Alright...
Now if I have two masses in space, and I know the radius between them, I can use the equation:
F = GMm/R²
It's Newton's Theory of Universal Gravitation, and it's used to calculate force.
If one body is traveling too fast around it's central hub, it will speed off. Yet if it's too slow, it will simply crash into the object it's orbiting around. Not a complex idea by any means.
Now my question is pretty simple - Starting with the force between my planet and its star, how do I figure out a good speed so that my planet will have a perfect orbit around it's star?
Thank you so much!
Brent
