Solar system chaos and the Paleocene-Eocene boundary age constrained by geology and astronomy
Richard E. Zeebe, Lucas J. Lourens

TL;DR
This study combines geologic data and a new astronomical model to establish an accurate astrochronology up to 58 million years ago, refining the Paleocene-Eocene boundary age and linking the PETM onset to orbital variations.
Contribution
It introduces a new astronomical solution (ZB18a) that aligns with geologic data, providing an improved astrochronology and boundary age, and reveals a chaotic resonance transition in the solar system at around 50 Ma.
Findings
New astrochronology up to 58 Ma established.
Refined Paleocene-Eocene boundary age to 56.01 Ma.
Linked PETM onset to a 405-kyr eccentricity maximum.
Abstract
Astronomical calculations reveal the solar system's dynamical evolution, including its chaoticity, and represent the backbone of cyclostratigraphy and astrochronology. An absolute, fully calibrated astronomical time scale has hitherto been hampered beyond 50 Ma, because orbital calculations disagree before that age. Here we present geologic data and a new astronomical solution (ZB18a), showing exceptional agreement from 58 to 53 Ma. We provide a new absolute astrochronology up to 58 Ma and a new Paleocene-Eocene boundary age (56.01 0.05 Ma). We show that the Paleocene-Eocene Thermal Maximum (PETM) onset occurred near a 405-kyr eccentricity maximum, suggesting an orbital trigger. We also provide an independent PETM duration (170 30 kyr) from onset to recovery inflection. Our astronomical solution requires a chaotic resonance transition at 50 Ma in the solar…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
