Abstract
The quadrupole Kozai mechanism, which describes the hierarchical three-body problem for a test particle when the gravitational potential of the tertiary is expanded to leading order (quadrupole) in the ratio of semimajor axes, a/aper ≪ 1, and is doubly averaged over the orbits, is shown to be equivalent to a simple pendulum. The change in the eccentricity squared equals the height of the pendulum from its lowest point: emax2 − e2 = h = l (1 − cos θ). In particular, this results in useful expressions for the Kozai-Lidov cycles (KLC) period, and the maximal and minimal eccentricities in terms of orbital constants. We derive the equivalence using the vector coordinates α = j + e, β = j − e for the inner Keplerian orbit, where j is the normalized specific angular momentum, and e is the eccentricity vector. The equations of motion for α and β simplify to α = 2∂αφ × α and β = 2∂βφ × β, where φ is the normalized averaged interaction potential, and are symmetric under α ↔ β for the KLC quadratic potential. Their constraints simplify to α2 = β2 = 1, and they are distributed uniformly and independently on the unit sphere for a uniform distribution in phase space (with a fixed energy).
Original language | English |
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Pages (from-to) | L43-L46 |
Journal | Monthly Notices of the Royal Astronomical Society: Letters |
Volume | 541 |
Issue number | 1 |
Early online date | 20 May 2025 |
DOIs | |
State | Published - 1 Jul 2025 |
All Science Journal Classification (ASJC) codes
- Astronomy and Astrophysics
- Space and Planetary Science