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| DOI | 10.1016/J.SEDGEO.2018.01.002 | ||||
| Año | 2018 | ||||
| Tipo | artículo de investigación |
Citas Totales
Autores Afiliación Chile
Instituciones Chile
% Participación
Internacional
Autores
Afiliación Extranjera
Instituciones
Extranjeras
Megaturbidites have been the focus of many paleoseismic and paleoenvironmental studies because they can provide evidence for catastrophic and/or hazardous events with potentially major environmental implications. During a recent research cruise in Baker Fjord, Chile (47 degrees 54 ' S-74 degrees 30 ' W), a megaturbidite was described between the Northern and Southern Patagonian Icefields. Here, we aim to determine the depositional processes of the megaturbidite and identify its origin. Based on the turbidite's location, a possible origin was the early Holocene drainage of paleo-lake General Carrera, which was recently proposed in the literature as having produced a Glacial Lake Outburst Flood (GLOF) that drained through Baker Fjord. Due to the fjord's location in a subduction zone, and close to the Chile Triple Junction, however, seismic activity must also be considered as a potential triggering mechanism. To achieve our goals, we undertook a multi-proxy analysis of sediment core MD07-3121, including sedimentology (grain size, loss-on-ignition, foraminifera counts), magnetic properties, bulk organic geochemistry, and radiocarbon dating, and we analysed bathymetric maps and sub-bottom profiles. Our grain-size results display a diagnostic fining upward trend and show evidence of seiching in the 733-cm-thick megaturbidite. The age of the event (5513-5211 cal yr BP) contradicts the hypothesis of an early Holocene GLOF origin. Bulk organic geochemical results indicate that the sediments that compose the turbidite are clearly of marine origin, which further goes against a GLOF origin. In addition, the megaturbidite is underlain by a 1136 cm thick mass transport deposit (MTD), also composed of marine sediments. According to the sub-bottom profiles, the MTD and the megaturbidite originate from the reworking of thick packages of sediment previously deposited on nearby sills and on the fjord's flanks. Furthermore, similar coeval deposits are found in an adjacent sub-basin. We therefore interpret these deposits to be triggered by an earthquake during the late mid-Holocene. While megathrust and intraslab earthquakes are possible in the region, we argue that a crustal earthquake is the most likely seismic trigger in the study area. This study reveals the first earthquake-triggered megaturbidite south of the Chile Triple Junction. (C) 2018 Elsevier B.V. All rights reserved.
| Ord. | Autor | Género | Institución - País |
|---|---|---|---|
| 1 | Piret, Loic | - |
Univ Ghent - Bélgica
Universiteit Gent - Bélgica |
| 2 | Bertrand, Sebastien | Hombre |
Univ Ghent - Bélgica
Universiteit Gent - Bélgica |
| 3 | Kissel, Catherine | Mujer |
Univ Paris Saclay - Francia
Universite de Versailles Saint-Quentin-en-Yvelines - Francia |
| 4 | DE POL-HOLZ, RICARDO HERNAN | Hombre |
Universidad de Magallanes - Chile
|
| 5 | Tamayo Hernando, Alvaro | Hombre |
Universidad de Concepción - Chile
|
| 6 | Van Daele, M. | Hombre |
Univ Ghent - Bélgica
Universiteit Gent - Bélgica |
| Fuente |
|---|
| FONDECYT |
| FONDAP |
| Fondo Nacional de Desarrollo Científico y Tecnológico |
| Iniciativa Científica Milenio |
| Institut Polaire Francais Paul Emile Victor |
| Ghent University |
| Universiteit Gent |
| Fonds Wetenschappelijk Onderzoek |
| FWO project |
| LSCE |
| Laboratoire de Mesures Carbone |
| Camille Wandres |
| Agradecimiento |
|---|
| This work was part of the first author's MSc thesis at Ghent University and was financed by FWO project G0D7916N "Paleo-GLOFs" to S.B. R.D.P.-H. and A.T.H. were funded by Iniciativa Cientifica Milenio NC120066, Fondecyt 1140536 and Fondap 15110009. We would like to thank the captain and crew of RN Marion Dufresne for the successful 'PACHIDERME' MD/159 cruise. The lab assistance by Camille Wandres (LSCE, Paris) and Elke Vandekerkhove (UGent) is greatly acknowledged. We are indebted to the Laboratoire de Mesures Carbone 14 (LMC14) in Saclay (France) for handling the radiocarbon dating with Artemis, Xavier Morin from IPEV for the sub -bottom profile data and Naomi Harada together with the whole JAMSTEC team for the multibeam data gathered during the MR08-06 cruise onboard RN Mirai. Carina Lange (UdeC, Chile) and Elisabeth Michel (LSCE, France) are acknowledged for constructive discussions. We thank Zakaria Ghazoui for his elaborate comments on the figures and the two anonymous reviewers for their constructive and insightful comments. |
| This work was part of the first author's MSc thesis at Ghent University and was financed by FWO project G0D7916N “Paleo-GLOFs” to S.B. R.D.P.-H. and A.T.H. were funded by Iniciativa Científica Milenio NC120066, Fondecyt 1140536 and Fondap 15110009. We would like to thank the captain and crew of R/V Marion Dufresne for the successful ‘PACHIDERME’ MD/159 cruise. The lab assistance by Camille Wandres (LSCE, Paris) and Elke Vandekerkhove (UGent) is greatly acknowledged. We are indebted to the Laboratoire de Mesures Carbone 14 (LMC14) in Saclay (France) for handling the radiocarbon dating with Artemis, Xavier Morin from IPEV for the sub-bottom profile data and Naomi Harada together with the whole JAMSTEC team for the multibeam data gathered during the MR08-06 cruise onboard R/V Mirai. Carina Lange (UdeC, Chile) and Elisabeth Michel (LSCE, France) are acknowledged for constructive discussions. We thank Zakaria Ghazoui for his elaborate comments on the figures and the two anonymous reviewers for their constructive and insightful comments. |