*Michael Fowler, UVa Physics, 12/1/07*

The object of this exercise is to show explicitly how it is possible for two
observers in inertial frames moving relative to each other at a relativistic
speed to each see the other’s clocks as running slow and as being
unsynchronized, and yet if they both look at the same clock at the same time
from the same place (which may be far from the clock), they will *agree*
on what time it shows!

Suppose that in Jack’s frame we have two synchronized clocks *C*_{1} and *C*_{2} set 18 x 10^{8}
meters apart (that’s about a million miles, or 6 light-seconds). Jill’s spaceship, carrying a clock
*C'*,* * is traveling at 0.6*c*, that is 1.8
x 10^{8} meters per second, parallel to the line *C*_{1}*C*_{2}, passing close by each clock.

Suppose *C' * is
synchronized with *C*_{1}
as they pass, so both read zero.

As measured by Jack the spaceship will take just 10 seconds to reach *C*_{2}, since the distance is 6
light seconds, and the ship is traveling at 0.6*c*.

What does clock *C'* (the clock on
the ship) read as it passes *C _{2}*?

The time dilation factor

_{}

so *C**'*, Jill’s clock, will read 8 seconds.

Thus if both Jack and Jill are at *C _{2}*
as Jill and her clock

*How, then, can Jill claim
that Jack’s clocks C*_{1},* C*_{2}* are the ones that
are running slow?*

To Jill, *C _{1}*,

Therefore, Jill will
conclude that since *C*_{2}
reads 10 seconds as she passes it, at that instant *C*_{1} must be registering 6.4
seconds. Jill’s own clock
reads 8 seconds at that instant, *so she concludes that C*_{1}* is running slow by the
appropriate time dilation factor of 4/5*. This is how the change in synchronization
makes it possible for both Jack and Jill to see the other’s clocks as
running slow.

Of course, Jill’s assertion that as she passes Jack’s second
“ground” clock *C*_{2} the first “ground”
clock *C*_{1} must be registering 6.4 seconds is not completely
trivial to check! After all, that
clock is now a million miles away!

Let us imagine, though, that both observers are equipped with Hubble-style telescopes attached to fast acting cameras, so reading a clock a million miles away is no trick.

To settle the argument, the two of them agree that as she passes the second
clock, Jack will be stationed at the second clock, and at the instant of her
passing they will both take telephoto digital snapshots of the faraway clock *C*_{1}, to see what time it reads.

Jack, of course, knows that *C*_{1} is 6 light seconds away, and
is synchronized with *C*_{2}
which at that instant is reading 10 seconds, so his snapshot must show *C*_{1} to read 4 seconds. That is, looking at *C*_{1}
he sees it as it was six seconds ago.

What does Jill’s
digital snapshot show? It must be
identical—two snapshots taken from the same place at the same time must
show the same thing! So, Jill* must also* gets a picture
of *C*_{1} reading
4 seconds.

*How can she reconcile a picture of the clock reading 4 seconds with
her assertion that at the instant she took the photograph the clock was
registering 6.4 seconds? *

The answer is that she can if she knows her relativity!

*First point: length contraction*. To Jill, the clock *C*_{1} is actually only 4/5 x 18 x 10^{8} meters away
(she sees the distance *C*_{1}*C*_{2} to be Lorentz contracted!).

*Second point: The light didn’t even have to go that far!* In her frame, the clock *C*_{1} is *moving away*, so the
light arriving when she’s at *C*_{2} must have left *C*_{1} when it was closer—at distance *x *in the
figure below.* *The figure shows the light in her frame moving from the clock
towards her at speed *c*, while at the same time the clock itself is
moving to the left at 0.6*c*.

It might be helpful to imagine yourself in her frame of reference, so you
are at rest, and to think of clocks *C*_{1} and *C*_{2}
as being at the front end and back end respectively of a train that is going
past you at speed 0.6*c*. Then,
at the moment the back of the train passes you, you take a picture (through
your telescope, of course) of the clock at the front of the train. Obviously, the light from the front clock
that enters your camera at that instant left the front clock some time ago. During the time that light traveled
towards you at speed *c*, the front of the train itself was going in the
opposite direction at speed 0.6*c*. But you know the length of the train
in your frame is 4/5 x 18 x 10^{8} meters, so since at the instant you
take the picture the back of the train is passing you, the front of the train
must be 4/5 x 18 x 10^{8} meters away. Now that distance, 4/5 x 18 x 10^{8},
is the sum of the distance the light entering your camera traveled plus the
distance the train traveled in the same time, that is, (1 + 0.6)/1 times the
distance the light traveled.

So the image of the first ground clock she sees and records as she passes
the second ground clock must have been emitted when the first clock was a
distance* x* from her in her frame, where

_{}

Having established that the clock image she is
seeing as she takes the photograph left the clock when it was only 9 x 10^{8}
meters away, that is, 3 light seconds, she concludes that she is observing the
first ground clock as it was three seconds ago.

*Third point: time dilation*. The story so far: she has a photograph of
the first ground clock that shows it to be reading 4 seconds. She knows that
the light took three seconds to reach her. So, what can she conclude the clock must
actually be registering at the instant the photo was taken? If you are tempted to say 7 seconds, you
have forgotten that in her frame, the clock is moving at 0.6*c* and hence *runs
slow* by a factor 4/5.

Including the time dilation factor correctly, she concludes that in the 3 seconds that the light from the clock took to reach her, the clock itself will have ticked away 3 × 4/5 seconds, or 2.4 seconds.

Therefore, since the photograph shows the clock to read 4 seconds, and she finds the clock must have run a further 2.4 seconds, she deduces that at the instant she took the photograph the clock must actually have been registering 6.4 seconds, which is what she had claimed all along!

The key point of this lecture is that at first it seems impossible for two observers moving relative to each other to both maintain that the other one’s clocks run slow. However, by bringing in the other necessary consequences of the theory of relativity, the Lorentz contraction of lengths, and that clocks synchronized in one frame are out of synchronization in another by a precise amount that follows necessarily from the constancy of the speed of light, the whole picture becomes completely consistent!