Hey so for kepler law of periods (rcubed on T^2 and so), what exactly is r?
I did some questions and it seems to be (in the example of Earth and the Sun) the distance from the Earth to the Sun + the radius of the Sun - why isn't the radius of the Earth included? Thanks!
For Kepler's \(r\) is always the distance between the
centres of the two objects, so you would definitely need to include Earth's radius, at least in theory. However, when compared to the distance between the Earth and Sun, Earth's radius is minuscule - Adding it or not won't change your answer in any significant way. It is general practice to, when the object orbiting is far smaller than the object it orbits (in most cases), ignore the radius of the smaller orbiting object. Just take the distance they give you and add it to the radius of what you are orbiting, for ease
