Chemical and stable isotope composition (18O/16O, 2H/1H) of formation waters from the Carabobo Oilfield, Venezuela

被引:4
|
作者
Boschetti, T. [1 ]
Angulo, B. [2 ]
Quintero, F. [2 ]
Volcan, J. [3 ]
Casalins, A. [4 ]
机构
[1] Univ Parma, Dept Chem Life Sci & Environm Sustainabil, Parco Area Sci, I-43124 Parma, Italy
[2] Petroleos Venezuela SA PDVSA, Inst Tecnol Venezolano Petroleo INTEVEP, Dept Invest Estrateg Explorac, Apartado 76343, Caracas 1070A, Los Teques, Venezuela
[3] Univ Cent Venezuela, Inst Ciencias Tierra, Apartado 3895, Caracas 1010A, Venezuela
[4] Petrolera Sinovensa, Estudios Integrados, Torre BVC, Barcelona 6001, Venezuela
关键词
Orinoco Oil Belt; Carabobo area; Formation water; Chemical and isotope composition; EASTERN VENEZUELAN; RESERVOIR; GENERATION; MIGRATION; EVOLUTION; GEOLOGY; ORIGIN; AREA; PART;
D O I
10.1344/GeologicaActa2018.16.3.2
中图分类号
P5 [地质学];
学科分类号
0709 ; 081803 ;
摘要
In this short note, we present the first data on stable isotope composition of the oilfield waters from Carabobo area of the Faja Petrolifera del Orinoco "Hugo Chavez" (Orinoco Oil Belt). From a chemical point of view, the formation waters show a main Na-Cl level (TDS up to 30g/l) with a dilution trend toward Na-HCO3 composition (down to 1g/l). Until now, such a clear net chemical compositional trend was ascribed to a meteoric dilution (fresh/brackish bicarbonate) of the seawater endmember (the saltiest chloride). The isotope results of this study reveal that the seawater mother water was modified during a high-temperature thrusting event (120-125 degrees C), forming O-18-enriched diagenetic water (up to +4 parts per thousand), which was diluted in recent times by glacial meltwater and present-day meteoric water. The hypothetical presence of flood by a meteoric paleo-water also offers new hints to explain the low API gravity (<10 degrees API biodegraded, extra heavy oil) and composition of the local crude.
引用
收藏
页码:257 / +
页数:11
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