List
Language
Relative equilibrium
Relative equilibriumUnstable
Lagrange equilateral
Orbit: the bodies keep an equilateral triangle shape while the whole system rotates.
Status: exact relative equilibrium, but unstable for equal masses by the classical Routh-Gascheau condition.
Source: one of Euler and Lagrange's classical central configurations.
Thin dashed circles show the ideal relative-equilibrium orbit.
Integrator
t = 0.00
zoom 1.00x