Magnetic suceptibility, carbon and oxygen stable isotope ratios and reflectance from the Bottaccione Gorge and Furlo section, Italy


Autoria(s): Batenburg, Sietske J
Cobertura

MEDIAN LATITUDE: 43.503115 * MEDIAN LONGITUDE: 12.646565 * SOUTH-BOUND LATITUDE: 43.361830 * WEST-BOUND LONGITUDE: 12.582030 * NORTH-BOUND LATITUDE: 43.644400 * EAST-BOUND LONGITUDE: 12.711100

Data(s)

19/09/2016

Resumo

The oceans at the time of the Cenomanian-Turonian transition were abruptly perturbed by a period of bottom-water anoxia. This led to the brief but widespread deposition of black organic-rich shales, such as the Livello Bonarelli in the Umbria-Marche Basin (Italy). Despite intensive studies, the origin and exact timing of this event are still debated. In this study, we assess leading hypotheses about the inception of oceanic anoxia in the Late Cretaceous greenhouse world, by providing a 6-Myr-long astronomically-tuned timescale across the Cenomanian-Turonian boundary. We procure insights in the relationship between orbital forcing and the Late Cretaceous carbon cycle by deciphering the imprint of astronomical cycles on lithologic, geophysical, and stable isotope records, obtained from the Bottaccione, Contessa and Furlo sections in the Umbria-Marche Basin. The deposition of black shales and cherts, as well as the onset of oceanic anoxia, is related to maxima in the 405-kyr cycle of eccentricity-modulated precession. Correlation to radioisotopic ages from the Western Interior (USA) provides unprecedented age control for the studied Italian successions. The most likely tuned age for the Livello Bonarelli base is 94.17 ± 0.15 Ma (tuning #1); however, a 405-kyr older age cannot be excluded (tuning #2) due to uncertainties in stratigraphic correlation, radioisotopic dating, and orbital configuration. Our cyclostratigraphic framework suggests that the exact timing of major carbon cycle perturbations during the Cretaceous may be linked to increased variability in seasonality (i.e. a 405-kyr eccentricity maximum) after the prolonged avoidance of seasonal extremes (i.e. a 2.4-Myr eccentricity minimum). Volcanism is probably the ultimate driver of oceanic anoxia, but orbital periodicities determine the exact timing of carbon cycle perturbations in the Late Cretaceous. This unites two leading hypotheses about the inception of oceanic anoxia in the Late Cretaceous greenhouse world.

Formato

application/zip, 2 datasets

Identificador

https://doi.pangaea.de/10.1594/PANGAEA.864716

doi:10.1594/PANGAEA.864716

Idioma(s)

en

Publicador

PANGAEA

Direitos

CC-BY: Creative Commons Attribution 3.0 Unported

Access constraints: unrestricted

Fonte

Supplement to: Batenburg, Sietske J; De Vleeschouwer, David; Sprovieri, Mario; Hilgen, Frederik J; Gale, Andrew S; Singer, Brad S; Koeberl, Christian; Coccioni, Rodolfo; Claeys, Philippe; Montanari, Alessandro (2016): Orbital control on the timing of oceanic anoxia in the Late Cretaceous. Climate of the Past, 12, 23 pp, doi:10.5194/cp-2015-182

Palavras-Chave #d13C carb; d18O carb; delta 13C, carbonate; delta 18O, carbonate; Depth; DEPTH, sediment/rock; Magnetic susceptibility; MAGS; Refl; Reflectance; VPDB
Tipo

Dataset