Conference Agenda

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Session Overview
Session
2.2-2 The imprint of astronomical climate forcing: geochronometer and paleoclimate archive
Time:
Monday, 24/Aug/2020:
5:50pm - 7:05pm

Location: Room 2.02

Session Abstract

by Christian Zeeden1, Diederik Liebrand2, Anna-Joy Drury3, Stefanie Kaboth-Bahr4, Qiang Fang5

1: Leibniz Institute for Applied Geophysics, Hanover, Germany; 2: MARUM, Bremen, Germany; 3: University College London, London, UK; 4: University of Potsdam, Potsdam, Germany; 5: China University of Geosciences, Beijing, China

The pacing of the global climate system by variations in orbital parameters is clearly demonstrated in the timing and specific patterns of e.g. sapropels and glacial-interglacial cycles beside many other examples. The imprint of astronomical cycles can be used as high-precision geochronometer, and as paleoclimatic information. We invite contributions utilizing the imprint of Milankovic cycles as preserved in the geological record in any way. This includes the often not very well understood mechanisms that translate this forcing into geoarchives. Submissions exploring proxy data and/or modelling work are welcome; we aim to bring together proxy-based, theoretical and modelling studies focused on global and regional climate responses to astronomical forcing at different time scales.


Presentations
5:50pm - 6:05pm
ID: 259
Virtual Presentation | ECS

Age-depth model derived from borehole logging and seismic data - sedimentological evolution of Lake Ohrid (North Macedonia/Albania) for the last 1 million years

Arne Ulfers1, Christian Zeeden1, Bernd Wagner2, Sebastian Krastel3, Thomas Wonik1

1Leibniz Institute for Applied Geophysics, Germany; 2Institute of Geology and Mineralogy, University of Cologne, Germany; 3Institute of Geosciences, Christian-Albrechts-Universitaet zu Kiel, Germany

To understand the evolution of lake basins, a robust age-depth model is essential. Usually, such model is created based on core material using various dating techniques (e.g. radiometric dating, magnetostratigraphy, tephra dating/identification, biostratigraphy etc.). However, suitable core material is not always available and other less direct methods have to be applied. In this study, we present an approach to develop an age-depth model based on integrating downhole logging data and seismic survey data from Lake Ohrid to obtain a rough but representative model before core opening. Logging data was acquired during an International Continental Scientific Drilling Program campaign in 2013 and seismic data is from pre-site surveys conducted in 2007 and 2008.

First, the interpretation of seismic data and the use of cyclostratigraphic methods on downhole logging data lead to development of age-depth models derived from direct correlation to the LR04 benthic stack (Lisiecki and Raymo, 2005) at three drill sites at the Lake Ohrid. Based on seismic surveys data, marker horizons are interpreted to support our understanding of accumulation rates. Additional information on sedimentation processes is provided by the evaluation of eccentricity related amplitude modulations using Meyers' timeOptTemplate method (2015, 2019). The use of various, independent methods and the comparison of their age estimations ensures a robust verification of obtained age-depth models.

In a second step, we apply cluster analysis to the physical properties of the sediments, construct artificial lithology logs and integrate them into the age-depth models. This step makes first interpretations of the sedimentological evolution possible.

Ulfers-Age-depth model derived from borehole logging and seismic data_Info.pdf


6:05pm - 6:20pm
ID: 278
Virtual Presentation

Decadal sea surface temperature variability in the Eastern Mediterranean during the Last Interglacial

Igor Obreht1, David De Vleeschouwer1, Lars Wörmer1, Michal Kucera1, Devika Varma1, Thomas Laepple1,2, Jenny Wendt1, Matthias Prange1, Sri D. Nandini-Weiss1, Hartmut Schulz3, Kai-Uwe Hinrichs1

1MARUM, University of Bremen, Germany; 2Alfred Wegener Institute Helmholtz Centre for Polar and Marine Research; 3University of Tübingen

