A repository of vanilla long term integrations of the Solar System
arXiv:2012.05177 · doi:10.3847/2515-5172/abd103
Abstract
We share the source code and a 121 GB dataset of 96 long-term N-body simulations of the Solar System. This dataset can be analyzed by itself to study the dynamics of the Solar System. In addition, our simulations can be the starting point for future studies wishing to explore different initial conditions or additional physical effects on the Solar System. Our simulations can also be used as a comparison and benchmark for new numerical algorithms.
arXiv commentPublished in Res. Notes AAS, 3 pages, 1 figure, data repository: https://zenodo.org/record/4299102
References in corpus (6)
- REBOUND: An open-source multi-purpose N-body code for collisional dynamics
- WHFast: A fast and unbiased implementation of a symplectic Wisdom-Holman integrator for long term gravitational simulations
- REBOUNDx: A Library for Adding Conservative and Dissipative Forces to Otherwise Symplectic N-body Integrations
- Chaotic diffusion in the Solar System
- On the Dynamical Stability of the Solar System
- High order symplectic integrators for planetary dynamics and their implementation in REBOUND
Cited by in corpus (5)
- On the long-term stability of the Solar System in the presence of weak perturbations from stellar flybys
- Rare Event Sampling Improves Mercury Instability Statistics
- Stepsize errors in the -body problem: discerning Mercury's true possible long-term orbits
- Timescales of Chaos in the Inner Solar System: Lyapunov Spectrum and Quasi-integrals of Motion
- Simple physics and integrators accurately reproduce Mercury instability statistics