3D N-body simulation
Drag to orbit · scroll to zoom. Pick a central body, set distances in the body's natural units, then watch how the orbit evolves.
Time
Central body
G-type main-sequence star · 1 M☉
F = G·M·m / r². Distances input in AU.
Satellites
Edit · SAT-01
Circular speed at r = 21.064 km/s
0° = equatorial prograde. ±90° = polar.
Computed