting features observed along the ridge and we further establish a morphometric analysis of submarine landslides. The spatial variation of failure morphology is strongly related to the topography of the basement. The highest volumes of multi-events generated slides are mobilized along the southern portion of the ridge. There, the estimated volume of evacuated material during a slide is up to 45 km (super 3) . Combining these new observations with re-interpreted ODP seismic lines (Leg 117) documents sporadic mass wasting events through time along the southern segment of the ridge since its uplift in the Early Miocene, with a typical recurrence rate of the order of 10 (super 5) -10 (super 6) years. Although seismicity may still be the final triggering process, mass wasting frequency is mainly controlled by the slow pelagic sedimentation rates and hence, time needed to build up the 40-80 m thick pelagic cover required to return to a mechanically unstable pelagic cover. Abstract Copyright (2012) Elsevier, B.V.completedStratigraphyApplied geophysicsacoustical methodsacoustical profilesArabian PeninsulaArabian SeaAsiabathymetryCenozoiccontinental marginDeep Sea Drilling ProjectDSDP Site 222echo soundingfailuresgeophysical methodsgeophysical profilesgeophysical surveysIndian OceanIndus FanLeg 117Leg 23mass movementsMioceneNeogenenorthwestern Indian OceanOcean Drilling Programocean floorsODP Site 721OmanOwen fracture zoneOwen Ridgeseamountsslumpingsonar methodssurveysTertiaryurn:org.iodp:exp:117urnlargerWorkCitationcampaignurn:org.iodp:exp:23urnlargerWorkCitationcampaignurn:org.iodp:exp:23:site:222urnlargerWorkCitationstudyurn:org.iodp:exp:23urnlargerWorkCitationcampaignurn:org.iodp:exp:117:site:721urnlargerWorkCitationstudyurn:org.iodp:exp:117urnlargerWorkCitationcampaignEnglishgeoscientificInformation58.000063.000015.000022.0000