

Lyapounov Time 
The Lyapounov time (L) is a parameter that measures the speed rate at which orbits diverge (or, in other words, it measures how much chaotic an orbit is). L is the period of time for the distance between two near possible orbits to increase of a factor e. The bigger this value is, the more stable is the orbit (L has typical values of a few years for chaotic asteroids, upt to 5 million years for the inner planets and hundred million years for the external planets).
For a non chaotic orbit (above
picture) the distance between two near orbits that have
similar initial conditions, is a linear function of time.
The two orbits diverge slowly, and their distance can be
expressed as a linear function of time:
For chaotic orbits, the distance between two near orbits can be expressed as an exponential function of time with the formula: This formula means that after a period of 2 L, the 2 orbits will be at a distance of , meaning that this distance varies exponentially with time. 