Precise future predictions of Mediterranean sea surface temperature (SST) variability as one of the most sensitive regions to climate change are hampered by insufficient knowledge of accurate SST reconstructions in resolution relevant for human time-scales from warmer-than-present periods. The Last Interglacial (LIG; ~130,000 to 116,000 years ago) is the most recent period with warmer-than-present climate; however, continuous subdecadal records of LIG SST are unavailable due to a small number of undisturbed sedimentary records and sample-size limitations of conventional methodologies. We circumvent these issues by applying Mass Spectrometry Imaging on finely laminated sapropel S5 sediment deposited in the Eastern Mediterranean; the result is an alkenone-based SST time-series in 1-4 year resolution. These data reveal prominent and rapid decadal SST oscillations in the Eastern Mediterranean with a ~60 years cyclicity that is persistent throughout most of the record, suggesting similar LIG decadal climate oscillations as in the Holocene. We also compare the reconstructed rate of SST change during the LIG to the present-day observational record, and find that LIG temperature change often exceeded the present-day rate of change. On the other hand, comparison of the LIG multidecadal SST to the projected increase in Mediterranean SST until 2100 AD suggests SST increase at the end of the 21st century to be unprecedented in magnitude and duration. We thus conclude that future warming of the Mediterranean could cause an unrivalled change in the Mediterranean planktonic ecosystems and their biological responses.

Obreht-Decadal sea surface temperature variability in the Eastern Mediterranean during the Last Interglacial_Info.pdf


6:20pm - 6:35pm
ID: 269
Virtual Presentation | ECS

Milankovitch-scale paleoclimatic variability recorded in Permian loessite (south-central France)

Lily S. Pfeifer1, Linda Hinnov2, Christian Zeeden3, Christian Rolf3, Christian Laag3,4, Gerilyn S. Soreghan1

1University of Oklahoma, United States of America; 2Department of Atmospheric, Oceanic, and Earth Sciences, George Mason University, Fairfax, VA, United States; 3Leibniz Institute for Applied Geophysics, Hanover, Germany; 4Institut de Physique du Globe de Paris (IPGP), CNRS, Université de Paris, Paris, France

We present the findings from our recent paper wherein rock magnetic data record discernible Milankovitch-scale paleoclimatic variability through the Permian Salagou Formation loessite (south-central France). Analysis and modeling of this stratigraphic series (~1000 m of magnetic susceptibility data measured with a portable magnetic susceptibility meter) shows a persistent 10-m-thick cyclicity inferred to represent orbital eccentricity-scale (~100 kyr) variability through the middle to late Cisuralian (ca. 285—275 Ma), and subordinate, higher-frequency cycles (3.3—3.5 and ~1.8 m-thick) that likely represent obliquity and precession-scale variability. Optimal sedimentation rates increase up-section, ranging between 9.4 cm/kyr and 13 cm/kyr. As evinced by laboratory rock magnetic data, the driver of the magnetic signal in the Salagou Formation is hematite, which has generally low magnetic enhancement compared to Eurasian Quaternary loess deposits. If the magnetic signal is pedogenic, then the ~10 m thick cyclicity may represent the thickness of loessite-paleosol couplets in the Salagou Formation. The predominance of hematite (as opposed to magnetite and maghemite) may be attributed to differing conditions of formation such as more arid and/or oxidizing climate conditions than in present Eurasia and/or post depositional oxidation of magnetite and maghemite. This work contributes to a growing evidence for astronomically-forced climate change in Permian loessite at low latitudes.

Pfeifer-Milankovitch-scale paleoclimatic variability recorded_Info.pdf


6:35pm - 6:50pm
ID: 318
Virtual Presentation

Astronomically forced sphalerite growth and groundwater circulation in the Upper Mississippi Valley District, USA

Mingsong Li, Hubert Barnes

Pennsylvania State University, United States of America

Groundwater plays an essential role in global water cycles via feedback between groundwater and climate systems. However, the geologic history of groundwater activity remains unclear due to limited data. Sphalerite color banding in the Upper Mississippi Valley District (USA) is apparently caused by variation in oxidation state during sulfide precipitation which is controlled by the penetration of deeply circulating groundwater. Here, time series analysis of the grayscale profile of the Permian sphalerite banding in this district shows the banding correlates with Earth’s eccentricity, obliquity, and precession forcing.

We have found that this astronomical forcing controlled penetration of groundwater into sedimentary hydrothermal fluids which regulated regionally the penetration of groundwater into the ore zone to fixt sphalerite banding. Orbital forcing of climate had a significant impact on a groundwater reservoir at depths near 1 km. The results demonstrate that banding in sphalerite follows the Milankovitch climate frequencies over 103 – 105 years. Consequently, groundwater oxidation has a major role in depositing the iron-rich bands of the sphalerite and, as a final corollary, that the banding itself can be used to decipher the effects of climate on groundwater variations in the global water cycle.

Li-Astronomically forced sphalerite growth and groundwater circulation_Info.pdf