Abstract
The Huayna Potosi, Zongo and Taquesi are Triassic plutons located at the core of the Real Cordillera of Bolivia. In this paper, several Rb-Sr and K-Ar ages obtained in the past at the Sao Paulo Geochronology Laboratory, yet unpublished, will be presented, along with newer U-Pb Sensitive High-Resolution Ion Microprobe (SHRIMP) determinations made in the same laboratory, allowing us to redefine the geologic history of this part of the Central Andes. Rb/Sr analyses of some low grade metapelitic country rocks of the early Paleozoic (Amutara and Cancaniri Formations) yielded a Rb-Sr isochron age of 344 ± 38 Ma, indicating the action of an early Gondwanide regional event. A five-point Rb-Sr isochron from a granite outcrop of the Huayna Potosi pluton yielded an age of 224 ± 28 Ma. In addition, an important Ar loss in micas was detected in the Zongo granitoids and their country rocks, recording a thermal event that opened this isotopic system in the Oligocene. Newer U-Pb SHRIMP zircon ages of ca. 221 Ma were obtained in two other granitic outcrops of the Huayna Potosi granite. They confirmed its Triassic crystallization age, and a similar U-Pb SHRIMP age of 221.9 ± 1.5 Ma was obtained for one sample of the Taquesi pluton. For the Zongo pluton, many of the zircon grains obtained from one sample of its Kuticucho facies yielded extremely high uranium content, which produced reverse discordant apparent ages. However, due to the fair alignment of the analytical points in the Concordia diagram, possibly corresponding to a linear correlation, we made a regression calculation and the interception of the Concordia curve resulted in a rather imprecise age of 220 ± 20 Ma. Our conclusion was that the final magmatic crystallization and the intrusion of plutons in the central part of the Cordillera Real of Bolivia have occurred close to 221.5 ± 2.0 Ma, in late Triassic times. Finally, the U-Pb SHRIMP ages obtained in inherited zircon xenocrysts from the four available granitic rocks yielded very different ages, and many of them are related to previous magmatic episodes of the Andean Tectonic System. A few other age measurements indicated sources related to much older Proterozoic magmatic events associated with rocks from the Andean basement.
Highlights
The first dating of the Huayna Potosí pluton of the Cordillera Real of Bolivia (Fig. 1) was found by Evernden et al (1977) using a few K/Ar measurements in micas
During the field excursion mentioned in the introduction, organized in 1978 by geologists from the geological service of Bolivia, GEOBOL, La Paz, made along the Zongo River, under the leadership of Guillermo Cortez Arce and with the participation of UGC, few rock samples were collected from a few outcrops of the Paleozoic metasedimentary country rocks, the Huayna Potosi and the Zongo plutons
The geochronological data available for the Huayna Potosí, Zongo and Taquesi plutons of the Real Cordillera of Bolivia are a relevant contribution to the assessment of the geological history of that region
Summary
The first dating of the Huayna Potosí pluton of the Cordillera Real of Bolivia (Fig. 1) was found by Evernden et al (1977) using a few K/Ar measurements in micas. A series of samples was analyzed at the University of São Paulo laboratory, by the Rb/Sr and K/Ar methods, and a presentation was made at the Symposium on the “Magmatic Evolution of the Andes” within the International Geological Congress held in Paris, France, in 1980 (Cordani et al 1980). This presentation had the support of only an abstract, which shall be considered as a preliminary geological piece of information for the region of interest. Farrar et al (1990) and Gillis et al (2006) dated several plutons of the Real Cordillera using the U/Pb method in zircon for the first time
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