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Geological Society, London, Special Publications; 2001; v. 183; p. 163-183;
DOI: 10.1144/GSL.SP.2001.183.01.09
© 2001 Geological Society of London

Astronomical calibration of the Danian time scale

Ursula Röhl1, James G. Ogg2, Tricia L. Geib2 & Gerold Wefer1

1 Geosciences Department, Bremen University, D-28334 Bremen, Germany uroehl{at}allgeo.uni-bremen.de
2 Department of Earth and Atmospheric Sciences, Purdue University, West Lafayette, In 47907-1397, USA

Ocean Drilling Program Sites 1001A (Caribbean Sea) and 1050C (western North Atlantic) display obliquity and precession cycles throughout polarity zone C27 of the late Danian stage (earliest Cenozoic time). Sliding-window spectra analysis and direct cycle counting on downhole logs and high-resolution Fe variations at both sites yield the equivalent of 35–36 obliquity cycles. This cycle-tuned duration for polarity chron C27 of 1.45 Ma (applying a modern mean obliquity period of 40.4 ka) is consistent with trends from astronomical tuning of early Danian polarity chron C29 and 40Ar/39Ar age calibration of the Campanian-Maastrichtian magnetic polarity time scale. The cycle-tuned Danian stage (sensu Berggren et al. 1995, in SEPM Special Publications, 54, 129–212) spans 3.65 Ma (65.5–61.85 Ma). Spreading rates on a reference South Atlantic synthetic profile display progressive slowing during the Maastrichtian to Danian stages, then remained relatively constant through late Palaeocene and early Eocene time.