Critical Questions:
- What do the orbits of the planets really look like?
- What causes the tides?
- How do artificial satellites orbit the Earth?
Back in Section 2.9, I explained a bit about how orbits work. I said that things in space orbit other things because gravity acts as a centripetal force, resulting in circular motion that goes on forever because there is no friction to slow things down. Now I get to do the fun part: go back and explain why much of what I said then was incorrect.
First of all, no orbits are perfectly circular. Circular orbits require a very specific combination of speeds, forces, and distances, but nature doesn’t like specific requirements, preferring instead the exciting chaos of random numbers. If you take a planet and get it moving near a star, then there are a few possible outcomes depending on speed and distance. The planet may end up with a circular orbit, but that is so unlikely it’s essentially impossible.
The second option is an elliptical orbit. An ellipse is just a circle that has been flattened (a circle is actually just a special kind of ellipse, just like a square is a special kind of rectangle). The ellipse is the shape of all of the orbits we know about, including Earth’s path around the sun and the moon’s path around the Earth. And in an elliptical orbit, the thing that is being orbited doesn’t sit at the exact center of the ellipse, but is located a bit off to one side.





![By NASA Headquarters - Greatest Images of NASA (NASA-HQ-GRIN) [Public domain], via Wikimedia Commons 726px-NGC_4414_NASA-med](https://popphysics.com/wp-content/uploads/2012/05/726px-NGC_4414_NASA-med-300x247.jpg)

