The effects of astronomically forced climate change on hemipelagic carbonate sedimentation in a tectonically active settingthe Albian Mioño Formation in Castro Urdiales, Cantabria, N Spain

  1. Aitor Payros 1
  2. Naroa Martínez Braceras 1
  3. Luis M. Agirrezabala 1
  4. Jaume Dinarès Turell
  5. Idoia Rosales
  1. 1 Universidad del País Vasco/Euskal Herriko Unibertsitatea
    info

    Universidad del País Vasco/Euskal Herriko Unibertsitatea

    Lejona, España

    ROR https://ror.org/000xsnr85

Revista:
Journal of iberian geology: an international publication of earth sciences

ISSN: 1886-7995,  1698-6180

Año de publicación: 2022

Volumen: 48

Número: 4

Páginas: 405-423

Tipo: Artículo

DOI: 10.1007/S41513-022-00198-Z DIALNET GOOGLE SCHOLAR lock_openAcceso abierto editor

Otras publicaciones en: Journal of iberian geology: an international publication of earth sciences

Resumen

El conocimiento sobre la expresión estratigráfica de los ciclos de cambio climático producidos astronómicamente en la banda de frecuencia de Milankovitch ha aumentado considerablemente en las últimas décadas. Sin embargo, hay algunos aspectos de los que aún no se tiene mucha información, como la naturaleza de los procesos ambientales climáticamente regulados que, en última instancia, determinan la sedimentación cíclica. Del mismo modo, no se dispone de mucha información sobre la expresión de los ciclos de Milankovitch en sucesiones acumuladas en cuencas tectónicamente activas. Con el fin de paliar estas deficiencias, en este trabajo se estudian los depósitos hemipelágicos albienses de la Formación Mioño de Castro Urdiales (Cuenca Vasco-Cantábrica), los cuales se acumularon durante una fase de rifting con fuerte actividad tectónica. El análisis sedimentológico, petrográfico y cicloestratigráfico demuestra que, a pesar de la existencia de inestabilidades tectónicas y alguna alteración diagenética, la alternancia carbonatada hemipelágica de hace 110.68–110.47 Ma estuvo regulada astronómicamente. Las fluctuaciones de estacionalidad inducidas por los ciclos de precesión causaron variaciones periódicas (20 ka) en las tasas de producción carbonatada (abundancia de plancton pelágico calcáreo y micrita exportada desde áreas someras adyacentes) y/o dilución silícea (aporte de sedimento siliciclástico terrestre y producción de partículas silíceas por esponjas). Estas variaciones determinaron la formación de calizas margosas cuando la estacionalidad anual era baja (i.e., verano boreal en el afelio, invierno en el perihelio) y la acumulación de margas cuando aumentaba la estacionalidad (i.e., verano boreal en el perihelio, invierno en el afelio). La incidencia de estos procesos aumentaba y disminuía en consonancia con la modulación de la estacionalidad producida por los ciclos de excentricidad corta de 100 ka. En conclusión, este estudio demuestra que los ciclos de Milankovitch pueden quedar fielmente registrados en sucesiones hemipelágicas acumuladas en contextos tectónicamente activos si los flujos gravitacionales de sedimento u otras perturbaciones no afectan a la sedimentación autóctona.

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