somega said:
Let's say I can see a star in a distance of 1ly in front of me.
I'm sitting on an office chair and begin to rotate with a speed of 1/s (1 rotation per second).
Then I consider me as not rotating and everything else as rotating.
This is basically where you're going wrong. You wish to apply the methods that you are familiar with from a non-rotating frame to a rotating frame, but the sort of methods you are familiar with are not applicable to a rotating frame.
Calling the rotating frame "non-rotating" still won't allow you to apply the methods that you appear to be using to a rotating frame.
The easiest solution is to simply not use rotating frames. A frame is something that one is free to chose, and it's generally wise to make the easiest possible choice, rather than to confuse oneself by making it unnecessarily complex.
The next step up is to learn how to deal with rotating frames in the context of Newtonian physics. AT has some helpful posts in this regard.
At the end of this, you should be able to work a problem in a non-rotating frame, or a rotating frame, transform a known solution from a non-rotating frame to a rotating frame and vica-versa, and demonstrate that the solutions are equivalent, so that it doesn't matter which frame you decide to use.
From your attempt to work out the collison speed, I would say you are not at this point yet.
After learning how to deal with rotating frames correctly in Newtonian physics, the next step would probably be to learn how to do special relativity in a non-rotating frame. The math isn't that hard, but some of the concepts may be challenging. A certain amount of un-learning may be necessary, this always seems to be tricky.
Only after you have mastered rotating Newtonian frames and non-rotating relativistic frames would I recommend even trying to learn about relativistically rotating frames.