Copyright © Michael Richmond.
This work is licensed under a Creative Commons License.
Today, we will look at how one can use the motion of objects around their center of mass to detect planets around other stars. We'll use tools you've studied in this class:
We'll also have to include one physical phenomenon we haven't studied -- but which you'll see in University Physics II:
Okay, now let's explore other stellar systems.
Copyright © Michael Richmond.
This work is licensed under a Creative Commons License.