Untangling the Palaeocene climatic rhythm: an astronomically calibrated Early Palaeocene magnetostratigraphy and biostratigraphy at Zumaia (Basque basin, northern Spain)☆
Introduction
The tuning of primarily marine cyclic sedimentary successions to orbital solutions for the recent past has proved to be a powerful geochronometer (see [1] for a recent review). Milankovitch climate cyclicity tied to magnetic polarity stratigraphy for 0–5.23 Ma has resulted in an astronomical polarity time scale (APTS) accepted as the definitive chronology for the Pliocene and Pleistocene, superseding other chronostratigraphic frameworks (i.e. high-precision radiometric dating is actually calibrated against the APTS). Extensions of the astronomical calibration to the late Miocene (5.23 to ∼10 Ma) and older periods are increasingly being published [2], [3]. Developing orbitally tuned time scales in strata older than the limit of precise astronomical solutions for the Earth’s orbital variations (estimated to be 35–50 Ma in [4]) has so far been risky. Nevertheless, refinements in long-term integrations of planetary orbits make it possible to extend the accuracy of astronomical time series to increasingly older ages [5]. In any case, it is possible to build up an orbital chronology, albeit floating, if the more stable eccentricity modulation of precession can be identified in the geological record [1], [4], [6].
The aim of this paper is to present a detailed magnetostratigraphy and biostratigraphy along the cyclic hemipelagic lower Palaeocene succession in the Zumaia section from the Basque basin, northern Spain, and to assess the Milankovitch climate forcing on the lithologic stacking pattern to derive an Early Palaeocene cyclochronology.
Section snippets
Geological setting and previous work
The Zumaia Palaeocene section (latitude/longitude 42°18.00′N/2°15.30′W) is a sea-cliff section outcropping at the Aitzgorri headland and Itzurun beach, in the Gipuzkoa province of northern Spain (Fig. 1, Fig. 2). The Palaeocene sediments were deposited at an estimated water depth of about 1000 m in an E–W elongated offshore basin called the Basque basin opening westwards into the Bay of Biscay [7], [8] (Fig. 1). The Early Palaeocene interval is represented by rhythmic alternations of
Biostratigraphic determinations
Fifty-three samples (average weight of 1 kg) were collected for planktonic foraminifera biostratigraphy from the less indurated levels (marls and marly limestones) along the studied section (Image 1, Image 21). Samples were washed and screened to obtain a residue in the 50–500-μm grain-size fraction, which has been studied under a Nikon SMZ-U binocular lens equipment. To make it chronostratigraphically useful, the study of planktonic foraminifera has
Planktonic foraminifera
All studied samples contained planktonic foraminifera although the content was variable with the poorest at the K/T boundary clay (200–300 specimens/g and smaller than 100 μm). Higher in the section, the richness, diversity and size of planktonic foraminifera increase gradually, allowing the separation of more than 500 specimens per sample.
The distribution of species at Zumaia (Fig. B1 and Table A11 in the Background Data Set) largely coincides with that proposed in the standard biozonation
Magnetostratigraphy
The intensity of the NRM was generally around 1×10−3 A/m although it was lower for some of the whitish-coloured carbonate-rich beds. Three magnetisation components can be recognised in most samples upon demagnetisation, in addition to a viscous magnetisation removed below 100–150°C. A low-temperature component (L) is unblocked between 100–150°C and 250–300°C (Fig. 3). Component L corresponds in geographic co-ordinates to the present-day field dipole and therefore is regarded as a secondary
Cyclostratigraphy
The stacking of hemipelagic marlstone and limestone lithologies at Zumaia defines a cyclic (or rhythmic) bedding pattern [8] (Fig. 5 and Image 1, Image 21). The basic noticeable cycles are the bedding couplets, which consist of alternating pairs of marl and limestone beds in different relative proportions or a vertical variation in carbonate content within marl or limestone intervals. The thickness of these couplets ranges from 15 to 45 cm (average of about 25 cm). The limestone/marl couplets
Evaluation of the tuned time series
The tuned time series was re-evaluated with the CWT to explore the existence of long-period periodicities (Fig. 8). Indeed, the eccentricity/bundle cycle now appears persistent throughout the entire section and centred at a period of 102 kyr. Power at the precession band (centred at 21 kyr in the global spectrum) is also obvious all through the section. No persistent longer-period peaks are found for the coded lithologic series under study. Nevertheless, significant power at ∼360 kyr exists
Conclusions
The new astronomically calibrated Early Palaeocene chronology from Zumaia is a step forward in current efforts for the development of integrated orbitally tuned time scales (i.e. [1], [47]. The precession (∼21 kyr) and the short eccentricity cycle (∼110 kyr) were unambiguously identified and provide the basis for a cycle-tuned Early Palaeocene polarity and biostratigraphic time scales. The Zumaia chronostratigraphic framework is more complete (and slightly different) than the astronomically
Acknowledgements
J.D.-T. acknowledges support through a grant from EU Project ERBFMRXCT98-0247 and J.I.B. from a ‘Ramón y Cajal’ research grant from the Spanish Ministry of Science and Technology. Wavelet software was provided by C. Torrence and G. Compo, and is available at URL http://paos.colorado.edu/research/wavelets/. Constructive comments by reviewer B. Cramer helped to improve the paper. This research is a contribution to projects UPV 121-310-EB191/98, 121.310-G12/99 and DGICCYT-PB98-0243.[BARD]
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Supplementary data associated with this article can be found at doi:10.1016/S0012-821X(03)00557-0