Abstract
Orbital forcing has been shown to be a fundamental driver of climate change through both icehouse and greenhouse periods. To reveal the impact of orbital-forcing on the oceanic environment through a greenhouse-icehouse transition, we established ~4Myr-long cyclostratigraphy of the Bajocian-Callovian (Middle Jurassic; ~160Ma) Basal Radiolarites at the Torre De Busi and Corre Di Sogno sections in the Lombardian Basin, N-Italy. Stratigraphic changes in chert abundance (chert/shale thickness ratio) and color (darkness) of Radiolarites show hierarchal periodicities of 8cm, 16cm, 40cm, 160cm, and ~4m, corresponding to ~20kyr, 40kyr, 100kyr, 400kyr, and ~1Myr cycles based on the biostratigraphic age model. Black cherts in intervals with high chert abundance might reflect oxygen-depleted conditions due to orbital-scale high productivity. On the other hand, black cherts in intervals with low chert abundance (high detrital input) might reflect oxygen-depleted conditions, probably due to orbital-scale sea-level drop and stratification. On 40kyr and 100kyr cycles, the anoxic condition occurred in low chert abundance intervals across ~8m above (~2Myr after) the base of the Radiolarites. These results imply that the formation of the restricted basin resulted from tectonic and/or eustatic sea-level drop, which is consistent with increased black chert deposition and redox-sensitive elements abundances (Mo/TOC, Mo/U). Their out-of-phase relationships on the 405kyr cycle throughout the sequence (~4Myr-long) with increasing amplitude above −8M level would be caused possibly by tectonic activity, or more likely by glacio-eustatic sea-level changes reported from sequence stratigraphy, similar to those of the Oligocene to Pliocene glacial cycles, but probably with less amplitude.
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