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Distribution of major and trace elements in La Luna Formation, Southwestern Venezuelan Basin

Organic Geochemistry, 2002
The La Luna Formation (Maraca section), Maracaibo Basin, was studied by means of V and Ni analysis of the bitumen, total organic carbon (TOC), total sulfur (St), major elements (Si, Al, Fe, Mg, Mn, Ca, Ti, Na, K, P), trace elements (V, Ni, Co, Cr, Cu, and Zn), and electron microprobe analysis (EPMA) of the whole rock, and St, major elements (Si, Al, Fe,
S. Mónaco   +5 more
semanticscholar   +2 more sources

Turonian–Santonian Calcareous Nannofossil Biozonation for La Luna Formation, Middle Magdalena Valley Basin, Northern Colombia

Advances in South American Micropaleontology, 2018
A well site biostratigraphic study was carried out in the Chuira-2 ST-1 well, through the Umir and La Luna Formations in the Middle Magdalena Valley Basin (MMVB), north of Colombia. Results of the calcareous nannofossil analysis are presented and compared to local biozonations for planktonic foraminifera and palinomorphs for La Luna Formation in the ...
J. P. P. Panera   +6 more
semanticscholar   +2 more sources

Campanian Bolivinoides and microfacies from the La Luna Formation, western Venezuela

Marine Micropaleontology, 1995
Abstract Tres Esquinas, the upper member of the La Luna Formation, a 1–3 m thick condensed sequence composed of glauconitic phosphorite, signals the commencement of the Late Cretaceous regression in western Venezuela. This is the last of a series of thin phosphatic beds, the others non-glauconitic, occurring in the upper La Luna Formation.
L. Romero, F. Galea-Alvarez
semanticscholar   +2 more sources

Global and local controls influencing the deposition of the La Luna Formation (Cenomanian-Campanian), western Venezuela

Chemical Geology, 1996
Bulk and molecular geochemical, micropalaeontological, and carbon-isotopic data are used to address the different local and global factors influencing the environment of sedimentation of the La Luna Formation (Cenomanian-Campanian, approximate palaeolatitude 15°N) in a single section in western Venezuela.
Julio Perez-Infante   +2 more
semanticscholar   +3 more sources

Paleogeography and Stratigraphy of the La Luna Formation and Related Cretaceous Anoxic Depositional Systems

PALAIOS, 2003
Earth’s past includes episodes when environments in much of the ocean were very different from those of today. One of these episodes, that has enormous economic repercussions, occurred in the mid-Cretaceous between ∼80–125 Ma, and led to deposition of organic carbon (Corg)-rich sediments, informally known as “black shales,” over large regions of the ...
T. Bralower, M. Lorente
semanticscholar   +2 more sources

Trace metals and organic geochemistry of the Machiques Member (Aptian-Albian) and La Luna Formation (Cenomanian-Campanian), Venezuela

Chemical Geology, 1999
Abstract Two proposed source-rock sequences in the Lower (Aptian–Albian) and the Upper (Cenomanian–Campanian) Cretaceous sediments of the Perija Range, Maracaibo Basin, were geochemically analyzed in order to find environmentally controlled characteristic fingerprints.
M. Alberdi-Genolet, R. Tocco
semanticscholar   +2 more sources

Regional Sequence Stratigraphy of the Upper Cretaceous La Luna Formation in the Magdalena Valley Basin, Colombia.

Proceedings of the 2nd Unconventional Resources Technology Conference, 2014
La Luna Formation is known as one of the most prolific source rocks in the northern Andes and worldwide. However, despite this proven potential and the increasing interest in La Luna Fm. as an unconventional play the regional sequence-stratigraphic framework and its depositional system remain poorly understood.
H. Galvis-Portilla   +12 more
semanticscholar   +2 more sources

Vanadium of petroleum asphaltenes and source kerogens (La Luna Formation, Venezuela): isotopic study and origin

Fuel, 2002
High-resolution mass spectrometry indicates that the isotopic abundance of (50)vanadium (V) of the Late Cretaceous La Luna petroleum asphaltenes and related source kerogens of marine origin (both highly enriched with V GT 2000 ppm) is higher by about 3.5% than that of inorganic source (VOSO4.5H(2)O, Merck).
P. Premović
semanticscholar   +4 more sources

Trace elements as palaeoenvironmental markers in strongly mature hydrocarbon source rocks: the Cretaceous La Luna Formation of Venezuela

Sedimentary Geology, 1996
Abstract The Late Cretaceous La Luna Formation is the main hydrocarbon source-rock formation in Venezuela. In the Lake Maracaibo area, the formation shows a steep maturation gradient affecting sedimentary organic matter (OM) and clay minerals, related to local burial history and thrusting events.
Thierry Mongenot   +4 more
semanticscholar   +2 more sources

Organic carbon and phosphate distributions in the La Luna Formation, Western Venezuela

AAPG Bulletin, 1996
The Upper Cretaceous La Luna Formation in Western Venezuela is believed to be the major source rock in the Maracaibo basin. In order to obtain an approximation of the total amount of hydrocarbons that could have possibly been generated in this basin, the vertical and areal distribution of total organic carbon (TOC) was studied.
P. S. Stoufer, W. Scherer
semanticscholar   +2 more sources

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