About the Newton's Cannon and Satellites simulation
In the Principia Newton imagined a cannon on a very high mountain. Fire the ball slowly and it falls back to Earth; fire it faster and it lands further round the curved planet; fire it at the right speed and the ground curves away beneath it as fast as it falls — it is in orbit. Faster still, it escapes. The Moon and every satellite are cannonballs that keep missing.
This orbital velocity simulation uses real Earth numbers: 7.9 km/s for a circular orbit at the surface and 11.2 km/s to escape. A second tab launches a satellite at any speed and angle and shades the areas it sweeps in equal times, showing Kepler's second law and the constant angular momentum behind it.
Also covers: orbital velocity, escape velocity, newton cannonball, satellite launch, kepler second law, equal areas.




