Sealevel changes control diagenetic dolomite formation in hemipelagic sediments of
the Peru Margin
Patrick Meister
a,b,
⁎, Stefano M. Bernasconi
b
, Crisógono Vasconcelos
b
, Judith A. McKenzie
b
a
Max-Planck-Institute for Marine Microbiology, Celsiusstrasse 1, 28359 Bremen, Germany
b
Geological Institute, ETH Zürich, 8092 Zürich, Switzerland
ABSTRACT ARTICLE INFO
Article history:
Received 22 March 2007
Received in revised form 16 March 2008
Accepted 5 April 2008
Keywords:
dolomite
oxygen isotopes
deep biosphere
glacial/interglacial cycles
paleo-temperatures
Peru Margin
The first experimentally determined temperature dependent oxygen-18 fractionation factor between
dolomite and water at low temperatures [Vasconcelos, C., McKenzie, J.A., Warthmann, R., Bernasconi, S.,
2005. Calibration of the δ
18
O paleo-thermometer with dolomite formed in microbial cultures and natural
environments. Geology 33, 317–320] allows now the precise calculation of temperatures during early
diagenetic dolomite precipitation. We use δ
18
O values of early diagenetic dolomite beds sampled during ODP
Legs 112 and 201 on the Peru continental margin (Sites 1227, 1228 and 1229) [Meister, P., McKenzie, J.A.,
Vasconcelos, C., Bernasconi, S., Frank, M., Gutjahr, M., Schrag, D.P., 2007. Dolomite formation in the dynamic
deep biosphere, results from the Peru Margin, OPD Leg 201. Sedimentology 54, 1007–1032] to calculate
paleo-porewater temperatures at the time of dolomite precipitation. We assumed unaltered seawater δ
18
O
values in the porewater, which is supported by δ
18
O values of the modern porewater presented in this study.
The dolomite layers in the Pleistocene part of the sedimentary columns showed oxygen isotope temperatures
up to 5 °C lower than today. Since Sites 1228 and 1229 are located at 150 and 250 m below sealevel,
respectively, their paleo-porewater temperatures would be influenced by considerably colder surface water
during glacial sealevel lowstands. Thus, Pleistocene dolomite layers in the Peru Continental margin probably
formed during glacial times. This finding is consistent with a model for dolomite precipitation in the Peru
Margin recently discussed by Meister et al. [Meister, P., McKenzie, J.A., Vasconcelos, C., Bernasconi, S., Frank,
M., Gutjahr, M., Schrag, D.P., 2007. Dolomite formation in the dynamic deep biosphere, results from the Peru
Margin, OPD Leg 201. Sedimentology 54, 1007–1032], where dolomite forms episodically at the sulphate
methane interface. It was shown that the sulphate methane interface migrates upwards and downwards
within the sedimentary column, but dolomite layers may only form when the sulphate–methane interface
stays at a fixed depth for a sufficient amount of time. We hypothesize that the sulphate–methane interface
persists within TOC-rich interglacial sediments, while this zone is buried by TOC-poor sedimentation during
glacial times. Thus, the presented oxygen isotope data provide additional information on the timing of early
diagenetic dolomite formation and a possible link between episodicity in dolomite formation and sealevel
variations. A similar link between early diagenesis and oceanography may also explain spacing of dolomite
layers in a Milankovitch type pattern observed in the geological record, such as in the Miocene Monterey
Formation.
© 2008 Elsevier B.V. All rights reserved.
1. Introduction
Dolomite layers and nodules are commonly observed in the
geological record in organic carbon-rich deep-sea hemipelagic sedi-
ments. They are found in the Miocene Monterey Fm. (Murata et al.,
1969; Baker and Burns, 1985; Burns and Baker, 1987; Burns et al., 1988;
Compton, 1988) and were first observed in recent ocean margin
sediments during drilling in the California Borderland (DSDP Leg 63;
Pisciotto and Mahoney, 1981), the Gulf of California (DSDP Leg 64;
Kelts and McKenzie, 1982), and later on the Peru Margin (ODP Leg 112;
Suess et al., 1988). These studies led to the formulation of the “organic
dolomite model”, where the essential part of the inorganic carbon is
delivered from organic matter degradation. Claypool and Kaplan
(1974) concluded from the variable positive and negative δ
13
C values
that dolomite layers form at different depths and in different diage-
netic zones. In the sulphate reduction zone, carbonate with negative
δ
13
C values is produced, and, in the methanogenic zone, carbonate
with positive δ
13
C values is produced. The diagenetic zone, in which
dolomite formation occurs, was considered to depend on the
sedimentation rate, which limits the downward diffusion of SO
4
2-
and, thus, the depth of organic matter degradation, which leads to
supersaturation with respect to dolomite (Kelts and McKenzie, 1984).
Marine Geology 252 (2008) 166–173
⁎ Corresponding author. Max-Planck-Institute for Marine Microbiology, Celsius-
strasse 1, 28359 Bremen, Germany.
E-mail address: pmeister@mpi-bremen.de (P. Meister).
0025-3227/$ – see front matter © 2008 Elsevier B.V. All rights reserved.
doi:10.1016/j.margeo.2008.04.001
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