On the astronomical origin of the Hallstatt oscillation found in radiocarbon and climate records throughout the Holocene
Nicola Scafetta, Franco Milani, Antonio Bianchini, Sergio Ortolani

TL;DR
This study demonstrates that the 2100-2500 year Hallstatt oscillation in radiocarbon and climate records has an astronomical origin linked to the resonance of the four Jovian planets, influencing cosmic rays and climate through orbital dynamics.
Contribution
It reveals the astronomical basis of the Hallstatt cycle, connecting planetary resonances to long-term climate and radionucleotide variations in Holocene records.
Findings
The Hallstatt cycle aligns with the 2318-year resonance of Jovian planets.
Orbital pulsations modulate cosmic ray flux and dust influx, affecting climate.
Multiple stable orbital resonances correlate with climate and solar activity records.
Abstract
An oscillation with a period of about 2100-2500 years, the Hallstatt cycle, is found in cosmogenic radioisotopes (C-14 and Be-10) and in paleoclimate records throughout the Holocene. Herein we demonstrate the astronomical origin of this cycle. Namely, this oscillation is coherent to the major stable resonance involving the four Jovian planets - Jupiter, Saturn, Uranus and Neptune - whose period is p=2318 yr. The Hallstatt cycle could derive from the rhythmic variation of the circularity of the solar system disk assuming that this dynamics could eventually modulate the solar wind and, consequently, the incoming cosmic ray flux and/or the interplanetary/cosmic dust concentration around the Earth-Moon system. The orbit of the planetary mass center (PMC) relative to the Sun is used as a proxy. We analyzed how the instantaneous eccentricity vector of this virtual orbit varies from 13,000 B.…
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Taxonomy
TopicsAstro and Planetary Science · Solar and Space Plasma Dynamics · Atmospheric Ozone and Climate
