Me. Weber et al., Biological response to Milankovitch forcing during the late Albian (Kirchrode I borehole, northwestern Germany), PALAEOGEO P, 174(1-3), 2001, pp. 269-286
We studied the biological response to orbital forcing in marine Upper Albia
n sediments recovered from the 245 m-long Kirchrode I borehole in the Lower
Saxony basin in northwestern Germany. Results from quantitative analysis o
f planktonic and benthic foraminifera, of calcareous nannofossils, and radi
olaria were used for this study. Spectral analysis in the depth domain indi
cates for the high sedimentation rate part of the Upper Albian dominant per
iods with wavelengths of 10-13 m, 5-6 m, and 2-3 m, which we interpret to r
epresent the biological response to orbital forcing in the Milankovitch fre
quency bands eccentricity, obliquity, and precession, respectively. In addi
tion, a low amplitude 40-50 m cycle was found, which would represent the lo
ng-term eccentricity variation of roughly 400 ka. Microfossil cyclicity doe
s not change significantly within the whole core indicating sedimentation r
ates of 11-12 cm/ka on an average, with variations between 3.5 and 13 ka).
Microfossils show greater variability in their abundance changes than the p
hysical and chemical parameters and also greater power in the higher-freque
ncy bands (obliquity and precession). While most of the planktonic foramini
fer species studied are dominated by variations in the obliquity, most bent
hic foraminifer species show an additional strong influence of precession.
These differences in the cyclicity of the abundance changes are interpreted
as reflecting a stronger influence of low latitude water in the deep water
s of the Late Albian Lower Saxony basin than in the shallow waters. This ba
sin was part of a wide, 'Boreal' epicontinental sea, which was connected to
the Tethys to the south via the Polish strait and via the Paris basin, and
which was connected with the North Atlantic and Arctic to the north. In an
alogy to results from analysis of data from the Late Neogene, strong effect
s of precession interpreted as being more characteristic for changes/influe
nces triggered in the low latitudes and those of obliquity to be more chara
cteristic for influences from the high latitudes.
The presence of a relatively strong eccentricity cycle, not only in the com
pound parameters, but also in the abundance changes of single species durin
g the Late Albian means that there must have been a non-linear response to
orbital forcing and internal feedbacks. (C) 2001 Elsevier Science B.V. All
rights reserved.