Geochronology and magmatic evolution of the Huautla volcanic field: last stages of the extinct Sierra Madre del Sur igneous province of southern Mexico

被引:15
作者
Gonzalez-Torres, Enrique A. [1 ]
Moran-Zenteno, Dante J. [1 ]
Mori, Laura [1 ]
Diaz-Bravo, Beatriz [2 ]
Martiny, Barbara M. [1 ]
Sole, Jesus [1 ]
机构
[1] Univ Nacl Autonoma Mexico, Inst Geol, Mexico City 04510, DF, Mexico
[2] Univ Nacl Autonoma Mexico, Ctr Geociencias, Queretaro 76230, Mexico
基金
美国国家科学基金会;
关键词
southern Mexico; Sierra Madre del Sur; Huautla volcanic field; silicic flare-up; Sierra Madre Occidental; Farallon plate underflow; SOUTHWESTERN MEXICO; TECTONIC SIGNIFICANCE; FORE-ARC; MARGIN; DEFORMATION; SUBDUCTION; GUERRERO; EXTENSION; COLLAPSE; INSIGHTS;
D O I
10.1080/00206814.2013.767504
中图分类号
P5 [地质学];
学科分类号
0709 ; 081803 ;
摘要
The Huautla volcanic field (HVF), in the Sierra Madre del Sur (SMS), is part of an extensive record of Palaeogene magmatism reflecting subduction of the Farallon plate along the western edge of North America. Igneous activity resulting from Farallon subduction is also exposed to the north, in the Sierra Madre Occidental (SMO) and Mesa Central (MC) provinces. We present the results of a stratigraphic and K-Ar, Ar-Ar, and U-Pb geochronological study of the Huautla volcanic successions, in order to refine our knowledge on the petrologic and temporal evolution of the northern SMS and gain insights on magmatic-tectonic contrasts between the SMS and the SMO-MC provinces. The HVF is made up of lava flows and pyroclastic successions that overlie marine Cretaceous sequences and post-orogenic continental deposits of Palaeogene age. In the study area, the main Oligocene succession is pre-dated by the 36.7 million years its caldera west of the Sierra de Huautla. The HVF succession ranges in age from approximate to 33.6 to 28.1 Ma and comprises a lower group of andesitic-dacitic lava flows, an intermediate sequence of ignimbrites and dacitic lavas, and an upper group of andesitic units. The silicic succession comprises a crystal-poor ignimbrite unit (i.e. the Maravillas ignimbrite; 31.4 +/- 0.6, 32.0 +/- 0.4 Ma; approximate to 260 km(3)), overlain by a thick succession of dacitic lavas (i.e. the Agua Fria dacite; 30.5 +/- 1.9, 31.0 +/- 1.1 Ma). Integration of the new stratigraphic and geochronological data with prior information from other explosive centres of the north-central SMS allows us to constrain the temporal evolution of a silicic flare-up episode, indicating that it occurred between 37-32 Ma; it consisted of three major ignimbrite pulses at approximate to 36.5, approximate to 34.5, and approximate to 33-32 Ma and probably resulted from a progressive, mantle flux-driven thermomechanical maturation of the continental crust, as suggested in the HVF by the transition from andesitic to voluminous siliceous volcanism. The information now available for the north-central sector of the SMS also allows recognition of differences between the temporal and spatial evolution of magmatism in this region, and of that documented in the southern SMO and MC provinces, suggesting that such contrasts are probably related to local differences in configuration of the subduction system. At approximate to 28 Ma, the MC and southern SMO provinces experienced a trenchward migration of volcanism, associated with slab rollback; on the other hand, the broad, more stable distribution of Oligocene magmatism in the central and north oceanic plate was subducting at a low angle.
引用
收藏
页码:1145 / 1161
页数:17
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