choran said:
Oh, forgot to mention another one I just can't visualize: I shoot a single pulse of light away from me as I move at .5 c. I aim it at a distant star. I continue along at .5 c. A guy who started out standing next to me, motionless with respect to me, also looks at that pulse of light move away toward the star. Now, when that pulse hits the star (let's say it was one light year from me at start), I will be .5 light years from the star when the pulse reaches the star, while my buddy will still be one light year away from the star when the pulse hits the star. Given that, it is hard to see how the beam of light travels with the same velocity relative to both of us. Yep, it's a postulate, and SR says "That's life, no exceptions" but at the end of the day, it's a tough one.
Maybe it would help to visualize if you had some spacetime diagrams to look at. You've described everything according to the Inertial Reference Frame (IRF) of the guy who remained motionless and of the star. So here's a spacetime diagram that depicts what you described. The thick blue line represents the motionless guy, the thick red line is the star and you are shown as the thick black line. The dots represent one-year intervals of time for each object. The thin black line is the pulse of light that you shoot towards the star. The thin red line is its reflection back to you and the motionless guy:
Note that neither you nor the motionless guy can see the light arriving at the star, you both have to wait for the reflection to get back to each of you. And when you do see the reflection, you measure how long it took from the time it was emitted (at time zero) until you see the reflection, and you divide that interval by 2 and assume that the moment of reflection occurred at the half-way point of your measurement interval. This is the application of Einstein's second postulate because you are assuming that the light took the same amount of time to reach the star as it took for the reflection to reach you. Furthermore, you assume that the distance away from you that the star was at the moment of reflection was the same value in light-years.
It is easy to see that since it took 2 years for the light to propagate from its point of emission to the star and to reflect back to the motionless guy, he will determine that the light reached the star 1 year after it was emitted and that the star was 1 light-year away.
Now in order for him to determine where you were at that same time (according to his rest IRF), he has to send out another pulse of light one half year after you left. This pulse reflects off of you and returns to him at his time of 1.5 years. Since it took 1 year to make the round trip, he divides that by 2 and assumes that it reached you at his time of 1 year and that you were 0.5 light-years away:
All his measurements, assumptions and calculations agree with the coordinates depicted in the IRF describing the scenario because he remains at rest in it.
You, on the other hand, come to a different conclusion because you see the reflection at your time of 1.1547 years and so you assume that since the light took the same amount of time to get to the star as it did for the reflection to get back to you, the star was 0.577 light-years away from you and the reflection occurred at your time of 0.577 years.
Also, since you arrive at the star at your time of 1.732 years, you can calculate the relative speed between you and the star by taking the distance and dividing it by the difference in the two times. That is 0.577/(1.732-0.577) = 0.577/1.155 = 0.5.
These measurements, assumptions and calculations that you make do not match the coordinates that are depicted in the motionless guy's rest IRF but we can transform all the events (the dots and the intersections of the lines) from his rest IRF to your rest IRF using a speed of 0.5 to do the transformation. Here is the resulting spacetime diagram of your rest IRF:
Now you can see that all your determinations match the coordinates of your rest IRF. And note that all the measurements made by the motionless guy are also correctly depicted in your rest IRF just like your measurements are correctly depicted in his rest IRF. Well, I didn't include his measurement of your position in your rest IRF so I'll do another spacetime diagram that includes that detail:
Hopefully, these spacetime diagrams will help you visualize how a scenario described in one rest IRF can correctly show the measurements of all observers and how transforming to the rest IRF of another observer continues to show all the measurements of all observers. In other words, it doesn't matter what IRF we use, none is preferred, not even a rest IRF of any particular observer.
One last comment: if you want to cling to the idea that nature is operating on an absolute time, then you're claiming that one IRF is preferred above all others. But clearly, since you can always transform the coordinates of any IRF to any other IRF and they all correctly show all the measurements that every observer makes, there can be no way to identify a preferred IRF based on any measurement that anyone can make, so the concept of an absolute time is useless, don't you agree?