Geophysical modeling and structure of Ushuaia Pluton, Fuegian Andes, Argentina
Within the area of Ushuaia Bay (Tierra del Fuego, southernmost South America) the deformed Lower Cretaceous sedimentary rocks of Yahgán Formation host the Ushuaia Pluton. The intrusive body is oval in map view; it is compositionally varied with rocks ranging from the ultrabasic to the mesosiliceous...
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2009
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| LEADER | 21213caa a22016937a 4500 | ||
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| 003 | AR-BaUEN | ||
| 005 | 20230518203812.0 | ||
| 008 | 190411s2009 xx ||||fo|||| 00| 0 eng|d | ||
| 024 | 7 | |2 scopus |a 2-s2.0-70349777272 | |
| 040 | |a Scopus |b spa |c AR-BaUEN |d AR-BaUEN | ||
| 100 | 1 | |a Peroni, J.I. | |
| 245 | 1 | 0 | |a Geophysical modeling and structure of Ushuaia Pluton, Fuegian Andes, Argentina |
| 260 | |c 2009 | ||
| 270 | 1 | 0 | |m Peroni, J.I.; CONICET-INGEODAV, Dpto. de Ciencias Geológicas, Facultad de Ciencias Exactas y Naturales, Ciudad Universitaria, Pabellon 2, CP-C1428EHA Buenos Aires, Argentina; email: peroni@gl.fcen.uba.ar |
| 506 | |2 openaire |e Política editorial | ||
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| 520 | 3 | |a Within the area of Ushuaia Bay (Tierra del Fuego, southernmost South America) the deformed Lower Cretaceous sedimentary rocks of Yahgán Formation host the Ushuaia Pluton. The intrusive body is oval in map view; it is compositionally varied with rocks ranging from the ultrabasic to the mesosiliceous realm. The emplacement time is constrained within the Albian-Cenomanian span by new amphibole K/Ar data. Meso- and microstructures of Ushuaia Pluton and its host indicate a synkinematic emplacement with a dominant extensional component. A set of transcurrent and normal faults related to the sinistral strike-slip Beagle Channel Fault System affects the pluton and its host. On the basis of aeromagnetic data combined with field information, a new model is presented for the Ushuaia Pluton. Modeling results fit well with a laccolithic body with an estimated volume of around 111 km3. The model pluton cross-section displays a central zone with an average thickness of 2000 m which progressively thins toward the margins (∼ 500 m) and a southern root which reaches 5000 m deep. The combined structural and geophysical model supports a transtensive scenario for the Ushuaia Pluton emplacement at Early-Late Cretaceous boundary. © 2009 Elsevier B.V. All rights reserved. |l eng | |
| 593 | |a CONICET-INGEODAV, Dpto. de Ciencias Geológicas, Facultad de Ciencias Exactas y Naturales, Ciudad Universitaria, Pabellon 2, CP-C1428EHA Buenos Aires, Argentina | ||
| 593 | |a Istituto di Scienze della Terra, Università di Urbino, Campus Scientifico Universitario, 61029 Urbino, Italy | ||
| 593 | |a CONICET, Dept. Cs. Geológicas, FCEyN, Argentina | ||
| 690 | 1 | 0 | |a MAGNETIC MODELING |
| 690 | 1 | 0 | |a PLUTON EMPLACEMENT |
| 690 | 1 | 0 | |a STRIKE-SLIP ACTIVITY |
| 690 | 1 | 0 | |a AEROMAGNETIC DATA |
| 690 | 1 | 0 | |a CENOMANIAN |
| 690 | 1 | 0 | |a CENTRAL ZONE |
| 690 | 1 | 0 | |a FAULT SYSTEM |
| 690 | 1 | 0 | |a GEOPHYSICAL MODELING |
| 690 | 1 | 0 | |a GEOPHYSICAL MODELS |
| 690 | 1 | 0 | |a LATE CRETACEOUS |
| 690 | 1 | 0 | |a LOWER CRETACEOUS |
| 690 | 1 | 0 | |a MAGNETIC MODELING |
| 690 | 1 | 0 | |a MODELING RESULTS |
| 690 | 1 | 0 | |a NEW MODEL |
| 690 | 1 | 0 | |a NORMAL FAULTS |
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| 690 | 1 | 0 | |a STRIKE-SLIP ACTIVITY |
| 690 | 1 | 0 | |a GEOPHYSICS |
| 690 | 1 | 0 | |a SEDIMENTOLOGY |
| 690 | 1 | 0 | |a STRUCTURAL GEOLOGY |
| 690 | 1 | 0 | |a SEDIMENTARY ROCKS |
| 690 | 1 | 0 | |a ALBIAN |
| 690 | 1 | 0 | |a CENOMANIAN |
| 690 | 1 | 0 | |a CONTINENTAL MARGIN |
| 690 | 1 | 0 | |a DEFORMATION |
| 690 | 1 | 0 | |a EMPLACEMENT |
| 690 | 1 | 0 | |a EXTENSIONAL TECTONICS |
| 690 | 1 | 0 | |a MAGNETIC METHOD |
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| 690 | 1 | 0 | |a POTASSIUM-ARGON DATING |
| 690 | 1 | 0 | |a ROCK MICROSTRUCTURE |
| 690 | 1 | 0 | |a STRIKE-SLIP FAULT |
| 690 | 1 | 0 | |a USHUAIA BAY |
| 651 | 4 | |a TIERRA DEL FUEGO | |
| 651 | 4 | |a ARGENTINA | |
| 651 | 4 | |a SOUTH AMERICA | |
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| 651 | 4 | |a TIERRA DEL FUEGO [(PRV) ARGENTINA] | |
| 650 | 1 | 7 | |2 spines |a PLUTON |
| 700 | 1 | |a Tassone, A.A. | |
| 700 | 1 | |a Menichetti, M. | |
| 700 | 1 | |a Cerredo, M.E. | |
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