6533b854fe1ef96bd12addfa
RESEARCH PRODUCT
Cyclostratigraphy and high-frequency carbon isotope fluctuations in Upper Cretaceous shallow-water carbonates, southern Italy
Bruno D'argenioVittoria FerreriAdriana BellancaRodolfo NeriGaetano FerruzzaFrancesco Paolo BuonocuntoMario Sprovierisubject
Sedimentary depositional environmentWaves and shallow waterPaleontologyIsotopes of carbonCarbonate platformStratigraphyGeologySedimentary rockCyclostratigraphyCretaceousGeologyDiagenesisdescription
A detailed carbon isotope study has been carried out on a Santonian (Upper Cretaceous) carbonate platform succession that crops out at Monte Sant'Erasmo (southern Italy). Previous centimetre-scale studies on this succession have shown that high-frequency eustatic changes, resulting from the Earth's orbital fluctuations, controlled the hierarchical organization of the depositional and early diagenetic features in elementary cycles, bundles (groups of three to five elementary cycles) and superbundles (groups of three or four bundles). The elementary cycles, which correspond to single beds, suggest a control caused by Earth's precession; the bundles and superbundles record the short ( 100 kyr) and long ( 400 kyr) eccentricity periodicity respectively. The δ 1 3 C signal of the Monte Sant'Erasmo succession is cyclic in nature and may be considered to be a reliable proxy for the sedimentary evolution (and related sea-level history) of the analysed sequence. The carbon isotope cyclicity is recorded at bundle and superbundle level, but it is not evident at the scale of the elementary cycles, at least with the sampling interval used in this study. Spectral analysis of the δ 1 3 C record shows two main peaks corresponding to the short- and long-eccentricity periodicity, whereas the precession signal is not evident in the power spectrum. In addition, lithofacies analysis shows that, in each bundle (and superbundle), higher C isotope values occur in sediments characterized by marine cements, whereas lower values are normally found in more restricted deposits overprinted by early meteoric diagenesis. Early diagenesis, driven by periodic sea-level fluctuations, developed in either shallow-subtidal (marine diagenesis) or subaerial-exposed (meteoric overprint) sedimentary environments and directly influenced the carbon isotope signature. As a consequence, the δ 1 3 C record at Monte Sant'Erasmo reflects high-frequency climatic oscillations controlling both environmental and early diagenetic changes. The long-term isotopic record is similar to that of contemporaneous pelagic sections in England and elsewhere in Italy. It is concluded that the δ 1 3 C signature of shallow-water carbonates, such as those of Monte Sant'Erasmo, offers great potential for correlation with coeval sections, including those of the pelagic realm.
year | journal | country | edition | language |
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2002-12-01 | Sedimentology |