A secular solar system resonance that disrupts the dominant cycle in Earth's orbital eccentricity (g2-g5): Implications for astrochronology
Richard E. Zeebe, Margriet L. Lantink

TL;DR
This study reveals that the dominant 405,000-year Earth's orbital eccentricity cycle, long considered stable for geological dating, can become unstable due to solar system chaos, impacting astrochronology and climate models.
Contribution
It demonstrates that the (g2-g5) eccentricity cycle can become unstable over long timescales due to secular resonance, challenging its use as a reliable chronometer.
Findings
(g2-g5) can become unstable over long periods.
Resonance σ_{12} causes (g2-g5) disruption.
Implications for astrochronology and climate models.
Abstract
The planets' gravitational interaction causes rhythmic changes in Earth's orbital parameters (also called Milankovi\'c cycles), which have powerful applications in geology and astrochronology. For instance, the primary astronomical eccentricity cycle due to the secular frequency term (g2-g5) (~405 kyr in the recent past) utilized in deep-time analyses is dominated by Venus' and Jupiter's orbits, aka long eccentricity cycle. The widely accepted and long-held view is that (g2-g5) was practically stable in the past and may hence be used as a "metronome" to reconstruct accurate ages and chronologies. However, using state-of-the-art integrations of the solar system, we show here that (g2-g5) can become unstable over long time scales, without major changes in, or destabilization of, planetary orbits. The (g2-g5) disruption is due to the secular resonance = (g1 - g2) + (s1 - s2),…
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Taxonomy
TopicsAstro and Planetary Science · Geophysics and Gravity Measurements · Stellar, planetary, and galactic studies
