Lyapunov time
Template:Short description In mathematics, the Lyapunov time is the characteristic timescale on which a dynamical system is chaotic. It is named after the Russian mathematician Aleksandr Lyapunov. It is defined as the inverse of a system's largest Lyapunov exponent.<ref>Template:Cite book</ref>
UseEdit
The Lyapunov time mirrors the limits of the predictability of the system. By convention, it is defined as the time for the distance between nearby trajectories of the system to increase by a factor of e. However, measures in terms of 2-foldings and 10-foldings are sometimes found, since they correspond to the loss of one bit of information or one digit of precision respectively.<ref name="gaspard" /><ref>Template:Cite arXiv</ref>
While it is used in many applications of dynamical systems theory, it has been particularly used in celestial mechanics where it is important for the problem of the stability of the Solar System. However, empirical estimation of the Lyapunov time is often associated with computational or inherent uncertainties.<ref>Template:Cite journal</ref><ref>Template:Cite arXiv</ref>
ExamplesEdit
Typical values are:<ref name="gaspard">Pierre Gaspard, Chaos, Scattering and Statistical Mechanics, Cambridge University Press, 2005. p. 7</ref>
| System | Lyapunov time |
|---|---|
| Pluto's orbit | 20 million years |
| Solar System | 5 million years |
| Axial tilt of Mars | 1–5 million years |
| Orbit of 36 Atalante | 4,000 years |
| Rotation of Hyperion | 36 days |
| Chemical chaotic oscillations | 5.4 minutes |
| Hydrodynamic chaotic oscillations | 2 seconds |
| 1 cm3 of argon at room temperature | 3.7×10−11 seconds |
| 1 cm3 of argon at triple point (84 K, 69 kPa) | 3.7×10−16 seconds |