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Depositional evolution of an extinct sinter mound from source to outflow, El Tatio, Chile
Indexado
WoS WOS:000568162600013
Scopus SCOPUS_ID:85089017725
DOI 10.1016/J.SEDGEO.2020.105726
Año 2020
Tipo artículo de investigación

Citas Totales

Autores Afiliación Chile

Instituciones Chile

% Participación
Internacional

Autores
Afiliación Extranjera

Instituciones
Extranjeras


Abstract



Siliceous sinter deposits from El Tatio, Chile, preserve a wide variety of depositional environments and biosignatures, from high-temperature (~85 °C) vent-proximal facies to distal deposits dominated by silicified microbial mats. Four cores were drilled into an El Tatio sinter mound and associated distal apron to investigate changes in hydrothermal environments over geologic timescales. Sedimentary and geochemical analysis of multiple sinter cores records the initiation and accretion of diverse depositional features still observed today in El Tatio. Facies adjacent to hydrothermal vents are dominated by laminated sinter crusts on the steep margins of a high-temperature pool, with sparse microbial preservation. Outer margins of the same pool contain extensive sinter columns up to ten centimeters in length, precipitated during repeated cycles of pool overflow and subsequent evaporation. Low-relief hydrothermal pools also form minor deposits within distal debris aprons, and analogous pools are still active close to sampling locations. Debris aprons are dominated by palisade, tufted, and arborescent microbial fabrics, with distinct mat textures revealing well preserved microfossils. Surficial deposits in all cores feature detrital-rich and microbially-influenced sinters overlying higher-temperature facies, indicating a relative decrease in hydrothermal activity over time. Geochemical proxies for hydrothermal fluids and detrital input match depositional interpretations based on sedimentary structures. 14C ages from core deposits extend the mound's history by 11,000 years, recording at least three thousand years of sinter deposition on top of glacial sandstones (13,337–10,232 y. cal. BP). Importantly, this work provides a detailed depositional model unavailable through surficial sedimentology alone.

Revista



Revista ISSN
Sedimentary Geology 0037-0738

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Disciplinas de Investigación



WOS
Geology
Scopus
Geology
Stratigraphy
SciELO
Sin Disciplinas

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Publicaciones WoS (Ediciones: ISSHP, ISTP, AHCI, SSCI, SCI), Scopus, SciELO Chile.

Colaboración Institucional



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Autores - Afiliación



Ord. Autor Género Institución - País
1 Wilmeth, Dylan T. Hombre Institut de Physique du Globe de Paris - Francia
UNIV PARIS - Francia
Université Paris Cité - Francia
2 Nabhan, Sami Hombre Institut de Physique du Globe de Paris - Francia
UNIV PARIS - Francia
Université Paris Cité - Francia
3 Myers, Kimberly D. Mujer Institut de Physique du Globe de Paris - Francia
UNIV PARIS - Francia
Université Paris Cité - Francia
4 Slagter, Silvina Mujer Institut de Physique du Globe de Paris - Francia
Yale University - Estados Unidos
UNIV PARIS - Francia
YALE UNIV - Estados Unidos
Université Paris Cité - Francia
5 Lalonde, Stefan V. Hombre Institut Universitaire Européen de la Mer (IUEM) - Francia
Inst Univ Europeen Mer - Francia
6 Sansjofre, Pierre Hombre Sorbonne Université - Francia
Sorbonne Univ - Francia
7 Homann, Martin Hombre University College London - Reino Unido
UCL - Reino Unido
8 Konhauser, Kurt O. Hombre University of Alberta - Canadá
Univ Alberta - Canadá
9 Munoz-Saez, Carolina Mujer Centro de Excelencia en Geotermia de Los Andes - Chile
Universidad de Chile - Chile
10 van Zuilen, Mark A. Hombre Institut de Physique du Globe de Paris - Francia
UNIV PARIS - Francia
Université Paris Cité - Francia

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Financiamiento



Fuente
European Research Council
European Union's Horizon 2020 research and innovation program
Horizon 2020 Framework Programme
European Union’s Horizon 2020 research and innovation program
European Research Council under the European Union'sHorizon 2020 Research and Innovation Program

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Agradecimientos



Agradecimiento
This research was funded by the European Research Council under the European Union’s Horizon 2020 Research and Innovation Program (Grant Agreement # 646894 ) to M.V.Z. The authors would like to thank Prisca Grandin for geochemical laboratory assistance (IUEM, Brest, France), Jean-Pierre Oldra (IUEM, Brest, France) and the Thin Section Lab (Toul, France), for petrographic preparation, Stefan Borensztajn (IPGP, Paris, France) and the Toconce and Caspana communities managing the El Tatio Geyser Field tourism and outreach for permission to sample in the area.
This researchwas funded by the European Research Council under the European Union'sHorizon 2020 Research and Innovation Program (Grant Agreement #646894) to M.V.Z. The authors would like to thank Prisca Grandin for geochemical laboratory assistance (IUEM, Brest, France), Jean-Pierre Oldra (IUEM, Brest, France) and the Thin Section Lab (Toul, France), for petrographic preparation, Stefan Borensztajn (IPGP, Paris, France) and the Toconce and Caspana communitiesmanaging the El Tatio Geyser Field tourismand outreach for permission to sample in the area.

Muestra la fuente de financiamiento declarada en la publicación.