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When to Use Three-Body Problem 3D Explorer - Best Sessions and Limits


Open the Three-Body Problem 3D Explorer when you need the figure-8 choreography picture - Chenciner-Montgomery 2000 solution, Newton G=6.674e-11 literacy - and skip it when you only need a gravity-well surface or a flyby assist.


A five-minute classroom demo

A five-minute classroom demo starts when you open Three-Body Problem 3D Explorer, add a tiny IC kick, and pause so students see the once-periodic figure-8 trails drift apart while the unperturbed run keeps tracing the same loop.


Choreography literacy in Three-Body Problem 3D Explorer

Choreography literacy in Three-Body Problem 3D Explorer stays readable when you keep the facts panel open for G=6.674e-11 and the 2000 figure-8 solution while resetting to the classic initial conditions.


Sessions Three-Body Problem 3D Explorer does not fit

Sessions Three-Body Problem 3D Explorer does not fit are general N-body ephemerides, real asteroid or spacecraft trajectories, or gravity-well potential surfaces. Use Gravity Well 3D for potential surfaces or Gravitational Slingshot 3D for flyby assists. Walk the controls in the Three-Body Problem 3D Explorer step-by-step guide.

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