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• W2099720117 abstract "Other| October 01, 2003 Biostratigraphic, Sedimentologic, and Chemostratigraphic Study of the La Luna Formation (Late Turonian–Campanian) in the San Miguel and Las Hernández Sections, Western Venezuela EGLEE ZAPATA; EGLEE ZAPATA 1Universidad Central de Venezuela, Faculty of Engineering, Department of Geology, Los Chaguáramos, Caracas, 10, Venezuela, zapata.eglee@excite.com Search for other works by this author on: GSW Google Scholar VICTOR PADRON; VICTOR PADRON 1Universidad Central de Venezuela, Faculty of Engineering, Department of Geology, Los Chaguáramos, Caracas, 10, Venezuela, zapata.eglee@excite.com Search for other works by this author on: GSW Google Scholar ISIRIS MADRID; ISIRIS MADRID 1Universidad Central de Venezuela, Faculty of Engineering, Department of Geology, Los Chaguáramos, Caracas, 10, Venezuela, zapata.eglee@excite.com Search for other works by this author on: GSW Google Scholar VANESSA KERTZNUS; VANESSA KERTZNUS 1Universidad Central de Venezuela, Faculty of Engineering, Department of Geology, Los Chaguáramos, Caracas, 10, Venezuela, zapata.eglee@excite.com Search for other works by this author on: GSW Google Scholar IRENE TRUSKOWSKI; IRENE TRUSKOWSKI 2Petróleos de Venezuela, PDVSA, Exploración, Apdo. 829, Caracas 1010A, Venezuela Search for other works by this author on: GSW Google Scholar MARIA ANTONIETA LORENTE MARIA ANTONIETA LORENTE 2Petróleos de Venezuela, PDVSA, Exploración, Apdo. 829, Caracas 1010A, Venezuela Search for other works by this author on: GSW Google Scholar Author and Article Information EGLEE ZAPATA 1Universidad Central de Venezuela, Faculty of Engineering, Department of Geology, Los Chaguáramos, Caracas, 10, Venezuela, zapata.eglee@excite.com VICTOR PADRON 1Universidad Central de Venezuela, Faculty of Engineering, Department of Geology, Los Chaguáramos, Caracas, 10, Venezuela, zapata.eglee@excite.com ISIRIS MADRID 1Universidad Central de Venezuela, Faculty of Engineering, Department of Geology, Los Chaguáramos, Caracas, 10, Venezuela, zapata.eglee@excite.com VANESSA KERTZNUS 1Universidad Central de Venezuela, Faculty of Engineering, Department of Geology, Los Chaguáramos, Caracas, 10, Venezuela, zapata.eglee@excite.com IRENE TRUSKOWSKI 2Petróleos de Venezuela, PDVSA, Exploración, Apdo. 829, Caracas 1010A, Venezuela MARIA ANTONIETA LORENTE 2Petróleos de Venezuela, PDVSA, Exploración, Apdo. 829, Caracas 1010A, Venezuela Publisher: SEPM Society for Sedimentary Geology Accepted: 01 Jun 2003 First Online: 03 Mar 2017 Online ISSN: 1938-5323 Print ISSN: 0883-1351 Society for Sedimentary Geology PALAIOS (2003) 18 (4-5): 367–377. https://doi.org/10.1669/0883-1351(2003)018<0367:BSACSO>2.0.CO;2 Article history Accepted: 01 Jun 2003 First Online: 03 Mar 2017 Cite View This Citation Add to Citation Manager Share Icon Share Facebook Twitter LinkedIn MailTo Tools Icon Tools Get Permissions Search Site Citation EGLEE ZAPATA, VICTOR PADRON, ISIRIS MADRID, VANESSA KERTZNUS, IRENE TRUSKOWSKI, MARIA ANTONIETA LORENTE; Biostratigraphic, Sedimentologic, and Chemostratigraphic Study of the La Luna Formation (Late Turonian–Campanian) in the San Miguel and Las Hernández Sections, Western Venezuela. PALAIOS 2003;; 18 (4-5): 367–377. doi: https://doi.org/10.1669/0883-1351(2003)018<0367:BSACSO>2.0.CO;2 Download citation file: Ris (Zotero) Refmanager EasyBib Bookends Mendeley Papers EndNote RefWorks BibTex toolbar search Search Dropdown Menu toolbar search search input Search input auto suggest filter your search All ContentBy SocietyPALAIOS Search Advanced Search Abstract Depositional paleoenvironments of the La Luna Formation were established based on investigation of sedimentology, foraminiferal assemblages, and stable isotope composition of two sections in the Venezuelan Andes. Planktonic foraminiferal biostratigraphy indicates that the age of the San Miguel section spans from the late Turonian to the early Campanian and the Las Hernández section ranges from the early Coniacian to the early Campanian. The base of the La Luna Formation becomes progressively younger towards the south. Early-diagenetic processes have altered stable isotopic composition of carbonates, however stratigraphic changes in carbon isotope values can be used to correlate between the sections.The environment of deposition of the La Luna Formation changed during the Late Cretaceous. Interval I, from the early Coniacian to mid-Santonian, was characterized by anoxic conditions. Alternating anoxic-dysoxic environments in Interval II lasted from the mid-Santonian to the base of the Campanian. Interval III, in the early Campanian, was marked by more oxygenated conditions. These trends can be partially observed in other ocean basins. You do not have access to this content, please speak to your institutional administrator if you feel you should have access." @default.
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