Long chain alkenones in the Early Pliocene Sicilian sediments (Trubi Formation — Punta di Maiata section): Implications for the alkenone paleothermometry

The U k′ 37 record and coccolithophorid remains in sediments from the early Pliocene Sicilian Trubi Formation (Punta di Maiata) have been estimated to assess the possible influence of changes in the alkenone-producing coccolithophorids on the U k′ 37–temperature relationship. The samples were domina...

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Published inPalaeogeography, palaeoclimatology, palaeoecology Vol. 308; no. 3; pp. 253 - 263
Main Authors Beltran, C., Flores, J.-A., Sicre, M.-A., Baudin, F., Renard, M., de Rafélis, M.
Format Journal Article
LanguageEnglish
Published Elsevier B.V 01.08.2011
Elsevier
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Summary:The U k′ 37 record and coccolithophorid remains in sediments from the early Pliocene Sicilian Trubi Formation (Punta di Maiata) have been estimated to assess the possible influence of changes in the alkenone-producing coccolithophorids on the U k′ 37–temperature relationship. The samples were dominated by small Reticulofenestra ( R. minuta and R. minutula) and the C 37 and C 38 methyl and ethyl unsaturation ratios (U k′ 37, U k 38Me and U k 38Et) were similar to those found in modern populations ( E. huxleyi and G. oceanica). Those results suggest that the Early Pliocene small Reticulofenetrids had a similar temperature sensitivity of U k′ 37 to that found in present day. These results support the application of the U k′ 37 modern calibrations to reconstruct SST at least back in the Pliocene. ► We have studied the coccolithophorid remains in sediments from the early Pliocene Sicilian Trubi Formation. ► Aim: to assess the influence of changes in the alkenone-producing coccolithophorids on the U k′ 37 –temperature relationship. ► The samples were dominated by small Reticulofenestra ( R. minuta and R. minutula). ► The C 37 and C 38 methyl and ethyl unsaturation ratios were similar to those in modern populations. ► Early Pliocene small Reticulofenetrids may have had a similar temperature sensitivity of U k′ 37 to that found in present day.
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ISSN:0031-0182
1872-616X
DOI:10.1016/j.palaeo.2011.03.017