
With this applet, you can investigate mass ratios that lead to stable ring
systems vs. unstable ones. If the mass of each ring body is no more than
2.3 times the mass of Saturn divided by the cube of the number of ring
particles, then the system can be expected to be stable; otherwise not.
In the applet at left, M is the mass of Saturn (in Earthmasses), m is the mass of an individual ring body, and n is the number of ring bodies. The textfield labeled gamma is the ratio m*n^3/M. If this value is smaller than 2.3, the system will be stable. Large values will be unstable. You will find that you don't need to increase m very much to make the system unstable. If you set "warp" to 100, the integrator will show the instability very quickly. Give it a whirl. Note: the warp parameter only controls how often the screen is updatedlarge values mean that many time steps of the integrator are performed between each screen update. This makes the simulation run much faster as updating the screen image is more time consuming that a step of the integrator. For a JAVA applet version of the simulator, click here. 