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<OAI-PMH schemaLocation=http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd> <responseDate>2018-01-15T18:22:22Z</responseDate> <request identifier=oai:HAL:hal-01356155v1 verb=GetRecord metadataPrefix=oai_dc>http://api.archives-ouvertes.fr/oai/hal/</request> <GetRecord> <record> <header> <identifier>oai:HAL:hal-01356155v1</identifier> <datestamp>2018-01-11</datestamp> <setSpec>type:COMM</setSpec> <setSpec>subject:sdu</setSpec> <setSpec>collection:CNRS</setSpec> <setSpec>collection:UNIV-AG</setSpec> <setSpec>collection:UNIV-ORLEANS</setSpec> <setSpec>collection:ISTO</setSpec> <setSpec>collection:GM</setSpec> <setSpec>collection:OSUC</setSpec> <setSpec>collection:BRGM</setSpec> <setSpec>collection:AGROPOLIS</setSpec> <setSpec>collection:GIP-BE</setSpec> <setSpec>collection:INSU</setSpec> <setSpec>collection:B3ESTE</setSpec> <setSpec>collection:UNIV-MONTPELLIER</setSpec> </header> <metadata><dc> <publisher>HAL CCSD</publisher> <title lang=en>The Mn-Carbonate Rich Black Shales of the Bangombe Plateau, Francevillian Basin, Gabon</title> <creator>DUBOIS, Manon</creator> <creator>LOPEZ, Michel</creator> <creator>Orberger, Beate</creator> <creator>Rodriguez, Celine</creator> <creator>Boussafir, Mohammed</creator> <creator>Dreux, Geoffrey</creator> <creator>Rodrigues, Sophie</creator> <creator>Pambo, Florent</creator> <contributor>Géosciences Montpellier ; Université des Antilles et de la Guyane (UAG) - Institut national des sciences de l'Univers (INSU - CNRS) - Université de Montpellier (UM) - Centre National de la Recherche Scientifique (CNRS)</contributor> <contributor>Institut des Sciences de la Terre d'Orléans - UMR7327 (ISTO) ; Bureau de Recherches Géologiques et Minières (BRGM) (BRGM) - Institut national des sciences de l'Univers (INSU - CNRS) - Université d'Orléans (UO) - Centre National de la Recherche Scientifique (CNRS)</contributor> <contributor>COMILOG</contributor> <source>13th Biennial SGA Meeting</source> <coverage>Nancy, France</coverage> <identifier>hal-01356155</identifier> <identifier>https://hal.archives-ouvertes.fr/hal-01356155</identifier> <source>https://hal.archives-ouvertes.fr/hal-01356155</source> <source>13th Biennial SGA Meeting, Aug 2015, Nancy, France. pp.1905-1908, Mineral resources in sustainable world</source> <language>en</language> <subject lang=en>Rhodochrosite Kutnohorite</subject> <subject lang=en>Dolomite</subject> <subject lang=en>black shales</subject> <subject lang=en>Proterozoic</subject> <subject lang=en>Gabon</subject> <subject lang=en>Organic matter</subject> <subject>[SDU.STU.MI] Sciences of the Universe [physics]/Earth Sciences/Mineralogy</subject> <type>info:eu-repo/semantics/conferenceObject</type> <type>Conference papers</type> <description lang=en>Eight drill cores cutting through the Mn-carbonate bearing black shales from the Bangombé Plateau were studied. Mn-carbonates (up to 80 m thick) are underlain by laminated pyrite rich shales with organic carbon contents of about 4 wt. % and MnO contents of about 6 wt. %. Mn and Fe, S poor shales are intercalated. Mn-carbonate rich shales (20-29 wt. % MnO) have low contents of phyllosilicates, but are rich in organic carbon (about 7 wt. %) with moderate S contents (about 2 wt. %). All shale facies were deposited in a closed basin through suspension settling and precipitations under anoxic conditions. The Mn-carbonates, towards the top, were formed most likely under suboxic conditions. Pyrite and Mn-carbonates are characterized by bacteriomorphous structures. The latter are composed of micrometric carbonates finely intergrown with clays, quartz and organic matter. They formed around and corroded the dolomite and/or organic matter. Mn-carbonates and pyrite both form also several tenths of micrometer large agglomerates and sub-automorphous grains. The agglomerates can be attributed to evolving diagenesis. Carbonate chemistry varies mainly from rhodochrosite to dolomite. The present results point to primary microbial Mn-carbonate formation. No signs for a Mn-oxide precursor were detected. Slumping and shearing structures, distortion and disruption of thin pyrite beds indicate synsedimentary deformations.</description> <date>2015-08-24</date> </dc> </metadata> </record> </GetRecord> </OAI-PMH>