Reduced variations in Earth's and Mars' orbital inclination and Earth's obliquity from 58 to 48 Myr ago due to solar system chaos
Richard E. Zeebe

TL;DR
This study uses geologic records and advanced modeling to show that chaos in the solar system caused reduced variations in Earth's and Mars' orbital inclination and Earth's obliquity from 58 to 48 million years ago, impacting planetary climate evolution.
Contribution
The paper introduces a new method combining geologic data with astronomical solutions to better understand solar system chaos and its effects on planetary orbital variations over millions of years.
Findings
Reduced orbital inclination and obliquity variations from 58 to 48 Ma.
Resonance transition around 50 Ma linked to chaos.
Changes in $g$- and $s$-mode contributions affecting orbital dynamics.
Abstract
The dynamical evolution of the solar system is chaotic with a Lyapunov time of only 5 Myr for the inner planets. Due to the chaos it is fundamentally impossible to accurately predict the solar system's orbital evolution beyond 50 Myr based on present astronomical observations. We have recently developed a method to overcome the problem by using the geologic record to constrain astronomical solutions in the past. Our resulting optimal astronomical solution (called ZB18a) shows exceptional agreement with the geologic record to 58 Ma (Myr ago) and a characteristic resonance transition around 50 Ma. Here we show that ZB18a and integration of Earth's and Mars' spin vector based on ZB18a yield reduced variations in Earth's and Mars' orbital inclination and Earth's obliquity (axial tilt) from 58 to 48 Ma -- the latter being consistent with paleoclimate records.…
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Taxonomy
TopicsAstro and Planetary Science · Stellar, planetary, and galactic studies · Geomagnetism and Paleomagnetism Studies
