A physics-based simulation demonstrating Kepler's Third Law: The square of an orbital period is proportional to the cube of the orbital distance. Enter orbital periods (in seconds) for up to seven moons, and watch them orbit in real-time!
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| d1 | px | |
| d2 | px | |
| d3 | px | |
| d4 | px | |
| d5 | px | |
| d6 | px | |
| d7 | px |
| t | s |