Maximilian Vahlenkamp
A lower to middle Eocene astrochronology for the Mentelle Basin (Australia) and its implications for the geologic time scale
Vahlenkamp, Maximilian; De Vleeschouwer, David; Batenburg, Sietske J.; Edgar, Kirsty M.; Hanson, Emma; Martinez, Mathieu; Pälike, Heiko; MacLeod, Kenneth G.; Li, Yong-Xiang; Richter, Carl; Bogus, Kara; Hobbs, Richard W.; Huber, Brian T.
Authors
David De Vleeschouwer
Sietske J. Batenburg
Kirsty M. Edgar
Emma Hanson
Mathieu Martinez
Heiko Pälike
Kenneth G. MacLeod
Yong-Xiang Li
Carl Richter
Kara Bogus
Richard W. Hobbs
Brian T. Huber
Abstract
The geologic time scale for the Cenozoic Era has been notably improved over the last decades by virtue of integrated stratigraphy, combining high-resolution astrochronologies, biostratigraphy and magnetostratigraphy with high-precision radioisotopic dates. However, the middle Eocene remains a weak link. The so-called “Eocene time scale gap” reflects the scarcity of suitable study sections with clear astronomically-forced variations in carbonate content, primarily because large parts of the oceans were starved of carbonate during the Eocene greenhouse. International Ocean Discovery Program (IODP) Expedition 369 cored a carbonate-rich sedimentary sequence of Eocene age in the Mentelle Basin (Site U1514, offshore southwest Australia). The sequence consists of nannofossil chalk and exhibits rhythmic clay content variability. Here, we show that IODP Site U1514 allows for the extraction of an astronomical signal and the construction of an Eocene astrochronology, using 3-cm resolution X-Ray fluorescence (XRF) core scans. The XRF-derived ratio between calcium and iron content (Ca/Fe) tracks the lithologic variability and serves as the basis for our U1514 astrochronology. We present a 16 million-year-long (40-56 Ma) nearly continuous history of Eocene sedimentation with variations paced by eccentricity and obliquity. We supplement the high-resolution XRF data with low-resolution bulk carbon and oxygen isotopes, recording the long-term cooling trend from the Paleocene-Eocene Thermal Maximum (PETM – ca. 56 Ma) into the middle Eocene (ca. 40 Ma). Our early Eocene astrochronology corroborates existing chronologies based on deep-sea sites and Italian land sections. For the middle Eocene, the sedimentological record at U1514 provides a single-site geochemical backbone and thus offers a further step towards a fully integrated Cenozoic geologic time scale at orbital resolution.
Citation
Vahlenkamp, M., De Vleeschouwer, D., Batenburg, S. J., Edgar, K. M., Hanson, E., Martinez, M., Pälike, H., MacLeod, K. G., Li, Y.-X., Richter, C., Bogus, K., Hobbs, R. W., & Huber, B. T. (2020). A lower to middle Eocene astrochronology for the Mentelle Basin (Australia) and its implications for the geologic time scale. Earth and Planetary Science Letters, 529, Article 115865. https://doi.org/10.1016/j.epsl.2019.115865
Journal Article Type | Article |
---|---|
Acceptance Date | Sep 26, 2019 |
Online Publication Date | Oct 9, 2019 |
Publication Date | Jan 1, 2020 |
Deposit Date | Oct 15, 2019 |
Publicly Available Date | Oct 15, 2019 |
Journal | Earth and Planetary Science Letters |
Print ISSN | 0012-821X |
Publisher | Elsevier |
Peer Reviewed | Peer Reviewed |
Volume | 529 |
Article Number | 115865 |
DOI | https://doi.org/10.1016/j.epsl.2019.115865 |
Public URL | https://durham-repository.worktribe.com/output/1288002 |
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Copyright Statement
©2019 The Author(s).Published by Elsevier B.V. This is an open access article under the CCBY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/).
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