scorecompute
All demonstrationsKEPLER / TWO-BODY MODEL

Follow an ellipse through time.

Change the shape and elapsed time of an ideal orbit, then inspect its trajectory, position and orbital period.

compute_orbitTry the real call
Concept artwork · not calculation evidence
01 / UNDERSTAND THE METHOD

Orbit the geometry.

ILLUSTRATION · NOT A CALCULATION
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Preparing the orbital scene…

IDEAL ORBIT · INPUT PREVIEWOne ellipse. A moving world.Illustrative cycle · not the requested position or elapsed time.

Drag to orbit the camera. Body sizes are illustrative; orbital coordinates keep their proportions. The preview cycle follows ideal Kepler geometry at an illustrative speed. Returned coordinates stay fixed; camera rotation never changes them.

Teaching animation only · no MCP request
02 / ASK THE ACTUAL TOOL

Make it your experiment.

Complete tool arguments

Arrays, coordinates and nested contracts remain editable here. Units and limits are checked by the real tool.

Runs only when you press the button. Input edits discard the previous displayed result. Public compute limits apply.

KNOW WHAT THE RESULT MEANS

Useful evidence needs boundaries.

  • This educational two-body model has no observed epoch and does not locate a real planet in the sky.
  • Perturbations, other bodies, relativity and non-elliptical trajectories are omitted.
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