georefid:2006-047648SEDIS Publication Catalogueana.macario@awi.dehttp://sedis.iodp.org/pub-catalogue/informationpointOfContact2011-06-23T00:00:00Zhttp://sedis.iodp.org/pub-catalogue/index.php?id=2006-047648<gco:CharacterString>Australasian microtektites in the South China Sea; implications regarding the location and size of the source crater</gco:CharacterString>2003-01-01publicationgeorefid:2006-047648Glass, B. P.University of Delaware, Geology Department, Newark, DE, United StatesauthorLunar and Planetary Science Conference, Houston, TX, United StatespublisherdocumentDigitalIn: Anonymous, Lunar and planetary science, XXXIV; papers presented to the Thirty-fourth lunar and planetary science conference34The highest concentration of Australasian microtektites and the highest ratio of unmelted ejecta to microtektites has been found in at ODP Hole 1144A in the northern South China Sea. These, and other data, were used to reevaluate the location and size of the Australasian strewn field source crater.completedPetrology of meteorites and tektitesAsiaAustralasian strewn fieldCambodiacoesitecorrelation coefficientejectaFar Eastframework silicatesimpact cratersimpact featuresLaosLeg 184microtektitesmorphologyNorth PacificNorthwest PacificOcean Drilling ProgramODP Site 1144Pacific Oceanprovenancequartzsilica mineralssilicatessizeSouth China Seastatistical analysisstishovitestrewn fieldstektitesThailandthicknessWest PacificX-ray diffraction dataurn:org.iodp:exp:184urnlargerWorkCitationcampaignurn:org.iodp:exp:184:site:1144urnlargerWorkCitationstudyurn:org.iodp:exp:184urnlargerWorkCitationcampaignEnglishgeoscientificInformation115.1818117.250810.535420.0311application/pdfunknownSEDIS Publication Catalogueana.macario@awi.dehttp://sedis.iodp.org/pub-catalogue/informationpointOfContacthttp://www.lpi.usra.edu/meetings/lpsc2003/pdf/1092.pdfdownload