Special relativity clocks observed from two frames

AI Thread Summary
In the discussion, observers S and S' are moving relative to each other at a speed of 0.6c, each with synchronized clocks set to zero. For part A, the time recorded on the S' clock when the S clock shows 5 microseconds can be calculated using time dilation. The confusion arises in part B, where the observer S needs to determine what they actually see on the S' clock through a telescope at the same moment. It's emphasized that the time calculated using relativistic effects differs from what is visually observed, highlighting a common misunderstanding among beginners. Understanding the distinction between calculated time and observed time is crucial for solving the problem accurately.
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Homework Statement


Observers S and S' stand at the origins of their respective frames, which are moving relative to each other with a speed of .6c. Each has a standard clock, which, as usual, they set to zero when the two origins coincide. Observer S keeps the S' clock visually in sight. (a) What time will the S' clock record when the S clock records 5 micro seconds? (b) What time will Observer S actually read on the S' clock when his own clock reads 5 micro seconds?


Homework Equations


time dilation: t = gamma (proper time)


The Attempt at a Solution


I can solve part A by using time dilation. My confusion comes in understanding how to interpret the conditions set on part b - how is part b different from part A? I know that for time dilation, the proper time is the time measured when the clock is at rest. But how can I calculate what one observer sees on a clock in another frame?
 
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I assume that part a is in observer S's frame.
I guess they just want to make it clear
that the relativistically calculated time on the S' clock
is different from the time on clock S' as
actually physically observed by S through a telescope.

This is a common mistake by beginners and
they just want to make sure that everyone understands it correctly
 
but how would I go about calculating what observer S sees on the clock of S' through a telescope? That's the part I don't understand.
 
work backward
 
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