Restricted 3-Body (map)
In the circular restricted three-body problem, a massless particle moves in the rotating frame of two primaries in circular orbit. The effective potential includes gravitational and centrifugal terms; Coriolis forces appear in the equations of motion. This page integrates many initial conditions with zero corotating velocity to classify short-horizon outcomes: collision with a primary, escape to large radius, or remaining bound. A shadow trajectory with a tiny initial offset estimates sensitivity to initial conditions — a qualitative stand-in for chaotic regions with fractal-like basin boundaries.
Who it's for: Follows the Lagrange points page; for advanced students before full Poincaré sections.
Key terms
- restricted three-body problem
- corotating frame
- Jacobi-like dynamics
- chaos
- basin boundaries
How it works
The **circular restricted three-body problem** tracks a **massless** particle in the **corotating** frame of two **massive** bodies in a **circular** orbit. Here each grid cell starts the particle with **zero velocity** in that frame; forward integration reveals whether the orbit **hits** a primary (**collision**), **escapes** a large radius, or remains **bound** for a fixed horizon. A **nearby** duplicate initial condition measures **exponential-like** separation (**chaotic** sensitivity) — a **pedagogical** stand-in for **Lyapunov** structure. **Boundaries** between outcomes can be **fractally** complicated.
Key equations
Frequently asked questions
- Is the purple region “proved” chaotic?
- No — it is a finite-time separation proxy, not a rigorous Lyapunov exponent. It highlights sensitive dependence on initial conditions.
- Why zero initial velocity?
- It is a simple, repeatable sweep of initial positions. Different velocity choices would change the map.
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