When a planet or a comet moves around the Sun in an elliptical orbit, it travels faster when it is closer to the Sun (at the perihelion) and slower when it is farther away (at the aphelion). This is a direct consequence of the conservation of energy.
Imagine a roller‑coaster that starts at a high hill. As it rolls down, it speeds up because the gravitational potential energy is converted into kinetic energy. When it reaches the lowest point, it’s moving the fastest. Then it climbs back up, slowing down as it gains potential energy again. The same idea happens with planets: the Sun’s gravity pulls them in, turning potential energy into kinetic energy.
| Distance from Sun (AU) | Speed (km/s) |
|---|---|
| 0.39 (Mercury perihelion) | ~ 47.9 |
| 0.39 (Mercury aphelion) | ~ 29.8 |
| 1.00 (Earth perihelion) | ~ 30.3 |
| 1.00 (Earth aphelion) | ~ 29.3 |
The key takeaway is that in an elliptical orbit, speed is inversely related to distance from the Sun because the Sun’s gravitational pull converts potential energy into kinetic energy as the planet moves closer. This beautiful dance is governed by the simple yet powerful law of conservation of energy.