Articles | Volume 13, issue 9
https://doi.org/10.5194/cp-13-1129-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
https://doi.org/10.5194/cp-13-1129-2017
© Author(s) 2017. This work is distributed under
the Creative Commons Attribution 3.0 License.
the Creative Commons Attribution 3.0 License.
Astronomical calibration of the Ypresian timescale: implications for seafloor spreading rates and the chaotic behavior of the solar system?
MARUM – Center for Marine Environmental Sciences, University of
Bremen, Leobener Straße, 28359 Bremen, Germany
Ursula Röhl
MARUM – Center for Marine Environmental Sciences, University of
Bremen, Leobener Straße, 28359 Bremen, Germany
Thomas Frederichs
Faculty 5 Geosciences, University of Bremen, 28359 Bremen, Germany
Claudia Agnini
Dipartimento di Geoscienze, Università degli Studi di Padova, via G.
Gradenigo 6, 35131 Padua, Italy
Isabella Raffi
Dipartimento di Ingegneria e Geologia (InGeo) – CeRSGeo, Universitaà
degli Studi “G. d'Annunzio” Chieti-Pescara, via dei Vestini 31, 66013
Chieti-Pescara, Italy
James C. Zachos
Department of Earth and Planetary Sciences, University of California
Santa Cruz, 1156 High Street, Santa Cruz, CA 95064, USA
Roy H. Wilkens
Institute of Geophysics and Planetology, University of Hawai'i,
Honolulu, HI 96822, USA
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Latest update: 23 Nov 2024
Short summary
We assembled a very accurate geological timescale from the interval 47.8 to 56.0 million years ago, also known as the Ypresian stage. We used cyclic variations in the data caused by periodic changes in Earthäs orbit around the sun as a metronome for timescale construction. Our new data compilation provides the first geological evidence for chaos in the long-term behavior of planetary orbits in the solar system, as postulated almost 30 years ago, and a possible link to plate tectonics events.
We assembled a very accurate geological timescale from the interval 47.8 to 56.0 million years...