Fast numerics for the spin orbit equation with realistic tidal dissipation and constant eccentricity
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Publication:1680319
DOI10.1007/s10569-017-9760-1zbMath1479.70070OpenAlexW2597306254WikidataQ59605225 ScholiaQ59605225MaRDI QIDQ1680319
Guido Gentile, Jonathan H. B. Deane, Michele V. Bartuccelli
Publication date: 15 November 2017
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10569-017-9760-1
Numerical methods for initial value problems involving ordinary differential equations (65L05) Orbital mechanics (70M20)
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Fast numerics for the spin orbit equation with realistic tidal dissipation and constant eccentricity
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Cites Work
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- Tidal synchronization of close-in satellites and exoplanets. II: Spin dynamics and extension to Mercury and exoplanet host stars
- Measures of basins of attraction in spin-orbit dynamics
- Quasi-periodic attractors in celestial mechanics
- Fast numerics for the spin orbit equation with realistic tidal dissipation and constant eccentricity
- The high-order Euler method and the spin-orbit model
- Solving Ordinary Differential Equations I
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